Articles tagged with Mars
Researchers used a climate change model on Earth to analyze Mars' polar regions, finding a correlation between the layers of ice and dust and changes in climate. The study suggests that Mars' climate changes can be explained by orbital theory, similar to Earth.
A new undersea data network, MARS, will be deployed in Monterey Bay to provide real-time monitoring of ocean conditions. The network will support a variety of research devices and supply power to instruments, enabling continuous and long-term data collection.
Researchers conducted a high-tech simulation to test the Mars Exploration Rover mission, which will arrive on Mars in early 2004. The test aimed to understand the nature and accumulation patterns of Mars' signature red dust, crucial for ensuring astronaut safety.
The proposed system uses autonomous spaceships to transport crews between Earth and Mars, enabling frequent 5-month trips. The design architecture includes Astrotels and Taxis, which will facilitate sustainable Mars habitation and exploration.
MERBoards will provide a new tool to support collaborative processes in Mars Surface Operations, enhancing mission operations with interactive displays and annotation capabilities.
The Marsquake sensors will detect weight shuddering caused by liquid water beneath the Martian equator, pinpointing each quake's location. This new method will help scientists find life on Mars and shed light on the planet's internal structure.
A recent study by Dr. Lidija Siller from Newcastle University suggests that water might be trapped beneath the surface of Mars' south polar ice cap, a key factor in the formation of life on the planet. The research involves studying photochemical reactions in ice and has potential implications for the detection of life on Mars.
Researchers found that volcanic regions on Mars' Hellas basin were eroded by liquid carbon dioxide due to explosive eruptions. The 'magmatic erosion model' suggests catastrophic erosion occurred when molten rock rose to the surface, causing debris flow and shaping features.
Professor Norman Pace believes life exists elsewhere in the universe due to non-equilibrium gases like oxygen and methane. However, he doubts Earth-like conditions on Mars and Europa can sustain life.
As scientists search for life beyond Earth, the possibility of microbial disease-causing organisms emerging in new environments raises concerns. Experts like Salyers highlight examples of unexpected adaptations, such as Legionnaires' disease and Listeria monocytogenes, which can thrive in harsh conditions and cause human disease.
Researchers plan to use cycler spacecraft, which would constantly ferry people and materials between Earth and Mars, to enable human exploration and colonization of the Red Planet. The cyclers would rotate slowly to create artificial gravity and provide comfortable accommodations for passengers on long trips.
Scientists found a unique microbial community in Idaho's Beverhead Mountains that thrives without sunlight, using hydrogen gas from deep Earth as an energy source. This discovery mirrors Martian subsurface chemistry and has implications for searching for life on Mars.
Recent Martian gullies and debris flows likely resulted from the melting of near-surface ground ice due to warming temperatures. The orientation of these features closely matches the predicted latitudinal distribution of warmest near-surface temperatures at high obliquity.
Researchers found dramatic erosion of frosty layers on Mars' south pole, suggesting global climate change. The Martian snow is dense and ice-like, and its seasonal cycle affects the planet's long-term climate and atmosphere.
Researchers analyzed topographic maps and meteorites to determine that water circulated in the upper part of Mars' crust within the last billion years. This finding suggests that water may still be present near the surface, with evidence of recent gullies forming in high-latitude regions.
A recent discovery of buried impact craters on Mars indicates that the planet's northern lowlands formed very early in its history, possibly as a result of a shallow ocean. This finding provides crucial insights into the origin of Mars' crustal dichotomy and challenges traditional theories about the planet's geological evolution.
Recent studies on Mars' Elysium and Amazonis Planitia regions reveal regionally extensive lava eruptions from the same vent system as water. The findings suggest that these volcanic and hydrologic events are both young and related in origins, potentially indicating ongoing volcanic activity.
The Mars Odyssey spacecraft has entered into orbit around Mars, providing a key communications link for the Mars Exploration Rover (MER) mission. The two Rovers will be able to upload data on mineral and element composition of rocks and soils to a state-of-the-art communications package.
NASA's Mars Global Surveyor and Hubble Space Telescope provide a unique view of the largest global dust storm on Mars in several decades. The storm, which has engulfed the entire planet for three months, raises questions about Mars' thin atmosphere and climate change.
A USC neuroscientist re-analyzed data from the Viking landers, finding a distinct biological rhythm in the soil that suggests the presence of life. The signal has a precise circadian rhythm of 24.66 hours, entrained to temperature fluctuations on Mars.
