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531 Zerlina

From Wikipedia, the free encyclopedia
Main-belt asteroid

531 Zerlina
Lightcurve-based 3D-model of Zerlina
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date12 April 1904
Designations
(531) Zerlina
PronunciationItalian:[dzerˈliːna][2]
Named after
Zerlina, Masetto's fiancée
(Don Giovanni)[3]
1904 NW · 1955 HA
main-belt · (middle)
Pallas[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc112.56 yr (41,114 days)
Aphelion3.3356AU
Perihelion2.2379 AU
2.7867 AU
Eccentricity0.1970
4.65yr (1,699 days)
104.09°
0° 12m 42.84s / day
Inclination33.994°
197.73°
57.751°
Physical characteristics
Dimensions13.65±0.32 km[5]
13.87±4.02 km[6]
14.11±0.45 km[7]
15.12 km(derived)[8]
15.19±1.3 km[9]
15.8±1.6 km[10]
16±2 km[11]
17.804±0.178 km[12]
12h[13]
16 h[8]
16.716±0.003 h[14]
16.706±0.001 h[15]
0.10±0.02[11]
0.10±0.08[6]
0.101±0.007[12]
0.11±0.02[10]
0.1225(derived)[8]
0.1460±0.028[9]
0.150±0.030[5]
0.185±0.014[7]
SMASS =B[1] · B[8]
11.80[7][9][12]
12.0[1][8][5][11][10]
12.25[6]

531 Zerlina, provisional designation 1904 NW, carbonaceous Palladianasteroid from the central region of theasteroid belt, approximately 18 kilometers in diameter. It was discovered by German astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory on 12 April 1904.[16]

Orbit and characteristics

[edit]

Observations using theIRAS satellite have shown it to have anabsolute magnitude of 11.8, a diameter of 15.19 kilometers, a rotational period of 16.706 hours, and analbedo of 0.1460.[1]

Naming

[edit]

It is named for a character inMozart's opera,Don GiovanniH 57).[3]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 531 Zerlina (1904 NW)" (2016-11-04 last obs.).Jet Propulsion Laboratory. Retrieved4 September 2017.
  2. ^John Mario,Batti batti – Italian Pronunciation Guide #14 for Singers, YouTube
  3. ^abSchmadel, Lutz D. (2007). "(531) Zerlina".Dictionary of Minor Planet Names – (531) Zerlina.Springer Berlin Heidelberg. p. 56.doi:10.1007/978-3-540-29925-7_532.ISBN 978-3-540-00238-3.
  4. ^"Asteroid 531 Zerlina – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^abcMasiero, 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.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.S2CID 46350317. Retrieved4 September 2017.
  6. ^abcNugent, 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.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.S2CID 119289027.
  7. ^abcUsui, 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.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  8. ^abcde"LCDB Data for (531) Zerlina". Asteroid Lightcurve Database (LCDB). Retrieved4 September 2017.
  9. ^abcTedesco, 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. Retrieved22 October 2019.
  10. ^abcAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614.
  11. ^abcAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680.S2CID 119214002. Retrieved4 September 2017.
  12. ^abcMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 118700974.
  13. ^Székely, P.; Kiss, L. L.; Szabó, Gy. M.; Sárneczky, K.; Csák, B.; Váradi, M.; et al. (August 2005)."CCD photometry of 23 minor planets".Planetary and Space Science.53 (9):925–936.arXiv:astro-ph/0504462.Bibcode:2005P&SS...53..925S.doi:10.1016/j.pss.2005.04.006.S2CID 119361591. Retrieved4 September 2017.
  14. ^Brinsfield, James W. (June 2008)."The Rotation Periods of 531 Zerlina, 1194 Aleta 1352 Wawel, 2005 Hencke, 2648 Owa, and 3509 Sanshui".The Minor Planet Bulletin.35 (2):86–87.Bibcode:2008MPBu...35...86B.ISSN 1052-8091. Retrieved4 September 2017.
  15. ^Pilcher, Frederick; Brinsfield, James W. (October 2011)."Rotation Period Determination for 531 Zerlina".The Minor Planet Bulletin.38 (4): 206.Bibcode:2011MPBu...38Q.206P.ISSN 1052-8091. Retrieved4 September 2017.
  16. ^"531 Zerlina (1904 NW)".Minor Planet Center. Retrieved4 September 2017.

External links

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