1) New measurements of tungsten isotopes in lunar rocks indicate that the Moon formed later than previously thought, between 62-150 million years after the formation of the solar system, challenging current models of early planetary formation.
2) This later formation of the Moon requires revising our understanding of the timing of events like the giant impact that formed the Earth-Moon system and the solidification of the lunar magma ocean.
3) The new timeline suggests Earth's core may have formed independently of the giant impact and that magma oceans on Earth and other terrestrial planets took longer to solidify than models predicted.
The document provides an overview of a course on Earth science and the universe. It includes 12 lessons covering topics like mapping the seafloor, plate tectonics, earthquakes and volcanoes, the origin of the universe, the solar system, what we are made of, the extinction of dinosaurs, and whether life exists elsewhere. The first lesson introduces concepts of time, space, the structure of Earth, and the rock cycle. Subsequent lessons will explore these topics in more depth.
The document reports on the Kepler-47 system which consists of two planets orbiting an eclipsing binary star system. The inner planet has a radius of 3.0 Earth radii and orbits every 49.5 days, while the outer planet has a radius of 4.6 Earth radii and orbits every 303.2 days. Eighteen transits of the inner planet were observed, allowing for a detailed characterization of its orbit and that of the binary stars. The timing and duration of the transits vary, indicating the planets orbit both stars in the binary system. Kepler-47 establishes that circumbinary planetary systems can exist around close binary star systems.
Origin and Abundance of elements in the Solar system and in the Earth and its...AkshayRaut51
Definition of Elements and atom
Origin of Universe
Theories of origin of Solar system and Earth
Chemical Composition of Planets
Chemical Composition of Earth
Chemical composition of Meteorites
Abundance of Elements
The document discusses methods that scientists use to determine the age of the Earth. It explains that radiometric dating is used to measure the decay of radioactive isotopes in rocks and minerals to estimate their age. While this provides a means to directly date some igneous rocks, most rocks cannot be directly dated and must be bracketed between dated materials. The document reviews several examples of dated rocks and materials. Though radiometric dating provides a framework, determining the exact age of the Earth remains an ongoing effort as techniques are refined.
Isotopic evolution of the protoplanetary disk and the building blocks of Eart...Sérgio Sacani
Nucleosynthetic isotope variability among Solar System objects
is often used to probe the genetic relationship between meteorite
groups and the rocky planets (Mercury, Venus, Earth and Mars),
which, in turn, may provide insights into the building blocks
of the Earth–Moon system1–5. Using this approach, it has been
inferred that no primitive meteorite matches the terrestrial
composition and the protoplanetary disk material from which
Earth and the Moon accreted is therefore largely unconstrained6
.
This conclusion, however, is based on the assumption that the
observed nucleosynthetic variability of inner-Solar-System objects
predominantly reflects spatial heterogeneity. Here we use the
isotopic composition of the refractory element calcium to show that
the nucleosynthetic variability in the inner Solar System primarily
reflects a rapid change in the mass-independent calcium isotope
composition of protoplanetary disk solids associated with early
mass accretion to the proto-Sun. We measure the mass-independent
48Ca/44Ca ratios of samples originating from the parent bodies of
ureilite and angrite meteorites, as well as from Vesta, Mars and
Earth, and find that they are positively correlated with the masses
of their parent asteroids and planets, which are a proxy of their
accretion timescales. This correlation implies a secular evolution of
the bulk calcium isotope composition of the protoplanetary disk in
the terrestrial planet-forming region. Individual chondrules from
ordinary chondrites formed within one million years of the collapse
of the proto-Sun7
reveal the full range of inner-Solar-System massindependent
48Ca/44Ca ratios, indicating a rapid change in the
composition of the material of the protoplanetary disk. We infer
that this secular evolution reflects admixing of pristine outer-SolarSystem
material into the thermally processed inner protoplanetary
disk associated with the accretion of mass to the proto-Sun. The
identical calcium isotope composition of Earth and the Moon
reported here is a prediction of our model if the Moon-forming
impact involved protoplanets or precursors that completed their
accretion near the end of the protoplanetary disk’s lifetime.
1) The oldest rocks on Earth are around 3.7-3.8 billion years old based on radiometric dating.
2) Even older zircon crystals around 4.0-4.2 billion years have been found embedded in younger rocks.
3) The best estimate for the age of the Earth itself comes from lead isotope dating of meteorites, yielding an age of 4.54 billion years.
Are the creation ministries shooting straight with usTimothy Helble
Each week, thousands of people attend “creation conferences” put on by various young earth creation ministries and hear convincing-sounding arguments for a recent creation (6,000 years ago) and against what they broadly refer to as evolution. These young earth presenters talk just like us and share our spiritual beliefs, so we’d much rather believe them than the host of intellectual-sounding scientists who tell us that the Earth and our universe is very old. In my opinion, the young earth creation ministries have not been truthful with Christians at these conferences and it is time to call them to task for this. Can I substantiate my claim with solid evidence that doesn’t rest on opinions? Review this presentation and see for yourself.
1. The formation and evolution of the Solar System began about 4.57 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center to form the Sun, while the rest flattened into a protoplanetary disk from which the planets, moons, asteroids and other small bodies formed.
2. According to the nebular hypothesis, Earth formed about 4.54 billion years ago from accretion of planetary material in the solar nebula. Within the first 100-200 million years, early Earth had formed extensive oceans and seas.
3. Key events in the development of early Earth included the formation of its layered internal structure through the sinking of
The document provides an overview of a course on Earth science and the universe. It includes 12 lessons covering topics like mapping the seafloor, plate tectonics, earthquakes and volcanoes, the origin of the universe, the solar system, what we are made of, the extinction of dinosaurs, and whether life exists elsewhere. The first lesson introduces concepts of time, space, the structure of Earth, and the rock cycle. Subsequent lessons will explore these topics in more depth.
The document reports on the Kepler-47 system which consists of two planets orbiting an eclipsing binary star system. The inner planet has a radius of 3.0 Earth radii and orbits every 49.5 days, while the outer planet has a radius of 4.6 Earth radii and orbits every 303.2 days. Eighteen transits of the inner planet were observed, allowing for a detailed characterization of its orbit and that of the binary stars. The timing and duration of the transits vary, indicating the planets orbit both stars in the binary system. Kepler-47 establishes that circumbinary planetary systems can exist around close binary star systems.
Origin and Abundance of elements in the Solar system and in the Earth and its...AkshayRaut51
Definition of Elements and atom
Origin of Universe
Theories of origin of Solar system and Earth
Chemical Composition of Planets
Chemical Composition of Earth
Chemical composition of Meteorites
Abundance of Elements
The document discusses methods that scientists use to determine the age of the Earth. It explains that radiometric dating is used to measure the decay of radioactive isotopes in rocks and minerals to estimate their age. While this provides a means to directly date some igneous rocks, most rocks cannot be directly dated and must be bracketed between dated materials. The document reviews several examples of dated rocks and materials. Though radiometric dating provides a framework, determining the exact age of the Earth remains an ongoing effort as techniques are refined.
Isotopic evolution of the protoplanetary disk and the building blocks of Eart...Sérgio Sacani
Nucleosynthetic isotope variability among Solar System objects
is often used to probe the genetic relationship between meteorite
groups and the rocky planets (Mercury, Venus, Earth and Mars),
which, in turn, may provide insights into the building blocks
of the Earth–Moon system1–5. Using this approach, it has been
inferred that no primitive meteorite matches the terrestrial
composition and the protoplanetary disk material from which
Earth and the Moon accreted is therefore largely unconstrained6
.
