Here's How We Could Measure the Mass of SgrA* to Within One Solar Mass

By Brian Koberlein - January 14, 2025 02:02 PM UTC | Milky Way
The mass of the Milky Way's supermassive black hole, SgrA*, is roughly 4.3 million times the mass of the Sun, give or take a few hundred thousand solar masses. But a team of astronomers thinks they can dial that accuracy down to know with an error rate of a single solar mass. They propose to do this by measuring gravitational waves from SgrA* as brown dwarfs orbit it closely. These dwarfs act like natural probes mapping out the warped space around SgrA*.
Continue reading

Astronomers are Losing the Night Sky (and Radio Sky) to Satellite Megaconstellations

By Brian Koberlein - January 08, 2025 11:11 AM UTC | Observing
At the end of 2023, there were more than 5,000 satellites orbiting Earth, with 10s of 1000s more on the way. Although individual satellites might be invisible to the unaided eye, their collective light might already be causing a 10% brightness increase in the night sky. Large surveys like Vera Rubin will see frequent satellite trails obscuring important data. And the radio pollution is also increasing with communications satellites. What can be done to restore the sky?
Continue reading

This Fast Radio Burst Definitely Came From a Neutron Star

By Brian Koberlein - January 03, 2025 11:28 AM UTC | Physics
Since the first fast radio burst (FRB) was discovered in 2007, astronomers have been puzzling over their source. These bright radio flashes come from seemingly random directions across the universe. Finally, astronomers have pinned down one FRB to a specific neutron star in a galaxy about 200 light-years away. The FRB was unleashed from a region within 10,000 km of the neutron star and probably emerged from its magnetosphere.
Continue reading