text:   Planet-Hosting Solar-type Star: Kepler 17",4,"['Our new paper ""Temporal Evolution of Spatially-Resolved Individual Star Spots on a Planet-Hosting Solar-type Star: Kepler 17""  is accepted to ApJ and now in arXiv !!  <LINK> \n\nAuthors:  @KosOlo8, @jradavenport, @brettmor  @astronomy_stars , and many !', '@KosOlo8 @jradavenport @brettmor Using exoplanet transits and rotational modulations of Kepler-17,we investigated number of spots, spot locations, and the temporal evolution. Although the temporal evolution derived from the rotational modulation differs from those of in-transit spots to a certain degree, ..... https://t.co/p0kcZKulA8', '@KosOlo8 @jradavenport @brettmor .... the emergence/decay rates of in-transit spots are within an order of magnitude of those derived for sunspots as well as our previous research based only on rotational modulations.  This supports a hypothesis that .... https://t.co/vyS3JAIkvu', '@KosOlo8 @jradavenport @brettmor ....  that the emergence/decay of sunspots and extremely-large star spots on solar-type stars occur through the same underlying processes.\n\nAlso, we can say large star spots having a potential to produce superflares are found to survive more than\n100 days (up to 1 year)...😲 https://t.co/LQ4TMDwgWr']",20,02,1140