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.

Të drejtat:

ESO

Rreth fotografisë

Id:eso0427c
Tipi:Hartë
Data e Publikimit:25 Gusht 2004
Publikime të ngjashme:eso0427
Përmasat:800 x 794 px

Rreth objektit

Emri:mu Arae
Tipi:Milky Way : Star : Spectral Type : G
Milky Way : Star : Circumstellar Material : Planetary System
Distanca:50 vite dritë
Kategori:Exoplanets

Formate Fotografish

JPEG i madh
101,3 KB

 

Shih dhe