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i Horologii - radial velocity variations
The combined radial velocity variations of iota Hor vrs. orbital phase of the newly discovered planet. The planet is in front of the star near phase 0.5 and on the other side at phase 0 and 1. The maximal velocities are when the planet is approaching or receding around 0.25 and 0.75, respectively. The orbital period is 320 days.
Kilde:ESO
Om billedet
Id: | eso9938b |
Type: | Diagram |
Udgivelsesdato: | 29. juli 1999 |
Relaterede pressemeddelelser: | eso9938 |
Størrelse: | 1045 x 705 px |
Om objektet
Navn: | Iota Horologii |
Type: | Milky Way : Star : Circumstellar Material : Planetary System |
Afstand: | 55 lysår |
Kategori: | Exoplanets |