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(153201) 2000 WO107
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Sub-kilometer asteroid
October 2019
yes
(153201) 2000 WO 107
#FFC2E0
2000WO107-20201128.jpg
Goldstone radar images showing the two lobes of contact binary 2000 WO 107.
LINEAR
Lincoln Lab's ETS
29 November 2000
(153201) 2000 WO 107
AtenNEOPHA
2020-May-31 (JD 2459000.5)
0
20.0 yr (7,304 days)
1.6231 AU
0.2000 AU
13 October 2020
0.9115 AU
0.7807
0.87 yr (318 days)
206.45°
1.1327 ms / day
7.7703°
69.252°
213.72°
0.0031 AU e3km LD unit on
0.510 0.083 km
4.8 hours
0.129 0.058
SMASS X
19.3
(153201) 2000 WO 107 is a sub-kilometer asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. It is a contact binary.
Orbit
The orbit of this potentially hazardous asteroid (PHA) has been well-established with 20 years of observations. It orbits from inside the orbit of Mercury out to the orbit of Mars. It makes close approaches to all of the inner planets.
2020
The asteroid came to perihelion on 13 October 2020 when it passed the Sun going 88 km/s km/h off us.speed The asteroid was not more than 60 degrees from the Sun until 26 November 2020 and was observed by Goldstone radar on 27 November 2020. On 29 November 2020 the asteroid passed 0.02876 AU e6km LD unit on from Earth. Even the 2018 orbit solution had a known accuracy of roughly ±150 km for the close approach. With the radar observations the close approach distance is known with an accuracy of roughly ±5 km.
2140
This asteroid will pass 0.00162 AU e3km LD unit on from Earth on 1 December 2140. The 2140 close approach distance is known with an accuracy of roughly ±1000 km. For comparison, the distance to the Moon is about 0.0026 AU (384,400 km).
The Jupiter Tisserand invariant, used to distinguish different kinds of orbits, is 6.228.
Physical characteristics
In the SMASS classification, the object's spectral type is that of an X-type. According to the space-based survey by NASA's NEOWISE mission, the asteroid measures 510 meters in diameter and its surface has an albedo of 0.129.
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 2 April 2007. As of 2018, it has not been named.
__NOTOC__
See also
2002 NY 40
2014 HQ 124
(388188) 2006 DP 14
(53319) 1999 JM 8
Notes
speed v = 42.1219 1/r − 0.5/a, where r is the distance from the Sun, and a is the major semi-axis. Objects move fastest at perihelion and slowest at aphelion.
References
30em 2020-11-28 last obs.
JPL Small-Body Database Browser: 153201 (2000 WO107)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2153201;cad=1
Jet Propulsion Laboratory
https://web.archive.org/web/20201106120852/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2153201;cad=1
2020-11-06 live
29 November 2020
153201 (2000 WO107)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=153201
13 January 2018
Goldstone Radar Observations Planning: (7753) 1988 XB, 2017 WJ16, and 2000 WO107
Asteroid Radar Research
https://echo.jpl.nasa.gov/asteroids/1988XB/1988xb.2020.goldstone.planning.html
29 November 2020
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
24 February 2018
6
A. Mainzer
T. Grav
J. Bauer
J. Masiero
R. S. McMillan
R. M. Cutri
R. Walker
E. Wright
P. Eisenhardt
D. J. Tholen
T. Spahr
R. Jedicke
L. Denneau
E. DeBaun
D. Elsbury
T. Gautier
S. Gomillion
E. Hand
W. Mo
J. Watkins
A. Wilkins
G. L. Bryngelson
A. Del Pino Molina
S. Desai
M. Gómez Camus
S. L. Hidalgo
I. Konstantopoulos
J. A. Larsen
C. Maleszewski
M. A. Malkan
J.-C. Mauduit
B. L. Mullan
E. W. Olszewski
J. Pforr
A. Saro
J. V. Scotti
L. H. Wasserman
December 2011
NEOWISE Observations of Near-Earth Objects: Preliminary Results
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...743..156M
The Astrophysical Journal
743
2
17
2011ApJ...743..156M
10.1088/0004-637X/743/2/156
1109.6400
13 January 2018
Richard P. Binzel Andrew S. Rivkin J. Scott Stuart Alan W. Harris Schelte J. Bus Thomas H. Burbine Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes http://www.mtholyoke.edu/~tburbine/binzel.icarus.2004.pdf Icarus 170 2 20 March 2004 259–294 2004Icar..170..259B 10.1016/j.icarus.2004.04.004 October 2026 InternetArchiveBot
External links
List Of The Potentially Hazardous Asteroids (PHAs), Minor Planet Center
153201
153201 2000WO107
2007 UW 1
Large NEO Earth close approach(inside the orbit of the Moon) 1 December 2140
(85640) 1998 OX 4
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