79P/du Toit–Hartley
| Discovery | |
|---|---|
| Discovered by | Daniel du Toit, Boyden Observatory, South Africa and Malcolm Hartley of the UK Schmidt Telescope Unit, Siding Spring, Australia |
| Discovery date | 9 April 1945 |
| Designations | |
| 1987 IX, 1986q, 79P/1982 C1-A, 1982 II, 1982b, 79P/1945 G1, 1945 II, 1945c | |
| Orbital characteristics | |
| Epoch | 9 December 2014 |
| Aphelion | 4.83 AU |
| Perihelion | 1.1233 AU |
| Semi-major axis | 2.9460 AU |
| Eccentricity | 0.6187 |
| Orbital period | 5.06 a |
| Inclination | 3.145° |
| Last perihelion | 23 Aug 2013 |
| Next perihelion | 13 Sep 2018[1] |
79P/du Toit–Hartley or du Toit 2 is a periodic comet, now divided into two parts, in the Solar System with an orbital period of 5.06 years.
It was originally discovered by Daniel du Toit at the Boyden Observatory, Bloemfontein, South Africa (then administered by Harvard College) on 9 April 1945 with a brightness of apparent magnitude 10.[2]
Uncertainties in the calculation of the orbit meant the comet was lost until rediscovered by Malcolm Hartley of the UK Schmidt Telescope Unit, Siding Spring, Australia in 1982, when it was found to have broken into two parts, probably in 1976. Both parts had a brightness of magnitude 17. Observed in 1987, it was missed in 1992 but rediscovered by astronomers at Los Molinos Observatory, Uruguay on 4 March 2003 at magnitude 17.
See also
References
- ^ MPC
- ^ "79P/du Toit-Hartley". Cometography. Retrieved 25 February 2015.
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