Articles tagged with Mars
Numerical simulations suggest asteroids Ryugu and Bennu may have formed from the disruption of a single parent asteroid. Analysis of return samples will verify this by measuring their composition and determining their formation age.
The MAVEN spacecraft has created a map of electric current systems in Mars' atmosphere, revealing a crucial role in atmospheric loss. The currents, generated by solar wind interaction, transform energy into magnetic and electric fields that accelerate charged particles into space.
Scientists studying Martian rocks find evidence of long-lived lakes, organic compounds, and a cold ancient environment. The discovery suggests that Mars' climate may have changed over time, with factors like volcanic activity and changes in the planet's obliquity contributing to these shifts.
A team of researchers recreated Martian conditions in a low-pressure chamber, observing the flow of mud that behaves similarly to pahoehoe lava flows on Earth. The study confirms sedimentary volcanism is possible on Mars, prompting a reevaluation of geological structures previously attributed to lava flows.
Researchers found that free flowing mud under Martian conditions behaves differently from on Earth due to rapid freezing and icy crust formation. The experimental mud flows formed similar shapes to 'pahoehoe' lava, explaining the formation of lava-like flow morphologies on Mars.
Scientists have measured the velocity of seismic waves in iron-sulfur alloys thought to comprise Mars' core, providing crucial information about the planet's internal structure. This study simulates the Martian core's composition and origin, helping researchers compare observations with Martian space probes.
A Southwest Research Institute scientist modeled Mars' atmosphere to determine that salty pockets of water on the Red Planet are unlikely to be habitable by Earth-based life. The study found stable brines could form seasonally, but temperatures are too low to support life.
Researchers from UBC have discovered a new timeline for the ancient magnetic field on Mars, with evidence of dynamo activity at 4.5 billion and 3.7 billion years ago. The findings suggest that the Martian dynamo was active earlier than previously thought, providing insights into the planet's thermal history and evolution.
Scientists have detected 4-billion-year-old nitrogen-bearing organic compounds in a Martian meteorite, suggesting early Mars may have been habitable and favourable for life to start. The discovery provides strong evidence that evidence for early life can be preserved and detected today.
Researchers analyzed satellite imagery and found river delta deposits in Jezero crater that formed over time scales promoting habitability and preservation of evidence. The study suggests ancient life could have existed near the Martian surface, with potential implications for understanding life evolution on Earth.
Researchers create tiny aircraft made from 'nanocardboard' that can levitate and carry payloads ten times heavier than themselves in the Martian atmosphere. The design uses a temperature differential to generate thrust, enabling the flyers to potentially serve as atmospheric probes on Mars, Pluto, and other planets.
Researchers have developed a biohybrid system that uses bacteria on nanowires to convert carbon dioxide and water into organic building blocks. The system has achieved a record efficiency of 3.6% in converting solar energy into carbon bonds, making it comparable to sugar cane's 4-5% efficiency.
Researchers analyzed Martian meteorites to reconstruct Mars' chaotic history and find that the planet likely received water from at least two distinct sources. The findings suggest Mars never had an ocean of magma completely encompassing the planet, contradicting previous theories.
Herold, a former tropical cyclone, has weakened to a low-pressure area with wispy clouds and minimal heavy rainfall. NASA's Aqua satellite provided forecasters with a visible image of the storm's center on March 20.
Astrobiologists Dirk Schulze-Makuch and Jacob Heinz found thiophene molecules on Mars consistent with biological origins. Non-biological processes, such as meteor impacts or thermochemical sulfate reduction, also remain possible explanations.
A new study reveals that a site in southern Germany's Nordlinger Ries crater may provide insights into Mars' ancient atmosphere. The team used nitrogen isotope ratios to estimate the pH of ancient waters, suggesting high levels of carbon dioxide could have made liquid water possible on the red planet.
The SEIS seismometer has measured over 174 probable 'Mars quakes', providing valuable data on the planet's composition. The analysis indicates a layer of rock 10 kilometres thick, with waves spreading at relatively slow speeds, suggesting fissured or chemically altered rock.
Researchers analyzed Marsquakes from InSight mission, finding moderate seismic activity intermediate between Earth and the Moon. The data revealed geological layers within the planet and identified areas of high geological activity, guiding future missions searching for potential life.
The NASA InSight lander has recorded over 450 marsquakes on Mars, providing insights into the planet's internal structure and tectonic activity. The data reveals a stronger attenuation in the upper mantle compared to the lower mantle, indicating a more fractured crust.
