Mars is a particularly attractive candidate among known astronomical objects
to potentially host life. Results from space exploration missions have provided
insights into Martian geochemistry that indicate oxychlorine species, particularly perchlorate, are ubiquitous features of the Martian geochemical landscape. Perchlorate presents potential obstacles for known forms of life due to
its toxicity. However, it can also provide potential benefits, such as producing
brines by deliquescence, like those thought to exist on present-day Mars. Here
we show perchlorate brines support folding and catalysis of functional RNAs,
while inactivating representative protein enzymes. Additionally, we show
perchlorate and other oxychlorine species enable ribozyme functions,
including homeostasis-like regulatory behavior and ribozyme-catalyzed
chlorination of organic molecules. We suggest nucleic acids are uniquely wellsuited to hypersaline Martian environments. Furthermore, Martian near- or
subsurface oxychlorine brines, and brines found in potential lifeforms, could
provide a unique niche for biomolecular evolution.
Extremophiles are organisms that thrive in extreme conditions of pH, temperature, or salinity. Some bacteria and archaea live in extremely hot or cold temperatures, while others live in very salty or acidic/alkaline environments. One example is Nanoarchaeum equitans, a dwarf archaeon that lives in temperatures between 70-98°C. Methanogens are a group of archaea that produce methane through anaerobic metabolism. Halophilic archaea thrive in hypersaline environments through adaptations like transport proteins that pump ions across their cell membranes. Acidophiles maintain pH homeostasis through active proton pumps and passive DNA/protein repair systems that protect against acid damage.
In this presentation, I would like to provide the Resistance Mechanism and Molecular Responses to the Salinity.
There are two types of plants Halophytes and Glycophytes (categories on the basis of their responses to the salinity) examples are Thellungiella halophila and Arabidopsis thaliana, respectively.
Earlier Arabidopsis was considered as Model organism incase of plants but it can't tolerate high saline condition that's the reason for the limited study of plant towards salinity responses. But in the year 2004 the discovery of new plant Thellungiella halophila generates new knowledge about the tolerance mechanism of plants towards salinity responses because it's a halophytes which can tolerate extreme saline condition.
And also it has very similarity with the Arabidopsis so it's considered as the Model organism for the study of Salt stress physiology.
There are major two pathways involved in response to Salt stress (described in presentation).
This document summarizes information about the enzyme urease. It discusses that urease is a nickel-containing metalloenzyme found in many organisms that catalyzes the hydrolysis of urea to produce ammonia and carbon dioxide. The active site contains two nickel ions that are bridged by ligands. Urease plays important roles in nitrogen cycling in soils and the digestive systems of ruminants and humans. Deficiencies in urease or related enzymes can cause health issues if not properly treated.
Haloarchaea, or halobacteria, are a group of microorganisms that can grow in extremely salty environments exceeding normal food pickling levels. They have unusual features such as red, orange, or purple pigmentation and the ability to use sunlight to power proton pumps. Haloarchaea are found in hypersaline lakes and salterns, and have adapted mechanisms to balance osmotic pressure through accumulating potassium ions intracellularly. They have potential applications in biotechnology due to their stable enzymes that function in high salinity conditions unsuitable for most other organisms.
Dr. Bruce Damer @ QAU Pakistan-The Origin of Life & Life in the UniverseBruce Damer
Dr. Bruce Damer presents a talk linking the new "Hot Spring Hypothesis" for the origin of life to the search for life in our Solar System and beyond on exoplanets. His host, the renowned physicist and activist Dr. Pervez Hoodbhoy, hosted this talk at the Physics department auditorium at Quaid-i-Azam University in Islamabad , Pakistan. Dr. Bruce “inflamed the minds” of Pakistani students and professors alike as he took them on a rapid romp through life’s possible origins on Earth to the search for evidence for life on Mars in 2020, icy Enceladus in the next decade and onward to the likelihood of life on exoplanets. Dr. Bruce Damer and Prof. Pervez Hoodbhoy (presenters), Elixir Technologies Pakistan (recording and support). [presented 17 November 2017]. Find a podcast with audio, video and additional information about this presentation at: http://www.levityzone.org/lz-episode-059-origins-science-comes-pakistan/
This document reports on a study of the oxygenation properties of hemoglobin from the earthworm Lumbricus terrestris under varying conditions of pH, salts, and temperature. Key findings include:
1) Hemoglobin from L. terrestris exhibits relatively small cooperativity (free energy of 1.6-2.8 kcal/mol) and a large, pH-dependent Hill coefficient that reaches a maximum of 7.9.
2) Cations, not anions, control oxygen binding, with divalent cations having a larger effect than monovalent cations. Effectiveness decreases in the order Ca2+ > Sr2+ > Ba2+ and Mg2+ > Na+.
Factors influencing distribution of nutrition elements in seaNazmul Ahmed Oli
- The document discusses factors that influence the distribution of nutrients in the ocean, specifically carbon, nitrogen, and phosphorus.
- Photosynthetic phytoplankton near the surface produce organic matter using nutrients from the water. After dying, this organic matter either decomposes and returns nutrients to the water or sinks deeper.
- Nutrients are depleted at the surface but enriched deeper where organic matter decomposes. Upwelling currents return nutrients to the surface, fueling new growth.
- The ratios of phosphorus, nitrogen and oxygen in seawater closely match what phytoplankton need, though the reasons for this are still debated. Organic processes may help control nutrient ratios available for life.
The document summarizes the history of life on Earth based on evidence from the fossil record. It describes how early Earth's atmosphere allowed for the abiotic synthesis of organic molecules around 4 billion years ago. The earliest life forms were single-celled prokaryotes that formed around 3.5 billion years ago. Oxygen began accumulating in the atmosphere around 2.7 billion years ago due to cyanobacteria. Eukaryotic cells developed around 2.1 billion years ago through endosymbiosis. Multicellular life emerged around 1.5 billion years ago. The Cambrian explosion saw a rapid diversification of life around 535 million years ago. Plants and fungi first colonized land around 500 million years ago
Extremophiles are organisms that thrive in extreme conditions of pH, temperature, or salinity. Some bacteria and archaea live in extremely hot or cold temperatures, while others live in very salty or acidic/alkaline environments. One example is Nanoarchaeum equitans, a dwarf archaeon that lives in temperatures between 70-98°C. Methanogens are a group of archaea that produce methane through anaerobic metabolism. Halophilic archaea thrive in hypersaline environments through adaptations like transport proteins that pump ions across their cell membranes. Acidophiles maintain pH homeostasis through active proton pumps and passive DNA/protein repair systems that protect against acid damage.
In this presentation, I would like to provide the Resistance Mechanism and Molecular Responses to the Salinity.
There are two types of plants Halophytes and Glycophytes (categories on the basis of their responses to the salinity) examples are Thellungiella halophila and Arabidopsis thaliana, respectively.
Earlier Arabidopsis was considered as Model organism incase of plants but it can't tolerate high saline condition that's the reason for the limited study of plant towards salinity responses. But in the year 2004 the discovery of new plant Thellungiella halophila generates new knowledge about the tolerance mechanism of plants towards salinity responses because it's a halophytes which can tolerate extreme saline condition.
And also it has very similarity with the Arabidopsis so it's considered as the Model organism for the study of Salt stress physiology.
There are major two pathways involved in response to Salt stress (described in presentation).
This document summarizes information about the enzyme urease. It discusses that urease is a nickel-containing metalloenzyme found in many organisms that catalyzes the hydrolysis of urea to produce ammonia and carbon dioxide. The active site contains two nickel ions that are bridged by ligands. Urease plays important roles in nitrogen cycling in soils and the digestive systems of ruminants and humans. Deficiencies in urease or related enzymes can cause health issues if not properly treated.
Haloarchaea, or halobacteria, are a group of microorganisms that can grow in extremely salty environments exceeding normal food pickling levels. They have unusual features such as red, orange, or purple pigmentation and the ability to use sunlight to power proton pumps. Haloarchaea are found in hypersaline lakes and salterns, and have adapted mechanisms to balance osmotic pressure through accumulating potassium ions intracellularly. They have potential applications in biotechnology due to their stable enzymes that function in high salinity conditions unsuitable for most other organisms.
Dr. Bruce Damer @ QAU Pakistan-The Origin of Life & Life in the UniverseBruce Damer
Dr. Bruce Damer presents a talk linking the new "Hot Spring Hypothesis" for the origin of life to the search for life in our Solar System and beyond on exoplanets. His host, the renowned physicist and activist Dr. Pervez Hoodbhoy, hosted this talk at the Physics department auditorium at Quaid-i-Azam University in Islamabad , Pakistan. Dr. Bruce “inflamed the minds” of Pakistani students and professors alike as he took them on a rapid romp through life’s possible origins on Earth to the search for evidence for life on Mars in 2020, icy Enceladus in the next decade and onward to the likelihood of life on exoplanets. Dr. Bruce Damer and Prof. Pervez Hoodbhoy (presenters), Elixir Technologies Pakistan (recording and support). [presented 17 November 2017]. Find a podcast with audio, video and additional information about this presentation at: http://www.levityzone.org/lz-episode-059-origins-science-comes-pakistan/
This document reports on a study of the oxygenation properties of hemoglobin from the earthworm Lumbricus terrestris under varying conditions of pH, salts, and temperature. Key findings include:
1) Hemoglobin from L. terrestris exhibits relatively small cooperativity (free energy of 1.6-2.8 kcal/mol) and a large, pH-dependent Hill coefficient that reaches a maximum of 7.9.
2) Cations, not anions, control oxygen binding, with divalent cations having a larger effect than monovalent cations. Effectiveness decreases in the order Ca2+ > Sr2+ > Ba2+ and Mg2+ > Na+.
Factors influencing distribution of nutrition elements in seaNazmul Ahmed Oli
- The document discusses factors that influence the distribution of nutrients in the ocean, specifically carbon, nitrogen, and phosphorus.
- Photosynthetic phytoplankton near the surface produce organic matter using nutrients from the water. After dying, this organic matter either decomposes and returns nutrients to the water or sinks deeper.
- Nutrients are depleted at the surface but enriched deeper where organic matter decomposes. Upwelling currents return nutrients to the surface, fueling new growth.
- The ratios of phosphorus, nitrogen and oxygen in seawater closely match what phytoplankton need, though the reasons for this are still debated. Organic processes may help control nutrient ratios available for life.
The document summarizes the history of life on Earth based on evidence from the fossil record. It describes how early Earth's atmosphere allowed for the abiotic synthesis of organic molecules around 4 billion years ago. The earliest life forms were single-celled prokaryotes that formed around 3.5 billion years ago. Oxygen began accumulating in the atmosphere around 2.7 billion years ago due to cyanobacteria. Eukaryotic cells developed around 2.1 billion years ago through endosymbiosis. Multicellular life emerged around 1.5 billion years ago. The Cambrian explosion saw a rapid diversification of life around 535 million years ago. Plants and fungi first colonized land around 500 million years ago
This document summarizes the key stages and discoveries in photosynthesis research:
1. Moll's half leaf experiment in the 1700s showed that CO2 is required for photosynthesis.
2. In the 1800s, Priestley, Ingenhousz, and van Niel discovered oxygen evolution and that sunlight and water are essential.
3. In the 1900s, Calvin used radioactive tracers to discover the Calvin cycle, where CO2 is fixed into 3-carbon compounds in chloroplasts, using enzymes like RuBisCO.
4. C4 and CAM pathways were discovered as alternatives to the C3 Calvin cycle that improve efficiency in hot/dry conditions through additional CO2
Mars exploration has been guided by the search for water. The more complex quest by Mars Science
Laboratory for habitable environments should illuminate the Martian environmental history, and
possibly deliver insights into extraterrestrial life.
Microbial habitability of Europa sustained by radioactive sources Sérgio Sacani
This document summarizes a scientific report that models the potential for microbial life in Europa's subsurface ocean, sustained by energy from radioactive decay. The model proposes that radiation from uranium, thorium, and potassium in the seabed could produce sulfate through water radiolysis, similar to how bacteria thrive in deep mines on Earth. Calculations show that sulfate production could meet the energy demands of sulfate-reducing bacteria, like those found 2.8 km below Earth's surface. The model provides a framework to further evaluate habitability in icy moons through radioactive sources and future exploration.
Settlement rates of invasive tunicates were observed over 4 weeks at different locations and depths in Pillar Point Harbor, California. Clod dissolution plates and settlement plates were used to measure flow rates and tunicate recruitment. Results showed no relationship between flow and settlement, but temperature increases, heavy algal growth, and predation on plates correlated with lower settlement. Further study of how temperature, competition, and predation impact recruitment is needed to better manage invasive tunicates.
