Sorry! This page is not yet available in your preferred language, so we're displaying the original version instead.
Velocity variation of mu Arae observed by HARPS
Illustration of the high-quality radial velocity measurements obtained with HARPS. Here also, the solid line shows the best fit to the measurements, assuming the existence of two planets. The data were obtained over a time span of 80 days and the first points shown are the data from the 8 nights in June. Note that the full span of the vertical axis is only 40 m/s! Error bars indicate the accuracy of the measurements. The lower part of the diagram displays the deviation of the measurements from the best fit.
Kredit:ESO
O snímku
Id: | eso0427c |
Typ: | Mapa |
Datum zveřejnění: | 25. srpna 2004 |
Související články: | eso0427 |
Velikost: | 800 x 794 px |
O objektu
Jméno: | mu Arae |
Typ: | Milky Way : Star : Spectral Type : G Milky Way : Star : Circumstellar Material : Planetary System |
Vzdálenost: | 50 světelné roky |
Kategorie: | Exoplanets |