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(136617) 1994 CC

Near-Earth asteroid

(136617) 1994 CC

Near-Earth asteroid

FieldValue
minorplanetyes
name(136617) 1994 CC
background#FFC2E0
image1994CC-with-moons.gif
caption
discovery_ref
discovered3 February 1994
discovererSpacewatch
discovery_siteKitt Peak National Obs.
mpc_name(136617) 1994 CC
alt_names1994 CC
named_after
mp_categoryNEOPHAApollo
Earth-crosser
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc28.45 yr (10,391 days)
aphelion2.3206 AU
perihelion0.9551 AU
semimajor1.6378 AU
eccentricity0.4169
period2.10 yr (766 days)
mean_anomaly321.07°
mean_motion/ day
inclination4.6806°
asc_node268.55°
arg_peri24.842°
moid0.0157 AU6.1 LD
satellites2
mean_diameterkm
km
rotationh
h
albedo0.3821 (derived)
spectral_typeSqSaS
abs_magnitude17.0017.7

Earth-crosser km h

**** is a sub-kilometer triple asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group.

Discovery

was discovered by Spacewatch's Jim Scotti at Kitt Peak National Observatory on 3 February 1994. In June 2009 it was shown to be a triple system, i.e. the largest body is orbited by two satellites; only about one percent (1%) of near-Earth asteroids observed by a radar are found to be triple systems such as this one. The only other unambiguously identified triple asteroids in the near-Earth population are , which was discovered to be a triple system in 2008, and 3122 Florence, which was found to be a triple system in 2017.

Observations

1994 CC}} at two different times with its two moons

A team of NASA's Jet Propulsion Laboratory (JPL) (Pasadena, California) scientists led by Marina Brozovic and Lance Benner, made the discovery using radar imaging at NASA's Goldstone Solar System Radar on June 12 and June 14, 2009. They showed that the near-Earth asteroid is a triple system, which encountered Earth within 2.52 million kilometers on June 10, 2009. This relatively close approach to Earth made the discovery possible, as before the approach, scientists knew very little about this asteroid. In fact, is only the second triple system known in the near-Earth objects population.

1994 CC consists of a central object about 700 meters in diameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the detection of all three objects. The scientists plan to use the combined observations from the Goldstone and Arecibo observatories to study 's orbital and physical properties further.

The next similar Earth flyby for the asteroid will happen in 2074 when the triple system is projected to fly past Earth at a distance of 2.5 million kilometers.

Orbital characteristics of satellites

The orbital properties of the satellites are listed in this table. The orbital planes of both satellites are inclined relative to each other, by approximately 16°. Such a large inclination is suggestive of past evolutionary events (e.g. close encounter with a terrestrial planet, mean-motion resonance crossing) that may have excited their orbits from a coplanar configuration to an inclined state.

NameMass
[109 kg]Semi-major axis
[km]Orbital period
[days]EccentricityInclination
(relative to asteroid)
[°]
Beta~61.71.2430.00295
Gamma~16.18.3760.19279

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 5 December 2006. , it has not been named.

References

References

  1. Fang, Julia. (May 2011). "Orbits of Near-Earth Asteroid Triples 2001 SN263 and {{mp". Astronomical Journal.
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