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.

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ESO

Om bilden

ID:eso9938b
Typ:Diagram
Publiceringsdatum:29 juli 1999
Relaterade pressmeddelanden:eso9938
Storlek:1045 x 705 px

Om objektet

Namn:Iota Horologii
Typ:Milky Way : Star : Circumstellar Material : Planetary System
Avstånd:55 ljusår
Kategori:Exoplanets

Bildformat

Originalstorlek
95,8 kB
Stor jpeg
99,7 kB
Skärmstor jpeg
94,1 kB