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1215 Boyer

Stony Eunomian asteroid


Stony Eunomian asteroid

FieldValue
minorplanetyes
name1215 Boyer
background#D6D6D6
discovery_ref
discovered19 January 1932
discovererA. Schmitt
discovery_siteAlgiers Obs.
mpc_name(1215) Boyer
alt_names1932 BA
named_afterLouis Boyer
(French astronomer)
mp_categorymain-belt(middle)
EunomiaMaria
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc85.46 yr (31,214 days)
aphelion2.9213 AU
perihelion2.2352 AU
semimajor2.5783 AU
eccentricity0.1331
period4.14 yr (1,512 days)
mean_anomaly324.91°
mean_motion/ day
inclination15.915°
asc_node123.74°
arg_peri266.02°
dimensionskm
km
17.47 km (calculated)
km
km
km
rotationh
albedo
0.21 (assumed)
spectral_typeTholen = SS
B–V = 0.900
U–B = 0.459
abs_magnitude11.00
11.1
11.14

(French astronomer) EunomiaMaria km 17.47 km (calculated) km km km

0.21 (assumed)

B–V = 0.900 U–B = 0.459 11.1 11.14

1215 Boyer, provisional designation , is a stony Eunomian asteroid from the central region of the asteroid belt, approximately 20 kilometers in diameter. It was discovered by astronomer Alfred Schmitt in 1932, who named it after French astronomer and college Louis Boyer.

Discovery

Boyer was discovered on 19 January 1932, by French astronomer Alfred Schmitt at the Algiers Observatory in Algeria, North Africa. Eight days later, it was independently discovered by Karl Reinmuth at Heidelberg Observatory in Germany. The body's observation arc begins at Algiers with its official discovery observation.

Classification and orbit

Boyer is a member of the Eunomia family (502), the most prominent family in the intermediate main-belt, which mostly consists of stony asteroids. Conversely, Boyer has also been grouped into the Maria family (506).

It orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,512 days). Its orbit has an eccentricity of 0.13 and an inclination of 16° with respect to the ecliptic.

Physical characteristics

In the Tholen classification, Boyer is a common, stony S-type asteroid.

Lightcurves

In August 2008 and May 2012, two rotational lightcurves of Boyer were obtained from photometric observations by an international collaboration of astronomers studying the rotational properties of Maria asteroids, using the ground-based Wise Observatory in Israel. Lightcurve analysis gave a rotation period of 10.36 hours with a brightness variation of 0.31 and 050 magnitude, respectively ().

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Boyer measures between 13.041 and 24.65 kilometers in diameter and its surface has an albedo between 0.116 and 0.3012.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21, derived from the Eunomia family's largest member and namesake, 15 Eunomia, and calculates a diameter of 17.47 kilometers with an absolute magnitude of 11.1.

Naming

This minor planet was named by the discoverer after his colleague at Algiers Observatory, Louis Boyer (1901–1999), who worked extensively on asteroids and comets. Boyer himself was a discoverer of minor planets at Algiers. He later worked on identifications at Nice observatory. The official was published by the Minor Planet Center on 1 August 1978 (M.P.C. 4418).

References

Info: Wikipedia Source

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