2012 FN
| Discovery | |
|---|---|
| Discovered by | Mount Lemmon Survey (G96) | 
| Discovery date | 17 March 2012 | 
| Designations | |
| Apollo NEO[1] | |
| Orbital characteristics[1] | |
| Epoch 17 March 2012 (JD 2456003.5) | |
| Uncertainty parameter 9 | |
| Aphelion | 1.4500 AU (216.92 Gm) | 
| Perihelion | 0.99291 AU (148.537 Gm) | 
| 1.2214 AU (182.72 Gm) | |
| Eccentricity | 0.18710 | 
| 1.35 yr (493.07 d) | |
| 21.742° | |
| Inclination | 3.2329° | 
| 356.91° | |
| 147.89° | |
| Earth MOID | 0.015601 AU (2.3339 Gm) | 
| Jupiter MOID | 3.54794 AU (530.764 Gm) | 
| Physical characteristics | |
| Dimensions | ~5 meters (16 ft) | 
| 29.2[1] | |
|  | |
2012 FN is an Apollo asteroid and a near-Earth object[1] that has a 1 in 4 billion chance of impacting Earth on 7 March 2113.[2] It is estimated to be 5 meters in diameter, which means that it poses no threat if it impacts Earth. An impact would have the kinetic energy of about 3 kt of TNT,[2] and would probably result in an air burst in the upper atmosphere. It is the least threatening asteroid listed on the Sentry Risk Table.[3] The very short observation arc of only 3 hours[2] results in a very poorly constrained orbit, and it could just as easily be 2 AU from Earth on 7 March 2113.[4]
See also
References
- 1 2 3 4 "JPL Small-Body Database Browser: (2012 FN)" (last observation: 2012-03-17; arc: 3 hours; uncertainty: 9). Jet Propulsion Laboratory. Retrieved 1 April 2016.
- 1 2 3 NASA JPL. "2012 FN Impact Risk". Retrieved 2014-10-25.
- ↑ Sentry Risk Table (NASA JPL)
- ↑ "2012FN Ephemerides for 6-8 March 2113". NEODyS (Near Earth Objects – Dynamic Site). Retrieved 2014-10-25.
External links
- List of Apollo asteroids - The International Astronomical Union Minor Planet Center
- 2012 FN at the JPL Small-Body Database
| 
 | ||||||||||||||||||||||||||||||||||||||
| 
 | ||||||||||||||||||||||||||||
This article is issued from Wikipedia - version of the Friday, April 01, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.