Researchers have devised a new method to identify habitable planets and potentially inhabited planets by comparing atmospheric CO2 levels, which suggests the presence of liquid water. This signature can be detected with current telescopes, providing a path to identify life on exoplanets.
Researchers uncover six transiting planets around HD110067, a bright star with a chain of resonances spanning five pairs. The precise gravitational dance enabled the team to solve the previously unsolvable puzzle of the system's arrangement, revealing planetary orbits and orbital periods.
Astronomers have discovered a rare six-planet system, HD110067, that exhibits an orbital resonance pattern, repeating every three and four orbits. This unique configuration provides valuable information on how sub-Neptunes form, evolve, and potentially support liquid water on their surfaces.
Researchers created lab-made haze to understand how it affects observations of distant planets, which could lead to misinterpretations of global temperatures and biological activity. The new data offers a better understanding of exoplanet atmospheres, helping scientists focus on specific planets and improve their search for life.
New studies show that giant gas planets in nearby star systems can prevent life on smaller, rocky planet neighbors by kicking them out of orbit and wreaking havoc on their climates. Researchers found that four giant planets in the HD 141399 system are likely to destroy the chances for life on Earth-like planets.
University of Leicester astronomers confirm the existence of an infrared aurora on Uranus, offering clues to its magnetic fields and potential for life. The discovery may also help identify other habitable planets with similar characteristics.
A new study reveals that magma oceans on rocky exoplanets can affect their size, evolutionary path, and mantle structure. The research found that these ocean's compressible nature can make lava-rich planets denser than solid planets of similar size.
Scientists have discovered a simple test for signs of past or present life on other planets, using artificial intelligence to distinguish between biological and abiotic samples with high accuracy. The method has the potential to revolutionize the search for extraterrestrial life and deepen our understanding of Earth's earliest life.
Researchers from University of New Mexico and Massachusetts Institute of Technology have detected two long-period giant planets orbiting an early K dwarf star. The exoplanets, TOI-4600 b and c, have orbital periods of 82.69 days and 482.82 days, respectively, making them the longest-period planets found by TESS to date.
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.
The James Webb Space Telescope has detected water vapor in the inner disk of PDS 70, a star with both an inner and outer disk of gas and dust. This discovery suggests that rocky planets may form with water available to them from the beginning.
Using ALMA, astronomers have found evidence of a cloud of debris that might be the building blocks of a new planet or the remnants of one already formed. This discovery would confirm the existence of Trojan planets outside our Solar System, which are rocky bodies sharing the same orbit as a planet.
A new study by NASA and Japan's Osaka University suggests that rogue planets, drifting through space without a star, may outnumber stars with orbiting worlds. The Roman Space Telescope could discover up to 400 Earth-mass rogue planets, according to the findings.
Scientists have discovered a young exoplanet, MWC 758c, that may be generating the spiral arms in its infant planetary system. The planet's massive size is estimated to be at least twice the mass of Jupiter, yet it was invisible to other telescopes due to its reddish color, which makes it more difficult to detect.
Researchers believe Earth's formation was facilitated by the accumulation of small pebbles, resulting in the presence of water as a byproduct. This new theory increases the likelihood of finding habitable planets outside our Solar System.
Researchers have discovered a large gas giant orbiting two stars using the radial velocities method for the first time. The newly found system, TOI-1338/BEBOP-1, is only the second binary star system known to host multiple planets ever confirmed.
The CHEOPS satellite has successfully detected two elusive exoplanets, TOI 5678 b and HIP 9618 c, using its precise measurements. The planets have sizes similar to Neptune and Earth radii, respectively, with orbital periods of 48 days and 52.5 days.
Astronomers at MIT and University of Wisconsin have discovered two validated planets, K2-416 b and K2-417 b, in Kepler's last week of high-quality data. The third planet candidate, EPIC 246251988 b, orbits its star every 10 days and is slightly farther away from Earth than the other two.
A team of astrophysicists and citizen scientists have identified three potentially habitable exoplanets discovered during NASA's Kepler space telescope's final days of operation. The planets, including K2-416 b and K2-417 b, are between the size of Earth and Neptune and orbit their stars closely.
New analysis reveals that two-thirds of planets around small stars could be sterilized by tidal forces, leaving one-third with potentially habitable zones. Hundreds of millions of promising targets have been identified for future studies.
A new study suggests expanding the search for habitable planets to consider the space between a star and the soot line in planet-forming disks, which could lead to discovering worlds with rich organic carbon and poor water content. This new model proposes that such planets may have more carbon than Earth and potentially harbor life.
Researchers detect two planets, super-Earths and mini-Neptunes, in a synchronized dance around a cool star. The system's unique configuration could help explain the formation mechanism of these mysterious planetary types.
Scientists have discovered the first-ever extrasolar radiation belt, orbiting the brown dwarf LSR J1835+3259. The discovery reveals that this magnetic structure is filled with extremely high-energy electrons and charged particles, sparking new questions about the universality of such phenomena.
Ancient Mayans used an 819-day calendar that covered a much larger timeframe than previously thought. By increasing the calendar length to 20 cycles of 819 days, researchers found a pattern emerges in which the synodic periods of all visible planets align with station points in the larger calendar.
A new study from NASA's Chandra program reveals that exploded stars can pose a significant risk to nearby planets due to intense X-ray radiation, potentially altering atmospheric chemistry and causing mass extinctions.
