Researchers at the University of Tokyo have discovered a rare, hot Jupiter with an eccentric orbit that provides a unique opportunity to study this class of planet. The planet, TOI-1355 b, orbits its star in just two Earth days and will soon disappear from view due to its rapidly changing orbit.
SwRI's Strofio, a neutral mass spectrometer, will sample Mercury's sparse exosphere to measure surface particles. This will provide a global understanding of Mercury's surface composition and space environment, answering scientific questions about its origin story.
Researchers using NASA's James Webb Space Telescope and Gemini Observatory study a distant icy object, Centaur 450P/LONEOS, as it awakens and releases gas and dust, behavior more commonly associated with comets. The study provides new insight into how centaurs evolve into active comets as they migrate inward through the solar system.
Researchers studied 72 young Sun-like stars and their protoplanetary disks, finding that different types of winds are more important at different stages in a planetary system's early life. The study shows that gas giants like Jupiter must assemble their massive atmospheres quickly before winds carry that raw material away.
The University of Hong Kong will host the 2028 Magnetospheres of Outer Planets (MOP) Conference, a premier global symposium in space physics. Hundreds of top scientists will convene in Hong Kong to explore international collaboration on major Jupiter exploration missions.
Juno's Microwave Radiometer reveals Io's heat output by looking below the surface, breaking new observational ground for volcanic and icy worlds. The findings suggest a steep gradient of rising temperatures just several feet into Io's surface, with possible explanations including conductive crust heating or cooling lava flows.
Researchers propose a multiple-moon-aided Jovian capture method utilizing solar gravity perturbation (SGP) to reduce velocity increments. The study uses four dynamic models and computes datasets to analyze the mechanism of SGP, revealing its influence on perijove radius change.
The discovery of an exomoon in the CD-35 2722 system, orbiting a brown dwarf rather than a planet, challenges our understanding of planetary objects. The exosatellite is estimated to be at least as massive as Jupiter and orbits a highly massive companion, blurring the lines between stars, planets, and moons.
Astronomers have discovered a third planet, Beta Pictoris d, in the system, which is 100 times fainter than Beta Pictoris b and 2.4 times more massive than Jupiter. The planet's wide orbit and extreme faintness make its detection a significant achievement.
A team of researchers, including Michael Fausnaugh from Texas Tech University, have identified a new planet using the Transiting Exoplanet Survey Satellite (TESS) mission. The planet, Gaia23bra b, is a super Jupiter orbiting far from its host star and offers insight into the detection methods used in astronomy.
A team of astronomers used the James Webb Space Telescope to study the exoplanet WD 1856 b and its unusual orbit around a white dwarf. The research found that the planet is significantly warmer than expected, with a temperature of about 400 Kelvins, indicating it must have been heated in the past.
The TESS mission has discovered a planet orbiting a distant star through microlensing, revealing a world about 1.63 times as massive as Jupiter at an orbital distance similar to Jupiter's. This finding suggests additional microlensing planets may be hidden within archived TESS observations.
Researchers have discovered two rare 'super-puff' planets with densities lower than candy floss, orbiting an F7-type dwarf star. The study provides a unique laboratory for understanding how these planets form and evolve, offering insights into their extremely low densities.
The SwRI-led Lucy mission has found that asteroid Donaldjohanson rotates on two axes, with a wobbling pattern observed every 10.5 and 26.5 Earth days.
Astronomers at Caltech IPAC have settled on a leading hypothesis for the unusual hot spot on CoRoT-2 b, a hot Jupiter that defies previous assumptions about its behavior. The planet's slow rotation speed, which is equivalent to about three Earth days per orbit, suggests it is not tidally locked to its host star.
Phosphorus and nitrogen, two elements necessary for life, were found in distinct ratios in asteroidal bodies related to iron meteorites compared to younger asteroids. Researchers recreated the crystallization of iron meteorites in the lab and analyzed their chemical composition, which suggested that these life-essential elements origin...
Researchers measured wind speeds on seven hot, Jupiter-like exoplanets and found that magnetic fields govern the winds. The team's findings provide the strongest evidence yet of magnetism on planets outside our Solar System.
Researchers found strong magnetic fields on ultra-hot Jupiters, similar to those in our Solar System. The presence of these fields could affect planetary climates and potentially create dramatic aurorae displays.
Researchers at Max Planck Institute for Solar System Research identified the ring-shaped region outside Jupiter's orbit as a 'pluripotent' planetesimal breeding ground. Computer simulations show diverse populations of planetesimals can form over millions of years, establishing a connection to specific groups of meteorites.
Researchers have discovered daily cloud cycles on WASP-94A b, a Hot Jupiter planet, using data from the James Webb Space Telescope. The findings reveal different weather patterns on the morning and evening sides of the planet, with magnesium silicate clouds forming in the mornings and clearing up by nightfall. This breakthrough provide...
