Articles tagged with Planetary Bodies
Researchers at Stanford University have discovered a way to interpret the meaning of dune patterns, which can be used to understand environmental changes on planetary bodies such as Mars, Venus, and Titan. The study found that high interaction density between dunes signals recent or local changes in boundary conditions.
A new study has captured the early stages of planetary evolution, observing a young gas planet's violent and erratic atmospheric shedding. The research, led by Dartmouth researchers, provides insights into the most common experiences of planets beyond our solar system.
Research suggests that larger cosmic dust aggregates are less likely to stick together after collisions. This limits the growth of planetary building blocks, complicating the process of planet formation. Simulations reveal that size is a critical factor in determining sticking probability, with larger aggregates more prone to bouncing.
A Southwest Research Institute-led team modeled the early impact history of Venus to explain how it maintains a youthful surface despite lacking plate tectonics. The findings suggest that higher-speed, higher-energy impacts created a superheated core that promoted extended volcanism and resurfaced the planet.
A study by Caltech scientists reveals that Earth primarily consisted of dry, rocky materials during its early stages, with a major addition of life-essential volatiles occurring only in the last 15% of its formation. This finding provides crucial insights into the planet's formation process and has important implications for theories o...
An international group of experts has developed a planetary protection policy to safeguard Earth from potential threats and avoid compromising the search for lifeforms on other celestial bodies. The policy aims to prevent biological and organic contamination of space missions, ensuring the safety of our planet.
Researchers found tiny salt crystals in an asteroid sample, indicating the presence of liquid water. The discovery challenges previous assumptions that ordinary chondrite asteroids lack hydrated minerals.
Researchers suggest a massive young planet is burning up in a superheated soup of raw material swirling around it, causing the star to flare. The simulation reveals a 'disc inferno' process where the planet's atmosphere ignites, feeding the star and making it shine brighter.
A team of scientists led by NYU Abu Dhabi researcher Mohamad Ali-Dib discovered an Earth-sized exoplanet named LP 791-18 d. The planet may be carpeted with volcanoes and sustain water in liquid form, making it potentially habitable.
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.
A team from Heidelberg University discovered a new class of asteroids rich in water, similar to dwarf planet Ceres. The small bodies are thought to have formed in a cold region at the edge of the Solar System before being impacted by gravitational disruptions.
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.
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.
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.
Scientists have discovered new evidence of phosphorus availability in Enceladus's ocean, making it a prime target in the search for extraterrestrial life. The discovery suggests that Enceladus's subsurface ocean is likely habitable due to its high levels of dissolved phosphorus.
A recent study by Dr Joseph Michalski from HKU suggests that the number of ancient Martian lakes may have been significantly overestimated. The analysis of satellite data reveals evidence for smaller lakes on Mars, which could contain critical information about past climates.
Researchers found that developing sea anemones use hydraulic muscles to regulate body pressure and sculpt tissue. The more active larvae are, the longer they take to develop, suggesting a trade-off between movement and growth.
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
Researchers have discovered a new technique for detecting dim bodies, including planets, orbiting Cataclysmic Variables (CVs). The method analyzes changes in brightness caused by perturbations of a third body orbiting the inner two stars. Two out of four studied CV systems show signs of planetary mass objects in orbit around them.
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.
Asteroids like Bennu and Ryugu appear rough due to the loss of fine-grained regolith caused by tiny space dust grains hopping around on their surfaces. This process may help small asteroids migrate faster through space, affecting their orbits.
The Biofinder instrument has successfully detected bio-residue in ancient fish fossils from the Green River formation, confirming that biological residues can survive millions of years. The device's capabilities make it an ideal tool for future NASA missions to detect signs of past life on other planetary bodies.
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.
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.
Scientists have developed a new way to date asteroid collisions, providing a clearer picture of how planets formed. By analyzing the Chelyabinsk meteorite, researchers found evidence of two distinct collision stages, shedding light on the timing and processes involved in planetary formation.
Researchers have discovered a ring of planetary debris orbiting close to a white dwarf star, suggesting the presence of a nearby planet in the habitable zone. The planet is thought to be similar in size to terrestrial planets in our solar system and could support liquid water, making it potentially habitable.
Astronomers have observed the moment that debris from destroyed planets impacts a white dwarf star for the first time, confirming decades of indirect evidence. The event was detected using X-rays and provides direct measurement of accretion of rocky material onto a white dwarf.
Researchers have uncovered the truth behind the missing volatiles in meteorites, revealing a massive shockwave phenomenon that stripped elements from planetary building blocks. This finding has significant implications for our understanding of Earth's geochemical evolution and the Solar System's youth.
A team of scientists simulated over 200,000 hypothetical Earth-like worlds to understand the types of environments astronomers can expect to find on real exoplanets. They found that in 90% of cases with liquid water on the surface, there are no ice sheets, but rather permanent ice belts along the equator.
A study suggests the IAU's current definition of a planet is flawed and rooted in folklore and astrology. Researchers propose a new definition focused on a planet's geological activity, clearing its own orbit to be the largest gravitational force.
A team of scientists measured the masses of two young giant planets in a 20 million-year-old system, finding they reached their final size at an early stage of evolution. This challenges current models, suggesting that giant planets can contract and mature rapidly.
A group of global healthcare and tech companies has pledged to decarbonize the NHS supply chain by 2045, aiming to support the NHS's ambition to become the world's first net zero health service. The International Leadership Group for a Net Zero NHS has urged suppliers to commit to reducing their operations' carbon footprint by 2045.
Researchers have discovered evidence of a giant impact that occurred in a nearby star system, stripping part of the planet's atmosphere. The team observed carbon monoxide gas around the star, which they believe was released from a massive impact involving two proto-planets.
