Orcus rotation period
WebRotation 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 ... WebSo far, Orcus’ rotation properties are not uniquely defined: 0.03 to 0.18 magnitude amplitude variations are measured over a period ranging from ∼7 to 21h (Duffard et al. 2009, and ref-erences therein), although Sheppard (2007) finds no lightcu rve variations within the photometric uncertainties of his measure-ments.
Orcus rotation period
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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 … WebMay 13, 2010 · We also find that Vanth has a nearly face-on circular orbit with a period of 9.5393 ± 0.0001 days and semimajor axis of 8980 ± 20 km, implying a system mass of (6.32 ± 0.01) × 10 20 kg or 3.8% the mass of dwarf planet Eris.
WebAug 31, 2015 · Much like Pluto, Orcus has a very long orbital period, taking 245.18 years (89552 days) to complete a single rotation around the sun. … 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 …
WebMay 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 … 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.
WebJan 1, 2011 · The position of Orcus at the start of the run is indicated by a circle and its trajectory is shown as a white line. The square indicates where the trajectory ended. North …
Webwith the Ortiz et al. (2006)andThirouin et al. (2010) rotational lightcurves. These results already seem to indicate that Orcus’ rotation is not tidally locked to its satellite, but because the satellite orbital period is much longer than the usual observing windows for ro-tational variability studies, the question arises as to whether the desktop shortcuts disappear windows 10Webrotation 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 … desktop shortcuts missingOrcus 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 perihelia above the ecliptic), but is oriented differently. Although at one point its orbit … See more Orcus (minor-planet designation 90482 Orcus, provisional designation 2004 DW) is a trans-Neptunian dwarf planet with a large moon, Vanth. It has a diameter of 870 to 960 km (540 to 600 mi), the size of or somewhat smaller … See more Size and magnitude The absolute magnitude of Orcus is approximately 2.3. The detection of Orcus by the Spitzer Space Telescope in the far infrared and by Herschel Space Telescope in submillimeter estimates its diameter at 958.4 km (595.5 mi), … See more • List of possible dwarf planets • List of trans-Neptunian objects • List of Solar System objects by size See more Discovery Orcus was discovered on 17 February 2004, by American astronomers Michael Brown of Caltech, Chad Trujillo of the Gemini Observatory, and David Rabinowitz of Yale University. Precovery images taken by the Palomar Observatory as … See more Orcus has one known moon, Vanth (full designation (90482) Orcus I Vanth). It was discovered by Michael Brown and T.-A. Suer using discovery images taken by the Hubble Space Telescope See more • MPEC 2004-D09 announcing the discovery but attributing it to Raymond J. Bambery, Steven H. Pravdo, Michael D. Hicks, Kenneth J. Lawrence, Daniel MacDonald, Eleanor Helin and Robert Thicksten / NEAT • MPEC 2004-D13 correcting MPEC 2004-D09 See more desktop shortcuts addingWebAug 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. desktop shortcuts do not work in windows 10WebJan 11, 2011 · It's nearly circular, with a period of 9.5393 ± 0.0001 days at a distance of 8980 ± 20 kilometers. The total mass of the Vanth-Orcus system. This follows directly from … chucks auto repair 19006WebThe 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 … chucks auto rebuild-rstrtn shoreline wahttp://www.johnstonsarchive.net/astro/astmoons/am-90482.html desktop shortcuts for all users