Betelgeuse’s Companion Star May Have Been Seen at Last
Finally found: using speckle imaging, researchers have spotted what is likely the predicted 1.6-solar-mass companion to the red supergiant Betelgeuse.
Finally found: using speckle imaging, researchers have spotted what is likely the predicted 1.6-solar-mass companion to the red supergiant Betelgeuse.
What’s responsible for the haphazard orbits of the stars closest to our galaxy’s supermassive black hole? A second black hole, perhaps.
One of the first-look images from the Vera C. Rubin Observatory contained a rare find: a candidate circumstellar or protoplanetary disk in a region where few such disks have been discovered.
A search for oddities in archival JWST data has turned up something remarkable: a rare pair of collisional ring galaxies that may have birthed a supermassive black hole during their clash.
A recently discovered tidal disruption event has astronomers investigating new ways in which stars may be ripped apart by supermassive black holes.
A new method for handling data with significant gaps can be applied to extremely sparse datasets, such as Voyager data from the outer heliosphere.
New research suggests that JWST is capable of directly imaging planets that resemble the gas giants in our solar system, provided they orbit nearby stars.
A team of citizen scientists compared 5.4 million pairs of astronomical images, helping researchers create a database of image similarity information that can be used to test image-search algorithms.
With their extremely low surface brightness, ultra-diffuse galaxies are very difficult to detect, but a recent study has spotted one by searching for its globular clusters.
The massive nearby elliptical galaxy Messier 87 hosts one of the most-studied supermassive black holes in the universe. What have researchers recently learned about this black hole’s spin, jets, and flares?