TNOs and similar bodies |
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*Trans-Neptunian dwarf planets are "plutoids"
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Neptune trojans (named by analogy to Jupiter's Trojan asteroids) are Kuiper belt object-like bodies in solar orbit that have the same orbital period as Neptune and follow roughly the same orbital path.[1] Six of the seven found so far lie in the elongated, curved region around the Sun-Neptune L4 Lagrangian point 60° ahead of Neptune.
The discovery of 2005 TN53 in a high inclination (>25°) orbit was significant as it suggested a 'thick' cloud of trojans[2] (Jupiter trojans have inclinations up to 40°[3]). It is believed that large (radius ≈ 100 km) Neptune trojans could outnumber Jupiter trojans by an order of magnitude.[4][5]
Both 2005 TN74[6] and 2007 RW10 were believed to be Neptune trojans when first discovered, but were later reclassified.
On August 12th, 2010, the Minor Planet Center announced the discovery of the first known L5 Neptune trojan, 2008 LC18.[7] Neptune's trailing L5 region is very difficult to observe because it is along the line-of-sight to the the center of our galaxy, an area of the sky crowded with stars.
It may be possible for the New Horizons spacecraft to investigate L5 Neptune trojans discovered by 2014, when it passes through this region of space en route to Pluto.[5]
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As of August 2010, seven Neptune trojan objects are known. This table is constructed from information obtained from the List Of Neptune Trojans maintained by the IAU Minor Planet Center[1] and with diameters from Sheppard and Trujillo's paper on 2008 LC18.[8]
Provisional Designation |
Lagrangian Point |
Perihelion (AU) |
Aphelion (AU) |
Inclination (°) |
Absolute magnitude |
Diameter (km) |
Discovery year |
Reference |
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2001 QR322 | L4 | 29.428 | 31.349 | 1.3 | 8.2 | ~140 | 2001 | |
2004 UP10 | L4 | 29.351 | 31.259 | 1.4 | 8.8 | ~100 | 2004 | |
2005 TN53 | L4 | 28.253 | 32.284 | 25.0 | 9.1 | ~80 | 2005 | [2] |
2005 TO74 | L4 | 28.733 | 31.824 | 5.2 | 8.5 | ~100 | 2005 | |
2006 RJ103 | L4 | 29.345 | 31.005 | 8.2 | 7.5 | ~180 | 2006 | |
2007 VL305 | L4 | 28.131 | 32.171 | 28.1 | 8.0 | ~160 | 2007 | |
2008 LC18 | L5 | 27.547 | 32.468 | 27.5 | 8.4 | ~100 | 2008 | [8] |
Planetary Trojans - the main source of short period comets? (arXiv:1007.2541 : 15 Jul 2010)
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