4185 Phystech


4185 Phystech, provisional designation, is a Florian or background asteroid from the inner regions of the asteroid belt, approximately in diameter. It was discovered on 4 March 1975, by Soviet astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. The presumed S-type asteroid has a rotation period of 4.67 hours. It is named in honor of the Moscow [Institute of Physics and Technology] on its 50th anniversary.

Orbit and classification

Phystech is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. Based on osculating Keplerian orbital elements, the asteroid has also been classified as a member of the Flora family, a giant asteroid family and the largest family of stony asteroids in the main-belt.
It orbits the Sun in the inner asteroid belt at a distance of 2.0–2.4 AU once every 3 years and 4 months. Its orbit has an eccentricity of 0.10 and an inclination of 2° with respect to the ecliptic. The body's observation arc begins with a precovery taken at Palomar Observatory in October 1953, more than 21 years prior to its official discovery observation at Nauchnij.

Physical characteristics

Phystech is an assumed stony S-type asteroid, based on its family classification.

Rotation period

In March and April 2008, two rotational lightcurves of Phystech were obtained from photometric observations by American astronomers at LPL and Calvin College. Lightcurve analysis gave a well-defined rotation period of 4.66883 and 4.66904 hours with a brightness amplitude of 0.53 and 0.41 magnitude, respectively.

Diameter and albedo

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family – and calculates a diameter of 5.93 kilometers based on an absolute magnitude of 13.3.

Naming

This minor planet was named after the Moscow Institute of Physics and Technology on the occasion of its 50th anniversary in 1996, based on a proposal by the Institute of Theoretical Astronomy in Saint Petersburg, Russia. The official naming citation was published by the Minor Planet Center on 22 February 1997.