Researchers propose that giant hailstones called mushballs carry ammonia deep into the atmospheres of ice giants Uranus and Neptune, hiding it from detection. This process could explain the unexpected lack of ammonia in their atmospheres compared to other planets.
Astronomers have mapped out the chemicals inside planetary nurseries with unprecedented detail, revealing dozens of molecules within five protoplanetary disks. The locations of these molecules vary dramatically across each disk, resulting in diverse chemical environments that may impact planetary formation and potential for life.
A study using ALMA revealed that protoplanetary disks around five young stars are factories of organic molecules, including nitriles implicated in the origins of life. The discovery provides insights into planetary system formation and whether these systems have what it takes to host life.
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.
Researchers from Osaka University and NASA discovered that cold planets exist throughout the Milky Way, even in the Galactic bulge, a region previously thought to be inhospitable to planet formation. The study used gravitational microlensing to determine the distribution of planets across the galaxy.
An international team has identified five objects that could help distinguish brown dwarfs from low-mass stars. The companions, characterized by periods of 5-27 days and radii between Jupiter's, provide valuable information about their composition and formation.
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.
Astronomers have captured the first-ever spin measurements of HR 8799, revealing minimum rotation speeds of 10.1 km/s and 15 km/s for planets d and e, respectively. The findings provide new insights into planet formation and magnetic braking, hinting at a possible trend where lower mass planets spin faster.
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.
The newly launched NEID spectrometer will measure the minute gravitational tug of planets on their host stars, enabling the detection of rocky planets and characterization of exoplanetary atmospheres. By utilizing this technology, scientists aim to push the boundaries for searching smaller exoplanets and probing beyond past challenges.
Researchers found that planets with moderate tilts can increase oxygen production in oceans, favoring the emergence of complex life. This discovery helps refine the search for advanced life on exoplanets.
Scientists found that Mercury's large iron core is linked to the early sun's strong magnetic field, which pulled metal grains inward. This discovery sheds light on the formation of rocky planets' cores and their elemental distribution.
The Kepler Space Telescope has discovered four new planets that are consistent with Earth-sized masses and may be free-floating in space. These findings suggest the existence of a population of free-floating planets, which could have been ejected from host stars by gravitational forces.
Researchers have determined that a massive star, rather than the young sun, was responsible for the split in oxygen isotopes found in the sun and other planets. The study, led by Lionel Vacher, used an unusual meteorite named Acfer 094 to gain insight into the solar system's past.
A new study from the University of Maryland disputes the prevailing hypothesis on Mercury's big core, instead attributing it to solar magnetism. The model shows that a planet's core density and proportion of iron are correlated with the strength of the sun's magnetic field during planetary formation.
The discovery of exoplanet Nu2 Lupi d reveals a rare planet with no known equivalent, with a mass 8.8 times that of Earth and a radius 2.5 times larger than our own. The planet's mild stellar radiation and long orbital period make it an attractive target for future study.
The CHEOPS satellite unexpectedly detected a third planet passing in front of its star, revealing details about a strange planet without a known equivalent. The exoplanet, Nu2 Lupi d, has a radius 2.5 times that of Earth and orbits its star with an orbital period of over 107 days.
Astronomers using Gemini Observatory and WIYN 3.5-meter Telescope found 73 binary star systems among TESS exoplanet hosts, which could be hiding Earth-sized planets. The team discovered that small planets are harder to detect in binary systems due to glare from the companion star.
A new analysis of exoplanets reveals that Earth-like conditions for oxygen-based photosynthesis are much rarer than thought. Only a handful of potentially habitable planets have the necessary energy for complex biospheres to develop, with Kepler-442b being one exception.
A study led by the University of Warwick predicts that four massive planets in a perfect rhythm will be destabilized and turned into a chaotic system when their sun becomes a white dwarf. The planets' movements will become highly uncertain, with even small changes having a significant impact on the outcome.
