Articles tagged with Planetary Surfaces
Scientists have discovered that stagnant lid tectonics, not plate tectonics, existed on early Earth, releasing heat and forming continents. This finding contradicts previous assumptions about the role of mobile plate tectonics in life's emergence, suggesting an alternative mechanism was present.
Researchers have found high levels of phosphates in the water on Saturn's moon Enceladus, a key component of DNA and cell membranes. The discovery increases the chances of finding habitable worlds across the galaxy, as Enceladus can support life over a wider range of distances from its star.
Researchers at the University of Birmingham are studying how humans can live and operate on Mars, simulating conditions using a unique facility 1.1 km below the surface. The project aims to investigate biomedical procedures for treating tissue damage in space crews.
The newly discovered exoplanet LP 791-18 d orbits a small red dwarf star in the habitable zone, where liquid water could exist on its surface. Volcanic activity on this planet may sustain an atmosphere and potentially lead to the formation of life.
Astronomers have discovered an Earth-sized planet, LP 791-18d, with active volcanoes that could sustain an atmosphere, potentially allowing for liquid water and life. The planet's unique tidal locking creates a permanent day and night side, with the night side possibly experiencing condensation of water vapor.
Researchers determined the Martian crust's global structure using seismic data from a massive marsquake. The crust averages 42-56 kilometers in thickness, with variations between the northern and southern hemispheres.
Researchers developed a model to describe the interaction between a rocket plume and planetary surfaces, providing insights into erosion and contamination. The simulation estimates plume shape, temperature, and pressure, as well as material eroded or displaced, for safer landing sites and spacecraft design.
Researchers used NASA InSight data to directly measure Mars' core properties, finding a completely liquid iron-alloy core with high percentages of sulfur and oxygen. This discovery provides new insights into Martian formation and geological differences between Earth and Mars, potentially impacting planetary habitability.
Researchers found that metal-poor stars, with fewer heavy elements, emit less intense ultraviolet radiation into space. This allows their planets to form a protective ozone layer, making conditions more life-friendly. The study suggests that as the universe ages, it becomes increasingly unfavourable for complex life on new planets.
Researchers used zircon crystals to unlock information about early Earth's magmas and plate tectonic activity, suggesting that the process was occurring more than 4.2 billion years ago. This finding could be beneficial in the search for life on other planets.
Researchers Paul Byrne and Rebecca Hahn have compiled a global catalog of 85,000 volcanoes on Venus, providing the most comprehensive understanding of the planet's volcanic properties. The dataset includes detailed analyses of volcano distribution, size, and clustering, which will aid in locating future active lava flows.
The study identifies five exoplanets that resemble Venus in terms of radii, masses, and atmospheric conditions. By observing these 'exo-Venus' planets using the James Webb Space Telescope, scientists hope to uncover valuable insights into Earth's future and the possibility of a runaway greenhouse climate.
Scientists have identified clouds made from silicate particles on a distant planet using NASA's James Webb Space Telescope. The team discovered an atmosphere constantly rising and mixing, bringing hotter material up and pushing colder material down.
Scientists from the University of Cambridge have developed a model to predict a planet's interior water capacity based on its size and host star chemistry. The results suggest that larger planets may have drier rocky mantles, while smaller ones could hold more water-rich minerals.
Numerical simulations suggest that Mimas' Herschel impact basin is compatible with a thinning ice shell and geologically young ocean. The results imply that the present-day ocean within Mimas must have been warming and expanding since its formation, potentially making it an emerging ocean world.
A new study reveals that EU consumers are 'exporting' negative environmental impacts to their Eastern European neighbours while keeping economic benefits within the EU. The bulk of environmental pressures and impacts associated with EU consumption are felt in countries outside the bloc, with uneven distribution of costs and benefits wi...
Researchers have successfully replicated the type of gravity that exists on or near stars and planets using a glass sphere measuring 3 cm in diameter. This achievement could help scientists understand and predict how solar weather affects spacecraft and satellite communications systems.
A new study by Brown researchers reveals that changes in tectonic plate thickness impact the location of the Denali Fault, a major strike-slip fault. The findings provide key insights into how geological faults behave as they deepen, shedding light on earthquake hazards.
The MEDA instrument aboard the Perseverance rover has provided high-precision meteorological measurements of Mars' atmosphere, revealing seasonal and daily cycles as well as dynamic phenomena like dust devils. The analysis sheds light on the Martian climate and its potential for supporting life.
