Life Beyond the Habitable Zone
Can radioactive decay keep a planet warm enough that it could host liquid water — and life — even outside of its star’s habitable zone?
Can radioactive decay keep a planet warm enough that it could host liquid water — and life — even outside of its star’s habitable zone?
Planet-finding missions don’t just help us discover new planets — they can also be used to study internal motions in stars!
Why are some cluster stars unusually bright and blue? A closer look at the Collinder 261 open cluster sheds some light on these straggling members.
Collisions of tiny galaxies may be responsible for forming the black-hole binaries that we’ve recently seen merge.
How can solar physicists analyze their mountains of observational data? A new Python-based software package may help.
Why do many young stars undergo bright outbursts? New observations of a flaring system may provide an answer.
What were the first galaxies up to? New radio observations tell us about star formation when the universe was only a billion years old.
A recent study has unveiled a new discovery at the heart of globular cluster Omega Centauri: five long-anticipated pulsars.
The Parker Solar Probe has already flown closer to the Sun than any other spacecraft ever has. What have we learned from early observations?
What do we know about the second object to visit us from another stellar system? Detailed Hubble images have given us plenty to consider!