Researchers have calculated that exomoons orbiting free-floating planets could harbor sufficient water to make life possible and sustain it. The study found that the presence of cosmic radiation and tidal forces could keep water in a liquid state, making these systems promising for the detection of life beyond Earth.
New experiments show that water selectively leaches magnesium from typical rock minerals under extreme pressure and temperature conditions. This process could produce chemical gradients in the early history of water-rich sub-Neptune exo-planets, potentially preserving tracks of initial interactions between water and rocky material.
Researchers investigating the 'radius gap' in exoplanet sizes found that younger mini-Neptunes shrink drastically over billions of years, leaving behind solid cores and becoming super-Earths. As planets age, their gas is stripped away, shifting the radius gap between rocky super-Earths and larger, gas-shrouded planets.
Rice University scientists attribute Earth's nitrogen to rapid growth of moon- to Mars-sized bodies. The study shows that the competition between accretion and differentiation determines the retention of volatile elements like nitrogen.
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.
A new telescope may be able to spot biosignatures on other planets in just three days, with six gas dwarf planets potentially harboring life. Researchers have calculated that the James Webb Space Telescope could detect ammonia around these planets after a few orbits.
Researchers at UC Santa Cruz heated meteorite samples in a high-temperature furnace and analyzed the gases released. The study suggests that the initial atmospheres of terrestrial planets may differ significantly from current theoretical models.
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.
A new study highlights scenarios where a rocky planet around a sun-like star could have oxygen in its atmosphere without life. Astronomers say next-generation telescopes need to characterize planetary environments and detect multiple lines of evidence to distinguish false positives from signs of life.
An international team of scientists has discovered the spectral signatures of almost 1000 atmospheric molecules that could be related to phosphine production. The study provides a novel approach to follow up potential biosignatures and will aid in the detection of life on exoplanets as more powerful telescopes come online.
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.
Researchers at University of Chicago and Stanford University propose mechanism for formation and retention of water-dominated atmospheres on hot, rocky exoplanets. The model suggests these planets could have a water-rich atmosphere for long stretches, with some potentially keeping it for billions of years.
The Antikythera Mechanism, a 2,000-year-old device used to predict astronomical events, has a newly recreated gearing system that conforms to physical evidence and matches descriptions on the Mechanism. The team recovered cycles for all planets using an ancient Greek mathematical method.
Researchers found that weathering rates and atmospheric composition are crucial for a planet's habitability. Geochemistry plays a key role in determining the balance between radiation and liquid water, with extreme temperatures potentially altering this balance.
Scientists have discovered a super-Earth called Gliese 486b orbiting a nearby red dwarf star. The planet's composition is similar to that of Venus or Earth, with metallic nuclei inside it. Its atmosphere may be thin and hot, making it an ideal candidate for studying planetary atmospheres.
Researchers from the GLOBE Institute at University of Copenhagen found that water may be present during planet formation, applicable to Earth, Venus, and Mars. The study suggests that planets with similar building blocks and temperature conditions as Earth may have oceans and continents.
Researchers have discovered a potential Earth-like planet in the Alpha Centauri star system using unprecedented sensitivity data collection methods. The team's findings suggest that this exoplanet may be located in a habitable zone where liquid water could form.
CRIRES+ is a high-resolution infrared spectrograph designed to study planets outside our solar system. It detects super-Earths, planets in the habitable zone around their star, and analyzes their atmospheres during transits.
A team of scientists has discovered a planetary system with a backward-rotating star, K2-290, which exhibits stellar-planetary misalignment. The star's rotation is opposite to the planets' orbits, with a tilt of approximately 124° relative to their orbits.
Astronomers have discovered three hot worlds larger than Earth in the Pisces-Eridanus stream, a collection of young stars. The planets, TOI 451 b, c, and d, are expected to retain much of their atmospheres despite intense heat from their nearby star.
