Mass of eris in kg
WebEris is tidally locked to Dysnomia, which implies that the moon must have a mass within the range of (3–5) × 1020 kg (mass ratio 0.02–0.03) in order to have slowed Eris's rotation down by tidal interactions. This gives a likely density range of 1.8–2.4 g/cm3 for Dysnomia, which is exceptionally high for trans-Neptunian objects of similar size. [4] WebEris is not always the most distant dwarf planet. At Eris’ furthest point from the Sun (Aphelion) it is so distant it is outside the Kuiper Belt, however at its closet point (Perihelion) it is closer the the than Pluto’s most distant point. Diameter: 2,326 km. Mass: 1.66 × 10^22 kg (0.23 Moons) Orbit Distance: 10,120,000,000 km (68.01 AU)
Mass of eris in kg
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Web8 de oct. de 2024 · Key Facts & Summary. It was discovered in 2005 by a team of astronomers led by Mike Brown and announced in the same day as Makemake, and two days after Haumea.; It is the most distant … WebDiscovered in 2005, Eris is now the largest known dwarf planet in our solar system. Its diameter is estimated at 3000 km, and it weighs roughly 1.66 x 1022 kg, which is about 27% more massive than Pluto. Like Pluto, it is very difficult to make precise measurements of Eris' diameter and mass, but these are the most updated estimates.
Eris has been measured at 2,326 ± 12 kilometers (1,445 ± 7 mi) in diameter; its mass is 0.28% that of the Earth and 27% greater than that of Pluto, although Pluto is slightly larger by volume, both having a surface area that is comparable to the area of Russia or Antarctica. Ver más Eris (minor-planet designation 136199 Eris) is the most massive and second-largest known dwarf planet in the Solar System. It is a trans-Neptunian object (TNO) in the scattered disk and has a high-eccentricity orbit. … Ver más Eris is a trans-Neptunian dwarf planet (plutoid). Its orbital characteristics more specifically categorize it as a scattered-disk object (SDO), or a TNO that has been "scattered" from the Ver más Eris displays very little variation in brightness as it rotates due to its uniform surface, making measurement of its rotation period difficult. Precise long-term monitoring of Eris's brightness indicates that it is tidally locked to its moon Dysnomia, with a … Ver más Eris was discovered by the team of Mike Brown, Chad Trujillo, and David Rabinowitz on January 5, 2005, from images taken on October 21, 2003. … Ver más Eris is named after the Greek goddess Eris (Greek Ἔρις), a personification of strife and discord. The name was proposed by the Caltech team on … Ver más Eris has an orbital period of 559 years. Its maximum possible distance from the Sun (aphelion) is 97.5 AU, and its closest (perihelion) is 38 AU. As the time of perihelion is defined … Ver más In November 2010, Eris was the subject of one of the most distant stellar occultations yet from Earth. Preliminary data from this event cast doubt on … Ver más Web6 de ago. de 2024 · With a radius of about 722 miles (1,163 kilometers), Eris is about 1/5 the radius of Earth. Eris, like Pluto, is a little smaller than Earth's Moon. If the Earth were the size of a nickel, Eris would be about …
Web11 de abr. de 2024 · Gladman et al. estimated a total mass for the 30–50 au distance range of 0.04–0.1 M ⊕, using an albedo ν r = 0.04 for all TNOs; this includes all dynamical components, but because the main belt represents only about half the mass (determined using the CFEPS model; Petit et al. 2011) in the 30–50 au distance range, a 0.02–0.05 … WebЕрида (пуним именом 136199 Ерида, симбол: ) је највећа патуљаста планета и налази се у Расејаном диску.Иако су је научници који су је открили првобитно називали десетом планетом Сунчевог система, редефинисањем статуса ...
Web15 de jun. de 2007 · From the period and semimajor axis of the orbit of Dysnomia, we can use Kepler's laws to calculate a mass for the Eris …
Web18 de mar. de 2016 · Density, mass and volume. Although all of the planets beyond Mars are gas giants, Pluto is small and rocky. ... In 2003, the icy body of Eris was found far beyond the Kuiper Belt. convert 25 usd to cedisWebSolution for The discovery of Dysnomia was fortunate, because it allowed scientists to calculate the mass of Eris. After careful observation, it was determined ... Consider a spherical asteroid with radius 28.2 km and mass of 5.69 x 1018 kg. The acceleration due ... fallout 76 mods in fallout 4WebWeight = Mass X Acceleration of Gravity Weight = N (Newtons) Mass = Kg (Kilograms) Acceleration of gravity = m/s2 (metres per second) RED SHIFT: Red-shift is the increase in wavelength of radiation due to an object moving away from the observer. The galaxies furthest away from us have the greatest red-shift because they are moving faster. Red- convert 25 us to cdnWeb27 de ago. de 2015 · And with an estimated mass of 1.4 ± 0.1 × 10 21 kg, Quaoar is about as massive as Pluto’s moon Charon, equivalent to 0.12 times the mass of Eris, and approximately 2.5 times as massive as Orcus. fallout 76 modus medical terminalWeb9 de abr. de 2024 · 2007年6月，观测结果显示阋神星的质量大约是 (1.66 ± 0.02)×10 22 kg，比冥王星重27%。 命名 [ 编辑 ] 根据小行星的命名常规，此星体的临时命名2003 … convert 25 usd to randsWeb31 de mar. de 2024 · Mass (1021kg) 1.586 Mean density (kg/m3) 1700 Surface gravity (m/s2) 0.29 Escape velocity (km/s) 0.59 Geometric Albedo 0.42 Bond Albedo 0.25 Apparent visual magnitude 16.8 Other Moons of … convert 2.63 to inchesWeb1 de jul. de 2007 · The prograde and retrograde solutions provide a mean mass estimate of 1.75±0.07·10 21 kg, which is the fourth largest known mass among dwarf planets after … fallout 76 moldy food