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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.
Crédito:ESO
Sobre la imagen
Identificador: | eso0427c |
Tipo: | Mapa |
Fecha de publicación: | 25 de Agosto de 2004 |
Noticias relacionadas: | eso0427 |
Tamaño: | 800 x 794 px |
Sobre el objeto
Nombre: | mu Arae |
Tipo: | Milky Way : Star : Spectral Type : G Milky Way : Star : Circumstellar Material : Planetary System |
Distancia: | 50 años luz |
Categoría: | Exoplanets |