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52266 Van Flandern

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name52266 Van Flandern
background#D6D6D6
discovery_ref
discovered10 January 1986
discovererC. S. Shoemaker
E. M. Shoemaker
discovery_sitePalomar Obs.
mpc_name(52266) Van Flandern
alt_names1986 AD1975 CJ
2002 QQ
named_afterTom Van Flandern
(American astronomer)
mp_categorymain-beltPhocaea
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc41.88 yr (15,298 days)
aphelion2.8486 AU
perihelion1.8213 AU
semimajor2.3349 AU
eccentricity0.2200
period3.57 yr (1,303 days)
mean_anomaly275.98°
mean_motion/ day
inclination23.707°
asc_node302.17°
arg_peri229.79°
dimensionskm
km
4.60 km (calculated)
rotationh
h
h
h
albedo0.23 (assumed)
spectral_typeS
abs_magnitude13.9 (R)14.31

E. M. Shoemaker 2002 QQ (American astronomer) km 4.60 km (calculated) h h h

52266 Van Flandern (provisional designation ****) is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 10 January 1986, by American astronomers Carolyn and Eugene Shoemaker at the Palomar Observatory in California, United States. The asteroid was later named for American astronomer Tom Van Flandern.

Orbit and classification

Van Flandern is a member of the Phocaea family (701), a family of stony asteroids with similar orbital characteristics. It orbits the Sun in the inner main-belt at a distance of 1.8–2.8 AU once every 3 years and 7 months (1,303 days). Its orbit has an eccentricity of 0.22 and an inclination of 24° with respect to the ecliptic. The asteroid's observation arc begins 11 years prior to its official discovery observation, with its identification as at the Karl Schwarzschild Observatory in February 1975.

Physical characteristics

Van Flandern has been characterized as a common S-type asteroid by Pan-STARRS photometric survey.

Lightcurves

In January and February 2011, four rotational lightcurves of Van Flandern were obtained from photometric observations at the Via Capote Observatory , the Palomar Transient Factory, and the Australian Oakley Southern Sky Observatory (E09), as well as by astronomer René Roy at his Blauvac Observatory (627) in France. Lightcurve analysis gave a well-defined rotation period between 9.65 and 9.89 hours with a brightness variation between 0.52 and 0.61 magnitude ().

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Van Flandern measures 3.47 and 4.42 kilometers in diameter and its surface has an albedo of 0.30 and 0.249, respectively.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from 25 Phocaea, the family's most massive member and namesake – and calculates a diameter of 4.6 kilometers with an absolute magnitude of 13.9.

Naming

This minor planet was named in memory of American astronomer Tom Van Flandern (1940–2009), expert in lunar occultations and on the dynamics of binary minor planets at USNO in the 1970s.

Van Flandern also participated in the refinement of the Global Positioning System and published the Meta Research Bulletin for non-mainstream views on cosmology. The approved naming citation was published by the Minor Planet Center on 9 February 2009 (M.P.C. 65123).

References

Info: Wikipedia Source

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