Orcus rotation period
WebIt was initially and provisionally known as 2004 DW. The name Orcus, from a Roman god of the dead and another name for the Greek deity Hades, was approved by the International Astronomical Union (IAU) on November 22, 2004. It was chosen because Orcus moves in an orbit similar to that of Pluto. WebOrcus is in a 2:3 orbital resonance with Neptune, having an orbital period of 245 years, and is classified as a plutino. Its orbit is moderately inclined at 20.6 degrees to the ecliptic . [13] Orcus's orbit is similar to Pluto 's (both …
Orcus rotation period
Did you know?
WebThe fast rotation of Orcus obtained from TESS measurements. Csaba Kiss ... http://www.philipsedgwick.com/Centaur_TNO/KuiperKeywords.htm
WebOrcus is in a 2:3 orbital resonance with Neptune, having an orbital period of 245 years, and is classified as a plutino. Its orbit is moderately inclined at 20.6 degrees to the ecliptic. Orcus's orbit is similar to Pluto's (both have … Weborbital period P: 247.873825088923 yr (= 90537.8 d) eccentricity e: 0.21843 perihelion distance q: 30.8406 AU aphelion distance Q: 48.0789 AU inclination i: 20.552009° …
WebRotational period (hours) 13; Orbital period (years) 245; Orbital velocity (km/sec) 4.42; Eccentricity of orbit; 0.227; Tilt of axis (°) Inclination of orbit (°) 20.5; Surface gravity … Web1.1 Sources of Observed Magnetic Fields. Observed planetary magnetic fields can result from a variety of processes. For example, external sources that generate observed planetary magnetic fields include Venus' ionospheric currents, Earth's magnetospheric currents, and electromagnetic induction in the saltwater oceans of Europa, Ganymede, and Callisto due …
Webrotation period RP s: ... -- (90482) Orcus and Vanth --discovery and notes: Primary discovered 2004 Feb 17 from Palomar Observatory, California, USA by M. E. Brown, C. A. Trujillo, and D. L. Rabinowitz. Alternate designation(s): 2004 DW. Linked to prediscovery observations from 1951 Nov 08. Permanent number assigned 2004 Aug 30. Named 2004 …
WebJan 1, 2011 · The RA residuals of an orbital fit to the astrometric data revealed a periodicity of 9.7+-0.3 days, which is what one would expect to be induced by the known Orcus companion. The residuals are... novasoftwaredogWebOct 8, 2024 · The rotation period is estimated to be at 22.83 hours, relatively long for a dwarf planet and about 7.77 Earth hours to complete one sidereal rotation. These statistics suggest that a single day on Makemake is less … novasoft empleoWebThe perihelion of Orcus's orbit is around 120° from that of Pluto, while the eccentricities and inclinations are similar. Because of these similarities and contrasts, along with its large … how to soften hard brownies without microwaveWebrotation could be tidally locked to the satellite’s orbital period. We found that a photometric variability of 9.7 0.3 days is clear in our data, and is nearly coincident with the orbital … novasoft lotionWebAug 5, 2024 · Ceres takes 1,682 Earth days, or 4.6 Earth years, to make one trip around the Sun. As Ceres orbits the Sun, it completes one rotation every 9 hours, making its day length one of the shortest in the solar system. Ceres' axis of rotation is tilted just 4 degrees with respect to the plane of its orbit around the Sun. how to soften hard bread rollsWebMay 13, 2010 · If the post-impact Orcus was not rapidly rotating and had a spin period more like the ~10 hr periods of typical KBOs, however, the orbit would be doubly synchronous … novasoft payrollWebRotation period: 0.3781 d: Spectral class: G-type asteroid: Absolute magnitude: 3.34: Albedo (geometric) 0.113: Mean surface temperature ~167 K max: 239 K (-34 ° C) ... 90482 Orcus, and 90377 Sedna. At certain points in its orbit, Ceres can reach a magnitude of 7.0. This is generally regarded as being just barely too dim to be seen with the ... novasoft portal web