Articles tagged with Mars
The InSight mission has unveiled Mars' internal structure, revealing a large liquid core and an altered crust. The study analyzed seismic waves from over 600 Martian quakes, identifying discontinuities in the crust and determining the upper mantle's structure.
The InSight mission provides clues to Mars' composition, mapping its crust, mantle, and core for the first time. Researchers find a multi-layered crust with an average thickness of 24-72 kilometers and a thick lithosphere beneath.
Two University of Arkansas researchers will study how carbon-dioxide ice pits in Mars' polar caps have formed and evolved over time. They aim to better understand the seasonal and long-term cycles of these ice pits and their impact on Martian atmospheric dynamics.
A team of engineers at UC Riverside has developed a catalyst that removes perchlorate from water, which is abundant in Martian soil. The new technology could help produce oxygen for human explorers on Mars.
Astronomer Alicia Rutledge has been awarded a $200,000 NASA Planetary Science Early Career Award to support the development of a field-portable laboratory for her research on cold-climate alteration processes. The award will enable her to conduct analog fieldwork and train next-generation scientists in planetary analog science.
A new study by a joint Japan/US-based team has developed a machine learning technique that assesses complex organic mixtures using mass spectrometry to reliably classify them as biological or abiological. This approach may help detect extraterrestrial life with a different evolutionary history than Earth-life.
Researchers at University of Arizona discovered evidence of recent volcanic activity on Mars, suggesting eruptions could have taken place in past 50,000 years. The discovery of a previously unknown volcanic deposit raises possibility of habitable conditions below Martian surface.
Researchers at HI-SEAS analog lunar habitat in Hawaii use spacesuits to explore lava tubes, mimicking conditions on the moon and Mars. The study aims to improve methods and suits for future astrobiology research.
A new simulation led by University of Chicago geoscientist Edwin Kite finds that high-altitude water ice clouds could have created a greenhouse effect on early Mars, enabling the presence of flowing rivers and lakes. The study challenges previous assumptions about the Martian climate and offers insights into the planet's habitability.
A global climate model simulation suggests that a cloud greenhouse effect could have warmed early Mars to support liquid surface water, with low clouds and warm stable climates emerging near surface water-ice patches. The results are consistent with geological data indicating a warm, arid early climate for the planet.
The Marsquake Service has detected over 500 marsquakes, with most being high-frequency events occurring at great distances. Low-frequency events are less common and appear to decay more quickly than expected.
A new study published in Astrobiology finds that Martian meteorites contain the necessary ingredients to support microbial life, including water and radioactive elements. The researchers believe that wherever there's groundwater on Mars, there's a good chance of finding habitable environments for subsurface microbial life.
Ancient dune fields in Gale crater provide evidence of variable wind directions, shedding light on Mars' climate evolution. The findings suggest that the Martian surface may have been less hospitable to life than previously thought, with a vast expanse of desert sand representing a snapshot of time.
UMass Lowell's Kennedy College of Sciences is hosting a free event series showcasing cutting-edge research and educational opportunities. Experts will discuss COVID-19 vaccine development, search for life on Mars, and diversity in the sciences. The series is open to the public and features online events from April 10-16.
A French-US team has discovered that Mars' climate alternated between dry and wetter periods, with lake-deposited clays forming the base of Mount Sharp before drying up completely about 3 billion years ago.
The Curiosity rover has explored the stratigraphy of Gale crater, providing insights into Mars' early climatic history. The study reveals alternating wet and dry depositional environments recorded in the sedimentary sequence, shedding light on the Red Planet's environmental changes during the Hesperian age.
Researchers from Brown University have discovered a previously unknown type of ancient crater lake on Mars that differs from other Martian crater lakes. The crater was likely fed by runoff from a long-lost Martian glacier, which suggests the planet's early climate may have been warmer and wetter than previously thought.
The study found that dry ice sublimation can form unique radial systems on Mars' surface, similar to spiders. The experiments showed that the Leidenfrost Effect plays a crucial role in eroding the spider patterns, which were more branched with finer grain sizes.
A new study suggests that up to 99% of Mars' initial water was incorporated into minerals and buried in the planet's crust, not lost to space. Researchers used observational data and modeling to resolve long-standing contradictions about Martian water loss rates.
Dr. Nathalie Cabrol proposes that modern life on Mars could be more widespread and accessible than previously believed, and that understanding patterns resulting from extreme environmental interactions is key to finding life. She suggests taking the approach of Mars as a biosphere to find signs of microbial habitability.