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.
A UTSA-led research team has discovered a new exoplanet using indirect methods. The exoplanet, HIP 99770 b, is about 14 to 16 times the mass of Jupiter and orbits a nearly twice-as-massive star. This breakthrough opens a new avenue for scientists to discover and characterize exoplanets.
Astronomers using JWST discovered that the atmosphere of exoplanet HD149026b, a 'hot Jupiter,' is super-abundant in carbon and oxygen, far above expectations. This finding provides insight into planet formation and suggests that giant planets may have varied atmospheric compositions.
The James Webb Space Telescope detected the thermal emission of TRAPPIST-1 b, indicating a temperature of about 500 kelvins and no substantial atmosphere. This finding marks an important step in determining habitability around small, active stars like TRAPPIST-1.
Researchers found giant gas giants orbiting low-mass stars, challenging the widely accepted planet formation model. The study used NASA's TESS satellite data and identified 15 potential giant planets, with five confirmed as actual planets.
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.
Astronomers at UC Irvine have found that terminator zones on distant exoplanets could be prime sites for liquid water and potentially harbor life. The study suggests that these regions offer a unique climate stability, making them more promising than previously thought.
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.
A recent experiment by UC Riverside astrophysicist Stephen Kane demonstrates that a terrestrial planet in this location would have disastrous effects on the solar system. The simulation found that such a planet could destabilize Earth's orbit, making it far less habitable and potentially ejecting Mercury and Venus from the solar system.
The study reveals that 'similar' planetary systems are the most common type, followed by 'ordered' and then 'anti-ordered' systems. The researchers found that factors such as gas and dust disk mass and star abundance play a crucial role in determining system architecture.
New research from the University of Georgia reveals that artificial intelligence can be used to find planets outside our solar system. Machine learning can analyze environments where planets are still forming, helping scientists overcome difficulties such as distance and data thickness.
A team from UNIGE has observed a sample of planets at the edge of the Hot Neptune Desert to understand its creation. They found that most of these planets have an orbit misaligned with the stellar equator, indicating disruptive migration processes.
A new theory proposes that rocky planets form in a narrow band of the protoplanetary disk, where silicate vapors condense to form solid pebbles. This process creates a ring of material that constitutes the building blocks for planet formation, resulting in uniform systems of rocky super-Earths.
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.
Two temperate Earth-mass planets orbit GJ 1002, a cool and faint star suitable for atmospheric analysis. The discovery increases the number of known habitable planets to seven near the Sun.
Astronomers discovered that the building blocks of planets like Jupiter and Saturn form while their parent star is still growing. The study analyzed spectroscopic observations from polluted white dwarfs, which revealed signs of asteroid melting, indicating a rapid process of planet formation.
A new model accounts for the interplay of forces acting on newborn planets, explaining two puzzling observations: the radius valley and peas in a pod. The research suggests that giant impacts, like the one that formed our moon, are probably a generic outcome of planet formation.
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.
Astronomers have discovered barium in the upper layers of ultra-hot Jupiters WASP-76 b and WASP-121 b, raising questions about these planets' atmospheres. The detection challenges scientists' understanding of heavy elements' behavior in exoplanet environments.
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.
The Europlanet Prize for Public Engagement 2022 was awarded to Dr. Kosmas Gazeas and the team behind 'Planets In Your Hand', an interactive tactile exhibition that provides a multisensory experience of planetary surfaces. The exhibition has been traveling to schools, universities, and organizations, reaching thousands of visitors.
A study at Europlanet Science Congress 2022 found that super-thin planet nurseries can accelerate the formation of big planets. The team observed a remarkably thin disc of dust and gas around a young star, where large particles settled into a dense midplane, creating conditions favourable for planetary growth.
Astronomers have discovered a small Neptune-like planet in the protoplanetary disk LkCa 15, using high-resolution ALMA observations. The planet is estimated to be around one to three million years old and has accumulated material at the Lagrange points, providing strong evidence for its presence.
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 density measurements separate rocky and water-rich exoplanets around red dwarf stars, suggesting a third population with 50% rock and 50% water composition. This discovery improves our understanding of small planet formation and evolution, paving the way for future searches for signs of life.
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.
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.
Researchers at the University of Sheffield have proposed a novel origin for Jupiter-like planets around massive stars. Massive stars can capture or steal planets from other stars in densely populated stellar nurseries, a process known as a 'planetary heist'.
Researchers found that oxygen makes diamond formation more likely, allowing for a wider range of conditions and planets. This discovery could lead to new methods of fabricating nanodiamonds with various applications.
Astronomers using JWST have detected unambiguous evidence of carbon dioxide in the atmosphere of WASP-39b, a Saturn-mass exoplanet. The discovery provides valuable insights into giant planet composition and heavy element abundance, with implications for understanding how planets form.
Researchers discovered a Neptune-sized planet around a bright blue star, shedding light on the dearth of Hot Neptunes. The planet's proximity to its star makes it susceptible to stripping of its gas, but it may survive for a billion years.
A super-Earth planet, Ross 508 b, has been discovered near the habitable zone of a red dwarf star 37 light-years from Earth. The planet's orbit is elliptical, potentially placing it in the habitable zone for part of its orbit.
A 15-year study details the origins and diversity of every known mineral on Earth, with over 10,500 mineral kinds identified. The research also reveals that 80% of minerals were formed with water, and 40% have multiple formation processes.
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.