 The comet on 20 April 1917, as seen from Australia | |
| Discovery[1] | |
|---|---|
| Discovered by | John E. Mellish |
| Discovery date | 19 March 1917 |
| Designations | |
| 1917 I, 1917a | |
| Orbital characteristics[3] | |
| Epoch | 31 March 1917 (JD 2421318.5) |
| Observation arc | 38 days – 1,724 years |
| Earliestprecovery date | December 193 AD?[2] |
| Number of observations | 11 |
| Orbit type | Halley-type |
| Aphelion | 54.61 AU |
| Perihelion | 0.190 AU |
| Semi-major axis | 27.398 AU |
| Eccentricity | 0.9931 |
| Orbital period | 143.416 years |
| Inclination | 32.687° |
| 88.675° | |
| Argument of periapsis | 121.314° |
| Last perihelion | 11 April 1917 |
| Next perihelion | ~2060 |
| TJupiter | 0.644 |
| EarthMOID | 0.0618 AU |
| JupiterMOID | 1.5342 AU |
| Comet total magnitude (M1) | 11.0 |
C/1917 F1 (Mellish), also known asComet 1917Ι and1917a, is aHalley-type comet discovered byJohn E. Mellish on 19 March 1917. The comet has an orbital period of 143 years and last passed perihelion on 11 April 1917. It is the parent body of the DecemberMonocerotids and has also been suggested to be the parent body of daytime kappa Leonids,[4] April ρ-Cygnids, November Orionids, andCanis-Minoridsmeteor showers.[5][6]
The comet upon discovery was in the constellation ofAries and it was located low in the sky and was very condensed. On 23 March a short tail was reported.[1] After perihelion, on 11 April, the comet nucleus was reported to be very bright on 14 April, with a report mentioning it was brighter thanVenus,[7] while it developed a tail that measured 10 degrees in length. The comet faded quickly and by the end of April it was of 5th magnitude and the comet's tail was three degrees long.[8]
The comet has an orbital period of about 145 years, and thus fits the definition of Halley-type comets, which have an orbital period between 20 and 200 years. Its orbital period is similar tocomet Swift-Tuttle, the parent body of thePerseids. The comet has a relatively small perihelion distance, about 0.19 AU (28 million km; 18 million mi).[9] The minimum orbit intersection distance with Earth is 0.06 AU (9.0 million km; 5.6 million mi) while the same distance from Venus is 0.0084 AU (1.26 million km; 0.78 million mi), and could create a meteor shower in Venus.[10]
In 1979, Ichiro Hasegawa tentatively identified a comet observed in December 193 CE as a previous apparition of C/1917 F1 (Mellish).[2]
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