Astronomers have detected a new planet orbiting Proxima Centauri, the closest star to our Solar System, with a mass comparable to that of Earth. The newly discovered planet, named Proxima d, orbits its star at just five days, within the habitable zone.
Researchers have found that Saturn's unique aurorae are generated by swirling winds within its atmosphere, not just from the surrounding magnetosphere. The study uses infrared emission data and ionospheric mapping to identify the fundamental driver behind the observed periodicities.
Researchers at the University of Leicester have discovered a new mechanism driving Saturn's massive aurorae, which are fueled by swirling winds in its upper atmosphere. This discovery answers one of NASA's Cassini mission mysteries and highlights the complex interactions between atmospheric weather and aurora creation.
The study reveals the presence of titanium oxide in the atmosphere of WASP-189b, a hot gas giant planet 322 light years from Earth. The researchers used high-resolution spectroscopy to analyze the exoplanet's atmosphere, finding a layered type of chemistry that suggests three-dimensional effects and winds play a crucial role.
Three newly-discovered gas giant planets have extremely short orbits around subgiant or giant stars, with one planet TOI-2337b destined for consumption in less than 1 million years. The study's findings suggest chaotic planet-to-planet interactions and unpredictable heating rates, offering new insights into planetary system evolution.
The study of XO-3b reveals stronger seasonal variations than Earth's, with temperatures reaching 2,000 degrees C. The planet's oval orbit and high surface temperatures suggest a history of migration toward its parent star.
Researchers have discovered a giant gas planet, TOI-2180 b, with a diameter comparable to Jupiter's and a mass nearly three times that of Earth. The planet is also believed to contain 105 times the mass of elements heavier than helium and hydrogen.
The CHEOPS space telescope has detected the deformation of exoplanet WASP-103b, a rugby ball-shaped world with extreme tides. The planet's Love number indicates similarities with Jupiter's internal structure, suggesting it may be highly inflated due to heating from its star.
Researchers are using a multi-disciplinary approach to study the habitability of exoplanets, with Mars serving as a key example. The team is analyzing the atmospheres of different planets and how they might retain them under various conditions.
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.
Researchers found that iron played a crucial role in the development of complex life forms on Earth due to its essential nutrient properties. The study suggests that the amount of iron in a planet's mantle may indicate its potential for supporting life.
The newly discovered planet is classified as a rocky planet and has similarities to Mercury, with a mass 55% of Earth's. Its high density indicates an iron core, but the surface temperature could reach up to 1500 degrees Celsius due to its proximity to its star.
Researchers have discovered GJ 367b, a sub-Earth exoplanet with a density similar to that of pure iron, which orbits its red dwarf star host in under 24 hours. The planet's size and mass indicate it has lost its outer mantle, suggesting an iron-rich core, similar to Mercury's interior structure.
Astronomers have discovered an ultra-short-period planet GJ 367 b, which orbits its star in just eight hours and has a radius of 72% that of Earth. The planet's mass is 55% of the Earth's, indicating it likely has an iron-rich core, similar to Mercury's interior.
Astronomers have discovered an ultrahot Jupiter, TOI-2109b, with a record-breaking 16-hour orbit. The planet is estimated to be around 5 times the size of Jupiter and has a day side temperature of approximately 3,500 Kelvin.
Simulations show that a migrating planet can produce patterns matching those observed in disks, explaining why planets are rarely found near outer rings. The findings also help to confirm the planet theory for ring formation.
Researchers detected a planet in a 200-day orbit around two stars using TESS data from just one sector over 27 days. The discovery was made possible by observing the planet's transits and eclipses, providing new insights into circumbinary planets.
A new technique developed by University of Hawaii astronomer Nader Haghighipour has successfully detected a transiting circumbinary planet in TESS data. The discovery validates the method, which reduces the time to detect such planets from over a year to just five days.