This conclusion, however, is based on the assumption that the
observed nucleosynthetic variability of inner-Solar-System objects
predominantly reflects spatial heterogeneity. Here we use the
isotopic composition of the refractory element calcium to show that
the nucleosynthetic variability in the inner Solar System primarily
reflects a rapid change in the mass-independent calcium isotope
composition of protoplanetary disk solids associated with early
mass accretion to the proto-Sun. We measure the mass-independent
48Ca/44Ca ratios of samples originating from the parent bodies of
ureilite and angrite meteorites, as well as from Vesta, Mars and
Earth, and find that they are positively correlated with the masses
of their parent asteroids and planets, which are a proxy of their
accretion timescales. This correlation implies a secular evolution of
the bulk calcium isotope composition of the protoplanetary disk in
the terrestrial planet-forming region. Individual chondrules from
ordinary chondrites formed within one million years of the collapse
of the proto-Sun7
reveal the full range of inner-Solar-System massindependent
48Ca/44Ca ratios, indicating a rapid change in the
composition of the material of the protoplanetary disk. We infer
that this secular evolution reflects admixing of pristine outer-SolarSystem
material into the thermally processed inner protoplanetary
disk associated with the accretion of mass to the proto-Sun. The
identical calcium isotope composition of Earth and the Moon
reported here is a prediction of our model if the Moon-forming
impact involved protoplanets or precursors that completed their
accretion near the end of the protoplanetary disk’s lifetime.
1) The oldest rocks on Earth are around 3.7-3.8 billion years old based on radiometric dating.
2) Even older zircon crystals around 4.0-4.2 billion years have been found embedded in younger rocks.
3) The best estimate for the age of the Earth itself comes from lead isotope dating of meteorites, yielding an age of 4.54 billion years.
Are the creation ministries shooting straight with usTimothy Helble
Each week, thousands of people attend “creation conferences” put on by various young earth creation ministries and hear convincing-sounding arguments for a recent creation (6,000 years ago) and against what they broadly refer to as evolution. These young earth presenters talk just like us and share our spiritual beliefs, so we’d much rather believe them than the host of intellectual-sounding scientists who tell us that the Earth and our universe is very old. In my opinion, the young earth creation ministries have not been truthful with Christians at these conferences and it is time to call them to task for this. Can I substantiate my claim with solid evidence that doesn’t rest on opinions? Review this presentation and see for yourself.
1. The formation and evolution of the Solar System began about 4.57 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center to form the Sun, while the rest flattened into a protoplanetary disk from which the planets, moons, asteroids and other small bodies formed.
2. According to the nebular hypothesis, Earth formed about 4.54 billion years ago from accretion of planetary material in the solar nebula. Within the first 100-200 million years, early Earth had formed extensive oceans and seas.
3. Key events in the development of early Earth included the formation of its layered internal structure through the sinking of
The Search for Distant Objects in the Solar System Using Spacewatch - Astrono...Eric Roe
This document describes a survey conducted by the Spacewatch Project to search for distant and slow-moving bright objects in the outer solar system beyond Neptune. The survey used data taken over 34 months with multiple night detections to achieve sensitivity to motions as slow as 0.012 arcsec/hr. This allowed the survey to be sensitive to Mars-sized objects out to 300 AU and Jupiter-sized planets out to 1200 AU. No large objects were found at low inclinations despite having sufficient sensitivity, allowing the authors to rule out more than one or two Pluto-sized objects to 100 AU and one or two Mars-sized objects to 200 AU for low inclinations.
1. The document discusses several theories regarding the age of the Earth, including that some scientists believe it is approximately 4.6 billion years old based on evidence from fossils and geology, while some creationists believe it is only around 10,000 years old based on historical documents and some scientific evidence.
2. The document also discusses theories of how life on Earth originated, such as the primordial soup theory that early Earth's atmosphere allowed organic molecules to form, and the endosymbiont theory that early cells incorporated aerobic bacteria in a symbiotic relationship.
3. Determining the age of the Earth and theories of the origin of life involve assumptions and can never be proven absolutely, as scientists with different beliefs
The document discusses the history of determining the age of the Earth. Early estimates ranged from thousands to billions of years based on different methods and assumptions. In the late 19th century, radioactive dating methods were developed that provided evidence the Earth was millions to billions of years old, conflicting with a literal reading of the Bible. This sparked debates around assumptions made in dating methods and their application to estimating the Earth's age. While techniques have improved, disagreement remains on interpreting results within biblical or long-age frameworks.
The document discusses a lesson about what killed the dinosaurs. It presents two main explanations - an asteroid impact 65 million years ago, and a supervolcanic eruption. While the asteroid theory is supported by iridium found in rocks from that period, dinosaurs were already declining before the impact. The extinction cleared the way for mammals, and studying fossils helps understand which species were lost and emerged after.
La historia de la vida en la Tierra y en otras plataformas planetarios potenciales portadoras de vida están profundamente ligadas a la historia del Universo. Puesto que la vida, tal como la conocemos, se basa en elementos químicos forjados en estrellas pesadas moribundas, el Universo tiene que ser lo suficientemente antiguo para que las estrellas se formaran y evolucionaran. La teoría cosmológica actual indica que el Universo es de 13,7 ± 0,13 mil millones de años y que las primeras estrellas se formaron cientos de millones de años después del Big Bang. En este trabajo, se argumenta que podemos dividir la historia cosmológica en cuatro edades, desde el Big Bang a la vida inteligente.
Main points of The Grand Canyon Monument to an Ancient EarthTimothy Helble
This presentation presents the 177 main points of the book "The Grand Canyon Monument to an Ancient Earth, Can Noah's Flood Explain the Grand Canyon?" 120 of the main points are direct refutations of flood geology, most of the remaining ones can be considered to be indirect refutations of flood geology. This presentation was compiled by Tim Helble, one of the editors and authors of the book and has been coordinated with the other 10 authors.
The document summarizes research on the South Pole-Aitken basin, the largest impact crater on the Moon. It is over 2,500 km in diameter and more than 12 km deep. Spacecraft data show the basin has a higher concentration of iron than surrounding lunar highlands, suggesting it may expose deeper mantle rocks. However, the exact composition is debated, with some researchers arguing mantle rocks are not present based on mineral analysis. Understanding the basin's composition could provide insights into the Moon's interior structure and composition from the impact that formed the giant crater.
Geologists used new evidence from physics, including radioactive dating and heat sources within the Earth, to show that the Earth was older than physicists had estimated based on cooling models alone. Lord Kelvin had estimated the Earth's age as between 20-40 million years based on cooling rates, but radioactive elements provided additional heat sources and evidence that the Earth was at least 1.6 billion years old. By considering multiple heat sources and dating methods, geologists and physicists reconciled differing age estimates to establish that the Earth was over 3 billion years old.
The document discusses methods for determining the age of the Earth by examining fossils and rock layers. It describes how fossils are formed by rapid burial after death, and how studying the layers they are found in can reveal the conditions of the Earth during different time periods. Index fossils that are unique to a specific layer are useful for correlating the ages of different rock formations. The fossil record also provides evidence that species have evolved over long periods of time. Radiometric dating techniques allow scientists to directly determine the ages of rocks and provide evidence that the Earth is very old.
