90482 Orcus
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Discovery | |
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Discovered by: | M. Brown, C. Trujillo, D. Rabinowitz |
Discovery date: | February 17, 2004 |
Alternative names: | 2004 DW |
Minor planet category: | Plutino |
Orbital characteristics | |
Epoch November 10, 1951 (JD 2433960.5) | |
Aphelion distance: | 7226.801 Gm (48.31 AU) |
Perihelion distance: | 4567.091 Gm (30.53 AU) |
Semi-major axis: | 5896.946 Gm (39.419 AU) |
Eccentricity: | 0.22552 |
Orbital period: | 90396.4 d (247.492 a) |
Avg. orbital speed: | 4.68 km/s |
Mean anomaly: | 79.561° |
Inclination: | 20.55233° |
Longitude of ascending node: | 268.586° |
Argument of perihelion: | 73.8325° |
Satellites: | 1 (92-432 km) |
Physical characteristics | |
Dimensions: | 840 - 1880 km |
Mass: | 6.2 - 7.0×1020 kg |
Mean density: | 2.0? g/cm³ |
Equatorial surface gravity: | 0.2348 - 0.5254 m/s² |
Escape velocity: | 0.4441 - 0.9939 km/s |
Rotation period: | ? d |
Albedo: | 0.09 (assumed) |
Temperature: | ~45 K |
Spectral type: | B-V=0.68; V-R=0.37 [1] |
Absolute magnitude: | 2.3 |
90482 Orcus (originally known by the provisional designation 2004 DW) is a Kuiper Belt object (KBO) that was discovered by Michael Brown of Caltech, Chad Trujillo of the Gemini Observatory, and David Rabinowitz of Yale University. The discovery images of this object were acquired on February 17, 2004. Precovery images as early as November 8, 1951 were later identified.
Contents |
[edit] Orbit
Orcus is a typical plutino (an object in 2:3 orbital resonance with Neptune). Orcus's orbit is shaped similarly to Pluto's (both have perihelia above the ecliptic), but is differently oriented. Although at one point its orbit approaches that of Neptune, the resonance between the two bodies means that Orcus itself is always a great distance away from Neptune (there is always an angular separation of over 60 degrees between them).
[edit] Physical characteristics
[edit] Size and magnitude
The absolute magnitude of Orcus is 2.3 (comparable with the 2.6 of another KBO, 50000 Quaoar). Using an assumed albedo of 0.09, Trujillo estimates its diameter to be approximately 1600 km, which makes Orcus the largest known plutino after Pluto/Charon and the sixth-largest known trans-Neptunian object, after Eris, Pluto, (136472) 2005 FY9, (136108) 2003 EL61 and 90377 Sedna.
[edit] Colours and spectra
Observations in infrared by the European Southern Observatory give results consistent with mixtures of water ice and carbonaceous compounds.[2] Further, the infrared spectra taken with the Gemini telescope confirmed a modest water ice signature, compatible with a cover of 15–30%, but no more than 50% of the surface. This means there is less ice than on Charon, but a similar amount to that on Triton. Limitations were also placed on the amount of methane ice (less than 30%) leaving open the possibility for discovery of other components in the future.[3]
KBOs display a diversity of colours and spectra even among objects with similar orbits. Orcus presents a neutral colour in comparison with the redness of an object like Ixion.
[edit] Satellite
The discovery of a satellite of Orcus was reported in IAUC 8812 on 22 February 2007 [1]. The orbit of this satellite has yet to be determined.
The satellite was found at 0.25 arcsec from Orcus with magnitude difference of 2.7[4]. Assuming an albedo similar to that of the primary the magnitude suggests a quite substantial diameter (~220 km) compared with Orcus.
[edit] Name
Under the guidelines of the International Astronomical Union's naming conventions, objects with a similar size and orbit to that of Pluto are named after underworld deities. Accordingly, the discoverers suggested naming the object after Orcus, a god of the dead in Roman mythology. The name was approved and published on November 22, 2004.
[edit] External links and sources
- 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 F. Helin and Robert Thicksten / NEAT
- MPEC 2004-D13 correcting MPEC 2004-D09
- Chad Trujillo's page on 2004 DW
- First BBC article
- First New Scientist article
- Updated orbital elements from Lowell Observatory
- AstDys orbital elements
- Orbital simulation from JPL (Java)
[edit] References
- ^ Tegler, Stephen C. (2006-01-26). Kuiper Belt Object Magnitudes and Surface Colors. Retrieved on 2006-11-05.
- ^ C. de Bergh, A. Delsanti, G. P. Tozzi, E. Dotto, A. Doressoundiram and M. A. Barucci (2005). "The Surface of the Transneptunian Object 9048 Orcus". Astronomy & Astrophysics 437: 1115-1120. DOI:10.1051/0004-6361:20042533.
- ^ Chadwick A. Trujillo, Michael E. Brown, David L. Rabinowitz, Thomas R. Geballe (2005). "Near Infrared Surface Properties of the Two Intrinsically Brightest Minor Planets (90377) Sedna and (90482) Orcus". The Astrophysical Journal 627: 1057–1065. DOI:10.1086/430337. Preprint on arXiv.
- ^ Distant EKO The Kuiper Belt Electronic newsletter, March 2007
Minor planets | ||
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Previous minor planet | 90482 Orcus | Next minor planet |
List of asteroids |
Kuiper belt: Orcus · Pluto · Ixion · 2002 UX25 · Varuna · 2002 TX300 · 2003 EL61 · Quaoar · 2005 FY9 · 2002 AW197
Scattered disc: 2002 TC302 · Eris · 2004 XR190 · Sedna
For pronunciation, see: Centaur and TNO pronunciation.
Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Comets · Trans-Neptunians (Kuiper belt • Scattered disc • Oort cloud)
For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons and the Solar System.
For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names.