The MuSCAT2 instrument will use multi-color transit observations to separate actual exoplanets from eclipsing binary stars. This technique is essential for confirming a large number of new transiting exoplanet candidates, including Earth-like habitable planets orbiting stars near the Sun.
Astronomers use Hubble to detect a second 'very warm' Neptune losing its atmosphere at an unprecedented rate, shedding light on the mysterious hot-Neptune deficit. The planet's evaporation may be linked to its star's intense radiation and age.
Researchers using NASA's Hubble Space Telescope have discovered a medium-sized exoplanet, GJ 3470b, losing mass at a rate 100 times faster than similar planets. The study advances knowledge of planetary evolution and suggests that half of the planet may be gone in a few billion years.
Researchers discovered two warm Neptunes at the edge of the 'hot Neptune desert' losing their atmospheres at a rapid pace. This supports the idea that hot Neptunes transform into super-Earths, which are more numerous than previously thought. The study used NASA's Hubble Space Telescope to observe the evaporation of these planets.
A team of UNLV and international astronomers has conducted the first large-sample survey of protoplanetary disks using ALMA, yielding high-resolution images of 20 nearby disks. The results reveal a large population of young planets at wide-orbit similar to Neptune or Jupiter, which may be similar to our solar system
Researchers have discovered that large planets form quickly and in the outer reaches of their solar systems, which could explain the formation of rocky Earth-size worlds. High-resolution images of 20 nearby protoplanetary disks show common substructures, including concentric gaps and narrow rings.
A recent study found that 40% of protoplanetary disks surrounding young stars in the Taurus region have ring structures suggesting nascent planets. These findings coincide with exoplanet statistics, supporting the idea that super-Earths and Neptunes are the most common type of planets.
Researchers from UNIGE have detected helium in the atmosphere of an exoplanet, HAT-P-11b, which is swollen like a balloon due to stellar radiation. The discovery was made using the Carmenes spectrograph on a 4-metre telescope, and supported by numerical simulations that track the trajectory of helium atoms.
An international team of astronomers has confirmed over 100 exoplanets using a combination of space-based and ground-based telescopes. The discovery includes ultra-short orbital period planets and low-mass rocky exoplanets, offering insights into their formation processes.
Researchers have created updated climate models for the seven planets around TRAPPIST-1, revealing unexpected similarities and differences with our solar system. The study suggests that some planets may have evolved like Venus due to an extremely hot early stellar phase, while others could be habitable ocean worlds.
Researchers used a rotating water-filled device to simulate the magnetorotational instability, which helps explain how matter falls inward to form planets in a reasonable time. The experiment confirmed the strong impact of magnetic forces on metal behavior, paving the way for a clearer understanding of accretion disk dynamics.
Researchers at Yale and the Flatiron Institute found that compact, multiple-planet systems are more likely to form around stars with lower amounts of heavy elements. This discovery suggests new insights into the formation of smaller planets and their potential for supporting life.
A young star with a protoplanetary disc has been discovered to have four Jupiter and Saturn-sized planets in orbit around it. The system's extreme range of orbits raises questions about how such a system might have formed.
Chris Fox, a space buff since childhood, and his team discovered exoplanet Kepler 159d by analyzing the orbits of nearby planets. The exoplanet has a mass similar to Saturn's and likely consists of gases with no solid surface.
Astrophysicists estimate that Centaurs will have close encounters and impacts with terrestrial planets, potentially producing catastrophic events. The researchers found that half of the Centaurs can enter the terrestrial planet region, and about 7% can interact with them.
A team of UCSB students, led by Philip Lubin, are searching for signs of alien life in Andromeda using a suite of telescopes and photonic technology. They aim to detect potential signals from civilizations using optical beams that could be visible across the universe.
A cross-disciplinary team led by Rice University will investigate the formation of life-essential elements in rocky planets during their early evolution. The CLEVER Planets project aims to understand how these elements survive turbulent periods and ultimately lead to habitability, with a focus on rocky worlds beyond our solar system.
A new study published in Icarus challenges the International Astronomical Union's 2006 definition of a planet, which requires a celestial body to clear its orbit. Researchers argue that this standard is not supported by scientific literature and propose a new classification method based on size and gravitational dominance.
A new study challenges the idea that life requires an 'Earth clone' by finding that water worlds could be habitable for a significant percentage of simulated planets. Researchers used over 1,000 simulations to find that 10% of planets stay stable for more than a billion years without geochemical cycling.