Are the creation ministries shooting straight with us (200 dpi)Tim Helble
This presentation looks at several cases where it can be readily demonstrated that the young earth creation ministries are not being honest with their Christian audience.
The two largest impact basins recently discovered at Vesta's south pole are Rheasilvia and Veneneia. Rheasilvia is ~500 km wide and 19 km deep, making it one of the largest impact features on Vesta. It has a central massif and spiral ridge patterns on its floor. Veneneia is an older, partially buried ~400 km basin located beneath Rheasilvia. Crater counts date both basins to 1-2 billion years old, indicating major geological resetting of Vesta occurred relatively recently.
This document provides an overview of a module on plate tectonics that includes the following:
1) The module covers topics on evidence of plate tectonics and managing effects of natural phenomena associated with plate tectonics through 4 lessons on the structure of Earth, formation of continents, earthquakes, and volcanoes.
2) Students will complete a pre-assessment on their understanding of the structure of Earth, movement of tectonic plates, earthquakes, and volcanoes from elementary science.
3) The module will help students develop a better understanding of plate tectonics to inform decisions on managing effects of natural phenomena through acquiring scientific knowledge from the lessons and activities.
This document provides information about geochronology and dating the age of the Earth. It discusses how the Earth is estimated to be 4.6 billion years old based on dating of meteorites and the oldest Earth rocks. It describes the principles of relative dating methods like superposition and cross-cutting relationships. It also explains numerical dating techniques using radioactive isotopes like potassium-argon and uranium-lead dating to assign absolute ages to rocks in millions or billions of years. Finally, it briefly discusses isostatic adjustment and two hypotheses about isostasy proposed by J.H. Pratt and G.B. Airy.
Geologists used various dating methodologies involving ocean chemistry, erosion rates, and radiometric dating to determine that the Earth is billions of years old, contradicting earlier estimates by physicists like Kelvin of only millions of years based on cooling models. The discovery of radioactivity provided a major new heat source inside the Earth and revealed processes like radioactive decay that allowed for much older dating of rocks and minerals, establishing the age of the Earth to be over 4 billion years.
The document examines various hypotheses regarding the origin of life on Earth, such as abiogenesis, the RNA world, and panspermia. It discusses early Earth conditions and the emergence of the earliest life forms. While panspermia provides a favored hypothesis for how life began on our planet, the document concludes that delivery of organic molecules by comets alone was likely not sufficient and that additional triggers were needed to initiate life.
Were Most of Earth's Fossil-Bering Sedimentary Rock Layers Deposited by Noah'...Tim Helble
This presentation uses the Coconino Sandstone to evaluate the question of whether it is quantitatively reasonable for sedimentary formations to have been deposited by Noah's Flood.
The document summarizes findings from studying asteroid 4 Vesta using data from NASA's Dawn spacecraft. It finds that Vesta has experienced a violent collisional history, with large impacts creating steep slopes and resurfacing much of the surface. While no unambiguous volcanic deposits were found, some dark material in impact craters may be from excavated subsurface volcanic features. Smooth ponds found on Vesta are also seen on asteroid Eros and are thought to form from impact ejecta collecting in depressions.
The document discusses the history of determining the age of the Earth. It begins with pre-scientific beliefs that the Earth was only a few thousand years old based on biblical accounts. Starting in the 1600s, scholars began speculating on the Earth's origins but with little field work. In the late 1600s, Steno formulated principles of stratigraphy and rock layering that helped establish relative dating of formations. By the 1700-1800s, studies of strata, fossils, earthquakes, and erosion led to acceptance that the Earth was much older than previously believed. Radiometric dating methods developed in the 1800s-1900s allowed estimation of absolute ages, showing the Earth to be billions of years old.
The nebular theory proposes that the solar system formed from a large cloud of gas and dust called a solar nebula. Originally put forward by Immanuel Kant in 1775, it was later expanded on by Pierre-Simon Laplace. The theory suggests that the solar nebula collapsed under gravity and began rotating, flattening into a disk. Matter in the center condensed to form the Sun while the outer edges cooled to form planets. Modern astronomers generally accept a modified theory known as the condensation theory, which incorporates the role of dust in cooling the nebula and providing nuclei for matter to accumulate and form protoplanets.
This document discusses evidence that the Moon-forming impact occurred later than previously thought, at around 95 million years after the formation of the solar system. The study uses simulations of planetary formation to show a correlation between the timing of the last giant impact and the amount of mass later accreted by the planet. Comparing this to highly siderophile element abundances in Earth's mantle, which constrain the amount of late-accreted mass, the study determines the Moon-forming impact was most likely 95 million years after solar system formation. Earlier times of 40 million years or less are ruled out at a 99.9% confidence level. The simulations include both classical scenarios and scenarios where Jupiter and Saturn migrated inward early in the solar
The document summarizes the evolution of Earth from its formation to present day. It describes how:
- Dust and gas coalesced from the solar nebula to form planetesimals and eventually Earth around 4.5 billion years ago.
- Early Earth was mostly molten due to heavy bombardment and radioactive decay. The heat allowed the planet to differentiate into a core, mantle, and crust.
- As Earth cooled, water and an atmosphere formed. Photosynthetic life evolved and increased oxygen in the atmosphere around 2.4 billion years ago.
- Plate tectonics and volcanism have continuously recycled Earth's crust and regulated temperatures and atmospheric gases through geologic time.
The Search for Distant Objects in the Solar System Using Spacewatch - Astrono...Eric Roe
This document describes a survey conducted by the Spacewatch Project to search for distant and slow-moving bright objects in the outer solar system beyond Neptune. The survey used data taken over 34 months with multiple night detections to achieve sensitivity to motions as slow as 0.012 arcsec/hr. This allowed the survey to be sensitive to Mars-sized objects out to 300 AU and Jupiter-sized planets out to 1200 AU. No large objects were found at low inclinations despite having sufficient sensitivity, allowing the authors to rule out more than one or two Pluto-sized objects to 100 AU and one or two Mars-sized objects to 200 AU for low inclinations.
1. The document discusses several theories regarding the age of the Earth, including that some scientists believe it is approximately 4.6 billion years old based on evidence from fossils and geology, while some creationists believe it is only around 10,000 years old based on historical documents and some scientific evidence.
2. The document also discusses theories of how life on Earth originated, such as the primordial soup theory that early Earth's atmosphere allowed organic molecules to form, and the endosymbiont theory that early cells incorporated aerobic bacteria in a symbiotic relationship.
3. Determining the age of the Earth and theories of the origin of life involve assumptions and can never be proven absolutely, as scientists with different beliefs
The document discusses the history of determining the age of the Earth. Early estimates ranged from thousands to billions of years based on different methods and assumptions. In the late 19th century, radioactive dating methods were developed that provided evidence the Earth was millions to billions of years old, conflicting with a literal reading of the Bible. This sparked debates around assumptions made in dating methods and their application to estimating the Earth's age. While techniques have improved, disagreement remains on interpreting results within biblical or long-age frameworks.
The document discusses a lesson about what killed the dinosaurs. It presents two main explanations - an asteroid impact 65 million years ago, and a supervolcanic eruption. While the asteroid theory is supported by iridium found in rocks from that period, dinosaurs were already declining before the impact. The extinction cleared the way for mammals, and studying fossils helps understand which species were lost and emerged after.
