C/1894 G1 (Gale)

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C/1894 G1 (Gale)
Comet Gale.jpg
Comet Gale (1894 II) photographed by Edward E. Barnard from the Lick Observatory on 5 May 1894
Discovery [1]
Discovered by Walter F. Gale
Discovery site Sydney, Australia
Discovery date1 April 1894
Designations
1894 II, 1894b [2]
Orbital characteristics [3]
Epoch 4 June 1894 (JD 2412983.5)
Observation arc 82 days
Number of
observations
45
Aphelion 176.85 AU
Perihelion 0.983 AU
Semi-major axis 88.914 AU
Eccentricity 0.98298
Orbital period 838.42 years
Inclination 86.959°
207.89°
Argument of
periapsis
324.17°
Mean anomaly 0.060°
Last perihelion13 April 1894
TJupiter 0.124
Earth MOID 0.076 AU
Jupiter MOID 1.230 AU
Physical characteristics [4]
Comet nuclear
magnitude (M2)
6.3
3.0
(1894 apparition)

C/1894 G1 (Gale), also known formerly as 1894 II, is a long-period comet that became barely visible to the naked eye in May 1894. It is the first of three comets discovered by Australian astronomer Walter Frederick Gale.

Contents

Possible meteor shower

The comet's small minimum orbit intersection distance with Earth (0.076 AU) led scientists in 2021 to suggest that C/1894 G1 might potentially be the progenitor of a meteor shower known as the December Iota Ursae Majorids, however no definite link has yet been found between that particular shower and the comet. [5]

References

  1. W. F. Gale (1894). "Beobachtungen des Cometen 1894… (Gale April 3)". Astronomische Nachrichten (in German). 135 (8): 149–150. doi:10.1002/asna.18941350805.
  2. "Comet Names and Designations". International Comet Quarterly. Retrieved 23 May 2025.
  3. "C/1894 G1 (Gale) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory . Retrieved 23 May 2025.
  4. G. W. Kronk (2003). Cometography: A Catalog of Comets. Vol. 2: 1800–1899. Cambridge University Press. pp. 717–722. ISBN   978-0-521-58505-7.
  5. M. Hajduková; L. Neslušan (2021). "Modeling the Meteoroid Streams of comets C/1894 G1 (Gale) and C/1936 O1 (Kaho–Kozik–Lis)". Planetary and Space Science . Bibcode:2021P&SS..19505152H. doi:10.1016/j.pss.2020.105152.