Scientists at the National Air and Space Museum's Center for Earth and Planetary Studies have created a comprehensive map of small mare ridges (SMRs) on the Moon. The research, published in The Planetary Science Journal, reveals that SMRs are geologically young and widespread across the lunar maria.
Research on Mars' volcanic systems shows that they were shaped by long-lasting and evolving magma beneath the planet's surface. The study found that these volcanoes experienced multiple eruptive phases, transitioning from early fissure-fed lava emplacement to later point-source activity.
Experimental tests demonstrate that interactions between magma oceans and primitive atmospheres during early years can produce significant amounts of water. This process has major implications for the physical and chemical properties of planets' interiors, with potential effects on core development and atmospheric composition.
A new study of the South Pole-Aitken basin reveals clues about the moon's interior structure, crust composition, and evolutionary history. The research suggests that the moon's near side was heated by radioactive elements from a magma ocean, leading to intense volcanism.
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New research finds Mars' mantle preserves a record of its violent beginnings, with chunky layers containing ancient fragments up to 4km wide. This discovery offers a rare glimpse into the evolution of rocky planets and challenges current understanding of planetary formation.
Researchers discovered over 15,000 kilometers of ancient riverbeds on Mars, suggesting that the planet may have experienced warm and wet conditions for a geologically relevant period. The presence of fluvial sinuous ridges indicates that flowing water was once widespread in Noachis Terra.
A 2.35-billion-year-old meteorite offers fresh insights into the Moon's volcanic history and suggests ongoing internal heat generation processes. The rock's distinct composition provides new constraints on when and how volcanic activity occurred on the Moon.
Researchers suggest looking for tell-tale patterns of energy instead of particular molecules or compounds associated with life. They argue that any living organism is extremely unlikely to be on its own and will always be part of an ecological community.
Scientists precisely dated the formation of the Moon's largest impact crater, the South Pole-Aitken Basin, to 4.25 billion years ago using Chang'e-6 samples. The discovery provides critical insights into the early history of the Moon and the Solar System.
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A team of scientists from Rutgers University found that water did not arrive as early in Earth's formation as previously believed. Instead, the data suggest that water was delivered to the planet in smaller portions after the Moon's formation, far later during late accretion.
NASA has partnered with Firefly Aerospace to deliver UCF's Lunar Vulkan Imaging and Spectroscopy Explorer (Lunar-VISE) payload to the Moon's Gruithuisen Domes. The mission aims to investigate the mysterious silica-rich volcanic features and gather data on lunar regolith for future exploration.
A new study reveals that a giant meteorite impact, equivalent to four Mount Everests, triggered a tsunami that mixed ocean debris and heated the atmosphere. This led to a rapid recovery of bacterial life, with iron-metabolizing bacteria flourishing in its wake.
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A team of geoscientists has identified the origin of the massive asteroid that wiped out 70% of Earth's species 66 million years ago. The study found the asteroid was a carbonaceous-type asteroid that formed outside Jupiter's orbit.
A Rice-led team studied massif-type anorthosites to understand their formation, revealing they likely originated from melting of subducted oceanic crust beneath convergent continental margins. The research provides new insights into Earth's thermal and tectonic evolution and chronicles the physical evolution of our planet.
A study by University of Texas at Dallas geoscientist Dr. Robert Stern and colleague Taras Gerya suggests that plate tectonics, oceans, and continents are necessary for the evolution of intelligent civilizations. The researchers propose refining the Drake equation factor to account for these requirements, which could explain the Fermi ...
Researchers found that the dual moons, named Selam, are a contact binary, with one quarter of the asteroid breaking off to form a trough. The team theorized that Dinky's fast spinning motion caused it to shed debris into orbit, which aggregated to form Selam.
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The newly discovered SPECULOOS-3b is an Earth-sized, likely airless planet orbiting a nearby ultracool dwarf star. The planet's extremely close proximity to its star has likely vaporized any atmosphere, allowing scientists to study its surface composition and history in unprecedented detail.
