| Planet | Orbital Elements | Orbital Period (years) | Minimum Mass (ME) | Discovery | ||
|---|---|---|---|---|---|---|
| Designation | Semimajor Axis (AU) | Eccentricity | Discoverer Name | Announcement Date | ||
| HD192263 b | 0.15 | 0 | 0.066667 | 230 | N. Santos, et al | 1999 Sep 28 |
| Photometric brightness variations have been found with the same period as the supposed stellar velocity variations, implying that the velocity variations are caused by starspots, not by a planet; see A False Planet Around HD 192263 (G.Henry, S.Baliunas, R.Donahue) | ||||||
| Additional observations indicate that the radial-velocity variations are indeed being produced by the presence of a planet; see The return of the giant planet orbiting HD192263 | ||||||
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