2006 RH120

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2006 RH120
Currently in a heliocentric orbit with perihelion > 1 AU[1]
Discovered by Catalina Sky Survey (703)
Discovery date 14 September 2006
MPC designation 2006 RH120
Amor (2013)[1]
Apollo (2012)
Aten (2007)[3]
Orbital characteristics[3]
Epoch 4 January 2010 (2455200.5)
Aphelion 1.058 AU (Q)
Perihelion 1.007 AU (q)
1.033 AU (a)
Eccentricity 0.0244
1.05 yr
2.913° (M)
Inclination 0.5955°
Physical characteristics
Dimensions ~2–3 metres[4]
2.75 minutes[5]
Albedo 0.1 ?

2006 RH120 is a tiny near-Earth asteroid[3] with a diameter of about 2–3 meters[4] that ordinarily orbits the Sun but makes close approaches to the Earth–Moon system every twenty years or so,[6] when it can temporarily enter Earth orbit through temporary satellite capture (TSC). Most recently it was in Earth orbit from September 2006 to June 2007.[7]

Until given a minor planet designation on 18 February 2008,[2] the object was known as 6R10DB9, an internal identification number assigned by the Catalina Sky Survey.[5]


2006 RH120 was discovered on 14 September 2006 by the 27-inch (690 mm) Schmidt camera of the Catalina Sky Survey in Arizona.[8] "6R10DB9"[8] was the Catalina Sky Survey's own discovery designation for this object, which usually would only be used on the MPC's NEO Confirmation Page (NEOCP) until an IAU designation was applied, if the object was classified as a minor object. It was added on 14 September to the NEOCP and subsequently removed with the explanation that it "was not a minor planet."[9] Preliminary orbital calculations indicated it was captured by Earth's gravity from solar orbit of a period of about 11 months, which is similar to that of many spent rocket boosters dating to the Apollo program of the 1960s and early 1970s.

Some controversy existed regarding the origin of the object. Upon discovery, it was not given a formal name since its size, orbit and spectrum – consistent with the white titanium oxide paint used on Saturn V rockets[10] – suggested it might have been an artificial object. Precedents for this exist: J002E3 is currently thought to be the third stage Saturn S-IVB booster from Apollo 12 and was in an almost identical orbit,[11] and 6Q0B44E, discovered a month earlier, was also thought to be artificial.[12] Its status as satellite was also debated, with A. W. Harris of the Space Science Institute comments, "Claiming some bit of fluff in a temporary looping orbit to be a ‘satellite,’ with all the baggage that term carries, is mere hype".[6][13]

Analysis has shown that solar-radiation pressure is perturbing its motion perceptibly.[14] However, Paul Chodas in JPL's Solar System Dynamics Group suspects that the perturbations are consistent with expectations for a rocky object but not with old flight hardware.[14] One hypothesis is that the object is a piece of lunar rock ejected by an impact.[6] On 18 February 2008, the object was given a minor planet designation.[2]

The object made four Earth orbits of about three months each before being ejected after the June 2007 perigee. At that perigee, it dipped inside the Moon's orbit to a distance of 276,845 kilometres (172,024 mi).[5] 2006 RH120 became an Apollo-class asteroid in June 2007.

14 June 2007 perigee[edit]

On 14 June 2007, 2006 RH120 made its fourth and last perigee of the most recent Earth encounter.[15] It was 0.7 lunar distances at closest, with an apparent magnitude of 18.5–19.0.

Astronomers at JPL Goldstone in California, USA made radar astrometry measurements on 12, 14 and 17 June 2007.

The object is now in solar orbit.[13] By 2017, this object will likely be 2 AU from Earth on the other side of the Sun.[16] Systematic residuals in the positions of the object probably indicate that the model used to determine solar radiation pressure may be too simple to adequately describe its motion over a long period of time.[5] The next predicted near-Earth encounter is in 2028.[5][15]

See also[edit]

References and footnotes[edit]

  1. ^ a b "2006 RH120 Orbit". Minor Planet Center. Retrieved 2014-02-24. 
  2. ^ a b c Williams, Gareth V (18 February 2008). "MPEC 2008-D12 : 2006 RH120". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Archived from the original on 9 April 2010. Retrieved 26 February 2010. 
  3. ^ a b c d "JPL Small-Body Database Browser: (2006 RH120)" (last observation: 2007-06-22; arc: 281 days). Retrieved 26 February 2010. 
  4. ^ a b Brent W. Barbee. "Accessible Near-Earth Objects (NEOs)". 12th Meeting of the Small Bodies Assessment Group (SBAG) 2015. Retrieved 2015-01-12.  (pg 17 for diameter)
  5. ^ a b c d e Great Shefford Observatory. "2006 RH120 ( = 6R10DB9) – A second moon for the Earth?". Archived from the original on 9 May 2008. Retrieved 16 April 2008. 
  6. ^ a b c Bill Gray. "Pseudo-MPEC for 6R10DB9". Archived from the original on 27 September 2007. Retrieved 16 August 2007. 
  7. ^ I. Klotz - Mystery Mini Moons: How Many Does Earth Have? (2012) - Discovery News
  8. ^ a b "Distant Artificial Satellites Observation (DASO) Circular No. 68, 2006 Sept. 17, 16:59 UT". Retrieved 26 June 2007. 
  9. ^ "Major News About Minor Objects, April 18, 2007". Retrieved 27 June 2007. 
  10. ^ Spectrum measured by Carl Hergenrother and Rob Whitely of the University of Arizona.
  11. ^ Yeomans, Don (April 2010). "Is Another Moon Possible?". Astronomy. 
  12. ^ The Guardian, Spacewatch, 6 September 2006
  13. ^ a b Roger W. Sinnott (17 April 2007). "Earth's "Other Moon"". Sky & Telescope. Retrieved 25 February 2010. 
  14. ^ a b Dr. Lance A. M. Benner (20 June 2007). "6R10DB9 Planning". JPL/NASA Asteroid Radar Research. Retrieved 27 February 2010. 
  15. ^ a b "JPL Close-Approach Data: (2006 RH120)" (last observation: 2007-06-22; arc: 281 days). Retrieved 27 February 2010. 
  16. ^ Donald K. Yeomans and Alan B. Chamberlin. "Horizons Ephemeris". JPL Solar System Dynamics. Retrieved 25 February 2010. 

External links[edit]