31641 Cevasco

31641 Cevasco
Discovery [1]
Discovered by LINEAR
Discovery site Lincoln Lab's ETS
Discovery date 6 April 1999
Designations
MPC designation 31641 Cevasco
Named after
 Hannah Olivia Cevasco
(Broadcom MASTERS)[2]
1999 GW34 · 1993 RR14
main-belt · (inner) [3]
Orbital characteristics [1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 23.15 yr (8,455 days)
Aphelion 2.7522 AU
Perihelion 2.1234 AU
2.4378 AU
Eccentricity 0.1289
3.81 yr (1,390 days)
295.32°
Inclination 1.2135°
278.37°
215.83°
Physical characteristics
Dimensions 2.737±0.168[4][5]
3.26 km (calculated)[3]
2.6556±0.1936 h[3]
2.8167±0.0127 h[6]
2.820±0.010 h[7]
0.20 (assumed)[3]
0.3108±0.0672[4]
0.311±0.067[5]
S [3]
14.8[1][3] · 14.940[7]

    31641 Cevasco, provisional designation 1999 GW34, is a stony asteroid from the inner regions of the asteroid belt, approximately 3.3 kilometers in diameter. It was discovered on 6 April 1999, by the Lincoln Near-Earth Asteroid Research project (LINEAR) at Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico.[8]

    The S-type asteroid orbits the Sun at a distance of 2.1–2.8 AU once every 3 years and 10 months (1,390 days). Its orbit has an eccentricity of 0.13 and an inclination of 1° with respect to the ecliptic.[1] Cevasco was first identified as 1993 RR14 at ESO's La Silla Observatory in 1993, extending the body's observation arc by 6 years prior to its official discovery observation.[8]

    Photometric light-curve observations at the U.S. Palomar Transient Factory in 2010, 2012 and 2014, measured the asteroid's rotation period to be 2.6556±0.1936, 2.8167±0.0127 and 2.820±0.010 hours with a brightness variation of 0.71, 0.48 and 0.54 in magnitude, respectively (U=2).[6][7] According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Cevasco measures 2.7 kilometers in diameter and its surface has an albedo of 0.311,[4][5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.3 kilometers based on an absolute magnitude of 14.8.[3]

    The minor planet was named in honor of Hannah Olivia Cevasco (b. 2000) finalist in the 2015 Broadcom MASTERS, a math and science competition for middle school students, for her medicine and health sciences project. At the time she attended the St. Charles School in California.[8]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 31641 Cevasco (1999 GW34)" (2016-11-08 last obs.). Jet Propulsion Laboratory. Retrieved 2 December 2016.
    2. ↑ Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names –. Springer Berlin Heidelberg. ISBN 978-3-540-00238-3. Retrieved 27 January 2016.
    3. 1 2 3 4 5 6 7 "LCDB Data for (31641) Cevasco". Asteroid Lightcurve Database (LCDB). Retrieved 27 January 2016.
    4. 1 2 3 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 2 December 2016.
    5. 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096Freely accessible. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 2 December 2016.
    6. 1 2 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041Freely accessible. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 27 January 2016.
    7. 1 2 3 Chang, Chan-Kao; Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015). "Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory". The Astrophysical Journal Supplement Series. 219 (2): 19. arXiv:1506.08493Freely accessible. Bibcode:2015ApJS..219...27C. doi:10.1088/0067-0049/219/2/27. Retrieved 27 January 2016.
    8. 1 2 3 "31641 Cevasco (1999 GW34)". Minor Planet Center. Retrieved 27 January 2016.

    External links

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