Junior Peña, neutrino hunter

Growing up in South Central Los Angeles, Junior Peña learned to keep his eyes down and his schedule full. In his neighborhood, a glance could invite trouble, and many kids—including his older brother—were pulled into gang culture. He knew early on that he wanted something else. With his parents working long hours, he went to after-school programs, played video games, and practiced martial arts. But his friends had no idea that he also spent hours online poring over textbooks and watching lectures, teaching himself advanced mathematics and philosophy. “Being good at school wasn’t how people saw me,” he says. 

One night in high school, he came across a YouTube video about the Higgs boson—the so-called “God particle,” thought to give mass to nearly everything in the universe. “I remember my mind being flooded with questions about life, the universe, and our existence,” he recalls. He’d already looked into philosophers’ answers to those questions but was drawn to the more concrete explanations of physics.

After his independent study helped Peña pass AP calculus as a junior, his fascination with physics led him to the University of Southern California, the 2019 session of MIT’s Summer Research Program, and then MIT for grad school. Today, he’s working to shed light on neutrinos, the ghostly uncharged particles that slip effortlessly through matter. Particles that would require a wall of lead five light-years thick to stop.

As a grad student in the lab of Joseph Formaggio, an experimental physicist known for pioneering new techniques in neutrino detection, Peña works alongside leading physicists designing technology to precisely measure what are arguably the universe’s most elusive particles. Emanating from such sources as the sun and supernovas (and generated artificially by particle accelerators and nuclear reactors), neutrinos reveal their presence through an absence. Their existence was initially posited in the 1930s by the physicist Wolfgang Pauli, who noticed that energy seemed to go missing when atoms underwent a process known as radioactive beta decay. According to the law of conservation of energy, the total energy of the particles emitted during radioactive decay must equal the energy of the decaying atom. To account for the missing energy, Pauli proposed the existence of an undetectable particle that was carrying it away. 

Einstein’s E = mc2 tells us that if energy is missing, then mass must be too. Yet according to the standard model of physics—which offers our most trusted theory for how particles behave—neutrinos should have no mass at all. Unlike other particles, they don’t interact with the Higgs field, a kind of cosmic molasses that slows particles down and gives them mass. Because they pass through it untouched, they should remain massless. 

But by the early 2000s, researchers had discovered that neutrinos, which had first been detected in the 1950s, can shift between three types, a feat possible only if they have mass. So now the tantalizing question is: What is their mass? 

Determining neutrinos’ exact mass could explain why matter triumphed over antimatter, refine models of cosmic evolution, and clarify the particles’ role in dark matter and dark energy. And the Formaggio Lab is part of Project 8, an international collaboration of 71 scientists in 17 institutions working to make that measurement. To do this, the lab uses tritium, an unstable isotope of hydrogen that decays into helium, releasing both an electron and a particle called an antineutrino (“every particle has an antiparticle counterpart,” Formaggio explains). By precisely measuring the energy spectrum of those electrons, scientists can determine how much energy is missing, allowing them to infer the neutrinos’ mass.

At the heart of this experiment is a novel detection method called cyclotron radiation emission spectroscopy (CRES), first proposed in 2008 by Formaggio and his then postdoc Benjamin Monreal, which “listens” to the faint radio signals emitted as electrons spiral through a magnetic field. Peña was instrumental in designing a crucial part of the tool that will make this possible: a copper cavity that he likens to a guitar, with the electrons released during beta decay acting like plucked strings. The cavity will amplify their signals, helping researchers to measure them exactly. Peña spent more than a year developing and refining a flashlight-size prototype of the device in collaboration with machinists and fellow physicists.

Peña designed a prototype copper microwave resonator to amplify the signals of electrons emitted as tritium decays, allowing researchers to measure them exactly and infer the neutrino’s mass.
JESSICA CHOMIK-MORALES, SM ’25

“He had to learn the [design and simulation] software, figure out how to interpret the signals, and test iteration after iteration,” says Formaggio, Peña’s advisor. “It’s been incredible watching him take this from a rough idea to a working design.”

