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8187 Akiramisawa

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name8187 Akiramisawa
background#D6D6D6
image008187-asteroid shape model (8187) Akiramisawa.png
captionAkiramisawa modeled from its lightcurve
discovery_ref
discovererS. Otomo
discovery_siteKiyosato Obs.
discovered15 December 1992
mpc_name(8187) Akiramisawa
alt_names1992 XL
1971 VV
named_afterAkira Misawa
(Japanese botanist)
mp_categorymain-belt(outer)
Eos
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc44.79 yr (16,358 days)
aphelion3.3523 AU
perihelion2.6219 AU
semimajor2.9871 AU
eccentricity0.1223
period5.16 yr (1,886 days)
mean_anomaly351.90°
mean_motion/ day
inclination11.608°
asc_node83.066°
arg_peri277.60°
mean_diameter(calculated)
rotation
albedo0.057 (assumed)
spectral_typeC (assumed)
abs_magnitude12.8 (R)13.36

1971 VV (Japanese botanist) Eos

8187 Akiramisawa, provisional designation , is an Eos asteroid from the outer region of the asteroid belt. It was discovered by Japanese astronomer Satoru Otomo at Kiyosato Observatory on 15 December 1992. The assumed C-type asteroid has a rotation period of 5.8 hours and measures approximately 12 km in diameter. It was named after Japanese botanist Akira Misawa (1942–1994).

Orbit and classification

Akiramisawa is a member the Eos family (606), the largest asteroid family of the outer main belt consisting of nearly 10,000 known members. It orbits the Sun in the outer asteroid belt at a distance of 2.6–3.4 AU once every 5 years and 2 months (1,886 days). Its orbit has an eccentricity of 0.12 and an inclination of 12° with respect to the ecliptic. In October 1971, it was first identified as at the Chilean Cerro El Roble Station, extending the body's observation arc by 21 years prior to its official discovery observation at Kiyosato.

Naming

This minor planet was named in honour of Japanese botanist Akira Misawa (1942–1994), a professor at Chiba University, who examined the effects of light pollution on plants. The was published by the Minor Planet Center on 9 January 2001 (M.P.C. 41935).

Physical characteristics

A rotational lightcurve of Akiramisawa was obtained from photometric observations made at the Palomar Transient Factory in June 2010. Lightcurve analysis gave a rotation period of hours with a high brightness amplitude of 0.90 magnitude (). The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057, and calculates a diameter of 11.9 kilometers with an absolute magnitude of 13.36.

References

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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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