This document summarizes a study on testing two bodies of water, McKellar Lake and Brinkley Bayou, for the presence of sulphate reducing bacteria (SRBs). SRBs produce hydrogen sulfide, which is toxic and causes corrosion. The study aims to determine if McKellar Lake, near potential polluters, has problematic SRB levels compared to the control site of Brinkley Bayou in a state park. Soil samples were taken from both sites and tested using standard microbial techniques to quantify and compare SRB presence.
Sulfur is an essential element that plays an important role in biological processes through electron transfers. Understanding sulfur metabolism in model organisms like Escherichia coli and Bacillus subtilis is important to extend knowledge to other ecological niches. Sulfur metabolism involves three main processes: synthesis of sulfur-containing amino acids and coenzymes, catabolism and equilibration of sulfur molecules, and methionine recycling. Iron-sulfur proteins and copper proteins participate in one-electron transfers involving oxidation states of iron and copper.
Explain Langmuir isotherm model and derive its equationZakir Ullah
The document discusses soil chemistry concepts including:
1) Classification of silicate minerals into 1:1 and 2:1 clays based on their structure.
2) Isomorphic substitution in silicate minerals where ions of similar size but different charge replace one another.
3) Calculation of permanent charge in a trioctahedral 2:1 silicate mineral based on isomorphic substitution.
1. Early life on Earth likely originated from self-replicating RNA molecules between 3.8-4.3 billion years ago near hydrothermal vents on the ocean floor where conditions were stable. These RNAs may have eventually led to the first cells with lipid membranes and simple metabolic pathways using hydrogen and carbon dioxide.
2. Around 2.5 billion years ago, cyanobacteria evolved oxygenic photosynthesis, leading to accumulation of oxygen in the atmosphere over hundreds of millions of years and allowing aerobic respiration to evolve. This drove diversification of metabolism and the rise of eukaryotes.
3. Eukaryotic cells likely arose through endosymbiotic events where ancient bacteria capable of aerobic
- The researchers were able to amplify and sequence archaeal and bacterial 16S rDNA from samples taken from a Bahamian beach and salt marsh, identifying organisms from the genera Haloferax and Halomonas.
- Haloferax species were isolated from 1.5M NaCl enrichment cultures of Bahamian beach sand, growing between 1.5-3.3M NaCl salinity. Halomonas species were also identified from the beach sand samples.
- The researchers aim to further analyze the microbial communities in their enrichment cultures over time to changing salinity conditions and identify additional novel species, helping elucidate how extreme halophiles can migrate between marine and hypersaline environments.
This experiment aimed to determine the minimum amount of phosphorus needed to support algal growth and the residual phosphorus remaining after growth. Five reactors with varying concentrations of phosphorus from 0-100% of the standard amount were inoculated with marine algae. Little growth was observed due to the algae being marine species in freshwater media. The wrong type of algae was used, invalidating the use of the Lineweaver-Burk model to analyze phosphorus utilization and algal growth kinetics. Ultimately, the experimental goals were not achieved due to inadvertent use of marine algae rather than freshwater algae.
The divergent fates of primitive hydrospheric water on Earth and MarsSérgio Sacani
The document summarizes research comparing how Earth and Mars differently sequestered early surface water into their mantles. It finds that hydrated Martian basalts can structurally bind about 25% more water than terrestrial basalts, and retain it to greater depths within Mars. Calculations suggest over 9% of the Martian mantle may contain hydrous minerals from surface reactions, versus only about 4% for Earth's mantle. Additionally, hydrated Martian crust experiences little density change upon hydration or dehydration, allowing efficient overplating and burial in Mars' early stagnant-lid tectonic regime. This provided an important sink for Martian surface water and a mechanism for oxidizing its mantle. In contrast, Earth
This document discusses analytical issues related to the determination of arsenic speciation in natural waters using coupled ion chromatography-inductively coupled plasma mass spectrometry (IC-ICP-MS). Key issues addressed include isobaric interferences from polyatomic ions, matrix-dependent ionization effects in the plasma, and potential species-dependent fractionation during nebulization. The document also discusses factors that can cause arsenic speciation to change during sample storage, such as differential adsorption to iron oxides and microbial activity, and makes recommendations for sample preservation and analysis to improve the reliability of speciation measurements.
1. The document analyzes water quality parameters such as temperature, pH, dissolved oxygen, conductivity, chlorophyll a, and redox potential in five lakes located at the University of Notre Dame Research Center.
2. A variety of sampling equipment was used to collect samples from the lakes which were then tested in the lab.
3. The results found that redox potential and conductivity varied with depth in the lakes, influenced by factors like dissolved oxygen levels and dissolved ion concentrations. Respiration and methanogenesis were identified as important metabolic pathways supported by the redox potentials.
Microbes, Man and Environment (Microbial Evolution & Phylogeny ).pptxMidhatSarfraz
This document discusses the evolution of microbial life on Earth from its origins to the development of eukaryotic organisms. It describes how early Earth conditions allowed for the emergence of self-replicating molecules like RNA. Cellular life likely first arose in hydrothermal vents where conditions were stable. Early cells diversified metabolically, with some producing oxygen through photosynthesis. Accumulation of oxygen allowed for aerobic respiration and eukaryotic life, likely arising through endosymbiotic relationships between cells and oxygen-consuming or producing prokaryotes.
This document describes a study that used transposon mutagenesis and targeted gene deletions to identify genes involved in perchlorate reduction in the bacterium Azospira suillum PS. Transposon mutagenesis identified 18 mutants that were completely unable to grow using perchlorate as an electron acceptor (perchlorate null mutants). Most of these mutants had transposon insertions in genes located within the previously identified perchlorate reduction genomic island. Targeted deletions of each gene within this island identified 8 genes that were essential for perchlorate reduction, including those encoding the key enzymes chlorite dismutase and perchlorate reductase as well as genes for a putative regulatory system. This
Coral Reef Biomineralisation effect by Ocean AcidificationRoneet Ghosh
The document summarizes a study that investigated the physiological and cellular impacts of ocean acidification on the reef-building coral Acropora millepora. The key findings are:
1) Exposure to high CO2 conditions predicted for the future caused widespread changes in gene expression in A. millepora related to metabolism, membrane-cytoskeleton interactions, signaling, and other processes.
2) Physiologically, corals exposed to high CO2 lost over half their symbiotic algae (Symbiodinium) populations and had decreased photosynthesis and respiration rates.
3) While calcification was not observed to decrease over the 28-day study, the cellular and physiological changes observed
The document examines the effects of acid on the chlorophyll production and biomass of common duckweed (Lemna minor L.). Two experiments were conducted exposing duckweed to pH levels of 4.1, 5.4, and 6.5 (control) over 10-12 days. The first experiment showed no significant differences in biomass between pH treatments. The second experiment found significantly lower biomass at pH 4.1 compared to pH 5.4 and 6.5. Neither experiment found significant differences in chlorophyll content between pH treatments. The results partially supported the hypothesis, showing acid inhibited biomass but not through impacts on chlorophyll. Longer exposure periods or lower pH levels may be needed to impact chlorophyll.
This document discusses stromatolites and their importance for understanding microbial processes and environmental change over long time periods. Specifically, it mentions:
1) Stromatolite beds that are up to 600 million years old can provide insights into microbial life and Earth's early environments.
2) The formation of stromatolites depends on the bacterial community composition and environmental factors like the precipitation of calcium carbonate facilitated by microbial extracellular substances.
3) Living stromatolites exist today in locations like Cuatro Ciénegas, Mexico, which can serve as models to study microbial metabolic processes and their responses to environmental changes over time.
Substrate Inhibition in Ruthenium(III) Catalyzed Oxidation of Propane-1,3-dio...Ratnakaram Venkata Nadh
- Ruthenium(III) catalyzed oxidation of propane-1,3-diol by potassium periodate was studied in aqueous perchloric acid medium.
- The reaction was found to be first order in oxidant and catalyst concentrations, and inverse fractional order in acid concentration. Substrate inhibition was also observed with increasing substrate concentration.
- Various reaction conditions like temperature, addition of salts, and acetic acid-water solvent composition were varied to determine their effects. Based on the kinetic data, a plausible reaction mechanism was proposed.
The binding of cosmological structures by massless topological defectsSérgio Sacani
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
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2. In the 1800s, Priestley, Ingenhousz, and van Niel discovered oxygen evolution and that sunlight and water are essential.
3. In the 1900s, Calvin used radioactive tracers to discover the Calvin cycle, where CO2 is fixed into 3-carbon compounds in chloroplasts, using enzymes like RuBisCO.
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Settlement rates of invasive tunicates were observed over 4 weeks at different locations and depths in Pillar Point Harbor, California. Clod dissolution plates and settlement plates were used to measure flow rates and tunicate recruitment. Results showed no relationship between flow and settlement, but temperature increases, heavy algal growth, and predation on plates correlated with lower settlement. Further study of how temperature, competition, and predation impact recruitment is needed to better manage invasive tunicates.
This document summarizes a study on testing two bodies of water, McKellar Lake and Brinkley Bayou, for the presence of sulphate reducing bacteria (SRBs). SRBs produce hydrogen sulfide, which is toxic and causes corrosion. The study aims to determine if McKellar Lake, near potential polluters, has problematic SRB levels compared to the control site of Brinkley Bayou in a state park. Soil samples were taken from both sites and tested using standard microbial techniques to quantify and compare SRB presence.
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1) Classification of silicate minerals into 1:1 and 2:1 clays based on their structure.
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1. Early life on Earth likely originated from self-replicating RNA molecules between 3.8-4.3 billion years ago near hydrothermal vents on the ocean floor where conditions were stable. These RNAs may have eventually led to the first cells with lipid membranes and simple metabolic pathways using hydrogen and carbon dioxide.
2. Around 2.5 billion years ago, cyanobacteria evolved oxygenic photosynthesis, leading to accumulation of oxygen in the atmosphere over hundreds of millions of years and allowing aerobic respiration to evolve. This drove diversification of metabolism and the rise of eukaryotes.
3. Eukaryotic cells likely arose through endosymbiotic events where ancient bacteria capable of aerobic
- The researchers were able to amplify and sequence archaeal and bacterial 16S rDNA from samples taken from a Bahamian beach and salt marsh, identifying organisms from the genera Haloferax and Halomonas.
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This experiment aimed to determine the minimum amount of phosphorus needed to support algal growth and the residual phosphorus remaining after growth. Five reactors with varying concentrations of phosphorus from 0-100% of the standard amount were inoculated with marine algae. Little growth was observed due to the algae being marine species in freshwater media. The wrong type of algae was used, invalidating the use of the Lineweaver-Burk model to analyze phosphorus utilization and algal growth kinetics. Ultimately, the experimental goals were not achieved due to inadvertent use of marine algae rather than freshwater algae.
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1. The document analyzes water quality parameters such as temperature, pH, dissolved oxygen, conductivity, chlorophyll a, and redox potential in five lakes located at the University of Notre Dame Research Center.
2. A variety of sampling equipment was used to collect samples from the lakes which were then tested in the lab.
3. The results found that redox potential and conductivity varied with depth in the lakes, influenced by factors like dissolved oxygen levels and dissolved ion concentrations. Respiration and methanogenesis were identified as important metabolic pathways supported by the redox potentials.
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This document discusses the evolution of microbial life on Earth from its origins to the development of eukaryotic organisms. It describes how early Earth conditions allowed for the emergence of self-replicating molecules like RNA. Cellular life likely first arose in hydrothermal vents where conditions were stable. Early cells diversified metabolically, with some producing oxygen through photosynthesis. Accumulation of oxygen allowed for aerobic respiration and eukaryotic life, likely arising through endosymbiotic relationships between cells and oxygen-consuming or producing prokaryotes.
This document describes a study that used transposon mutagenesis and targeted gene deletions to identify genes involved in perchlorate reduction in the bacterium Azospira suillum PS. Transposon mutagenesis identified 18 mutants that were completely unable to grow using perchlorate as an electron acceptor (perchlorate null mutants). Most of these mutants had transposon insertions in genes located within the previously identified perchlorate reduction genomic island. Targeted deletions of each gene within this island identified 8 genes that were essential for perchlorate reduction, including those encoding the key enzymes chlorite dismutase and perchlorate reductase as well as genes for a putative regulatory system. This
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The document summarizes a study that investigated the physiological and cellular impacts of ocean acidification on the reef-building coral Acropora millepora. The key findings are:
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2) Physiologically, corals exposed to high CO2 lost over half their symbiotic algae (Symbiodinium) populations and had decreased photosynthesis and respiration rates.
