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1220 Crocus

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1220 Crocus
background#D6D6D6
image001220-asteroid shape model (1220) Crocus.png
captionShape model of Crocus from its lightcurve
discovery_ref
discovered11 February 1932
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
mpc_name(1220) Crocus
alt_names1932 CU1955 PC
pronounced
named_afterCrocus
mp_categorymain-beltEos
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc85.31 yr (31,161 days)
aphelion3.2243 AU
perihelion2.7807 AU
semimajor3.0025 AU
eccentricity0.0739
period5.20 yr (1,900 days)
mean_anomaly204.16°
mean_motion/ day
inclination11.365°
asc_node113.34°
arg_peri333.41°
dimensions
rotation
albedo
spectral_typeS
abs_magnitude11.72

1220 Crocus, provisionally designated , 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.

Orbit and classification

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. A

Physical characteristics

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

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 ().

Naming

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

References

References

  1. {{OED. crocus
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