The design of Peña’s cavity had to balance competing demands. It needed a way to extract the electrons’ signals that was compatible with the researchers’ methods for calibrating the system, one of which involves using an electron gun to inject electrons of a known, precise energy into the cavity. And it also needed to preserve the properties of the electromagnetic fields within the cavity. In May, Peña sent his final prototype to the University of Washington, where it was installed in July. Researchers hope to begin calibration this fall. Then Peña’s cavity and the full experimental setup will be scaled up so in a few years they can begin collecting CRES data using tritium.

“We’ve been working toward this for at least three years,” says Jeremy Gaison, a Project 8 physicist at the Pacific Northwest National Lab. “When we finally turn on the experiment, it’s going to be incredible to see if all of our simulations and studies actually hold up in real data.”

Peña’s contribution to the effort “is the core of this experiment,” says Wouter Van De Pontseele, another Project 8 collaborator and former Formaggio Lab postdoc. “Junior took an idea and turned it into reality.” 

Project 8 is still in its early stages. The next phase will scale up with larger, more complex versions of the technology Peña played a key role in developing, culminating in a vast facility designed to hunt for the neutrino’s mass. If that is successful, the findings could have profound implications for our understanding of the universe’s structure, the evolution of galaxies, and even the fundamental nature of matter itself.

Eager to keep probing such open questions in fundamental physics, Peña is still exploring options for his postdoc work. One possibility is focusing on the emerging field of levitated nanosensors, which could advance gravitation experiments, efforts to detect dark matter, and searches for the sterile neutrino, a posited fourth variety that interacts even more rarely than the others.

“Experimental particle physics is long-term work,” says Van De Pontseele. “Some of us will stay on this project for decades, but Junior can walk away knowing he made a lasting impact.”

Peña also hopes to have a lasting impact as a professor, opening doors for students who, like him, never saw themselves reflected in the halls of academia. “A summer program brought me here,” he says. “I owe it to the next kid to show they belong.”

MIT is worth fighting for

As I write in late July, we’re contending with a major tax increase on the annual returns from MIT’s endowment as well as other investments and assets. This new tax burden will strain the resources we use to support research, innovation, and student scholarships and financial aid—the heart and soul of the Institute. 

And the financial impact on us will be significant: This tax increase alone will cost in the range of 10% of MIT’s annual central budget. 

Unfortunately, we face the prospect of further threats to our mission and financial model this fall when Congress considers drastic cuts to the research budgets of federal agencies. And all this comes on the heels of multiple US science agencies capping their reimbursement of research infrastructure and administration expenses well below actual costs. These reimbursements are critical to operating our world-class research enterprise, and that’s why we have challenged the government’s actions in court. 

I don’t expect we all agree on the ideal contours of the Institute’s future. But I have to believe that we all agree it should have a future.

For more information—and ways to help—you can consult these online resources:

Visit Understanding MIT for a comprehensive view of the Institute’s value to the nation and the world.  

Go to Stand up for MIT and find ways to take action.

And visit MIT’s Response to government activity page to keep up to date on what’s happening in Washington and how it’s affecting the nation’s great research enterprise. 

MIT was built with the support of generations of alumni and friends—and it’s up to us to keep its foundations strong for those to come. 

So I hope you will join me in standing up for MIT.

Infinite Threads

Textiles account for 5% of landfill space—and clothing made with polyester can take up to 200 years to decompose. Massachusetts tackled the problem by banning disposal of clothing and fabrics in 2022. And Infinite Threads, a spinoff of the Undergraduate Association Sustainability Committee, is addressing it by collecting lightly used clothing from the MIT community and selling it for $2 to $6 per item at popup sales held several times each semester. 

“Our goal is simple: We want to keep clothing out of landfills,” says Cameron Dougal ’25, who led the effort with Erin Hovendon ’26 in 2024–’25. That year, the group sold over 1,000 items and gave about 750 pounds of unsold goods to Helpsy, an organization that collects used clothing for resale and recycling. Infinite Threads uses proceeds from its sales to pay student workers and to rent a U-Haul to bring clothing to the popups. 

people look through racks of clothes outdoors with a U-haul truck in the background

SARAH FOOTE

In addition to helping the planet, offering affordable clothing options generates a lot of positive feedback on campus. “I love hearing from students that they got clothing items they now wear frequently from one of our sales,” says Hovendon. 