3) While calcification was not observed to decrease over the 28-day study, the cellular and physiological changes observed
The document examines the effects of acid on the chlorophyll production and biomass of common duckweed (Lemna minor L.). Two experiments were conducted exposing duckweed to pH levels of 4.1, 5.4, and 6.5 (control) over 10-12 days. The first experiment showed no significant differences in biomass between pH treatments. The second experiment found significantly lower biomass at pH 4.1 compared to pH 5.4 and 6.5. Neither experiment found significant differences in chlorophyll content between pH treatments. The results partially supported the hypothesis, showing acid inhibited biomass but not through impacts on chlorophyll. Longer exposure periods or lower pH levels may be needed to impact chlorophyll.
This document discusses stromatolites and their importance for understanding microbial processes and environmental change over long time periods. Specifically, it mentions:
1) Stromatolite beds that are up to 600 million years old can provide insights into microbial life and Earth's early environments.
2) The formation of stromatolites depends on the bacterial community composition and environmental factors like the precipitation of calcium carbonate facilitated by microbial extracellular substances.
3) Living stromatolites exist today in locations like Cuatro Ciénegas, Mexico, which can serve as models to study microbial metabolic processes and their responses to environmental changes over time.
Substrate Inhibition in Ruthenium(III) Catalyzed Oxidation of Propane-1,3-dio...Ratnakaram Venkata Nadh
- Ruthenium(III) catalyzed oxidation of propane-1,3-diol by potassium periodate was studied in aqueous perchloric acid medium.
- The reaction was found to be first order in oxidant and catalyst concentrations, and inverse fractional order in acid concentration. Substrate inhibition was also observed with increasing substrate concentration.
- Various reaction conditions like temperature, addition of salts, and acetic acid-water solvent composition were varied to determine their effects. Based on the kinetic data, a plausible reaction mechanism was proposed.
Similar to Emergent ribozyme behaviors in oxychlorine brines indicate a unique niche for molecular evolution on Mars (20)
The binding of cosmological structures by massless topological defectsSérgio Sacani
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Tr...Sérgio Sacani
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the
atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets
receiving low insolation is still small, limiting our ability to understand the diversity of the atmospheric
composition and climates of temperate terrestrial planets. We report the discovery of an Earth-sized planet
transiting the nearby (12 pc) inactive M3.0 dwarf Gliese 12 (TOI-6251) with an orbital period (Porb) of 12.76 days.
The planet, Gliese 12 b, was initially identified as a candidate with an ambiguous Porb from TESS data. We
confirmed the transit signal and Porb using ground-based photometry with MuSCAT2 and MuSCAT3, and
validated the planetary nature of the signal using high-resolution images from Gemini/NIRI and Keck/NIRC2 as
well as radial velocity (RV) measurements from the InfraRed Doppler instrument on the Subaru 8.2 m telescope
and from CARMENES on the CAHA 3.5 m telescope. X-ray observations with XMM-Newton showed the host
star is inactive, with an X-ray-to-bolometric luminosity ratio of log 5.7 L L X bol » - . Joint analysis of the light
curves and RV measurements revealed that Gliese 12 b has a radius of 0.96 ± 0.05 R⊕,a3σ mass upper limit of
3.9 M⊕, and an equilibrium temperature of 315 ± 6 K assuming zero albedo. The transmission spectroscopy metric
(TSM) value of Gliese 12 b is close to the TSM values of the TRAPPIST-1 planets, adding Gliese 12 b to the small
list of potentially terrestrial, temperate planets amenable to atmospheric characterization with JWST.
Gliese 12 b, a temperate Earth-sized planet at 12 parsecs discovered with TES...Sérgio Sacani
We report on the discovery of Gliese 12 b, the nearest transiting temperate, Earth-sized planet found to date. Gliese 12 is a
bright (V = 12.6 mag, K = 7.8 mag) metal-poor M4V star only 12.162 ± 0.005 pc away from the Solar system with one of the
lowest stellar activity levels known for M-dwarfs. A planet candidate was detected by TESS based on only 3 transits in sectors
42, 43, and 57, with an ambiguity in the orbital period due to observational gaps. We performed follow-up transit observations
with CHEOPS and ground-based photometry with MINERVA-Australis, SPECULOOS, and Purple Mountain Observatory,
as well as further TESS observations in sector 70. We statistically validate Gliese 12 b as a planet with an orbital period of
12.76144 ± 0.00006 d and a radius of 1.0 ± 0.1 R⊕, resulting in an equilibrium temperature of ∼315 K. Gliese 12 b has excellent
future prospects for precise mass measurement, which may inform how planetary internal structure is affected by the stellar
compositional environment. Gliese 12 b also represents one of the best targets to study whether Earth-like planets orbiting cool
stars can retain their atmospheres, a crucial step to advance our understanding of habitability on Earth and across the galaxy.
The importance of continents, oceans and plate tectonics for the evolution of...Sérgio Sacani
Within the uncertainties of involved astronomical and biological parameters, the Drake Equation
typically predicts that there should be many exoplanets in our galaxy hosting active, communicative
civilizations (ACCs). These optimistic calculations are however not supported by evidence, which is
often referred to as the Fermi Paradox. Here, we elaborate on this long-standing enigma by showing
the importance of planetary tectonic style for biological evolution. We summarize growing evidence
that a prolonged transition from Mesoproterozoic active single lid tectonics (1.6 to 1.0 Ga) to modern
plate tectonics occurred in the Neoproterozoic Era (1.0 to 0.541 Ga), which dramatically accelerated
emergence and evolution of complex species. We further suggest that both continents and oceans
are required for ACCs because early evolution of simple life must happen in water but late evolution
of advanced life capable of creating technology must happen on land. We resolve the Fermi Paradox
(1) by adding two additional terms to the Drake Equation: foc
(the fraction of habitable exoplanets
with significant continents and oceans) and fpt
(the fraction of habitable exoplanets with significant
continents and oceans that have had plate tectonics operating for at least 0.5 Ga); and (2) by
demonstrating that the product of foc
and fpt
is very small (< 0.00003–0.002). We propose that the lack
of evidence for ACCs reflects the scarcity of long-lived plate tectonics and/or continents and oceans on
exoplanets with primitive life.
A Giant Impact Origin for the First Subduction on EarthSérgio Sacani
Hadean zircons provide a potential record of Earth's earliest subduction 4.3 billion years ago. Itremains enigmatic how subduction could be initiated so soon after the presumably Moon‐forming giant impact(MGI). Earlier studies found an increase in Earth's core‐mantle boundary (CMB) temperature due to theaccumulation of the impactor's core, and our recent work shows Earth's lower mantle remains largely solid, withsome of the impactor's mantle potentially surviving as the large low‐shear velocity provinces (LLSVPs). Here,we show that a hot post‐impact CMB drives the initiation of strong mantle plumes that can induce subductioninitiation ∼200 Myr after the MGI. 2D and 3D thermomechanical computations show that a high CMBtemperature is the primary factor triggering early subduction, with enrichment of heat‐producing elements inLLSVPs as another potential factor. The models link the earliest subduction to the MGI with implications forunderstanding the diverse tectonic regimes of rocky planets.
Climate extremes likely to drive land mammal extinction during next supercont...Sérgio Sacani
Mammals have dominated Earth for approximately 55 Myr thanks to their
adaptations and resilience to warming and cooling during the Cenozoic. All
life will eventually perish in a runaway greenhouse once absorbed solar
radiation exceeds the emission of thermal radiation in several billions of
years. However, conditions rendering the Earth naturally inhospitable to
mammals may develop sooner because of long-term processes linked to
plate tectonics (short-term perturbations are not considered here). In
~250 Myr, all continents will converge to form Earth’s next supercontinent,
Pangea Ultima. A natural consequence of the creation and decay of Pangea
Ultima will be extremes in pCO2 due to changes in volcanic rifting and
outgassing. Here we show that increased pCO2, solar energy (F⨀;
approximately +2.5% W m−2 greater than today) and continentality (larger
range in temperatures away from the ocean) lead to increasing warming
hostile to mammalian life. We assess their impact on mammalian
physiological limits (dry bulb, wet bulb and Humidex heat stress indicators)
as well as a planetary habitability index. Given mammals’ continued survival,
predicted background pCO2 levels of 410–816 ppm combined with increased
F⨀ will probably lead to a climate tipping point and their mass extinction.
The results also highlight how global landmass configuration, pCO2 and F⨀
play a critical role in planetary habitability.
Constraints on Neutrino Natal Kicks from Black-Hole Binary VFTS 243Sérgio Sacani
The recently reported observation of VFTS 243 is the first example of a massive black-hole binary
system with negligible binary interaction following black-hole formation. The black-hole mass (≈10M⊙)
and near-circular orbit (e ≈ 0.02) of VFTS 243 suggest that the progenitor star experienced complete
collapse, with energy-momentum being lost predominantly through neutrinos. VFTS 243 enables us to
constrain the natal kick and neutrino-emission asymmetry during black-hole formation. At 68% confidence
level, the natal kick velocity (mass decrement) is ≲10 km=s (≲1.0M⊙), with a full probability distribution
that peaks when ≈0.3M⊙ were ejected, presumably in neutrinos, and the black hole experienced a natal
kick of 4 km=s. The neutrino-emission asymmetry is ≲4%, with best fit values of ∼0–0.2%. Such a small
neutrino natal kick accompanying black-hole formation is in agreement with theoretical predictions.
Detectability of Solar Panels as a TechnosignatureSérgio Sacani
In this work, we assess the potential detectability of solar panels made of silicon on an Earth-like
exoplanet as a potential technosignature. Silicon-based photovoltaic cells have high reflectance in the
UV-VIS and in the near-IR, within the wavelength range of a space-based flagship mission concept
like the Habitable Worlds Observatory (HWO). Assuming that only solar energy is used to provide
the 2022 human energy needs with a land cover of ∼ 2.4%, and projecting the future energy demand
assuming various growth-rate scenarios, we assess the detectability with an 8 m HWO-like telescope.
Assuming the most favorable viewing orientation, and focusing on the strong absorption edge in the
ultraviolet-to-visible (0.34 − 0.52 µm), we find that several 100s of hours of observation time is needed
to reach a SNR of 5 for an Earth-like planet around a Sun-like star at 10pc, even with a solar panel
coverage of ∼ 23% land coverage of a future Earth. We discuss the necessity of concepts like Kardeshev
Type I/II civilizations and Dyson spheres, which would aim to harness vast amounts of energy. Even
with much larger populations than today, the total energy use of human civilization would be orders of
magnitude below the threshold for causing direct thermal heating or reaching the scale of a Kardashev
Type I civilization. Any extraterrrestrial civilization that likewise achieves sustainable population
levels may also find a limit on its need to expand, which suggests that a galaxy-spanning civilization
as imagined in the Fermi paradox may not exist.
Jet reorientation in central galaxies of clusters and groups: insights from V...Sérgio Sacani
Recent observations of galaxy clusters and groups with misalignments between their central AGN jets
and X-ray cavities, or with multiple misaligned cavities, have raised concerns about the jet – bubble
connection in cooling cores, and the processes responsible for jet realignment. To investigate the
frequency and causes of such misalignments, we construct a sample of 16 cool core galaxy clusters and
groups. Using VLBA radio data we measure the parsec-scale position angle of the jets, and compare
it with the position angle of the X-ray cavities detected in Chandra data. Using the overall sample
and selected subsets, we consistently find that there is a 30% – 38% chance to find a misalignment
larger than ∆Ψ = 45◦ when observing a cluster/group with a detected jet and at least one cavity. We
determine that projection may account for an apparently large ∆Ψ only in a fraction of objects (∼35%),
and given that gas dynamical disturbances (as sloshing) are found in both aligned and misaligned
systems, we exclude environmental perturbation as the main driver of cavity – jet misalignment.
Moreover, we find that large misalignments (up to ∼ 90◦
) are favored over smaller ones (45◦ ≤ ∆Ψ ≤
70◦
), and that the change in jet direction can occur on timescales between one and a few tens of Myr.
We conclude that misalignments are more likely related to actual reorientation of the jet axis, and we
discuss several engine-based mechanisms that may cause these dramatic changes.
