1191 Alfaterna
Discovery [1] | |
---|---|
Discovered by | L. Volta |
Discovery site |
Observatory of Turin (Pino Torinese) |
Discovery date | 11 February 1931 |
Designations | |
MPC designation | 1191 Alfaterna |
Named after | Nuceria Alfaterna[2] |
1931 CA · 1965 AA | |
main-belt · (outer) [3] | |
Orbital characteristics [1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 85.16 yr (31105 days) |
Aphelion | 3.0283 AU (453.03 Gm) |
Perihelion | 2.7553 AU (412.19 Gm) |
2.8918 AU (432.61 Gm) | |
Eccentricity | 0.047190 |
4.92 yr (1796.2 d) | |
98.183° | |
0° 12m 1.512s / day | |
Inclination | 18.494° |
134.73° | |
53.098° | |
Earth MOID | 1.79197 AU (268.075 Gm) |
Jupiter MOID | 2.03652 AU (304.659 Gm) |
Jupiter Tisserand parameter | 3.212 |
Physical characteristics | |
Dimensions |
±3 km ( 42.09IRAS: 17)[4] ±0.63 km 46.11[5] ±0.836 km 46.375[6] 42.01 km (derived)[3] |
Mean radius | ±1.5 21.045km |
3.664 h (0.1527 d)[1][3] ±1.92 (provisional) 33.12[7] | |
±0.009 (IRAS: 0.0574 17)[1][4] ±0.002 0.050[5] ±0.0053 0.0297[6] 0.0479 (derived)[3] | |
C [3] | |
10.8[1] | |
|
1191 Alfaterna, provisional designation 1931 CA, is a carbonaceous asteroid from the outer region of the asteroid belt, about 42 kilometers in diameter. It was discovered by Italian astronomer Luigi Volta at Pino Torinese Observatory, Northern Italy, on 11 February 1931.[8]
The C-type asteroid orbits the Sun at a distance of 2.8–3.0 AU once every 4 years and 11 months (1,796 days). Its orbit is tilted by 18 degrees to the plane of the ecliptic and shows an eccentricity of 0.05. It has a rotation period of 3.66 hours[3] with an alternative, provisional rotation of 33 hours[7] and an albedo between 0.03 and 0.06, according to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and the NEOWISE mission of the Wide-field Infrared Survey Explorer.[4][5][6]
It is named for the ancient Roman town of Nuceria Alfaterna, now known as Nocera Inferiore. The ancient city was founded between Pompeii and Salerno by the Oschi around 1000 B.C. and is entombed beneath the present Nocera Superiore, birthplace of A. Fresa, who proposed the name in 1957.[2]
References
- 1 2 3 4 5 "JPL Small-Body Database Browser: 1191 Alfaterna (1931 CA)" (2015-06-18 last obs.). Jet Propulsion Laboratory. Retrieved 1 May 2016.
- 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1191) Alfaterna. Springer Berlin Heidelberg. p. 100. ISBN 978-3-540-29925-7. Retrieved 22 December 2015.
- 1 2 3 4 5 6 "LCDB Data for (1191) Alfaterna". Asteroid Lightcurve Database (LCDB). Retrieved 22 December 2015.
- 1 2 3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. Bibcode:2004PDSS...12.....T. Retrieved 22 December 2015.
- 1 2 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. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 22 December 2015.
- 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". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 22 December 2015.
- 1 2 Behrend, Raoul. "Asteroids and comets rotation curves – (1191) Alfaterna". Geneva Observatory. Retrieved 22 December 2015.
- ↑ "1191 Alfaterna (1931 CA)". Minor Planet Center. Retrieved 22 December 2015.
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1191 Alfaterna at the JPL Small-Body Database