Kaboom kaboom. That’s what an international team of astronomers saw when they tracked the death of one of the most massive stars that can exist.
Japanese supernova hunter, Koichi Itagaki, first discovered an exploding star in the galaxy UGC4904 back in 2004. It flared briefly and then faded away over the course of 10 days. Two years later, he discovered another supernova in exactly the same location.
Subsequent observations with larger telescopes confirmed that the supernova, named SN2006jc, did indeed happen at exactly the same location as the previous detonation. The 2004 event must have just been a large outburst, similar to what was seen on Eta-Carinae back in the 1850s.
The researchers think this kind of event could actually be more common than previously believed. A new survey called Pan-STARRS may check up on previous supernova events to see if there’s any new activity.
Original Source: Queen’s University Belfast News Release
The James Webb Space Telescope (JWST) was specifically intended to address some of the greatest…
The James Webb Space Telescope was designed and built to study the early universe, and…
Titan is one of the solar system's most fascinating worlds for several reasons. It has…
Catching the best sky watching events for the coming year 2025. Comet C/2023 A3 Tsuchinshan-ATLAS…
For decades cosmologists have wondered if the large-scale structure of the universe is a fractal:…
A current mystery in astronomy is how supermassive black holes gained so much heft so…