 Comet 50P/Arend photographed byGeorge van Biesbroeck on 4 November 1951 | |
| Discovery | |
|---|---|
| Discovered by | Sylvian Arend |
| Discovery date | 4 October 1951[1] |
| Designations | |
| P/1951 T1, P/1959 N1 | |
| |
| Orbital characteristics | |
| Epoch | 21 November 2025 (JD 2461000.5) |
| Aphelion | 6.252AU |
| Perihelion | 1.922 AU |
| Semi-major axis | 4.087 AU |
| Eccentricity | 0.5297 |
| Orbital period | 8.26a |
| Inclination | 19.100° |
| Last perihelion | 12 May 2024[2] |
| Next perihelion | 7 August 2032[3] |
| Physical characteristics[4] | |
Mean radius | 0.95 km (0.59 mi) |
| 0.04 (assumed) | |
| |
| Comet total magnitude (M1) | 13.9[5] |
Comet Arend or50P/Arend is aperiodic comet in theSolar System which was discovered on October 4, 1951.[1] It was discovered byastronomerSylvain Julien Victor Arend[1] at theRoyal Observatory of Belgium located in themunicipality of Uccle. The comet was illustrated at approximately a magnitude of 14 and also exhibited a nucleus within a coma 14 arc seconds across. It has been observed on its every subsequent apparition since discovery, with the most recent one occurred in 2024. The comet's next perihelion will be in the year 2032.[3]
50P/Arend was observed at its brightest at amaximum magnitude of 14 when it was discovered in 1951. At the comet's next apparition on September 1, 1959, did not exceed 17 if it had not been for an outburst in November which affected its brightness to magnitude 15.5. The observedorbital period was 7.8 years at the time of its discovery however at each succeeding perihelion has led to less favorable observations due to its 0.64astronomical units (AU) as it approachedJupiter in 1969, even if its maximum magnitude was 15. This approach also led to the comet's orbital period to increase to 8.0 years.[1]
Long-term motion studies conducted byBrian G. Marsden on the comet 50P/Arend renders the comet's orbital eccentricity at 0.5 which makes it relatively undisturbed by Jupiter over the last 200-year cycles despite as passage of only 0.49 AU.[1][6][7][8] The study was conducted inside the interval wherelibration happens. Several comets, namely 50P/Arend,4P/Faye,6P/d'Arrest,22P/Kopff,36P/Whipple,78P/Gehrels,92P/Sanguin,4015 Wilson-Harrington, and128P/Shoemaker-Holt, were observed at thePalomar Observatory.Visible coma activity was only observed from 4P/Faye and 50P/Arend out of the 9 other comets from data obtained in May 2000 and March 2001.[9] There have been 1069 observations from October 8, 1951, to February 19, 2008, also where itsmean residual is at 0".60.[10]
The nucleus of the comet has a radius of 0.95 ± 0.03 kilometers, assuming ageometric albedo of 0.04.[4]
| Numbered comets | ||
|---|---|---|
| Previous 49P/Arend–Rigaux | 50P/Arend | Next 51P/Harrington |
.png)
