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(136617) 1994 CC
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Near-Earth asteroid
September 2020
yes
(136617) 1994 CC
#FFC2E0
1994CC-with-moons.gif
Goldstone animation of 1994 CC orbited by two minor-planet moons in 2009 padding: 5px 0;
3 February 1994
Spacewatch
Kitt Peak National Obs.
(136617) 1994 CC
NEOPHAApolloEarth-crosser
4 September 2017 (JD 2458000.5)
0
28.45 yr (10,391 days)
2.3206 AU
0.9551 AU
1.6378 AU
0.4169
2.10 yr (766 days)
321.07°
0.4702 ms / day
4.6806°
268.55°
24.842°
0.0157 AU6.1 LD
2
0.62 0.06 km0.650 km
2.69 0.329 11 kg (system mass) Wm. Robert Johnston (136617) 1994 CC, "Beta", and "Gamma" Johnston's Archive 21 September 2014 http://www.johnstonsarchive.net/astro/astmoons/am-136617.html 9 June 2019
2.5935 0.1315 11 kg (primary)Fang Julia Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution 2011AJ....141..154F Astronomical Journal 131 5 154 May 2011 10.1088/0004-6256/141/5/154 1012.2154v2
2.1 0.6 g/cm3 (system)
1.98 g/cm3 (primary)9
2.3886 0.0001 h2.38860 0.00009 h
0.3821 (derived)0.42 0.1
SqSaS
17.0017.718.12 0.84
(136617) 1994 CC is a sub-kilometer triple asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group.
Discovery
1994 CC 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 (153591) 2001 SN 263, which was discovered to be a triple system in 2008, and 3122 Florence, which was found to be a triple system in 2017.
Observations
thumb|left|Radar images of 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 1994 CC 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, 1994 CC 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 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 1994 CC's orbital and physical properties further.
The next similar Earth flyby for the asteroid 1994 CC 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.
Name Mass[109 kg] Semi-major axis[km] Orbital period[days] Eccentricity Inclination(relative to asteroid)[°] Beta 5.8 0.3 0.5 1.729 0.008 1.243 0.0329 0.002 0.015 83.376 11.158 Gamma 0.911 2.0 0.9 6.130 0.108 8.376 0.404 0.192 0.014 71.709 8.994
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 5 December 2006. 2019, it has not been named.
See also
List of exceptional asteroids
2004 FH
87 Sylvia
433 Eros
(153591) 2001 SN 263
References
30em 2017-02-25 last obs.
JPL Small-Body Database Browser: 136617 (1994 CC)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2136617
Jet Propulsion Laboratory
1 June 2017
136617 (1994 CC)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=136617
22 March 2017
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
24 February 2018
Triple Asteroid System Triples Observers' Interest
6 August 2009
NASA
http://www.nasa.gov/topics/solarsystem/features/neo20090806.html
Radar imaging at NASA's Goldstone Solar System Radar [..] revealed that near-Earth asteroid 1994 CC is a triple system
22 March 2017
8 November 2010
https://web.archive.org/web/20101108232812/http://www.nasa.gov/topics/solarsystem/features/neo20090806.html
dead
136617
22 March 2017
6
M. Brozovic
L. A. M. Benner
M. C. Nolan
E. S. Howell Ellen Howell
C. Magri
J. D. Giorgini
P. A. Taylor
J. L. Margot
M. W. Busch
M. K. Shepard
L. M. Carter
J. S. Jao
J. van Brimmer
C. R. Franck
M. A. Silva
M. A. Kodis
D. T. Kelley
M. A. Slade
A. Bramson
K. J. Lawrence
J. T. Pollock
P. Pravec
D. E. Reichart
K. M. Ivarsen
J. Haislip
M. C. Nysewander
A. P. Lacluyze
June 2009
(136617) 1994 CC
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009IAUC.9053....2B
IAU Circ.
9053
2009IAUC.9053....2B
22 March 2017
6
Marina Brozovic
Lance A. M. Benner
Patrick A. Taylor
Michael C. Nolan
Ellen S. Howell Ellen Howell
Christopher Magri
Daniel J. Scheeres
Jon D. Giorgini
Joseph T. Pollock
Petr Pravec
Adrián Galád
Julia Fang
Jean-Luc Margot
Michael W. Busch
Michael K. Shepard
Daniel E. Reichart
Kevin M. Ivarsen
Joshua B. Haislip
Aaron P. LaCluyze
Joseph Jao
Martin A. Slade
Kenneth J. Lawrence
Michael D. Hicks
November 2011
Radar and optical observations and physical modeling of triple near-Earth Asteroid (136617) 1994 CC
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011Icar..216..241B
Icarus
216
1
241–256
2011Icar..216..241B
10.1016/j.icarus.2011.09.002
1310.2000
22 March 2017
Cristina A. Thomas
Joshua P. Emery
David E. Trilling
Marco Delbó
Joseph L. Hora
Michael Mueller
January 2014
Physical characterization of Warm Spitzer-observed near-Earth objects
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014Icar..228..217T
Icarus
228
217–246
2014Icar..228..217T
10.1016/j.icarus.2013.10.004
22 March 2017 1310.2000
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
22 March 2017
B. Carry
E. Solano
S. Eggl
F. E. DeMeo
April 2016
Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016Icar..268..340C
Icarus
268
340–354
2016Icar..268..340C
10.1016/j.icarus.2015.12.047
1601.02087
22 March 2017
External links
Spacewatch Discoveries for 1994, Spacewatch NEO Detections by Year, University of Arizona
Official press release by NASA on triplet system https://web.archive.org/web/20101108232812/http://www.nasa.gov/topics/solarsystem/features/neo20090806.html 8 November 2010
(136617) 1994 CC compiled by Wm. Robert Johnston
Julia Fang, "Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution",
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