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

Billedformater

Stor JPEG
99,7 KB
Skrærm JPEG
94,1 KB