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.
High scientific demand, sustainable management of sea
resources, assessment and monitoring of pollution sources and of
their environmental impact, urgency to understand how does the
biologic processes link to the Carbon cycle and how do they
impact climate: oceanic biologic parameters (primary production,
biomass, and pelagic populations) are in the depths of vital stakes
for our society sustainable development.
Today, Mercator-Ocean is strongly involved in producing
operational bulletins of the physical “blue” ocean. To use new
requirements, it is going to integrate the forecasting of the living
world seas’ component and become more “green”. A first quasireal
time demonstration phase will be launched in the beginning of
2006. LOBSTER biologic model will be integrated in the Mercator
operational chain. This new stage was made possible thanks to
the Bionuts research/operational collaboration. Five structures
contribute to this project: LEGOS (Toulouse), LEGI (Grenoble),
IPSL/OCEAN and IPSL/LSCE (Paris) and the GIP Mercator-
Ocean. In the News, Patrick Monfray & al. present us this project,
its stakes, as well as some recent results.
The three other Newsletter’s articles present an overview of the
Mercator associated research works on the “biology” thematic.
François Royer & al. are interested on the pelagic species’ spatial
dynamic, unavoidable stage for a better management of the sea
resources.
A toxic bloom of the cyanobacteria, Nodularia
spumigena has been reported in the Baltic Sea. On
July 24, 2003, SeaWiFS captured this view of the
blooming Baltic. (credits NASA)
In the scope of the Bionuts project, Leo Berline & al. have studied the assimilation impact (temperature, salinity, sea level)
on the biologic parameters of coupled biology/physical model. In fact, the confrontation of physical models to biology
constraints has revealed some negative effects of the assimilation scheme on the vertical processes performance. So,
improve them is a crucial stake for the biology/physical coupling.
At last, coupling between biologic and physical models is a great opportunity for Scientists to investigate how does the
dynamic impact the biology. Isabelle Dadou & al. have looked at the Rossby waves influence on the primary production.
Have a very good read!
High scientific demand, sustainable management of sea
resources, assessment and monitoring of pollution sources and of
their environmental impact, urgency to understand how does the
biologic processes link to the Carbon cycle and how do they
impact climate: oceanic biologic parameters (primary production,
biomass, and pelagic populations) are in the depths of vital stakes
for our society sustainable development.
Today, Mercator-Ocean is strongly involved in producing
operational bulletins of the physical “blue” ocean. To use new
requirements, it is going to integrate the forecasting of the living
world seas’ component and become more “green”. A first quasireal
time demonstration phase will be launched in the beginning of
2006. LOBSTER biologic model will be integrated in the Mercator
operational chain. This new stage was made possible thanks to
the Bionuts research/operational collaboration. Five structures
contribute to this project: LEGOS (Toulouse), LEGI (Grenoble),
IPSL/OCEAN and IPSL/LSCE (Paris) and the GIP Mercator-
Ocean. In the News, Patrick Monfray & al. present us this project,
its stakes, as well as some recent results.
The three other Newsletter’s articles present an overview of the
Mercator associated research works on the “biology” thematic.
François Royer & al. are interested on the pelagic species’ spatial
dynamic, unavoidable stage for a better management of the sea
resources.
A toxic bloom of the cyanobacteria, Nodularia
spumigena has been reported in the Baltic Sea. On
July 24, 2003, SeaWiFS captured this view of the
blooming Baltic. (credits NASA)
In the scope of the Bionuts project, Leo Berline & al. have studied the assimilation impact (temperature, salinity, sea level)
on the biologic parameters of coupled biology/physical model. In fact, the confrontation of physical models to biology
constraints has revealed some negative effects of the assimilation scheme on the vertical processes performance. So,
improve them is a crucial stake for the biology/physical coupling.
At last, coupling between biologic and physical models is a great opportunity for Scientists to investigate how does the
dynamic impact the biology. Isabelle Dadou & al. have looked at the Rossby waves influence on the primary production.
Have a very good read!
Microbial habitability of Europa sustained by radioactive sources Sérgio Sacani
There is an increasing interest in the icy moons of the Solar System due to their potential habitability and as targets for future exploratory missions, which include astrobiological goals. Several studies have reported new results describing the details of these moons’ geological settings; however, there is still a lack of information regarding the deep subsurface environment of the moons. The purpose of this article is to evaluate the microbial habitability of Europa constrained by terrestrial analogue environments and sustained by radioactive energy provided by natural unstable isotopes. The geological scenarios are based on known deep environments on Earth, and the bacterial ecosystem is based on a sulfatereducing bacterial ecosystem found 2.8 km below the surface in a basin in South Africa. The results show the possibility of maintaining the modeled ecosystem based on the proposed scenarios and provides directions for future models and exploration missions for a more complete evaluation of the habitability of Europa and of icy moons in general.