The InSight lander has detected gravity waves, surface swirling dust devils and the steady rumble of infrasound on Mars. The team also found daily pressure and temperature fluctuations stronger than on Earth, and convective vortices known as dust devils.
Scientists have discovered that Mars' magnetic field is ten times stronger than previously estimated, with fluctuations revealing clues about the planet's upper atmosphere. The findings provide valuable insights into Mars' interior structure and how it formed.
Scientists Takashi Yoshizaki and Bill McDonough developed a new compositional model for Mars, predicting the depth to its core-mantle boundary at around 1,800 km. The model suggests moderate amounts of sulfur, oxygen, and hydrogen in Mars' core, with the core accounting for only about one-sixth of the planet's mass.
Scientists modeled early impact events on Mars, revealing a heterogeneous mantle and challenging previous estimates of the planet's formation time. The new research provides insight into the Red Planet's evolution and composition.
A new study suggests that Mars' ancient waters were characterized by high salinity and a neutral pH, creating an environment potentially suitable for microbial life. The research found evidence of hyposaline lakes on early Mars, which could have supported life forms similar to those found on Earth.
Scientists have discovered evidence that the magnetic field forming around Earth was even stronger 4 billion years ago, generating a protective shield from harmful solar wind and cosmic rays. This finding has implications for understanding the future sustainability of Earth's magnetic shield and its potential for supporting life.
Researchers found large atmospheric pockets of water vapour at an altitude of over 80 km, accumulating in unexpected proportions. The capacity for water to escape increases during certain seasons due to the observed supersaturation rates.
Scientists studied Martian atmospheric water vapor using ExoMars Trace Gas Orbiter data, finding seasonal changes were the dominant regulator. The study suggests that warm seasons can lead to increased water loss into space, impacting Mars' continued desiccation.
Joanna Clark is developing a technique to study past Martian climate conditions using silica minerals. She plans to create silica minerals in the laboratory and analyze them for oxygen isotopes.
Researchers successfully collect wind data on Mars, revealing circulation patterns that bear the signature of mountains and valleys hundreds of kilometers below. The study's findings provide valuable insights into Martian climate and potentially inform studies on Earth's upper atmosphere.
Researchers at Embry-Riddle Aeronautical University present findings that a type of Martian aurora is the most common on the Red Planet, offering insights into water loss and climate change. The study uses data from NASA's MAVEN spacecraft to track hydrogen escape and understand how Mars' atmosphere has changed over time.
A new study using MAVEN data reveals that the proton aurora on Mars occurs more than 14% of dayside observations, increasing to over 80% during southern summer. This correlation suggests that changes in solar activity and Martian atmospheric conditions lead to increased water loss.
Researchers used MAVEN data to map global circulation of Mars' upper atmosphere, providing insights into the planet's climate stability and atmospheric waves. The study reveals simpler circulation patterns than Earth's, with stable winds over Martian seasons.
A new study models Earth's axis tilt and finds that 87% of exo-Earths in binary systems should have similar steady tilts, favoring climate stability for complex life. However, a modeled exo-Earth around Alpha Centauri B shows unstable dynamics due to the star system's powerful gravity, making it challenging for evolution.
A new study reveals that the Jezero crater landing site is home to hydrated silica deposits, which are exceptional at preserving microfossils and other biosignatures. The rover will be able to perform fine-scale chemical analysis and provide a close-up view of these deposits to help determine their origin.
Véronique Dehant's research aims to understand Mars' core, which is essential for determining the planet's habitability and potential for life. The ExoMars mission will collect Martian radio science data and analyze the planet's rotation to gain insights into its innards.
Kathy Benison, a WVU geologist, has been chosen as part of the Return Sample Selection Participating Scientist team for NASA's Mars 2020 expedition. She will help select promising rocks and sediments for the rover to cache or study on Mars.
A $1.2 million NSF-funded study led by Texas A&M University is exploring the use of virtual reality training simulators to train workers for extreme environments. The researchers aim to create a framework for scenario-based simulations and games that utilize virtual reality, eye tracking, and brain wave data.
Researchers at University College London analysed Martian landslide structures to understand their formation. The study found that high-speed rock particles and vibrations could create the unique ridges and furrows, contradicting the idea of icy substrates.
A team of scientists, including Texas A&M University researcher Marion Nachon, found that Mars' Gale Crater lake underwent drying episodes, potentially linked to the planet's global drying. The study reveals signs of liquid water and salt ponds similar to those on Earth, particularly in South America's Altiplano region.
