Named Comets, Part 6 Codexery

50P/Arend

Periodic comet discovered in 1951 by Sylvain Arend.

50P/Arend

50P/Arend is a periodic comet in the Solar System discovered on October 4, 1951, by astronomer Sylvain Julien Victor Arend at the Royal Observatory of Belgium in Uccle. It has been observed at every subsequent apparition since its discovery, with the most recent occurring in 2024, and its next perihelion is predicted for 2032.

Quick Facts

Discoverer
Sylvian Arend
Discovery Date
4 October 1951
Mpc Name
P/1951 T1, P/1959 N1
Designations
1951 X, 1959 V, 1967 VI · 1975 VI, 1983 VIII · 1991 VIII
Epoch
21 November 2025 (JD 2461000.5)
Earliest Precovery Date
1 October 1951
Obs
1,984
Aphelion
6.252 AU
Perihelion
1.922 AU
Semimajor
4.087 AU
Eccentricity
0.5297
Period
8.26a

Facts from the source article.

Lore & Background

At its discovery in 1951, 50P/Arend was observed at a maximum magnitude of 14, with a nucleus within a coma 14 arc seconds across. During its next apparition on September 1, 1959, the comet did not exceed magnitude 17 until an outburst in November raised its brightness to magnitude 15.5. The comet's orbital period was 7.8 years at discovery, but an approach to Jupiter in 1969 at 0.64 AU increased the period to 8.0 years and made subsequent apparitions less favorable for observation, though its maximum magnitude reached 15.

Long-term motion studies by Brian G. Marsden determined the comet's orbital eccentricity at 0.5, indicating it is relatively undisturbed by Jupiter over 200-year cycles despite passing as close as 0.49 AU. In observations at Palomar Observatory in May 2000 and March 2001, visible coma activity was detected only from 50P/Arend and 4P/Faye among nine comets studied. The nucleus has a radius of 0.95 ± 0.03 kilometers, assuming a geometric albedo of 0.04.

Reader's Guide

50P/Arend holds significance as a regularly observed periodic comet that has been tracked at every apparition since its 1951 discovery, providing a long baseline for studying its orbital evolution. Its close approach to Jupiter in 1969 altered its orbital period from 7.8 to 8.0 years, a change documented through continued observations. The comet's relatively stable orbit over 200-year cycles, as shown by Brian G. Marsden's studies, makes it a useful object for understanding long-term dynamics in the inner Solar System. Its detection of visible coma activity in 2000–2001, alongside only one other comet in a survey of nine, highlights its ongoing activity. With 1,069 observations recorded from October 8, 1951, to February 19, 2008, and a mean residual of 0.60 arcseconds, the comet's astrometric data contribute to precise orbital modeling. The measured nucleus radius of 0.95 km provides a physical benchmark for comparing similar periodic comets.

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