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950 Ahrensa

From Wikipedia, the free encyclopedia
Phocaea asteroid and slow rotator

950 Ahrensa
Modelled shape of Ahrensa from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date1 April 1921
Designations
(950) Ahrensa
Named after
Ahrens family
(friends of discoverer)[2]
1921 JP · 1955 SU2
1974 VG3 · A904 RF
main-belt · Phocaea[3]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc111.60 yr (40761 days)
Aphelion2.7477 AU (411.05 Gm)
Perihelion1.9958 AU (298.57 Gm)
2.3717 AU (354.80 Gm)
Eccentricity0.15851
3.65yr (1334.1d)
53.005°
0° 16m 11.424s / day
Inclination23.477°
181.81°
348.19°
Physical characteristics
15.03±1.8(IRAS:15) km[4]
16.21±0.53 km[5]
14.299±0.070 km[6]
16.66±0.41 km[7]
15.34 km(derived)[3]
202±1h,[8] 202 h (8.4 d)[1]
0.1793±0.054(IRAS:15)[1][4]
0.158±0.011[5]
0.1988±0.0203[6]
0.231±0.031[7]
0.2727(derived)[3]
SMASS = Sa
S[3]
11.2[1]

950 Ahrensa, provisional designation1921 JP, is a stony Phocaeaasteroid andslow rotator from the inner regions of theasteroid belt, approximately 15 kilometers in diameter. It was discovered on 1 April 1921, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[9]

Description

[edit]

TheS-type asteroid, classified as a Sa-subtype in theSMASS taxonomic scheme, is a member of thePhocaea family, a group of asteroids with similar orbital characteristics. It orbits the Sun at a distance of 2.0–2.7 AU once every 3 years and 8 months (1,334 days). Its orbit shows aneccentricity of 0.16 and istilted by 23 degrees to the plane of theecliptic.

A photometriclightcurve analysis at the U.S. Palmer Divide Observatory in 2009, showed that the body has an exceptionally longrotation period of 202 hours.[8] According to the surveys carried out by the Infrared Astronomical Satellite,IRAS, the JapaneseAkari satellite, and the U.S.Wide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the surface of the asteroid has analbedo in the range of 0.16 to 0.23, while the Collaborative Asteroid Lightcurve Link derives an even higher value of 0.27 for the stony body.[3][4][5][6][7]

The minor planet was named in honor of friends of the discoverer Karl Reinmuth, the Ahrens family, who helped him financially at the Heidelberg Observatory. Reinmuth also named the minor planet909 Ulla after Ulla Ahrens, a member of this family.[2]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 950 Ahrensa (1921 JP)" (2015-10-30 last obs.).Jet Propulsion Laboratory. Retrieved2 May 2016.
  2. ^abSchmadel, Lutz D. (2003). "(950) Ahrensa".Dictionary of Minor Planet Names – (950) Ahrensa.Springer Berlin Heidelberg. p. 84.doi:10.1007/978-3-540-29925-7_951.ISBN 978-3-540-29925-7.
  3. ^abcde"LCDB Data for (950) Ahrensa". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2016.
  4. ^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.
  5. ^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)
  6. ^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. Retrieved4 January 2016.
  7. ^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. Retrieved4 January 2016.
  8. ^abWarner, Brian D. (January 2010)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 June-September".The Minor Planet Bulletin.37 (1):24–27.Bibcode:2010MPBu...37...24W.ISSN 1052-8091. Retrieved4 January 2016.
  9. ^"950 Ahrensa (1921 JP)".Minor Planet Center. Retrieved4 January 2016.

External links

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