THE STRUCTURES OF STELLAR INTERIORS ARE KNOWN TO TRANSITION FROM PARTIALLY CONVECTIVE FOR STARS LIKE THE SUN TO FULLY CONVECTIVE AROUND MID-M DWARFS. IN THE PAST IDENTIFYING THE LOCATION OF THE TRANSITION HAS RELIED ON ESTIMATED MASSES OR SPECTRAL
$213,696FY2021National Aeronautics and Space AdministrationNASA
Georgia State University Research Foundation Inc