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1635 Bohrmann

From Wikipedia, the free encyclopedia
"Bohrmann" redirects here. For the German astronomer, seeAlfred Bohrmann. For the German football goalkeeper, seeHarry Bohrmann. For the German-American fashion photographer, seeHorst P. Horst.
Asteroid

1635 Bohrmann
Alightcurve-based 3D-model ofBohrmann
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date7 March 1924
Designations
(1635) Bohrmann
Named after
Alfred Bohrmann
(astronomer[2]
1924 QW · 1931 VH1
1936 UJ · 1938 CH
1939 HL · 1943 EG1
1948 EA1 · 1953 FH
main-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.24 yr (34,057 days)
Aphelion3.0174AU
Perihelion2.6894 AU
2.8534 AU
Eccentricity0.0575
4.82yr (1,761 days)
357.19°
0° 12m 16.2s / day
Inclination1.8222°
184.35°
136.06°
Physical characteristics
Dimensions16.60±0.82 km[4]
17.12 km(calculated)[3]
17.127±0.171[5]
17.533±0.244 km[6]
19.12±0.70 km[7]
5.864±0.001 h[8]
5.86427±0.00005 h[9]
11.730±0.005 h[10]
11.73±0.01h[11]
0.187±0.015[7]
0.2104±0.0154[6]
0.219±0.049[5]
0.24(assumed)[3]
0.255±0.052[4]
SMASS =S[1] · S[3]
10.95±0.01[8] · 11.0[1][3][4] · 11.05±0.24[12] · 11.1[6][7]

1635 Bohrmann, provisional designation1924 QW, is a stony Koronianasteroid from the outer region of theasteroid belt, approximately 17 kilometers in diameter. It was discovered on 7 March 1924, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany, and named for astronomerAlfred Bohrmann.[2][13]

Orbit and classification

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The stonyS-type asteroid belongs to theKoronis family, a group consisting of few hundred known bodies with nearlyecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,761 days). Its orbit has aneccentricity of 0.06 and aninclination of 2° with respect to the ecliptic.[1]

As noprecoveries were taken,Bohrmann'sobservation arc begins with the first used observation taken on the night following its discovery.[13]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bohrmann measures between 16.6 and 19.1 kilometers in diameter, and its surface has analbedo between 0.187 and 0.255.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for members of the Koronian family of 0.24, and calculates a diameter of 17.1 kilometers with anabsolute magnitude of 11.0.[3]

Lightcurves

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In September and October 2003, four rotationallightcurves were obtained for this asteroid from photometric observations at several observatories around the world, including the Whitin Observatory in Wellesley, Massachusetts, as well as by U.S. astronomersRobert Stephens andBrian Warner. The lightcurves gave two different solutions for theBohrmann'srotation period. One solution gave5.864±0.001[8] and5.86427±0.00005[9] hours, while the alternative solution gave11.73±0.01[11] and11.730±0.005[10] hours. The lightcurves had a concurring brightness variation of 0.25 inmagnitude (U=2/2/3/n.a.).[3]

Naming

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Thisminor planet was named after German astronomerAlfred Bohrmann (1904–2000), a long-time observer of minor planets at the discovering Heidelberg Observatory and adiscoverer of minor planets himself. During his career he had published several hundreds of precise observations of asteroids.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3931).[14]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1635 Bohrmann (1924 QW)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1635) Bohrmann".Dictionary of Minor Planet Names – (1635) Bohrmann.Springer Berlin Heidelberg. p. 130.doi:10.1007/978-3-540-29925-7_1636.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1635) Bohrmann". Asteroid Lightcurve Database (LCDB). Retrieved6 August 2016.
  4. ^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. Retrieved6 August 2016.
  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. Retrieved8 December 2016.
  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. ^abcSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved6 August 2016.
  9. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy and Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved6 August 2016.
  10. ^abStephens, Robert D.; Warner, Brian D. (March 2004)."Lightcurve analysis of Koronis family asteroid 1635 Bohrmann".The Minor Planet Bulletin.31 (1):3–4.Bibcode:2004MPBu...31....3S.ISSN 1052-8091. Retrieved6 August 2016.
  11. ^abSimpson, Christine M. (March 2004)."Rotation period and lightcurve of asteroid 1635 Bohrmann".The Minor Planet Bulletin.31 (1): 2.Bibcode:2004MPBu...31....2S.ISSN 1052-8091. Retrieved6 August 2016.
  12. ^Veres, 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. Retrieved6 August 2016.
  13. ^ab"1635 Bohrmann (1924 QW)".Minor Planet Center. Retrieved6 August 2016.
  14. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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