Wednesday, May 13, 2015

Kapteyn's Star's Habitable Zone Exoplanet is Really Just Stellar Activity, False Positive

Stellar activity mimics a habitable-zone planet around Kapteyn's star

Authors:

Robertson et al

Abstract:

Kapteyn's star is an old M subdwarf believed to be a member of the Galactic halo population of stars. A recent study has claimed the existence of two super-Earth planets around the star based on radial velocity (RV) observations. The innermost of these candidate planets--Kapteyn b (P = 48 days)--resides within the circumstellar habitable zone. Given recent progress in understanding the impact of stellar activity in detecting planetary signals, we have analyzed the observed HARPS data for signatures of stellar activity. We find that while Kapteyn's star is photometrically very stable, a suite of spectral activity indices reveals a large-amplitude rotation signal, and we determine the stellar rotation period to be 143 days. The spectral activity tracers are strongly correlated with the purported RV signal of "planet b," and the 48-day period is an integer fraction (1/3) of the stellar rotation period. We conclude that Kapteyn b is not a planet in the Habitable Zone, but an artifact of stellar activity.

Robertson killed Gliese 581g, too.   He's going to get a reputation if he keeps this up.  The M Dwarf Planet Killer!

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