astro.wikisort.org - Asteroid

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 smallest asteroid in the Solar System with a well-known orbit. 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]

2006 RH₁₂₀

Discovery[1]
Discovered by	Catalina Sky Survey (Eric Christensen)
Discovery date	14 September 2006
Designations
MPC designation	2006 RH120
Minor planet category	Amor (MPC 2013)[2] Apollo (JPL 2012)[3] Aten (2007)[4] (Temporary satellite of Earth 2006–2007)
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)
Semi-major axis	1.0331 AU (154.55 Gm) (a)
Eccentricity	0.02452 (e) (Geocentric hyperbolic e=2500000)[6]
Orbital period (sidereal)	1.05 yr
Mean anomaly	313.7° (M)
Inclination	0.59486° (i)
Longitude of ascending node	51.18° (Ω)
Time of perihelion	~2028-Nov-11
Argument of perihelion	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]
Synodic rotation period	2.75 minutes[8] 0.04583 h (2.750 min)[9]
Geometric albedo	0.1 ?[clarification needed]
Apparent magnitude	30+ (until 2027)
Absolute magnitude (H)	29.5[9]

Discovery

2006 RH₁₂₀ was discovered on 14 September 2006 by Eric Christensen with the 27-inch (690 mm) Schmidt camera of the Catalina Sky Survey in Arizona.[13] "6R10DB9"[13] was the Catalina Sky Survey's own discovery designation for this object, which usually would only be used on the MPC's Near-Earth Object 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".[14] Preliminary orbital calculations indicated it was captured by Earth's gravity from solar orbit of a period of about 12 months,[11] which is similar to that of many spent rocket boosters dating to the Apollo program of the 1960s and early 1970s. 6R10DB was assigned the designation 2006 RH₁₂₀ on 18 February 2008.[1]

Origin

Some controversy existed regarding the origin of the object. Upon discovery, it was not given a formal name because its spectrum was consistent with the white titanium-oxide paint used on Saturn V rockets,[15] which meant it could be 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,[16] and 6Q0B44E, discovered a month earlier, was also thought to be artificial.[17] Its status as a satellite was also debated, with A. W. Harris of the Space Science Institute commenting, "Claiming some bit of fluff in a temporary looping orbit to be a 'satellite', with all the baggage that term carries, is mere hype".[10][18] Radar observations strongly suggest that the object is a natural body.[11]

Orbit

Analysis has shown that solar-radiation pressure is perturbing its motion perceptibly.[19] 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.[19] One hypothesis is that the object is a piece of lunar rock ejected by an impact.[10]

2006 RH₁₂₀ made four Earth orbits of about three months each with perigee (closest approach to Earth) on 11 September 2006, 3 January 2007, 25 March 2007, and 14 June 2007.[9] During the 12-month capture from July 2006 to July 2007 when it was inside of Earth's hill sphere,[11] it stayed within 0.0116 AU (1.74 million km) of Earth.[12] It was ejected after the 14 June 2007 perigee when it dipped inside the Moon's orbit to a distance of 276,840 kilometres (172,020 mi).[8] 2006 RH₁₂₀ became an Apollo-class asteroid in June 2007 as it was escaping Earth's hill sphere. Though it was outside of Earth's hill sphere, the geocentric orbital eccentricity was not greater than 1 until 17 September 2007.[20]

It is now in solar orbit[18] as an Amor-class asteroid[5] with an orbit completely outside of Earth's orbit. As of 2022, this object is 1.7 AU from Earth on the other side of the Sun and will not be less than 1 AU from Earth until March 2025.[21]

Future events

Around 18 August 2028 (±3 days) it will pass Earth with a relative velocity of 136 m/s (300 mph)[9][22] and will then pass Earth with a relative velocity of 784 m/s (1,750 mph) around 9 October 2028 as it speeds up for a November 2028 perihelion passage[23] (closest approach to the Sun and when an object moves fastest in its orbit). For comparison, on 13 April 2029, asteroid 99942 Apophis will pass Earth at a relative speed of 7.4 km/s (17,000 mph).[24]

2006 RH120 has a 1-in-270 (0.37%) chance of Earth impact on 8 February 2044 and would impact with a harmless 1 kiloton of energy if it did impact.[25] (The Chelyabinsk meteor released about 440 kt of energy.) JPL Horizon's nominal orbit has the asteroid passing 0.0069 AU (1.03 million km) from Earth on 29 January 2044 (10 days before the virtual impactor).[26] As a result of a 281 day observation arc and radar observations, JPL's solution accounts for non-gravitational forces[9] as the multi-decade motion of a very small object is greatly affected by solar heating.

