Prof. Dava Newman speaks with USA Today reporter Sara D. Wire about NASA’s plans to return to the moon and, hopefully, Mars in the 2030s. The “moon is a three-day trip," Newman explains. "Mars, you need eight months. Those are very different targets.”
Prof. Salvatore Vitale and graduate student Jack Heinzel speak with Scientific American reporter K.R. Callaway about the LIGO-Virgo-KAGRA (LVK) Collaboration’s latest catalog of gravitational wave detections, which “more than doubles the number of gravitational-wave candidate events—and reveals unexpected complexities of merging black holes.” Says Heinzel: “We’re learning a lot of things that are qualitative and phenomenological from the catalog. Starting to see all these different structures emerge is pretty fascinating.”
Prof. Raymond Pierrehumbert and his colleagues have discovered an exoplanet orbiting a star 34 light-years from Earth that is "covered with a perpetual ocean of magma and enveloped by a noxious and fiercely hot sulfur-rich atmosphere," reports Will Dunham for Reuters. "The era of exoplanet discovery keeps showing us new kinds of worlds, indeed 'strange new worlds,' generally stranger than anything in 'Star Trek,'" says Pierrehumbert. “This offers all sorts of exciting opportunities to put together fundamental physics in very novel ways."
Using new observations from the James Webb Space Telescope (JWST), astronomers from MIT determined that asteroid 2024 YR4 will not collide with the moon, reports Hannah Devlin for The Guardian. “[Asteroid] 2024 YR4 is exceedingly faint right now, reflecting about as much light as an almond at the distance of the moon,” explain Prof. Julien de Wit and Andy Rivkin PhD '91, who co-led the observations. “Webb is the only observatory that could hope to make these measurements, as it is the only one with the required sensitivity and stability combined with precise moving-target tracking needed to follow and study objects like this.”
Using the James Webb Space Telescope (JWST), astronomers from MIT and other institutions have determined that asteroid 2024 YR4 will not collide with the moon, reports Ashley Strickland for CNN. “Every time we observe an asteroid, we reduce the range of possible trajectories,” explains Prof. Julien de Wit. “In this case, the JWST observations both provided very precise positional measurements and significantly extended the time span over which the asteroid has been observed.”
Prof. Richard Teague speaks with CNN reporter Asuka Koda about how an international team of astronomers have “captured the most complete, high-resolution map of the cold gas at the center of the Milky Way, which contains the raw material from which stars and planets are made” using the Atacama Large Millimeter/submillimeter Array, or ALMA. “I think astronomy on this scale is really no longer about small individual people pushing in their labs, but about huge international collaborations,” says Teague. “And I think that’s what’s particularly impressive about this piece of work, just the scale of that collaboration that you need to make it happen.”
Prof. Danielle Wood speaks with CNBC reporter Laya Neelakandan about NASA’s Artemis III, the United States’ first venture back to the moon in over 50 years, which will carry the first female and first Black astronaut to the Moon. “NASA’s been thinking through this whole process, two decades’ worth, of what we’re going to do is prepare the government to focus on these harder, next-generation missions and be able to do things that are not already demonstrated,” says Wood.
A study by researchers at MIT has found that high levels of greenhouse gas emissions in the atmosphere is impacting the satellite orbits that typically force objects back to Earth, leading to an increased amount of space junk, reports Sachi Kitajima Mulkey for The New York Times. “[W]e’re losing this cleaning force that we rely on” says William Parker PhD '25.
Prof. Anna-Christina Eilers and postdoctoral associate Rohan Naidu speak with Scientific American reporter Rebecca Boyle about the discovery and study of Little Red Dots, mysterious, red spots that showed up in images from the James Webb Space Telescope. The dots, which astronomers dated to 600 million years after the big bang, “are in every single image the telescope takes,” says Naidu. “We have to find out about them if we want to tell a complete story about the early universe."
A new study by Prof. Sara Seager and her colleagues has found a solar system that contradicts the patterns commonly “seen across the galaxy and in our own solar system,” reports Jacopo Prisco for CNN. The study offers “some of the first evidence for flipping the script on how planets form around the most common stars in our galaxy,” says Seager. “Even in a maturing field, new discoveries can remind us that we still have a long way to go in understanding how planetary systems are built.”
Prof. Olivier de Weck speaks with Forbes reporter Alex Knapp about the challenges and opportunities posed by building data centers in space. Data centers are “physically secure from intrusion and environmentally friendly once operational,” says de Weck. “Essentially, the three primary resources required on Earth—land, power, and cooling—are available ‘for free’ in space after the initial launch and deployment costs are covered.”
A new study by MIT physicists demonstrates that quark-gluon plasma behaves like a liquid, findings that could shed more light on the makeup of the early universe, reports Gayoung Lee for Gizmodo. “The researchers anticipate that the methods of the new study will greatly advance our understanding of matter in the early universe,” explains Lee.
Quanta Magazine reporter Jonathan O’Callaghan spotlights Prof. David Kaiser and graduate student Alexandra Klipfel, and their work searching for evidence of primordial black holes. “Very little mass gets radiated over the majority of the black hole’s lifetime,” explains Klipfel. “But then, right at the end, it emits a majority of its mass in a very rapid explosion. It heats up really, really quickly, a runaway process that ends in a big explosion of ultra-high-energy particles.”
A new analysis conducted by postdoctoral associate Rohan Naidu and his colleagues has found evidence that suggests “little red dot” galaxies may contain baby black holes, reports Alex Wilkins for New Scientist. “In ordinary black holes, what you actually see with your eyes is the tip of the iceberg of the total energy that is coming out of the system, but the little red dots we now understand should really be thought of as these puffed-up black hole stars,” says Naidu. “It seems that most of their energy is coming out at these wavelengths that we see with our eyes, so what you see is what you get.”
The Economist chronicles the life and work of Prof. Nuno Loureiro, from his childhood in Portugal where he dreamed of becoming a scientist to his work at MIT as a “fusion pioneer” leading the Plasma Science and Fusion Center. “He walked into his classes beaming, ready to cover the blackboard with figures. He joked like a friend, but he worked his students vigorously, advising them that if they were not yet the best, they should strive to be. Failure was not to be feared, because it showed they were trying to tackle the really hard problems.”