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4957 Brucemurray

Stony asteroid


Stony asteroid

FieldValue
minorplanetyes
name4957 Brucemurray
background#FFC2E0
discovery_ref
discovererE. F. Helin
discovery_sitePalomar Obs.
discovered15 December 1990
mpc_name(4957) Brucemurray
alt_names1990 XJ
named_afterBruce C. Murray
(American planetary scientist)
mp_categoryNEOAmor
Mars-crosser
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc41.35 yr (15,102 days)
aphelion1.9082 AU
perihelion1.2228 AU
semimajor1.5655 AU
eccentricity0.2189
period1.96 yr (715 days)
mean_anomaly282.15°
mean_motion/ day
inclination35.011°
asc_node254.90°
arg_peri97.487°
moid0.4258 AU165.9 LD
dimensionskm
km
3.11 km (calculated)
km
rotationh
h
albedo
0.20 (assumed)
spectral_typeSMASS SS
B–V =
V–R =
V–I =
abs_magnitude14.915.1

(American planetary scientist) Mars-crosser km 3.11 km (calculated) km h

0.20 (assumed) B–V = V–R = V–I =

4957 Brucemurray, provisional designation , is a stony asteroid, classified as near-Earth object of the Amor group and as Mars-crosser, approximately 3 kilometers in diameter. It was discovered by American astronomer Eleanor Helin at the Palomar Observatory in California on 15 December 1990. The asteroid was named after American planetary scientist Bruce C. Murray.

Orbit and classification

Brucemurray orbits the Sun at a distance of 1.2–1.9 AU once every 1 years and 12 months (715 days). Its orbit has an eccentricity of 0.22 and an inclination of 35° with respect to the ecliptic.

The body's observation arc begins with a precovery taken at the Australian Siding Spring Observatory in March 1976, or more than 14 years prior to its official discovery observation.

Close approaches

This deep Mars-crosser makes close approaches both to Earth and Mars. It has an Earth minimum orbital intersection distance of 0.4258 AU which corresponds to 165.9 lunar distances. On 18 May 2033, the asteroid will also pass 0.0684 AU from Mars.

Physical characteristics

In the SMASS classification, Brucemurray is a stony S-type asteroid. BVRIZ photometry also found that the asteroid is an S-type NEO.

Rotation period and axis

In the 1990s, two rotational lightcurves of Brucemurray were obtained from photometric observations by Czech astronomer Petr Pravec at Ondřejov Observatory. Lightcurve analysis gave a rotation period of 2.892 hours in both cases with a brightness variation of 0.28 and 0.36 magnitude, respectively ().

In 2004, an international study modeled a lightcurve with a concurring period of 2.8922 hours and found a spin axis of (358.0°, −50.0°) in ecliptic coordinates (λ, β) ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of Wide-field Infrared Survey Explorer and the ExploreNEOs survey using the Spitzer Space Telescope, Brucemurray measures between 3.01 and 3.499 kilometers in diameter and its surface has an albedo between 0.132 and 0.18.

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.11 kilometers based on an absolute magnitude of 14.9.

Naming

This minor planet was named after American planetary scientist Bruce C. Murray (1931–2013), director of the Jet Propulsion Laboratory, co-founder of The Planetary Society and professor at California Institute of Technology. This asteroid which comes close both to Mars and Earth, is considered a particularly appropriate object for Murray, who had diligently championed a mission to Mars.

The official naming citation was published by the Minor Planet Center on 29 November 1993 (M.P.C. 22829).

References

Info: Wikipedia Source

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