Articles tagged with Habitable Planets
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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.
A new study led by University of Maryland researchers found that melted meteorites have extremely low water content, ruling them out as the primary source of Earth's water. The team suggests that unmelted, or chondritic, meteorites may be responsible for delivering water to our planet.
Researchers used AI to map sparse life hidden in salt domes, rocks, and crystals at Salar de Pajonales, a Martian analog. The study found that microbial life is concentrated in patchy biological hotspots linked to water availability, and AI can detect biosignatures up to 87.5% of the time.
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.
The Martian meteorite Tissint has revealed a rich inventory of organic compounds, offering insights into Mars' habitability. The study, published in Science Advances, discovered an unprecedented diversity of organic molecules, including magnesium compounds not previously seen on 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.
Astronomers found that a planet like GJ 1252b, orbiting an M dwarf star, would likely lose its atmosphere due to intense heat and radiation. The discovery narrows the search for habitable planets around these stars, but leaves room for possibilities further away from the star.
A new system classifies atmospheres of distant planets to identify those suitable for future human habitation, without physically visiting them. The research study found that planet TRAPPIST-1e has a significantly more sensitive atmosphere than Earth, which could lead to extreme climate changes.
Researchers propose nitrous oxide as a potential biosignature for exoplanets, detectable by the James Webb Space Telescope. They modeled N2O production on Earth-like planets and found it could be comparable to CO2 or methane in star systems like TRAPPIST-1.
Simulations suggest a 'day at the beach' for life on Earth-like exoplanets around red dwarfs, increasing chances of finding multiple analogs in coming decades. This discovery sheds light on the diversity of water content in terrestrial exoplanets, which is crucial for a temperate climate.
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.
The discovery of LP 890-9b and LP 890-9c, two 'super-Earth' type planets orbiting the small star LP 890-9, was made using ground-based telescopes. The planets have sizes similar to that of Earth and orbits that place them in the habitable zone around their star.
Astronomers at the University of Birmingham have discovered two super-Earth planets, LP 890-9b and LP 890-9c, orbiting the cool star LP 890-9. The second planet, SPECULOOS-2c, is about 40% larger than Earth and has a longer orbital period, placing it in the habitable zone around its star.
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 study published in Nature Geoscience found that clouds likely prevented oceans from being completely covered by ice, allowing life to survive. The research used global climate models and an idealized energy balance model to investigate Cryogenian climatic conditions, revealing the importance of clouds in predicting climate changes.
A new study suggests that younger rocky exoplanets are more likely to support temperate climates due to the decay of radioactive isotopes. This critical heat source is necessary for a planet's mantle convection and surface volcanic degassing, which helps regulate climate.
Tiny zircons found in South Africa hold the oldest evidence of subduction, a key element of plate tectonics, dating back to around 3.8 billion years ago. This discovery provides new insights into when plate tectonics was set in motion and how it may have shaped Earth's surface and climate.
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 new study on Mars' ice deposits provides insight into the planet's past climate, matching layers to Martian orbital dynamics with unprecedented resolution. The findings help scientists understand Mars' climate history and identify potential periods of habitability.
Methane may be the first detectable indication of life beyond Earth, according to a new study that establishes conditions for biological activity. The researchers found that atmospheric methane is more likely to be considered a strong indication of life if it co-exists with carbon dioxide and lacks carbon monoxide.
A team of scientists has created a detailed prediction of an Earth-sized planet in the α Centauri A/B system. The model suggests the planet, dubbed 'α-Cen-Earth', would have a mantle dominated by silicates and be geochemically similar to our Earth.
Researchers propose that cognitive activity operating on a planetary scale is necessary to tackle global issues. A mature technosphere involves integrating technological systems with Earth through feedback loops, making it self-maintaining and exhibiting emergent behavior.
