WebThe rotation of Orcus has been observed. It completes a rotation on its axis every 13.19 hours. No Close Approaches Orcus's orbit is 29.20 AU from Earth's orbit at its closest …
90482 Orcus - Orbit and Rotation Orbit Rotation
WebOct 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 … http://www.johnstonsarchive.net/astro/astmoons/am-90482.html how many fighters did b17s shoot down
In Depth Ceres – NASA Solar System Exploration
Webrotation 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 … Orcus 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 Webrotation 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 … how many fighters are in a squadron