![]() Comet Russell 4 imaged by Kevin Heider on 19 February 2010 while it was 2.2 AU from the Sun. | |
Discovery | |
---|---|
Discovered by | Kenneth S. Russell |
Discovery date | 7 March 1984 |
Designations | |
1984 I;1990 XI | |
Orbital characteristics [1] [2] | |
Epoch | October 1, 2009 |
Aphelion | 4.793 AU (Q) |
Perihelion | 2.240 AU (q) |
Semi-major axis | 3.517 AU (a) |
Eccentricity | 0.3630 |
Orbital period | 6.60 yr |
Inclination | 6.182° |
Last perihelion | 21 May 2023 |
Next perihelion | 17 December 2029 [3] |
Physical characteristics | |
Mean radius | 2.6 km (1.6 mi) [4] |
20.7 hours [5] | |
0.043±0.007 | |
(V–R) = 0.62±0.05 [6] |
94P/Russell 4 is a periodic comet in the Solar System.
It was discovered by Kenneth S. Russell on photographic plates taken by M. Hawkins on March 7, 1984. [7] In the discovery images, Russell estimated that the comet had an apparent magnitude of 13 and a noticeable tail of 5 arcminutes. [7] In the year of discovery, the comet had come to perihelion in January 1984. [8]
With an aphelion of 4.7 AU (700 million km), [1] comet 94P currently has an orbit contained completely inside of the orbit of Jupiter. It fits the definition of an Encke-type comet with (TJupiter > 3; a < aJupiter). [1]
In July 1995, 94P was estimated to have a radius of about 2.6 km (1.6 mi) with an absolute magnitude (H) of 15.1. [4] It may have a very elongated nucleus with an axial ratio of a/b ≥ 3. [4] It is determined that it has a rotation period of 20.7 hours. [5]