Articles tagged with Mars
Scientists have discovered a possible explanation for Mars' limestone-free climate: sulfur dioxide in the atmosphere. The greenhouse gas interfered with carbonate rock formation, but led to the creation of silicates and sulfites instead.
Harvard researchers suggest sulfur dioxide played a crucial role in maintaining Mars' warmer climate between 3.5 and 4 billion years ago. The presence of sulfur dioxide would have prevented the formation of limestone deposits, leading to the absence of carbonate on Mars today.
New software helps NASA's Spirit rover find a safe winter haven on Mars, called Von Braun. However, the path to get there is too treacherous, with no suitable bail out spots along the route. The software uses satellite images and rover images to map features on the surface.
A Carnegie Institution-led team finds organic compounds containing carbon and hydrogen in Martian meteorite Allan Hills 84001, suggesting that building blocks of life formed on Mars early in its history. The discovery was made by analyzing the rock's association with iron oxide mineral magnetite.
NASA researchers present groundbreaking discoveries on polar mesospheric clouds, Voyager 2's solar system boundary, Mars rovers' water evidence, and Northern Lights dynamics.
Researchers compare images of Mars gullies to McMurdo Dry Valleys' saltwater flows, finding similarities that suggest liquid water on Mars. The study bolsters the notion of microbial life on Mars, as bacteria thrive in the Antarctic landscape's similar conditions.
Researchers found that Mars' surface remained molten for 100 million years, implying a thick atmosphere to insulate the planet and slow cooling. This persistence is surprisingly long, with implications for the planet's early history.
Recent high-resolution images from NASA's Mars orbiters show extensive evidence of ice-made features on the planet's surface, including glacial debris and valley deposits. The findings suggest a dynamic history of Martian climate change, with water ice playing a key role in shaping the planet's geology.
NASA's CRISM instrument provides critical data for selecting a Mars rover landing site with a mineral record indicative of past water. The instrument offers 544 spectral variations to detect minerals, mapping the Martian surface in unprecedented detail.
A heat-sensitive camera has discovered seven small, deep holes on the flanks of Arsia Mons, a giant volcano on Mars. The team suggests that these holes may be openings to underground caves, formed as faults created stresses that opened spaces underground.
A new approach to detect life on Mars, based on technology similar to pregnancy test kits, was successfully launched into space. The Life Marker Chip experiment has the potential to detect trace levels of biomarkers in the Martian environment.
The UK Space Exploration Working Group recommends involvement in both human and robotic elements of space exploration to play a full role in the century's unique opportunities. The report stresses the need for a new vision, suggesting preparatory human space flight activities and maintaining UK's significant role in planetary science.
Scientists using the Alpha Particle X-ray Spectrometer instrument have observed fluctuations in argon composition of the Martian atmosphere. The study reveals a constant change in the ratio of argon to carbon dioxide as winter sets in at one of the poles, indicating mixing between polar air and tropics.
The Phoenix Mars Lander Mission aims to study the history of water and search for complex organic molecules in Martian soil. The team, led by Kounaves, will analyze the chemical record left in the soil to decipher the climatic history of Mars, which may hold vital clues on climate change on Earth.
The BioSuit is a lightweight, skintight suit designed to allow superior mobility when humans reach Mars or return to the moon. It uses mechanical counter-pressure and stretches with the body, allowing freedom of movement.
Researchers suggest that perennial water-ice deposits at Mars' South Pole are juggled between the North and South Poles every 51,000 years due to precession. Water vapour is transported from the North Pole to the South Pole, where it re-condenses and freezes, forming a thick layer.
Researchers at the University of Michigan are conducting experiments to understand how Martian winds and dust affect NASA's Phoenix mission. They are simulating the effects of blowing Mars dust in a laboratory setting to provide insight for the Phoenix team.
Researchers found changes in Mars' topography that could be explained by surface deformation from 'true polar wander', a phenomenon where a planet's spin axis shifts. The study suggests large oceans on Mars existed in the past, with evidence pointing to the presence of vast oceans and massive deformations along ancient shorelines.
UC Berkeley scientists discovered that Mars' shoreline variations can be explained by the movement of its spin axis, and thus its poles. The team calculated that an initial shift of 50 degrees from today's pole would disrupt the Arabia shoreline.
A team of Canadian and U.S. researchers have found evidence that ragged features on Mars' surface were once shorelines of massive ancient oceans. The study suggests that a shift in Mars' spin axis within the past 2-3 billion years deformed these shorelines.