Researchers at Brown University have discovered direct evidence of climate change on Mars, finding that water ice was once present closer to the equator. The findings suggest that the icy region has moved from the planet's poles to nearer its equator due to climate change.
Scientists have observed a sudden shift in Mars' atmosphere, with temperatures increasing by about 30 degrees Centigrade, due to a massive dust storm. This phenomenon is similar to Earth's global warming, but much more extreme and potentially leading to a significant cooling of the planet.
Dr. Baerbel K. Lucchitta's research finds that some Martian outflow channels display similar characteristics to those on the Antarctic sea floor, carved by ice streams. The study suggests an ancient ocean may have existed in Mars' northern plains.
Researchers believe that parts of ancient Mars may have resembled a land of lakes, with layered geologic outcrops suggesting sedimentary rock deposited in horizontal layers. The discovery suggests an extremely dynamic environment on early Mars, with water likely playing a key role in shaping the planet's geology.
Scientists have discovered a wealth of green minerals, including olivine, on the Martian surface, indicating low levels of chemical weathering by water. This suggests that Mars has remained cold and dry for most of its geologic history, contradicting previous theories about a warm, wet past.
Researchers found that a specific orbital alignment in 2014 provides an ideal escape route back to Earth in case of an emergency on the way to Mars. This trajectory is only possible within a few days of January 14, 2014, making it a critical launch window for future human missions.
Cornell University has been selected by NASA to lead the science team for the next Mars mission, which will include a large roving vehicle carrying six scientific instruments. The rover's Pancam panoramic camera system will reveal terrain around the vehicle and help select rock targets for study.
A new study by Dr. Laurie A. Leshin found that the crust of Mars may hold two to three times more water than scientists had previously believed. The research compares the amount of deuterium in a meteorite with the Martian atmosphere, suggesting that significant groundwater reservoirs currently exist on the planet.
A recent analysis of a 1.2 billion-year-old Martian meteorite has shown the presence of water-soluble ions that resemble those found in Earth's oceans. The study suggests that ancient Martian oceans had a chemical composition similar to Earth's, with elements like sodium and chloride present in high concentrations.
Researchers from Malin Space Science Systems found steep-sided gullies and sinuous channels that suggest liquid water may be present beneath the Martian surface. The team proposes a scenario where water seeps through porous rock layers, builds up pressure, and eventually bursts forth in short-lived torrents.
The Mars Global Surveyor's Thermal Emission Spectrometer has mapped the mineral composition of Mars' surface, revealing a primarily volcanic surface with distinct differences between southern and northern hemispheres. The survey provides valuable insights into Martian geology and may help explain changes in the planet's interior.
NASA scientists presented new findings on ozonesonde data, glaciers, Mars impact features, Landsat-7 mission performance, tropical landscapes, and more. The results include insights into ozone layer changes, ice stream movements, and buried impact basins on Mars.
Researchers use data from the Mars Orbiter Laser Altimeter to test hypotheses of oceans on Mars, finding four types of quantitative evidence supporting an ancient ocean. The discovery has implications for understanding long-term climate change and its relevance to Earth's future.
The Mars Descent Imager will capture a series of about 20 images of the Martian surface, from 4 miles to 30 feet altitude, using a 'nesting' technique to create a complete scale of pictures. The high-resolution images will aid in studying the layers of ice and dust covering the polar region.
The University of Iowa team will use a low-frequency radar to probe beneath the Martian surface and study the planet's ionosphere. The goal is to detect signs of liquid water, which may be responsible for carving the planet's canyons.
Researchers have created a highly accurate global map of Mars' topography, providing insights into the planet's evolution over 4 billion years. The map reveals the Hellas basin's massive size and its impact on water transport and cycles, with dramatic slopes affecting ponding of water in certain areas.
Magnetic patterns on Mars indicate ancient plate tectonics system, with implications for understanding of the planet's topography. The team found evidence of symmetrical mirror-image stripes, similar to those on Earth, which could be remnants of a long-lost plate tectonics system.
Scientists have discovered magnetic stripes on Mars, similar to those found on Earth, suggesting the planet was once magnetized and had a global magnetic field. These findings provide insights into Mars' formation and evolution, shedding light on its potential for hosting liquid water.
The Mars Pathfinder mission sent back 2.3 gigabits of new data, including over 17,000 images and 16 chemical analyses of rocks and soil. The mission provided key findings on Mars' geology, magnetic properties, atmosphere, and cartography.
The sundial is designed to track the passage of hours and seasons on Mars, with calibration targets to adjust camera brightness and tint. The instrument carries a message from Earth to future Martian explorers, wishing them a safe journey and joy of discovery.