A University of Maryland-led team developed a miniaturized analyzer to detect signs of life on other planets. The instrument combines a pulsed ultraviolet laser with Orbitrap analysis to identify chemical structures in planetary samples.
Researchers developed DeepLandforms, an open-source AI tool for mapping planetary surfaces, demonstrating its effectiveness in creating accurate geological maps on Mars. The tool's use of deep learning techniques enables fast and customizable mapping of planets, paving the way for future exploration and discovery.
Scientists at Washington University in St. Louis found that manganese oxides can be formed without atmospheric oxygen under Mars-like conditions. The study, published in Nature Geoscience, used kinetic modeling to show that halogens like chlorate and bromate can convert manganese into minerals thousands of times faster than by oxygen.
Researchers have identified two exoplanets, Kepler-138c and d, as 'water worlds,' with a significant fraction of their volume likely composed of water. The planets are about one and a half times the size of Earth and have much lower densities than our planet.
The largest earthquake on Mars, a 4.7 magnitude marsquake, revealed layers in the crust suggesting a massive meteoroid impact, with possible alternating volcanic and sedimentary rocks. This finding provides evidence for past collision events that shaped the planet.
Researchers propose using Earth's karst caves to simulate extraterrestrial lava tubes, demonstrating feasibility in structure and environmental aspects. Karst caves are comparable in size and provide mild environments, reducing energy consumption in terms of heat control.
University of Central Florida researchers have discovered a method that uses microwaves to melt lunar soil, coupled with beneficiation technology, may be the best option for building safe and economical lunar landing pads. This approach could increase microwave absorption by up to 80% using magnetic fields, making it more energy-effici...
A Martian megatsunami was likely triggered by an asteroid collision similar to the Chicxulub impact that led to mass extinctions on Earth. The crater formed as a result of this impact may have caused a tsunami that reached over 1,500 kilometres from the center, measuring up to 250 meters tall on land.
Wynne's work identifies key questions and answers needed to study Martian caves, which could hold secrets of life and provide insights into Earth's formation. Caves may also serve as radiation shielding for astronaut habitats on the Moon and Mars.
Researchers analyzed data from two meteorite impacts recorded by NASA's InSight spacecraft, revealing a very uniform structure and high density of the Martian crust. The findings provide new insights into the planet's core, mantle, and crust, shedding light on the formation and evolution of Mars.
Scientists have detected seismic surface waves on Mars for the first time, providing new insights into the planet's crust and structure. The study estimates the average properties of the Martian crust between 3 to 18.6 miles below the surface, revealing faster seismic velocities that suggest compositional differences or reduced porosity.
Researchers at Carnegie Mellon University have developed a new approach for conducting automated science in space by balancing risk and scientific value. The approach uses a model that estimates science value and risk, allowing rovers to chart their own course while protecting against high-risk missions.
A Cornell research team synthesized 16 types of rock surfaces that may form on exoplanets, providing a tool to decipher their composition. The study's findings offer clues to early planetary evolution and the chemical makeup of distant planets.
Researchers located four new craters created by impacts on Mars' surface using data from a seismometer and visuals acquired from the Mars Reconnaissance Orbiter. This is the first time that researchers have captured the dynamics of an impact on Mars.
A new study suggests that Earth's habitability could increase if Jupiter's orbit becomes more eccentric, leading to parts of the surface warming up and becoming habitable for multiple life forms. The researchers also found that this change in Jupiter's orbit could have implications for the search for habitable planets around other stars.
A new study reveals that many exoplanets around M-dwarf stars may be composed of half water and half rock, rather than having surface oceans. The discovery suggests that these planets are likely to have water embedded in the rock or in pockets below the surface.
Researchers at Washington State University have created a strong and high-performance material by mixing Martian regolith with a titanium alloy. The composite showed better properties than the metal alone, making it suitable for making tools or rocket parts on Mars.
The Perseverance rover collected igneous cumulate rocks from four sites on the floor of Jezero Crater, providing evidence of aqueous alteration. These rocks will help scientists determine when Mars' climate was conducive to lakes and rivers, addressing major questions about the planet's history.
Researchers found large impacts can fracture a planet's crust, introducing porosity that increases its potential for life. This discovery has implications for early Earth and Mars, suggesting life could have survived in pore spaces during intense impact periods.
A team of scientists used modeling to reveal that Ceres's interior decays radioactive elements, generating heat and powering geological activity. This process is different from the typical hot-cool pattern seen in larger planets, with similarities to Uranus's moons
New paleomagnetic research suggests the solid inner core formed around 550 million years ago and restored Earth's magnetic field. The study provides clues about planetary evolution, habitability, and the potential for life on other planets.
