Learning from LIGO’s Second Binary Neutron Star Detection
LIGO’s second observation of colliding neutron stars carries with it some interesting uncertainties and implications.
LIGO’s second observation of colliding neutron stars carries with it some interesting uncertainties and implications.
A new study explores how clouds might affect our ability to search for signs of water vapor in potentially habitable planet atmospheres.
What happens when the large-scale drama of a violent galaxy merger plays out on small scales for a pair of dwarf galaxies?
The discovery of nine more repeating fast radio bursts brings us a little closer to understanding their origin.
What can infrared emission from black hole X-ray binaries tell us about the speeds of their powerful jets?
A new study proposes that the rings and spirals we see in protoplanetary disks may have a dramatic origin.
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.