1632 Sieböhme

1632 Sieböhme
Discovery [1]
Discovered by K. Reinmuth
Discovery site Heidelberg Obs.
Discovery date 26 February 1941
Designations
MPC designation 1632 Sieböhme
Named after
 Siegfried Böhme
(astronomer)[2]
1941 DF · 1930 UJ
1942 JC · 1947 RB
1951 MN · 1956 TM
A917 SO
main-belt · (middle) [3]
Orbital characteristics [1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 97.80 yr (35720 days)
Aphelion 3.0181 AU (451.50 Gm)
Perihelion 2.2916 AU (342.82 Gm)
2.6549 AU (397.17 Gm)
Eccentricity 0.13683
4.33 yr (1580.0 d)
292.01°
0° 13m 40.224s / day
Inclination 5.7170°
199.81°
127.26°
Earth MOID 1.28396 AU (192.078 Gm)
Jupiter MOID 2.32274 AU (347.477 Gm)
Jupiter Tisserand parameter 3.368
Physical characteristics
Dimensions 26.70 km
29.38±0.41 km[4]
28.842±0.383 km[5]
26.58 km (derived)[3]
Mean radius
 13.35 ± 1 km
56.65 h (2.360 d)[1][6]
56.81±0.01 h[7]
56.8129±0.1652 h[8]
0.0748
0.043±0.008[4]
0.0643±0.0074[5]
0.0522 (derived)[3]
0.0748 ± 0.013[1]
S [3]
11.7

    1632 Sieböhme, provisional designation 1941 DF, is a stony asteroid and slow rotator from the middle region of the asteroid belt, about 27 kilometers in diameter. It was discovered by German astronomer Karl Reinmuth at Heidelberg Observatory on 26 February 1941.[9]

    The asteroid orbits the Sun at a distance of 2.3–3.0 AU once every 4 years and 4 months (1,580 days). Its orbit shows an eccentricity of 0.14 and is tilted by 6 degrees to the plane of the ecliptic. Light-curve observations measured a long rotation period of more than 56 hours.[6][7][8] For a stony S-type asteroid, it has an exceptionally low geometric albedo of around 0.07, according to observations carried out by the WISE and NEOWISE missions.[4][5]

    The minor planet was named in honor of German astronomer Siegfried Böhme (1909–1996), staff member at Astronomisches Rechen-Institut in Heidelberg since 1949. He improved upon the orbital elements of many asteroids, in particular upon 919 Ilsebill.[2]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 1632 Siebohme (1941 DF)" (2015-07-13 last obs.). Jet Propulsion Laboratory. Retrieved 22 April 2016.
    2. 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1632) Sieböhme. Springer Berlin Heidelberg. p. 129. ISBN 978-3-540-29925-7. Retrieved 13 November 2015.
    3. 1 2 3 4 "LCDB Data for (1632) Siebohme". Asteroid Lightcurve Database (LCDB). Retrieved 13 November 2015.
    4. 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; 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:1209.5794Freely accessible. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved 13 November 2015.
    5. 1 2 3 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 13 November 2015.
    6. 1 2 Behrend, Raoul. "Asteroids and comets rotation curves – (1632) Siebohme". Geneva Observatory. Retrieved 13 November 2015.
    7. 1 2 Carbognani, Albino (January 2014). "Asteroids Lightcurves at Oavda: 2012 June - 2013 March". The Minor Planet Bulletin. 41 (1): 4–8. Bibcode:2014MPBu...41....4C. ISSN 1052-8091. Retrieved 13 November 2015.
    8. 1 2 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041Freely accessible. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 13 November 2015.
    9. ↑ "1632 Siebohme (1941 DF)". Minor Planet Center. Retrieved 13 November 2015.

    External links


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