Researchers have successfully sampled Vesta's mantle using meteorites derived from the dwarf planet, resolving the 'missing mantle problem' and providing a record of the earliest era in solar system formation. This breakthrough pushes back our knowledge to just two million years after the beginning of solar system formation.
A study of metal-rich asteroids has found that they have surfaces with 85% metal such as iron and nickel, similar to stony-iron meteorites. The research also identified four possible asteroid families in the main asteroid belt, which may hold clues about their origins.
The study proposes a novel 'hit-and-run-return' scenario, where pre-planetary bodies crash into each other, slow down, and then merge again. This led to the formation of Venus as having had a very different experience in its growth compared to Earth.
A new study from Washington University in St. Louis suggests that Mars' small size limits its habitability due to a lack of retained volatiles. Researchers used potassium isotopes to determine the presence and abundance of volatile elements on Mars, finding a correlation between body size and volatile composition.
The European facility will study samples from asteroids and the Moon at a macroscopic level, unlocking exciting science on the formation and evolution of planetary bodies. The first instruments will be delivered in summer 2022, with the laboratory expected to fully operational by 2023.
Scientists recreated Titan's conditions, studying properties of organic molecules ACN and PCN on the moon's surface. The findings could provide insights into Titan's surface cracking and confirm its mineral composition.
Researchers at the University of Rochester found that lunar samples do not show signs of magnetization from a magnetic shield. The lack of magnetization suggests that the moon has never had a prolonged dynamo field. Without this protection, solar wind implanted volatiles like helium 3 in the lunar soil.
Researchers found that large asteroids from the outer half of the main asteroid belt strike Earth at least 10 times more often than previously calculated
Scientists conducted new experiments on carbon partitioning between metal and silicate using chondritic starting materials. The results suggest that planetary embryos may have had nearly saturated carbon content in their mantles, which could be a natural consequence of core-mantle partitioning during Earth's formation.
A new study by Hebrew University researcher Professor Barak Kol introduces a novel approach to the three-body problem, predicting the probability of each body escaping the system. The theory avoids infinite probabilities and provides strong agreement with computer simulations, indicating a paradigm shift in understanding the system.
Researchers at North Carolina State University conducted a pilot study to model ferrovolcanism, the predicted manifestation of planetary volcanism on metallic worlds. They found that metallic lava flows travel 10 times faster and spread more thinly than rocky flows, creating braided channels with smooth, thin layers.
Researchers found a 4.565 billion-year-old meteorite with an andesite crust, unlike known asteroids, suggesting andesitic crusts may have been common in early protoplanets.
A new study reveals that humans are responsible for a majority of the seasonal surface water storage variability on Earth, accounting for 57% of total changes. Human-managed reservoirs have a significant impact, especially in arid regions where human control surges to 90% and above.
Exposure to chemicals has contributed to over 1.3 million premature deaths worldwide. A global intergovernmental science-policy body is proposed to tackle this issue by conducting scientific assessments and identifying policy-relevant research needs.
Researchers at the University of Rochester used magnetism to determine when carbonaceous chondrite asteroids arrived in the inner solar system. This discovery provides insights into the evolution of the solar system and the origin of Earth's habitability. The study also offers data for the discovery of new exoplanets.
Researchers at Brown University developed a new remote sensing method for studying olivine, a key mineral in planetary bodies. The technique can predict magnesium and iron content with high accuracy, offering insights into the early evolution of the Moon and Mars.
Researchers propose that volatile outgassing led to the flattening shape of Arrokoth, a small Kuiper Belt object. The study suggests sublimation mass loss could be a ubiquitous process shaping KBOs' structures.
The Spitzer Space Telescope made significant discoveries in the solar system during its 16-year mission, providing a never-before-possible look at the universe. New papers catalog these findings and offer guidance for future scientists studying exoplanets and planet formation.
Researchers investigate how Arrokoth's pancake-flat shape emerged from the formation process of the Solar System. They suggest that the body may have started as a merger between a spherical and an oblate body, or that its shape developed gradually due to favorable orbital conditions.
Researchers discover two types of boulders on Ryugu, hinting at a collision between a small S-type and C-type parent asteroid. The findings provide clues to the asteroid's turbulent past and may shed light on Earth's history.
Researchers uncover new details about the oldest planetary objects in our Solar System, which formed iron-rich meteorites. The distinct chemical signatures of these meteorites can be explained by core crystallization in their parent bodies, deepening our understanding of the geochemistry occurring in the Solar System's youth.
A team of scientists at MIT and elsewhere has determined that a family of oddball meteorites likely came from an early planetesimal with a magnetic core. The discovery suggests that the diversity of the earliest objects in the solar system may have been more complex than previously thought.
Researchers suggest that radioactive elements uniquely distributed after the Moon-forming collision led to the near and far sides' differences. The unique composition of KREEP rocks, linked to radioactively unstable elements, provides a key explanation for the Moon's asymmetry.
Researchers challenge long-held idea that magma chambers are composed mostly of crystals. A new study reveals large basaltic magma chambers may be entirely liquid-dominated.
Researchers analyzed 70 years of records on North American deer mouse population trends, finding a general decrease in mass over time, despite expected links to climate and urbanization. Urban areas showed shorter mice with similar body mass, hinting at complex relationships between environmental factors and mammalian adaptation.
Astronomers previously believed Fomalhaut b to be a planet, but Hubble observations reveal it may have been a cloud of dust particles from a titanic collision. The object's unusual brightness and trajectory are explained by a massive dust cloud experiencing radiative forces from the central star.