The solar dynamo begins near the surfaceSérgio Sacani
The magnetic dynamo cycle of the Sun features a distinct pattern: a propagating
region of sunspot emergence appears around 30° latitude and vanishes near the
equator every 11 years (ref. 1). Moreover, longitudinal flows called torsional oscillations
closely shadow sunspot migration, undoubtedly sharing a common cause2. Contrary
to theories suggesting deep origins of these phenomena, helioseismology pinpoints
low-latitude torsional oscillations to the outer 5–10% of the Sun, the near-surface
shear layer3,4. Within this zone, inwardly increasing differential rotation coupled with
a poloidal magnetic field strongly implicates the magneto-rotational instability5,6,
prominent in accretion-disk theory and observed in laboratory experiments7.
Together, these two facts prompt the general question: whether the solar dynamo is
possibly a near-surface instability. Here we report strong affirmative evidence in stark
contrast to traditional models8 focusing on the deeper tachocline. Simple analytic
estimates show that the near-surface magneto-rotational instability better explains
the spatiotemporal scales of the torsional oscillations and inferred subsurface
magnetic field amplitudes9. State-of-the-art numerical simulations corroborate these
estimates and reproduce hemispherical magnetic current helicity laws10. The dynamo
resulting from a well-understood near-surface phenomenon improves prospects
for accurate predictions of full magnetic cycles and space weather, affecting the
electromagnetic infrastructure of Earth.
Extensive Pollution of Uranus and Neptune’s Atmospheres by Upsweep of Icy Mat...Sérgio Sacani
In the Nice model of solar system formation, Uranus and Neptune undergo an orbital upheaval,
sweeping through a planetesimal disk. The region of the disk from which material is accreted by
the ice giants during this phase of their evolution has not previously been identified. We perform
direct N-body orbital simulations of the four giant planets to determine the amount and origin of solid
accretion during this orbital upheaval. We find that the ice giants undergo an extreme bombardment
event, with collision rates as much as ∼3 per hour assuming km-sized planetesimals, increasing the
total planet mass by up to ∼0.35%. In all cases, the initially outermost ice giant experiences the
largest total enhancement. We determine that for some plausible planetesimal properties, the resulting
atmospheric enrichment could potentially produce sufficient latent heat to alter the planetary cooling
timescale according to existing models. Our findings suggest that substantial accretion during this
phase of planetary evolution may have been sufficient to impact the atmospheric composition and
thermal evolution of the ice giants, motivating future work on the fate of deposited solid material.
Exomoons & Exorings with the Habitable Worlds Observatory I: On the Detection...Sérgio Sacani
The highest priority recommendation of the Astro2020 Decadal Survey for space-based astronomy
was the construction of an observatory capable of characterizing habitable worlds. In this paper series
we explore the detectability of and interference from exomoons and exorings serendipitously observed
with the proposed Habitable Worlds Observatory (HWO) as it seeks to characterize exoplanets, starting
in this manuscript with Earth-Moon analog mutual events. Unlike transits, which only occur in systems
viewed near edge-on, shadow (i.e., solar eclipse) and lunar eclipse mutual events occur in almost every
star-planet-moon system. The cadence of these events can vary widely from ∼yearly to multiple events
per day, as was the case in our younger Earth-Moon system. Leveraging previous space-based (EPOXI)
lightcurves of a Moon transit and performance predictions from the LUVOIR-B concept, we derive
the detectability of Moon analogs with HWO. We determine that Earth-Moon analogs are detectable
with observation of ∼2-20 mutual events for systems within 10 pc, and larger moons should remain
detectable out to 20 pc. We explore the extent to which exomoon mutual events can mimic planet
features and weather. We find that HWO wavelength coverage in the near-IR, specifically in the 1.4 µm
water band where large moons can outshine their host planet, will aid in differentiating exomoon signals
from exoplanet variability. Finally, we predict that exomoons formed through collision processes akin
to our Moon are more likely to be detected in younger systems, where shorter orbital periods and
favorable geometry enhance the probability and frequency of mutual events.
Continuum emission from within the plunging region of black hole discsSérgio Sacani
The thermal continuum emission observed from accreting black holes across X-ray bands has the potential to be leveraged as a
powerful probe of the mass and spin of the central black hole. The vast majority of existing ‘continuum fitting’ models neglect
emission sourced at and within the innermost stable circular orbit (ISCO) of the black hole. Numerical simulations, however,
find non-zero emission sourced from these regions. In this work, we extend existing techniques by including the emission
sourced from within the plunging region, utilizing new analytical models that reproduce the properties of numerical accretion
simulations. We show that in general the neglected intra-ISCO emission produces a hot-and-small quasi-blackbody component,
but can also produce a weak power-law tail for more extreme parameter regions. A similar hot-and-small blackbody component
has been added in by hand in an ad hoc manner to previous analyses of X-ray binary spectra. We show that the X-ray spectrum
of MAXI J1820+070 in a soft-state outburst is extremely well described by a full Kerr black hole disc, while conventional
models that neglect intra-ISCO emission are unable to reproduce the data. We believe this represents the first robust detection of
intra-ISCO emission in the literature, and allows additional constraints to be placed on the MAXI J1820 + 070 black hole spin
which must be low a• < 0.5 to allow a detectable intra-ISCO region. Emission from within the ISCO is the dominant emission
component in the MAXI J1820 + 070 spectrum between 6 and 10 keV, highlighting the necessity of including this region. Our
continuum fitting model is made publicly available.
WASP-69b’s Escaping Envelope Is Confined to a Tail Extending at Least 7 RpSérgio Sacani
Studying the escaping atmospheres of highly irradiated exoplanets is critical for understanding the physical
mechanisms that shape the demographics of close-in planets. A number of planetary outflows have been observed
as excess H/He absorption during/after transit. Such an outflow has been observed for WASP-69b by multiple
groups that disagree on the geometry and velocity structure of the outflow. Here, we report the detection of this
planet’s outflow using Keck/NIRSPEC for the first time. We observed the outflow 1.28 hr after egress until the
target set, demonstrating the outflow extends at least 5.8 × 105 km or 7.5 Rp This detection is significantly longer
than previous observations, which report an outflow extending ∼2.2 planet radii just 1 yr prior. The outflow is
blueshifted by −23 km s−1 in the planetary rest frame. We estimate a current mass-loss rate of 1 M⊕ Gyr−1
. Our
observations are most consistent with an outflow that is strongly sculpted by ram pressure from the stellar wind.
However, potential variability in the outflow could be due to time-varying interactions with the stellar wind or
differences in instrumental precision.
Travis Hills' Endeavors in Minnesota: Fostering Environmental and Economic Pr...Travis Hills MN
Travis Hills of Minnesota developed a method to convert waste into high-value dry fertilizer, significantly enriching soil quality. By providing farmers with a valuable resource derived from waste, Travis Hills helps enhance farm profitability while promoting environmental stewardship. Travis Hills' sustainable practices lead to cost savings and increased revenue for farmers by improving resource efficiency and reducing waste.
Phenomics assisted breeding in crop improvementIshaGoswami9
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Remote Sensing and Computational, Evolutionary, Supercomputing, and Intellige...University of Maribor
Slides from talk:
Aleš Zamuda: Remote Sensing and Computational, Evolutionary, Supercomputing, and Intelligent Systems.
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Inter-Society Networking Panel GRSS/MTT-S/CIS Panel Session: Promoting Connection and Cooperation
https://www.etran.rs/2024/en/home-english/
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...Leonel Morgado
Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.
Authoring a personal GPT for your research and practice: How we created the Q...Leonel Morgado
Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.
When I was asked to give a companion lecture in support of ‘The Philosophy of Science’ (https://shorturl.at/4pUXz) I decided not to walk through the detail of the many methodologies in order of use. Instead, I chose to employ a long standing, and ongoing, scientific development as an exemplar. And so, I chose the ever evolving story of Thermodynamics as a scientific investigation at its best.
Conducted over a period of >200 years, Thermodynamics R&D, and application, benefitted from the highest levels of professionalism, collaboration, and technical thoroughness. New layers of application, methodology, and practice were made possible by the progressive advance of technology. In turn, this has seen measurement and modelling accuracy continually improved at a micro and macro level.
Perhaps most importantly, Thermodynamics rapidly became a primary tool in the advance of applied science/engineering/technology, spanning micro-tech, to aerospace and cosmology. I can think of no better a story to illustrate the breadth of scientific methodologies and applications at their best.
The technology uses reclaimed CO₂ as the dyeing medium in a closed loop process. When pressurized, CO₂ becomes supercritical (SC-CO₂). In this state CO₂ has a very high solvent power, allowing the dye to dissolve easily.
ESR spectroscopy in liquid food and beverages.pptxPRIYANKA PATEL
With increasing population, people need to rely on packaged food stuffs. Packaging of food materials requires the preservation of food. There are various methods for the treatment of food to preserve them and irradiation treatment of food is one of them. It is the most common and the most harmless method for the food preservation as it does not alter the necessary micronutrients of food materials. Although irradiated food doesn’t cause any harm to the human health but still the quality assessment of food is required to provide consumers with necessary information about the food. ESR spectroscopy is the most sophisticated way to investigate the quality of the food and the free radicals induced during the processing of the food. ESR spin trapping technique is useful for the detection of highly unstable radicals in the food. The antioxidant capability of liquid food and beverages in mainly performed by spin trapping technique.
ESR spectroscopy in liquid food and beverages.pptx
Emergent ribozyme behaviors in oxychlorine brines indicate a unique niche for molecular evolution on Mars
1. Article https://doi.org/10.1038/s41467-024-48037-2
Emergent ribozyme behaviors in oxychlorine
brines indicate a unique niche for molecular
evolution on Mars
Tanner G. Hoog1
, Matthew R. Pawlak 2
, Nathaniel J. Gaut 2
, Gloria C. Baxter 1
,
Thomas A. Bethel3
, Katarzyna P. Adamala 1,2
& Aaron E. Engelhart 1,2
Mars is a particularly attractive candidate among known astronomical objects
to potentially host life. Results from space exploration missions have provided
insights into Martian geochemistry that indicate oxychlorine species, parti-
cularly perchlorate, are ubiquitous features of the Martian geochemical land-
scape. Perchlorate presents potential obstacles for known forms of life due to
its toxicity. However, it can also provide potential benefits, such as producing
brines by deliquescence, like those thought to exist on present-day Mars. Here
we show perchlorate brines support folding and catalysis of functional RNAs,
while inactivating representative protein enzymes. Additionally, we show
perchlorate and other oxychlorine species enable ribozyme functions,
including homeostasis-like regulatory behavior and ribozyme-catalyzed
chlorination of organic molecules. We suggest nucleic acids are uniquely well-
suited to hypersaline Martian environments. Furthermore, Martian near- or
subsurface oxychlorine brines, and brines found in potential lifeforms, could
provide a unique niche for biomolecular evolution.
The possibility of life on Mars has attracted intense interest due to its
similarities to Earth, especially during its Noachian period, during
which liquid water was thought to be present. At this time, both bodies
were rocky planets harboring an ocean world with reducing environ-
ments conducive to prebiotic chemistry1,2
. These similarities have led
researchers to speculate that life could have started on Earth and Mars
independently. There is a large body of evidence to support this claim,
including recent work suggesting wet-dry cycling was present during
the late Noachian-Hesperian transition3,4
. Wet-dry cycles have been
invoked as potentially important enabling mechanisms for prebiotic
chemical evolution due to their ability to concentrate reaction sub-
strates and drive dehydration-condensation reactions, such as drying
of sugars and nucleobases to form nucleosides or clay-promoted RNA
polymerization5–8
. Several missions have identified chemical species
on Mars that could support these reactions, such as borates, which
stabilize sugars and were identified at Gale Crater by ChemCam9
, and
phyllosilicate clays, which promote RNA polymerization and were
identified by the Mars Reconnaissance Orbiter10
.
Despite growing evidence that early Martian conditions were
suitable for prebiotic chemistry, obstacles on present-day Mars exist
for sustained life into the present Amazonian era. The most notable
caveat to life on Mars is the current lack of bulk liquid water. This is due
to low temperatures and atmospheric pressure11
, which allowed the
Noachian oceans of Mars to dry. A second obstacle to extant Martian
life is perchlorate (ClO4
-
) and other oxychlorine species which have
been shown to be ubiquitous across Mars’ surface. Evidence for this
from multiple investigations spanning from the Phoenix lander at
Green Valley in the Vastitas Borealis artic12
, to the Curiosity rover at
Mars’ equator (Gale Crater’s Aeolis Palus)13
, and even to the analysis of
the Martian meteorite EETA 79001 found on Earth14–16
. Multiple
Received: 29 November 2023
Accepted: 19 April 2024
Check for updates
1
Department of Genetics, Cell Biology, and Development, University of Minnesota, 6-160 Jackson Hall, 321 Church Street SE, Minneapolis, MN 55455, USA.
