Articles tagged with Mars
Researchers develop a modular 'life detection platform' to directly detect and characterize microorganisms in extreme environments. The platform uses existing low-cost technology in new ways, enabling real-time analysis of microbial ecology and DNA sequencing.
A study published in Physical Review E suggests that Martian winds were capable of digging up tens of thousands of cubic kilometers of sediment from the Gale Crater over a billion years. The wind-driven movement of sediment and dust is thought to have played a key role in shaping the Martian landscape.
Scientists have identified eight locations on Mars with significant water ice deposits, providing insights into the planet's climate history and habitability. The ice is found to be cohesive and strong, with distinct layers that could help understand changes in Mars' climate over time.
A recent study published in Nature found that Mars' surface water was absorbed by its crust over time, leaving the planet essentially dry. The research suggests that approximately 300 meters of surface water on Mars could have been locked up in microscopic mineral structures.
Scientists propose that Martian surface reacted with water and then absorbed it, increasing rock oxidation. The planet's composition, temperature profile and iron content made the surface prone to reaction, dragging water down into the mantle.
The MAVEN mission helps answer the question of how long a rocky planet might be habitable by orbiting a red dwarf star. Based on Mars' atmospheric loss data, researchers estimated that such a planet's atmosphere could lose charged particles and neutral particles at significantly higher rates.
Researchers found that Mars' atmosphere is well-protected from the solar wind due to its induced magnetosphere. The study, led by Robin Ramstad, suggests that only a small portion of atmospheric pressure was lost over 3.9 billion years, contradicting previous assumptions.
The US space exploration program should focus on robotic sample recovery and human missions to Mars, according to Scott Hubbard, Editor-in-Chief of New Space. He highlights the benefits of this strategy, including offsetting costs through international partnerships.
Researchers propose a new scenario for ancient clay mineral formation on Mars, suggesting clays formed during the planet's creation from molten magma. The steamy atmosphere created by the magma ocean could have converted vast swaths of the surface to clay, leading to the widespread distribution seen today.
A team of scientists from MSU developed a compact spectral polarimeter for studying the surface composition of astronomical bodies. The device operates in the near-infrared range and was tested on two minerals simulating lunar and Martian surfaces.
A new study explores the impact of ice on Martian landslides, finding similarities with Earth's ice-lubricated landslides and demonstrating how ice influences shape and velocity. The research uses glacial morphology and remote sensing measurements to model landslide dynamics.
New research identifies Recurring Slope Lineae on Mars as granular flows, not liquid water, indicating present-day Mars may lack significant liquid water. The study supports the hypothesis that Mars is dry and limits Earth-like life near its surface.
A new University of Washington study reveals that Don Juan Pond in Antarctica is fed by a regional deep groundwater system, not from moisture seeping down from local valley slopes. This finding has significant implications for understanding the formation of similar environments on Mars.
Researchers found permanent effects on human brain structure due to microgravity, including crowding and narrowing of the brain's central sulcus. The study aimed to understand the causes of VIIP syndrome, a condition affecting astronauts' vision and intracranial pressure.
NASA engineer Justin Jones used an industrial X-ray CT scanner to evaluate volcanic rocks and other specimens, revealing previously undetected minerals and 3D arrangements. The technology has potential applications in planetary exploration, including the analysis of samples from Mars and asteroids.
Researchers found that CO2 sublimation can create unique features on Mars, such as Sand Furrows and linear gullies. These processes are unlike anything seen on Earth and provide new insights into Martian geomorphology.
The research found that Mars' magnetotail is unique, with a twist caused by magnetic reconnection between the solar wind and embedded surface fields. This process may also propel some of Mars' atmosphere into space.
A NASA study reveals that powerful solar eruptions could charge areas of the Martian moon Phobos to hundreds of volts, potentially affecting sensitive electronics. The charging effects could also affect astronauts on potential human missions to Phobos.
Researchers discover that non-thermal plasma can efficiently produce oxygen on Mars through decomposition of CO2. The process could provide a stable and reliable source of oxygen for manned missions, reducing costs and risks.
Researchers found a potential bridge between Martian geology and atmospheric models, suggesting peak daily temperatures above freezing could cause melting at glacier edges. This meltwater could have carved the features observed on Mars today, supporting the formation of water-carved valleys and lakebeds.
