A number of MIT affiliates featured prominently at the 43rd Annual News and Documentary Emmy Awards presented by The National Academy of Television Arts and Sciences — including a winner of the Emmy for Outstanding Science and Technology Documentary. “The Hunt for Planet B” — which focuses, in part, on Sara Seager, MIT’s Class of

Professor Deepto Chakrabarty, principal investigator at the MIT Kavli Institute for Astrophysics and Space Research, has been named head of the Department of Physics, effective Aug. 29. Chakrabarty succeeds Peter Fisher, the Thomas A. Frank (1977) Professor of Physics, who has led the department since Nov. 13, 2013. “Professor Chakrabarty will continue to provide strong

Astronomers at MIT and universities across Canada and the United States have detected a strange and persistent radio signal from a far-off galaxy that appears to be flashing with surprising regularity. The signal is classified as a fast radio burst, or FRB — an intensely strong burst of radio waves of unknown astrophysical origin, that

Astronomers at MIT and elsewhere have discovered a new multiplanet system within our galactic neighborhood that lies just 10 parsecs, or about 33 light-years, from Earth, making it one of the closest known multiplanet systems to our own. At the heart of the system lies a small and cool M-dwarf star, named HD 260655, and astronomers

Seven MIT community members have been honored with 2022 American Astronomical Society (AAS) prizes and awards.  Those awarded include two assistant professors of physics, Erin Kara and Kiyoshi Masui, as well as alumni Camille Carlisle SM ’10, Charles Keith Gendreau PhD ’95, Laura Lopez ’04, Richard Mushotzky ’68, and Donald York ’66. Newton Lacy Pierce Prize

Peter H. Fisher, the Thomas A. Frank (1977) Professor of Physics, will step down as the head of the Department of Physics, effective Aug. 31. He will begin his new role as the head of the Office of Research Computing and Data (ORCD) — a venture through the Office of the Vice President for Research

Scattered across our Milky Way galaxy are tens of millions of black holes — immensely strong gravitational wells of spacetime, from which infalling matter, and even light, can never escape. Black holes are dark by definition, except on the rare occasions when they feed. As a black hole pulls in gas and dust from an

Technologies that depend on lightweight, high-precision optical systems, like space telescopes, X-ray mirrors, and display panels, have developed significantly over the past several decades, but more advanced progress has been limited by seemingly simple challenges. For example, the surfaces of mirrors and plates with microstructures that are necessary in these optical systems can be distorted