2181 Fogelin (prov. designation: 1942 YA) is an Eunomia asteroid from the central regions of the asteroid belt, approximately 11 kilometers (7 miles) in diameter. It was discovered on 28 December 1942, by Germany astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany.[1] In 1980, it was named for Eric S. Fogelin an assistant at the Minor Planet Center.[1] The likely elongated S-type asteroid has a rotation period of 14.07 hours.[3]
![]() Shape model of Fogelin from its lightcurve | |
Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 28 December 1942 |
Designations | |
(2181) Fogelin | |
Named after | Eric S. Fogelin [1] (MPC staff member) |
1942 YA · 1952 HC2 1975 VF9 | |
main-belt [1][2] · (middle) Eunomia [3][4] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 75.08 yr (27,422 d) |
Aphelion | 2.8986 AU |
Perihelion | 2.2836 AU |
2.5911 AU | |
Eccentricity | 0.1187 |
4.17 yr (1,523 d) | |
354.25° | |
0° 14m 10.68s / day | |
Inclination | 13.007° |
17.286° | |
116.18° | |
Physical characteristics | |
10.067±0.109 km[5] 10.420±0.089 km[6] 11.29±0.85 km[7] 11.55 km (calculated)[3] | |
14.07±0.01 h[8] | |
0.200±0.031[7] 0.21 (assumed)[3] 0.2376±0.0548[6] 0.252±0.046[5] | |
S (assumed)[3] | |
12.0[2][3] · 12.10[6][7] | |
Orbit and classification
editFogelin is a member of the Eunomia family (502),[3][4] a prominent family of stony asteroid and the largest one in the intermediate main belt with more than 5,000 known members.[9] It orbits the Sun in the central main-belt at a distance of 2.3–2.9 AU once every 4 years and 2 months (1,523 days; semi-major axis of 2.59 AU). Its orbit has an eccentricity of 0.12 and an inclination of 13° with respect to the ecliptic.[2] The body's observation arc begins at Heidelberg with its official discovery observation in December 1942.[1]
Naming
editThis minor planet was named by Brian Marsden and Conrad Bardwell of the Minor Planet Center, after their assistant, Eric S. Fogelin. During 1979–1980, he was preparing the center's computerized data and helped publishing the Minor Planet Circulars.[1] The official naming citation was published by the Minor Planet Center on 1 August 1980 (M.P.C. 5451).[10]
Physical characteristics
editFogelin is an assumed S-type asteroid,[3] in line with the overall spectral type seen among Eunomian asteroids.[9]: 23 Near-IR spectroscopy at the NASA Infrared Telescope Facility with the SpeX instrument showed that the asteroid contains mafic minerals, which are rich in magnesium and iron.[11]
Rotation period
editIn March 2010, a rotational lightcurve of Fogelin was obtained from photometric observations by Richard Durkee at the Shed of Science Observatory (H39) in the United States. Lightcurve analysis gave a well-defined rotation period of 14.07 hours with a brightness amplitude of 0.57 magnitude, indicative of an elongated shape (U=3).[8]
Diameter and albedo
editAccording to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Fogelin measures between 10.067 and 11.29 kilometers in diameter and its surface has an albedo between 0.200 and 0.252.[5][6][7] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the family's parent body and namesake – and calculates a diameter of 11.55 kilometers based on an absolute magnitude of 12.0.[3]
References
edit- ^ a b c d e f g "2181 Fogelin (1942 YA)". Minor Planet Center. Retrieved 19 March 2018.
- ^ a b c d "JPL Small-Body Database Browser: 2181 Fogelin (1942 YA)" (2018-01-25 last obs.). Jet Propulsion Laboratory. Retrieved 19 March 2018.
- ^ a b c d e f g h i "LCDB Data for (2181) Fogelin". Asteroid Lightcurve Database (LCDB). Retrieved 19 March 2018.
- ^ a b "Asteroid 2181 Fogelin – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
- ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
- ^ a b c d 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.
- ^ a b c d 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. (online, AcuA catalog p. 153)
- ^ a b Durkee, Russell I. (July 2010). "Asteroids Observed from the Shed of Science Observatory: 2009 October - 2010 March". The Minor Planet Bulletin. 37 (3): 125–127. Bibcode:2010MPBu...37..125D. ISSN 1052-8091.
- ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 19 March 2018.
- ^ Birlan, Mirel; Barucci, Maria Antonietta; Vernazza, Pierre; Fulchignoni, Marcello; Binzel, Richard P.; Bus, Schelte J.; et al. (June 2004). "Near-IR spectroscopy of asteroids 21 Lutetia, 89 Julia, 140 Siwa, 2181 Fogelin and 5480 (1989YK8), potential targets for the Rosetta mission; remote observations campaign on IRTF". New Astronomy. 9 (5): 343–351. arXiv:astro-ph/0312638. Bibcode:2004NewA....9..343B. doi:10.1016/j.newast.2003.12.005.
External links
edit- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 2181 Fogelin at AstDyS-2, Asteroids—Dynamic Site
- 2181 Fogelin at the JPL Small-Body Database