C/1948 V1 Explained

C/1948 V1
Discovery Date:1 November 1948
Designations:Eclipse Comet of 1948
1948 V1
1948 XI
Observation Arc:137 days
Obs:17
Epoch:10 January 1949 (JD 2432926.5)
Semimajor:1,574.79 AU
Perihelion:0.1354 AU
Aphelion:3,149.44 AU
Eccentricity:0.9999
Inclination:23.116°
Asc Node:211.043°
Arg Peri:107.249°
Period:62,494.39 years
Tjup:0.423
Earth Moid:0.1883 AU
Jupiter Moid:1.8182 AU
Last P:27 October 1948
M1:9.0
Magnitude:–1.0
(1948 apparition)
B Semimajor:1,931 AU -->
B Period:~84,800 years -->

The Eclipse Comet of 1948, formally known as C/1948 V1, was an especially bright comet discovered during a solar eclipse on November 1, 1948. Although there have been several comets that have been seen during solar eclipses, the Eclipse Comet of 1948 is perhaps the best-known; it was however, best viewed only from the Southern Hemisphere.

When it was first discovered during totality, it was already quite bright, at magnitude –1.0; as it was near perihelion, this was its peak brightness. Its visibility during morning twilight improved as it receded outward from the Sun; it peaked near zero magnitude, and at one point displayed a tail roughly 30 degrees in length, before falling below naked eye visibility by the end of December.