i Horologii - radial velocity variations
This chart shows radial velocity measurements (with individual errors shown as bars) of the 5.4-mag solar-type star iota Hor over a period of nearly six years. The thin line indicates the variation that is caused by the new planet (as a best-fit Keplerian orbit).
Credit:ESO
About the Image
Id: | eso9938a |
Type: | Chart |
Release date: | 29 July 1999 |
Related releases: | eso9938 |
Size: | 1053 x 702 px |
About the Object
Name: | Iota Horologii |
Type: | Milky Way : Star Milky Way : Star : Circumstellar Material : Planetary System |
Distance: | 55 light years |
Category: | Exoplanets |
Colours & filters
Band | Telescope |
---|---|
Optical | Coudé Auxiliary Telescope |