A significant portion of Mars's water is still present on the planet, with estimates suggesting 30-99 percent is trapped within minerals in the crust. This discovery challenges the current theory that the Red Planet's water escaped into space due to low gravity.
Research reveals that airborne dust plumes are produced by sliding blocks of dry ice each spring, which kick up sand and dust along the way. This process carves and modifies linear gullies on the slopes of a Martian sand dune.
Researchers from the GLOBE Institute at University of Copenhagen found that water may be present during planet formation, applicable to Earth, Venus, and Mars. The study suggests that planets with similar building blocks and temperature conditions as Earth may have oceans and continents.
Researchers at the University of Oregon found that small electrical sparks may be triggered by friction in Martian dust particles. The sparks, likely to be small and pose little danger, suggest that Mars may be an electrically active place with unique characteristics.
Scientists have successfully grown cyanobacteria using Martian gases and regolith, a breakthrough that could make long-term missions to Mars sustainable. This discovery uses Anabaena cyanobacteria as a model organism, demonstrating their ability to thrive in low-pressure environments.
Researchers from HKU have discovered evidence of a reduced atmosphere on ancient Mars, dating back 3.5 billion years. The team used infrared remote sensing and spectroscopy to analyze mineralogy and geochemistry of ancient rocks, revealing weathered conditions indicative of a reducing environment.
A Southwest Research Institute scientist has updated Mars chronology models to suggest that terrains shaped by ancient water activity on the planet's surface may be hundreds of millions of years older than previously thought. The new model also provides a revised age for Isidis Basin, now estimated to be 4-4.2 billion years old.
The Emirates Mars Mission will provide crucial science data on the Martian atmosphere, measuring dust particles, ice clouds, and water vapor. The mission's launch marks a significant milestone in space exploration for an Arab nation and has enormous positive impacts on science communities.
Researchers propose that underground salts and melting ice are responsible for Martian landslides, including the seasonal Recurring Slope Lineae features. Lab experiments suggest that thin layers of liquid-like water form near -50 °C, followed by gradual melting, which could lead to surface changes and dust storms.
Researchers from the University of the Basque Country have developed a novel non-destructive analytical strategy to characterize Martian samples. The proposed method utilizes Raman spectroscopy to identify molecular compositions and geochemical properties of unknown samples.
Researchers used data from Curiosity rover and Earth comparisons to determine temperature impact on Martian rocks, finding it was the biggest factor in weathering sediments.
A new analysis reveals Mars underwent 6-20 separate ice ages during the past 300-800 million years, with rocks trapped in glaciers providing a natural experiment. The findings hold implications for planetary geology and space exploration, including the potential for life on Mars.
High-resolution imaging revealed debris-covered glacier deposits on Mars formed in multiple punctuated episodes of ice accumulation over long timescales. Boulder size and distribution varied across the glacial landforms, contradicting predictions for a single continuous deposition period.
Researchers have created the largest image ever made of Mars' surface, mapping three billion-year-old sedimentary rocks and identifying 18 new fluvial ridges. The study provides unprecedented insight into ancient river systems on Mars, which could prove valuable targets for future exploration of past climates and tectonics.
Researchers created maps of where brines are most likely to be found on Mars by considering global weather patterns and multiple phase changes. Favorable conditions for stable brines are mostly in mid- to high-northern latitudes, large impact craters in the southern hemisphere, and shallow subsurface near the equator.
A Rutgers-led study suggests the most habitable region for life on Mars would be up to several miles below its surface due to subsurface melting of thick ice sheets. Liquid water may have been stable at great depths, allowing life to thrive through hydrothermal activity and rock-water reactions.
Engineers at Washington University in St. Louis have developed a brine electrolysis system that produces oxygen and hydrogen from salty water, potentially changing the game for Mars missions and resource utilization on Earth.
Researchers from Cornell University and NASA's Jet Propulsion Laboratory discovered evidence of massive floods in Gale Crater, suggesting conditions for microbial life. The flooding, likely caused by a meteoritic impact, deposited unique geological structures indicating flowing water and wind on Mars.
A team of scientists discovered ancient zircon minerals in a Martian meteorite that date back to 4.5 billion years ago, but also contain younger ages suggesting volcanic activity in the northern hemisphere. The zircons' hafnium isotope composition reveals a primitive reservoir in Mars' interior, unchanged since the planet's formation.
Researchers analyzed zircon crystals from a Martian meteorite, discovering ages ranging from 4.485 to 1.548 billion years, suggesting heavy bombardment and volcanic activity on Mars. The findings imply a previously unrecognized primitive mantle reservoir and significant implications for Mars' tectonic history.
