And a spacecraft called Lisa Pathfinder launched last December to test technology for a proposed space - based observatory that will be sensitive to longer - wavelength gravitational waves from
supermassive black hole collisions.
Not exact matches
Collisions between
supermassive black holes (SN Online: 8/31/15) can be heard from much farther away, but they send out long, undulating waves to which LIGO is deaf.
They may be a new class of midsize
black holes, weighing 100 solar masses or so, which could have formed either by the
collision of smaller
black holes or by the death of
supermassive stars.
As each of these theories predicts different initial masses for the seeds of
supermassive black hole seeds, the
collisions would produce different gravitational wave signals.
Two detections of gravitational waves caused by
collisions between
supermassive black holes should be possible each year using space - based instruments such as the Evolved Laser Interferometer Space Antenna (eLISA) detector that is due to launch in 2034, the researchers said.
The objects causing these low - frequency ripples — such as orbiting
supermassive black holes at the centers of distant galaxies — would be different from the higher frequency ripples, emitted by
collisions of much smaller
black holes, that have so far been detected on Earth.
Through these efforts, astronomers are attempting to understand recently discovered phenomena such as the first detections of gravitational waves from neutron star
collisions and the accompanying electromagnetic fireworks as well as regular stars being engulfed by
supermassive black holes.
An unusual object about 90 million light - years from Earth might be a
supermassive black hole kicked out of its home galaxy during a
collision with another galaxy, a new study suggests.
But if all goes well, the team even has a prediction of where the
collision is most likely to take place: In a neighborhood like the Sombrero Galaxy, where a slightly less massive
supermassive black hole means the
collision would happen more slowly, leaving scientists more time to spot its signature.
Astrophysicists think we'll be able to detect
collisions of
supermassive black holes — theoretically each containing as much as billions of times the amount of matter as our sun — within just the next ten years.
We now know that galaxies began dying fairly early in the history of the universe, and that central
supermassive black holes and galactic
collisions play key roles in galactic evolution.
Researchers have «dissected» the mysterious gases oozing from two
supermassive black holes on the verge of
collision in galaxy NGC 6240 for the first time.
From
supermassive black holes at galactic centers to giant bursts of star formation to titanic
collisions between galaxies, these discoveries allow astronomers to probe the current properties of galaxies as well as examine how they formed and developed.
Hubble also probed the cores of
collisions, showing that interactions fuel
supermassive black holes at the centers of galaxies.