Discovery[1] | |
---|---|
Discovered by | Catalina Sky Survey (Eric Christensen) |
Discovery date | 14 September 2006 |
Designations | |
2006 RH120 | |
Orbital characteristics[5] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 1 | |
Observation arc | 281 days |
Aphelion | 1.058 AU (158.3 Gm) (Q) |
Perihelion | 1.0078 AU (150.76 Gm) (q) |
1.0331 AU (154.55 Gm) (a) | |
Eccentricity | 0.02452 (e) (Geocentric hyperbolic e=2500000)[6] |
1.05 yr | |
313.7° (M) | |
Inclination | 0.59486° (i) |
51.18° (Ω) | |
~2028-Nov-11 | |
10.060° (ω) | |
Earth MOID | 0.01682 AU (2,516,000 km) |
Jupiter MOID | 3.93 AU (588 Gm) |
Physical characteristics | |
Dimensions | ~2–3 m[7] |
0.1 ?[clarification needed] | |
30+ (until 2027) | |
29.5[9] | |
2006 RH120 is a tiny near-Earth asteroid[9] and fast rotator with a diameter of approximately 2–3 meters[7] that ordinarily orbits the Sun but makes close approaches to the Earth–Moon system around every twenty years,[10] when it can temporarily enter Earth orbit through temporary satellite capture (TSC). Most recently, it was in Earth orbit from July 2006 to July 2007,[11] during which time it was never more than 0.0116 AU (1.74 million km) from Earth.[12] As a consequence of its temporary orbit around the Earth, it is currently the second smallest asteroid in the Solar System with a well-known orbit, after 2021 GM1. Until given a minor planet designation on 18 February 2008,[1] the object was known as 6R10DB9, an internal identification number assigned by the Catalina Sky Survey.[8]
MPEC2008-D12
was invoked but never defined (see the help page).mpc
was invoked but never defined (see the help page).geocentric
was invoked but never defined (see the help page).Barbee2015
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).Pseudo-MPEC
was invoked but never defined (see the help page).Kwiatkowski2009
was invoked but never defined (see the help page).Horizons2006-2007
was invoked but never defined (see the help page).