![]() ![]() However, the supermassive black holes at the centers of galaxies have millions to billions of times as much mass as our sun, and give off lower frequencies of gravitational waves than those detected by LIGO. The National Science Foundation's LIGO (Laser Interferometer Gravitational-Wave Observatory), which is managed jointly by Caltech and MIT, detects gravitational waves from pairs of black holes up to dozens of times the mass of our sun. As the black holes spiral toward each other, they increasingly disturb the fabric of space and time, sending out gravitational waves, which were first predicted by Albert Einstein more than 100 years ago. When galaxies merge, their black holes "sink" to the middle of the newly formed galaxy and eventually join together to form an even more massive black hole. Most, if not all, galaxies possess monstrous black holes at their cores, including our own Milky Way galaxy. "When we realized that the peaks and troughs of the light curve detected from recent times matched the peaks and troughs observed between 19, we knew something very special was going on," says Sandra O'Neill, lead author of the new study and an undergraduate student at Caltech who is mentored by Tony Readhead, Robinson Professor of Astronomy, Emeritus. The combination of the radio data yields a nearly perfect sinusoidal light curve unlike anything observed from quasars before. Five different observatories registered these oscillations, including Caltech's Owens Valley Radio Observatory (OVRO), the University of Michigan Radio Astronomy Observatory (UMRAO), MIT's Haystack Observatory, the National Radio Astronomy Observatory (NRAO), Metsähovi Radio Observatory in Finland, and NASA's Wide-field Infrared Survey Explorer (WISE) space satellite. This causes periodic changes in the quasar's radio-light brightness. According to the study, a powerful jet emanating from one of the two black holes within PKS 2131-021 is shifting back and forth due to the pair's orbital motion. The telltale evidence came from radio observations of PKS 2131-021 that span 45 years. The first candidate pair, within a quasar called OJ 287, orbit each other at greater distances, circling every nine years versus the two years it takes for the PKS 2131-021 pair to complete an orbit. Reporting in The Astrophysical Journal Letters, the researchers argue that PKS 2131-021 is now the second known candidate for a pair of supermassive black holes caught in the act of merging. Astronomers already knew quasars could possess two orbiting supermassive black holes, but finding direct evidence for this has proved difficult. The quasar observed in the new study, PKS 2131-021, belongs to a subclass of quasars called blazars in which the jet is pointing toward the Earth. In some quasars, the supermassive black hole creates a jet that shoots out at near the speed of light. Quasars are active cores of galaxies in which a supermassive black hole is siphoning material from a disk encircling it. When the pair merge in roughly 10,000 years, the titanic collision is expected to shake space and time itself, sending gravitational waves across the universe.Ī Caltech-led team of astronomers has discovered evidence for this scenario taking place within a fiercely energetic object known as a quasar. ![]() ![]() The two giant bodies each have masses that are hundreds of millions of times larger than that of our sun, and the objects are separated by a distance roughly 50 times that which separates our sun and Pluto. Locked in an epic cosmic waltz 9 billion light years away, two supermassive black holes appear to be orbiting around each other every two years. Each black hole is about a hundred million times the mass of our sun, with the black hole in the foreground being slightly less massive. In this view of the system, gravity from the foreground black hole (right) can be seen twisting and distorting the light of its companion, which has a powerful jet. Image: This artist's concept shows two candidate supermassive black holes at the heart of a quasar called PKS 2131-021.
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