The search for extrasolar life is a multidisiplinary endeavor. How can astronomers use current understandings of pre-cellular biology to inform what it means for a planet to be “habitable”?
Today’s paper takes a prospective look at possible concerns for future gravitational wave observations, and finds that perhaps no concern is needed.
Today’s paper takes a look at circumstellar disks’ chemistries, and addresses how their chemical composition can be impacted by their host stars.
