Astronomy and astrophysics

MIT students and community members spoke with 7 News Boston about their experiences viewing Wednesday’s partial solar eclipse, using the Unistellar eVscope Two, a smart telescope provided by the MIT Astrogazers, an outreach group largely made up of MIT graduate students. “To be able to see this celestial event in a way that’s so approachable, and the way that everybody in the community can enjoy it, especially when you have the right gear, is a really special opportunity,” says Joe Diaz, program manager and STEAM educator at the MIT Media Lab. 

As the moon began to obscure portions of the sun during a partial solar eclipse, the MIT Astrogazers, an outreach group of MIT graduate students, brought telescopes to Kendall Square and offered passersby the opportunity to view the celestial showcase, reports Jay Willett for WBZ News Radio. “This is a Unistellar eVscope Two, so it can take the image that falls on that sensor, and project it to an iPad, another tablet, a smartphone, or even the eyepiece itself,” explained alumnus and Astrogazer, David DePalma ‘26. Graduate student Sydney Jenkins shared: “We’re trying to show everyone what the eclipse looks like, but safely.” 

Popular Science’s Andrew Paul spotlights how MIT astronomers have identified a black hole star (MoM-BH*-1), a gigantic, dense gas cloud fueled by a central black hole, discovered in an image of a large red dot on NASA’s James Webb Space Telescope (JWST). “The groundbreaking realization and newest addition to the cosmic catalogue wouldn’t have been possible without the JWST, whose smallest discoveries have massive ramifications,” writes Paul. “Even something as tiny as a 100-million-year-old red dot.” 

Using NASA’s James Webb Space Telescope (JWST), MIT researchers have discovered a black hole star, MoM-BH*‑1, the earliest example of a black hole in the universe, writes Mashable’s Elisha Sauers. “We argue that Black Hole Stars may be powering all of JWST's Little Red Dots that are found almost everywhere in the early Universe,” says Postdoctoral Associate Rohan Naidu. “Which is to say, this channel of making massive black holes must be very common, to the point where every massive black hole (like the Milky Way's) may have gone through this phase.” 

Postdoctoral Associate Rohan Naidu speaks to The Guardian’s Ian Sample about his team’s research discovering a black hole star, a cosmic object the size of the entire solar system. “They [black hole stars] may govern when stars are able to form and when they cease forming, setting the course for everything that follows from star formation: the birth of planets, the rise of life, the emergence of species that may one day piece together this entire history,” says Naidu.  

Forbes’ “50 Over 50” list spotlights four MIT faculty leading innovation in science and technology: Prof. Paula Hammond, dean of the MIT School of Engineering; Prof. Dina Katabi; Prof. Nergis Mavalvala, dean of the MIT School of Science; and Aude Oliva, director of MIT-IBM Computing Research Lab. The 50 “science and technology standouts on this list are advancing how we use AI, fight osteoporosis and deploy clean energy.”  

MIT researchers have discovered space matter that has been ‘missing’ since the 1990s using Fast Radio Bursts, individual flashes of radio waves traveling through space and coming from the distant universe, reports WCVB 5’s Cindy Fitzgibbon. “The takeaway of the study is that by discovering the distribution of the missing matter around galaxies, we have found evidence for strong activities in galaxies,” says graduate student Haochen Wang, a co-author on the study. “In other words, galaxies are busier and messier than we thought.” 

Prof. Salvatore Vitale and graduate student Cailin Plunkett join John Batchelor and David Livingston, hosts of the Hotel Mars podcast, to discuss their discovery that 14% of black holes were created from the merger of two smaller ones, and their goal to use gravitational wave detectors to uncover the origins of the black hole in the Milky Way. “In ten years [with added gravitational wave technology and observatories], we’ll go from seeing the first gravitational wave ever to seeing them irrespective of where they happen in the universe—which would of course, be fantastic,” says Vitale.  

New Scientist’s Jacklin Kwan highlights Prof. Christoph Kehle’s work demonstrating that extremal black holes, a variety of black hole that has zero temperature, could exist. “Extremal black holes were thought of as an idealised, unattainable limit: something you could write down as a solution, but which could never be reached [through any real physical] process, but we proved that wrong,” says Kehle. 

Prof. Richard Binzel discusses Apophis, an asteroid roughly 340-meters in diameter, set to pass within 32,000 kilometers of Earth on April 13, 2029 with Scientific American’s Andrew Jones. Apophis’s close approach in 2029 will offer “a once-per-millennium natural experiment,” says Binzel.  

In a video for PBS Nova, alumna Elba Alonso-Monsalve PhD ‘26 explains the definition of primordial black holes (PBHs), and how dark matter may be formed from them. “Think like the mass of an asteroid but packed into the volume of a single atom, and these [PBHs] would be floating around our universe, maybe even our own solar system,” says Alonso-Monsalve. “There could be enough of these PBHs lurking around to make up all of the dark matter, and they would be tiny enough to be hard to spot.” 

By studying ‘smears’ in fast radio bursts, fleeting flashes of radiation, MIT researchers discovered diffuse clouds of baryonic gas may contain the missing ordinary matter in the universe, writes Gizmodo’s Gayoung Lee. “These diffuse clouds may be flung outside galaxies through black hole jets,” Lee explains. 

Prof. Brett McGuire joins Peter O'Dowd, host of WBUR’s “Here & Now,” to discuss astronomers’ discovery of Erythrulose, the sugar found in raspberries, in clouds of gas about 25,000 light-years away from Earth. “By a chemist's formal definition this is a sugar—given its structure, the way its atoms are bonded together,” says McGuire. "It’s not the sort of sugar that we think of as involved in making things sweet for us. But it is still a sugar in that it is a compound that stores energy and is involved in biological processes that access that energy and allow it to be used by living organisms." 

After analyzing data from the LIGO, Virgo and KAGRA gravitational wave detectors, MIT researchers have found that 14% of black holes may be second-generation, formed by the merger of two smaller black holes, writes Gayoung Lee for Gizmodo. The scientists “created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above,” Lee explains.  

Prof. David Kaiser joins GBH “Particles of Thought” podcast host Dr. Hakeem Oluseyi to discuss his hunt for primordial black holes. “It’s a lot easier to find stuff coming off of a very bright, hot source, than a cold, dim one. So, the Hawking temperature of a black hole that has the same mass as our sun, or a little bigger would be so cold we would literally never be able to measure [its] radiation,” says Kaiser. “You’ll never see it [Hawking Radiation] from stellar collapse black holes, you’ll never see it from supermassive black holes, or even colder. The only hope to ever see it would be a smaller mass black hole.”