Researchers use Juno spacecraft data to characterize Jupiter's atmospheric vortices, including the GRS. The studies find that the storm extends deeper into the planet's atmosphere than expected, with possible connections to Jupiter's interior.
Exoplanets HD3167b and two mini-Neptunes orbit in planes perpendicular to each other, with the innermost planet still in the equatorial plane. The discovery suggests an unknown celestial body responsible for this disorder is likely at play.
A team of scientists led by University of Hawaii at Manoa has discovered a newly-formed planet, 2M0437b, which can be directly observed. The planet is estimated to be several times more massive than Jupiter and formed with its star around the time of main Hawaiian Island emergence.
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.
Researchers identified a potential circumtriple planet in the star system GW Ori, with implications for our understanding of planet formation. The discovery, made using ALMA telescope observations, suggests that planet formation may be more active than previously thought.
Clouds have been detected on the distant exoplanet WASP-127b, and their altitude has been measured for the first time. The observations reveal that water vapor is present at lower levels but screened by clouds opaque to visible light, while sodium is found in an unexpected place.
Researchers analyzed deuterium abundance ratios in protoplanetary disks and found significant variations within a single disk, suggesting differences in chemical composition and physical state at formation sites. The study also reveals the presence of complex organic molecules, including nitriles, in planet-forming disks.
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.
Researchers from FSU and Rice University have estimated that the outer core contains between 5.5 and 36.8 × 10^24 grams of carbon, a massive amount considering its size. This refinement provides better constraints on the composition of the Earth's core and sheds light on the planet's carbon inventory.
Researchers measuring the impact of the Montreal Protocol found that banning CFCs preserved plant's ability to absorb CO2, preventing a further acceleration of climate change. The study predicts a 2.5°C rise in global temperatures without the ban, exceeding the 1.5°C limit seen as critical for avoiding climate damage.
A team of scientists assembled observations from NASA's Juno spacecraft, W.M. Keck Observatory, and Japan's Hisaki satellite to discover the source of Jupiter's thermal boost. They found that Jupiter's intense aurora is responsible for heating the entire planet's upper atmosphere, contrary to previous models.
The InSight mission provides clues to Mars' composition, mapping its crust, mantle, and core for the first time. Researchers find a multi-layered crust with an average thickness of 24-72 kilometers and a thick lithosphere beneath.
Scientists from Cornell University have found evidence of explosive volcanic activity on Venus, using phosphine gas as a geological signature. This discovery supports the idea that volcanism is responsible for phosphine's presence in the planet's upper atmosphere.
Researchers have solved a decades-old mystery as to how Jupiter produces spectacular bursts of X-rays every few minutes. The X-rays are triggered by periodic vibrations of Jupiter's magnetic field lines, creating waves of plasma that send charged particles towards the planet's atmosphere.
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 the CHEOPS space telescope have detected a unique exoplanet, Nu2 Lupi d, which is 9 times the size of Earth and has masses between those of Earth and Neptune. The discovery reveals that the planet has a mild stellar radiation environment, making it an ideal target for studying its composition.
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 study reveals features on Venus that suggest limited yet global crustal deformation driven by convection in the planet's interior. The findings support the hypothesis that planetary heat flux and a thinner lithosphere were present during Earth's Archean Eon.
The newly discovered exoplanet, TOI-1231 b, has a substantial atmosphere making it an attractive target for atmospheric studies. Its similarity in size and density to Neptune suggests it may have a large, gaseous atmosphere.
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.
The Hubble Space Telescope has captured the first-ever direct image of a giant exoplanet, PDS 70b, which is feeding off material surrounding its young star. The observations provide a unique look at radiation from extremely hot gas falling onto the planet, allowing scientists to estimate how fast it's gaining mass.
Researchers have pinned down the precise length of a day on Venus, the tilt of its axis and the size of its core. The new measurements reveal an average day on Venus lasts 243.0226 Earth days, roughly two-thirds of an Earth year, with variations in rotation rate due to the planet's heavy atmosphere.