A recent study by a UT graduate student has unraveled the enigma of how tectonic plates break Earth's rock-hard shell. By monitoring seismic images and matching them with rock samples, the researcher found that a small break in the Australian plate grew over millions of years until it unzipped and set in motion a runaway geologic process.
A team of researchers detected a ring of planetary debris surrounding the white dwarf WD1054–226, suggesting a nearby planet may be present in its habitable zone. The study found that the debris is kept in a precise arrangement by a nearby planet's gravitational influence.
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.
A new FQXi report re-assesses the 'fine-tuned universe' hypothesis, proposing that intelligent life could have evolved under drastically different physical conditions. This challenges popular arguments for a multiverse and suggests that the universe may be able to produce life under a wider range of circumstances than previously thought.
Researchers found that only certain types of planets can form large moons in respect to their host planets. They propose that smaller planets are better candidates to host fractionally large moons. This study provides constraints for future observations and sheds light on the formation of Earth's unique moon.
A recent study discovered that a hydrothermal crater lake in Costa Rica's Poás volcano is home to a diverse range of microorganisms, including the single 'extremophile' genus Acidiphilium. These bacteria have adapted to survive in extreme conditions, such as high temperatures and toxic metals, which may be similar to those found on Mars.
A recent study suggests that a chemical compound called magnesium hydrosilicate, stable at high pressures and temperatures, could have stored water deep within the Earth's mantle during its violent early days. This finding has significant implications for understanding the origin of water on Earth and potentially habitable exoplanets.
Researchers used computer simulations to model how dust collides and grows into solid cores for gas giants. This process enables the formation of massive cores necessary for gas accumulation within a few hundred thousand years.
A new study proposes that life could neutralize acidic environment, creating habitable pockets in Venus' clouds. The researchers identified a chemical pathway by which life could produce ammonia, explaining observed anomalies and anomalies.
Scientists suggest that possible lifeforms in Venus' clouds are producing ammonia, which neutralizes sulfuric acid and increases the pH of the clouds. This process makes the environment more tolerable to live in, despite being extremely acidic. The study proposes a biological origin for the ammonia, rather than non-biological sources.
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.
Researchers used TRAPPIST-1's harmonious orbits to determine the impact history of its seven Earth-sized planets. The study found that these planets could have withstood only limited late bombardment, implying a relatively small amount of water arrived on time for potential life.
The University of Sydney's project searches for Earth-like planets around Alpha Centauri to determine if life could survive there. The team is using advanced telescope technology to analyze the stars' atmospheres and detect signs of life.
Researchers provide first direct measurement of overall impact of ocean eddy killing, finding a continuous loss of 50 gigawatts of kinetic energy. This phenomenon, known as 'eddy killing,' counterintuitively reduces the most energetic components of ocean currents.
Researchers from Washington University in St. Louis have discovered a new type of exoplanet known as 'eggshell planets,' which are likely to have little topography and no plate tectonics. These planets may resemble the lowlands on Venus, with vast expanses of lava but little high-standing terrain.
Researchers found fatty acid compounds, GDGTs, and archaeol compounds in salt sediments of Qaidam Basin, a promising analog site for Mars exploration. The distribution of lipids provides important references for understanding Martian habitability.
A new study by MIT scientists uses a novel gene-analyzing technique to estimate that oxygenic photosynthesis first originated around 2.9 billion years ago. This evolutionary innovation allowed for the accumulation of oxygen in the atmosphere and oceans, paving the way for life on 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.
Researchers at the University of Illinois propose a new method to detect moons around planets in double star systems. By analyzing transit timing variations, they can infer the presence of a moon. The study suggests that exomoons may play a key role in keeping planets habitable and could be critical for the evolution of life.
The Dartmouth Engineering team will conduct research on planetary science relating to icy planets' geophysics and astrobiology, aiming to understand the nature of these worlds and their habitability. The project will provide valuable tools for interpreting measurements taken by future missions.
