List of the brightest Kuiper belt objects
Main article: Kuiper belt
Since the year 2000, a number of Kuiper belt objects (KBOs) with diameters of between 500 and 1500 km (more than half that of Pluto) have been discovered. 50000 Quaoar, a classical KBO discovered in 2002, is over 1200 km across. Makemake and Haumea, both announced on 29 July 2005, are larger still. Other objects, such as 28978 Ixion (discovered in 2001) and 20000 Varuna (discovered in 2000) measure roughly 500 km across.[1] This has led gradually to the acceptance of Pluto as the largest member of the Kuiper belt.
The brightest known dwarf planets and other KBOs (with absolute magnitudes < 4.0), are:
Permanent Designation |
Provisional Designation |
Absolute magnitude |
Albedo (%)[2] | Equatorial diameter (km)[2] |
Semimajor axis (AU) |
Date found | Discoverer | Diameter method |
---|---|---|---|---|---|---|---|---|
Pluto[3] | -1.0 | 60 | 2370. | 39.4 | 1930 | C. Tombaugh | occultation | |
Makemake | 2005 FY9[4] | -0.3 | 80. +10.−20. | 1500. -200+400 | 45.7 | 2005 | M. Brown, C. Trujillo & D. Rabinowitz | Thermal |
Haumea | 2003 EL61[5] | 0.1 | 84. +10−20 | 1150. -100+250 | 43.3 | 2005 | Sierra Nevada Observatory, Spain[6] | Thermal |
Charon[7] | S/1978 P 1 | 1 | 40 | 1205. | 39.4 | 1978 | J. Christy | occultation |
Orcus | 2004 DW | 2.3 | 19.72 +3.40−2.76 | 946.3 -72.3+74.1 | 39.4 | 2004 | M. Brown, C. Trujillo & D. Rabinowitz | Thermal |
Quaoar | 2002 LM60 | 2.6 | 19.9 +13.2−7. | 844. -190+207 / 1260 ± 190 | 43.5 | 2002 | C. Trujillo & M. Brown | Disk resolved/thermal |
Ixion | 2001 KX76 | 3.2 | 12 +14−6 | 650. -220+260 | 39.6 | 2001 | DES | Thermal |
278361 | 2007 JJ43 | 3.2[8] | 47.8 | 2007 | Palomar Observatory | |||
55636 | 2002 TX300 | 3.3 | 10. or more | 800. or less | 43.1 | 2002 | NEAT | Thermal |
55565 | 2002 AW197 | 3.3 | 11.77 +4.42−3.00 | 734.6 -108.3+116.4 | 47.4 | 2002 | C. Trujillo, M. Brown, E. Helin, Steven H. Pravdo, K. Lawrence & Michael D. Hicks; Palomar Observatory |
Thermal |
55637 | 2002 UX25 | 3.6 | 11.50 +5.09−3.09 | 681.2 -114.0+115.6 | 42.5 | 2002 | Anne S. Descour; Spacewatch | Thermal |
Varuna | 2000 WR106 | 3.7 | 16. +10−8 | 500. -100+100 | 43.0 | 2000 | R. McMillan | Thermal |
307261 | 2002 MS4 | 3.8 | 08.41 +3.78−2.26 | 726.2 -122.9+123.2 | 41.8 | 2002 | C. Trujillo, M. Brown | Thermal |
471143 | 2010 EK139[8] | 3.8 | 25 +0.02-0.05 | 470 +35-10 | 40.5 | 2010 | A. Udalski, S. Sheppard, M. Kubiak, and C. Trujillo | Thermal |
208996 | 2003 AZ84[9] | 3.9 | 12.32 +4.31−2.91 | 685.8 -95.5+98.8 | 39.6 | 2003 | C. Trujillo, M. Brown, E. Helin, Steven H. Pravdo, K. Lawrence & Michael D. Hicks |
Thermal |
2010 KZ39[8] | 3.9 | 45.8 | 2010 | A. Udalski, S. Sheppard, M. Szymanski, and C. Trujillo | ||||
See also
References
- ↑ Audrey Delsanti & David Jewitt. "The Solar System Beyond The Planets" (PDF). Institute for Astronomy, University of Hawaii. Archived from the original (PDF) on 2007-01-29. Retrieved 2007-03-09.
- 1 2 John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; Jean-Luc Margot (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv:astro-ph/0702538.
- ↑ NASA Pluto planetary factsheet accessed on July 1, 2007
- ↑ "MPEC 2005-O42 : 2005 FY9". Retrieved 2007-06-01.
- ↑ Wm. Robert Johnston. "(136108) 2003 EL61, S/2005 (2003 EL61) 1, and S/2005 (2003 EL61) 2". Retrieved 2007-07-01.
- ↑ "MPEC 2005-O36 : 2003 EL61".
- ↑ Wm. Robert Johnston. "Pluto, Charon, Nix, and Hydra". Retrieved 2007-07-01.
- 1 2 3 http://arxiv.org/pdf/1107.5309v1.pdf
- ↑ "MPEC 2003-B27 : 2003 AZ84". Minor Planet Center. Retrieved 2007-07-02.
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