La historia de la vida en la Tierra y en otras plataformas planetarios potenciales portadoras de vida están profundamente ligadas a la historia del Universo. Puesto que la vida, tal como la conocemos, se basa en elementos químicos forjados en estrellas pesadas moribundas, el Universo tiene que ser lo suficientemente antiguo para que las estrellas se formaran y evolucionaran. La teoría cosmológica actual indica que el Universo es de 13,7 ± 0,13 mil millones de años y que las primeras estrellas se formaron cientos de millones de años después del Big Bang. En este trabajo, se argumenta que podemos dividir la historia cosmológica en cuatro edades, desde el Big Bang a la vida inteligente.
Main points of The Grand Canyon Monument to an Ancient EarthTimothy Helble
This presentation presents the 177 main points of the book "The Grand Canyon Monument to an Ancient Earth, Can Noah's Flood Explain the Grand Canyon?" 120 of the main points are direct refutations of flood geology, most of the remaining ones can be considered to be indirect refutations of flood geology. This presentation was compiled by Tim Helble, one of the editors and authors of the book and has been coordinated with the other 10 authors.
The document summarizes research on the South Pole-Aitken basin, the largest impact crater on the Moon. It is over 2,500 km in diameter and more than 12 km deep. Spacecraft data show the basin has a higher concentration of iron than surrounding lunar highlands, suggesting it may expose deeper mantle rocks. However, the exact composition is debated, with some researchers arguing mantle rocks are not present based on mineral analysis. Understanding the basin's composition could provide insights into the Moon's interior structure and composition from the impact that formed the giant crater.
Geologists used new evidence from physics, including radioactive dating and heat sources within the Earth, to show that the Earth was older than physicists had estimated based on cooling models alone. Lord Kelvin had estimated the Earth's age as between 20-40 million years based on cooling rates, but radioactive elements provided additional heat sources and evidence that the Earth was at least 1.6 billion years old. By considering multiple heat sources and dating methods, geologists and physicists reconciled differing age estimates to establish that the Earth was over 3 billion years old.
The document discusses methods for determining the age of the Earth by examining fossils and rock layers. It describes how fossils are formed by rapid burial after death, and how studying the layers they are found in can reveal the conditions of the Earth during different time periods. Index fossils that are unique to a specific layer are useful for correlating the ages of different rock formations. The fossil record also provides evidence that species have evolved over long periods of time. Radiometric dating techniques allow scientists to directly determine the ages of rocks and provide evidence that the Earth is very old.
Are the creation ministries shooting straight with us (200 dpi)Tim Helble
This presentation looks at several cases where it can be readily demonstrated that the young earth creation ministries are not being honest with their Christian audience.
The two largest impact basins recently discovered at Vesta's south pole are Rheasilvia and Veneneia. Rheasilvia is ~500 km wide and 19 km deep, making it one of the largest impact features on Vesta. It has a central massif and spiral ridge patterns on its floor. Veneneia is an older, partially buried ~400 km basin located beneath Rheasilvia. Crater counts date both basins to 1-2 billion years old, indicating major geological resetting of Vesta occurred relatively recently.
This document provides an overview of a module on plate tectonics that includes the following:
1) The module covers topics on evidence of plate tectonics and managing effects of natural phenomena associated with plate tectonics through 4 lessons on the structure of Earth, formation of continents, earthquakes, and volcanoes.
2) Students will complete a pre-assessment on their understanding of the structure of Earth, movement of tectonic plates, earthquakes, and volcanoes from elementary science.
3) The module will help students develop a better understanding of plate tectonics to inform decisions on managing effects of natural phenomena through acquiring scientific knowledge from the lessons and activities.
This document provides information about geochronology and dating the age of the Earth. It discusses how the Earth is estimated to be 4.6 billion years old based on dating of meteorites and the oldest Earth rocks. It describes the principles of relative dating methods like superposition and cross-cutting relationships. It also explains numerical dating techniques using radioactive isotopes like potassium-argon and uranium-lead dating to assign absolute ages to rocks in millions or billions of years. Finally, it briefly discusses isostatic adjustment and two hypotheses about isostasy proposed by J.H. Pratt and G.B. Airy.
Geologists used various dating methodologies involving ocean chemistry, erosion rates, and radiometric dating to determine that the Earth is billions of years old, contradicting earlier estimates by physicists like Kelvin of only millions of years based on cooling models. The discovery of radioactivity provided a major new heat source inside the Earth and revealed processes like radioactive decay that allowed for much older dating of rocks and minerals, establishing the age of the Earth to be over 4 billion years.
The document examines various hypotheses regarding the origin of life on Earth, such as abiogenesis, the RNA world, and panspermia. It discusses early Earth conditions and the emergence of the earliest life forms. While panspermia provides a favored hypothesis for how life began on our planet, the document concludes that delivery of organic molecules by comets alone was likely not sufficient and that additional triggers were needed to initiate life.
Were Most of Earth's Fossil-Bering Sedimentary Rock Layers Deposited by Noah'...Tim Helble
This presentation uses the Coconino Sandstone to evaluate the question of whether it is quantitatively reasonable for sedimentary formations to have been deposited by Noah's Flood.
The document summarizes findings from studying asteroid 4 Vesta using data from NASA's Dawn spacecraft. It finds that Vesta has experienced a violent collisional history, with large impacts creating steep slopes and resurfacing much of the surface. While no unambiguous volcanic deposits were found, some dark material in impact craters may be from excavated subsurface volcanic features. Smooth ponds found on Vesta are also seen on asteroid Eros and are thought to form from impact ejecta collecting in depressions.
The document discusses the history of determining the age of the Earth. It begins with pre-scientific beliefs that the Earth was only a few thousand years old based on biblical accounts. Starting in the 1600s, scholars began speculating on the Earth's origins but with little field work. In the late 1600s, Steno formulated principles of stratigraphy and rock layering that helped establish relative dating of formations. By the 1700-1800s, studies of strata, fossils, earthquakes, and erosion led to acceptance that the Earth was much older than previously believed. Radiometric dating methods developed in the 1800s-1900s allowed estimation of absolute ages, showing the Earth to be billions of years old.
The nebular theory proposes that the solar system formed from a large cloud of gas and dust called a solar nebula. Originally put forward by Immanuel Kant in 1775, it was later expanded on by Pierre-Simon Laplace. The theory suggests that the solar nebula collapsed under gravity and began rotating, flattening into a disk. Matter in the center condensed to form the Sun while the outer edges cooled to form planets. Modern astronomers generally accept a modified theory known as the condensation theory, which incorporates the role of dust in cooling the nebula and providing nuclei for matter to accumulate and form protoplanets.
This document discusses evidence that the Moon-forming impact occurred later than previously thought, at around 95 million years after the formation of the solar system. The study uses simulations of planetary formation to show a correlation between the timing of the last giant impact and the amount of mass later accreted by the planet. Comparing this to highly siderophile element abundances in Earth's mantle, which constrain the amount of late-accreted mass, the study determines the Moon-forming impact was most likely 95 million years after solar system formation. Earlier times of 40 million years or less are ruled out at a 99.9% confidence level. The simulations include both classical scenarios and scenarios where Jupiter and Saturn migrated inward early in the solar
The document summarizes the evolution of Earth from its formation to present day. It describes how:
- Dust and gas coalesced from the solar nebula to form planetesimals and eventually Earth around 4.5 billion years ago.
