KOI-961 is an M-dwarf with transit signals of at least three short-period planets. The properties of the star are very similar to those of Barnard's star, the fourth closest star to the Sun. All planets in the system are very close to their host star and thought to be rocky. The system is more similar in size to Jupiter and its moons than any other planetary system. 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.