2
Department of Biochemistry, Molecular Biology and Biophysics, University of Minnesota, 321 Church Street SE, Minneapolis, MN 55455, USA. 3
Department of
Ecology, Evolution, and Behavior, University of Minnesota, 140 Gortner Laboratory, 1479 Gortner Avenue, St. Paul, MN 55108, USA.
e-mail: enge0213@umn.edu
Nature Communications| (2024)15:3863 1
1234567890():,;
1234567890():,;
2. mechanisms of perchlorate formation have been postulated, with
many of these requiring an arid surface to create the perchlorate
concentration we see today17
. However, perchlorate has also been
found within samples of the Sheepbed mudstone lacustrine deposit in
the Yellowknife Bay of Gale Crater18
. This sediment dates back to the
Noachian-Hesperian era19
, consistent with perchlorate having been a
near-constant presence across most of Martian history. This also aligns
with proposed mechanisms of perchlorate formation that require
aqueous soltions20,21
. Perchlorate is particularly dangerous due to its
toxicity to terrestrial life, which is enhanced by ultraviolet radiation, a
third obstacle that bombards Mars’ surface22
. However, these factors
can be mitigated. Perchlorate salts exhibit a high degree of hygro-
scopicity and readily adsorb water from the atmosphere which sug-
gests near-surface perchlorate brines could act as a refuge for extant
life23–25
. Ultraviolet radiation can be substantially reduced by just mil-
limeter thicknesses of regolith, suggesting that the near- or below-
surface of Mars could be well protected. Perchlorate brines may pro-
vide a stable source of liquid water on present-day Mars, but they also
add another problem for habitability: perchlorate solutions are chao-
tropic and tend to be destabilizing to biomolecules.
Motivated by these reports, and suggestions from investigators
that the selection pressures associated with perchlorate brines would
drive molecular evolution towards more perchlorate-tolerant
organisms26
, we sought to examine how perchlorate brines could
have impacted molecular evolution on Mars as a moderately saline
environment, such as Noachian oceans27
, transitioned to a hypersaline
one, such as recurring slope lineae-associated brines or subglacial
reservoirs25,28
. If Martian life emerged within oxychlorine brines, it
would necessarily have addressed this either during prebiotic
evolution29
, or as halophilic Martian organisms evolved, as has been
observed on Earth30
. Such molecular adaptations would have been
relevant to either scenario. Given that RNA is a particularly salt-tolerant
biopolymer, we speculated thatit could bewell-adapted to perchlorate
brines.
In this work, we find that ribozymes have an innate tolerance to
perchlorate-like highly evolved thermo- and halophilic proteins, as well
as show that oxychlorine brines can support ribozyme activity by
enabling homeostasis-like regulatory behaviors and chlorination of
organic molecules.
Results
Functional RNAs exhibit > 10-fold higher tolerance to per-
chlorate than a mesophilic protein enzyme
Ribozymes, like proteins, fold into intricate three-dimensional struc-
tures, imparting the polymer with a specific function. To assess the
ability of ribozymes to resist perchlorate denaturation, we examined
the impact of perchlorate on a prototypical ribozyme: the self-cleaving
hammerhead nuclease (Fig. 1a). We assessed perchlorate-induced
changes in the function of this ribozyme in mixed sodium-magnesium
chloride and perchlorate solution. We found that the hammerhead
ribozyme exhibited a biphasic perchlorate-activity response, with
increasing activity up to a maximum at 5 M NaClO4 (apparent first-
order rate constant kapp = 0.79 h-1
) and retention of function in brines
as high as 6-7 M NaClO4 (kapp =0.24 h-1
for 6 M ClO4; Fig. 1b, c; Sup-
plementary Figs. 1 and 2a). The perchlorate-associated rate optimum
occurred at approximately the same concentration of sodium per-
chlorate as a saturated sodium chloride solution (i.e., 5 M). The self-
cleavage rate in chloride solution was approximately twice that of
perchlorate solution (1.9-fold higher; 1.48 h-1
for 5 M NaCl, Supple-
mentary Fig. 2a). Thus, while high concentrations of perchlorate
somewhat suppressed ribozyme function, they still permitted catalysis
in solutions nearing the saturation point of sodium per-
chlorate (9.5 M).
The hammerhead ribozyme consensus sequence we examined
was derived from the avocado sunblotch viroid31,32
. The host organism
that it infects, avocado (Persea americana), is mesophilic and well-
known to be salt-sensitive, with the well-known Hass cultivar tolerating
only sub-millimolar levels of the salinity in irrigation water, even when
grafted to salt-tolerant rootstocks33
. Therefore, we initially compared
the hammerhead nuclease to a mesophilic protein nuclease, the
restriction enzyme EcoRI (Fig. 1d). In contrast to the hammerhead
ribozyme, which exhibits considerable tolerance to perchlorate, EcoRI
loses function at perchlorate concentrations ca. one order of magni-
tude lower (i.e., as low as 0.2–0.5 M, Fig. 1e, f). EcoRI retained only
marginal activity in both 0.2 M NaClO4 and NaCl with a 10.7-fold
reduced rate of catalysis in perchlorate solutions (Supplementary
Fig. 2b; 0.048 h−1
for NaCl versus 0.0045 h-1
for NaClO4). A second
mesophilic protein produced by E. Coli was tested. RNase HII, an RNA/
DNA hybrid endonuclease, also lost all catalytic activity at just 0.2-
0.5 M NaClO4 (Supplementary Fig. 3)34
.
As a second model functional RNA, we examined a representative
member of another class: aptamers, which are RNAs that bind specific
ligands. The Broccoli aptamer forms a ligand-receptor pair with a small
molecule dye, DFHBI-1T, activating its fluorescence upon binding
(Fig. 1g)35
. Broccoli exhibited considerable perchlorate tolerance with
retention of function at perchlorate concentrations as high as 5 M
NaClO4 (Fig. 1h, i). Remarkably, even at perchlorate concentrations as
high as 5 M NaClO4, fluorescent melting analysis of Broccoli/DFHBI-1T
reveals sigmoidal traces indicating the proper cooperative folding
needed to bind to DFHBI-1T (Supplementary Fig. 4). This retention of
function is notable, as the Broccoli aptamer was selected in a meso-
philic organismal chassis (E. coli). Despite this, the Broccoli aptamer
exhibited a more modest response to perchlorate than EcoRI, with 80%
retention of activity (as measured by fluorescence) at 2 M perchlorate
and 6% at 5 M perchlorate (its upper limit for perchlorate tolerance).
Binding (Broccoli aptamer) and degradative catalysis (hammer-
head ribozyme nuclease) represent crucial functions of biology. To
better assess the capacity of RNA to assume additional biological roles,
we examined a biosynthetic ribozyme: the tC19z ribozyme
polymerase36
. This ribozyme can perform template-directed RNA
synthesis, polymerizing single ribonucleotide triphosphates into lar-
ger polymers (Fig. 1j). tC19z exhibited gradual diminution of function
with increasing perchlorate (Δyield/d[ClO4
-
] = –7.4%/M). The ion
dependence of yield in perchlorate was slightly more than half that
observed with increasing NaCl (Δyield/d[Cl-
] = –4.1%/M). Indeed, tC19z
retained catalytic function at perchlorate concentrations as high as
3–3.5 M (Fig. 1k, l). It only lost its ability to catalyze extension past 7
nucleotides at 3.5 M, with complete loss of activity at 4 M. tC19z, like
other functional RNAs tested, was not selected in perchlorate brines,
demonstrating that RNA-based functional polymers appear to exhibit
innate resistance to the denaturing effects of perchlorate.
Mesophilic RNAs exhibit capacity to recover from perchlorate-
induced denaturation that is similar to extremophilic proteins
EcoRI and RNase HII are two model enzymes from a mesophilic
microbial organism (E. coli), resembling those more likely to be found
in moderate-salt environments that are unlike current Martian condi-
tions. To test model functional biopolymers evolved in conditions
more challenging to folding, we examined two protein enzymes from
extremophiles found on present-day Earth. As an extremophilic pro-
tein analog of EcoRI, we tested the restriction enzyme TaqI-v2 (Fig. 2a),
derived from the thermophilic organism Thermus aquaticus37
. We
reasoned that the enhanced thermodynamic stability observed in
thermophilic biopolymers would impart resilience to perchlorate-
induced denaturation. Despite this, TaqI-v2 was remarkably suscep-
tible to perchlorate, with a complete loss of function at 0.2 M NaClO4
(Fig. 2b, c) while still retaining function in 0.2 M NaCl (kapp = 0.42 h−1
;
Supplementary Fig. 5a).
We next sought to examine a salt-adapted protein enzyme cata-
lyst. We employed the β-lactamase derived from the halophilic
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 2
3. bacterium Chromohalobacter sp. 560 (HaBlap)38
. Proteins from this
genus are known to exhibit adaptations to high salt, including a higher
proportion of acidic residues39
. To assess the impact of perchlorate on
the catalytic activity of HaBlap, we monitored β-lactamase activity
using nitrocefin, a small molecule that exhibits a color change upon
hydrolysis of its β-lactam ring (Fig. 2d). While HaBlap demonstrated
the expected resilience to sodium chloride, its activity decreased in the
presence of perchlorate, particularly at concentrations ranging from 3
to 4 M NaClO4 (Fig. 2e, f). Despite exhibiting a high degree of haloto-
lerance, the rate of catalysis by HaBlap was still particularly susceptible
to perchlorate (kapp = 0.68 h-1
and kapp = 0.12 h-1
at 0 M and 1 M NaClO4
respectively) compared to sodium chloride (kapp = 0.94 h-1
at 1 M NaCl;
Supplementary Fig. 5b–d), exhibiting a 7.7-fold decrease in activity at
1 M perchlorate/chloride. Overall, this protein exhibited resistance to
perchlorate comparable to levels we observed for ribozymes. This is
consistent with a model in which RNAs, with their polyanionic back-
bones and salt requirements for folding, exhibit innate perchlorate
tolerance comparable to that found only in halophilic proteins that
have undergone selective pressure and evolution in the presence of
high salt.
One model for perchlorate brines on present-day Mars that has
attracted intense attention invokes so-called recurring slope lineae
(RSL)25
. It has been speculated that RSL undergoes transient hydration-
dehydration cycles. In such cycles, salt concentration would necessa-
rily vary significantly, with high- and low-salt excursions. To examine
the tolerance of biopolymers to such cyclic salt concentrations,
0
Product →
Substrate→
ClO4
-
0.05 M
0.20 M
1 2 3
Time (h)
Product →
Substrate→
0
Product →
Substrate→
ClO4
-
6 M
7 M
20 40 60
Time (min)
Product →
Substrate→
Primer →
0.5 M 3.5
M
Primer →
Cl-
ClO4
-
0.1 1 2 3 4 5 6 7 8
ClO4
- (M)
b
d e
g
a
h
k
j
c
f
i
l
-1.6
-1.2
-0.8
-0.4
0.0
ln
(S/S
0
)
60
50
40
30
20
10
0
Time (min)
4 M ClO4
-
5 M ClO4
-
6 M ClO4
-
7 M ClO4
-
5 M Cl
-
-0.8
-0.6
-0.4
-0.2
0.0
ln
(S/S
0
)
3
2
1
0
Time (hours)
0.00 M ClO4
-
0.05 M ClO4
-
0.20 M ClO4
-
0.50 M ClO4
-
0.20 M Cl
-
30
20
10
0
Product
>
+7
nucleotide
(%)
3.5
3.0
2.5
2.0
1.5
1.0
0.5
Salt [M]
ClO4
-
Cl
-
4
24 nt
10 nt
24 nt
25 nt
19 nt
25 nt
10 nt
18 nt
10 nt
18 nt
12 x 10
3
10
8
6
4
2
0
Δ
Fluorescence
(arb.
units)
0.1 1 2 3 4 5 6 7 8 M
(M)
ClO4
-
Cl
-
4
Fig. 1 | Mesophilic ribozymes are resistant to perchlorate denaturation, while a
mesophilic protein is not. a Cartoon depiction of the hammerhead ribozyme
reaction, cleaving one of its component RNA strands. b Gel images of the ham-
merhead self-cleavage kinetic assay (100 nM of each hammerhead strand A and B,
50 mM Tris-HCl buffer pH 8, and 2.5 mM magnesium) in perchlorate brines,
showing activity is retained at concentrations as high as 6 M perchlorate.
c Graphical representation of (b) with NaCl control. d Cartoon depiction of the
EcoRI protein enzyme reaction, cleaving a double-stranded DNA polymer. e Gel
image of the EcoRI nuclease assay (0.05 U/µL EcoRI, and 1 µM duplex DNA) in
perchlorate solutions. f Graphical representation of d with NaCl control. g The
Broccoli aptamer binds DFHBI-1T, inducing fluorescence. h DFHBI-1T/Broccoli
fluorescence in perchlorate brines with 2 µM Broccoli aptamer, 50 µM DFHBI-1T,
and 10 mM magnesium. i Bar graphs of (g) compared to NaCl controls. j tC19z
ribozyme recruits an RNA template and NTPs to elongate an RNA primer sequence.
k Gel images of RNA primer extension catalyzed by tc19z in different concentra-
tions of sodium perchlorate/chloride. Reactions consisted of 500 nM tC19z,
500 nM template, 500 nM RNA primer, 4 mM nucleotide triphosphates, 50 mM tris-
HCl pH 8.3, 200 mM magnesium. l Graphical representation of k. Error bars
represent the standard error of the mean with n = 3 independent experiments.
