Articles tagged with Planetary Surfaces
A University of Calgary scientist proposes two novel geoengineering approaches to mitigate global warming: releasing engineered nano-particles and sulphuric acid. These methods aim to reduce the negative effects of sulphates, which are blunt instruments for climate engineering.
Researchers found that ancient cratonic roots have low water content beyond a certain depth, making them harder to deform or break up. This explains why these roots are resistant to destruction and preserved the oldest continents.
Scientists studying the Venus Express mission have found that Venus likely had oceans billions of years ago, but they were likely atmospheric and short-lived. The loss of water into space has left the planet's surface dry today.
A new model of tectonic-plate movements has been developed by University of Wisconsin-Madison geophysicist Chuck DeMets and his collaborators. The MORVEL model offers a precise description of the relative movements of 25 interlocking plates, accounting for 97% of the Earth's surface.
MESSENGER will zip within 142 miles of Mercury's surface, taking high-resolution color images and ultraviolet measurements. CU-Boulder's MASCS instrument aims to pinpoint iron on the planet's surface, which maintains its magnetic field.
The rover Opportunity has revealed new insights into Mars' geologic history, including the presence of hematite spheres, sulfate-rich sandstone, and minerals commonly found in meteorites. The data supports previous findings that water once flowed on Mars' surface, with a likely underground source.
Researchers from University of Alaska Fairbanks present research on planetary landscapes using computer models and satellite images. The team also explores new tools to support countries' claims to resources and collaborates with Google on K-12 outreach and education initiatives.
A CU-Boulder study suggests a single plume of hot material drove the migration of volcanic activity on Mars. The theory, proposed by Shijie Zhong, explains how the Tharsis Rise region formed and how the Crustal Dichotomy's crust moved relative to the underlying mantle.
A new MIT study suggests that young, hot planets like Earth could stay hotter for millions of years, making them detectable by current telescopes. This extended molten surface would increase the brightness of the planet in infrared light, reducing the contrast with its star and allowing for easier detection.
MESSENGER spacecraft will make its second flyby of Mercury on Oct. 6, providing a region unseen before by spacecraft and revealing details about the planet's atmosphere and surface. The mission aims to gather data and images from Mercury for about 90 minutes, including observations in the far ultraviolet portion of the light spectrum.
McGill researchers have found the oldest rocks on Earth, dating back to around 4.28 billion years ago. The discovery provides new insights into the early separation of Earth's mantle and crust, shedding light on the planet's mysterious beginnings.
A University of Michigan instrument on the MESSENGER spacecraft has detected silicon, sodium, sulfur, and water ions around Mercury, suggesting that they were blasted from the surface or exosphere by solar wind. The findings provide a new understanding of Mercury's composition and its interaction with the sun's magnetic field.
Researchers from Brown University have discovered evidence of past volcanic activity on Mercury, suggesting that the planet underwent intense changes to its landscape around 3-4 billion years ago. The findings were made possible by detailed images from NASA's MESSENGER spacecraft and provide new insights into Mercury's geologic history.
The MESSENGER spacecraft completed its first flyby of Mercury, collecting scientific data and imagery of the planet's surface. The mission will provide new insights into Mercury's previously unseen surface features.
Scientists at CU-Boulder's Laboratory for Atmospheric and Space Physics are leading a team that will make measurements of Mercury's surface and tenuous atmosphere using the MESSENGER spacecraft. The mission will provide new insights into the composition, formation, and evolution of Mercury.
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.
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.
Researchers have created conditions similar to those inside the Earth to study its inner workings. The study provides new insights into the planet's materials and processes under high pressure, revealing surprising findings about the D'' layer near the core.
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.
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.
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.
Jupiter's atmosphere is driven by heat from within the planet, creating organized wind chaos. The computer models explain why there are two classes of jet winds: strong and narrow near the equator, but weak and wide at higher latitudes due to the planet's curvature and rotation.
A new study by Dartmouth researchers suggests that methane on Mars can be produced from non-living sources, including the mineral olivine. The findings provide a plausible explanation for a warmer and wetter early Mars, with abundant liquid water present on the surface.
According to a new study published in Science, the Earth's surface has been getting brighter for more than a decade, with an increase of about 4% over the past decade. This trend may accelerate warming at the surface and unmask the full effect of greenhouse warming.
Researchers at Ohio State will develop a new radar instrument to peer beneath earth's ice cover and analyze how ice accumulates. The project aims to understand the impact of melting ice on global sea levels and temperature regulation.
The Cassini mission has captured high-resolution images of Titan, revealing a geologically young surface with signs of tectonic resurfacing and erosion by liquid hydrocarbons. The surface features complex patterns, including channels and linear boundaries, indicating ongoing geological processes.
Researchers found diverse surface materials, including hydrated minerals, which suggest water was common on Mars. The study suggests areas like Syrtis Major, Valles Marineris, and Terra Meridiani are strong candidates for future Mars missions.
