Scientists Measure the Spin Rates of Supermassive Black Holes
This
artist’s concept illustrates a supermassive black hole with millions to
billions times the mass of our sun. Supermassive black holes are
enormously dense objects buried at the hearts of galaxies. (Smaller
black holes also exist throughout galaxies.) In this illustration, the
supermassive black hole at the center is surrounded by matter flowing
onto the black hole in what is termed an accretion disk. This disk forms
as the dust and gas in the galaxy falls onto the hole, attracted by its
gravity. Also shown is an outflowing jet of energetic particles,
believed to be powered by the black hole’s spin. The regions near black
holes contain compact sources of high energy X-ray radiation thought, in
some scenarios, to originate from the base of these jets. This high
energy X-radiation lights up the disk, which reflects it, making the
disk a source of X-rays. The reflected light enables astronomers to see
how fast matter is swirling in the inner region of the disk, and
ultimately to measure the black hole’s spin rate. Image credit:
NASA/JPL-Caltech
Pasadena, California — Two X-ray space observatories, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) and the European Space Agency’s XMM-Newton, have teamed up to measure definitively, for the first time, the spin rate of a black hole with a mass 2 million times that of our sun.
The supermassive black hole lies at the dust- and gas-filled heart of a galaxy called NGC 1365, and it is spinning almost as fast as Einstein’s theory of gravity will allow. The findings, which appear in a new study in the journal Nature, resolve a long-standing debate about similar measurements in other black holes and will lead to a better understanding of how black holes and galaxies evolve.
“This is hugely important to the field of black hole science,” said Lou Kaluzienski, a NuSTAR program scientist at NASA Headquarters in Washington.
The observations also are a powerful test of Einstein’s theory of general relativity, which says gravity can bend space-time, the fabric that shapes our universe, and the light that travels through it.
“We can trace matter as it swirls into a black hole using X-rays emitted from regions very close to the black hole,” said the coauthor of a new study, NuSTAR principal investigator Fiona Harrison of the California Institute of Technology in Pasadena. “The radiation we see is warped and distorted by the motions of particles and the black hole’s incredibly strong gravity.”
NuSTAR, an Explorer-class mission launched in June 2012, is designed to detect the highest-energy X-ray light in great detail. It complements telescopes that observe lower-energy X-ray light, such as XMM-Newton and NASA’s Chandra X-ray Observatory. Scientists use these and other telescopes to estimate the rates at which black holes spin.
Until now, these measurements were not certain because clouds of gas could have been obscuring the black holes and confusing the results. With help from XMM-Newton, NuSTAR was able to see a broader range of X-ray energies and penetrate deeper into the region around the black hole. The new data demonstrate that X-rays are not being warped by the clouds, but by the tremendous gravity of the black hole. This proves that spin rates of supermassive black holes can be determined conclusively.
Scientists
measure the spin rates of supermassive black holes by spreading the
X-ray light into different colors. The light comes from accretion disks
that swirl around black holes, as shown in both of the artist’s
concepts. They use X-ray space telescopes to study these colors, and, in
particular, look for a “fingerprint” of iron — the peak shown in both
graphs, or spectra — to see how sharp it is. Prior to observations with
NASA’s Spectroscopic Telescope Array, or NuSTAR, and the European Space
Agency’s XMM-Newton telescope, there were two competing models to
explain why this peak might not appear to be sharp. The “rotation” model
shown at top held that the iron feature was being spread out by
distorting effects caused by the immense gravity of the black hole. If
this model were correct, then the amount of distortion seen in the iron
feature should reveal the spin rate of the black hole. The alternate
model held that obscuring clouds lying near the black hole were making
the iron line appear artificially distorted. If this model were correct,
the data could not be used to measure black hole spin. NuSTAR helped to
solve the case, ruling out the alternate “obscuring cloud” model. Its
high-energy X-ray data — shown at top as green bump to the right of the
peak — revealed that features in the X-ray spectrum are in fact coming
from the accretion disk and not from the obscuring clouds. Together with
XMM-Newton, the space observatories were able to make the first
conclusive measurement of a black hole’s spin rate, and more generally,
confirm that the “gravitational distortion” model is accurate. Image
credit: NASA/JPL-Caltech
Measuring the spin of a supermassive black hole is fundamental to understanding its past history and that of its host galaxy.
“These monsters, with masses from millions to billions of times that of the sun, are formed as small seeds in the early universe and grow by swallowing stars and gas in their host galaxies, merging with other giant black holes when galaxies collide, or both,” said the study’s lead author, Guido Risaliti of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., and the Italian National Institute for Astrophysics.
Supermassive black holes are surrounded by pancake-like accretion disks, formed as their gravity pulls matter inward. Einstein’s theory predicts the faster a black hole spins, the closer the accretion disk lies to the black hole. The closer the accretion disk is, the more gravity from the black hole will warp X-ray light streaming off the disk.
Astronomers look for these warping effects by analyzing X-ray light emitted by iron circulating in the accretion disk. In the new study, they used both XMM-Newton and NuSTAR to simultaneously observe the black hole in NGC 1365. While XMM-Newton revealed that light from the iron was being warped, NuSTAR proved that this distortion was coming from the gravity of the black hole and not gas clouds in the vicinity. NuSTAR’s higher-energy X-ray data showed that the iron was so close to the black hole that its gravity must be causing the warping effects.
With the possibility of obscuring clouds ruled out, scientists can now use the distortions in the iron signature to measure the black hole’s spin rate. The findings apply to several other black holes as well, removing the uncertainty in the previously measured spin rates.
For more information on NASA’s NuSTAR mission, visit: http://www.nasa.gov/nustar .
For more information on ESA’s XMM-Newton mission, visit: http://go.nasa.gov/YUYpI6 .
The California Institute of Technology in Pasadena manages JPL for NASA.
Publication: G. Risaliti, et al. “A rapidly spinning supermassive black hole at the center of NGC 1365,” Nature 494, 449–451 (28 February 2013); doi:10.1038/nature11938
Source: Whitney Clavin, Jet Propulsion Laboratory; NASA
Images: NASA/JPL-Caltech
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