Astronomy:4082 Swann

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4082 Swann
Discovery [1]
Discovered byC. Shoemaker
Discovery sitePalomar Obs.
Discovery date27 September 1984
Designations
(4082) Swann
Named afterGordon Swann
(American geologist)[2]
1984 SW3 · 1947 UF
1969 PE
Minor planet categorymain-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc69.54 yr (25,399 days)
|{{{apsis}}}|helion}}3.0076 AU
|{{{apsis}}}|helion}}1.7721 AU
2.3899 AU
Eccentricity0.2585
Orbital period3.69 yr (1,349 days)
Mean anomaly317.29°
Mean motion0° 16m 0.48s / day
Inclination9.5978°
Longitude of ascending node294.36°
100.28°
Physical characteristics
Dimensions5.85 km (derived)[3]
9.535±0.066 km[4]
11.06±0.29 km[5]
Rotation period4.03632±0.00009 h[lower-alpha 1]
4.1±0.1 h[6]
Geometric albedo0.029±0.012[4]
0.101±0.006[5]
0.20 (assumed)[3]
SMASS = Ch [1] · C[3]
Absolute magnitude (H)12.90[5] · 13.08±0.2 (R)[lower-alpha 1] · 13.4[1] · 13.46±0.206[3][7] · 13.58±0.27[8] · 14.55[4]


4082 Swann, provisional designation 1984 SW3, is a carbonaceous asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter.

The asteroid was discovered on 27 September 1984, by American astronomer Carolyn Shoemaker at Palomar Observatory in California, United States, and later named for American geologist Gordon Swann.[2][9]

Orbit and classification

Swann orbits the Sun in the inner main-belt at a distance of 1.8–3.0 AU once every 3 years and 8 months (1,349 days). Its orbit has an eccentricity of 0.26 and an inclination of 10° with respect to the ecliptic.[1] First identified as 1947UF at the Finnish Turku Observatory in 1947, Swann's observation arc was extended by 37 years prior to its official discovery observation at Palomar.[9]

Physical characteristics

The C-type asteroid is classified as a Ch-subtype in the SMASS taxonomy.[1]

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Swann measures 9.5 and 11.1 kilometers in diameter and its surface has an albedo of 0.029 and 0.101, respectively.[4][5] The Collaborative Asteroid Lightcurve Link, however, assumes a standard albedo for stony asteroids of 0.20 and derives a much smaller diameter of 5.85 kilometers, based on an absolute magnitude of 13.46.[3]

Rotation period

In July 2006, a rotational lightcurve of Swann was obtained from photometric observations by Petr Pravec at the Ondřejov Observatory in the Czech Republic. It gave a rotation period of 4.03632±0.00009 hours with a brightness variation of 0.67 magnitude ({{{1}}}).[lower-alpha 1] A second lightcurve obtained by Jean-Gabriel Bosch in September 2006, gave a period of 4.1±0.1 hours and an amplitude of 0.35 magnitude ({{{1}}}).[6]

Naming

This minor planet was named after American geologist Gordon A. Swann (born 1931). He served as the principal investigator of the "Apollo Lunar Geologic Experiment" conducted at the lunar landing sites of Apollo 14 and Apollo 15.[2] The official naming citation was published by the Minor Planet Center on 12 December 1989 (M.P.C. 15576).[10]

Notes

  1. 1.0 1.1 1.2 Pravec (2006) web: rotation period of 4.03632±0.00009 hours with a brightness amplitude of 0.67 mag. Summary figures for (4082) Swann at Collaborative Asteroid Lightcurve Link (CALL) and Pravec, P.; Wolf, M.; Sarounova, L. (2006)

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 "JPL Small-Body Database Browser: 4082 Swann (1984 SW3)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004082. 
  2. 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(4082) Swann". Dictionary of Minor Planet Names – (4082) Swann. Springer Berlin Heidelberg. p. 348. doi:10.1007/978-3-540-29925-7_4060. ISBN 978-3-540-00238-3. 
  3. 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (4082) Swann". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=4082%7CSwann. 
  4. 4.0 4.1 4.2 4.3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C. et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. doi:10.1088/2041-8205/759/1/L8. Bibcode2012ApJ...759L...8M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 30 October 2016. 
  5. 5.0 5.1 5.2 5.3 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan 63 (5): 1117–1138. doi:10.1093/pasj/63.5.1117. Bibcode2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  6. 6.0 6.1 Behrend, Raoul. "Asteroids and comets rotation curves – (4082) Swann". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#004082. 
  7. Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus 221 (1): 365–387. doi:10.1016/j.icarus.2012.07.026. Bibcode2012Icar..221..365P. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012Icar..221..365P. Retrieved 17 December 2015. 
  8. Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus 261: 34–47. doi:10.1016/j.icarus.2015.08.007. Bibcode2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 30 October 2016. 
  9. 9.0 9.1 "4082 Swann (1984 SW3)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=4082. 
  10. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 

External links