Researchers detected a new chemical signature, hydroxyl radical (OH), on the dayside of WASP-33b, an ultra-hot Jupiter. The discovery provides insight into the chemistry of exoplanet atmospheres and could help search for 'Earth-like' planets.
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.
Astronomers have identified six chemicals in the atmosphere of HD 209458b, a planet that formed far from its star before migrating to its current location. The discovery provides insights into planetary formation and could be used to detect signs of potentially habitable planets.
New research reveals the permanent rise of oxygen in our atmosphere happened 100 million years after initial estimates. The discovery suggests fluctuations in atmospheric oxygen levels played a key role in extreme climate changes and extinction events.
A new study suggests that up to 99% of Mars' initial water was incorporated into minerals and buried in the planet's crust, not lost to space. Researchers used observational data and modeling to resolve long-standing contradictions about Martian water loss rates.
A significant portion of Mars's water is still present on the planet, with estimates suggesting 30-99 percent is trapped within minerals in the crust. This discovery challenges the current theory that the Red Planet's water escaped into space due to low gravity.
A study published in Science Advances has found rare evidence of the Earth's early magma ocean preserved in ancient rocks from southwestern Greenland. The discovery provides a window into the planet's solidification and internal chemistry, suggesting that other rocks may also preserve signs of ancient magma oceans.
Scientists using NASA's Hubble Space Telescope have discovered a distant planet, GJ 1132 b, that may have lost its atmosphere but regained a second one. The team believes the current atmospheric hydrogen is being slowly released through volcanic processes to form a new atmosphere.
Astronomers have discovered a secondary atmosphere on GJ 1132 b, rich in hydrogen and hydrocarbons, which is believed to be replenished by volcanism and tidal heating. The new findings provide insights into the exoplanet's geology and offer a window into its interior.
Researchers have found a curious signal that could be the first known world around Vega. The alien planet would orbit close to Vega and rank as the second hottest world known to science.
Researchers detected Gliese 486 b using both transit and radial velocity data, revealing its mass, radius, and density. The planet's equilibrium temperature of about 700 Kelvin makes it an ideal candidate to study its atmosphere and habitability.
A newly discovered rocky planet, Gliese 486b, has been found to have a 'piping-hot' surface temperature of 430 degrees Celsius, making it inhospitable to human life. However, studying its atmosphere could provide valuable insights into the possibility of habitable planets and signs of life beyond Earth.
Researchers found evidence of tectonic activity on exoplanet LHS 3844b, resulting in extreme temperature contrasts and potential volcanic activity. The planet's surface receives intense radiation, causing blistering heat during the day and freezing temperatures at night.
NASA's Parker Solar Probe captured stunning views of Venus during its close flyby in July 2020. The onboard Wide-field Imager for Parker Solar Probe detected a bright rim around the edge of the planet that may be nightglow.
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 from HKU have discovered evidence of a reduced atmosphere on ancient Mars, dating back 3.5 billion years. The team used infrared remote sensing and spectroscopy to analyze mineralogy and geochemistry of ancient rocks, revealing weathered conditions indicative of a reducing environment.
New research reveals that deforestation in the U.S. does not always cause planetary warming; instead, in some places, it actually cools the planet due to the albedo effect. The study found that forest loss east of the Mississippi River and in Pacific Coast states causes planetary warming.
Research led by NCAR found that COVID-19 lockdowns caused a slight warming effect on the planet, with temperatures rising by 0.2-0.5 degrees Fahrenheit in some regions. The study highlights the complex influence of aerosol emissions on climate, which can either cool or warm the planet depending on the type and amount.
Astronomers at the Center for Astrophysics have detected a cloud-free exoplanet, WASP-62b, which is similar to Jupiter. The discovery was made using spectroscopy and revealed the presence of sodium in the planet's atmosphere. This finding provides valuable insights into the formation and composition of such rare planets.
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.