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4185 Phystech

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Main-belt asteroid

4185 Phystech
Discovery 
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date4 March 1975
Designations
MPC designation(4185) Phystech
Named afterMoscow Institute of Physics and Technology
Alternative designations1975 ED · 1982 KD
1982 KH4 · 1988 BT
Minor planet categorymain-belt  · (inner)
background  · Flora
Orbital characteristics
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc64.48 yr (23,550 d)
Aphelion2.4339 AU
Perihelion2.0008 AU
Semi-major axis2.2174 AU
Eccentricity0.0977
Orbital period (sidereal)3.30 yr (1,206 d)
Mean anomaly311.69°
Mean motion0° 17 54.6 / day
Inclination2.2303°
Longitude of ascending node265.78°
Argument of perihelion320.99°
Physical characteristics
Mean diameter5.93 km (calculated)
Synodic rotation period4.66883±0.00014 h
4.66904±0.00003 h
Geometric albedo0.24 (assumed)
Spectral typeS (assumed)
Absolute magnitude (H)13.3

4185 Phystech, provisional designation 1975 ED, is a Florian or background asteroid from the inner regions of the asteroid belt, approximately 6 kilometers (4 miles) 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 ("PhysTech") 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 (402), 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 (1,206 days; semi-major axis of 2.22 AU). 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 (H62). 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 (U=3/3).

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 (informally: "PhysTech"; Физтех) on the occasion of its 50th anniversary in 1996, based on a proposal by the Institute of Theoretical Astronomy (ITA) in Saint Petersburg, Russia. The official naming citation was published by the Minor Planet Center on 22 February 1997 (M.P.C. 29143).

References

  1. ^ "4185 Phystech (1975 ED)". Minor Planet Center. Retrieved 27 April 2018.
  2. ^ "JPL Small-Body Database Browser: 4185 Phystech (1975 ED)" (2018-03-24 last obs.). Jet Propulsion Laboratory. Retrieved 27 April 2018.
  3. ^ "Small Bodies Data Ferret". Nesvorny HCM Asteroid Families V3.0. Archived from the original on 2 August 2017. Retrieved 27 April 2018.
  4. ^ "Asteroid 4185 Phystech – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
  5. ^ "LCDB Data for (4185) Phystech". Asteroid Lightcurve Database (LCDB). Retrieved 27 April 2018.
  6. ^ Dykhuis, Melissa J.; Molnar, Lawrence A.; Gates, Christopher J.; Gonzales, Joshua A.; Huffman, Jared J.; Maat, Aaron R.; et al. (March 2016). "Efficient spin sense determination of Flora-region asteroids via the epoch method". Icarus. 267: 174–203. Bibcode:2016Icar..267..174D. doi:10.1016/j.icarus.2015.12.021. Retrieved 27 April 2018.
  7. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 27 April 2018.

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