Articles tagged with Dwarf Planets
Astronomers have discovered that dwarf planet Makemake lacks a significant atmosphere, revealing new insights into its composition. The study used observations of Makemake passing in front of a star to determine its size, density, and albedo, with findings comparable to dirty snow.
Scientists found that carbon-rich asteroids have been splattering dark material on Vesta's surface over billions of years, creating a youthful appearance. The protoplanet's bright outer layer remains pristine, with tiny metallic particles absent, indicating minimal weathering.
Scientists discover unique space weathering process on asteroid Vesta, distinct from other asteroids like the Moon, where meteorite impacts mix soils mechanically rather than forming nanoparticles.
Researchers found that asteroid Vesta's extensive system of troughs is likely the result of faults formed by a large collision. The troughs' unique characteristics, such as flat floors and distinct walls, suggest a fault moving apart, rather than simple cracking on the surface.
The US Department of Homeland Security has created a surrogate semi-submersible called PLUTO to test detection systems for maritime security. The vessel is designed to mimic the features of illegal narco subs used by South American drug cartels, allowing operators to test and improve their sensors in real-world conditions.
The discovery of the new moon provides additional clues for unraveling how the Pluto system formed and evolved. The team is using Hubble's powerful vision to scour the Pluto system to uncover potential hazards to NASA's New Horizons spacecraft.
New findings from NASA's Dawn spacecraft provide the first geological overview of asteroid (4)Vesta, confirming two giant impact basins in its southern hemisphere. The surface is complex and varied, with abundant impact craters and preserved ejecta blankets, but no evidence of volcanic features.
Vesta's surface boasts a diverse array of terrain, including large impact craters and steep slopes. The planet's composition suggests it once had a molten interior, with an iron core at its center.
A team of researchers discovered that a giant impact crater on Asteroid Vesta was formed in a recent collision. The analysis of high-resolution images from the Dawn spacecraft suggests that the impact occurred only about 1 billion years ago, which is unexpectedly young considering Vesta's formation age.
The average global temperatures and illumination models suggest that roughly half of Vesta's surface is cold and dark enough for water ice to survive. The polar regions are thought to be favorable for water ice existence, but may be buried beneath a layer of dry regolith.
A recent study using the TRAPPIST telescope has accurately measured the shape and size of dwarf planet Eris, confirming its status as Pluto's twin. The findings show that Eris is approximately 2326 kilometers in diameter, with an accuracy of 12 kilometers.
Astronomers at Caltech have discovered that the dwarf planet 2007 OR10, or Snow White, is an icy world with about half its surface covered in water ice. The findings suggest that the red-tinged dwarf planet may be covered in a thin layer of methane, remnants of an atmosphere slowly being lost into space.
Astronomers using the Hubble Space Telescope have discovered a fourth moon orbiting Pluto, the smallest discovered to date. The new moon, temporarily designated P4, was found in a survey searching for rings around Pluto and has an estimated diameter of 8-21 miles.
Researchers develop method to locate satellite galaxies based on hydrogen gas distribution, predicting Galaxy X's mass and location. The technique has broad implications for dark matter detection and alternative gravity theories.
The Panoramic Survey Telescope & Rapid Response System (Pan-STARRS) PS1 telescope has discovered ten Kuiper Belt residents, ranging in size from 180 to 300 miles, and is expected to find a whole range of objects including dwarf planets and comets.
A team of scientists led by Jay Pasachoff observed the shiniest object in the solar system, 2002 TX300, a fragment of Haumea, using a network of telescopes. The measurements reveal its icy surface and size, confirming it as a small, reflective body with an age estimated to be around a billion years.
Astronomers have discovered a small brown dwarf star orbiting a Sun-like star with a planet, revealing a new class of coldest brown dwarfs called T dwarfs. The team also found another smaller brown dwarf in the same system, which may be the youngest known T dwarf, providing a snapshot of early brown-dwarf development.
