Haystack postdoc Kazunori Akiyama speaks with Gizmodo reporter Ryan Mandelbaum about the effort to capture the first image of a black hole, and notes that in the future, additional observations should shed light on how the region around the black hole is changing. “By accumulating observations over the next year with additional telescopes, we can identify what’s changing the black hole image,” Akiyama explains.
Fortune reporter Chris Morris explores how the Event Horizon Telescope has captured the first image of a black hole. “We’ve demonstrated that the EHT is the observatory to see a black hole on an event horizon scale,” says Haystack postdoc Kazunori Akiyama. “This is the dawn of a new era of black hole astrophysics.”
WBZ-TV’s Ken MacLeod visits MIT’s Haystack Observatory to learn about how scientists there processed enormous quantities of data to develop the first image of a black hole. “My goodness, we just proved that Einstein was right at a scale that no one has dreamed of,” says Haystack’s Michael Hecht. “Most of us still don’t believe it’s possible, even though we have done it.”
MassLive reporter Kristin LaFratta spotlights how researchers from the MIT Haystack Observatory played a key role in processing the first image of a black hole. “This project has been my life ever since the beginning of it. It’s overwhelming,” says Haystack’s Michael Titus. “It’s something that’s been a long time coming.”
Haystack research scientist Vincent Fish speaks with Radio Boston about the significance of capturing the first image of a black hole. “It seemed like it would take forever for us to constitute an array to actually be able to make an image,” recalls Fish of the early days of the project. “Actually making an image, I’m glad to be able to do that.”
Boston Globe reporter Martin Finucane spotlights how MIT Haystack Observatory researchers played a “major role in the effort to create the first-ever picture of a black hole.” “I’m very proud,” says Vincent Fish, a research scientist at Haystack. “I’ve spent most of my professional life on this and I’m just really glad we got such great results out of this.”
Wall Street Journal reporter Leigh Kamping-Carder highlights how MIT researchers are developing a number of new technologies aimed at easing the transition to space for future amateur astronauts. A robotic tail developed by Media Lab researchers could help space travelers “grab objects, anchor to surfaces and balance while floating in environments with reduced gravity.”
Prof. Nergis Mavalvala speaks with NPR’s Nell Greenfieldboyce about recent upgrades made to the LIGO gravitational wave detectors, which should increase their ability to sense previously undiscovered cosmic events. "That's how discovery happens," explains Mavalvala. "You turn on a new instrument, you point it out at the sky, and you see something that you had no idea existed."
Writing for Smithsonian, Alice George highlights Margaret Hamilton’s work leading the team at the MIT Instrumentation Lab that developed the software for the Apollo 11 mission. “She was a pioneer when it came to development of software engineering,” says Teasel Muir-Harmony, a curator at the National Air and Space Museum, and “a pioneer as a woman in the workplace contributing to this type of program, taking on this type of role.”
Prof. Nergis Mavalvala speaks with Ira Flatow of Science Friday about how she and her colleagues are working on a new technology called squeezed light, which could enable LIGO to see even more of the cosmos. Mavalvala explains that squeezed light is “a somewhat exotic quantum state of light that we engineer in our labs to improve the sensitivity of LIGO.”
Prof. Sara Seager speaks with National Geographic reporter Jamie Shreeve about her work searching for an Earth-like planet orbiting a sunlike star. “You never know what’s going to happen,” Seager says. “But I know that something great is around those stars.”
Postdoctoral fellow Dheeraj Pasham speaks with Ira Flatow of Science Friday about his research calculating that a supermassive black hole 300 million light years from Earth is spinning at half the speed of light. Pasham explains that a black hole's spin rate provides information about the “channel through which it grew, all the way from a couple of years after the Big Bang until now.”
Space.com reporter Mike Wall writes that researchers have calculated a supermassive black hole’s rotation rate by analyzing the X-rays it emitted after consuming a nearby star. The researchers found that “the huge black hole, known as ASASSN-14li, is spinning at least 50 percent the speed of light.”
Gizmodo reporter Ryan Mandelbaum writes that researchers determined how fast a supermassive black hole spins by measuring a star being swallowed by the black hole. Postdoctoral fellow Dheeraj Pasham explains that, “this measurement is different in the sense that we were able to measure the spin of a black hole that was dormant.”
Astronomers from MIT have detected echoes in X-ray flares emitted by a black hole consuming stellar material, writes Charles Q. Choi for Space.com. The findings “might shed light on how matter behaves not just as it falls into stellar-mass black holes,” writes Choi, “but also supermassive black holes millions to billions of times the mass of the sun.”