Starspots to Measure Small Differential Rotation Rates
On using photometric data from Kepler to study starspots, and to measure differential rotation rates.
On using photometric data from Kepler to study starspots, and to measure differential rotation rates.
Very low-mass M-dwarfs are a missing link in our theory of stellar interiors. Stars this small probably have fully convective interiors, but we don’t have a complete understanding of how that affects global properties like radius or temperature. It’s important to get right, if for no other reason because lots of exoplanets orbit M-dwarfs.
For planets too old for plate tectonics, a companion planet could drive tidal heating to keep conditions primed for life.
The low-mass primitive halo star, SDSS J102915+172927, puzzled astronomers because of it’s extremely low metal content. This article aims to answer under what physical conditions can a star like this form.