Scientists have developed a new modelling technique to simulate the effects of both gravity and magnetism on planetary formation. The study suggests that magnetic fields can make it difficult for growing planets to accumulate mass beyond a certain point, resulting in a higher frequency of intermediate-mass planets.
University of Warwick astronomers detect lithium and potassium in the atmospheres of four nearby white dwarf stars, revealing remnants of rocky planet crusts. The chemical composition of these crusts is similar to Earth's continental crust, providing a glimpse of the planets that may have orbited these dying stars billions of years ago.
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.
Researchers use the Z machine to apply extreme gravitational pressures on super-Earths, determining which might support life. A data-supported table reveals when a planet's interior would be solid, liquid or gaseous under various pressures and temperatures.
The Roman mission will use microlensing to detect exoplanets in the Milky Way galaxy, uncovering thousands of worlds similar to those in our solar system. The survey will also reveal extreme planets and planet-like bodies, including hot Jupiters and brown dwarfs, thanks to their gravitational tug on stars.
A new study measured the densities of seven exoplanets in the TRAPPIST-1 system with extreme precision, finding remarkably similar compositions among all planets. The researchers propose three hypotheses to explain this similarity, including lower iron content, oxygen-enriched compositions, and water enrichment.
A team of researchers discovered that the early Solar System formed in two distinct steps, resulting in different planetary compositions and evolutionary paths. The study explains why the inner planets are small and dry, while the outer planets are larger and wet.
Researchers found that WASP-107b's massive gas envelope could form easily with a less massive core than previously thought, contradicting classical models of gas-giant planet formation. The discovery has significant implications for our understanding of exoplanet formation and the variety of planets in the universe.
Astronomers have confirmed an exoplanet, HD 106906 b, with a highly eccentric orbit around its binary star, similar to the hypothetical Planet Nine. The planet's orbit is likely bound, and its presence suggests that distant planets can form within the first tens of millions of years of a star's life.
The UCR-led team is studying Earth's diverse chapters of history to find templates for examining exoplanets. By analyzing ancient rock samples and modern sediments, the team will design telescopes and refine models to detect biosignature gases in distant exoplanet atmospheres.
Researchers found that massive planets can wipe out spiral structures in young protoplanetary discs. This suggests that planets may form rapidly and early in the disc's lifecycle, requiring scientists to reassess formation times.
Researchers propose that water emerges during planet formation, contradicting previous 'accidental' asteroid collision theory. The study found water on Mars for the first 90 million years of existence, suggesting it was a bioproduct of the planet's formation process.
Astronomers detect tiny free-floating planet with timescale of just 42 minutes, shedding light on turbulent past of young planetary systems. The discovery demonstrates that low-mass free-floating planets can be detected and characterized using ground-based telescopes.
A team of scientists, led by Matt Clement, used simulations to study the formation of Jupiter and Saturn. The findings suggest that these two planets were originally closer together than previously thought, with a ratio of two Jupiter orbits to one Saturnian orbit being more consistent with the current configuration.
Researchers propose new method to verify star and planet formation theory by simulating the Princeton Magnetorotational Instability (MRI) Experiment. The study finds that instabilities can be seen before the upper limit of experimental rotation rate is reached, shedding light on the growth of celestial bodies.
Astronomers have found compelling evidence that planets start to form while infant stars are still growing. The ALMA radio observatory has captured a high-resolution image of the proto-star IRS 63 with multiple gaps and rings of dust, indicating that seeds of planets are forming in these cosmic cradles.
Astronomers have identified 1,004 main-sequence stars that might contain Earth-like planets in their habitable zones, all within 300 light-years of Earth. These exoplanets could detect signs of a biosphere in Earth's atmosphere.
Researchers at the University of Sydney have developed a new 'photonic wavefront sensor' using AI and machine learning to correct atmospheric distortion, allowing for direct imaging of exoplanets from Earth. This innovation could revolutionize the study of exoplanets and their potential for life.