- Early Earth was mostly molten due to heavy bombardment and radioactive decay. The heat allowed the planet to differentiate into a core, mantle, and crust.
- As Earth cooled, water and an atmosphere formed. Photosynthetic life evolved and increased oxygen in the atmosphere around 2.4 billion years ago.
- Plate tectonics and volcanism have continuously recycled Earth's crust and regulated temperatures and atmospheric gases through geologic time.
The solar system formed 4.6 billion years ago from a giant cloud of dust and gas called a solar nebula. As the cloud contracted under gravity, the proto-Sun formed at the center and a disk of dust and ice particles formed around it. These particles collided and merged to become planetesimals and eventually the planets. The inner planets like Earth are rocky due to higher temperatures in the inner solar system, while outer planets are gaseous. The Moon formed from debris ejected during a giant impact between Earth and a Mars-sized planet. Life on Earth began as single-celled organisms and changed the atmosphere through photosynthesis over billions of years.
Age of Jupiter inferred from the distinct genetics and formation times of met...Sérgio Sacani
The age of Jupiter, the largest planet in our Solar System, is still
unknown. Gas-giant planet formation likely involved the growth
of large solid cores, followed by the accumulation of gas onto
these cores. Thus, the gas-giant cores must have formed before
dissipation of the solar nebula, which likely occurred within less
than 10 My after Solar System formation. Although such rapid
accretion of the gas-giant cores has successfully been modeled,
until now it has not been possible to date their formation. Here,
using molybdenum and tungsten isotope measurements on iron
meteorites, we demonstrate that meteorites derive from two
genetically distinct nebular reservoirs that coexisted and remained
spatially separated between ∼1My and ∼3–4My after Solar System
formation. The most plausible mechanism for this efficient separation
is the formation of Jupiter, opening a gap in the disk and
preventing the exchange of material between the two reservoirs.
As such, our results indicate that Jupiter’s core grew to ∼20 Earth
masses within <1 My, followed by amore protracted growth to ∼50
Earth masses until at least ∼3–4 My after Solar System formation.
Thus, Jupiter is the oldest planet of the Solar System, and its solid
core formed well before the solar nebula gas dissipated, consistent
with the core accretion model for giant planet formation.
Lesson 1 the origin of the universe and solar systemMaryJoyValentino
The document provides an overview of Earth science topics including the origin of the universe, solar system, and Earth. It discusses theories of how the universe and solar system formed, including the nebular hypothesis which proposes that the solar system condensed from a giant cloud of gas and dust. Key events included gravitational collapse of the solar nebula forming the Sun and planets condensing from the disk as it rotated and cooled.
foundations of astronomy - the very basicsMaryPavlenko
The document provides information about the Earth and Moon. It summarizes that the Earth is differentiated with an iron core, silicate mantle and crust. The mantle flows like a liquid due to heat convection. Plate tectonics causes geological activity. Radiometric dating indicates the Earth is approximately 4.6 billion years old. The Moon has no atmosphere or magnetic field and its surface is dominated by impact craters. Evidence suggests there may be water ice at the lunar poles.
1) Researchers have developed a new technique called mechanophotopatterning (MPP) that uses light irradiation and mechanical deformation to precisely control the topology of light-responsive elastomers, establishing a new patterning method.
2) Using MPP, a variety of surface topologies can be produced, making it potentially useful for applications. When optically thick samples are irradiated, they bow into 3D shapes with promising applications in advanced optics.
3) The intrinsic material properties of the polymers remain unchanged after deformation, allowing for diverse applications at the interface of cell biology and tissue engineering through dynamic control of mechanical feedback to cells.
The document discusses the solar system from a broader perspective. It provides details on the formation of the solar system based on the nebular hypothesis, including how planets formed from a rotating cloud of gas and dust. It also describes the different types of objects in the solar system such as the terrestrial and gas planets, asteroids, comets, and Pluto. Additionally, it discusses theories for the origin of the Moon and evidence that Mars once had liquid water on its surface.
This document discusses the field of geology. It defines geology as the study of the Earth, including its physical and chemical properties from its creation to present day. The main branches of geology are described as crystallography, mineralogy, petrology, paleontology, and stratigraphy. The layers of the Earth are also summarized, including the inner core, outer core, mantle, and crust. Finally, several hypotheses for the origin of the Earth are outlined, such as the nebular hypothesis, planetesimal hypothesis, gaseous tidal hypothesis, and gas dust cloud hypothesis.
This chapter discusses the origin and evolution of the Earth and the solar system. It begins with an overview of the Big Bang theory for the origin of the universe and then describes the nebular hypothesis for the formation of the solar system from a primordial cloud of gas and dust. Key points include the differentiation of the Earth into a core, mantle and crust due to melting after accretion and the abundance of iron in the Earth's core versus the crust. The chapter also provides details about the different types of planets, asteroids, comets and meteorites that make up the solar system.
This document discusses comets, meteors, asteroids, and the moon. It provides details on their composition, sizes, orbits, and the potential effects of large impacts. A large comet impact would likely only injure humans, while the largest meteor ever could endanger humanity. The largest known asteroid impact 65 million years ago caused the extinction of dinosaurs. A second moon would result in bigger tides and more frequent solar eclipses.
This document provides information about comets, meteors, asteroids, and the moon. It defines each celestial object and describes their composition and origins. It notes that a large comet impact would likely only injure humans, while a large meteor could endanger humanity or damage Earth's orbit. The largest known asteroid impact 65 million years ago likely caused the extinction of dinosaurs. It also describes the moon's phases and how eclipses occur.
The document discusses nucleosynthesis in the early universe and provides evidence for the Big Bang theory. It explains that during the first three minutes after the Big Bang, most deuterium combined to form helium and trace amounts of lithium. The predicted abundances of these light elements depend on the density of ordinary matter and agree well with observations, providing strong evidence for the Big Bang.
The document discusses evidence that asteroids, comets, and dwarf planets originated from a planet called Astra that was destroyed billions of years ago. Data from the Rosetta mission showed that Comet 67P resembled material from Earth's oceans, supporting the theory that it originated from Astra's oceans. Images of asteroids revealed some have spherical shapes, likely from molten rock ejected during Astra's destruction. The document argues this new data contradicts older theories and supports Astra being shattered to form the asteroids and comets we observe today.
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.
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.
The Limited Role of the Streaming Instability during Moon and Exomoon FormationSérgio Sacani
It is generally accepted that the Moon accreted from the disk formed by an impact between the proto-Earth and
impactor, but its details are highly debated. Some models suggest that a Mars-sized impactor formed a silicate
melt-rich (vapor-poor) disk around Earth, whereas other models suggest that a highly energetic impact produced a
silicate vapor-rich disk. Such a vapor-rich disk, however, may not be suitable for the Moon formation, because
moonlets, building blocks of the Moon, of 100 m–100 km in radius may experience strong gas drag and fall onto
Earth on a short timescale, failing to grow further. This problem may be avoided if large moonlets (?100 km)
form very quickly by streaming instability, which is a process to concentrate particles enough to cause gravitational
collapse and rapid formation of planetesimals or moonlets. Here, we investigate the effect of the streaming
instability in the Moon-forming disk for the first time and find that this instability can quickly form ∼100 km-sized
moonlets. However, these moonlets are not large enough to avoid strong drag, and they still fall onto Earth quickly.
