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2815 Soma

Binary Florian asteroid


Summary

Binary Florian asteroid

FieldValue
minorplanetyes
name2815 Soma
background#D6D6D6
discovery_ref
discovered15 September 1982
discovererE. Bowell
discovery_siteAnderson Mesa Stn.
mpc_name(2815) Soma
alt_names1982 RL1955 MH
1970 AC1974 DL
pronounced
named_afterSoma cube
(mechanical puzzle)
mp_categorymain-beltFlora
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc61.77 yr (22,562 days)
aphelion2.6107 AU
perihelion1.8552 AU
semimajor2.2329 AU
eccentricity0.1692
period3.34 yr (1,219 days)
mean_anomaly168.50°
mean_motion/ day
inclination5.7042°
asc_node119.87°
arg_peri237.53°
satellites1
(Ds/Dp: )
(orbital period: 17.915 h)
dimensionskm
km
7.07 km (taken)
km
rotationh
h
albedo
spectral_typeS
abs_magnitude(R) (R)12.612.7

1970 AC1974 DL

(mechanical puzzle) (Ds/Dp: ) (orbital period: 17.915 h) km 7.07 km (taken) km h

2815 Soma, provisional designation , is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 15 September 1982, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona, in the United States . It is named for the mechanical puzzle Soma cube.

Orbit and classification

Soma is a member of the Flora family, a large family of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,219 days). Its orbit has an eccentricity of 0.17 and an inclination of 6° with respect to the ecliptic. It was first identified as at Goethe Link Observatory in 1955. The body's observation arc begins with at Crimea-Nauchnij, 12 years prior to its official discovery at Anderson Mesa.

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer (WISE) with its subsequent NEOWISE mission, Soma measures 6.641 and 7.158 kilometers in diameter and its surface has an albedo of 0.365 and 0.3207, respectively. The Collaborative Asteroid Lightcurve Link adopts Peter Pravec's revised WISE-data, that is, an albedo of 0.2273 and a diameter of 7.067 kilometers with an absolute magnitude of 12.98.

Moon and lightcurve

Primary

In November 2009, a rotational lightcurve of Soma was obtained from photometric observations by astronomers Petr Pravec, Donald Pray and Peter Kušnirák at Carbuncle Hill Observatory, Rhode Island, and Ondřejov Observatory, in the Czech Republic, respectively. Lightcurve analysis gave a rotation period of 2.7327 hours with a brightness variation of 0.08 magnitude, indicating that the body has a nearly spheroidal shape (). The body's spin rate is within the 2.2-to-20 hours range found for most asteroids, about half an hour longer than the so-called fast rotators.

Secondary

In March 2011, photometric observations revealed that Soma is a synchronous binary asteroid with a minor-planet moon orbiting it every 17.915 hours. The system has a secondary-to-primary mean-diameter ratio of 0.25, which means that satellite's diameter measures approximately 25% of that of Soma (the primary), and translate into a diameter of 1.75 kilometers. The observations also gave a refined rotation period for Soma of 2.73325 hours and an amplitude of 0.07 magnitude (). The system has an absolute magnitude of 12.53, and a phase slope parameter (G) of 0.27.

Naming

This minor planet was named for the Soma cube, following a proposal by Belgian astronomer Jean Meeus (also see ). The Soma cube a dissection puzzle with seven pieces, invented by the Danish mathematician Piet Hein and popularized by American writer Martin Gardner (also see ). The approved naming citation was published by the Minor Planet Center on 10 September 1984 (M.P.C. 9080).

Notes

References

References

  1. {{MW. soma
Wikipedia Source

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