New X-ray emission patterns from white dwarf by July 2025?
Yes • 50%
No • 50%
Reports from the European Space Agency or other astronomical observatories
Astronomers Detect X-rays from White Dwarf Orbiting Supermassive Black Hole in 1ES 1927+654
Jan 14, 2025, 02:29 PM
Astronomers have made a groundbreaking discovery by observing a white dwarf star in close proximity to a supermassive black hole in the galaxy 1ES 1927+654, located approximately 270 million light-years from Earth. The white dwarf, with a mass about 10% that of the Sun, is orbiting the black hole, which has a mass about 1.4 million times that of the Sun. Observations using the European Space Agency's XMM-Newton telescope have detected increasing flashes of X-rays emanating from the white dwarf as it approaches the black hole's event horizon. The white dwarf's orbit appears to have stabilized, possibly due to its outer layers being drawn into the black hole, preventing it from crossing the event horizon. This phenomenon marks the closest object ever observed orbiting a supermassive black hole, offering new insights into the interactions between stellar remnants and black holes.
View original story
Decrease to every 10 minutes • 25%
Increase to every 5 minutes • 25%
No significant change • 25%
Increase to every 3 minutes • 25%
New theory involving relativity • 25%
New theory involving quantum effects • 25%
New theory involving dark matter • 25%
No new theory published • 25%
Change in gravitational field detected • 25%
New type of radiation detected • 25%
Other phenomena detected • 25%
No new phenomena detected • 25%
Another binary star system • 25%
Planetary system • 25%
Unusual stellar activity • 25%
Other • 25%
Solar wind • 25%
Solar corona heating • 25%
Solar flares • 25%
Coronal mass ejections • 25%
Black hole accretion processes • 25%
Other • 25%
Star formation dynamics • 25%
Gravitational effects on nearby objects • 25%
5 to 10 years • 25%
1 to 5 years • 25%
Less than 1 year • 25%
More than 10 years • 25%
Matter accretion onto the white dwarf • 25%
Interaction with the black hole's magnetic field • 25%
Collision with another stellar object • 25%
Other • 25%