Infinite Threads also gives away leftover T-shirts from residence hall events and career fairs, which Dougal says demonstrates the importance of a hyperlocal reuse ecosystem. “As soon as these types of items leave campus,” he says, “there is a much lower chance that they will find a new home.”

Fix damaged art in hours with AI

Art restoration takes steady hands and a discerning eye. For centuries, conservators have identified areas needing repair and then mixed the exact shades needed to fill in one area at a time. Restoring a single painting can take anywhere from a few weeks to over a decade. Now an MIT graduate student in mechanical engineering has used artificial intelligence to speed up the process by orders of magnitude.

Digital restoration tools are not new; computer vision, image recognition, and color matching have all helped generate repaired versions of damaged paintings in recent years. But until now, there has been no way to apply the results directly onto an original canvas. Instead, they are usually displayed virtually or printed as stand-alone works.

In his study, Alex Kachkine, SM ’23, presents a new method he’s developed that involves printing the restoration on a very thin polymer film that can be carefully aligned with a painting and adhered to it or easily removed. As a demonstration, he used the method to repair a highly damaged 15th-century oil painting he owned. First he used traditional techniques to clean the painting and remove any past restoration efforts. Then he scanned the painting, including the many regions where paint had faded or cracked, and used existing algorithms to create a virtual version of what it may have looked like originally.

Next, Kachkine used software he developed to create a map of regions on the original painting that require infilling, along with the exact colors needed. The method automatically identified 5,612 regions in need of repair and filled them in using 57,314 different shades. This map was then translated into a physical, two-layer mask printed onto polymer-based films. The first layer was printed in color, while the second layer was printed in the exact same pattern but in white.

“In order to fully reproduce color, you need both white and color ink to get the full spectrum,” Kachkine explains. He used high-fidelity commercial inkjets to print the mask’s two layers, which he carefully aligned with the help of computational tools he developed. Then he overlaid them by hand onto the original painting and adhered them with a thin spray of conventional varnish. The films are made from materials that can be easily dissolved in case conservators need to reveal the original, damaged work. The entire process took 3.5 hours, which he estimates is about 66 times faster than traditional restoration methods.

If this method is adopted widely, Kachkine emphasizes, conservators should be involved at every step, to ensure that the final work is in keeping with an artist’s style and intent. The digital file of the mask can also be saved to document exactly what was restored. “Because there’s a digital record of what mask was used, in 100 years, the next time someone is working with this, they’ll have an extremely clear understanding of what was done to the painting,” Kachkine says. “And that’s never really been possible in conservation before.”

The result, he hopes, will be a new lease on life for many works that have not had a chance to be repaired by hand. “There is a lot of damaged art in storage that might never be seen,” he says. “Hopefully with this new method, there’s a chance we’ll see more art.” 

Emergency help for low blood sugar

Most people with type 1 diabetes inject insulin to prevent their blood sugar levels from getting too high. However, if their blood sugar gets too low, it can lead to confusion, seizures, and even death.

To combat this hypoglycemia, some patients carry syringes of glucagon, a hormone that stimulates release of glucose. Now MIT engineers have developed an alternative that could work even when people don’t realize they are becoming hypoglycemic. It could also help during sleep, or for children who are unable to inject themselves. “Our goal was to build a device that is always ready to protect patients,” says Daniel Anderson, a professor in MIT’s Department of Chemical Engineering and the senior author of a study on the work.

The implantable device, about the size of a quarter, contains a polymer reservoir holding powdered glucagon and sealed with a material that can be programmed to change shape when heated. It also includes an antenna that allows the user to remotely turn on a small electrical current, which heats that material until it bends and releases the drug. Because the device can receive wireless signals, it could also be triggered automatically by a glucose monitor.

The researchers have successfully tested the implant in mice and say it could also be used to deliver epinephrine to treat heart attacks or prevent anaphylactic shock. 

