3674 Erbisbühl

3674 Erbisbühl
Discovery[1]
Discovered by C. Hoffmeister
Discovery site Sonneberg Obs.
Discovery date 13 September 1963
Designations
MPC designation 3674 Erbisbühl
Named after
Erbisbühl (mountain)[2]
1963 RH · 1970 OD
1986 AA
Mars-crosser[1][3]
main-belt (inner)[4]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 52.67 yr (19,236 days)
Aphelion 3.2464 AU
Perihelion 1.4731 AU
2.3597 AU
Eccentricity 0.3757
3.62 yr (1,324 days)
197.62°
 16m 18.84s / day
Inclination 21.026°
296.86°
98.231°
Earth MOID 0.6406 AU
Physical characteristics
Dimensions 10.32±0.71 km[5]
11.83 km (calculated)[4]
11.28±0.01 h[6]
0.249±0.037[5]
0.20 (assumed)[4]
SMASS = Sk[1] · S[4]
12.0[1][4]
12.10[5]
12.23±0.59[7]

    3674 Erbisbühl, provisional designation 1963 RH, is an stony asteroid and one of the largest Mars-crossers from the innermost regions of the asteroid belt, approximately 11 kilometers in diameter. It was discovered by German astronomer Cuno Hoffmeister at his Sonneberg Observatory in Eastern Germany, on 13 September 1963.[3]

    In the SMASS taxonomic scheme, the stony S-type asteroid is classified as a Sk-subtype, a transitional form to the uncommon K-type. It orbits the Sun at a distance of 1.5–3.2 AU once every 3 years and 8 months (1,324 days). Its orbit has a high eccentricity of 0.38 and an inclination of 21° with respect to the plane of the ecliptic.[1] The asteroid's observation arc starts in 1963, as no precoveries were taken and no identifications were made prior to its discovery.[3]

    A rotational light-curve for this asteroid was obtained from photometric observations made at the U.S. Antelope Hills Observatory in December 2003. It rendered a rotation period of 11.28±0.01 hours with a brightness variation of 0.40 in magnitude (U=3).[6] According to the survey carried out by the Japanese Akari satellite, the asteroid has a high albedo of 0.249 with a corresponding diameter of 10.3 kilometers,[5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.8 kilometers.[4]

    The minor planet was named for the mountain "Erbisbühl" on which the discovering Sonneberg Observatory is located (also see 1039 Sonneberga). Cuno Hoffmeister, discoverer of this asteroid and founder of the observatory, lived and worked at Erbisbühl for many decades.[2] Naming citation was published on 2 February 1988 (M.P.C. 12809).[8]

    References

    1. 1 2 3 4 5 6 "JPL Small-Body Database Browser: 3674 Erbisbuhl (1963 RH)" (2016-05-13 last obs.). Jet Propulsion Laboratory. Retrieved 28 May 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (3674) Erbisbühl. Springer Berlin Heidelberg. p. 309. ISBN 978-3-540-00238-3. Retrieved 28 May 2016.
    3. 1 2 3 "3674 Erbisbuhl (1963 RH)". Minor Planet Center. Retrieved 28 May 2016.
    4. 1 2 3 4 5 6 "LCDB Data for (3674) Erbisbuhl". Asteroid Lightcurve Database (LCDB). Retrieved 28 May 2016.
    5. 1 2 3 4 Usui, 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. Retrieved 28 May 2016.
    6. 1 2 Koff, Robert A. (June 2004). "Lightcurve photometry of Mars-crossing asteroids 1474 Beira and 3674 Erbisbuhl". The Minor Planet Bulletin. 31 (2): 33–34. Bibcode:2004MPBu...31...33K. ISSN 1052-8091. Retrieved 1 February 2016.
    7. 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 28 May 2016.
    8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 28 May 2016.

    External links

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