A new method developed by Iris Fernandes increases topography mapping accuracy on the moon, making it possible for safe landing and robotic movement. The method uses shadows in images to extract exact topography details, eliminating previous computational inefficiencies and assumptions.
Scientists from Johns Hopkins APL have compiled the first complete map of hydrogen abundances on the Moon's surface using data collected over two decades ago. The map identifies two types of lunar materials containing enhanced hydrogen and corroborates previous ideas about lunar hydrogen and water.
A recent study published in Nature Communications has uncovered the likely Martian origin of a 4.48-billion-year-old meteorite named Black Beauty. The team found that this ancient fragment may have come from a region on Mars similar to Earth's continents, providing valuable insights into our planet's geological past.
Researchers found the moon's crust was highly porous, about one-third as porous as pumice, due to massive impacts that shattered much of the crust. The team estimated the moon experienced double the number of impacts as seen on its surface, which limits constraints on solar system formation and evolution.
Researchers develop a motorless sailplane concept that harnesses wind energy to explore Mars' atmosphere and geology. The innovative design, inspired by albatross flight, enables the sailplanes to fly for days at a time without relying on solar panels or batteries.
A new study suggests that long-term liquid water can occur on planets with massive primordial atmospheres, which could lead to the emergence of life. The research found that sufficient geothermal heat and radiation from a star are not necessary for conditions to prevail at the surface.
Researchers reveal the likely composition of Charon's dynamic methane atmosphere and propose a possible source for its red polar zone. The team's novel experiments and atmospheric modeling suggest that ultraviolet light breaking down methane molecules is key to understanding the moon's unique albedo.
Asteroid Psyche's varied surface suggests a dynamic history, with metallic eruptions, asteroid-shaking impacts, and a lost rocky mantle. The new maps hint at the asteroid's ancient core, which could be composed of silicate-rich material that has since disappeared.
A new study published in Science Advances suggests that life on Mars is unlikely due to limited water circulation. Researchers used neutron and X-ray tomography to analyze a 1.3 billion-year-old meteorite, finding only small amounts of water reacted with the rock.
Researchers from UC Berkeley found that a photovoltaic array using compressed hydrogen for energy storage can efficiently power human missions on Mars. The system beats out nuclear power across about 50% of the Martian surface.
A new study developed a way to use satellite imaging data to create 3D images that can quickly detect changes on the Earth's surface. The tool could be used to detect significant natural disasters in remote regions, giving first responders accurate information about the needs of the affected region.
Researchers found that around 3.8 billion years ago, a major transition in the geochemistry of zircons occurred, suggesting the onset of plate tectonics. This discovery provides hints about how the planet became habitable and under which conditions the earliest forms of life developed.
Researchers have developed a model to explain how Titan's distinct landscapes form, including dunes, plains, and labyrinth terrains. The study reveals that seasonal liquid transport cycles drive the movement of grains over the moon's surface, creating an Earth-like environment with hydrocarbon sand dunes.
The study suggests that Venus' atmosphere plays a crucial role in determining its rotation speed, with fast winds dragging along the surface and slowing it down. This has significant consequences for the sweltering Venusian climate, with average temperatures of up to 900 degrees Fahrenheit.
Scientists have found a new way dunes can form on Io's surface, which is icy and roiling. The researchers used mathematical equations to simulate the forces on a single grain of basalt or frost and calculate its path.
Researchers propose a modular Mars exploration rover system consisting of four two-wheeled robots that can operate independently or combine in various constellations. The approach enables longer missions and gathers more information about the planet's history and potential habitability.
A team of researchers led by Purdue University's Michael Sori found that smaller Martian ice deposits hold key evidence for the planet's orbit and axial tilt's impact on its climate. The study used NASA's HiRISE camera images to analyze layer shapes in an ice deposit, providing insights into Mars' climate history.
Impact craters reveal insights into planetary bodies' evolution, structure, and composition. By studying impact craters on various planets and asteroids, researchers can determine the formation timeline of these celestial bodies and gain knowledge about their interiors.
The researcher will use a combination of rover, orbital, and analog data to understand the geological record on Mars. The team aims to link the orbital data with images and thermal infrared data from the Curiosity Rover to improve our understanding of past depositional conditions across Mars.
A new color catalog of icy planet surface signatures has been created to aid in the search for life on frozen worlds. The catalog, based on microorganisms found in subarctic conditions, provides a tool for comparing Earth's biological microbes with those on other planets.