This suggests that the vapor-rich disks may not form the large Moon, and therefore the models that produce vaporpoor disks are supported. This result is applicable to general impact-induced moon-forming disks, supporting the
previous suggestion that small planets (<1.6 R⊕) are good candidates to host large moons because their impactinduced disks would likely be vapor-poor. We find a limited role of streaming instability in satellite formation in an
impact-induced disk, whereas it plays a key role during planet formation.
Unified Astronomy Thesaurus concepts: Earth-moon system (436)
Discovery of Merging Twin Quasars at z=6.05Sérgio Sacani
We report the discovery of two quasars at a redshift of z = 6.05 in the process of merging. They were
serendipitously discovered from the deep multiband imaging data collected by the Hyper Suprime-Cam (HSC)
Subaru Strategic Program survey. The quasars, HSC J121503.42−014858.7 (C1) and HSC J121503.55−014859.3
(C2), both have luminous (>1043 erg s−1
) Lyα emission with a clear broad component (full width at half
maximum >1000 km s−1
). The rest-frame ultraviolet (UV) absolute magnitudes are M1450 = − 23.106 ± 0.017
(C1) and −22.662 ± 0.024 (C2). Our crude estimates of the black hole masses provide log 8.1 0. ( ) M M BH = 3
in both sources. The two quasars are separated by 12 kpc in projected proper distance, bridged by a structure in the
rest-UV light suggesting that they are undergoing a merger. This pair is one of the most distant merging quasars
reported to date, providing crucial insight into galaxy and black hole build-up in the hierarchical structure
formation scenario. A companion paper will present the gas and dust properties captured by Atacama Large
Millimeter/submillimeter Array observations, which provide additional evidence for and detailed measurements of
the merger, and also demonstrate that the two sources are not gravitationally lensed images of a single quasar.
Unified Astronomy Thesaurus concepts: Double quasars (406); Quasars (1319); Reionization (1383); High-redshift
galaxies (734); Active galactic nuclei (16); Galaxy mergers (608); Supermassive black holes (1663)
Mapping the Growth of Supermassive Black Holes as a Function of Galaxy Stella...Sérgio Sacani
The growth of supermassive black holes is strongly linked to their galaxies. It has been shown that the population
mean black hole accretion rate (BHAR) primarily correlates with the galaxy stellar mass (Må) and redshift for the
general galaxy population. This work aims to provide the best measurements of BHAR as a function of Må and
redshift over ranges of 109.5 < Må < 1012 Me and z < 4. We compile an unprecedentedly large sample with 8000
active galactic nuclei (AGNs) and 1.3 million normal galaxies from nine high-quality survey fields following a
wedding cake design. We further develop a semiparametric Bayesian method that can reasonably estimate BHAR
and the corresponding uncertainties, even for sparsely populated regions in the parameter space. BHAR is
constrained by X-ray surveys sampling the AGN accretion power and UV-to-infrared multiwavelength surveys
sampling the galaxy population. Our results can independently predict the X-ray luminosity function (XLF) from
the galaxy stellar mass function (SMF), and the prediction is consistent with the observed XLF. We also try adding
external constraints from the observed SMF and XLF. We further measure BHAR for star-forming and quiescent
galaxies and show that star-forming BHAR is generally larger than or at least comparable to the quiescent BHAR.
Unified Astronomy Thesaurus concepts: Supermassive black holes (1663); X-ray active galactic nuclei (2035);
Galaxies (573)
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...Sérgio Sacani
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
Signatures of wave erosion in Titan’s coastsSérgio Sacani
The shorelines of Titan’s hydrocarbon seas trace flooded erosional landforms such as river valleys; however, it isunclear whether coastal erosion has subsequently altered these shorelines. Spacecraft observations and theo-retical models suggest that wind may cause waves to form on Titan’s seas, potentially driving coastal erosion,but the observational evidence of waves is indirect, and the processes affecting shoreline evolution on Titanremain unknown. No widely accepted framework exists for using shoreline morphology to quantitatively dis-cern coastal erosion mechanisms, even on Earth, where the dominant mechanisms are known. We combinelandscape evolution models with measurements of shoreline shape on Earth to characterize how differentcoastal erosion mechanisms affect shoreline morphology. Applying this framework to Titan, we find that theshorelines of Titan’s seas are most consistent with flooded landscapes that subsequently have been eroded bywaves, rather than a uniform erosional process or no coastal erosion, particularly if wave growth saturates atfetch lengths of tens of kilometers.
SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole⋆Sérgio Sacani
Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4
Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...Sérgio Sacani
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS
+
53.13485
−
27.82088
with a host spectroscopic redshift of
2.903
±
0.007
. The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red (
�
(
�
−
�
)
∼
0.9
) despite a host galaxy with low-extinction and has a high Ca II velocity (
19
,
000
±
2
,
000
km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low-
�
Ca-rich population. Although such an object is too red for any low-
�
cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement (
≲
1
�
) with
Λ
CDM. Therefore unlike low-
�
Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high-
�
truly diverge from their low-
�
counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...Sérgio Sacani
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDSSérgio Sacani
The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.
Anti-Universe And Emergent Gravity and the Dark UniverseSérgio Sacani
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
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.
This talk will cover ScyllaDB Architecture from the cluster-level view and zoom in on data distribution and internal node architecture. In the process, we will learn the secret sauce used to get ScyllaDB's high availability and superior performance. We will also touch on the upcoming changes to ScyllaDB architecture, moving to strongly consistent metadata and tablets.
[OReilly Superstream] Occupy the Space: A grassroots guide to engineering (an...Jason Yip
The typical problem in product engineering is not bad strategy, so much as “no strategy”. This leads to confusion, lack of motivation, and incoherent action. The next time you look for a strategy and find an empty space, instead of waiting for it to be filled, I will show you how to fill it in yourself. If you’re wrong, it forces a correction. If you’re right, it helps create focus. I’ll share how I’ve approached this in the past, both what works and lessons for what didn’t work so well.
Discover top-tier mobile app development services, offering innovative solutions for iOS and Android. Enhance your business with custom, user-friendly mobile applications.
Connector Corner: Seamlessly power UiPath Apps, GenAI with prebuilt connectorsDianaGray10
Join us to learn how UiPath Apps can directly and easily interact with prebuilt connectors via Integration Service--including Salesforce, ServiceNow, Open GenAI, and more.
The best part is you can achieve this without building a custom workflow! Say goodbye to the hassle of using separate automations to call APIs. By seamlessly integrating within App Studio, you can now easily streamline your workflow, while gaining direct access to our Connector Catalog of popular applications.
We’ll discuss and demo the benefits of UiPath Apps and connectors including:
Creating a compelling user experience for any software, without the limitations of APIs.
Accelerating the app creation process, saving time and effort
Enjoying high-performance CRUD (create, read, update, delete) operations, for
seamless data management.
Speakers:
Russell Alfeche, Technology Leader, RPA at qBotic and UiPath MVP
Charlie Greenberg, host
Northern Engraving | Modern Metal Trim, Nameplates and Appliance PanelsNorthern Engraving
What began over 115 years ago as a supplier of precision gauges to the automotive industry has evolved into being an industry leader in the manufacture of product branding, automotive cockpit trim and decorative appliance trim. Value-added services include in-house Design, Engineering, Program Management, Test Lab and Tool Shops.
The Microsoft 365 Migration Tutorial For Beginner.pptxoperationspcvita
This presentation will help you understand the power of Microsoft 365. However, we have mentioned every productivity app included in Office 365. Additionally, we have suggested the migration situation related to Office 365 and how we can help you.
