Radial Velocity Curve of HD 47536
Radial velocity curve of HD 47536, caused by the pull of the orbiting planet during the 712-day period (abscissa: Julian Date - 2,400,000; ordinate: velocity in kilometres per second along the line-of-sight). Error bars indicate the accuracy of the measurements. The fully-drawn curve is the computed velocity curve, corresponding to the best-fitting planetary orbit. The lower part of the diagram displays the deviation of the measurements from this curve — in the mean about 0.025 km/sec, or 25 m/sec.
Credit:
ESO
About the Image
| Id: | eso0305c |
| Type: | Chart |
| Release date: | 22 January 2003 |
| Related releases: | eso0305 |
| Size: | 800 x 781 px |
About the Object
| Name: | HD 47536 |
| Type: | • Milky Way : Star : Spectral Type : K • X - Stars |
| Distance: | 400 light years |
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