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From Wikipedia, the free encyclopedia
Comet Machholz, formally designated C/2004 Q2, is a long-period comet discovered by Donald Machholz on August 27, 2004. It reached naked eye brightness in January 2005. Unusual for such a relatively bright comet, its perihelion was farther from the Sun than the Earth's orbit.
Comet Machholz in February 2005 | |
| Discovery | |
|---|---|
| Discovered by | Donald Machholz |
| Discovery date | 2004 |
| Designations | |
| Comet Machholz | |
| Orbital characteristics | |
| Epoch | 2453415.5 (February 14, 2005) |
| Aphelion | ~5000 AU (inbound)[1] ~1100 AU (outbound) |
| Perihelion | 1.205 AU |
| Eccentricity | 0.9995 |
| Orbital period | ~130,000 yr (inbound)[1] ~12,400 yr (outbound) |
| Inclination | 38.6° |
| Last perihelion | January 24, 2005 |
Given the orbital eccentricity of this object, different epochs can generate quite different heliocentric unperturbed two-body best-fit solutions to the aphelion distance (maximum distance) of this object. For objects at such high eccentricity, the Suns barycentric coordinates are more stable than heliocentric coordinates. Using JPL Horizons the barycentric orbital elements for epoch 2050 generate a semi-major axis of 537 AU and a period of approximately 12,400 years.[1]
There are six other long-period comets named Machholz: C/1978 R3 (a.k.a. 1978 XIII, 1978l), C/1985 K1 (a.k.a. 1985 VIII, 1985e), C/1988 P1 (a.k.a. 1988 XV, 1988j), C/1992 N1 (a.k.a. 1992 XVII, 1992k), C/1994 T1 (a.k.a. 1994 XXVII, 1994r), and C/2010 F4. In addition, there are C/1992 F1 (Tanaka-Machholz), C/1994 N1 (Nakamura-Nishimura-Machholz) and C/2018 V1 (Machholz-Fujikawa-Iwamoto).
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