C/1948 V1 Explained

C/1948 V1 (Eclipse Comet)
Discovery Date:November 1, 1948
Designations:Eclipse Comet, 1948 XI, 1948 V1
Epoch:2432840.5
Semimajor:1931 AU
Perihelion:0.135 AU
Aphelion:3861 AU
Eccentricity:0.99994
Period:~84,800 yr.[1]
Inclination:23.1°
Last P:October 27, 1948
Next P:unknown

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 -2; as it was near perihelion, this was its peak brightness.[2] 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.[2]

External links

Notes and References

  1. Web site: Horizons output . Barycentric Osculating Orbital Elements for Comet C/2004 Q2 (Machholz) . 2011-02-03. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
  2. Web site: When was the last time we had two bright comets in the same year?. Dr. Sten Odenwald. Ask the Astronomer. 2006-02-13.