A University of Leicester-led study suggests that the orbital instability of the giant planets in our Solar System occurred between 60-100 million years after its beginning, based on analysis of enstatite meteorites. This instability is believed to have led to the formation of the Moon and may have impacted the habitability of Earth.
Scientists developed a reliable proxy to reconstruct ancient marine oxygen levels, revealing a significant rise during the Late Paleozoic era. This finding suggests early animals evolved in oxygen-poor oceans, providing critical context for studying exoplanet atmospheres.
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The Lunar Environment Monitoring System, developed by UMD researchers, will track seismic activity on the moon's surface during the upcoming Artemis III mission. The system's data will help prepare NASA for a long-term presence on other planetary bodies.
A groundbreaking scientific drilling project has unearthed the world's longest geological record of the Cretaceous period, spanning over 50 million years. The project, led by Professor Wang Chengshan, has provided crucial insights into paleoclimate research and will continue to aid in predicting future climate trends.
A team of astronomers has shed new light on the process of planet formation through a groundbreaking survey of over 80 young stars. The research provides a wealth of data and unique insights into how planets arise in different regions of our galaxy, revealing diverse patterns of planet-forming discs.
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Researchers have discovered a multi-planet system that provides a rare glimpse into the formation of planets around a young star. The system consists of six confirmed planets and potentially a seventh, all forming under similar conditions at an age of just 700 million years.
A joint research team has reported the discovery of buried palaeo-polygonal terrain beneath Utopia Planitia on Mars using the Zhurong rover's radar. This finding suggests that ancient Mars experienced a cold polar region and significant climate changes.
Researchers from EPFL and University of Bologna used asteroseismology to calculate star distances, providing accurate measurements and validating Gaia's parallax data. The study analyzed over 12,000 oscillating red giant stars, measuring their vibrations and oscillations to determine stellar properties.
Scientists have detected solar-wind hydrogen in lunar samples, indicating that water on the Moon's surface may provide a vital resource for future lunar bases and longer-range space exploration. Hydrogen has the potential to be used directly on the lunar surface when there are more regular or permanent installations.
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A new SwRI study posits that the large mounds on Kuiper Belt object Arrokoth are similar in size and shape, suggesting a common origin. This finding supports the streaming instability model of planetesimal formation, where gentle collision speeds allowed objects to accumulate and form Arrokoth.
The University of Texas at El Paso has received multiple grants from NASA to support its space research efforts. Researchers will examine planetary bedrock and prepare astronauts for the Artemis lunar mission. The grants aim to provide valuable insights into constructing infrastructure on other planets and identify lunar resources.
Origin-of-life chemists suggest glyoxylate reaction scenario could have yielded simple sugars without drawbacks of formaldehyde-based reactions. The researchers aim to demonstrate this hypothesis in the laboratory and explore potential commercial applications.
The study identifies five exoplanets that resemble Venus in terms of radii, masses, and atmospheric conditions. By observing these 'exo-Venus' planets using the James Webb Space Telescope, scientists hope to uncover valuable insights into Earth's future and the possibility of a runaway greenhouse climate.
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Scientists from the University of Cambridge have developed a model to predict a planet's interior water capacity based on its size and host star chemistry. The results suggest that larger planets may have drier rocky mantles, while smaller ones could hold more water-rich minerals.
The 57th annual meeting of the Geological Society of America's South-Central Section will take place in Oklahoma, USA, from March 13-14. The event features a diverse program covering various geologic disciplines and includes environmental-related sessions on topics such as hydrogeology and unconventional resources.
Researchers found microorganisms in Martian rocks that are difficult to detect with current instrumentation. The team suggests more powerful tools or bringing samples to Earth to conclusively address whether life existed on Mars. A European Mars rover expected to launch in 2028 will carry a drill capable of analyzing sediments deeper, ...
Researchers used computational simulations to model Charon's internal ocean freeze and its effects on the moon's surface. The study found that the freezing of an internal ocean may have formed deep depressions along Charon's girth but was unlikely to lead to cryovolcanoes erupting with ice and water in its northern hemisphere.
