90482 Orcus
Appearance
Discovery | |
---|---|
Discovered by | M. Brown, C. Trujillo, D. Rabinowitz |
Discovery date | February 17, 2004 |
Designations | |
2004 DW | |
Plutino[1] | |
Orbital characteristics | |
Epoch November 30, 2008 (JD 2 454 800) | |
Aphelion | 7 188.17 Gm (48.05 AU) |
Perihelion | 4 535.80 Gm (30.32 AU) |
5 862.44 Gm (39.188 AU) | |
Eccentricity | 0.226 18 |
89 606 d (245.33 yr) | |
Average orbital speed | 4.68 km/s |
164.68° | |
Inclination | 20.593° |
268.722° | |
72.474° | |
Known satellites | 1 (92-432 km) |
Physical characteristics | |
Dimensions | 946.3 +74.1 −72.3 km (diameter)[2] |
Mass | ~7.5×1020 kg |
Mean density | ~1.5 g/cm³ (assumed) |
~0.2 m/s² | |
~0.44 km/s | |
13.19h[3] | |
Albedo | 19.75 +3.40 −2.76 % |
Temperature | ~45 K |
Spectral type | B-V=0.68; V-R=0.37 [4] |
19.1 (opposition)[5] | |
2.3[6] | |
90482 Orcus, originally known by the provisional designation 2004 DW) is a Kuiper belt object (KBO) and could be a dwarf planet. It was found by Michael Brown, Chad Trujillo and David Rabinowitz on February 17, 2004. It was also seen in pictures from November 8, 1951.
Moon
A moon of Orcus was found on 22 February 2007.[7] The orbit of this moon has yet to be found out.
The satellite was found at 0.25 arcsec from Orcus with magnitude difference of 2.7.[8] Assuming an albedo similar to that of the primary, the magnitude suggests a diameter of about 220 km. It is thought to be a smaller KBO that was captured.
Other websites
- 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) / Ephemeris
References
- ↑ Buie, Marc W. (2007-12-22). "Orbit Fit and Astrometric record for 90482". SwRI (Space Science Department). Archived from the original on 2012-02-08. Retrieved 2008-09-19.
{{cite web}}
: Unknown parameter|deadurl=
ignored (|url-status=
suggested) (help) - ↑ Stansberry, J. (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope".
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suggested) (help) - ↑ "Overlooked dwarf planet candidates". BBC. 2008-02-19. Retrieved 2008-07-25.
- ↑ Tegler, Stephen C. (2006-01-26). "Kuiper Belt Object Magnitudes and Surface Colors". Archived from the original on 2007-11-16. Retrieved 2006-11-05.
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suggested) (help) - ↑ "HORIZONS Web-Interface". JPL Solar System Dynamics. Archived from the original on 2012-02-08. Retrieved 2008-07-02.
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ignored (|url-status=
suggested) (help) - ↑ "JPL Small-Body Database Browser: 90482 Orcus (2004 DW)". 2008-02-10 last obs. Archived from the original on 2012-02-08. Retrieved 2008-07-02.
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ignored (|url-status=
suggested) (help) - ↑ (90482) Orcus and Vanth Archived 8 February 2012 at WebCite
- ↑ Distant EKO The Kuiper Belt Electronic newsletter, March 2007