C/1785 A1 (Messier–Méchain)

Parabolic comet From Wikipedia, the free encyclopedia

Comet Messier–Méchain, also known as C/1785 A1 from its modern nomenclature, is a faint parabolic comet that was observed several times by French astronomers, Charles Messier and Pierre Méchain, in January 1785.

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C/1785 A1 (Messier–Méchain)
Discovery[1]
Discovered byCharles Messier
Pierre Méchain
Discovery siteParis, France
Discovery date7 January 1785
Designations
1785 I[2]
Orbital characteristics[3]
Epoch27 January 1785 (JD 2373045.325)
Observation arc32 days
Number of
observations
9
Perihelion1.143 AU
Eccentricity~1.000
Inclination70.238°
267.21°
Argument of
periapsis
205.63°
Last perihelion27 January 1785
Physical characteristics[4]
7.5
(1785 apparition)
Close

Discovery and observations

Charles Messier discovered this comet using a small refractor following an observation of Uranus on the night of 7 January 1785.[1] Approximately 40 minutes later, Pierre Méchain also discovered the same comet from the Paris Observatory.[4] At the time, the comet was located within the constellation Cetus.[a]

Messier described the comet as a faint object surrounded by a "central condensation" around it, where he also noted that it became brighter on 9 January than it was two days earlier, but it never became visible to the naked eye.[4] He continued to observe the comet until 17 January 1785, when it was no longer visible near the star ε Cet.[5]

Orbit

The only known orbital calculations of the comet were written by Méchain in 1788, where he determined a parabolic trajectory that indicated the comet had reached perihelion on 27 January, while making its closest approach to Earth a day later at a distance of 0.417 AU (62.4 million km)[4]

In 2012, Maik Meyer noted that the preliminary orbital calculations for the comet C/2012 L2 (LINEAR) were strikingly similar to that of Messier–Méchain, however he concluded that this is only a coincidence rather than a return of C/1785 A1 itself.[6]

References

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