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5481 Kiuchi

Bright binary Vestian asteroid

Field	Value
minorplanet	yes
name	5481 Kiuchi
background	#D6D6D6
discovery_ref
discovered	15 February 1990
discoverer	K. Endate
K. Watanabe
discovery_site	Kitami Obs.
mpc_name	(5481) Kiuchi
alt_names	1990 CH1970 SR
named_after	Tsuruhiko Kiuchi
(Japanese amateur astronomer)
mp_category	main-beltVesta
orbit_ref
epoch	4 September 2017 (JD 2458000.5)
uncertainty	0
observation_arc	46.14 yr (16,851 days)
aphelion	2.4858 AU
perihelion	2.1936 AU
semimajor	2.3397 AU
eccentricity	0.0624
period	3.58 yr (1,307 days)
mean_anomaly	194.33°
mean_motion	/ day
inclination	5.9569°
asc_node	326.10°
arg_peri	250.69°
satellites	1 (Ds/Dp 0.33, P: 20.90 h)
mean_diameter	(calculated)
rotation
albedo	0.40 (assumed)
spectral_type	V
abs_magnitude	(R)13.4

K. Watanabe (Japanese amateur astronomer)

5481 Kiuchi, provisional designation **, is a bright binary Vestian asteroid from the inner regions of the asteroid belt, approximately 4 km in diameter. It was discovered on 15 February 1990, by Japanese astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory in Hokkaidō, Japan, and named after their colleague Tsuruhiko Kiuchi. The V-type asteroid has a rotation period of 3.6 hours.

Family and orbit

Kiuchi is a bright core member of the Vesta family, one of the main-belt's largest families. It orbits the Sun in the inner main-belt at a distance of 2.2–2.5 AU once every 3 years and 7 months (1,307 days). Its orbit has an eccentricity of 0.06 and an inclination of 6° with respect to the ecliptic. It was first identified as ** at Crimea–Nauchnij in 1970, extending the body's observation arc by 20 years prior to its official discovery observation at Kitami.

Naming

This minor planet was named in honor of Japanese amateur astronomer and discoverer of comets, Tsuruhiko Kiuchi (born 1954), who is known for the rediscovery of the periodic Perseid Comet Swift–Tuttle, a previously lost comet (also see naming citations for and . Based on a prediction by Brian Marsden, Kiuchi made this rediscovery in 1992, using only binoculars. The approved naming citation was published by the Minor Planet Center on 1 September 1993 (M.P.C. 22510).

Binary asteroid

Satellite

In March 2008, a lightcurve of Kiuchi was obtained from photometric observations by astronomers Peter Kušnirák and Petr Pravec at Ondřejov Observatory in the Czech Republic, by Julian Oey at Leura Observatory, Australia, by Robert Stephens at Goat Mountain, California, by Mark Husárik at Skalnaté pleso Observatory, Slovakia, and by Judit Györgyey Ries at McDonald Observatory, Texas.

These photometric observations revealed, that Kiuchi is a synchronous binary asteroid with a minor-planet moon orbiting it every 20.90 hours based on mutual eclipsing and occultation events. The satellite's diameter is about a third of that of Kiuchi, which translates into 1.3 kilometers (secondary-to-primary mean-diameter ratio of ).

Primary

According to the surveys carried out by PanSTARRS, Kiuchi is a bright V-type asteroid. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 and calculates a diameter of 3.86 kilometers, using an absolute magnitude of 13.676 from Petr Pravec's revised WISE data.

Kiuchi itself has a rotation period of hours with a small brightness variation of 0.1 magnitude, indicating a nearly spheroidal shape (). Photometric follow-up observations by Petr Pravec confirmed the results in 2013 and 2016, giving a period of 3.6198 and 3.6196 hours with an amplitude of 0.08 and 0.1 magnitude, and an orbital period for the satellite of 20.9 and 20.9062 hours, respectively ().

Notes

References

Info: Wikipedia Source

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