‘Bubbles’ turn air into drinkable water

Today, 2.2 billion people in the world lack access to safe drinking water. But the atmosphere contains millions of billions of gallons of water in the form of vapor, and researchers have tried various strategies to capture and condense it in places where traditional sources are inaccessible. Now MIT engineers have improved on that approach with an atmospheric water harvester based on an absorbent hydrogel.

The gel they developed has more vapor-carrying capacity than some materials others have used to trap water from the air, and it is less likely to leak the salts that are often embedded in hydrogels to increase absorption. They also increased its surface area, and thus the amount of vapor it can hold, by molding it into a pattern of small domes resembling bubble wrap. 

a grid of bubbles on a dark surface

COURTESY OF THE RESEARCHERS

In the researchers’ prototype device, a half-square-meter panel of the hydrogel is enclosed in a glass chamber coated with a cooling polymer film. When the vapor captured by the textured material evaporates, the bubbles shrink down in an origami-­like transformation. The vapor then condenses on the glass, where it can flow out through a tube.

The system runs entirely on its own, unlike other designs that require batteries, solar panels, or electricity from the grid. The team ran it for over a week in Death Valley, California—the driest place in North America. Even in those conditions, it squeezed clean water from the air at rates of up to 160 milliliters (about two-thirds of a cup) per day.

“We have built a meter-scale device that we hope to deploy in resource-limited regions, where even a solar cell is not very accessible,” says Professor Xuanhe Zhao, the senior author of a paper on the work. The team estimates that a small array of the panels could passively supply a household with drinking water even in a desert, with greater production in temperate and tropical climates.

Chandrakasan named provost

Anantha Chandrakasan became the Institute’s new provost on July 1, succeeding Cynthia Barnhart, SM ’86, PhD ’88, who announced her decision to step down in February.

Chandrakasan, who earned his BS, MS, and PhD in electrical engineering and computer science from the University of California, Berkeley, joined MIT in 1994. Head of the Energy-Efficient Circuits and Systems Group, he has been dean of the School of Engineering since 2017 and MIT’s inaugural chief innovation and strategy officer, playing a key role in launching multiple new initiatives, since 2024. He headed the Department of Electrical Engineering and Computer Science, MIT’s largest academic department, for six years.

As MIT’s senior academic and budget officer, Chandrakasan will focus on understanding institutional needs and strategic financial planning, attracting and retaining top talent, and supporting cross-cutting research, education, and entrepreneurship programming. On all these fronts, he plans to seek frequent input from across the Institute. He also plans to establish a provost faculty advisory group, as well as student/postdoc advisory groups and an external provost advisory council.

“There is a tremendous opportunity for MIT to be at the center of the innovations in areas where the United States wants to lead,” Chandrakasan says. “It’s about AI. It’s about semiconductors. It’s about quantum, the bio­security and biomanufacturing space—but not only that. We need students who can do more than just code or design or build. We really need students who understand the human perspective and human insights.” 

One-shot vaccines for HIV and covid

A team at MIT and the Scripps Research Institute has made important progress toward vaccines that can protect against HIV, and potentially other diseases, with a single dose.

The researchers treated mice with a vaccine that combines two different adjuvants, materials that help stimulate the immune system—one incorporating a compound previously developed by Scripps professor Darrell Irvine. 

Irvine and MIT professor J. Christopher Love, the senior authors of a paper on the work, had found that the combination helped generate more robust immune responses. In the new paper, they showed that the dual-adjuvant vaccine accumulated in the lymph nodes, where white blood cells known as B cells encounter antigens and undergo rapid mutations that generate new antibodies. The vaccine’s antigens remained there for up to a month, allowing the immune system to build up a much greater number and diversity of antibodies against the HIV protein than the vaccine given alone or with one adjuvant.

“When you think about the immune system sampling all of the possible solutions, the more chances we give it to identify an effective solution, the better,” Love says. 

This approach may mimic what occurs during a natural infection and could lead to an immune response so strong and broad that vaccines only need to be given once. Love says, “It offers the opportunity to engineer new formulations for these types of vaccines across a wide range of different diseases, such as influenza, SARS-CoV-2, or other pandemic outbreaks.”

