In this article we will be analyzingHD 4208 b, a topic that has generated great interest and debate in contemporary society. _Var1 has proven to be a point of discussion in different areas, from politics to science, including culture and technology. Its relevance and impact on everyday life make it a topic of interest to a wide variety of people, regardless of age, gender, socioeconomic level or geographic location. Throughout this article we will explore different aspects of HD 4208 b, analyzing its origin, evolution, impact and possible future implications. In addition, we will address various perspectives and opinions on the matter, with the aim of offering a broad and enriching vision on this topic that is so relevant today.
Discovery | |
---|---|
Discovered by | California and Carnegie Planet Search |
Discovery site | Keck telescope |
Discovery date | 15 October 2001 |
Doppler Spectroscopy | |
Orbital characteristics | |
Apastron | 1.736 AU (259,700,000 km) |
Periastron | 1.564 AU (234,000,000 km) |
1.650 ± 0.096 AU (246,800,000 ± 14,400,000 km) | |
Eccentricity | 0.052 ± 0.040 |
828.0 ± 8.1 d 2.267 y | |
2,451,040 ± 120 | |
345 | |
Semi-amplitude | 19.06 ± 0.73 |
Star | HD 4208 |
Physical characteristics | |
Mass | >0.804 ± 0.073 MJ |
HD 4208 b, officially named Xolotlan, is an extrasolar planet discovered by the California and Carnegie Planet Search team using the Keck telescope. The planet is probably somewhat less massive than Jupiter, although only its minimum mass is known. Its orbital distance is 1.67 AU, slightly further than Mars, and its eccentricity is low.[1][2]
The planet HD 4208 b is named Xolotlan. The name was selected in the NameExoWorlds campaign by Nicaragua, during the 100th anniversary of the IAU. Xolotlan is the name of Lake Managua in Nahuatl language.[3][4]