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74P/Smirnova–Chernykh

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(Redirected from 74P/Smirnova-Chernykh) Periodic comet with 8 year orbit
74P/Smirnova–Chernykh
74P (apmag ~17; 3.6AU from the Sun) near galaxy PGC 49413
Discovery
Discovered byTamara Mikhailovna Smirnova
Nikolai Stepanovich Chernykh
Discovery dateMarch 4, 1975
Designations
Alternative designations1967 XV; 1975 VII; 1984 V;
1992 XXI
Orbital characteristics
EpochMay 1, 2009
Aphelion4.790 AU
Perihelion3.557 AU
Semi-major axis4.173 AU
Eccentricity0.1485
Orbital period8.53 yr
Inclination6.647°
Last perihelionJanuary 26, 2018
July 30, 2009
Next perihelion2034-Jun-14

74P/Smirnova–Chernykh is a periodic comet in the Solar System. It fits the definition of an Encke-type comet with (TJupiter > 3; a < aJupiter), and is a Quasi-Hilda comet. It was discovered in late March 1975 by Tamara Mikhajlovna Smirnova while examining exposures from the Crimean Astrophysical Observatory. In the discovery images the comet had an apparent magnitude of ~15. In the year of discovery, the comet came to perihelion on August 6, 1975.

The comet had been photographed during 1967, but was identified as an asteroid and assigned the designation 1967 EU.

The comet is estimated at 4.46 km in diameter, and currently has an orbit contained completely inside of the orbit of Jupiter.

References

  1. Syuichi Nakano (2007-07-09). "74P/Smirnova-Chernykh (NK 1485)". OAA Computing and Minor Planet Sections. Retrieved 2010-02-24.
  2. ^ Seiichi Yoshida (2005-08-28). "74P/Smirnova-Chernykh". Seiichi Yoshida's Comet Catalog. Retrieved 2010-01-25.
  3. MPC
  4. ^ "JPL Small-Body Database Browser: 74P/Smirnova-Chernykh". Jet Propulsion Laboratory. Retrieved 2010-01-25. 2009-12-30 last obs
  5. Toth, I. (March 2006). "The quasi-Hilda subgroup of ecliptic comets - an update". Astronomy and Astrophysics. 448 (3): 1191–1196. Bibcode:2006A&A...448.1191T. doi:10.1051/0004-6361:20053492.
  6. ^ Kronk, Gary W. "74P/Smirnova-Chernykh". Retrieved 2010-01-25. (Cometography Home Page)

External links


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