From MIT to low Earth orbit

Not everyone can point to the specific moment that set them on their life’s course. But for me, there’s no question: It happened in 1982, when I was a junior at MIT, in the Infinite Corridor. In those pre-internet days, it was where we got the scoop about everything that was happening on campus. One day, as I was racing to the chemistry labs, a poster caught my eye.

As I remember it, the poster showed a smiling woman in a flight suit, holding a helmet by her side. I recognized her immediately: Sally Ride, one of America’s first group of female astronauts. It had just been announced that she would be part of the crew for one of the upcoming space shuttle flights, making her the first American woman in space. And while she was visiting Lincoln Lab for training, she would be giving a speech and attending a reception hosted by the Association of MIT Alumnae. A woman speaker was still a novelty at MIT in those days. But a woman astronaut? I knew this was one event I had to attend. 

Coleman sits in the rear seat of a supersonic T-38 jet for pilot training as a newly minted NASA astronaut candidate in 1992. “When a chemist gets to fly a T-38, she will always be smiling,” she says.
NASA

On the day of Sally Ride’s talk, I hurried into 10-250, the large lecture hall beneath the Great Dome that is the emblem of MIT. Sandy Yulke, the chair of the Association of MIT Alumnae, was already introducing Sally. Sally. Just a first name. As if she were one of us. I slid into an empty seat just a few rows back as Sandy talked about how proud she was to welcome the soon-to-be first American woman in space. And Sally was standing there, right where our professors stood every day. A woman. And an astronaut. 

When I was growing up in the 1960s and ’70s, the image I’d had of astronauts—or any kind of explorer, for that matter—could not have been further from the figure before me that day. And I’m not just talking about images I saw in the media—I had one much closer to home. My dad—James Joseph Coleman, known as JJ—was a career naval officer who ultimately led the Experimental Diving Unit. A legend among Navy divers, he had also been a project officer for the Sealab program that built the first underwater habitats, allowing men—and it was all men at the time—to live and work in the deep seas for extended periods. The spirit of exploration, the desire to understand fascinating and challenging environments, seemed normal to me. But because none of the explorers I saw looked like me, it didn’t occur to me that I could be one. My dad worked in a male-dominated world where I’m sure very few of his colleagues imagined that people like me might belong too.

By the time I got to MIT, in 1979, only six women had been selected as NASA astronauts. But seeing Sally Ride on the stage that day turned a possibility into a reality—a reality that could include me. Instead of being larger than life, she was surprisingly real and relatable: a young, bright-eyed woman, with wavy brown hair kind of like mine, wearing a blue flight suit and black boots. She seemed a little shy, looking down at her hands as she was introduced and applauded. 

Sally was obviously passionate about her scientific work—she was an accomplished astrophysicist—but she also had this amazing job where she flew jets, practiced spacewalking, and was part of a crew with a mission. Both scientist and adventurer, she was accomplishing something that no American woman ever had—and, in the process, opening the door for the rest of us. As I listened to her speak that day, an utterly unexpected idea popped into my head: Maybe I—Cady Coleman—could have that job. 

If you can see it, you can be it. Representation doesn’t fix everything, but it changes, on a visceral level, the menu of options that you feel you can reach for. No matter how many people tell us we can be whatever we want to be—and my mother told me that from the moment I was old enough to understand—some of us need more than words. Representation matters. A lot. We are enormously influenced by the signals that we get from our surroundings. What do people expect of us? What models do we have? What limitations do we internalize without knowing it? In her quiet, matter-of-fact way, Sally Ride shattered assumptions I didn’t know I’d taken on. Like so many people at MIT, I was an explorer at heart. What if I could explore in space as well as in the lab? 

Becoming an astronaut

No one just becomes an astronaut. Every astronaut is something else first. At MIT, I had fallen in love with organic chemistry and was determined to become a research chemist, hoping to use science to improve people’s lives. Because I attended MIT on an ROTC scholarship, I was commissioned as a second lieutenant in the US Air Force upon graduation, but I was given permission to get my doctorate in polymer science and engineering from UMass Amherst before serving. I was then stationed at Wright-Patterson Air Force Base, where I worked on new materials for airplanes and consulted on NASA’s Long Duration Exposure Facility experiment. I also set endurance and tolerance records as a volunteer test subject in the centrifuge at the aeromedical laboratory, testing new equipment.