Researchers have discovered that a specific microbe can oxidize and metabolize metals from synthetic Martian regolith simulants, leaving behind unique signatures. This finding could enable the extraction of metals from asteroids and other celestial bodies using biological methods.
Researchers analyzed the structure of mimetic Martian water to understand how it could exist on the Martian surface. They found that concentrated perchlorate solutions could survive low temperatures, raising questions about the possibility of life on Mars.
Researchers explored racial microaggressions in STEM fields, finding they negatively impact underrepresented scientists. In another study, a 'dynamical shake-up' model explains why Mars is so small and there are no planets in the asteroid belt.
The article discusses a debate over Mars exploration strategies, with some experts proposing the relaxation of planetary protection policies to expand the search for life on Mars. Current robotic missions may be hindering the discovery of Martian life due to contamination concerns, but easing policies could lead to breakthroughs.
Scientists from the University of Bristol have discovered evidence suggesting that massive collisions during planetary accretion resulted in significant mass loss, altering a planet's composition. This process, which occurred in the Earth and Mars formation, led to their distinctive volatile poor compositions.
The NASA Mars 2020 rover will feature a new SuperCam instrument with Raman spectroscopy capabilities, allowing it to detect carbon-based signatures of organic materials. The instrument uses a conduction-cooled laser system and can produce 1000 shots in one burst, significantly improving sampling efficiency.
Researchers propose using the element vanadium to verify microfossils for signs of life on Mars. Vanadium can substitute into biological compounds and is found in known biological sources, such as chlorophyll.
Researchers have found river deposits on Mars that date back over 3.5 billion years, indicating a surface environment capable of supporting liquid water. The study suggests that large fluctuations in the size of the water body forced the formation of paleo-valleys, revealing long-term stability in the controlling water body.
Researchers found a lower density in Mars' crust, indicating possible porosity, which could impact the planet's formation and evolution. The new gravity map reveals variations in crust thickness beneath volcanoes.
Scientists discovered borates in a Martian crater, indicating that ancient conditions were favorable for RNA synthesis and potentially life. The presence of boron on Mars adds to evidence for habitability, opening possibilities for life's origins.
The Mars 2020 mission utilizes advanced techniques developed from studying early life on Earth to detect biosignatures in ancient Martian rocks. By mapping elemental and organic composition at high spatial resolution, scientists aim to determine if these features were formed by life.
The Planetary Spectrum Generator (PSG) is being enhanced with additional databases to provide more accurate predictions of instrument performance. This will enable scientists to design and plan future missions more efficiently, reducing costs and resources.
The Hubble Space Telescope has captured images of Phobos, the smallest moon in our solar system, as it orbits Mars. Phobos is just 16.5 miles across and completes an orbit in just 7 hours and 39 minutes, faster than Mars' rotation.
A new study suggests that a massive asteroid impact early in Mars' history could explain the planet's unique geological features. The research proposes that an asteroid at least 1,200 kilometers across crashed into Mars, depositing rare metals and creating the planet's hemispheres.
Researchers suggest using telepresence technology to reduce communication delays in space research, enabling scientists to conduct scientific investigations more quickly. This approach could expand the number of destinations where humans can do great science, including those currently inaccessible due to safety concerns.
MAVEN has made several groundbreaking discoveries about the Martian upper atmosphere, including unexpected exchanges of gas between lower and upper atmosphere layers. The mission has also revealed complex interactions between solar wind and planet, resulting in the loss of atmospheric gas to space.
The article presents Elon Musk's vision for a self-sustaining city on Mars, requiring significant improvements in transportation costs. The CEO of SpaceX discusses the advantages of using Mars as a hub for a multi-planetary species, including its planetary options and system architecture.
Researchers propose that Mars' Lyot valley networks were carved by meltwater produced when hot ejecta interacted with an icy surface. The team estimates thousands of cubic kilometers of meltwater were generated, enough to shape the valleys.
Researchers have solved a long-standing riddle in the analysis of meteorites from Moon and Mars using high-pressure experiments at DESY's X-ray light source PETRA III. The study reveals that cristobalite can transform into seifertite under non-hydrostatic conditions, challenging previous assessments of meteorite formation conditions.
A new study published in Nature Communications estimates that the ancient network of valleys on Mars required at least 10 times more water than previously thought to carve out. The research suggests that Mars once had a warmer climate and active hydrologic cycle, with an ocean playing a key role in shaping the planet's landscape.
