MASS IS A FUNDAMENTAL PROPERTY OF STARS AND IS NOTORIOUSLY DIFFICULT TO MEASURE FOR RED GIANT (RG) STARS. THE PHOTOMETRY PROVIDED BY TESS AND KEPLER HAS PROVEN TO BE A VITAL RESOURCE FOR MEASURING ACCURATE RG MASSES THANKS TO THE SCALING RELATIONS
$26,732FY2021National Aeronautics and Space AdministrationNASA
Association Of Universities For Research In Astronomy, Inc., Tucson AZ