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2004 Lexell
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Florian asteroid
October 2019
yes
2004 Lexell
#D6D6D6
22 September 1973
N. Chernykh
Crimean Astrophysical Obs.
(2004) Lexell
1973 SV 21938 WL1941 SN 11959 GC1972 HK
Anders Johan Lexell(Swedish-Russian astronomer)
main-beltFlora
4 September 2017 (JD 2458000.5)
0
78.55 yr (28,689 days)
2.3451 AU
1.9986 AU
2.1718 AU
0.0798
3.20 yr (1,169 days)
215.94°
0.3079 ms / day
2.4967°
4.5440°
58.504°
7.255 0.216 km7.456 0.084 km7.82 km (calculated)14.7 km
5.44 0.02 h5.441 0.002 h5.4429 0.0003 h
0.0560.24 (assumed)0.2908 0.05220.306 0.041
LSS
12.612.712.908 0.06413.04 0.00
2004 Lexell, provisional designation 1973 SV 2, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7.5 kilometers in diameter. The asteroid was discovered on 22 September 1973, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named for Swedish-Russian astronomer and mathematician Anders Johan Lexell.
Classification and orbit
Lexell is a member of the Flora family, one of the largest collisional populations of stony asteroids. It orbits the Sun at a distance of 2.0–2.3 AU once every 3 years and 2 months (1,169 days). Its orbit has an eccentricity of 0.08 and an inclination of 2° with respect to the ecliptic.
The asteroid was first identified as 1938 WL at the Finnish Turku Observatory in November 1938, extending the body's observation arc by 35 years prior to its official discovery observation at Nauchnij.
Physical characteristics
Pan-STARRS photometric survey characterized Lexell as a LS-type asteroid, which transitions between the common S-type and rare L-type asteroid.
Rotation period
In March 2013, two rotational lightcurves of Lexell were obtained from photometric observations by Gary Haagen at Stonegate Observatory, Massachusetts, and by a group of astronomers at the Oakley Southern Sky Observatory (E09), Australia. Lightcurve analysis gave a well-defined rotation period of 5.441 and 5.4429 hours with a brightness variation of 0.45 and 0.42 magnitude, respectively (U=3/3).
In February 2013, observations made by French amateur astronomer Pierre Antonini gave a concurring period of 5.44 hours with an amplitude of 0.51 magnitude (U=3-).
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lexell measures 7.255 and 7.456 kilometers in diameter and its surface has an albedo of 0.306 and 0.2908, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 7.82 kilometers based on an absolute magnitude of 12.7.
Naming
This minor planet was named after Anders Johan Lexell (1740–1784), a Swedish-Russian astronomer and mathematician. The official 2004 naming citation was published by the Minor Planet Center on 15 October 1977 (M.P.C. 4238). The lunar crater Lexell was also named in his honor, as is Lexell's Comet, of which he computed its orbit.
References
30em 2017-06-03 last obs.
JPL Small-Body Database Browser: 2004 Lexell (1973 SV2)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002004
Jet Propulsion Laboratory
29 June 2017
Dictionary of Minor Planet Names – (2004) Lexell
Schmadel Lutz D.
Springer Berlin Heidelberg
162
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_2005 (2004) Lexell
2004 Lexell (1973 SV2)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=2004
29 June 2017
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
Springer Berlin Heidelberg
221
978-3-642-01964-7
10.1007/978-3-642-01965-4
Asteroids and comets rotation curves – (2004) Lexell
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#002004
29 June 2017
3 August 2003
https://web.archive.org/web/20030803183423/http://obswww.unige.ch/~behrend/page4cou.html#002004
dead
6
Joseph R. Masiero
T. Grav
A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
August 2014
Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
29 June 2017
2004
29 June 2017
Vander Haagen, Gary A.
October 2010
Lightcurve and H-G Parameters for 2004 Lexell
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37..137V
The Minor Planet Bulletin
37
4
137–138
1052-8091
2010MPBu...37..137V
29 June 2017
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
6
Kenda Albers
Katherine Kragh
Adam Monnier
Zachary Pligge
Kellen Stolze
Josh West
Arnold Yim
Richard Ditteon
October 2010
Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2009 October thru 2010 April
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37..152A
The Minor Planet Bulletin
37
4
152–158
1052-8091
2010MPBu...37..152A
29 June 2017
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
29 June 2017
External links
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
2004
2003 Harding 2004 2005 Hencke
002004
Category:Discoveries by Nikolai Chernykh
Category:Named minor planets
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