The International Astronomical Union has named the newly discovered dwarf planet Eris and its moon Dysnomia. The name Eris was proposed by Michael Brown and accepted unanimously by the Working Group for Planetary System Nomenclature and the Committee for Small Body Nomenclature.
The IAU defined a planet as a celestial body in orbit around the Sun with sufficient mass to assume hydrostatic equilibrium. The new definition includes our solar system's eight recognized planets and a distinct class of dwarf planets, including Pluto.
The IAU draft definition of a planet, which includes eight classical planets, three new 'plutons,' and Ceres, has been reached after two years of work. The definition states that a planet must be in orbit around a star and have sufficient mass to assume a hydrostatic equilibrium shape.
Researchers have devised a method to catch the early stages of gas-giant core accretion, suggesting that young intermediate-sized cores could be a clear indicator of core accretion. The existence of these cores would likely yield gas-giant planets in as little as 1,000 years around small, gravitationally weak stars.
Astronomers have confirmed the presence of two new moons around Pluto, provisionally designated S/2005 P 1 and S/2005 P 2. The new discoveries were made possible by the exceptional resolution of the Hubble Space Telescope, which revealed the small moons' orbits with similarities to Charon's.
Astronomers have discovered a new planet, 2003 UB313, which is larger than Pluto and located in the Kuiper Belt. The object's size was determined through thermal emission measurements, revealing a diameter of approximately 3000 km.
The University of Colorado's Student Dust Counter instrument will monitor dust grain density in space as New Horizons approaches Pluto. The team hopes to identify undetected clumps of dust, shedding light on the solar system's formation and other stars' planetary systems.
Astronomers have discovered a candidate planetary companion to a relatively bright young brown dwarf star located 225 light-years away in the southern constellation Hydra. The object, detected by NASA's Hubble Space Telescope, is estimated to be about five times the mass of Jupiter and orbits its host at a 99% confidence level.
Astronomers use Hubble's Near Infrared Camera and Multi-Object Spectrometer to observe a faint companion object orbiting a relatively bright young brown dwarf star. The observations provide strong evidence for the existence of an extrasolar planet, which is estimated to be about five times the mass of Jupiter.
The Johns Hopkins University Applied Physics Laboratory (APL) has been selected by NASA to develop the first mission to explore Pluto and the Kuiper Belt region. The New Horizons: Shedding Light on Frontier Worlds mission will use a team of scientists and engineers from various institutions to design, build, and operate the spacecraft.
Astronomers discover that asteroid 1929 Kollaa was once part of the larger asteroid 4 Vesta, which is believed to be the source of meteorites found on Earth. This finding helps scientists build a geologic map of the asteroid belt and understand forces that have acted on asteroids in the past.
Researchers have discovered 18 planet-like objects drifting free of a central star in the Orion constellation. The objects' cool temperatures suggest they may be planets or brown dwarfs, challenging current theories on planetary formation.
Scientists find five stars with unexplained wobbles, suggesting the presence of a second companion planet. The discovery of three new gas giants adds to the list of 41 known planets outside our solar system, revealing patterns in planetary formation and dynamics.
The solar system's ultimate fate is predicted to be a collapse of the sun into a white dwarf, incinerating the Earth and inner planets in the process. However, a close encounter with a passing star may rescue life by hurling the Earth out of the solar system.
When a star swallows a planet, it can experience profound effects on its evolution, including changes in spin rate and emission of infrared radiation. The simulations show that large planets can survive for thousands of years before being vaporized by the heat, leaving behind tell-tale signs such as high lithium abundance.
Scientists capture high-resolution images of Neptune's clouds and their movement, providing fresh insight into the planet's extraordinary weather. The observations reveal a powerful equatorial jet stream and storms dwarfing Earth's most violent storms.
A new theoretical study reproduces actual observations of the confirmed brown dwarf Gliese 229 B, providing insights into its atmosphere and formation. The research helps accelerate searches for brown dwarfs and giant extrasolar planets, shedding light on their composition and formation processes.