Figure 1a, g, and j were created with BioRender.com and released under a Creative
Commons Attribution-NonCommercial-NoDerivs 4.0 International license.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 3
4. we investigated the reversibility of perchlorate-induced denaturation
by examining whether proteins and RNAs could regain functionality
after dilution in perchlorate brines. Among those studied, the ther-
mophilic restriction enzyme TaqI-v2 regained all activity upon dilution
to low salt, the halophilic β-lactamase HaBlap recovered partial activity
(30%), and the mesophilic restriction enzyme EcoRI was irreversibly
denatured, with no activity upon dilution to lower salt (Fig. 2g). In
contrast, the three RNAs studied uniformly recovered activity upon
dilution (Fig. 2h). The Broccoli aptamer and hammerhead ribozyme
exhibited ca. 60% restored activity upon dilution and tC19z recovered
82% of its initial activity. Taken together, these results suggest that
functional RNAs possess salt tolerance comparable to that of the most
extremophilic proteins. This underscores the inherent resilience of
RNA to salt, since these RNAs were selected and evolved in conditions
comparable to those in which the substantially less salt-tolerant
mesophilic proteins evolved.
Perchlorate enables new regulatory functions for ribozymes
In addition to its role in RSLs on present-day Mars, wet-dry cycling has
been proposed as a means of catalyzing biologically relevant prebiotic
reactions, such as polymerization by dehydration-condensation
reactions40
. The wet cycle gathers and solubilizes the necessary com-
ponents, and the dry cycle concentrates them and removes water
produced in the reactions, thereby increasing the rate of reaction.
Prompted by recent findings supporting wet-dry cycles on early Mars
(late Noachian/early Hesperian)4
, we sought to examine the impact of
dilution/concentration cycles of perchlorate brines on ribozyme
activity.
A key function required of emergent life is a homeostatic function
or regulation of metabolic function in response to environmental
conditions. In a model of early Terran life, we previously showed that
the hammerhead ribozyme could exhibit a switchable function in the
presence of short random hexamers of RNA, as would be found in
nonenzymatic RNA polymerization reactions41
. These hexamers bind
to the ribozyme, preventing it from folding and performing its self-
cleavage reaction. In this system, we observed that the dilution
obtained by the growth of model protocells could activate ribozyme
function. Given the lower concentrations of perchlorate thought to
exist in the Noachian era on Mars, we speculated that perchlorate
could enable a similar role, acting as a nondenaturing counterion at
0
Product →
Substrate→
ClO4
-
0.10 M
0.20 M
20 40 60
Time (min)
Product →
Substrate→
- 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
ClO4
- (M)
b
d e
a c
f
h
g
-0.8
-0.6
-0.4
-0.2
0.0
ln
(S/S
0
)
60
40
20
0
Time (min)
0.0 M ClO4
-
0.1 M ClO4
-
0.2 M ClO4
-
0.2 M Cl
-
100
80
60
40
20
β-lactam
hydrolysis
(%)
0 1 2 3 4
(M)
ClO4
-
Cl
-
100
80
60
40
20
0
Relative
Activity
(%)
low → low high → high high → low
Perchlorate Concentration
EcoRI
HaBlap
TaqI-v2 100
80
60
40
20
0
Relative
Activity
(%)
low → low high → high high → low
Perchlorate Concentration
Hammerhead
Broccoli
tC19z
68 nt
11 nt
68 nt
11 nt
Fig. 2 | Recovery of activity by functional RNAs from perchlorate-induced
denaturation is general, while it is limited to only extremophilic protein
enzymes. a Cartoon depiction of TaqI-v2 nuclease cleaving dsDNA. b Gel images of
TaqI-v2 nuclease assay (0.05 U/µL EcoRI, and 1 µM duplex DNA) in perchlorate
solutions showing the enzyme is inactive at 0.2 M perchlorate. c Rate measure-
ments of TaqI-v2 nuclease assay with NaCl control. d HaBlap hydrolase opens a
β-lactam ring. e HaBlap activity assay (5 µM of HaBlap and 50 µM nitrocefin in 5 mM
phosphate buffer pH 7) in perchlorate brines performed with the colorimetric
β-lactamase substrate nitrocefin. f Yields of HaBlap reactions compared to NaCl
controls. g Activity recovery assay performed on the proteins EcoRI, HaBlap, and
TaqI-v2, showing recovery occurs upon dilution from high to low salt only in
extremophilic proteins. High and low perchlorate solutions were 5 and 0.05 M,
respectively. h Activity recovery assay performed on the functional RNAs ham-
merhead ribozyme, Broccoli aptamer, and tC19z ribozyme, showing recovery
occurs upon dilution from high to low salt in all three RNAs. High and low per-
chlorate solutions were 8 and 0.8 M for hammerhead and Broccoli and 5 and 0.5 M
for tC19z. Error bars represent the standard error of the mean with n = 3 inde-
pendent experiments. Figure 2a, d, g, and h created with BioRender.com released
under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 Interna-
tional license.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 4
5. low concentrations. At higher but not saturating concentrations, such
as those found in a drying pool, they could enable the denaturation of
inactive hammerhead-hexamer complexes while still allowing for the
formation of active hammerhead. Consistent with our results in the
model protocell system, we observed loss of hammerhead function at
low salt in the presence of 100 molar equivalents of random hexamers
(Fig. 3a–c; kapp = 0.14 h−1
without hexamers, no product detected with
hexamers). This trend stayed the same when the Hofmeister-neutral
anion chloride was in solution (kapp = 0.39 h-1
without hexamers, no
product detected with hexamers). When modest perchlorate was
present (3 M), we observed restoration of 69% of ribozyme function by
the apparent first-order rate constant (kapp = 0.29 h-1
without hexam-
ers, 0.20 h-1
with hexamers). We also examined hammerhead activity in
solutions with the neutral denaturant urea. The hammerhead ribo-
zyme was completely deactivated in the urea solutions with the same
molarity used with perchlorate (3 M), and in lower concentrations of
urea (1 M) it remained inactive in the presence of interfering hexamers
(Supplementary Fig. 6; kapp = 0.04 h-1
without hexamers, no product
detected with hexamers). These results show perchlorate’s mild
denaturing properties for RNA can dissociate interfering oligomers, as
might be found in a primitive RNA synthesis reaction, without
destroying the ribozyme’s native fold. This type of denaturation would
be ideal in scenarios such as wet-dry cycles where RNA can exhibit
enhanced function upon concentration in perchlorate brines. This
behavior could allow for the dissociation of replication intermediates
in copying reactions performed in dilute solution, allowing for
switching on of functional ribozymes upon concentration.
An RNA-heme holoenzyme catalyzes halogenation reactions
with the oxychlorine species chlorite
Motivated by the emergent functions enabled by perchlorate, we
considered the impact of other oxychlorine species on ribozyme
function. By redox potential alone, perchlorate is characterized as a
strong oxidizing agent (NaClO4/NaClO3 E° = 1.226 V). However, due to
a large electronegative ionic sphere surrounding a kinetically inac-
cessible chlorine center, this compound is inert to both nucleophilic
attack and reduction42
. Numerous investigators have noted per-
chlorate’s lack of reactivity, with one investigator reporting that a ca.
25-year-old bottle of concentrated 72% HClO4 had maintained its acid
titer and showed no sign of chloride buildup over this time42
.
Perchlorate (ClO4
-
) is the highest (+7) oxidation state of chlorine,
but less oxidized oxychlorine species such as chlorite (ClO2,
-
+3) and
hypochlorite (ClO-
, + 1) are thought to be formed in the Martian
chlorine cycle43
. These oxychlorine species are also much more reac-
tive, exhibiting a higher redox potential than perchlorate (NaClO2/
NaClO E° = 1.674 V; NaClO/Cl2 E° = 1.630 V respectively). These com-
pounds can perform halogenation reactions with protein enzymes.
The horseradish peroxidase (HRP) enzyme, which is best known for its
namesake reaction with hydrogen peroxide, can also react with
chlorite (Fig. 4a), performing a complete peroxidase cycle with its
heme (a porphyrin ring with an iron core) cofactor44
. In this reaction
cycle, chlorine dioxide is formed, which can subsequently chlorinate a
range of substrates, such as monochlorodimedon (MCD; Fig. 4b).
Several G quadruplex nucleic acids are well-known to perform
HRP-like peroxidase chemistry. A G quadruplex is a secondary struc-
ture of RNA composed of stacks of quartets of four guanines coordi-
nating a monovalent cation such as potassium (Fig. 4c). This structure
can bind heme (Supplementary Fig. 7a), catalyzing the same perox-
idase reactions as HRP, which we have previously demonstrated in
high-perchlorate solutions using DNA45
. We observed that these reac-
tions also occur in the RNA context with the RNA G quadruplex rPS2.M
even in near-saturated perchlorate solutions of 8 M (Supplementary
Fig. 7b)46,47
. Motivated by these findings, we hypothesized that this
same RNAzyme could also catalyze halogenation reactions.
Accordingly, we assessed the capacity of the rPS2.M/heme
holoenzyme to catalyze chlorination reactions with NaClO2 (Fig. 4d).
To monitor this reaction, we employed monochlorodimedon, a well-
known substrate for enzymatic chlorinations44
. MCD undergoes a loss
of absorption at 290 nm when its 1,3-diketone enolate tautomer is
disrupted upon full chlorination of its α-carbon to dichlorodimedon
(DCD). As we hypothesized, rPS2.M/heme exhibited the expected loss
of MCD absorbance consistent with chlorination (Fig. 4d, e). Analysis
of rPS2.M/heme-catalyzed chlorinations by Job’s method48
of con-
tinuous variation with varied chlorite/MCD ratios showed the reaction
occurred with a stoichiometry of 3 NaClO2:2 MCD (Fig. 4d inset).
Notably, this differs from HRP-catalyzed chlorinations, which occurred
with a 1:1 stoichiometry (Fig. 4b inset). We hypothesize that this dif-
ference in stoichiometry is due to hypochlorous acid accumulating as a
byproduct of the peroxidation cycle. Previous research investigating
the halogenation reaction with HRP has shown that hypochlorous acid
can oxidize heme to Compound I44
, and our results show that HRP is
capable of catalyzing peroxidation cycles of heme using only sodium
hypochlorite, while rPS2.M/heme does not (Supplementary Fig. 8a).
These results indicate that the rPS2.M/heme holoenzyme is mechan-
istically distinct from HRP in chlorination reactions. Notably, the
RNAzyme performed MCD chlorinations faster than HRP, with an
initial apparent first-order rate constant of 1.45 min-1
, 2.5-fold higher
than HRP chlorination (kapp = 0.57 min-1
; Fig. 4e). We also found that
0
Salt
Nil
10 20 30
Time (min)
Product →
Substrate→
Product →
Substrate→
Product →
Substrate→
0 10 20 30
Time (min)
-r(N6) +r(N6)
3 M
Cl-
3 M
ClO4
-
b
a
c
-0.25
-0.20
-0.15
-0.10
-0.05
0.00
ln
(S/S
0
)
30
20
10
0
Time (min)
2.5 mM MgCl2
3.0 M Cl
-
3.0 M ClO4
-
-0.25
-0.20
-0.15
-0.10
-0.05
0.00
ln
(S/S
0
)
30
20
10
0
Time (min)
2.5 mM MgCl2
3.0 M Cl
-
3.0 M ClO4
-
25 nt
19 nt
25 nt
19 nt
25 nt
19 nt
Additional
Fig. 3 | Perchlorate-controlled ribozyme nuclease activity. a Gel images of
hammerhead self-cleavage assay performed in the presence of rN6 and different
chaotropic solutions. Reaction conditions consisted of 200 mM Tris-HCl pH 8,
100 nM Hammerhead strand A and B, 250 µM rN6, 2.5 mM magnesium.
b, c graphical representation of a exhibiting perchlorate denaturing catalytically
unproductive hammerhead-rN6 complexes, allowing hammerhead renaturation
and cleavage. Error bars represent the standard error of the mean with n = 3
independent experiments. Figure 3b, c was created with BioRender.com released
under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 Interna-
tional license.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 5
6. the rPS2.M/heme holoenzyme can withstand up to 5–6 M perchlorate
and still catalyze chlorination of MCD compared to heme alone (Sup-
plementary Fig. 8b–d). HRP was also able to withstand perchlorate in
the 5–6 M range. This enzyme possesses a network of disulfide bonds
stabilizing its fold, providing a potential explanation for its high
stability49
.
