(277810) 2006 FV35

(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.

(277810) 2006 FV35
Discovery[1][2]
Discovered bySpacewatch
Discovery siteKitt Peak National Obs.
Discovery date29 March 2006
Designations
(277810) 2006 FV35
2006 FV35
Apollo · NEO[2]
Orbital characteristics[2]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 1
Observation arc21.98 yr (8,029 days)
Aphelion1.3794 AU
Perihelion0.6233 AU
1.0013 AU
Eccentricity0.3775
1.00 yr (366 days)
5.8541°
 59m 0.96s / day
Inclination7.1041°
179.51°
170.85°
Earth MOID0.1047 AU · 40.8 LD
Physical characteristics
Mean diameter
140–320 m[3]
21.8[2] · 21.915[4]

    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]

    gollark: Yep! CC, anyway.
    gollark: Shouldn't you work on the asm2bf target first?
    gollark: It probably can be? It would just be annoying.
    gollark: <@113673208296636420> This is very synchronous code and therefore heretical.
    gollark: PotatOS, for instance, relies on some advanced sandboxing stuff which leans quite heavily on Lua environments.

    See also

    References

    1. "277810 (2006 FV35)". Minor Planet Center. Retrieved 20 January 2018.
    2. "JPL Small-Body Database Browser: 277810 (2006 FV35)" (2017-03-25 last obs.). Jet Propulsion Laboratory. Retrieved 20 January 2018.
    3. Gerhard Hahn. "EARN: 2006 FV35". Archived from the original on 17 May 2009. Retrieved 19 April 2009.
    4. Stacey, R. Greg; Connors, Martin (February 2009). "Delta-v requirements for earth co-orbital rendezvous missions". Icarus. (Proof) (7): 822. Bibcode:2009P&SS...57..822G. doi:10.1016/j.pss.2009.01.013.
    5. Wajer, P. (2010). "Dynamical evolution of Earth's quasi-satellites: 2004 GU9 and 2006 FV35" (PDF). Icarus. 209 (2): 488–493. Bibcode:2010Icar..209..488W. doi:10.1016/j.icarus.2010.05.012.

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