Researchers successfully grew ten crops in Mars and Moon soil simulant, including garden cress, tomato, and radish. The study found that nine out of ten crops produced edible parts, with the exception of spinach.
A study published in New Space: The Journal of Space Entrepreneurship and Innovation models population growth, caloric needs, land use, and potential food sources to determine Mars' food self-sufficiency. A diet composed of plants, insects, and cellular agriculture can meet human nutritional requirements.
Researchers tripled the shelf life of ready-to-eat macaroni and cheese from 12 months to 36 months using a special coating that keeps oxygen away. The technology has benefits not only for space travel but also for improving military meals (MREs) and consumer food products.
A new study suggests that ancient Mars experienced warm periods with flowing water, followed by cold periods where water froze. This finding is significant as it increases the chances of simple life developing on Mars around the same time as it did on Earth.
Researchers at Newcastle University have found that wind erosion is unlikely to be the primary cause of methane gas release on Mars. The team used high-resolution imagery and data to rule out wind erosion as a viable mechanism for producing detectable levels of methane in the Martian atmosphere.
Brittany Seto, a UC Riverside alumna, interned at NASA's Jet Propulsion Laboratory and is now working on Mars projects. The university has set a record for the number of UCR undergraduates interning at JPL, with 22 students participating in the FIELDS program.
The three Mars rovers, including NASA's Perseverance rover, ExoMars rover, and China's HX-1 rover, will analyze rocks and soil for evidence of life on the Red Planet. The missions aim to determine whether life could have existed on Mars in the past.
Researchers at Beth Israel Deaconess Medical Center found that resveratrol supplementation preserved muscle function and mitigated muscle atrophy under Martian gravity. The study suggests that resveratrol could be a key dietary supplement to maintain musculoskeletal health on long-term Mars missions.
A Harvard study suggests that resveratrol can preserve muscle mass and strength in rats exposed to simulated Mars gravity, with almost complete rescue of front and rear paw grip. The compound's anti-inflammatory and antioxidant effects may help conserve muscle and bone in astronauts on long missions to Mars.
Silica aerogel could warm the Martian surface, increasing atmospheric pressure and temperatures similar to Earth's greenhouse effect. This regional approach to making Mars habitable offers a more achievable solution than global atmospheric modification.
Researchers discovered thriving bacterial communities in ancient, isolated brine samples from an Alaskan cryopeg. The findings provide insights into the potential for life on Mars and other planetary bodies.
Aarhus University researchers suggest a previously overlooked process explains methane's consumption on Mars, leading to doubts about its presence and potential biosignature. The new mechanism involves erosion and chemistry, affecting the possibility of life on or near Martian surface.
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 discovered that meteors create 'meteoric smoke' in Mars' middle atmosphere, condensing into thin clouds. These clouds have a significant impact on the Martian climate, influencing temperatures and potentially affecting past evolution.
Researchers have identified a bacterium, Sulfurihydrogenibium yellowstonense, as a potential sign of life on Mars. The bacterium can thrive in harsh environments with low oxygen levels and forms unique rock formations that resemble pasta, making it an easy target for detection.
A team of planetary scientists found that processes on Mars differ significantly from those on Earth, with large-scale features and differences in landform surface temperature playing key roles. The study reveals that active sand dunes are concentrated in three distinct regions, including Syrtis Major and North Polar Erg.
A new study suggests that a strange mineral deposit near the landing site of NASA's next Mars rover is likely sourced from ancient volcanic explosions. The research provides tangible evidence for the importance of explosive volcanism on early Mars, shedding light on the water budget, groundwater abundance, and atmospheric thickness.
Newly discovered layers of ice on Mars reveal a record of past climate and could hold the key to understanding if the planet was ever habitable. The ice reserves are estimated to be as much as 90% water, equivalent to a global layer 1.5 meters deep.
Scientists at the Swedish Museum of Natural History have compiled an atlas of fossils in volcanic rock to guide where and what to look for in the search for Martian life. The atlas aims to identify which types of microorganisms are most likely to have been preserved on Mars, based on their metabolism and geochemical conditions.
Numerical modeling explains the escape of hydrogen atoms from Martian atmosphere into outer space due to water photodissociation. Seasonal winds and dust storms affect water circulation, but not in an obvious way.
UTSA joins NASA's Resilient ExtraTerrestrial Habitats institute (RETHi) to advance space smart habitat designs for deep space habitats, leveraging expertise in civil infrastructure with advanced technology fields.