Electron transfer biocatalysts must all contend with the fact that
they perform reactions that are potentially destructive to the catalyst
itself50
. We assessed rPS2.M/heme for the maximum turnover number
of the heme cofactor by performing reactions containing excess
rPS2.M and NaClO2. In these reactions, we found that heme underwent
an average turnover number of 12.5 peroxidation cycles before
becoming nonfunctional (Supplementary Fig. 9). Thus, the rPS2.M/
heme holoenzyme is a true, multiple-turnover chlorination ribozyme
catalyst.
We sought to interrogate possible ribozyme-catalyzed chlorina-
tions further by chlorinating a second substrate, phenol red. Phenol
red, a polyaromatic molecule, differs as a chlorination substrate from
MCD, a cyclic 1,3-diketone. When monitored by visible spectroscopy,
phenol red exhibited a change in its absorption spectrum upon reac-
tion with NaClO2 and either HRP or the PS2.M/heme holoenzyme,
consistent with aromatic chlorination and production of chlorophenol
red (and chlorination intermediates, Fig. 4f; Supplementary
Fig. 10a–d). Analyses of these reactions by electrospray mass spec-
trometry (ESI-MS) revealed mono-, di-, and trichlorination products
from both the rPS2.M/heme holoenzyme and HRP (Fig. 4g, h; Sup-
plementary Fig. 10e, f).
Discussion
Here, we have shown experimental evidence that demonstrates RNA is
uniquely well-suited to function within hypersaline oxychlorine brines
like those thought to occur on Mars. This is evident from the fact that
(1) functional RNAs, even when selected in low salt, retain function in
highly concentrated (3–6 M) solutions of perchlorate; (2) perchlorate
enables emergent ribozyme function due to its property of acting as a
mild denaturant for RNA, enabling regulatory behavior; and (3)
chlorite allows a G quadruplex/heme holoenzyme complex to perform
chlorination of organic substrates. These findings add to the growing
number of studies showing that perchlorate is not as deleterious to
biomolecular function as was once thought. For example, perchlorate
has been shown to increase the activity of α-chymotrypsin at low
temperatures by lowering its activation enthalpy51
. Additionally, pres-
sure can reverse the deleterious effects of perchlorate on biomolecular
interactions such as on liquid-liquid phase separation thought to be
necessary for compartmentalization of prebiotic life52
, and even the
binding of small ligands to tRNA53
.
The observation of oxychlorine species in Martian regolith has led
several investigators to seek out perchlorate-tolerant extremophiles in
Mars analog environments on Earth, such as the Atacama Desert in
Chile and Pilot Valley Basin in the United States44,54–56
. The most
perchlorate-tolerant organism found to date is Debaryomyces hansenii
which can grow in solutions up to 2.4 M NaClO426
. Furthermore,
perchlorate-reducing bacteria such as Dechlorospirillum, Azospira, and
Dechloromonas employ perchlorate reductase enzymes using per-
chlorate as an electron acceptor and transforming it to a more reduced
species, such as chloride57,58
. These organisms evolved in the presence
of perchlorate, and their salt tolerance and capacity for employing
perchlorate as an electron acceptor is thought to be an evolutionary
event that followed the last universal common ancestor (LUCA) on
Earth. The survey of the functional landscape of several representative
RNAs and proteins in perchlorate brines presented here shows that
RNA is innately resistant to perchlorate, that it is more resistant to
perchlorate than several mesophilic proteins, and that it possesses this
resistance without the requirement for extended periods of selective
pressure and evolution to retain function in perchlorate brines.
Ions can impact biopolymer folding by indirect classical Hofme-
ister effects caused by affecting the water network. They can also have
direct interactions with biopolymers, such as anions (like perchlorate)
b
a d
g
f
+Cl
+2Cl
+3Cl
+Cl
+2Cl
+3Cl
h
c e
1.6
1.2
0.8
0.4
0.0
Absorbance
340
320
300
280
260
Wavelength (nm)
1
0
Abs
(290
nm)
1
0
[NaClO2] / [MCD] (μM)
[NaClO2] / [MCD]
0.0
↓
1.8
1.0
0.8
0.6
0.4
0.2
0.0
Absorbance
340
320
300
280
260
Wavelength (nm)
1.0
0.5
0.0
Abs
(290
nm)
2.0
1.0
0.0
[NaClO2] / [MCD] (μM)
[NaClO2] / [MCD]
0.0
2.4
↓
1.0
0.8
0.6
0.4
0.2
0.0
Abs
(290
nm)
4
3
2
1
0
Time (min)
water
heme
HRP
PS2.M/heme
1.4
1.2
1.0
0.8
0.6
Abs
(574
nm)
4
3
2
1
0
Time (min)
water
heme
HRP
PS2.M/heme
3000
2000
1000
0
Intensity
460
440
420
400
380
360
340
m/z
10000
5000
0
Intensity
460
440
420
400
380
360
340
m/z
200
100
0
460
440
Fig. 4 | An RNA/heme holoenzyme catalyzes halogenation reactions with
chlorite. a Horseradish peroxidase (HRP) catalyzes a chlorination reaction using
chlorite (ClO2
-
) as an electron acceptor and chlorine donor. b HRP-catalyzed
chlorination of monochlorodimedon (MCD) with titrating amounts of NaClO2. c A
G quadruplex-heme ribozyme (rPS2.M/heme) catalyzes a chlorination reaction
using chlorite. d rPS2.M/heme-catalyzed chlorination of MCD titrating amounts of
chlorite. e Kinetic assay of HRP- and rPS2.M/catalyzed MCD chlorination monitored
by absorbance at 290 nm. The assay was performed with 5 µM catalyst (HRP,
rPS2.M/heme, or just heme), 50 µM MCD, and 100 µM NaClO2 in 100 mM Li-HEPES
pH 7.4. f Kinetic assay of phenol red (50 µM) chlorination monitored by change in
absorbance at 574 nm catalyzed by HRP or rPS2.M/heme with 200 µM NaClO2.
g, h Electrospray ionization mass spectrometry of phenol red after chlorination
reaction catalyzed by HRP (g) and rPS2.M/heme (h +3 Cl product shown in zoomed
inset). Expected molecular weights: 353.05, 387.01, 420.97, and 454.93. Found
molecular weights: 353.1, 387.1, 421.1, and 455.0. Error bars represent the standard
error of the mean with n = 3 independent experiments. Figure 4a was created with
BioRender.com and released under a Creative Commons Attribution-
NonCommercial-NoDerivs 4.0 International license.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 6
7. with hydrophobic residues, which disrupts the hydrophobic collapse
that is critical for protein folding. In nature, many halophilic bacteria
produce proteins that possess surface negative charge, maximizing
their stability in high-salt solution through like-charge repulsion59
. Our
prior work with A-tract containing DNA and bisulfite-catalyzed dea-
mination of cytosine residues is consistent with this model60
. There we
observed enhanced deamination in A-rich sequences with relatively
high surface positive charge, consistent with relaxed electrostatic
repulsion of the bisulfite anion. Similarly, we have also observed
nucleic acid folding within high-salt nonaqueous solvents, such as the
deep eutectic solvent formed by a 2:1 molar mixture of urea and
choline chloride, or the ionic liquid HMIm-BF4
61
. Given that RNA is a
polyanionic molecule, our results agree with a model in which this
polymer is innately resilient to perchlorate denaturation (and salt-
induced denaturation generally), owing to its polyanionic backbone.
Despite perchlorate’s reputation as a strong oxidizer, per-
chlorate is kinetically inert under the reaction conditions tested, with
RNAs ranging from unstructured (polymerization templates), to
moderately structured (hammerhead ribozyme, Broccoli aptamer,
rPS2.M/heme holoenzyme), to highly structured (tC19z ribozyme
polymerase) retaining function. Furthermore, we observed highly
specific chemical transformations in our chlorination reactions. The
RNAs we have studied show resistance to perchlorate-induced loss of
function occurs at concentrations at least 10-fold higher than
mesophilic proteins (EcoRI and RNase HII), an innate ability to refold
after perchlorate-induced denaturation similar to that of thermo-
philic proteins (TaqI-v2) and halotolerance equal to or greater than
that of halophilic proteins (HaBlap). While the protein and RNA
enzymes tested here have been studied under different conditions,
with single-turnover conditions that are standard for hammerhead
ribozyme and multiple-turnover conditions for the protein enzymes
surveyed, the results of this survey are instructive. Given the appar-
ent innate capacity of RNA to resist perchlorate denaturation, we
propose that RNA and related molecules, such as DNA or putative
pre-RNAs with alternative but still polyanionic backbones, exist
within a unique niche of solvent and salt tolerance.
The presence of oxychlorine species during molecular evolution
would thus have afforded a powerful evolutionary advantage to RNA-
based functional behaviors within multiple milieus throughout Mar-
tian history as oxychlorine species started to accumulate43
to the high
concentrations we see today. Such adaptations to these environments
could have been relevant to early or late, as well as prebiotic or biotic
molecular evolution. In any such scenario, our results, and those found
from the studies of extremophilic life on Earth, suggest that Martian
molecular evolution in the presence of high concentrations of per-
chlorate salts would have had a profound impact on the preferred
biopolymers, folds, and catalytic strategies employed in Martian (pre)
biotic chemistry. Further, our observation that RNA-heme complexes
can catalyze carbon-chlorine bond formation extends the chemical
repertoire of known ribozymes to include a key synthetic reaction in
organic chemistry, suggesting that oxychlorine ion-ribozyme interac-
tions could have played a key role in prebiotic chemistry. A rich suite of
chemical transformations is made possible through the agency of
cofactors bound to protein enzymes, and our results extend the
transformations possible with ribozyme-cofactor complexes. This
adds to the growing lines of evidence that as-yet-undiscovered RNA-
cofactor pairs could catalyze a wider range of chemistries than cur-
rently known62,63
.
Numerous forms of RNA-based metabolism on Earth have been
posited as relics of a past RNA world, despite protein having sup-
planted RNA as the principal functional biopolymer in known bio-
chemical systems. These RNA-based systems include machinery
involved in diverse biochemical processes ranging from peptide
synthesis (the peptidyl transfer center of the ribosome in which pep-
tide bonds are formed)64
, RNA splicing (Group I and II introns and self-
cleaving ribozymes)65,66
, and transcriptional and translational control
of gene expression (riboswitches)67
. In the case of the ribosome, the
evolutionary cost of fully replacing the translational machinery is
thought to be so high that a catalyst with only modest rates is still
employed across all known biology. However, in the case of introns,
RNases, and riboswitches, other protein-based machinery is employed
in biological systems with similar functions that appear to be products
of later evolution, but it has not fully replaced its putative ancestral
analogs. For example, the Group I and II introns coexist alongside the
spliceosome, self-cleaving ribozymes, and protein nucleases both
occur in extant biological systems, and riboswitches have not been
fully supplanted by the numerous protein-based regulatory elements
for transcriptional and translational control of gene expression65,67
.
Thus, even in extant biology on Earth, functional biopolymers coexist
in competition with one another, and RNA has not fully ceded all its
putative ancestral roles to proteins. Regardless of whether perchlorate
was present at the advent of a potential Martian biochemistry or a later
event in Martian geochemical evolution, we suggest the unique bio-
polymer folding environment provided by high concentrations of
perchlorate would have provided a powerful selection pressure to
favor further forms of RNA-based functional behaviors on present-
day Mars.
Methods
Oligonucleotides
All oligonucleotides were obtained from Integrated DNA Technologies
(Coralville, IA) with either standard desalting (DNA) or HPLC purifica-
tion (RNA). All oligonucleotide sequences can be found in Supple-
mentary Table 1.
