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3674 Erbisbühl

Mars-crossing asteroid


Mars-crossing asteroid

FieldValue
minorplanetyes
name3674 Erbisbühl
background#FA8072
image003674-asteroid shape model (3674) Erbisbühl.png
captionShape model of *Erbisbühl* from its lightcurve
discovery_ref
discovered13 September 1963
discovererC. Hoffmeister
discovery_siteSonneberg Obs.
mpc_name(3674) Erbisbühl
alt_names1963 RH1970 OD
1986 AA
named_afterMount Erbisbühl
(Eastern Germany)
mp_categoryMars-crosser
main-belt (inner)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc52.80 yr (19,285 days)
aphelion3.2468 AU
perihelion1.4723 AU
semimajor2.3596 AU
eccentricity0.3760
period3.62 yr (1,324 days)
mean_anomaly306.42°
mean_motion/ day
inclination21.029°
asc_node296.85°
arg_peri98.240°
mars_moid0.1997 AU
mean_diameter
km
rotation
albedo
spectral_typeSMASS = Sk
abs_magnitude12.012.10

1986 AA (Eastern Germany) main-belt (inner) km

3674 Erbisbühl (prov. designation: ) is an stony asteroid and one of the largest Mars-crossers from the innermost regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 13 September 1963, by German astronomer Cuno Hoffmeister at his Sonneberg Observatory on Mount Erbisbühl in Eastern Germany.

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. The body's observation arc starts in 1963, as no precoveries were taken and no identifications were made prior to its official discovery.

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. The official naming citation was published by the Minor Planet Center on 2 February 1988 (M.P.C. 12809).

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.

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 hours with a brightness variation of 0.40 in magnitude ().

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, while the NEOWISE mission gives a diameter of 9.1 kilometers and an albedo of 0.31. TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.8 kilometers.

Notes

References

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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