Ursäkta oss! Den här sidan finns ännu inte på ditt språk. Vi visar istället originalversionen.
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.
Källa:ESO
Om bilden
ID: | eso0427c |
Typ: | Diagram |
Publiceringsdatum: | 25 augusti 2004 |
Relaterade pressmeddelanden: | eso0427 |
Storlek: | 800 x 794 px |
Om objektet
Namn: | mu Arae |
Typ: | Milky Way : Star : Spectral Type : G Milky Way : Star : Circumstellar Material : Planetary System |
Avstånd: | 50 ljusår |
Kategori: | Exoplanets |