Kepler-91 b is a planet very close its host star. It might be destroyed within the next 55 million years. The planet was initially discovered by the Kepler telescope and later confirmed by a group of European researchers led by Jorge Lillo-Box. The radial velocities of the star show a linear trend after fitting the variations due to the planet. Link to scientific paper Your name Note: Your commit will be vetted before it is merged into the public version. It is crucial that you include a link to a scientific publication. For more information on the meaning of the different datafields see the readme file in the Open Exoplanet Catalogue repository on github.