2012 FC71
2012 FC71, also written 2012 FC71, is a small asteroid trapped in a Kozai resonance with the Earth.[4]
| Discovery [1] | |
|---|---|
| Discovered by | Mt. Lemmon Survey A. Boattini (unofficial credits) |
| Discovery date | 31 March 2012 |
| Designations | |
| 2012 FC71 | |
| Orbital characteristics [2] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter | |
| Observation arc | 21 days |
| Aphelion | 1.0750 AU |
| Perihelion | 0.9008 AU |
| 0.9879 AU | |
| Eccentricity | 0.0882 |
| 0.98 yr (359 days) | |
| 150.11° | |
| 1° 0m 13.68s / day | |
| Inclination | 4.9430° |
| 38.142° | |
| 348.30° | |
| Earth MOID | 0.0566 AU (22.1 LD) |
| Physical characteristics | |
| Dimensions | 20–40 m[a][3] |
| 25.2[2] | |
Discovery, orbit and physical properties
It was first observed on 31 March 2012 by Andrea Boattini, observing for the Mt. Lemmon Survey.[5][6] Its orbit is characterized by low eccentricity (0.088), low inclination (4.97º) and a semi-major axis of 0.9895 AU.[6] It is an Aten asteroid but also an Earth crosser. As of 21 April 2012 its orbit is based on 35 observations spanning a data-arc of 21 days. This short observation arc results in an orbit uncertainty of 7. It has not been seen since and is unlikely to be seen again for several decades. It will remain both very dim (around apparent magnitude 27), and close in the sky to the Sun (solar elongation of less than 90 degrees), making it impossible to observe with current ground based telescopes till the 2060s. A number of times during the decade it will again be visible in the night sky and at times be brighter than apparent magnitude 21, as when it was first observed.[2]
Kozai resonator and future orbital evolution
2012 FC71 is locked in a Kozai resonance and as such it has a very slow orbital evolution and it will remain relatively unperturbed for hundreds of thousands of years.[4] It had a close encounter with the Earth on 18 April 2012 at 0.076 AU when it was discovered and another on 17 May 2013 at 0.0581 AU, which was not observed.
Origin
It may have been originated within the Venus-Earth-Mars region or in the main asteroid belt like other Near-Earth Objects, then transitioned to an Amor-class asteroid before entering Earth's co-orbital region.[4]
Notes
- ^ This is assuming an albedo of 0.20–0.04.
References
- "2012 FC71". Minor Planet Center. Retrieved 2 February 2017.
- "JPL Small-Body Database Browser: 2012 FC71" (2012-04-21 last obs.). Jet Propulsion Laboratory. Retrieved 2 February 2017.
- "Absolute Magnitude (H)". NASA/JPL. Retrieved 2 February 2017.
- de la Fuente Marcos, C.; de la Fuente Marcos, R. (July 2013). "A resonant family of dynamically cold small bodies in the near-Earth asteroid belt". Monthly Notices of the Royal Astronomical Society: Letters. 434 (1): L1–L5. arXiv:1305.2825. Bibcode:2013MNRAS.434L...1D. doi:10.1093/mnrasl/slt062.
- Discovery MPEC
- MPC data on 2012 FC71
- Further reading
- Secular perturbations of asteroids with high inclination and eccentricity Kozai, Y. 1962, Astronomical Journal, Vol. 67, p. 591
- The Kozai resonance for near-Earth asteroids with semimajor axes smaller than 2AU Michel, P., & Thomas, F. 1996, Astronomy and Astrophysics, Vol. 307, p. 310
- A resonant family of dynamically cold small bodies in the near-Earth asteroid belt de la Fuente Marcos, C., de la Fuente Marcos, R. 2013, Monthly Notices of the Royal Astronomical Society: Letters, Vol. 434, Issue 1, pp. L1-L5
External links
- List Of Aten Minor Planets, Minor Planet Center
- MPEC 2012-G13 : 2012 FC71, discovery Minor Planet Electronic Circular (MPEC)
- AstDys-2 on 2012 FC71 at AstDys
- NEODyS-2 on 2012 FC71 at NEODyS
- 2012 FC71 at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 2012 FC71 at ESA–space situational awareness
- 2012 FC71 at the JPL Small-Body Database