The divergent fates of primitive hydrospheric water on Earth and MarsSérgio Sacani
Despite active transport into Earth’s mantle, water has been
present on our planet’s surface for most of geological time1,2
.
Yet water disappeared from the Martian surface soon after its
formation. Although some of the water on Mars was lost to space
via photolysis following the collapse of the planet’s magnetic field3–5,
the widespread serpentinization of Martian crust6,7
suggests that
metamorphic hydration reactions played a critical part in the
sequestration of the crust. Here we quantify the relative volumes
of water that could be removed from each planet’s surface via the
burial and metamorphism of hydrated mafic crusts, and calculate
mineral transition-induced bulk-density changes at conditions
of elevated pressure and temperature for each. The metamorphic
mineral assemblages in relatively FeO-rich Martian lavas can
hold about 25 per cent more structurally bound water than those
in metamorphosed terrestrial basalts, and can retain it at greater
depths within Mars. Our calculations suggest that in excess of
9 per cent by volume of the Martian mantle may contain hydrous
mineral species as a consequence of surface reactions, compared to
about 4 per cent by volume of Earth’s mantle. Furthermore, neither
primitive nor evolved hydrated Martian crust show noticeably
different bulk densities compared to their anhydrous equivalents,
in contrast to hydrous mafic terrestrial crust, which transforms
to denser eclogite upon dehydration. This would have allowed
efficient overplating and burial of early Martian crust in a stagnantlid
tectonic regime, in which the lithosphere comprised a single
tectonic plate, with only the warmer, lower crust involved in mantle
convection. This provided an important sink for hydrospheric water
and a mechanism for oxidizing the Martian mantle. Conversely,
relatively buoyant mafic crust and hotter geothermal gradients on
Earth reduced the potential for upper-mantle hydration early in
its geological history, leading to water being retained close to its
surface, and thus creating conditions conducive for the evolution
of complex multicellular life
The Results of the Final Engineering and Geological Studies of the Mass of Ly...YogeshIJTSRD
The results of investigation of morphological, retrospective and prognoses engineering geological tasks concerning loess soils massifs are formulated. The main result of solution of retrospective engineering geological tasks is the proposal of hypothesizes and mechanisms of loess soils subsidence formation. They are the base for four special and general theory of subsidence formation.The result of solution of prognoses engineering geological tasks is the elaboration of methods for calculation the expected subsidence of loess soils massifs under different mode of their wetting and the development of different methods hydrogeomechanical, geochemical, geotechnical and complex of improvement of loess soils massifs properties. J. Ravshanov "The Results of the Final Engineering and Geological Studies of the Mass of Lyoss Grits" Published in International Journal of Trend in Scientific Research and Development (ijtsrd), ISSN: 2456-6470, Special Issue | Innovative Development of Modern Research , April 2021, URL: https://www.ijtsrd.com/papers/ijtsrd40021.pdf Paper URL : https://www.ijtsrd.com/engineering/other/40021/the-results-of-the-final-engineering-and-geological-studies-of-the-mass-of-lyoss-grits/j-ravshanov
Microbial habitability of Europa sustained by radioactive sources Sérgio Sacani
There is an increasing interest in the icy moons of the Solar System due to their potential habitability and as targets for future exploratory missions, which include astrobiological goals. Several studies have reported new results describing the details of these moons’ geological settings; however, there is still a lack of information regarding the deep subsurface environment of the moons. The purpose of this article is to evaluate the microbial habitability of Europa constrained by terrestrial analogue environments and sustained by radioactive energy provided by natural unstable isotopes. The geological scenarios are based on known deep environments on Earth, and the bacterial ecosystem is based on a sulfatereducing bacterial ecosystem found 2.8 km below the surface in a basin in South Africa. The results show the possibility of maintaining the modeled ecosystem based on the proposed scenarios and provides directions for future models and exploration missions for a more complete evaluation of the habitability of Europa and of icy moons in general.
The divergent fates of primitive hydrospheric water on Earth and MarsSérgio Sacani
Despite active transport into Earth’s mantle, water has been
present on our planet’s surface for most of geological time1,2
.
