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(5645) 1990 SP
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Eccentric and tumbling asteroid
October 2019
yes
(5645) 1990 SP
#FFC2E0
20 September 1990
R. H. McNaught
Siding Spring Obs.
(5645) 1990 SP
ApolloNEO
4 September 2017 (JD 2458000.5)
0
40.89 yr (14,935 days)
1.8798 AU
0.8302 AU
1.3550 AU
0.3873
1.58 yr (576 days)
339.42°
0.6249 ms / day
13.507°
45.762°
48.178°
0.0537 AU
1.648 km1.65 km (taken)1.668 0.018 km1.849 0.334 km2.20 0.74 km
30.39 0.04 h
0.06 0.080.062 0.0790.068 0.0320.08270.121 0.022
PCXTS
16.75 0.2 (R)16.817.117.20 0.317.24 0.206
(5645) 1990 SP is an eccentric and tumbling asteroid, classified as a near-Earth object of the Apollo group, approximately 1.7 kilometers in diameter. It was discovered on 20 September 1990, by Scottish–Australian astronomer Robert McNaught at the Siding Spring Observatory in Canberra, Australia. Scientists have said that it has a '1 in 364 billion chance' of colliding with the Earth.
Orbit and classification
The asteroid orbits the Sun at a distance of 0.8–1.9 AU once every 1 years and 7 months (576 days). Its orbit has an eccentricity of 0.39 and an inclination of 14° with respect to the ecliptic.
Close approaches
This near-Earth asteroid has an Earth minimum orbit intersection distance of 0.055 AU km on, only slightly above the threshold minimum distance of 19.5 lunar distances (0.05 AU) to make it a potentially hazardous object. It also makes close approaches to Mars. On 14 April 1969, it passed the Red Planet at only 0.013 AU km on 2.
Precovery
Published by the Digitized Sky Survey (DSS), a first precovery was taken at the discovering observatory in 1974, extending the asteroid's observation arc by 16 years prior to its discovery.
Physical characteristics
The stony S-type asteroid is also characterized as a P-type, based on post-cryogenic observations by the Spitzer Space Telescope, while observations at the NASA Infrared Telescope Facility using its SpeX instrument during a follow-up campaign of the Spitzer-observed objects between 2009 and 2012, gave it a C/X/T spectral type.
Rotation
In April 2002, Czech astronomer Petr Pravec obtained a rotational lightcurve from a photometric observations, which gave a relatively long period of 30.39 0.04 hours with a brightness variation of 0.7 in magnitude (U=2). The observations have also shown that the body is most likely in a tumbling motion.
Diameter and albedo
Estimates for the body's diameter range from 1.6 to 2.2 kilometers with an albedo for its surface between 0.06 and 0.12, according to observations made by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and by the Spitzer Space Telescope. The Collaborative Asteroid Lightcurve Link takes the revised WISE data – an albedo of 0.0872 and a diameter of 1.65 kilometers – as the best of all available results.
References
30em 2015-07-04 last obs.
JPL Small-Body Database Browser: 5645 (1990 SP)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2005645
Jet Propulsion Laboratory
26 May 2017
5645 (1990 SP)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=5645
29 June 2016
5645
29 June 2016
6
Michael Mueller
M. Delbo'
J. L. Hora
D. E. Trilling
B. Bhattacharya
W. F. Bottke
S. Chesley
J. P. Emery
G. Fazio
A. W. Harris
A. Mainzer
M. Mommert
B. Penprase
H. A. Smith
T. B. Spahr
J. A. Stansberry
C. A. Thomas
April 2011
ExploreNEOs. III. Physical Characterization of 65 Potential Spacecraft Target Asteroids
The Astronomical Journal
141
4
9
2011AJ....141..109M
10.1088/0004-6256/141/4/109 https://authors.library.caltech.edu/23152/1/Mueller2011p13239Astron_J.pdf
Petr Pravec
Alan W. Harris
Peter Kusnirák
Adrián Galád
Kamil Hornoch
September 2012
Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations
Icarus
221
1
365–387
2012Icar..221..365P
10.1016/j.icarus.2012.07.026 11104/0217021
free
6
A. Mainzer
T. Grav
J. Masiero
J. Bauer
R. M. Cutri
R. S. McMillan
C. R. Nugent
D. Tholen
R. Walker
E. L. Wright
November 2012
Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey
The Astrophysical Journal Letters
760
1
6
2012ApJ...760L..12M
10.1088/2041-8205/760/1/L12
1210.0502 41459166
6
A. Mainzer
T. Grav
J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
J. Watkins
W. Mo
C. Maleszewski
November 2011
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407 118700974
6
P. Pravec
A. W. Harris
P. Scheirich
P. Kusnirák
L. Sarounová
C. W. Hergenrother
S. Mottola
M. D. Hicks
G. Masi
Yu. N. Krugly
V. G. Shevchenko
M. C. Nolan
E. S. Howell
M. Kaasalainen
A. Galád
P. Brown
D. R. DeGraff
J. V. Lambert
W. R. Cooney
S. Foglia
January 2005
Tumbling asteroids
Icarus
173
1
108–131
2005Icar..173..108P
10.1016/j.icarus.2004.07.021
6
C. A. Thomas
D. E. Trilling
J. P. Emery
M. Mueller
J. L. Hora
L. A. M. Benner
B. Bhattacharya
W. F. Bottke
S. Chesley
M. Delbó
G. Fazio
A. W. Harris
A. Mainzer
M. Mommert
A. Morbidelli
B. Penprase
H. A. Smith
T. B. Spahr
J. A. Stansberry
September 2011
ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population
The Astronomical Journal
142
3
12
2011AJ....142...85T
10.1088/0004-6256/142/3/85 free
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
Icarus
228
217–246
2014Icar..228..217T
10.1016/j.icarus.2013.10.004
1310.2000 119278697
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
The Astrophysical Journal
743
2
17
2011ApJ...743..156M
10.1088/0004-637X/743/2/156
1109.6400 239991
External links
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
5645
5645 1990SP
5644 Maureenbell 5645 (5646) 1990 TR
005645
Category:Discoveries by Robert H. McNaught
19900920