Researchers used JWST to observe WASP-94A b and found aerosols dominated by condensation-driven clouds. Clouds form on cooler side, circulate, and evaporate as they move into the hotter day side.
The Juice and Europa Clipper spacecraft captured simultaneous images of both hemispheres of the interstellar comet 3I/ATLAS. The observations revealed hydrogen, oxygen, and carbon emissions, providing insights into the comet's origin and composition.
Researchers studied the unique planet using James Webb Space Telescope data, finding an atmosphere similar to Jupiter's, mostly composed of hydrogen and helium. The exoplanet orbits its star at just six Earth days, moving four times faster than Mercury around our sun.
Scientists have measured the atmosphere of the mini-Neptune, revealing a heavy composition with water vapor, carbon dioxide, and sulfur dioxide. The findings suggest that both planets formed far from their host star, then were drawn inward through a gradual process, preserving their atmospheres.
Jupiter is found to be about 8 km less wide at the equator and 24 km flatter at the poles, requiring an updated understanding of the giant planet's size and shape. This research has broader implications for studying gas planets in general and provides new insights into Jupiter's powerful winds and interior structure.
Researchers found massive amounts of ammonia gas expected but less than anticipated, and instead discovered thick patchy water-ice clouds on the exoplanet. The discovery sheds light on the limits of current models for studying exoplanet atmospheres.
Researchers studied the TOI-201 system, finding that the planets' orbits are tilted relative to each other, causing them to slowly change orientations. The team used multiple observational techniques to confirm the system's existence and predict future transits.
Researchers found that Jupiter's strong magnetic field created a cavity in its circumplanetary disk, which captured the largest four moons, including Ganymede. In contrast, Saturn's weaker magnetic field failed to form a cavity, resulting in only one large moon, Titan. This discovery provides insight into the formation of satellite sys...
The discovery of TOI-5205 b, a Jupiter-sized planet orbiting a four times more massive star than our Sun, reveals its atmosphere has fewer heavy elements than expected. The research suggests that the planet's interior and atmosphere are not mixing, resulting in a carbon-rich, oxygen-poor atmosphere.
The collaboration aims to assess cross-border climate risk across the minerals-energy-food complex using Jupiter's ClimateScore Global platform. The MEF complex framework examines how climate hazards propagate through supply chains, affecting commodity prices and the pace of the energy transition.
Researchers have discovered a second planet, WISPIT 2c, in the same system as the previously detected WISPIT 2b, which is estimated to be about 5 million years-old and has a mass ten times that of Jupiter. The young gas giant was detected using the European Southern Observatory's Very Large Telescope Interferometer.
A team of scientists using the James Webb Space Telescope discovered a cold spot within Io's auroral footprint with temperatures much lower than expected and extraordinarily high densities. This finding opens up new ways to study Jupiter and its moon system, potentially revealing similar phenomena in other planetary systems.
Astronomers have found that the fundamental physical processes generating auroras are common to different celestial bodies, including the largest moon in the solar system. Observations of Ganymede's auroras reveal locally fragmented patches similar to those on Earth and Jupiter, suggesting a universal mechanism for aurora formation.
Researchers using ESA's Cheops satellite find a small rocky planet in LHS 1903 system, which defies conventional understanding of planetary order and formation. The discovery sparks renewed interest in exploring alternative explanations for this unusual system.
Astronomers at UCLA and UCSD have discovered hydrogen sulfide in the atmospheres of four distant gas giant planets orbiting HR 8799, confirming their planetary status. The detection uses a new data analysis technique that will improve the search for life on other planets.
Researchers believe a gigantic ring system surrounding a brown dwarf or super-Jupiter could have blocked the star's light, causing an extremely rare fading star phenomenon. The dimming lasted nearly 200 days, making it one of the longest ever observed.
A team of researchers used spectral data from the James Webb Space Telescope to study the HR 8799 star system, finding clear evidence of sulfur on three gas giant planets. This discovery suggests that these massive planets likely formed through core accretion, contradicting older models.
Researchers propose that dense, nutrient-rich ice can separate from surrounding ice and descend into the ocean, addressing a longstanding habitability problem on Europa. The study suggests a novel idea inspired by crustal delamination, which could be a consistent means of recycling ice and providing nutrients to the ocean.
A new international study finds that Io and Europa's contrasting water makeup was established at birth, contradicting the idea that it evolved over time. The research suggests that Io formed from dry materials and Europa accreted from ice-rich building blocks.
Scientists found that a planet's interior composition, specifically the 'softness' of its vortex base, determines the formation of polar vortices. The study suggests that Saturn may have a harder interior than Jupiter, leading to a single massive polar vortex, while Jupiter's softer interior gives rise to multiple smaller vortices.
