WebPallas (minor-planet designation: 2 Pallas) is the second asteroid to have been discovered, after Ceres.It is believed to have a mineral composition similar to carbonaceous chondrite meteorites, like Ceres, though significantly less hydrated than Ceres. It is the third-largest asteroid in the Solar System by both volume and mass, and is a likely remnant protoplanet. WebMay 19, 2024 · Ceres is about 1,000 km in diameter and accounts for a third of the mass in the main asteroid belt.It dwarfs most of the other bodies in the belt. Now we know that it's …
Dwarf Planets: Definition, Characteristics, and Locations - Study.com
WebCeres is a dwarf planet orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Ceres as potentially hazardous because its … WebOrbit eccentricity: 0.0934: Aphelion (106 km) 249.2: Sidereal rotation period (hrs) 24.6229: Obliquity to orbit (deg) 25.19 Discoverer: Unknown: Discovery Date: Prehistoric: Distance from Earth: Minimum (106 km): 54.5 Maximum (106 km): 401.3. Martian Atmosphere Surface Pressure: ~6.1 mb (variable) [6.9 mb to 9 mb (Viking 1 Lander site)] ... haley wheeler kentucky
Astronomy 101: Homework Instructions - Vanderbilt University
WebView Keplers Laws Worksheet - rachael.pdf from ASTR 1030 at Clemson University. Kepler’s Laws Worksheet These lab activities have evolved over many years of use in Clemson University’s Department of WebPallas, third largest asteroid in the asteroid belt and the second such object to be discovered, by the German astronomer and physician Wilhelm Olbers on March 28, 1802, following the discovery of Ceres the year before. It is named after Pallas Athena, the Greek goddess of wisdom. Pallas’s orbital inclination of 34.8° is rather large, but its moderate … WebJun 1, 2024 · Ceres comprises about 0.33% of the total mass of the asteroid belt and has low density (2.2 g/cm 3), low albedo and a spectral reflectance similar to carbonaceous chondrites (McCord and Sotin, 2005). Ceres orbits the Sun deep in the main belt, with a semimajor axis of 2.767 au, an eccentricity of 0.097 and an inclination of about 9.73°. bumper honda