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2181 Fogelin

From Wikipedia, the free encyclopedia
Asteroid

2181 Fogelin
Shape model ofFogelin from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date28 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 arc75.08yr (27,422 d)
Aphelion2.8986AU
Perihelion2.2836 AU
2.5911 AU
Eccentricity0.1187
4.17 yr (1,523 d)
354.25°
0° 14m 10.68s / day
Inclination13.007°
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]

2181 Fogelin (prov. designation:1942 YA) is anEunomia asteroid from the central regions of theasteroid belt, approximately 11 kilometers (7 miles) in diameter. It was discovered on 28 December 1942, by Germany astronomerKarl Reinmuth at theHeidelberg Observatory in southwest Germany.[1] In 1980, it was named for Eric S. Fogelin an assistant at theMinor Planet Center.[1] The likely elongatedS-type asteroid has arotation period of 14.07 hours.[3]

Orbit and classification

[edit]

Fogelin is a member of theEunomia family (502),[3][4] a prominentfamily 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 thecentral 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 aneccentricity of 0.12 and aninclination of 13° with respect to theecliptic.[2] The body'sobservation arc begins at Heidelberg with its official discovery observation in December 1942.[1]

Naming

[edit]

Thisminor planet was named byBrian Marsden and Conrad Bardwell of theMinor Planet Center, after their assistant, Eric S. Fogelin. During 1979–1980, he was preparing the center's computerized data and helped publishing theMinor 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

[edit]

Fogelin is an assumedS-type asteroid,[3] in line with the overallspectral type seen among Eunomian asteroids.[9]: 23  Near-IR spectroscopy at theNASA Infrared Telescope Facility with theSpeX instrument showed that the asteroid containsmafic minerals, which are rich in magnesium and iron.[11]

Rotation period

[edit]

In March 2010, a rotationallightcurve ofFogelin was obtained fromphotometric observations by Richard Durkee at the Shed of Science Observatory (H39) in the United States. Lightcurve analysis gave a well-definedrotation period of 14.07 hours with a brightness amplitude of 0.57magnitude, indicative of an elongated shape (U=3).[8]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Fogelin measures between 10.067 and 11.29 kilometers in diameter and its surface has analbedo between 0.200 and 0.252.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, the family'sparent body and namesake – and calculates a diameter of 11.55 kilometers based on anabsolute magnitude of 12.0.[3]

References

[edit]
  1. ^abcdefg"2181 Fogelin (1942 YA)".Minor Planet Center. Retrieved19 March 2018.
  2. ^abcd"JPL Small-Body Database Browser: 2181 Fogelin (1942 YA)" (2018-01-25 last obs.).Jet Propulsion Laboratory. Retrieved19 March 2018.
  3. ^abcdefghi"LCDB Data for (2181) Fogelin". Asteroid Lightcurve Database (LCDB). Retrieved19 March 2018.
  4. ^ab"Asteroid 2181 Fogelin – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcMasiero, 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.
  6. ^abcdMainzer, 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.
  7. ^abcdUsui, 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. ^abDurkee, 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.
  9. ^abNesvorný, 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.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved19 March 2018.
  11. ^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]
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