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1220 Crocus
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1220 Crocus

1220 Crocus
Shape model of Crocus from its lightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date11 February 1932
Designations
(1220) Crocus
Pronunciation/ˈkrkəs/[2]
Named after
Crocus[3]
1932 CU · 1955 PC
main-belt · Eos[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc85.31 yr (31,161 days)
Aphelion3.2243 AU
Perihelion2.7807 AU
3.0025 AU
Eccentricity0.0739
5.20 yr (1,900 days)
204.16°
0° 11m 21.84s / day
Inclination11.365°
113.34°
333.41°
Physical characteristics
Dimensions17.866±0.175[5]
491.4±0.1[6]
0.114±0.020[5]
S[4]
11.72[1]

1220 Crocus, provisionally designated 1932 CU, is a stony Eoan asteroid and slow rotator from the outer regions of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 11 February 1932, by German astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany.[7]

Orbit and classification

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Crocus is a member of the Eos family, a collisional population of mostly stony composition. It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 2 months (1,900 days). Its orbit has an eccentricity of 0.07 and an inclination of 11° with respect to the ecliptic.[1] A

Physical characteristics

[edit]

The asteroid has been characterized as a stony S-type asteroid.[4]

In December 2014, a rotational lightcurve of Crocus was obtained from photometric observations by an international collaboration of several astronomers from Europe and the United States. Lightcurve analysis gave a long rotation period of 491 hours with a brightness variation of 1.00 magnitude (U=3).[6]

Naming

[edit]

This minor planet was later named after the genus of flowering plants, Crocus, in the iris family.[3]

References

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