You may have heard that nothing escapes the gravitational grasp of a black hole, not even light. This is true in the immediate vicinity of a black hole, but a bit farther out -- in disks of material that swirl around some black holes -- light can escape. In fact, this is the reason actively growing black holes shine with brilliant X-rays.
Now, a new study accepted for publication in The Astrophysical Journal offers evidence that, in fact, not all of the light streaming from a black hole's surrounding disk easily escapes. Some of it gives in to the monstrous pull of the black hole, turns back, and then ultimately bounces off the disk and escapes.
"We observed light coming from very close to the black hole that is trying to escape but instead is pulled right back by the black hole like a boomerang," said Riley Connors, lead author of the new study and a postdoctoral scholar at Caltech.
"This is something that was predicted in the 1970s, but hadn't been shown until now," Connors added.
The new findings were made possible by combing through archival observations from NASA's now-defunct Rossi X-ray Timing Explorer (RXTE) mission, which came to an end in 2012. The researchers specifically looked at a black hole that is orbited by a sun-like star; together, the pair is called XTE J1550-564.
The black hole "feeds" off this star, pulling material onto a flat structure around it called an accretion disk. By looking closely at the X-ray light coming from the disk as the light spirals toward the black hole, the team found imprints indicating that the light had been bent back toward the disk and reflected off.
"The disk is essentially illuminating itself," said co-author Javier Garcia, a research assistant professor of physics at Caltech.
Garcia further said: "Theorists had predicted what fraction of the light would bend back on the disk, and now, for the first time, we have confirmed those predictions. "
The scientists say that the new results offer another indirect confirmation of Albert Einstein's general theory of relativity, and also will help in future measurements of the spin rates of black holes, something that is still poorly understood.
"Since black holes can potentially spin very fast, they not only bend the light but twist it. These recent observations are another piece in the puzzle of trying to figure out how fast black holes spin," said Connors
The new study, titled, "Evidence for Returning Disk Radiation in the Black Hole X-ray Binary XTEJ1550-564," was funded by NASA, the Alexander von Humboldt Foundation, and the Margarete von Wrangell Fellowship.
Disclaimer: No Business Standard Journalist was involved in creation of this content
You’ve reached your limit of {{free_limit}} free articles this month.
Subscribe now for unlimited access.
Already subscribed? Log in
Subscribe to read the full story →
Smart Quarterly
₹900
3 Months
₹300/Month
Smart Essential
₹2,700
1 Year
₹225/Month
Super Saver
₹3,900
2 Years
₹162/Month
Renews automatically, cancel anytime
Here’s what’s included in our digital subscription plans
Exclusive premium stories online
Over 30 premium stories daily, handpicked by our editors


Complimentary Access to The New York Times
News, Games, Cooking, Audio, Wirecutter & The Athletic
Business Standard Epaper
Digital replica of our daily newspaper — with options to read, save, and share


Curated Newsletters
Insights on markets, finance, politics, tech, and more delivered to your inbox
Market Analysis & Investment Insights
In-depth market analysis & insights with access to The Smart Investor


Archives
Repository of articles and publications dating back to 1997
Ad-free Reading
Uninterrupted reading experience with no advertisements


Seamless Access Across All Devices
Access Business Standard across devices — mobile, tablet, or PC, via web or app
