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5101 Akhmerov

Asteroid


Summary

Asteroid

FieldValue
minorplanetyes
name5101 Akhmerov
background#D6D6D6
discovery_ref
discovered22 October 1985
discovererL. V. Zhuravleva
discovery_siteCrimean Astrophysical Obs.
mpc_name(5101) Akhmerov
alt_names1969 TQ
named_afterVadim Akhmerov
(Ukrainian surgeon)
mp_categorymain-beltEos
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc47.37 yr (17,303 days)
aphelion3.3535 AU
perihelion2.6561 AU
semimajor3.0048 AU
eccentricity0.1160
period5.21 yr (1,903 days)
mean_anomaly60.772°
mean_motion/ day
inclination10.699°
asc_node205.91°
arg_peri174.12°
dimensionskm
12.32 km (calculated)
rotationh
albedo0.14 (assumed)
spectral_typeCXS
abs_magnitude12.212.3 (S)

(Ukrainian surgeon) 12.32 km (calculated)

5101 Akhmerov, provisional designation , is an Eos asteroid from the outer region of the asteroid belt, about 12 kilometers in diameter. It was discovered on 22 October 1985, by Russian astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. It was later named for Ukrainian surgeon Vadim Akhmerov.

Orbit and classification

Akhmerov is a member of the Eos family (606), the largest asteroid family in the outer main belt consisting of nearly 10,000 asteroids.

It orbits the Sun at a distance of 2.7–3.4 AU once every 5 years and 3 months (1,903 days). Its orbit has an eccentricity of 0.12 and an inclination of 11° with respect to the ecliptic. A first precovery was obtained at the discovering observatory in 1969, extending the body's observation arc by 16 years prior to its official discovery observation.

Physical characteristics

PanSTARRS photometric survey has characterized Akhmerov as a CX-type asteroid, a transitional group between the carbonaceous C-type asteroid and the metallic X-type asteroids.

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Akhmerov measures 11.0 kilometers in diameter and its surface has an albedo of 0.19. The Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.14 – derived from 221 Eos, the largest member and namesake of this orbital family – and calculates a diameter of 12.3 kilometers with an absolute magnitude of 12.3.

Rotation period

A rotational lightcurve of Akhmerov was obtained from photometric observations taken at the U.S. Palomar Transient Factory in September 2011. The lightcurve gave a rotation period of hours with a brightness amplitude of 0.33 in magnitude ().

Naming

This minor planet was named after (born 1929), long-time physician at the maternity hospital in Alushta on the Crimean peninsula. The official naming citation was published by the Minor Planet Center on 4 May 1999 (M.P.C. 34620).

References

Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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