The University of Arizona's HiRISE team has released over 1,200 Mars images to the Planetary Data System, making them available to the public through a user-friendly viewer tool. The images reveal hundreds of important discoveries about Mars, including crater impacts and dust avalanches.
Scientists on NASA's Mars Exploration Rover mission found evidence of long-past explosive volcanic activity at Home Plate, a plateau in Gusev Crater. The data collected by the rover supports earlier findings that water once existed at or beneath the planet's surface.
Phoenix will use a robotic digging arm to determine if the Martian soil environment was favorable for microbial life. The lander is equipped with instruments that suggest frozen water exists within arm's reach of the surface.
Researchers found that water ice exists in variable depths and is patchy across the Martian surface. The discovery was made using data from NASA's THEMIS camera on the Mars Odyssey orbiter, which showed that areas with rocky surfaces have deeper ice deposits, while dusty areas allow ice to survive closer to the surface.
Researchers completed laying a 52 km cable for the Monterey Accelerated Research System (MARS) observatory, providing power and data connectivity to deep-sea instruments. The MARS system will enable continuous monitoring of ocean conditions, allowing scientists to track changes over time.
Researchers at Northern Arizona University have identified possible caverns on Mars that could provide a habitat for future explorers and potentially preserve evidence of past or present microbial life. The team used techniques developed for cave detection on Earth to analyze images from the Mars Odyssey mission.
The MARSIS radar has mapped the South Polar region of Mars, revealing a giant dome-shaped area composed mainly of ice. The radar signals have also identified depressions with variable distribution and depth of ice deposits at high latitudes.
The Mars Express radar instrument has mapped the thickness of dusty ice deposits at Mars' south pole, estimating a liquid layer about 11 meters deep. The findings suggest that polar layered deposits contain most of the known water on modern Mars.
Expert suggests searching for past life on Mars by exploring old rocks and sediments, using instruments to analyze biosignatures and organic materials. Robotic drilling technology currently limits to a few yards depth, making exopaleontology the best approach.
New images from NASA's Mars Reconnaissance Orbiter show linear fractures and 'halos' of light-toned bedrock, suggesting past fluid flow through underlying bedrock. The findings provide a promising site to search for evidence of habitable niches in the Martian past.
Current drills may find essential signs of life on Mars but can't reach the living cells that could survive in ice at Elysium or recent craters due to radiation levels, scientists say. The team found that drilling depth required for finding living cells is much deeper than current probes can reach.
Researchers have found evidence of ancient impact basins and topographic depressions in the Martian lowlands using MARSIS instrument, confirming the subsurface's complexity. The discovery sheds light on the geologic evolution of Mars, revealing a dichotomy between the northern and southern hemispheres.
A Queen's University researcher has discovered a mineral that could explain the mountainous landscape of Mars, suggesting the planet was likely wetter in the past. The study reveals layering in rocks indicative of sediment manipulated by water, which would require significant water on the planet at some point.
Mars Express's OMEGA instrument reveals a thick slab of dry ice in the cryptic region, but dust contamination is caused by geysers triggered by sunlight heating the soil beneath. The geysers create spots and fans, which suggest a process that could significantly contribute to the dust contamination observed.
The HiRISE camera took a remarkable picture showing the entire 800-meter Victoria crater and the rover down to its tracks and shadows. The images reveal a distinctive scalloped shape to the crater's rim, layered sedimentary rocks, and sand dunes on the floor.
Scientists are researching ways to reduce radiation-induced brain damage for Mars missions, which could lead to new treatments for conditions like Alzheimer's disease. The research project is part of a $14-million study funded by NASA to determine the human brain's maximum safe cosmic radiation dose.
University of Houston and Lunar Planetary Institute researchers use data mining and machine learning to analyze Martian surface patterns. They develop new computational tools to characterize large portions of the Martian landscape, aiding understanding of past water activity on Mars.
The UK is investing in the ExoMars mission to explore the Martian surface and search for signs of past and present life. The mission will also study the planet's geochemistry, water distribution, and geophysics, aiming to identify potential hazards for future human missions.
Research papers in Geophysical Research Letters highlight climate change impacts on Mars, with data from orbiting spacecraft and rovers revealing a hemispheric dichotomy. In the Arctic, sea ice reduction is linked to inflows from the Pacific Ocean, while the Indian Ocean experiences decadal variability in its circulation. Scientists st...
Researchers suggest that finding organic nitrogen on Mars would be a strong indication of past biological activity. The presence of nitrogen in the Martian atmosphere is unlikely due to the planet's lack of biological activity, making it an important target for search missions.