Researchers found that Martian water vapor is transported to high altitudes during warmer seasons, where it's easily destroyed by electrically charged gas particles. The phenomenon contributes to Mars' loss of a global ocean of water over billions of years.
A new study reveals that water on Mars is directly transported to the upper atmosphere, where it is converted into atomic hydrogen that escapes to space. The process is more pronounced during dust storms, including the 2018 global dust storm.
Researchers discovered a large amount of water in the upper atmosphere of Mars, rapidly destroyed by ions, explaining part of the planet's mysterious dryness. This process contradicts the classical picture of water escape from Mars, suggesting it is incomplete and influenced by seasonal and dust storms.
Researchers propose that water emerges during planet formation, contradicting previous 'accidental' asteroid collision theory. The study found water on Mars for the first 90 million years of existence, suggesting it was a bioproduct of the planet's formation process.
Researchers discovered diverse microbes in Chile's Atacama Desert clay layers, which could indicate the presence of microorganisms on Mars. The study provides a guide for searching for life on the red planet, informing where to look and which instruments to use.
Analysis of a Martian meteorite suggests water was present on ancient Mars around 4.4 billion years ago, raising questions about the origin of water on Earth and potential for life beyond. The finding could impact theories on planetary formation and exploration.
Researchers developed artificial soil mixtures that mimic materials found on Mars, evaluating their fertility and potential for plant growth. The study found that Martian soils may be challenging to use due to textures and nutrient availability, but also identified potential solutions using Earth-based agricultural science.
Scientists from Chinese and German institutions report on time-resolved measurements of lunar surface radiation, revealing an equivalent dose rate of about 60 microsieverts per hour. This poses considerable exposure for humans, highlighting the need for shielding during long-term moon stays.
Researchers at George Mason University are using EUVM solar occultations to simulate Mars upper atmospheric processes. The project aims to identify the fundamental causes of observed variability driven by tides and gravity waves.
Researchers at Cornell University found that acidic fluids may have destroyed biological evidence hidden within Mars' iron-rich clays, making it difficult to search for life on the red planet. The study's lead author suggests that searching for organic compounds on Mars is a challenging task due to the degradation of biological material.
Researchers detected a slight tilt in the seismometer's signal during solar eclipses, likely due to ground cooling and deformation. This effect could be used to map Phobos' orbit with increased precision, important for future missions to the Martian moon.
Researchers from Tohoku University discovered a novel iron-based superelastic alloy capable of withstanding extreme temperatures. The new alloy can operate within a wider temperature range than conventional metal-based SEAs, making it suitable for outer-space exploration and other demanding applications.
The NASA JPL team is using deep learning to develop software for future Mars rovers, which will enable them to travel farther and explore more of the planet. The team has been training machine learning models on the Maverick2 supercomputer and developing novel capabilities such as Drive-By Science and Energy-Optimal Autonomous Navigation.
Researchers at the University of Bern have developed a new mass spectrometer, ORIGIN, capable of detecting and identifying the smallest amounts of extraterrestrial life traces. The instrument outperforms previous space instruments in terms of measurement sensitivity.
Researchers at the University of Texas at Austin found that precipitation must have been between 13-520 feet to fill ancient lake beds and river valleys on Mars. This study helps scientists understand the planet's climate and provides a crucial reference for future Mars missions.
Researchers discovered Martian and lunar lava tubes are up to 1,000 times wider than those on Earth, with volumes exceeding 1 billion cubic meters. The study highlights the potential of these underground cavities for future space exploration and settlement.
Researchers from Rice University have made the first direct measurements of three subsurface boundaries from Mars' crust to its core using NASA's InSight Lander data. The study provides insights into Mars' early history, planetary formation, and the planet's development from a chemical and thermal perspective.
New research published in Nature Geoscience reveals that early Mars was covered in ice sheets, not flowing rivers. The study analyzed over 10,000 Martian valleys and found striking similarities with subglacial channels in the Canadian Arctic Archipelago.
The Oak Ridge National Laboratory's production of ORNL-produced plutonium-238 enables the Perseverance rover to power its journey across Mars. The lab has been consistently increasing its Pu-238 production capabilities, aiming to produce 1.5 kilograms per year by 2026.
Astrophysicist Dimitra Atri's study suggests the presence of a life-supporting environment on ancient Mars due to traces of water and radiation-driven chemical reactions. The ExoMars mission may detect microbial life in this subsurface environment, providing valuable insights into the planet's habitability.