Yet water disappeared from the Martian surface soon after its
formation. Although some of the water on Mars was lost to space
via photolysis following the collapse of the planet’s magnetic field3–5,
the widespread serpentinization of Martian crust6,7
suggests that
metamorphic hydration reactions played a critical part in the
sequestration of the crust. Here we quantify the relative volumes
of water that could be removed from each planet’s surface via the
burial and metamorphism of hydrated mafic crusts, and calculate
mineral transition-induced bulk-density changes at conditions
of elevated pressure and temperature for each. The metamorphic
mineral assemblages in relatively FeO-rich Martian lavas can
hold about 25 per cent more structurally bound water than those
in metamorphosed terrestrial basalts, and can retain it at greater
depths within Mars. Our calculations suggest that in excess of
9 per cent by volume of the Martian mantle may contain hydrous
mineral species as a consequence of surface reactions, compared to
about 4 per cent by volume of Earth’s mantle. Furthermore, neither
primitive nor evolved hydrated Martian crust show noticeably
different bulk densities compared to their anhydrous equivalents,
in contrast to hydrous mafic terrestrial crust, which transforms
to denser eclogite upon dehydration. This would have allowed
efficient overplating and burial of early Martian crust in a stagnantlid
tectonic regime, in which the lithosphere comprised a single
tectonic plate, with only the warmer, lower crust involved in mantle
convection. This provided an important sink for hydrospheric water
and a mechanism for oxidizing the Martian mantle. Conversely,
relatively buoyant mafic crust and hotter geothermal gradients on
Earth reduced the potential for upper-mantle hydration early in
its geological history, leading to water being retained close to its
surface, and thus creating conditions conducive for the evolution
of complex multicellular life
The Results of the Final Engineering and Geological Studies of the Mass of Ly...YogeshIJTSRD
The results of investigation of morphological, retrospective and prognoses engineering geological tasks concerning loess soils massifs are formulated. The main result of solution of retrospective engineering geological tasks is the proposal of hypothesizes and mechanisms of loess soils subsidence formation. They are the base for four special and general theory of subsidence formation.The result of solution of prognoses engineering geological tasks is the elaboration of methods for calculation the expected subsidence of loess soils massifs under different mode of their wetting and the development of different methods hydrogeomechanical, geochemical, geotechnical and complex of improvement of loess soils massifs properties. J. Ravshanov "The Results of the Final Engineering and Geological Studies of the Mass of Lyoss Grits" Published in International Journal of Trend in Scientific Research and Development (ijtsrd), ISSN: 2456-6470, Special Issue | Innovative Development of Modern Research , April 2021, URL: https://www.ijtsrd.com/papers/ijtsrd40021.pdf Paper URL : https://www.ijtsrd.com/engineering/other/40021/the-results-of-the-final-engineering-and-geological-studies-of-the-mass-of-lyoss-grits/j-ravshanov
AP Human Geography: Unit 1 - Introduction to GeographyDaniel Eiland
Here is the Advanced Placement Human Geography Unit1 Powerpoint I will be using to teach my classes this year. It includes the sections "Introduction to Geography", "Tools Geographers Use", and "The Five Themes of Geography". You can find the guided notes for this presentation here: http://www.slideshare.net/deilands/ap-human-geography-unit-1-13583828
Lets start off the new school year in style! This is a re-imagining of an older resource designed to introduce the subject to new students in a highly visual manner. Feel free to use & share it. Check out the links.
As always, any feedback would be really useful.
Thanks, Simon
This Presentation will give you an overview about Artificial Intelligence : definition, advantages , disadvantages , benefits , applications .
We hope it to be useful .
The ppt Sujoy and I made for the Psi Phi ( An Inter School Competition held by our School). Our Topic was Artificial Intelligence.
Credits:
Theme Images from ESET NOD32 (My Antivirus of Choice)
Backgrounds from SwimChick.net (Amazing designs here)
Credits Image from Full Metal Alchemist (One of my favorite Anime).
Introduction to JIRA & Agile Project ManagementDan Chuparkoff
Join me for a brief introduction to JIRA & Agile Project Management. I'll talk about basic Agile concepts. I'll show you basic JIRA planning and working with Scrum and Kanban. And I'll show you the most important reports to master so you can build great software just like Atlassian.
By the year 2050, the world’s population is projected to swell to 9 billion. 80% of us will be urban-dwellers. Demand from developing countries for a wider range of foods is on the rise. Experts estimate that we will need new farmland larger than the size of Brazil to produce enough to meet the demands of growing populations.
Food security therefore represents one of the single biggest challenges of our future, with environmental, economic, political, and lifestyle implications.
How will we fix our broken and unsustainable systems of industrial food production to serve the needs of an ever-growing planet? In what ways will we rethink food via new practices and new technologies? This latest report from the Institute for Customer Experience considers how we are re-imagining our food practices in order to project anew our collective, global future.
Presented at Hofstra University on 3/9/12 in the Leo Guthart Cultural Center Theater. Topics discussed included the evolution of marketing, advertising, and how to best use social media for personal branding use.