Dr. Michael Davis, an astrophysicist at Southwest Research Institute, has been recognized by SPIE as a Fellow for his work on space instruments and UV imaging. He is the optics and detector scientist for NASA's Lunar Reconnaissance Orbiter and Juno mission to Jupiter.
A new study suggests that Europa's seafloor is geologically inactive, with no signs of tectonic motion or warm hydrothermal vents that could support life. The team calculated the gravitational forces from Jupiter and concluded that the tidal heating on Europa is not strong enough to drive significant geologic activity.
The UVS instrument collected data on the comet's composition, including oxygen, hydrogen, and dust-related features. The unique sunward viewpoint provided a downstream view of the comet's tails, allowing researchers to gain insights into its geometries.
The discovery of PSR J2322-2650b, a Jupiter-mass exoplanet orbiting a rapidly spinning neutron star, challenges our understanding of planet formation. The exoplanet's atmosphere is dominated by molecular carbon and exhibits a unique helium-carbon composition.
A team of researchers has discovered a distinct group of hot Jupiters whose circular orbits contradict the expected timescale for tidal migration. These planets exhibit characteristics consistent with disk migration, such as primordial alignment and planet multiplicity, suggesting they formed smoothly within the protoplanetary disk.
A team of astronomers detected with precision two huge tails of gas surrounding the ultra-hot Jupiter WASP-121b using the James Webb Space Telescope. The continuous observation revealed a trailing tail pushed back by radiation and a leading tail pulled towards the star, covering over three times the distance between planet and star.
The Subaru Telescope's OASIS program has discovered a massive planet and a brown dwarf orbiting distant stars. These discoveries enable the upcoming Roman Space Telescope to test critical technologies for imaging Earth-like planets.
Researchers have created the first 3D map of a planet orbiting another star, highlighting distinct temperature zones on WASP-18b. The technique allows for atmospheric variations to be mapped, providing insights into exoplanet temperatures and composition.
A team led by UMD astronomers has created the first three-dimensional temperature map of a planet orbiting another star, revealing distinct temperature zones and water vapor breakdown. The new technique lays the groundwork for future explorations of faraway planets.
Researchers link Jupiter's birth to the formation of chondrites, a family of stony meteorites that preserve clues about the solar system's origins. The study suggests that Jupiter's rapid early growth created gaps and rings that protected the separation between inner and outer solar system material.
A young rogue planet has displayed a record-breaking 'growth spurt', consuming 6 billion tons of gas and dust every second over several months. The observations provide insight into the turbulent infancy of such celestial bodies, revealing a tumultuous growth process similar to that of stars like our Sun.
Astronomers have detected phosphine (PH3) in the atmosphere of low-temperature brown dwarf Wolf 1130C using James Webb Space Telescope. The abundance is comparable to that of Jupiter and Saturn, with a value of 0.100 parts per million.
Astronomers have identified a rogue planet with a mass five to 10 times that of Jupiter, growing at an unprecedented rate of six billion tonnes per second. The discovery provides valuable insights into the formation and growth of rogue planets, suggesting they may share a similar path to star formation.
Astronomers detected phosphine in the atmosphere of a cool, ancient brown dwarf named Wolf 1130C using the James Webb Space Telescope. The discovery challenges previous theories and suggests that phosphorus chemistry might be more complex than initially thought.
Astronomers from Trinity College Dublin used the James Webb Space Telescope to study the weather of a nearby rogue planet, SIMP-0136. They found strong auroral activity similar to Earth's Northern Lights and detected minute changes in temperature, cloud cover, and chemistry.
Researchers have identified undetectable asteroids orbiting Venus that could collide with Earth in the distant future. The asteroids' low eccentricity makes them invisible from ground-based observatories, but simulations suggest they pose a real risk of devastating impacts on large cities.
Researchers at Nagoya University and the Italian National Institute for Astrophysics have determined how molten rock droplets formed in Jupiter's early days. Their study shows that chondrule characteristics are influenced by the water content of impacting planetesimals, providing a clearer picture of solar system formation.
The OSIRIS-REx sample return mission revealed asteroid Bennu's composition, history, and unique materials. Researchers found stardust from other stars and organic material formed in interstellar space, shedding light on the early solar system's formation.
Researchers propose that Jupiter-sized exoplanets may accumulate and collapse into detectable black holes due to dark matter. This process could potentially generate multiple black holes in a single exoplanet's lifetime, making exoplanet surveys a promising method for hunting superheavy dark matter particles.
New research suggests Jupiter's core is actually formed through gradual absorption of heavy and light materials as the planet grew, rather than a massive collision. This dilute core structure blends into the surrounding layers without a sharp boundary.