14 Herculis c
.png)
| |
| Odkrywca |
Goździewski et al.[1] |
|---|---|
| Data odkrycia |
2005 |
| Charakterystyka orbity (J2000) | |
| Półoś wielka | |
| Mimośród |
0,0[2] |
| Okres orbitalny |
6906 ± 70[2] |
| Czas przejścia przez perycentrum | |
| Charakterystyka fizyczna | |
| Masa minimalna (M·sin i) | |
14 Herculis c – niepotwierdzona planeta pozasłoneczna orbitująca wokół gwiazdy 14 Herculis. Jeśli istnieje, najprawdopodobniej należy do grupy gazowych olbrzymów, takich jak Jowisz czy Saturn.
Przypisy
- ↑ Krzysztof Goździewski, Maciej Konacki, Andrzej J. Maciejewski. Orbital Configurations and Dynamical Stability of Multiplanet Systems around Sun-like Stars HD 202206, 14 Herculis, HD 37124, and HD 108874. „The Astrophysical Journal”. 645 (1), s. 688-703, 2006-07-01. DOI: 10.1086/504030. (ang.).
- ↑ a b c d e Robert A. Wittenmyer, Michael Endl, William D. Cochran. Long-Period Objects in the Extrasolar Planetary Systems 47 Ursae Majoris and 14 Herculis. „The Astrophysical Journal”. 654 (1), s. 625-632, 2007-01-01. DOI: 10.1086/509110. (ang.).
Linki zewnętrzne
- 14 Herculis c w serwisie The Exoplanet Encyclopaedia (ang.)
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