![]() Comet Humason photographed from the Palomar Observatory on 4 September 1962 | |
Discovery | |
---|---|
Discovered by | Milton L. Humason |
Discovery date | 1 September 1961 |
Designations | |
1961e 1962 VIII | |
Orbital characteristics [1] | |
Epoch | 12 May 1963 (JD 2438161.5) |
Observation arc | 1,517 days (4.15 years) |
Number of observations | 80 |
Aphelion | 408.71 AU |
Perihelion | 2.133 AU |
Semi-major axis | 205.42 AU |
Eccentricity | 0.98961 |
Orbital period | 2,883 years (inbound) 2,516 years (outbound) |
Inclination | 153.278° |
155.439° | |
Argument of periapsis | 233.562° |
Last perihelion | 10 December 1962 |
TJupiter | –1.588 |
Earth MOID | 1.2247 AU |
Jupiter MOID | 1.0725 AU |
Physical characteristics [2] [3] | |
Dimensions | 30–41 km (19–25 mi) |
Comet total magnitude (M1) | 1.35–3.5 |
Comet nuclear magnitude (M2) | 10.1 |
Comet Humason, formally designated C/1961 R1 (a.k.a. 1962 VIII and 1961e), was a non-periodic comet discovered by Milton L. Humason on 1 September 1961. Its perihelion was well beyond the orbit of Mars, at 2.133 AU. The outbound orbital period is about 2,516 years.
It was a "giant" comet, much more active than a normal comet for its distance to the Sun, with an absolute magnitude of 1.35−3.5, [3] and a nucleus diameter estimated at 30–40 km (19–25 mi). [2] It could have been up to a hundred times brighter than an average new comet. It had an unusually disrupted or "turbulent" appearance. [4] It was also unusual in that the spectrum of its tail showed a strong predominance of the ion CO +, a result previously seen unambiguously only in C/1908 R1 (Morehouse). [5]
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