10 Steps of Project Management in Digital Agencies Alemsah Ozturk
This is part of our ( 41? 29! ) agency's culture series. Basicly this series of documents helps our teams learn the foundation of agency culture, basic rules to do their work. We are all about sharing the data & know how, so here we are ;)
Start-up Chile Marketing & Advertising Tribe session on Data Analysis tools for startups. Written by Pedro Villalobos (Lagiar.com), Felipe del Sol (Admetricks.com), Liane Siebenhaar (Mewe.co). This is a selection of tools you can use to shape your pitch and product. If you have any questions, don't hesitate to contact us.
Modern water at low latitudes on Mars: Potential evidence from dune surfacesSérgio Sacani
Landforms on the Martian surface are critical to understanding the nature of surface processes in the recent
past. However, modern hydroclimatic conditions on Mars remain enigmatic, as explanations for the formation
of observed landforms are ambiguous. We report crusts, cracks, aggregates, and bright polygonal ridges on the
surfaces of hydrated salt-rich dunes of southern Utopia Planitia (~25°N) from in situ exploration by the Zhurong
rover. These surface features were inferred to form after 1.4 to 0.4 million years ago. Wind and CO2 frost processes can be ruled out as potential mechanisms. Instead, involvement of saline water from thawed frost/snow is
the most likely cause. This discovery sheds light on more humid conditions of the modern Martian climate and
provides critical clues to future exploration missions searching for signs of extant life, particularly at low latitudes with comparatively warmer, more amenable surface temperatures.
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the Solar System is explored, including place where biology might exist.
Geology is the scientific study of the all constituents of planets, their internal and external forms and processes. More precisely, it is the study of nature, structure and history of the planet. Earth is the home to all life, well known to the humankind. Geology, itself, is a major part of The Earth and atmospheric sciences, which were born as twins . The subject of geology encompasses all aspects including the composition, structure, physical properties, and history of a planets'( like Earth's) inter-related components and the processes that are shaping the features on the surface. Geologists are the scientists who study the origin, occurrence, distribution and utilities of all materials(metallic, non-metallic, inorganic, etc), minerals, rocks, sediments, soils, water, oil and all other inorganic natural resources. It is a very vast subject covering a wide spectrum of scientific principles and holding hundred and fifty plus scientific branches. This report enumerates and highlights most of them, in a nutshell, for all those who intends to know for planning their career path.
Three new heteroleptic dithiocarbamate complexes with formula [M(Phen-dione)(Fcdtc)]PF6 (where M ¼
Ni(II) Ni-Fc, Cu(II) Cu-Fc) and [Co(Phen-dione)(Fcdtc)2]PF6 (Co-Fc) (Fcdtc ¼ N-ethanol-Nmethylferrocene
dithiocarbamate and Phen-dione ¼ 1,10-phenanthroline-5,6-dione; PF6
− ¼
hexafluorophosphate) were synthesized and characterized using microanalysis
Crystal Structure, Topological and Hirshfeld Surface Analysis of a Zn(II) Zwi...Awad Albalwi
Abstract: A mononuclear Zn(II) complex of (Zn(H2L) (CH3OH) Cl2
) (1) has been synthesized by using
a nonlinear optically active Zwitterionic Schiff base which is 4-((2-hydroxy-3-methoxybenzylidene)
amino) benzoic acid (H2L). Complex 1 has been structurally analyzed by FTIR and UV spectroscopy,
TGA, Powder-XRD and single crystal X-ray diffraction. X-Ray crystallographic studies revealed Zn(II)
complex crystallizes in a P21/c space group and exists in a distorted trigonal bipyramidal geometry
(τ = 0.68).
What evidence is there for water on mars 2009Awad Albalwi
Historical background and definition.
evidence(1) - sulphate salt .
evidence(2) - Sheet of water ice
evidence(3) – New deposits in craters
evidence(4) - Water-ice clouds
evidence(5) - Vapour water over the polar cap
Evidence (6)- Water vapour over the four big volcanoes
Application of Statistical and mathematical equations in Chemistry -Part 6Awad Albalwi
Application of Statistical and mathematical equations in Chemistry Part 6
Strong Acid and Base Titrations, Weak Acid and Strong Base Titration, Strong Acid and Weak Base Titrations ,Precipitation
Percentage calculation
Application of Statistical and mathematical equations in Chemistry -Part 6Awad Albalwi
Application of Statistical and mathematical equations in Chemistry Part 6
Strong Acid and Base Titrations .Weak Acid and Strong Base Titration ,Strong Acid and Weak Base Titrations ,Precipitation
Percentage calculation
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.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
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.