In this article, we will explore HD 20782 b in depth, analyzing its impact, its relevance and its implications in today's society. From its emergence to the present, HD 20782 b has captured the attention of many, generating debate and reflection in various sectors. Throughout this analysis, we will examine the key aspects that make HD 20782 b a topic of interest, as well as its possible repercussions in the social, political, economic and cultural spheres. Through a comprehensive and critical vision, we will seek to fully understand the importance of HD 20782 b in the current context, offering a complete overview that allows the reader to delve into its meaning and scope.
Discovery | |
---|---|
Discovered by | Jones et al. |
Discovery site | Anglo-Australian Planet Search |
Discovery date | March 14, 2006 |
Radial velocity | |
Orbital characteristics | |
1.36 ± 0.12 AU (203,000,000 ± 18,000,000 km) | |
Eccentricity | 0.97 ± 0.01[1] |
585.86 ± 0.03 d | |
2451687.1 ± 2.5 | |
147 ± 3 | |
Semi-amplitude | 115 ± 12 |
Star | HD 20782 |
HD 20782 b is an extrasolar planet located approximately 117 light-years away in the constellation of Fornax, orbiting the star HD 20782.
This planet orbits in the most eccentric orbit known (as of November 2012),[1] with a semi-major axis of 1.36 AU, and eccentricity e=0.97+/-0.01.[2] As a result, it also has one of the most extreme temperature swings.