Astronomers have identified a new class of habitable exoplanets dubbed 'Hycean' which are hot and ocean-covered with hydrogen-rich atmospheres, potentially supporting microbial life. These planets offer a wider habitable zone than Earth-like planets, making them promising candidates for finding biosignatures of life.
A new study reveals that planetary shields can buckle under intense stellar winds from dying stars, making it difficult for life to survive. Planets with weak magnetic fields are particularly vulnerable, while those with stronger fields may be able to withstand the effects.
New research from UBC Okanagan campus uses geology to predict planet habitability. By analyzing the amount of iron present, researchers can determine if a planet's crust is thick enough for liquid water and atmosphere.
Researchers identify five double star systems, Kepler-34, -35, -38, -64 and -413, as potential candidates for supporting life. The study shows that these systems have a permanent Habitable Zone, where liquid water could persist on the surface of any Earth-like planets.
Researchers identified a Goldilocks zone for raindrop size to determine which drops make it to the surface. This behavior helps model cloud cycles and predict exoplanet habitability.
A new method for directly imaging planets in the habitable zone of nearby stars has been developed, allowing for the detection of Earth-like planets. This technique uses a coronagraph and mid-infrared technology to improve sensitivity by a factor of 10 compared to existing capabilities.
An international team of astronomers has developed a new system to directly image exoplanets in the habitable zone of nearby stars, potentially harboring life. Using mid-infrared imaging and adaptive optics, they captured images of planets about three times the size of Earth within habitable zones around Alpha Centauri A and B.
A new framework has been developed to understand the interiors of super-Earths, which is crucial for assessing their potential for habitability. The study found that under extreme conditions, bridgmanite has a high melting point, which could impact interior dynamics.
Two University of Arizona research teams will explore the origins and evolution of life in the universe using $12 million NASA grants. Led by Betül Kaçar and Dániel Apai, the teams will investigate essential attributes of life and its relationship with metal elements on ancient Earth and potential habitability on alien planets.
A study by Washington State University scientists has identified two dozen exoplanets that could potentially support complex life. These superhabitable planets are characterized by being older, slightly warmer, and possibly wetter than Earth, with some orbiting stars that may be more suitable for life than our sun.
Astronomers have discovered a lost planet, NGTS-11b, which orbits a star 620 light years away and is located five times closer to its sun than Earth. The discovery brings astronomers closer to finding cooler planets in the habitable 'Goldilocks zone' that can support liquid water.
The newly discovered GJ 887 system hosts multiple super-Earth sized planets, making it an ideal target for the James Webb Space Telescope. The system's proximity and relatively quiet red dwarf star reduce the risk of harmful solar flares, providing a promising opportunity to study exoplanet atmospheres.
The study found that airborne dust can cool down the hotter dayside but also warm the night side, effectively widening the planet's habitable zone. This process is a negative climate feedback, postponing the loss of water and making the planet more habitable.
Astronomers have measured the stellar obliquity of TRAPPIST-1, a very low-mass star, and found it to be low and close to zero. This is the first detection of this effect for an exoplanet system with Earth-like planets, suggesting that planetary orbits may not be misaligned with star rotation.
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.
A new study by University of Arkansas astrophysicist Daniel Whitmire contradicts a previous theory that giant elliptical galaxies are more likely to host technological civilizations. The study suggests that galaxies like the Milky Way, where most stars and planets reside, are more likely to harbor intelligent life.
Astronomers will use transmission spectroscopy and phase curves to observe the atmospheres of seven rocky planets in the TRAPPIST-1 system. The goal is to determine if these planets have atmospheres and what they're made of, which could help find out if life as we know it could survive on these distant worlds.
A 'cold Neptune' and two temperate super-Earths, GJ180d and GJ229Ac, have been discovered orbiting nearby red dwarf stars, offering a chance to study potentially habitable worlds. The planets were found using the radial velocity method and offer insights into exoplanet formation and evolution.