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Scientists have detected seismic surface waves on Mars for the first time, providing new insights into the planet's crust and structure. The study estimates the average properties of the Martian crust between 3 to 18.6 miles below the surface, revealing faster seismic velocities that suggest compositional differences or reduced porosity.
A recent study by Dr Joseph Michalski from HKU suggests that the number of ancient Martian lakes may have been significantly overestimated. The analysis of satellite data reveals evidence for smaller lakes on Mars, which could contain critical information about past climates.
Scientists have developed a new method to distinguish between normal land structures and small asteroid craters by analyzing charcoal samples, revealing 30% of impact sites remain unlocated. The study found unique characteristics in impact charcoals that differ from wildfire charcoals.
A study published in Cell Reports Physical Sciences has measured the physical limits for liquid water in icy extraterrestrial worlds. The results show that cold, salty liquids can remain liquid at much cooler temperatures than previously thought, extending the range of possible habitats on icy moons.
New research suggests diverse microbial life existed on Earth at least 3.75 billion years ago, dating back to a time when the planet was still forming. The study, led by UCL researchers, analyzed ancient rock formations and found evidence of complex structures that could not have been created through chemical reactions alone.
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Researchers analyzing Martian sediment samples suggest three possible explanations for the carbon's origin, including cosmic dust, ultraviolet degradation of carbon dioxide, or biological activity. The findings provide insights into the ancient Mars' carbon cycle and its potential habitability.
A team of researchers from Northern Arizona University discovered that water briefly existed in the Arabia Terra region on Mars. The study used thermal inertia to understand how rock layers were formed, revealing that the deposits could have only had water for a brief period.
Researchers have discovered rocks in Santorini cove similar to Martian basaltic material, with properties comparable to those of the Spirit and Curiosity rovers and Martian meteorites. The findings suggest that Santorini can serve as a low-cost resource for experiments and characterization of geological processes on Mars.
Researchers estimate technosphere mass at 30 trillion tons, exceeding biotic species. Human-made structures and waste now outnumber living organisms on the planet.
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Research from University of Toronto and University of Aberdeen suggests ancient 'scars' in the Earth's crust may trigger earthquakes and mountain formation. The team proposes a new 'perennial plate tectonic map' to illustrate how past processes impact present-day geological activity.
Researchers developed a miniaturized instrument for dating rocks and measuring geochemistry, revealing the age of a Mars meteorite. The technique provides high-sensitivity detection of organics and requires minimal sample preparation.
A new Caltech study suggests the Grand Canyon was formed over 70 million years ago, contradicting conventional models of its creation. The research uses a novel method to analyze ancient rocks and provides crucial insights into the canyon's incision.
Researchers created a comprehensive catalog of large craters on the moon to study the chaotic early days of the inner solar system. The analysis suggests that larger projectiles dominated the bombardment, ending around 3.8 billion years ago.
Scientists recognize Anthropocene epoch, a new geological time period caused by massive human impact, which may lead to the Earth's sixth-largest mass extinction event. The term has gained widespread support within the geological community and could be formalized as a new unit on the Geological Time Scale.
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A new analysis of historical documents and geological maps reveals Jerusalem's karst geology played a pivotal role in the city's selection as David's capital, allowing it to successfully fend off Assyrian sieges. The discovery highlights the significance of water security in the region, with implications for modern-day life and politics.
Earth Science World received the 2004 Scientific American.com Web Award, recognizing its exceptional online presence. The site's Virtual Oil Well game and ImageBank were highlighted as notable components.
Researchers at Yale University have devised a method to precisely date the timing and temperature of a meteorite impact on Mars. The (U-Th)/He dating method provides a far more accurate picture than conventional methods, shedding light on the history of Martian impacts and their effects on interplanetary material transfer.
University of Michigan scientists estimate moon age between 4.52 billion to 4.50 billion years ago through tungsten isotope analysis. The data supports the hypothesis that the moon was formed from a large object colliding with Earth.