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.
Credit:ESO
About the Image
Id: | eso0427c |
Type: | Chart |
Release date: | 25 August 2004 |
Related releases: | eso0427 |
Size: | 800 x 794 px |
About the Object
Name: | mu Arae |
Type: | Milky Way : Star : Spectral Type : G Milky Way : Star : Circumstellar Material : Planetary System |
Distance: | 50 light years |
Category: | Exoplanets |