Discovery | |
---|---|
Discovery date | November 6, 1892 |
Designations | |
1892 V1; 1892 III; 1892f; 1899 L1; 1899 II; 1899d; 1906 III; 1906f; 1964 O1; 1964 X; 1964i; 1972 I; 1971b; 1979 IV; 1979f; 1986 V; 1986f; 1993 VII; 1993i | |
Orbital characteristics | |
Epoch | October 27, 2007 (JD 2454400.5) |
Aphelion | 5.183610 AU |
Perihelion | 2.053218 AU |
Semi-major axis | 3.618414 AU |
Eccentricity | 0.432564 |
Orbital period | 6.882994 a |
Inclination | 19.1126° |
Last perihelion | February 19, 2021[1][2] March 27, 2014 May 4, 2007 |
Next perihelion | January 31, 2028[3][4] |
Comet Holmes /ˈhoʊmz/ (official designation: 17P/Holmes) is a periodic comet in the Solar System, discovered by the British amateur astronomer Edwin Holmes on November 6, 1892. Although normally a very faint object, Holmes became notable during its October 2007 return when it temporarily brightened by a factor of a million, in what was the largest known outburst by a comet, and became visible to the naked eye.[5] It also briefly became the largest object in the Solar System, as its coma (the thin dissipating dust ball around the comet) expanded to a diameter greater than that of the Sun (although its mass remained minuscule).[6] Between 1857–2106 perihelion remains between 2.05–2.36 AU.[7]