In today's world, 178P/Hug–Bell has become a topic of great relevance and interest to many people. It has become a point of discussion and debate in different areas, whether on a personal, professional or academic level. The impact of 178P/Hug–Bell has been felt in society in a significant way, generating conflicting opinions and triggering research and studies that seek to delve deeper into its implications. Since its inception, 178P/Hug–Bell has captured the attention of millions of people around the world, sparking genuine interest and motivating professionals and experts to address its various facets and dimensions. In this context, it is important to fully explore the role of 178P/Hug–Bell today and its influence on daily life, as well as reflect on its projection in the future.
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Discovery | |
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Discovered by | Gary Hug and Graham E. Bell |
Discovery date | December 10, 1999 |
Designations | |
1999 X1, 2006 O1 | |
Orbital characteristics | |
Epoch | July 7, 2013 |
Aphelion | 5.405 AU |
Perihelion | 1.9337 AU |
Semi-major axis | 3.6993 AU |
Eccentricity | 0.4730 |
Orbital period | 7.03 a |
Inclination | 10.9755° |
Last perihelion | 2020-Jul-16[1] July 23, 2013[2] July 6, 2006 |
Next perihelion | 2027-Jun-21[3] |
178P/Hug–Bell is a periodic comet in the Solar System. It was discovered by Northeast Kansas Amateur Astronomers' League members Gary Hug and Graham Bell and is thought to be the first periodic comet to be discovered by amateurs. It was declared a comet less than two days after its initial discovery, after having its course confirmed on previous images.[4]
Hug-Bell's orbital period is about seven years; its orbit is eccentric, though less so than many comets. Hug-Bell's orbit lies entirely outside the orbit of Mars, but at its aphelion overlaps in solar distance with the orbit of Jupiter. Because it never comes closer to the Sun than about 2 AU, it is never expected to be a very bright comet, with a typical perihelion magnitude of 18–19.[5]