A new predictive model shows that radiation from cosmic rays can extend to healthy cells, doubling the cancer risk for astronauts on Mars missions. The study, published in Scientific Reports, highlights the need for additional research on cosmic ray exposures prior to long-term space missions.
The Curiosity rover mission has provided insights into a long-lasting lake on ancient Mars, which was stratified with distinct chemical and physical differences between its deep and shallow waters. The study found that the shallow water carried more oxygen at certain times, affecting mineral deposits and life's potential.
Scientists have discovered 'halos' on Mars that indicate the planet had liquid water much longer than previously believed. The finding reveals substantial amounts of groundwater were present for a longer period than thought, further expanding the window for when life might have existed on Mars.
A new scaling law has been developed to predict how objects move through sand, enabling the design of more optimized vehicles. The law, derived from common equations for granular flow, can be used to scale results between small-scale experiments and full-size vehicles.
Scientists have discovered 'halos' on Mars, indicating that liquid water lingered longer on the planet than previously believed. The findings suggest that substantial groundwater was present in Gale crater's past, expanding the window for when life might have existed on Mars.
A NASA scientist is developing an instrument to search for signs of life on Jupiter's moon Europa, leveraging experience from building a Mars instrument. The Ocean Worlds investigation will analyze molecular biosignatures in surface and subsurface samples.
New evidence suggests different origins of topography on Earth, Mars and Titan. Researchers found plate tectonics to be a key factor shaping Earth's surface but not as influential on Mars and Titan.
Researchers analyzed drainage patterns on three planets, revealing that long-wavelength features dominate the layout of river networks. The study suggests that short-wavelength features like mountains can divert rivers, leading to poor correlation between river flow directions and large-scale landscape topography.
Researchers found that Titan's topography may grow through tidal changes in its icy crust, unlike Earth and Mars which underwent active plate tectonics. The study also sheds light on Martian topography, suggesting major features formed early in the planet's history.
Researchers discovered that Titan's river networks, like Mars', formed topography without plate tectonics. This finding suggests a distinct geological history for the moons of Saturn and challenges our understanding of Earth's unique surface.
Researchers found that heavy rainfall on early Mars carved out river-like channels and altered impact craters, similar to Earth's effects. The study used physics principles to understand the relationship between Martian atmosphere pressure, raindrop size, and rainfall intensity.
Research by Brown University geologists reveals that ancient Mars impacts generated tornado-like wind vortices that scoured the surface, exposing blockier surfaces beneath. The winds, which reached speeds of up to 500 miles per hour, were responsible for creating bright streaks on the Martian surface.
A team of engineers at the University of California San Diego discovered a simple, no-bake method to make bricks from Martian soil by applying pressure. The resulting bricks are stronger than steel-reinforced concrete and may be compatible with additive manufacturing.
A team led by Dr. Bill Bottke from Southwest Research Institute discovered a 400-million-year lull in Mars' giant impact history, closely paralleling the bombardment histories of the Moon, asteroid belt, and Mercury. This finding supports the Late Heavy Bombardment theory and highlights an important period in Martian evolution.
Researchers have published a detailed geological history for Northeast Syrtis Major, a region on Mars known for its striking mineral diversity. The study maps the extent of key mineral deposits across the surface and places them within the region's larger geological context. This work could help inform NASA's decision on potential land...
The study detects iron, magnesium, and sodium ions in the Martian upper atmosphere, indicating a permanent presence of metal ions. The team believes that all solar system planets with substantial atmospheres likely have metal ions.
New measurements reveal that 66% of Mars' argon has disappeared from its thin atmosphere since formation, leading to huge climate changes. The research suggests that Mars once had a thicker atmosphere composed mainly of carbon dioxide, which was largely lost due to solar wind bombardment.
The study found that most of the Martian gas has been lost to space due to solar wind and radiation stripping, altering the planet's climate and habitability. The loss of argon and CO2 indicates that the atmosphere was once warm enough to support liquid water and life.
Researchers have identified a key step in the molecular process of DNA repair and found a treatment to reverse aging, improve DNA repair, and potentially mitigate effects of cosmic radiation. Human trials are set to begin within six months.
Researchers propose that debris from an asteroid impact could have formed Mars' rings, which would then break apart and re-form into moons. The model suggests that this cycle may repeat, potentially explaining sedimentary deposits found on Mars.