(277810) 2006 FV35, provisional designation 2006 FV35, is a sub-kilometer near-Earth asteroid in the dynamical Apollo asteroid group, discovered by Spacewatch at Kitt Peak National Observatory, Arizona, on 29 March 2006.[1] It is a quasi-satellite of Earth.[5] It is also notable for having a low delta-v requirement for rendezvous.[4] Although its orbital period is almost exactly 1 year, the orbit of 2006 FV35 has a high eccentricity which causes it to cross the paths of both Venus and Mars.
Contents
1Transfer energy
2See also
3References
4External links
Transfer energy
With a semi-major axis of almost exactly 1 astronomical unit, 2006 FV35 has a relatively low transfer energy from Earth. The delta-v required to transfer to the asteroid varies between 11 and 13 km/s; this change in delta-v oscillates over an approximately 200-year period with the current transfer cost near its maximum of 13 km/s.[4]
See also
(164207) 2004 GU9
References
↑ 1.01.1"277810 (2006 FV35)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=277810. Retrieved 20 January 2018.
↑Gerhard Hahn. "EARN: 2006 FV35". Archived from the original on 2006-10-03. https://web.archive.org/web/20061003035042/http://earn.dlr.de/nea/K06F35V.htm.
↑ 4.04.14.2Stacey, R. Greg; Connors, Martin (February 2009). "Delta-v requirements for earth co-orbital rendezvous missions". Icarus(Proof) (7): 822. doi:10.1016/j.pss.2009.01.013. Bibcode: 2009P&SS...57..822G.
↑Wajer, P. (2010). "Dynamical evolution of Earth's quasi-satellites: 2004 GU9 and 2006 FV35". Icarus209 (2): 488–493. doi:10.1016/j.icarus.2010.05.012. Bibcode: 2010Icar..209..488W. https://hal.archives-ouvertes.fr/hal-00676219/file/PEER_stage2_10.1016%2Fj.icarus.2010.05.012.pdf.
External links
MPEC 2006-F58, Minor Planet Electronic Circular
(277810) 2006 FV35 at NeoDyS-2, Near Earth Objects—Dynamic Site
Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
(277810) 2006 FV35 at ESA–space situational awareness