Orbital period of white dwarf around black hole by end of 2025?
Less than 1 year • 25%
1 to 5 years • 25%
5 to 10 years • 25%
More than 10 years • 25%
Observations and calculations published in scientific journals
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.
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Black hole formation • 25%
Black hole mergers • 25%
Dormant phases • 25%
Other focus • 25%
Planetary system • 25%
Other • 25%
Unusual stellar activity • 25%
Another binary star system • 25%
Other significant discovery • 25%
New type of black hole • 25%
Evidence of black hole merger • 25%
Another dormant black hole • 25%
Decrease to every 10 minutes • 25%
No significant change • 25%
Increase to every 5 minutes • 25%
Increase to every 3 minutes • 25%
No • 50%
Yes • 50%
Other • 25%
Star formation dynamics • 25%
Black hole accretion processes • 25%
Gravitational effects on nearby objects • 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%