A comprehensive mineral history of Mars reveals that conditions became increasingly dry and acidic around 3.5 billion years ago, making it an unlikely place for life to thrive. The study identifies clay-rich rocks and soil as potential targets for future lander missions.
A Mars meteorite containing tiny burrows has been discovered, sparking interest in the search for life beyond Earth. The discovery, published in Astrobiology journal, suggests that Martian rock formations may be similar to those created by bacteria on Earth.
Researchers are searching for signs of life on Mars by analyzing the distribution of a specific type of nitrogen in Martian rocks, soil, and water. They found that organisms leave behind unique nitrogen 'fingerprints' on rocks, which could be used to detect biosignatures of past or present life.
Scientists have found that macromolecular carbon in Martian meteorites is always associated with magnetite, a mineral catalyst for its formation. This association raises hopes that the meteorite's carbon complexes could be evidence of non-biological synthesis of organic molecules on Mars.
Scientists studied magma chamber pressure changes following a massive lava-dome collapse on Montserrat, finding an unprecedented increase in pressure. Another study revealed a simplified model of rock fracture dissolution, which predicts a power-law distribution of channel lengths. Additionally, researchers explored aerosol transport a...
The Mars Express and NASA's Mars Reconnaissance Orbiter missions are providing valuable insights into Mars' upper interior. The combination of radars on the two missions will directly map the structure of the upper portions of the interior, revealing information about water, ice caps, and crust deformation.
Researchers at Boston University found that X-ray bursts from the Sun cause dramatic alterations to Mars' ionosphere, as detected by NASA's MGS spacecraft. The team used measurements on Earth to confirm the findings and gain a better understanding of the phenomenon.
Researchers from UC Berkeley found no signature of life in Earth's topography, contrary to previous assumptions. Instead, they suggest that life's influence is more subtle, shaping landforms like rounded hills and meandering rivers, but not creating unique features.
Researchers found that tropical glaciers on Mars were formed from snow brought from the polar regions, similar to Earth's mountainous regions. This discovery sheds light on past climate changes on Mars and potential pockets of ice scattered across the planet.
A new U. of Colorado study challenges previous findings on Mars' Meridiani Planum region, suggesting it was more geologically similar to volcanic regions in North America or Europe. The research proposes that the region's chemical composition was created by sulfur-bearing steam vapors moving up through volcanic ash deposits.
Researchers suggest that Martian features can be explained by meteorite strikes rather than evaporated lakes. Base surges from massive explosions caused by meteorite impacts result in simple and consistent explanations for rock formations and sediment layers found at the Opportunity site.
Researchers found ancient microbes in ice cores from Greenland, which could be a preview of what's discovered under Mars' surface. The discovery suggests that methane-generating Archaea might exist on Mars, and state-of-the-art instruments could detect them around meteor craters.
Researchers discovered hundreds of auroras on Mars over six years, linked to strong magnetic field patches in the crust. These events produce ultraviolet light and are not as colorful as Earth's auroras.
NASA's Spirit and Opportunity rovers are uncovering evidence of wet, possibly habitable conditions on Mars in areas they're exploring. They've found variations of bedrock, including platform-like structures, that suggest a hot, violent past with volcanic explosions and impacts.
The MARSIS radar has provided direct information about Mars' deep subsurface, revealing buried impact craters and hints of underground water-ice. The radar's measurements have changed our perception of the Red Planet, adding a new dimension to its knowledge.
MARSIS reveals a 'lumpy' ionosphere on Mars with unexpected bumps related to strong magnetic fields, providing insights into the planet's subsurface. The discovery sheds light on what happened to water that likely carved deep canyons on Mars.
Data from Mars Express confirms the presence of hydrated minerals, implying long-term liquid water on Mars during the Noachian era. Phyllosilicates and sulphates were detected in various regions, suggesting two distinct climatic episodes: a moist environment for phyllosilicates and an acid environment for sulphates.
ICESat measures polar ice sheets, clouds, mountains, and forests with three lasers, enabling scientists to see objects in three dimensions. The Geoscience Laser Altimeter System (GLAS) instrument has fired its one billionth shot, collecting detailed information on the vertical structure of the Earth system.
The European Space Agency's Venus Express spacecraft is on its journey to Venus, where it will study the planet's extremely hot atmosphere, high pressure, and mysterious 'super-rotation'. The spacecraft will deploy instruments to probe the surface and atmosphere, with a planned mission duration of at least two Venusian days.
The Venus mission aims to study the planet's surface and atmosphere, with a focus on volcanoes and potential biological activity. The spacecraft will use advanced instruments to detect 'hotspots' in the clouds and make a positive detection of volcanoes.