HD 217107 b
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| Extrasolar planet | Lists of extrasolar planets | |
|---|---|---|
| Orbital elements | ||
| Semimajor axis | (a) | 0.074 ± 0.002 AU |
| Eccentricity | (e) | 0.13 ± 0.02 |
| Orbital period | (P) | 7.1269 ± 0.00022 d |
| Inclination | (i) | ?° |
| Longitude of periastron |
(ω) | 21.1° |
| Time of periastron | (τ) | 2,449,998.4241 ± 0.17 JD |
| Physical characteristics | ||
| Mass | (m) | >1.37 ± 0.14 MJ |
| Radius | (r) | ? RJ |
| Density | (ρ) | ? kg/m3 |
| Temperature | (T) | ? K |
| Discovery information | ||
| Discovery date | 1998 | |
| Discoverer(s) | Marcy et al. | |
| Detection method | Doppler Spectroscopy | |
| Discovery status | Confirmed | |
HD 217107 b is an extrasolar planet orbiting the Sun-like star HD 217107 every 7.1 days. It is the innermost known planet in its system, and was discovered by the California and Carnegie Planet Search team. It is a 'hot Jupiter' planet, so-called because of its high mass and proximity to its parent star.
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[edit] Discovery
As with the majority of extrasolar planet discoveries so far, it was found by detecting small variations in the radial velocity of the star it orbits, caused by the tug of its gravity. A study of the radial velocity of HD 217107 carried out in 1998 revealed that its motion along the line of sight varied over a 7.1 day cycle. The period and amplitude of this variation indicated that it was caused by a planetary companion in orbit around the star, with a minimum mass slightly greater than that of Jupiter [2]. The planet's mean distance from the star is less than one fifth of Mercury's distance from the Sun.
[edit] Indication of second planet
While most planets with orbital periods of less than 10 days have almost circular orbits, HD 217107 b has a somewhat eccentric orbit, and its discoverers hypothesised that this could be due to the gravitational influence of a second planet in the system at a distance of several astronomical units (AU)[3]. Confirmation of the existence of a second planet, HD 217107 c, followed in 2005
[edit] References
- ^ Vogt S.S., Butler R.P., Marcy G.W., Fischer D.A., Henry G.W., Laughlin G., Wright J.T., Johnson J.A (2005). "Five New Multicomponent Planetary Systems". Astrophysical Journal 632: 638 – 658.
- ^ Fischer D.A., Marcy G.W., Butler R.P., Vogt S.S., Apps K. (1999). "Planetary Companions around Two Solar-Type Stars: HD 195019 and HD 217107". Publications of the Astronomical Society of the Pacific 111: 50 – 56.
- ^ Fischer D.A., Marcy G.W., Butler R.P., Vogt S.S., Frink S., Apps K. (2002). "Planetary Companions to HD 12661, HD 92788, and HD 38529 and Variations in Keplerian Residuals of Extrasolar Planets". Astrophysical Journal 551: 1107 – 1118.
