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4524 Barklajdetolli

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name4524 Barklajdetolli
background#D6D6D6
discovery_ref
discovered8 September 1981
discovererL. V. Zhuravleva
discovery_siteCrimean Astrophysical Obs.
mpc_name(4524) Barklajdetolli
alt_names
1935 SN1973 FH
named_afterMichael Andreas Barclay de Tolly
(Russian Field Marshal)
mp_categorymain-beltVest
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc63.12 yr (23,055 days)
aphelion2.6292 AU
perihelion2.0123 AU
semimajor2.3208 AU
eccentricity0.1329
period3.54 yr (1,291 days)
mean_anomaly87.691°
mean_motion/ day
inclination7.2862°
asc_node177.20°
arg_peri149.44°
dimensions7.14 km (calculated)
km
km
rotationh
albedo
0.24 (assumed)
spectral_typeS
abs_magnitude12.7012.913.20

1935 SN1973 FH

(Russian Field Marshal) km km

0.24 (assumed)

4524 Barklajdetolli, provisional designation **, is an elongated Vestian asteroid and an exceptionally slow rotator from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 8 September 1981, by Russian–Ukrainian astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named for Russian field marshal Michael Andreas Barclay de Tolly.

Orbit and classification

Barklajdetolli is an attributed member of the Vestian family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,291 days). Its orbit has an eccentricity of 0.13 and an inclination of 7° with respect to the ecliptic.

In September 1935, it was first identified as ** and ** at Simeiz and Johannesburg Observatory, respectively. The body's observation arc begins with a precovery taken at Palomar Observatory in 1953, or 28 years prior to its official discovery observation at Nauchnyj.

Physical characteristics

Barklajdetolli has been characterized as a common stony S-type asteroid.

Slow rotator and shape

In August 2009, a rotational lightcurve for this asteroid was obtained at the Carbuncle Hill Observatory on Rhode Island, United States. Lightcurve analysis gave an exceptionally long rotation period of 1,069 hours with a high brightness amplitude of 1.26 in magnitude ().

While the period still may be wrong by a few hundred hours, it is one of the slowest rotating asteroids known to exist. The exceptionally high variation in brightness indicates that the body has a non-spheroidal shape.

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, the asteroid's surface has a low albedo of 0.05 and 0.10, respectively, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a much higher albedo of 0.24, derived from its Flora family classification. The divergent albedos also translate into different estimates for the body's size.

While the space-based surveys find a diameter of 12.1 and 13.6 kilometers, respectively, CALL calculates only 7.1 kilometers, as the higher a body's albedo (reflectivity), the smaller its diameter for a certain absolute magnitude.

Naming

This minor planet was named in memory of Russian field marshal of Scottish descent, Michael Andreas Barclay de Tolly (1761–1818). He was Russia's Minister of War and commander-in-chief of its armies during the French invasion of Russia in the Patriotic War of 1812. The official naming citation was published by the Minor Planet Center on 4 May 1999 (M.P.C. 34620).

References

Info: Wikipedia Source

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