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(192642) 1999 RD32
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Asteroid and suspected contact binary
September 2020
yes
(192642) 1999 RD 32
#FFC2E0
(192642) 1999 RD32.jpg
Goldstone radar image showing the two lobes of suspected contact binary 1999 RD 32.
LINEAR
Lincoln Lab's ETS
8 September 1999
(192642) 1999 RD 32
ApolloNEOPHA
4 September 2017 (JD 2458000.5)
0
21.92 yr (8,007 days)
4.6801 AU
0.6093 AU
2.6447 AU
0.7696
4.30 yr (1,571 days)
89.009°
0.2292 ms / day
6.7914°
310.04°
299.89°
0.0495 AU19.3 LD
0.6702 AU
1.63 km (calculated–dated)5 km (est.–radiometric)
17.08 0.03 hlightcurve-plot-Warner17.1 0.5 h
0.04 (est.–radiometric)0.20 (assumed–dated)
C
16.0016.23 0.0116.3
(192642) 1999 RD 32 is an asteroid and suspected contact binary on an eccentric orbit, classified as a large near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 5 km mi 1 off us in diameter. It was discovered on 8 September 1999, at a magnitude of 18, by astronomers of the LINEAR program using its 1-meter telescope at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, United States. The asteroid is likely of carbonaceous composition and has a rotation period of 17.08 hours.lightcurve-plot-Warner
Description
1999 RD 32 orbits the Sun at a distance of 0.6–4.7 AU once every 4 years and 4 months (1,571 days; semi-major axis of 2.64 AU). Its orbit has a high eccentricity of 0.77 and an inclination of 7° with respect to the ecliptic.
The asteroid's observation arc begins with a precovery taken at Palomar Observatory in January 1995. It is known that 1999 RD 32 passed 0.0093 AU km mi on on from Earth on 27 August 1969. During the 1969 close approach the asteroid reached about apparent magnitude 8.8. The similarly sized 4179 Toutatis also reached that brightness in September 2004. It passed less than 0.007 AU km mi on off from asteroid 29 Amphitrite on 17 January 1939.
Arecibo radar observations on 5–6 March 2012 showed that 1999 RD 32 is approximately 5 km 0 us in diameter and has an estimated albedo of only 0.04. Other sources calculate a smaller diameter of 1.63 kilometers based on a dated assumption, that the object is a stony rather than a carbonaceous asteroid. The two visible lobes suggest that 1999 RD 32 is a tight binary asteroid or contact binary. About 10–15% of near-Earth asteroids larger than 200 meters are expected to be contact binary asteroids with two lobes in mutual contact.
+Close-approaches to Earth Date Distance from Earth 1969-08-27 0.0093 AU km mi on on 2012-03-14 0.1487 AU km mi on off 2042-03-11 0.1428 AU km mi on off 2046-09-04 0.1071 AU km mi on off
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 13 November 2008. As of 2018, it has not been named.
Notes
lightcurve-plot-Warner Lightcurve plot of (192642) 1999 RD32, Palmer Divide Observatory, B. D. Warner (2012): rotation period 17.08 0.03 hours with a brightness amplitude of 0.28 0.02 mag. Summary figures at the LCDB
References
2016-12-04 last obs.
JPL Small-Body Database Browser: 192642 (1999 RD32)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2192642
Jet Propulsion Laboratory
16 January 2018
192642 (1999 RD32)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=192642
16 January 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
24 February 2018
MPEC 1999-R32 : 1999 RD32
IAU Minor Planet Center
1999-09-11
https://minorplanetcenter.net/mpec/J99/J99R32.html
2014-02-28 (J99R32D)
2012-11-03 last obs and observation arc=17.8 years
JPL Close-Approach Data: 192642 (1999 RD32)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1999RD32;cad=1#cad
2014-02-28
12 March 2012
(192642) 1999 RD32 Goldstone Radar Observations Planning
NASA/JPL Asteroid Radar Research
http://echo.jpl.nasa.gov/asteroids/1999RD32/1999RD32_planning.html
16 January 2018
2012-03-12
Near-Earth Asteroids and Radar Speckle Tracking
Michael Busch
http://www.aoc.nrao.edu/events/nmsymposium/2012/talks/Busch_2012_New_Mexico_Symposium.pdf
2014-02-28
1999RD32 Ephemerides for 25 August 1969 through 31 August 1969
NEODyS (Near Earth Objects – Dynamic Site)
http://newton.spacedys.com/neodys/index.php?pc=1.1.3.1&n=192642&oc=500&y0=1969&m0=8&d0=25&h0=0&mi0=0&y1=1969&m1=8&d1=31&h1=0&mi1=0&ti=3.0&tiu=hours
2014-02-28
192642
16 January 2018
Brian D. Warner
Ralph Megna
July 2012
Lightcurve Analysis of NEA (192642) 1999 RD32
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012MPBu...39..154W
The Minor Planet Bulletin
39
3
154
1052-8091
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16 January 2018
6
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August 2017
The EURONEAR Lightcurve Survey of Near Earth Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2017EM&P..120...41V
Earth
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10.1007/s11038-017-9506-9
16 January 2018 10316/80202
free
B. Carry
E. Solano
S. Eggl
F. E. DeMeo
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External links
Arecibo images from 2012
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
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