Today, C/1861 G1 (Thatcher) is a topic that has captured the attention of people of all ages and from different parts of the world. The importance of C/1861 G1 (Thatcher) in today's society has generated extensive debate and led to increased interest in understanding its implications in our daily lives. From its origins to its impact on the present, C/1861 G1 (Thatcher) has been the subject of numerous investigations, discussions and analyzes that seek to shed light on its multiple dimensions. In this article, we will explore in depth the different aspects of C/1861 G1 (Thatcher) and its influence on our environment, with the aim of providing a comprehensive and updated vision of this very relevant topic.
Discovery | |
---|---|
Discovered by | A. E. Thatcher |
Discovery date | April 5, 1861 |
Designations | |
1861 I | |
Orbital characteristics | |
Observation arc | 149 days |
Number of observations | 187 |
Orbit type | Long period comet |
Aphelion | 112 AU (beyond Eris) |
Perihelion | 0.921 AU (1861) 0.917 AU (2283) |
Semi-major axis | 56.3 AU |
Eccentricity | 0.983 |
Orbital period | 422 yr (barycentric) |
Inclination | 79.77° |
Last perihelion | 1861-Jun-03 |
Next perihelion | 2283 ±5 |
Comet C/1861 G1 (Thatcher) is a long-period comet with roughly a 422-year orbit that is expected to return around 2283. It was discovered by A. E. Thatcher. It is responsible for the April Lyrid meteor shower. Carl Wilhelm Baeker also independently found this comet. The comet passed about 0.335 AU (50.1 million km; 31.1 million mi) from the Earth on 5 May 1861 and last came to perihelion (closest approach to the Sun) on 3 June 1861.
C/1861 G1 is listed as a long-period "non-periodic comet" because it has not yet been observed at two perihelion passages. When it is seen to come back around 2283, it should receive the P/ designation.
The comet is the parent body of the April Lyrids meteor shower.