Discovery | |
---|---|
Discovered by | Charles Dillon Perrine & Antonín Mrkos |
Discovery date | December 9, 1896 |
Designations | |
1896 X1; 1896 VII; 1896g; 1909 P1; 1909 III; 1909b; 1955 U1; 1955 VII; 1955i; 1962 I; 1961h; 1968 VIII; 1968h | |
Orbital characteristics | |
Epoch | 2002-09-03 ( JD 2452520.5) |
Aphelion | 5.8537 AU |
Perihelion | 1.2872 AU |
Semi-major axis | 3.5705 AU |
Eccentricity | 0.6395 |
Orbital period | 6.75 a |
Inclination | 17.864° |
Last perihelion | 2017 Feb. 26?
[1] (unobserved) |
Next perihelion | ≈2025-Jan-01?
[1]
[2] ( Lost since 1969) [3] |
18D/Perrine–Mrkos is a periodic comet in the Solar System, originally discovered by the American-Argentine astronomer Charles Dillon Perrine ( Lick Observatory, California, United States) on December 9, 1896. For some time it was thought to be a fragment of Biela's Comet. [4]
It was considered lost after the 1909 appearance, but was rediscovered by the Czech astronomer Antonín Mrkos ( Skalnate Pleso Observatory, Slovakia) on October 19, 1955, using ordinary binoculars, it was later confirmed as 18D by Leland E. Cunningham ( Leuschner Observatory, University of California, Berkeley).
The comet was last observed during the 1968 perihelion passage when it passed 0.3144 AU (47,030,000 km; 29,230,000 mi) from the Earth. [5] The comet has not been observed during the following perihelion passages: [1]
The next predicted perihelion passage would be on 2025-Jan-01 [1] [2] but the comet is currently considered lost as it has not been seen since Jan 1969. [3]
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