There’s always more to learn about epsilon Eridani– the nearest sun-like star that hosts an exoplanet. These authors work to determine the emission processes and physics associated with radio emission detected from epsilon Eridani in 2020.
Will Betelgeuse go supernova in the next few decades? This paper suggests so…
How do cool stars vary in the ultraviolet? Why is that important for exoplaneteers to investigate? And what does this have to do with planetary magnetic fields?
Pulsating flares on M dwarfs can disrupt the atmospheres of exoplanets. However, in just the right amounts, they could be the genesis of primordial life. Today’s paper describes how!
Betelgeuse faded dramatically in 2019 and 2020. Fortunately a team of star doctors…(err, astrophysicists) have diagnosed the problem!
HAT-P-7b was one of the first exoplanets with evidence of atmospheric variability, but hold off on your application to be its resident weather forecaster! Today’s paper casts a shadow on the original detection…