Researchers identify smaller, bright sand dunes formed of sulfates possibly gypsum, while larger dark dune fields are made of grains eroded from lava flows. The winds on Mars create landforms remarkably similar to those in some deserts on Earth.
Researchers from CU-Boulder will create a virtual sensor by combining data from two instruments orbiting NASA's Mars Global Surveyor satellite. They aim to identify the surface composition of Mars' polar ice and plot its perimeters, gaining insights into climate change on both Earth and Mars.
A new study using precise elevation measurements from the Mars Global Surveyor spacecraft provides a detailed picture of Mars' north polar region. The findings suggest that any water in the region should flow towards the pole, rather than the equator, due to its depression-like structure.
The University of Florida is part of a virtual Astrobiology Institute studying the origin and evolution of life in the galaxy. Chemists are searching for universal DNA features that could be found in potential Martian life, which may help overcome the difficulty of recognizing non-terrestrial life.
Recent analysis of Mars data from the Mars Pathfinder Mission suggests that the C1 carbonaceous chondrite standard is incorrect, with Mars exhibiting a distinct elemental composition. This contradicts previous assumptions about the terrestrial planets' formation and density variations.
Scientists estimate a small amount of life could have existed on Mars through chemical reactions over billions of years. They also explore the possibility of life on Europa, estimating lower energy availability than on Mars.
A new Martian meteorite was discovered in the hot desert climate of the Sahara, increasing the total number of Martian meteorites to 13. The meteorite's inert gas inventory and elemental ratios confirm its Martian origin, providing valuable insights into Mars' geochemical processes and evolution.
Researchers discovered bacterial colonies thriving in Antarctic ice, surviving on minimal light and water. The findings suggest similar life forms may exist on Mars or Europa, and could provide insights for searching for life beyond our solar system.
Researchers at Arizona State University have found a large deposit of mineral hematite on Mars, suggesting the presence of hydrothermal activity and potentially water in the past. The find makes a strong case for future NASA missions to explore this area near the Martian equator.
The U.S. Geological Survey is using GIS techniques to investigate the origin of ancient river valleys on Mars and map impact craters, faults, and volcanoes. The research reveals that geothermal activity led to valley formation on early Mars.
Scientists from NASA's Marshall Space Flight Center discuss approaches to building lunar and Martian bases using in situ materials. Processing materials will be a challenge due to low gravity, which affects metal behavior and microstructure formation.
A team of Cornell experts is creating a database of food-processing information and menu items for NASA's future lunar and Martian colonies. The recipes, which include vegetarian options like seitan tacos and pasta primavera, will be grown hydroponically in space farms using crops such as wheat, potatoes, rice, soy, and peanuts.
The APXS instrument provides new insights into Martian soil and rocks, revealing a more Earth-like composition than previously assumed. The study suggests that Mars has complex geological provinces with varied compositions, indicating a more evolved planet.
Scientists confirm evidence of past water on Mars, including minerals and sedimentation patterns. Theories about the disappearing water include evaporation, seepage, or storage at Martian poles.
Researchers propose that reflective carbon dioxide ice clouds on ancient Mars retained thermal radiation near the surface, warming it enough for liquid water to exist. This mechanism provides clues about potential life forms on Mars and extends the habitable zone on extrasolar planets.
The Mars 2001 Lander mission aims to investigate the geological record of ancient Martian waterways and possible biology. Cornell's Athena rover will use its integrated scientific instruments to collect data on the planet's surface, including an imager, infrared spectrometer, and Alpha-Proton-X-Ray spectrometer.
The Mars Global Surveyor mission will spend nearly two years collecting data as it maps Mars' surface and atmosphere. The spacecraft will use aerobraking to trim its path around the planet, allowing for a global portrait of Mars' topography, mineral composition, and interior.
A study of Martian meteorites suggests that Mars formed quickly and became geologically quiet, with little plate tectonics. This process allowed the planet's internal structure to remain relatively unchanged since its earliest history.
A recent meteorite study has provided insights into Mars' formation by analyzing volatile elements in Martian meteorites. The findings indicate that the planet experienced at least two fractionation events, which allowed all elements to remain and record past events.
Researchers support a low-temperature origin for carbonate globules in the Martian meteorite ALH84001, suggesting microscopic depositions may be fossilized bacteria. The study uses secondary ion mass spectrometry to analyze oxygen and carbon isotope ratios, indicating a potential formation temperature of less than 300 degrees C.