2044 Virtual impactor[25]

Date	Impact probability (1 in)	JPL Horizons nominal geocentric distance (AU)	NEODyS nominal geocentric distance (AU)	MPC[27] nominal geocentric distance (AU)	Find_Orb nominal geocentric distance (AU)	uncertainty region (3-sigma)
2044-02-08 09:07	270	0.00776 AU (1.161 million km)[28]	0.223 AU (33.4 million km)[29]	0.253 AU (37.8 million km)	0.229 AU (34.3 million km)[30]	± 78 million km[28]

14 June 2007 perigee

On 14 June 2007, 2006 RH₁₂₀ made its fourth and last perigee of the most recent Earth encounter.[9] It was 0.72 lunar distances at closest, with an apparent magnitude of 18.5–19.0. Astronomers at JPL Goldstone in California made radar astrometry measurements on 12, 14 and 17 June 2007.

2006 RH₁₂₀ is listed as part of the Near-Earth Object Human Space Flight Accessible Targets Study (NHATS).[31]

See also

• 1991 VG – temporary Earth satellite discovered in 1991
• 2020 CD3 – another temporary Earth satellite discovered in 2020
• 6Q0B44E – small Earth satellite, probably artificial
• 3753 Cruithne – horseshoe companion of the Earth
• 2002 AA29 – horseshoe companion of the Earth
• (419624) 2010 SO16 – horseshoe companion of the Earth
• Natural satellite
• Claimed moons of Earth
• Quasi-satellite
• Space debris

References

External links

• Great Shefford Observatory's 6R10DB9 images and background
• Earth's "Other Moon", Roger W. Sinnott, Sky & Telescope, 17 April 2007
• JPL Radar Astrometry Page
• Bill Gray's Pseudo-MPEC Page on 6R10DB9
• Photometry of 2006 RH120: an asteroid temporarily captured into a geocentric orbit (Astronomy & Astrophysics 2009)
• Interactive 3D visualisation of the Earth 2006 RH120 capture event
• 2006 RH120 at NeoDyS-2, Near Earth Objects—Dynamic Site
  • Ephemerides · Observation prediction · Orbital info · MOID · Proper elements · Observational info · Close approaches · Physical info · Orbit animation
• 2006 RH120 at ESA–space situational awareness
  • Ephemerides · Observations · Orbit · Physical properties · Summary
• 2006 RH120 at the JPL Small-Body Database
  • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

На других языках

---

[de] 2006 RH120

2006 RH120 ist ein interplanetares Objekt von wenigen Metern Größe, das zwischen September 2006 und Juni 2007 temporär vom Gravitationspotential der Erde eingefangen wurde und diese dabei viermal umrundete. Gegenwärtig befindet sich 2006 RH120 in einer Umlaufbahn um die Sonne. Seine Bahn bringt das Objekt dabei immer wieder in Erdnähe, wobei es auch in Zukunft wieder zu einem temporären Einfangen kommen könnte.

---

- [en] 2006 RH120

---

[es] 2006 RH120

2006 RH120 es un pequeño asteroide cercano a la Tierra con un diámetro de dos a tres metros que orbita el Sol, sin embargo, periódicamente se acerca al sistema Tierra-Luna aproximadamente cada veinte años, con lo cual puede entrar temporalmente en la órbita terrestre a través de la captura de satélite temporal (TSC). Recientemente, estuvo en la órbita terrestre entre septiembre de 2006 y junio de 2007.

---

[ru] 2006 RH120

2006 RH120 — маленький околоземный астероид[1] диаметром около 2—3 метров[4], который обычно обращается вокруг Солнца, но приближается к системе Земля — Луна примерно каждые 20 лет[5]. Время от времени объект переходит на геоцентрическую орбиту. В период такого временного захвата спутника этот метеороид становится единственным известным естественным спутником Земли помимо Луны. В то же время Алан Харрис из Space Science Institute отмечает, что «называть кусок мусора на временной циклической орбите „спутником“, учитывая всю смысловую нагрузку данного термина, — это всего лишь преувеличение»[5][6].

---

---