Astronomy:1312 Vassar

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Short description: Carbonaceous Alauda asteroid
1312 Vassar
001312-asteroid shape model (1312) Vassar.png
Modelled shape of Vassar from its lightcurve
Discovery[1]
Discovered byG. van Biesbroeck
Discovery siteYerkes Obs.
Discovery date27 July 1933
Designations
(1312) Vassar
Named afterVassar College
(Vassar Observatory)[2]
1933 OT · 1944 QE
A908 CD
Minor planet categorymain-belt · (outer)[3]
Alauda[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.67 yr (30,562 days)
|{{{apsis}}}|helion}}3.7605 AU
|{{{apsis}}}|helion}}2.4268 AU
3.0937 AU
Eccentricity0.2156
Orbital period5.44 yr (1,988 days)
Mean anomaly104.98°
Mean motion0° 10m 51.96s / day
Inclination21.901°
Longitude of ascending node129.45°
261.33°
Physical characteristics
Dimensions27.56±6.84 km[5]
32.70±1.29 km[6]
36.28±1.1 km (IRAS:6)[7]
36.32 km (derived)[3]
Rotation period7.93189±0.00001 h[8]
7.93190±0.00005 h[9]
7.932±0.002 h[lower-alpha 1]
Geometric albedo0.0643±0.004 (IRAS:6)[7]
0.0703 (derived)[3]
0.081±0.007[6]
0.09±0.07[5]
C[3]
Absolute magnitude (H)10.68[5] · 10.7[1][3] · 10.76±0.44[10] · 10.80[6]


1312 Vassar, provisional designation 1933 OT, is a carbonaceous Alauda asteroid from the outer region of the asteroid belt, approximately 30 kilometers in diameter. It was discovered on 27 July 1933, by Belgian–American astronomer George Van Biesbroeck at Yerkes Observatory in Wisconsin, United States.[11] The asteroid was named for the American Vassar College.

Orbit and classification

Vassar is a member of the Alauda family (902),[4] a large family of typically bright carbonaceous asteroids and named after its parent body, 702 Alauda.[12]:23

It orbits the Sun in the outer main-belt at a distance of 2.4–3.8 AU once every 5 years and 5 months (1,988 days). Its orbit has an eccentricity of 0.22 and an inclination of 22° with respect to the ecliptic.[1] In 1908, it was first identified as A908 CD at Heidelberg Observatory. The body's observation arc begins with its official discovery observation at Yerkes in 1933.[11]

Physical characteristics

Rotation period and pole

In November 2011 American amateur astronomer David Higgins obtained a rotational lightcurve of Vassar from photometric observations taken at the Hunters Hill Observatory (E14) in Australia. It gave a well-defined rotation period of 7.932 hours with a brightness variation of 0.35 magnitude ({{{1}}}).[lower-alpha 1] In 2016, two modeled lightcurves were derived using data from the Lowell photometric database and other sources, giving a concurring period of 7.93189 and 7.93190 hours and a spin axis of (104.0°, −50°) and (251.0°, −23.0°) in ecliptic coordinates, respectively ({{{1}}}).[8][9]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Vassar measures between 27.56 and 36.28 kilometers in diameter, and its surface has an albedo between 0.064 and 0.09.[5][6][7] The Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS and derives an albedo of 0.0703 and a diameter of 36.32 kilometers with an absolute magnitude of 10.7.[3]

Naming

This minor planet was named by American astronomer Maud Worcester Makemson (1891–1977) after the U.S Vassar College (formerly: Vassar Female College), located in New York state. Makemson, who computed the asteroid's orbit, was a teacher at the private elite school and director of its Vassar College Observatory.[2] Naming citation was first published in The Names of the Minor Planets by Paul Herget in 1955 (H 120).[2]

Notes

  1. ↑ 1.0 1.1 Higgins (2011) web: rotation period 7.932±0.002 hours with a brightness amplitude of 0.35 mag. Summary figures for (1312) Vassar at Collaborative Asteroid Lightcurve Link (CALL) and Asteroid lightcurves at the Hunters Hill Observatory Higgins, D.J. (2011)

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1312 Vassar (1933 OT)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001312. Retrieved 25 July 2017. 
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(1312) Vassar". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 107. doi:10.1007/978-3-540-29925-7_1313. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (1312) Vassar". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1312%7CVassar. Retrieved 16 January 2017. 
  4. ↑ 4.0 4.1 "Asteroid 1312 Vassar – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1312+Vassar#Asteroid%201312%20VassarEAR-A-VARGBDET-5-NESVORNYFAM-V3.0. Retrieved 26 October 2019. 
  5. ↑ 5.0 5.1 5.2 5.3 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T. et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal 152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. 
  6. ↑ 6.0 6.1 6.2 6.3 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. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  7. ↑ 7.0 7.1 7.2 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019. 
  8. ↑ 8.0 8.1 Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database". Astronomy and Astrophysics 587: 6. doi:10.1051/0004-6361/201527573. Bibcode: 2016A&A...587A..48D. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016A&A...587A..48D. Retrieved 16 January 2017. 
  9. ↑ 9.0 9.1 Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M. et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". Astronomy and Astrophysics 586: 24. doi:10.1051/0004-6361/201527441. Bibcode: 2016A&A...586A.108H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016A&A...586A.108H. Retrieved 16 January 2017. 
  10. ↑ 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. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 16 January 2017. 
  11. ↑ 11.0 11.1 "1312 Vassar (1933 OT)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1312. Retrieved 16 January 2017. 
  12. ↑ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N. 

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