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Chris Jones, Director of Product Management at BrainChip , presents the “Temporal Event Neural Networks: A More Efficient Alternative to the Transformer” tutorial at the May 2024 Embedded Vision Summit.
The expansion of AI services necessitates enhanced computational capabilities on edge devices. Temporal Event Neural Networks (TENNs), developed by BrainChip, represent a novel and highly efficient state-space network. TENNs demonstrate exceptional proficiency in handling multi-dimensional streaming data, facilitating advancements in object detection, action recognition, speech enhancement and language model/sequence generation. Through the utilization of polynomial-based continuous convolutions, TENNs streamline models, expedite training processes and significantly diminish memory requirements, achieving notable reductions of up to 50x in parameters and 5,000x in energy consumption compared to prevailing methodologies like transformers.
Integration with BrainChip’s Akida neuromorphic hardware IP further enhances TENNs’ capabilities, enabling the realization of highly capable, portable and passively cooled edge devices. This presentation delves into the technical innovations underlying TENNs, presents real-world benchmarks, and elucidates how this cutting-edge approach is positioned to revolutionize edge AI across diverse applications.
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ScyllaDB is making a major architecture shift. We’re moving from vNode replication to tablets – fragments of tables that are distributed independently, enabling dynamic data distribution and extreme elasticity. In this keynote, ScyllaDB co-founder and CTO Avi Kivity explains the reason for this shift, provides a look at the implementation and roadmap, and shares how this shift benefits ScyllaDB users.
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👉 Check out our full 'Africa Series - Automation Student Developers (EN)' page to register for the full program:
https://bit.ly/Automation_Student_Kickstart
In this session, we shall introduce you to the world of automation, the UiPath Platform, and guide you on how to install and setup UiPath Studio on your Windows PC.
📕 Detailed agenda:
What is RPA? Benefits of RPA?
RPA Applications
The UiPath End-to-End Automation Platform
UiPath Studio CE Installation and Setup
💻 Extra training through UiPath Academy:
Introduction to Automation
UiPath Business Automation Platform
Explore automation development with UiPath Studio
👉 Register here for our upcoming Session 2 on June 20: Introduction to UiPath Studio Fundamentals: https://community.uipath.com/events/details/uipath-lagos-presents-session-2-introduction-to-uipath-studio-fundamentals/
In the realm of cybersecurity, offensive security practices act as a critical shield. By simulating real-world attacks in a controlled environment, these techniques expose vulnerabilities before malicious actors can exploit them. This proactive approach allows manufacturers to identify and fix weaknesses, significantly enhancing system security.
This presentation delves into the development of a system designed to mimic Galileo's Open Service signal using software-defined radio (SDR) technology. We'll begin with a foundational overview of both Global Navigation Satellite Systems (GNSS) and the intricacies of digital signal processing.
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1. NATURE|Vol 450|20/27 December 2007 NEWS & VIEWS
than can be achieved with other methods. But necessitate minimizing false-positive results, Jonathan W. Uhr is in the University of Texas
Nagrath and colleagues’ one-step method does particularly when only a few putative tumour Southwestern Medical Center, 6000 Harry Hines
have its limitations. For example, it cannot cells are isolated. One way to solve this prob- Boulevard, Dallas, Texas 75390-8576, USA.
examine individual cells for genetic changes lem would be to count sufficient numbers of e-mail: jonathan.uhr@utsouthwestern.edu
associated with progress of the tumour. chromosomes or genes in candidate cells to
Nonetheless, Nagrath and colleagues’ results1 detect one of the hallmarks of a malignant 1. Nagrath, S. et al. Nature 450, 1235–1239 (2007).
2. Fidler, I. J. J. Natl Cancer Inst. 45, 773–782 (1970).
bring us closer to having a fully automated cell — a significant deviation from the two-
3. Méhes, G. et al. Am. J. Pathol. 159, 17–20 (2001).
instrument that can detect circulating tumour copies-per-cell norm. A simpler alternative 4. Meng, S. et al. Clin. Cancer Res. 10, 8152–8162 (2004).
cells with exquisite sensitivity. Such an instru- might be to test for increased expression of the 5. Riethdorf, S. et al. Clin. Cancer Res. 13, 920–928 (2007).
ment would allow routine monitoring of blood many known malignancy-associated proteins. 6. Meng, S. et al. Proc. Natl Acad. Sci. USA 101, 9393–9398
for tumour cells as part of a medical exami- In time, it might even be possible to detect and (2004).
7. Cristofanilli, M. et al. N. Engl. J. Med. 351, 781–791
nation, and could result in early detection therapeutically target or remove the cells’ organ (2004).
and treatment, with the chance of obtaining of origin at an early enough stage to prevent the 8. Went, P. T. H. et al. Hum. Pathol. 35, 122–128 (2004).
higher cure rates. But this approach would also cancer from metastasizing. ■ 9. Allard, W. J. et al. Clin. Cancer Res. 10, 6897–6904 (2004).
PLANETARY SCIENCE
A younger Moon Core formation
Silicate differentiation
Earth
Alan Brandon Moon
Old Giant impact
The most recent study of lunar rocks indicates that the Moon formed later New
than previously thought — a conclusion that requires our view of the early Old LMO start
New
history of the inner Solar System to be revised.
Earliest crust LMO final?
It was almost 40 years ago that we found out occurred in the first 60 million years or so of
what the Moon is made of: lunar samples col- Solar System history, before most 182Hf decayed 0 50 100 150 200 250
lected during the Apollo missions turned out away. It is useful for tracking metal–silicate dif- Time (million years)
to consist of rocky material similar in compo- ferentiation times, because W has an affinity
sition to that found on Earth. We also think we for iron-rich metal cores whereas Hf favours Figure 1 | The earliest history of the Moon and
know that the Moon formed from the accre- mantle silicate and oxide minerals. If core for- Earth. Time 0 marks the onset of Solar System
tion of molten and vaporized ejecta produced mation occurred when 182Hf was still actively accretion at 4.567 billion years ago, with the rest
by a collision between proto-Earth and a giant decaying, then a record is preserved in the of the scale denoting time after that event. The
previously inferred ages for the giant impact and
Mars-sized impactor1,2. But the answer to the amount of 182W present.
the onset of solidification of a lunar magma ocean
‘When?’ of Moon formation has remained elu- The amount of 182W measured in Earth (LMO)4–6 were based on older W-isotope data for
sive. On page 1206 of this issue, Touboul et al.3 samples4,5 indicates that W was removed into Moon rocks. Touboul and colleagues’ W-isotope
examine this question with tungsten-isotope Earth’s core about 30 million years after the data3 provide a new and later time for the giant
measurements of lunar rocks. Solar System began to accrete 4.567 billion impact and for the start of solidification of the
The mass of the giant impactor that led to years ago (Fig. 1). Before Touboul and col- LMO. The final solidification time of the LMO
the formation of the Moon was as much as leagues’ new study3, the lunar 182W data had is obtained from the 146Sm–142Nd chronology of
30% of Earth’s mass today, and this collision is yielded two conclusions. First, that formation Moon rocks8. The vertical band is the earliest
thought to represent the last significant growth of the Moon — and so the giant impact event — time for the giant impact that formed the Moon;
stage of our planet1. The post-collision disk of occurred around the same time as Earth’s core error bars represent 2σ uncertainty estimates for
each event. Data points for events on Earth are
ejecta and the new bulk Earth were a combi- formed at about 30 million years4,5. Second,
given for comparison.
