Astronomy:3674 Erbisbühl
_Erbisb%C3%BChl.png) Shape model of Erbisbühl from its lightcurve | |
| Discovery [1] | |
|---|---|
| Discovered by | C. Hoffmeister |
| Discovery site | Sonneberg Obs. |
| Discovery date | 13 September 1963 |
| Designations | |
| (3674) Erbisbühl | |
| Named after | Mount Erbisbühl (Eastern Germany)[2] |
| 1963 RH · 1970 OD 1986 AA | |
| Minor planet category | Mars-crosser[1][3] main-belt (inner)[4] |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 52.80 yr (19,285 days) |
| |{{{apsis}}}|helion}} | 3.2468 AU |
| |{{{apsis}}}|helion}} | 1.4723 AU |
| 2.3596 AU | |
| Eccentricity | 0.3760 |
| Orbital period | 3.62 yr (1,324 days) |
| Mean anomaly | 306.42° |
| Mean motion | 0° 16m 18.84s / day |
| Inclination | 21.029° |
| Longitude of ascending node | 296.85° |
| 98.240° | |
| Mars MOID | 0.1997 AU |
| Physical characteristics | |
| Mean diameter | 9.068±1.623 km[5] 10.32±0.71 km[6] |
| Rotation period | 11.28±0.01 h[4][7][lower-alpha 1] |
| Geometric albedo | 0.249±0.037[6] 0.309±0.126[5] |
| SMASS = Sk [1] | |
| Absolute magnitude (H) | 12.0[1][4] · 12.10[6] |
3674 Erbisbühl (prov. 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 (6.8 miles) in diameter. It was discovered on 13 September 1963, by German astronomer Cuno Hoffmeister at his Sonneberg Observatory on Mount Erbisbühl in Eastern Germany.[3]
Orbit and classification
Erbisbühl orbits the Sun in the inner main-belt at a distance of 1.5–3.2 AU once every 3 years and 7 months (1,324 days). Its orbit has an eccentricity of 0.38 and an inclination of 21° with respect to the ecliptic.[1] The body's observation arc starts in 1963, as no precoveries were taken and no identifications were made prior to its official discovery.[3]
Naming
This minor planet was named for Mount 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] The official naming citation was published by the Minor Planet Center on 2 February 1988 (M.P.C. 12809).[8]
Physical characteristics
In the SMASS taxonomic scheme, Erbisbühl is a stony S-type asteroid, characterized as a Sk-subtype, a transitional form to the uncommon K-type asteroid.[1]
Lightcurve
A rotational lightcurve 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 ({{{1}}}).[7][lower-alpha 1]
Diameter and albedo
According to the survey carried out by the Japanese Akari satellite, Erbisbühl has a high albedo of 0.25 with a corresponding diameter of 10.3 kilometers,[6] while the NEOWISE mission gives a diameter of 9.1 kilometers and an albedo of 0.31.[5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.8 kilometers.[4]
Notes
- ↑ 1.0 1.1 Lightcurve plot of (3674) Erbisbuhl, Robert Koff, Antelope Hills Observatory (H09). Summary figures at LCDB
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "JPL Small-Body Database Browser: 3674 Erbisbuhl (1963 RH)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003674.
- ↑ 2.0 2.1 Schmadel, Lutz D. (2007). "(3674) Erbisbühl". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 309. doi:10.1007/978-3-540-29925-7_3672. ISBN 978-3-540-00238-3. https://archive.org/details/dictionaryminorp00schm.
- ↑ 3.0 3.1 3.2 "3674 Erbisbuhl (1963 RH)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=3674.
- ↑ 4.0 4.1 4.2 4.3 "LCDB Data for (3674) Erbisbuhl". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=3674%7CErbisbuhl.
- ↑ 5.0 5.1 5.2 Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T. et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal 814 (2): 13. doi:10.1088/0004-637X/814/2/117. Bibcode: 2015ApJ...814..117N. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N. Retrieved 5 December 2016.
- ↑ 6.0 6.1 6.2 6.3 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U. (online, AcuA catalog p. 153)
- ↑ 7.0 7.1 Koff, Robert A. (June 2004). "Lightcurve photometry of Mars-crossing asteroids 1474 Beira and 3674 Erbisbuhl". Minor Planet Bulletin 31 (2): 33–34. ISSN 1052-8091. Bibcode: 2004MPBu...31...33K. http://www.minorplanet.info/MPB/issues/MPB_31-2.pdf. Retrieved 19 March 2020.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
External links
- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 3674 Erbisbühl at AstDyS-2, Asteroids—Dynamic Site
- 3674 Erbisbühl at the JPL Small-Body Database
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