T7 transcription of RNA
Longer RNA molecules were transcribed in-house using T7 RNA poly-
merase. After polymerization, RNA was isolated by treating with
TURBO DNase (Invitrogen, Cat#AM2238) for 30 min at 37 °C, followed
by gel purification (10% urea-PAGE).
Salts and buffers
All salts and buffers used, except where specified, were obtained from
Sigma-Aldrich (Milwaukee, WI) and used as received.
Hammerhead kinetic assay
The hammerhead ribozyme was comprised of two strands (hammer-
head strand A/B; see Supplementary Table 1). The reaction conditions
were 100 nM hammerhead, 50 mM Tris-HCl buffer pH 8, 2.5 mM MgX2
(X = Cl-
or ClO4
-
), and NaCl or NaClO4 added as needed to reach the
final chloride or perchlorate concentration specified in the text. To
reach near-saturated levels of perchlorate/chloride, hammerhead
strand A, and buffer were lyophilized prior to the addition of NaX/
hammerhead strand B. Reactions were started with the addition of
magnesium and incubated at 25 °C. Reactions were stopped with the
addition of 3 volumes of ethanol and 100x molar equivalents of a DNA
complement to strand A to improve electrophoretic separation. The
oligonucleotides were isolated by ethanol precipitation. Cleavage was
monitored using a 5′-fluorescein label on hammerhead strand A, which
was separated on a 20% urea-PAGE gel and visualized using an Omega
Lum G Imaging System (Omega Lum Image Capture Software V
2.1.2017.0). Gel images were quantified using GelQuant (GelQuant.NET
V 1.8.2; Biochemlabsolutions.com) by analyzing the product as a per-
centage of all products.
Short hexamer interference assays were performed by first lyo-
philizing Tris-HCl, hammerhead strand A, and rN6 in the same tube.
Reactions were started by adding hammerhead strand B mixed with
the appropriate concentration of salt described in the text. The final
concentrations were 200 mM Tris-HCl pH 8, 100 nM Hammerhead,
250 µM rN6, 2.5 mM MgX, and variable NaX/urea.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 7
8. Restriction enzyme kinetic assay in NaClO4
EcoRI (New England BioLabs Inc. Cat#R0101S) activity in perchlorate
solutions generally consisted of 0.05 U/µL enzyme, 1X EcoRI buffer
(New England BioLabs Inc. Cat#B7006S), and 1 µM duplex DNA (see
Supplementary Table 1). NaX concentration varied per experiment as
noted in the text. Reactions were started by incubating at 37 °C.
Reactions were stopped and cleaned up with the addition of 75%
ethanol. DNA cleavage was quantified using a 5′-fluorescein label and a
20% urea-PAGE gel.
RNase HII (New England BioLabs Inc. Cat#M0288S) was assessed
with the same protocol but in 1X ThermoPol Buffer (New England
BioLabs Inc. Cat#B9004S).
TaqI-v2 ((New England BioLabs Inc. Cat#R0149S) was assessed
with the same protocol but in 1X rCutSmart Buffer (New England
BioLabs Inc. Cat#B6004S) and incubated at 65 °C. DNA was resolved
on a 10% urea-PAGE gel.
All gels were analyzed using an Omega Lum G Imaging System
using the Omega Lum Image Capture Software V 2.1.2017.0. GelQuant
(GelQuant.NET V 1.8.2) was used for quantification.
Broccoli fluorescence and melting temperature
Samples contained 2 µM Broccoli aptamer, 50 µM DFHBI−1T, 10 mM
MgX2 (X = Cl-
or ClO4
-
), and NaX added to reach the desired levels of
perchlorate/chloride (see text) in a buffer solution of 50 mM Li-HEPES
pH 7.4 (and 5% DMSO from DFHBI−1T stock). To reach near-saturated
levels of perchlorate/chloride, Broccoli oligo, and buffer were lyophi-
lized together prior to resuspension in salt/DFHBI-1T.
The melting traces of the broccoli aptamer were obtained using a
BioRad CFX96 Touch Real-Time PCR Detection System using the
software BioRad CFX Maestro 2.3 V 5.3.022.1030 measuring fluores-
cence every 1 °C in two cycles of 15 → 90 → 15 °C. Melting temperatures
were calculated by fitting a sigmoidal curve to the melting trace in Igor
Pro. Reported fluorescence values in Fig. 1 are from 15 °C of the second
heat curve.
Ribozyme polymerase assay
This assay was performed using a modification of the previously
published procedure36
. Briefly, tC19z and the RNA template strand (see
Supplementary Table 1) were annealed by heating to 80 °C for 2 min
then cooling to 4 °C for 5 min. Nucleotide triphosphates (NTPs), and
Tris-HCl pH 8.3 were mixed in, and the samples were lyophilized. The
reaction was started by adding an RNA primer (5-fluorescein labeled)
and salt solution to the lyophilized samples and incubated at 4 °C for
1 week. The final concentrations of the reaction were 500 nM tC19z,
500 nM template, 500 nM RNA primer, 4 mM NTPs, 50 mM Tris-HCl
pH 8.3, 200 mM MgX2 (X = Cl-
or ClO4
-
), and NaX was added to reach
the perchlorate/chloride concentration described in the text. After
incubation, the RNA was ethanol precipitated. The extended primer
products were displaced from the RNA template by adding 100x molar
equivalents of the template complement strand (DNA) and heated to
80 °C for 4 min. Extended primer products were resolved on a 20%
urea-PAGE and visualized using a 5′-fluorescein labeled primer. Gels
were imaged using an Omega Lum G Imaging System using Omega
Lum Image Capture Software V 2.1.2017.0. Quantification of each band
was obtained using GelQuant software (GelQuant.NET V 1.8.2).
β-lactamase (HaBlap) activity assay
The β-lactamase plasmid (pExp-Bla, Addgene plasmid #112561) was
expressed in E. coli and isolated using nickel agarose beads (Goldbio,
Cat# H-350-5). 5 µM of HaBlap was mixed with 50 µM nitrocefin in 5 mM
phosphate buffer pH 7. Perchlorate salt concentration varied by
experiment. Nitrocefin hydrolysis was monitored on a SpectraMax
340PC384 plate reader (using SoftMax Pro software V 5.4; Molecular
Devices) measuring absorbance at 486 nm and blanked to identical
solutions lacking nitrocefin. Kinetic assays were performed the same
way but with 5 nM HaBlap.
High-salt concentrations affected the extinction coefficient of
hydrolyzed nitrocefin, which distorted the absorbance readings. We
corrected the absorbance readings by incubating nitrocefin with
5 nM HaBlap in buffered solution for 30 min (to fully hydrolyze the
nitrocefin) and then diluting that reaction into an array of sodium
chloride/perchlorate solutions (nitrocefin final concentration:
50 µM). The extinction coefficient was calculated for each salt solu-
tion based on the Beer-Lambert law and graphed (Supplemen-
tary Fig. 11).
Perchlorate recovery assays
All perchlorate recovery assays were performed by incubating the
functional RNA/enzyme in an initial buffered molar perchlorate solu-
tion for 30 min at 4 °C before diluting into a working solution con-
taining the necessary components for their individual assays (see
individual assay requirements above). All recovery assays were nor-
malized to a positive control (low to low samples, Fig. 2g, h) and
compared to a negative control (high to high samples, Fig. 2g, h).
Functional RNAs. Since the hammerhead ribozyme and Broccoli
aptamer were the most tolerant of perchlorate, they received a
starting concentration of 8 M perchlorate and an ending con-
centration of 0.8 M perchlorate (10-fold dilution). The tC19Z ribo-
zyme was less salt tolerant and started in 5 M perchlorate and was
diluted 10-fold to 0.5 M perchlorate. The hammerhead ribozyme
was initially incubated with only NaClO4 and 2.5 mM Mg(ClO4)2 was
added to start the reaction. The Broccoli aptamer dilution/working
solution contained DFHBI-1T. The tC19z ribozyme was initially
incubated with the template and primer strand and the dilution
solution provided the NTPs to the reaction. All positive control
initial solutions contained 0.8 M perchlorate and diluted into a
working solution also containing 0.8 M perchlorate. The negative
controls were the opposite: the initial solution starting concentra-
tion was 8 M perchlorate and the working solution also contained
8 M perchlorate.
Proteins. Since all tested proteins were relatively susceptible to
perchlorate-induced inactivation, 5 M perchlorate was used as the
initial concentration and diluted 100-fold to 0.05 M. For the EcoRI and
TaqI-v2 assays the dilution solution contained their respective DNA
substrate (see Supplementary Table 1). The HaBlap working solution
contained nitrocefin. Positive and negative controls were set up like
those for the functional RNAs but with 0.05 M and 5 M perchlorate
respectively.
Chlorination assays
Kinetic assays. Working solutions generally consisted of 50 µM
monochlorodimedone (MCD), 10 µM G quadruplex RNA (rPS2.M),
5 µM hemin, 2.5% DMSO, 100 mM KCl, and 100 µM NaClO2 in a buffered
solution of 100 mM Li-HEPES pH 7.4. To keep the concentration of
heme consistent, 5 µM horseradish peroxidase (HRP) was used as a
control. The G quadruplex first underwent a heat-cool cycle to attain
the correct configuration: heat to 80 °C and cool to 10 °C at 1-min
intervals every 10 °C. Then the folded rPS2.M was incubated with
hemin for 10 min on ice. The assay was started with the addition of NaX
(X = ClO1
-
or ClO2
-
) and monitored using a Cary 60 UV-Visible spec-
trophotometer (Agilent Technologies; Cary WinUV ADL Shell Appli-
cation V5.0.0.1008). Data was referenced to a blank solution
containing all reaction components except MCD and NaX.
Phenol red chlorination kinetic assays were performed in the
same conditions as those used for MCD but with 50 µM phenol red and
200 µM NaClO2.
Article https://doi.org/10.1038/s41467-024-48037-2
Nature Communications| (2024)15:3863 8
9. Electrospray ionization mass spectrometry
Phenol red was isolated from the chlorination assays by running the
reaction through a Sep-Pak Plus C18 column (Waters Corporation,
Cat#WAT020515), washing with water, and eluting with 35% methanol.
Samples were desiccated and resuspended in 100% methanol. Samples
were analyzed on a Bruker BioTOF II/TOF-MS in negative mode and
2000 spectra were collected using the TOF Control V 2.2 software.
G quadruplex/hemin redox assay
The rPS2.M G quadruplex was heat-cycled to with NaClO4 to attain
proper configuration: heat to 80 °C and cool to 10 °C at 1-min inter-
vals every 10 °C. The sample was then incubated with hemin at room
temperature for 5 min. The G quadruplex/hemin RNAzyme was
allowed to react with 10-Acetyl-3,7-dihydroxyphenoxazine (Amplex
Red, Cayman Chemical Company, Cat#10010469) and Hydrogen
peroxide for 5 min. Fluorescence readings were taken on a Spec-
traMax Gemini EM microplate reader (Molecular Devices; SoftMax
Pro software V 5.4) with an excitation wavelength of 565 nm and an
emission wavelength of 585 nm. Data was normalized to a negative
control containing Amplex Red but no rPS2.M/hemin. Working
solutions contained 5 µM rPS2.M, 1 µM hemin, 5 mM phosphate buffer
pH 7.4, 5 µM Amplex Red, 10 µM H2O2, 0.5% DMSO, and variable
NaClO4.
Data analysis
Data analysis was performed in Igor Pro 9.00.
Reporting summary
Further information on research design is available in the Nature
Portfolio Reporting Summary linked to this article.
Data availability
The raw data generated in this study are provided in the Source Data
file. Source data are provided in this paper.
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Acknowledgements
We thank Loren Williams and members of the Adamala and Engelhart
laboratories for helpful discussions. This work was supported by NASA
Contract 80NSSC18K1139 under the Center for Origin of Life (to A.E.E.
and K.P.A.), Research Corporation for Science Advancement-Scialog
Award 28754 (to A.E.E.), Heising-Simons Foundation-Scialog Award
2021-3123 (to A.E.E.), and National Science Foundation Award 2123465
(to K.P.A.). Diagrams in figures were created with BioRender.com.
Author contributions
T.G.H., M.R.P., N.J.G., G.C.B., T.A.B. performed experiments. T.G.H.
analyzed and prepared all figures. K.P.A. provided ideas and discussion.
T.G.H. and A.E.E. designed the project and wrote the manuscript.
Competing interests
The authors declare no competing interests.
Additional information
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Aaron E. Engelhart.
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