nation of proto-Earth material and that of the that the lunar magma ocean largely solidified
impactor. The tremendous release of energy 10 million years after that6. This chronology
probably melted the Earth, producing a glo- provides a well-ordered Earth–Moon system of Touboul et al.3 show, the previous W isotope
bal-scale magma ocean. Iron-rich metal from that behaved exactly as we expected — rapid data for lunar materials were not completely
the proto-Earth and the impactor merged to accretion of Earth, core formation and corrected for 182W produced by the decay of
182
form the present Earth’s core, with Earth’s global-scale melting were coincident with Ta (tantalum). The isotope 182Ta forms when
mantle and crust forming from silicate and a giant impact, and were followed by rapid cosmic rays bombard the Moon. The excess
182
oxide (non-metal) material. The time intervals cooling and consequent solidification of the W from this process can result in spurious
between the various events — the giant impact, magma oceans of Earth and the Moon. ages using the 182Hf–182W clock.
the formation of Earth’s core, and the onset But some observations do not fit this simple When correctly accounting for 182W pro-
and solidification of magma oceans in Earth lunar history (Fig. 1). First, radiometric ages duced from 182Ta, Touboul et al.3 find that the
and the Moon — tell us when accretion was for the lunar crust, which was made from light amount of 182W in lunar samples indicates
completed and constrain the early differentia- minerals that solidified and floated to the top that the Moon could not have formed before
tion and cooling histories of the ‘terrestrial’ of the magma ocean, show that it began to form 62+ 90 million years after the initiation of Solar
−10
planets (Mercury, Venus, the Earth–Moon no earlier than 70 million to 150 million years System accretion, at least 16 million years after
system and Mars). after accretion of the Solar System began7. Sec- Earth’s core formed and no later than forma-
Enter the evidence from the 182Hf (hafnium) ond, the 146Sm (samarium) and 142Nd (neodym- tion of the first lunar crust (Fig. 1). These new
and 182W (tungsten) radiometric clock. The ium) radiometric clock shows that the lunar findings are in agreement with the slower rate
isotope 182Hf decays to 182W with a half-life of magma ocean largely began to solidify as late as of magma-ocean solidification obtained from
9 million years. This clock dates events that 215 million years8. Third, as the new lunar data ages for the lunar crust and 146Sm–142Nd data.
1169
2. NEWS & VIEWS NATURE|Vol 450|20/27 December 2007
E. A. CERNAN/NASA
50 YEARS AGO
“An experiment on ‘telepathy’
using television” by Donald
Michie & D. J. West — We
have made a small-scale trial
with the object of testing any
generalized extra-sensory
perception effect and looking
for individuals with strongly
manifested telepathic abilities
... The viewers were informed
that the cards would be drawn at
random from a pack consisting
of three types, depicting a canoe,
a wheelbarrow and a trumpet,
respectively. They were asked
to record their guesses on a
form printed in the TV Times
and post it to the programme
contractors … The pooled results
showed no significant deviation
from chance expectation. But
one entry, submitted by a Mr. B.
Downey, with 15 guesses out of
19 was considered sufficiently Moon rock — a picture
suggestive to justify further tests. from the Apollo 17 mission.
From Nature 21 December 1957. Harrison H. Schmitt is the
geologist–astronaut.
100 YEARS AGO
On the day of going to press, we
learn of the death of Lord Kelvin, The later time for the Moon’s formation we thought. Application of the 146Sm–142Nd
an announcement which will challenges the current view that the terrestrial clock to martian meteorites suggests that
be received with deep sorrow planets grew rapidly, and also challenges ideas the magma ocean in Mars took 60 million
throughout the civilised world about their early cooling histories4–6,9. It may to 100 million years to solidify11, likewise
… For the body of one who has mean that Earth and Mars took at least 50 mil- implying that Earth’s magma ocean probably
50 & 100 YEARS AGO
brought such honour to the British lion years, and possibly hundreds of millions took longer to solidify than some current mod-
nation, the only appropriate place of years, to reach their final mass (that is, 99% els predict. We need additional evidence to
of burial is Westminster Abbey. of their present size). By contrast, recent mod- further examine these issues on the earliest
els call for a more rapid accretion that took 30 history of the Earth–Moon system. The clues
ALSO: million years or less9. Interestingly, the first might lie in future samples returned from the
The increase in the efficiency of evidence from the 146Sm–142Nd clock of silicate Moon and Mars. ■
colleges and universities in this differentiation in Earth is about 40 million to Alan Brandon is at Astromaterials Research and
country is too pressing a need to 60 million years after accretion of the Solar Exploration Sciences, Johnson Space Center,
be dependent upon party politics. System began10. This probably records the NASA, 2101 Nasa Parkway, Houston, Texas
Unless our statesmen can be time of the onset of cooling of Earth’s magma 77058, USA.
made to realise the supreme ocean, which overlaps with the earliest new e-mail: alan.d.brandon@nasa.gov
importance of this matter and time for lunar formation and the giant impact
be persuaded to deal with it in a (Fig. 1). In turn, this implies that earlier core 1. Canup, R. M. Icarus 168, 433–456 (2004).
2. Pahlevan, K. & Stevenson, D. J. Earth Planet. Sci. Lett. 262,
patriotic manner, generously and formation in Earth did not necessarily coin- 438–449 (2007).
expeditiously, as if there were no cide with the development of a magma ocean, 3. Touboul, M., Kleine, T., Bourdon, B., Palme, H. & Wieler, R.
votes to retain or secure, we must and that, for a large terrestrial planet such as Nature 450, 1206–1209 (2007).
reconcile ourselves to the idea that Earth, rapid pulses of accretion, which could 4. Kleine, T., Münker, C., Mezger, K. & Palme, H. Nature 418,
952–955 (2002).
as manufacturing and distributing have been caused by a single giant impactor 5. Yin, Q. et al. Nature 418, 949–952 (2002).
people we shall in due course have that ultimately led to the formation of the 6. Kleine, T., Palme, H., Mezger, K. & Halliday, A. N. Science
to occupy a third or fourth place Moon, might have been necessary to initiate 310, 1671–1674 (2005).
among the nations of the world. In large-scale melting. 7. Norman, M. D., Borg, L. E., Nyquist, L. E. & Bogard, D. D.
Meteor. Planet. Sci. 38, 645–661 (2003).
Germany, the United States, and The long-lived magma ocean in the Moon 8. Rankenburg, K., Brandon, A. D. & Neal, C. R. Science 312,
now in Japan, rulers have learnt raises the question of how long Earth’s magma 1369–1372 (2006).
the lesson that efficient education ocean took to solidify. We do not know for cer- 9. Jacobsen, S. B. Science 300, 1513–1514 (2003).
10. Bennett, V. E., Brandon, A. D., Heiss, J. & Nutman, A.
and industrial success are related tain, but the implication of Touboul and col- Geochim. Cosmochim. Acta 71, A79 (2007).
to each other as cause and effect. leagues’ lunar W-isotope data3 is that accretion 11. Debaille, V., Brandon, A. D., Yin, Q. Z. & Jacobsen, B. Nature
From Nature 19 December 1907. and early cooling of Earth were not as rapid as 450, 525–528 (2007).
1170