Scientists have found that many exoplanets, especially those between two to four times the size of Earth, are likely to be water-rich. This suggests that water worlds may be common, with implications for the search for life in our Galaxy.
Researchers measured compositions of 18 planetary systems up to 456 light years away, finding similar proportions of elements to those on Earth. The study suggests that Earth-like planets may exist elsewhere in the galaxy.
Research team proposes that ultrahot Jupiters have normal compositions, with atmospheres resembling stars due to high temperatures and radiation. Water molecules are torn apart on the dayside, but may recombine into clouds in the nightside hemispheres.
A team of astronomers has unveiled 44 extrasolar planets, dwarfing typical confirmation numbers. Novel techniques validated the find, enabling precise determination of planet sizes and temperatures.
Astronomers have detected a strong magnetic field in a planetary-mass object beyond our Solar System, similar to Jupiter's but over 200 times stronger. The object is believed to be a free-floating planet, only 12.7 times more massive than Jupiter, and has a surface temperature of about 825 degrees Celsius.
Researchers found a group of planets outside our solar system where chemical conditions similar to Earth's exist. These planets are in the habitable range and receive sufficient ultraviolet light from their host stars to kick-start life. The study identifies potential candidates, including Kepler 452b, that could support life development.
A computer model of a planet's lifecycle reveals stagnant lid planets can sustain liquid water and potentially life for billions of years. The presence and amount of heat-producing elements are key indicators of habitability, according to Penn State researchers.
TESS starts its search for planets, monitoring the nearest and brightest stars for periodic dips in their light, which suggest a planet may be passing in front of its star. The mission aims to discover thousands of exoplanets, some potentially supporting life.
Scientists have found a new exoplanet, 2MASS 0249 c, that is nearly identical to the well-studied gas-giant planet beta Pictoris b. The two planets share similar mass, brightness, and spectrum but differ in their formation environments, with one orbiting a bright star and the other a pair of faint brown dwarfs.
Researchers have developed a new IR instrument to search for potentially habitable planets around small red dwarf stars. The instrument, IRD, uses advanced technology to measure the line-of-sight movement of stars and detect planets with high accuracy.
Scientists estimate that planets around almost every star in the galaxy may harbor life, prompting new research to identify biosignatures. Researchers propose solutions to detect gases and light signatures produced by life on exoplanets.
The UCR team's guidebook outlines three types of biosignatures that astrobiologists have proposed as markers for life on other planets. The review articles provide a comprehensive framework for scientists searching for signs of life, called biosignatures, in the data they collect from future telescope observations.
An international team of astronomers detected molecules on an exoplanet, allowing it to be visualized. The technique reveals the planet's surface composition and temperature, providing new insights into planetary atmospheres. Future spectrographs will enhance this method, enabling more accurate characterization of planets.
Two independent teams of astronomers identified three young planets in orbit around an infant star, using a new technique that analyzed anomalies in gas flow. The planets are similar in mass to Jupiter and are thought to be among the youngest in our galaxy.
A team of astronomers has developed a new technique to find young extrasolar planets by analyzing the motion of gas in protoplanetary disks. The method successfully confirmed the existence of two Jupiter-mass planets around star HD 163296, providing insight into planet formation and the process that shaped our own solar system.
Using ALMA, two teams of astronomers have confirmed the presence of three infant planets around a young star, HD 163296. The planets are located at distances of approximately 12 billion and 21 billion kilometers from the star, and were identified using a novel technique that analyzes gas flow patterns within a protoplanetary disc.
A new technomarker, the Clarke exobelt, could be used to detect intelligent civilizations. The optimal conditions for observing these artificial belts are found for planets in orbit around red dwarf stars.
Two new planetary systems have been discovered, one featuring three Earth-sized planets orbiting a red dwarf star. These planets are thought to be rocky worlds with temperatures tens of degrees higher than Earth due to their close proximity to the star.
A Rutgers-led ENIGMA team will investigate the evolution of protein nanomachines, which may have arisen before life began, using a $6 million NASA grant. The team aims to understand the earliest processes that support life, including the movement of electrons and hydrogen atoms.
A Brazilian scientist and her co-author found that an extrasolar asteroid has stably occupied a stable path corresponding to Jupiter's orbit for at least 4.5 billion years. The asteroid is believed to have originated from outside the Solar System, likely captured by Jupiter's powerful gravitational field.
