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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).
Kredit:ESO
O snímku
| Id: | eso9938a |
| Typ: | Mapa |
| Datum zveřejnění: | 29. července 1999 |
| Související články: | eso9938 |
| Velikost: | 1053 x 702 px |
O objektu
| Jméno: | Iota Horologii |
| Typ: | Milky Way : Star Milky Way : Star : Circumstellar Material : Planetary System |
| Vzdálenost: | 55 světelné roky |
| Kategorie: | Exoplanets |
Barvy & filtry
| Pásmo | Dalekohled |
|---|---|
| Optický | Coudé Auxiliary Telescope |