An Exoplanet With a 350,000-Mile-Long Comet-Like Tail
New W. M. Keck Observatory data confirms exoplanet WASP-69b, known for its escaping atmosphere, is forming a comet-like tail that’s significantly longer than previously observed — at least 350,000 miles long! A UCLA-led team successfully detected this Jupiter-sized planet’s atmospheric mass-loss in real-time.
Artist’s impression of WASP-69b orbiting its host star.
Origin of Rare Radio Circles Revealed
New data reveals the origin of odd radio circles (ORCs), which are so large they contain entire galaxies in their centers. A UC San Diego-led team used Keck Observatory’s Keck Cosmic Web Imager to study the first ORC discovered from the Northern Hemisphere. Their detective work revealed these rare radio rings are formed by outflowing galactic winds, possibly from massive stars that go supernova.
Odd radio circles are large enough to contain galaxies.
Strange New Luminous Fast Blue Optical Transient
Astronomers are baffled by a recent discovery of a mysterious and rare event called a Luminous Fast Blue Optical Transient (LFBOT). Typically, they explode once and fade within a few days. But this particular LFBOT, nicknamed the “Tasmanian Devil,” continued to produce a series of strange, extremely bright repetitive flares that lasted for months, emitting more energy than hundreds of billions of stars like our Sun combined.