A University of Oklahoma astrophysics team discovered that the growth of Mars was halted by an orbital instability among the outer solar system's giant planets. The study used computer simulations to show how this instability, linked to the Nice Model, prevented Mars from becoming a larger, habitable planet like Earth.
A team of UCSB physicists has created a device named DARKNESS, the first 10,000-pixel integral field spectrograph designed to overcome the limitations of traditional semiconductor detectors. This instrument enables direct imaging of planets around nearby stars and can detect fainter planets with higher contrast ratios.
Planets in short-period binary star systems are at risk of being ejected due to tidal forces, which slow down stellar rotations and expand orbital periods. This process removes at least one planet in 87% of multiplanet circumbinary systems, making them less suitable for habitability studies
The Transiting Exoplanet Survey Satellite (TESS) will survey nearly the entire sky for signs of passing planets. The spacecraft aims to detect thousands of stars hosting transiting planets and measure the masses of at least 50 small planets less than four times that of Earth.
A team at Plymouth University used artificial neural networks to classify five planets as potentially habitable, estimating a probability of life in each case. The technique may aid in selecting targets for future space missions with improved spectral detail.
Astronomers found intense X-ray radiation from red dwarf stars can strip away a planet's ozone layer, making it uninhabitable. This means that life on land might only survive in the oceans.
The TRAPPIST-1 planets are curiously light, suggesting the presence of water instead of atmospheric gases. The team found that the inner planets have less than 15% water by mass, while the outer planets have more than 50%.
The James Webb Space Telescope will study the chemical complexity of molecular clouds to understand the origin and evolution of water and other key molecules. By observing icy layers, protoplanetary disks, and individual stars, scientists aim to determine whether life-building blocks exist in every star system.
Astronomers have discovered a trio of super-Earths around the star GJ 9827, with two of them having radii between 1.7 times and 2.5 times that of Earth, sparking debate about their composition. The study's findings provide insight into how these planets form and evolve, with implications for the search for life beyond our Solar System.
The study rules out a cloud-free hydrogen-rich atmosphere for three planets, but leaves open the possibility for planet TRAPPIST-1g. The observations provide key insights into the potential habitability of these planets, paving the way for future studies with the James Webb Space Telescope.
Researchers have shed new light on the TRAPPIST-1 planetary system, revealing that all seven planets are mostly made of rock and contain up to 5% water. The study also found that five planets lack a hydrogen-dominated atmosphere, similar to Neptune or Uranus.
Researchers detected objects in extragalactic galaxies with masses ranging from the Moon to Jupiter using microlensing. The discovery marks the first time planets have been found outside the Milky Way galaxy.
Scientists have made significant progress in developing an ultra-stable telescope capable of detecting Earth-like planets and analyzing their atmospheres for signs of life. The team has successfully measured subatomic- or picometer-sized distortions across a five-foot segmented mirror, paving the way for future missions.
Astronomers discovered a 'hot Jupiter' with westward winds, defying theory. The planet's atmosphere may interact with its magnetic field or be affected by clouds, raising new questions about the phenomenon.
A recent study published in The Astronomical Journal found that exoplanets orbiting the same star are often similar in size and have regular orbital spacing. This pattern could suggest that most planetary systems have a different formation history than our solar system.
A team of astronomers discovered massive clouds of gas and dust orbiting the star RZ Piscium, which could have formed from destroyed planets. The star's unusual dimming episodes suggest it is a young Sun-like star with a debris disk.
Astronomer Catherine Pilachowski discovers star RZ Piscium is slowly consuming its planetary offspring, shedding light on a brief but volatile period in solar system history. The study provides insight into the evolution of planetary systems and why some young solar systems survive while others don't.
Researchers found small, Earth-like planets in Alpha Centauri that may have been overlooked and eliminated the possibility of large Jupiter-sized planets. The study uses advanced spectrographic instruments to narrow the search for habitable planets in our closest neighboring system.
Scientists from NASA and universities are investigating exoplanets to determine their habitability, focusing on astrophysics, Earth science, heliophysics, and planetary science. Researchers use tools like DSCOVR's high-resolution images to simulate habitable planets and study the interaction between stars and planets.
Scientists discovered a rare form of nitrogen gas in Earth's atmosphere, which is more abundant than expected. The discovery provides clues about the composition of life-supporting planets and their atmospheres.
A study using the W. M. Keck Observatory measured the spin rates of three planetary-mass companions, finding rates similar to those of small free-floating brown dwarfs, suggesting two possibilities: the companions could be brown dwarfs or planets that formed with similar spins