Researchers found that lake breach floods played a crucial role in shaping the Martian surface, creating river valleys with nearly a quarter of the Red Planet's total volume. The study's findings suggest that these floods had a lasting impact on the surrounding landscape, influencing the formation of other nearby river valleys.
Researchers used Mars Odyssey data to identify sub-surface water ice deposits in temperate regions of Mars. Seasonal variations suggest significant quantities of water ice can be found beneath the surface, making them ideal resources for future human missions.
China's space transportation systems have made significant leaps in recent decades, with advancements in launch vehicles, propulsion systems, and artificial intelligence. The country aims to become a powerful space nation by the mid-21st century, with plans for manned missions to the Moon and Mars.
Engineers at the University of Cincinnati have developed a carbon dioxide reactor that can convert CO2 into methane, a potential fuel source for Mars. The process, known as the Sabatier reaction, could reduce fuel needs by half for astronauts returning to Earth, making it a promising solution for future Mars missions.
A new study from Washington University in St. Louis suggests that Mars' small size limits its habitability due to a lack of retained volatiles. Researchers used potassium isotopes to determine the presence and abundance of volatile elements on Mars, finding a correlation between body size and volatile composition.
Researchers create AstroCrete, a strong concrete-like material using human serum albumin and urea-based binders, suitable for Martian construction. The material's compressive strength can be up to 40 MPa, making it a potential solution for in-situ resource utilization.
Researchers at Skoltech have identified a favorable window of opportunity for manned Mars missions in the mid-2030s. The study suggests that launching during the decaying phase of solar activity can help shield astronauts from cosmic rays, allowing for longer flight durations.
Researchers found that buttes on Mars can block about 20% of radiation from the sky, reducing the dose by a significant amount. However, this effect is limited by albedo radiation, which increases when the terrain reflects and emits radiation backwards.
An international team of space scientists finds that humans can travel to and from Mars safely if the spacecraft has sufficient shielding. The round trip should be shorter than four years. Scientists also recommend timing the mission during solar maximum to shield astronauts and the spacecraft from radiation.
A new study published in Geophysical Research Letters suggests that smectites, a type of clay, are the most likely explanation for the bright radar reflections discovered at Mars' south polar cap. The research team used multiple lines of evidence to demonstrate that clays can explain all observations, putting the lake hypothesis on ice.
A team at the Natural History Museum is testing spectral instruments for the ExoMars rover to identify meteorites on Mars. The rover's success rate is significantly higher than dedicated meteorite hunts on Earth, with one meteorite found per kilometre travelled.
The InSight mission has successfully mapped the internal structure of Mars using seismic waves detected by the SEIS instrument. The analysis revealed an estimate of the core size, crust thickness and mantle structure, providing valuable information on the planet's formation and thermal evolution.
A 2018 Martian dust storm destroyed a southern hemisphere cold air vortex and brought an early spring, whereas the northern hemisphere's vortex remained stable. The storm had profound effects on the atmosphere, including altering wind patterns and suppressing waves in the northern hemisphere.
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.
Researchers from ETH Zurich analyzed data from NASA's InSight mission, revealing that Mars' crust, mantle, and core have distinct structures. The findings suggest that Mars was once completely molten, but now has a thinner crust with a relatively high proportion of radioactive elements.
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.
Researchers have determined the crustal thickness of Mars for the first time, with values ranging from 20 to 39 kilometers. This independent measurement allows for a precise map of the planet's crust across its entire surface.
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 from the University of Toledo is working with NASA to develop more resilient solar power conversion systems for future Mars and Moon missions. The three-year grant will investigate ways to make these systems tolerant to space-related radiation, which degrades their performance.
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.
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 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.
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.
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.
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.
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.
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.
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.
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.
Researchers have developed porous carbon aerogels for electrodes in ultralow-temperature supercapacitors, reducing heating needs for future space and polar missions. The new technology could enable NASA's Mars rovers to operate without heaters, improving efficiency and extending their lifespan.
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 at NASA and German Aerospace Center sent microbes to Earth's stratosphere, replicating Martian conditions, to test their endurance. The study found that some microorganisms, such as spores from the black mold fungus, could survive high UV radiation and desiccation during space travel.
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.
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.
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.
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 at UNICAMP conducted over 120 experiments to model Mars' long, slow-moving barchan dunes. They identified five basic types of interaction between the dunes, including chasing and merging mechanisms.
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.
The AMADEE-18 Mars analog mission in Oman evaluated operational concepts and optimized strategies for future human missions. A benchmarking tool was developed to improve scientific output, mission safety, and efficiency.
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.
A recent study suggests that bacteria can extract useful materials from rocks on Mars and the Moon, paving the way for new technologies to support human exploration and settlement. The findings also highlight the potential of microorganisms to enhance the removal of rare earth elements from lunar and Martian landscapes.