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74P/Smirnova–Chernykh

Periodic comet with 8 year orbit


Periodic comet with 8 year orbit

FieldValue
name74P/Smirnova–Chernykh
image[[File:74p-2010Jan25-12UT.jpg240px]]
caption74P (apmag ~17; 3.6AU from the Sun) near galaxy [PGC 49413](http://server6.wikisky.org/starview?object_type=2&object_id=4970)
discovererTamara Mikhailovna Smirnova
Nikolai Stepanovich Chernykh
discovery_dateMarch 4, 1975
designations1967 XV; 1975 VII; 1984 V;
1992 XXI
epochNovember 21, 2025
semimajor5.11 AU
perihelion4.836 AU
aphelion5.39 AU
eccentricity0.0543
period11.56 yr
inclination6.015°
last_pJanuary 26, 2018{{cite web
date2007-07-09
title74P/Smirnova-Chernykh (NK 1485)
publisherOAA Computing and Minor Planet Sections
authorSyuichi Nakano
author-linkSyuichi Nakano
urlhttp://www.oaa.gr.jp/~oaacs/nk/nk1485.htm
access-date2010-02-24}}
July 30, 2009
next_pMarch 2, 2026
2034-Jun-14

Nikolai Stepanovich Chernykh 1992 XXI |author-link=Syuichi Nakano |access-date=2010-02-24}} July 30, 2009 2034-Jun-14

EpochPerihelion
(AU)
19295.68
19673.55
20264.84
20343.84

74P/Smirnova–Chernykh is a periodic comet in the Solar System. It fits the definition of an Encke-type comet with (TJupiter 3; a Jupiter), 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.

A close approach to Jupiter in 2021 lifted perihelion from 3.54 AU to 4.84 AU.

References

References

  1. {{mpc. 74p
  2. Toth, I.. (March 2006). "The quasi-Hilda subgroup of ecliptic comets - an update". [[Astronomy and Astrophysics]].
  3. Kronk, Gary W. "74P/Smirnova-Chernykh".
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