Scientists at Columbia University's Lamont Doherty Earth Observatory have made new discoveries about the formation of underwater mountains along the Mid-Ocean Ridge. They found that the height and width of these mountains are highly correlated to the direction the ridge and connecting plates move across the planet's surface.
The MARSIS project aims to probe several miles beneath Mars' surface and study the ionosphere. Researchers hope to detect signs of liquid water, which may have shaped the planet's deep canyons.
Researchers are studying Europa's icy shell to understand its composition and potential for supporting life. A computer model suggests organisms could thrive beneath the thick cap of ice, while another analysis reveals cracks and ridges formed by Jupiter's tides.
Scientists at the University of Michigan have developed a model that explains how slabs in the Earth's mantle drive convection and surface plate motion. The research found that slabs attached to plates can directly pull them towards subduction zones, while those not well attached create suction forces drawing nearby plates towards the ...
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.
Researchers believe that lunar debris may hold fossils from Earth's early microbial life, with potential insights into the evolution of life on our planet. By studying this ancient material, scientists can gain a better understanding of the moon's role as a window into Earth's history.
Global Aerospace Corporation wins NASA award to develop DARE system, which uses autonomous balloons to explore planetary atmospheres and surfaces from atmospheric altitudes. The system can deploy micro probes to study the atmosphere, surface, and subsurface, offering high-resolution imaging and direct measurements.
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.
Arjun Heimsath, a Dartmouth College researcher, measures dynamic land movement by calculating erosion rates in different parts of the world. Using cosmic isotopes extracted from rock and sediment samples, he determines how long material has been there and how fast it's eroding or breaking down.
The Near Earth Asteroid Rendezvous (NEAR) mission will attempt a controlled descent to the surface of asteroid 433 Eros on February 12, gathering close-up pictures of its boulder-strewn surface. The primary goal is to study the asteroid's composition and behavior, with a secondary aim of practicing maneuvers for future landing missions.
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.
The NEAR Shoemaker spacecraft will embark on a series of low-altitude passes over asteroid 433 Eros from Jan. 24 to Jan. 28, gathering detailed images of the surface. The controlled descent, set for Feb. 12, aims to capture high-resolution close-ups of Eros' cratered landscape.
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.
A University of Colorado Boulder research team has confirmed a theory about charged dust in space, explaining how it affects spacecraft and astronauts. The study used an experiment to levitate particles with positive charge above the moon's surface.
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 NEAR Shoemaker mission suggests asteroid Eros is a primordial relic from the solar system's formation, with an elemental composition similar to chondritic meteorites. Studying Eros could help scientists understand how rocky planets evolved.
A team of Boston University astronomers has captured new ground-based photos of Mercury's surface, revealing details similar to those on the Moon. The images, taken in August 1998, show bright craters and dark lunar mare-like markings, providing insights into Mercury's geology.
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.
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.
Researchers at Columbia University have found a link between the greenhouse effect and warmer winters in the northern hemisphere. They used a NASA model to suggest that increased greenhouse gases are causing stronger winds to carry warmer air from oceans to continents, leading to colder continental air near the oceans.
A critical chemical reaction previously thought to support microbial life deep below Earth's surface is now considered highly unlikely. Microorganisms are likely living on organic matter associated with rock, not hydrogen, according to researchers.
Scientists have gained a clearer picture of massive volcanic eruptions by analyzing lava composition, indicating that the lava originated from the lower mantle. The findings suggest that the eruptions played a role in the greatest mass extinction event in Earth's history, wiping out up to 95% of plant and animal species.
Io's volcanic hot spots reach surface temperatures of over 2,200 degrees Fahrenheit, more than double previous measurements. The extreme temperatures suggest a unique process of differentiation and heavy element composition, shedding light on the moon's geological history.
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.
A new model of Venus suggests that crustal plateaus and volcanic rises were formed by a mechanism similar to hot spot plumes, a process still active on Earth. The thickening of the Venusian lithosphere approximately one billion years ago largely shut down the creation of crustal plateaus.
Recent data from NASA's Galileo spacecraft suggests that Jupiter's moon Europa may have a slushy ocean beneath its icy surface, with evidence including shallow impact craters and gaps in the ice. The findings support the idea that warmth from tidal forces could be keeping parts of the ocean liquid.
Geologist Professor Joseph Smyth discovered wadsleyite can contain solid water bound in crystals at extreme pressures. The earth's interior may store large amounts of water in the form of wadsleyite, which could regulate surface water levels. Laboratory tests are underway to determine the amount of water in wadsleyite.
Scientists have discovered oxygen locked in ice on Callisto, a moon of Jupiter, with sunlight playing a key role in separating hydrogen and oxygen atoms. Meanwhile, the Galileo team has found that sulfur dioxide emissions from Io are caused by both volcanic activity and frost sublimation.
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.
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.