_2004_EW95&sq=Facebook&lang=en&file=File:120216-2004ew95_hst.jpg) Hubble Space Telescope image of 2004 EW95 taken in 2010 | |
| Discovery[1] | |
|---|---|
| Discovered by | Kitt Peak Obs. |
| Discovery date | 14 March 2004 |
| Designations | |
| (120216) 2004 EW95 | |
| Orbital characteristics[1] | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 4847 days (13.27 yr) |
| Aphelion | 52.590 AU (7.8674 Tm) |
| Perihelion | 26.975 AU (4.0354 Tm) |
| 39.783 AU (5.9515 Tm) | |
| Eccentricity | 0.32193 |
| 250.93 yr (91652 d) | |
| 359.95° | |
| 0° 0m 14.219s / day (n) | |
| Inclination | 29.234° |
| 25.704° | |
| 204.67° | |
| Earth MOID | 25.99 AU (3.888 Tm) |
| Jupiter MOID | 21.69 AU (3.245 Tm) |
| Uranus MOID | 9 AU (1.3 Tm)[4] |
| Physical characteristics | |
| Dimensions | 291 km[5] |
| 0.04 (dark)[5] | |
| ~21.0[6] | |
| 6.3[1] | |
(120216) 2004 EW95 (provisional designation 2004 EW95) is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter.[7] It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in this region of space.[8] It is thought to have originated closer to the Sun, perhaps even in the main asteroid belt.[8]
- ^ a b c d Cite error: The named reference
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AstDyswas invoked but never defined (see the help page). - ^ St. Fleur, Nicholas (10 May 2018). "This Asteroid Shouldn't Be Where Astronomers Found It". The New York Times. Retrieved 11 May 2018.
- ^ a b "Exiled asteroid discovered in outer reaches of solar system: ESO telescopes find first confirmed carbon-rich asteroid in Kuiper Belt". ScienceDaily. Retrieved 1 November 2018.