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3181 Ahnert

From Wikipedia, the free encyclopedia
Asteroid

3181 Ahnert
Discovery[1]
Discovered byF. Börngen
Discovery siteKarl Schwarzschild Obs.
Discovery date8 March 1964
Designations
(3181) Ahnert
Named after
Paul Ahnert(astronomer)[2]
1964 EC · 1932 RK
1936 XJ · 1951 GC1
1964 DE · 1975 NH1
1975 RD · 1979 SC12
1979 UO4 · 1979 WD8
1979 WU1 · 1982 RE1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.12 yr (31,454 days)
Aphelion2.3743AU
Perihelion2.0840 AU
2.2292 AU
Eccentricity0.0651
3.33yr (1,216 days)
9.5372°
0° 17m 45.96s / day
Inclination3.9579°
221.14°
304.92°
Physical characteristics
Dimensions7.961±0.097[4]
8.19 km(calculated)[3]
8.511±0.031 km[5]
8.57±0.24 km[6]
0.1856±0.0266[5]
0.216±0.019[4]
0.24(assumed)[3]
0.264±0.029[6]
SMASS =S[1] · S[3][7]
12.40[6] · 12.6[1][3] · 12.8[5] · 12.98±0.06[7]

3181 Ahnert, provisional designation1964 EC, is a stony Floraasteroid from the inner regions of theasteroid belt, about 8 kilometers in diameter. It was discovered by German astronomerFreimut Börngen at theKarl Schwarzschild Observatory in Tautenburg, eastern Germany, on 8 March 1964.[8]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.1–2.4 AU once every 3 years and 4 months (1,216 days). Its orbit has aneccentricity of 0.07 and aninclination of 4° with respect to theecliptic.[1] The firstprecovery was obtained atLowell Observatory in 1931, extending the asteroid'sobservation arc by 33 years prior to its discovery.[8]

Physical characteristics

[edit]

According to the surveys carried out by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures between 8.0 and 8.6 kilometers and its surface has analbedo between 0.19 and 0.26.[4][6][5] The Collaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – derived from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 8.2 kilometers.[3] As of 2016, the asteroid'srotation period and shape still remain unknown.

Naming

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Thisminor planet was named after German astronomerPaul Ahnert (1897–1989), author of theannual calendar of astronomical events (German:Kalender für Sternfreunde) and a renowned astronomer among professionals and amateurs. His fields of research included the physics of the Solar System and periods ofvariable stars at theSonneberg Observatory. (The minor planet1039 Sonneberga is named after this observatory.) Publisher of several books on performing astronomical observations, he also popularized the subject of astronomy to the general public.[2] The official naming citation was published by theMinor Planet Center on 2 July 1985 (M.P.C. 9771).[9]

References

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  1. ^abcde"JPL Small-Body Database Browser: 3181 Ahnert (1964 EC)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved16 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3181) Ahnert".Dictionary of Minor Planet Names – (3181) Ahnert.Springer Berlin Heidelberg. p. 264.doi:10.1007/978-3-540-29925-7_3182.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3181) Ahnert". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2016.
  4. ^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. Retrieved6 December 2016.
  5. ^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. Retrieved3 May 2016.
  6. ^abcdMasiero, 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. Retrieved3 May 2016.
  7. ^abVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved3 May 2016.
  8. ^ab"3181 Ahnert (1964 EC)".Minor Planet Center. Retrieved3 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2016.

External links

[edit]
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