But the ideas that Sally Ride had sparked were never far from my mind, and when NASA put out a call for new astronauts in 1991, I applied—along with 2,053 others. I was among the 500 who got our references checked, and then one of about 90 invited to Houston for an intense weeklong interview and physical. In 1992, after months of suspense, I got the fateful phone call asking, “Would you still like to come and work with us at NASA?” Thrilled beyond words, I felt a kind of validation I’d never experienced before and have never forgotten.

Four months later, I reported for duty at the Johnson Space Center. Knowing that years of rigorous training lay ahead before I might launch into space on a mission, I couldn’t wait to dive in.

That training turned out to be a wild ride. Within days of our arrival in Houston, we ASCANs (NASA-speak for astronaut candidates) headed to Fairchild Air Force Base in Washington state for land survival training. We practiced navigation skills and shelter building. Knots were tied. Food was scavenged. Worms were eaten. Tired, grubby people made hard decisions together. Rules were broken. Fun was had. And, importantly, we got to know one another. Water survival skills were next—we learned to disconnect from our parachutes, climb into a raft, and make the most of the supplies we had in case we had to eject from a jet or the space shuttle. 

Coleman and the rest of the STS-93 crew head to Launch Pad 39-B for their second attempt at liftoff on the space shuttle Columbia. With this mission, Eileen M. Collins (front row, right) would become the first woman to serve as commander of a shuttle mission.
NASA

Back in Houston, we learned about each of the shuttle systems, studying the function of every switch and circuit breaker. (For perspective, the condensed manual for the space shuttle is five inches thick.) The rule of thumb was that if something was important, then we probably had three, so we’d still be okay if two of them broke. We worked together in simulators (sims) to practice the normal procedures and learn how to react when the systems malfunctioned. For launch sims, even those normal procedures were an adventure, because the sim would shake, pitch, and roll just as the real shuttle could be expected to on launch day. We learned the basics of robotics, spacewalking, and rendezvous (how to dock with another spacecraft without colliding), and we spent time at the gym, often after hours, so we’d be in shape to work in heavy space suits. 

Our training spanned everything from classes in how to use—and fix—the toilet in space to collecting meteorites in Antarctica, living in an underwater habitat, and learning to fly the T-38, an amazing high-performance acrobatic jet used to train Air Force pilots. (On our first training flight, we got to fly faster than the speed of sound.) All of this helped us develop an operational mindset—one geared to making decisions and solving problems in high-speed, high-pressure, real-risk ­situations that can’t be simulated, like the ones we might encounter in space. 

Mission: It’s not about you, but it depends on you

Each time a crew of astronauts goes to space, we call it a mission. It’s an honor to be selected for a mission, and an acknowledgment that you bring skills thatwillmake it successful. Being part of a mission means you are part of something that’s bigger than yourself, but at the same time, the role you play is essential. It’s a strange paradox: It’s not about you, but it depends on you. On each of my missions, that sense of purpose brought us together, bridging our personal differences and disagreements and allowing us to achieve things we might never have thought possible. A crew typically spends at least a year, if not a few years, training together before the actual launch, and that shared mission connects us throughout.

In 1993, I got word that I’d been assigned to my first mission aboard the space shuttle. As a mission specialist on STS-73, I would put my background as a research scientist to use byperforming 30 experiments in microgravity. These experiments, which included growing potatoes inside a locker (just like Matt Damon in The Martian), using sound to manipulate large liquid droplets, and growing protein crystals, would advance our understanding of science, medicine, and engineering and help pave the way for the International Space Station laboratory.

While training for STS-73, I got a call from an astronaut I greatly admired: Colonel Eileen Collins. One of the first female test pilots, she would become the first woman to pilot the space shuttle in 1995, when the STS-63 mission launched. Collins had invited some of her heroes—the seven surviving members of the Mercury 13—to attend the launch, and she was calling to ask me to help host them. The Mercury 13 were a group of 13 women who in the early 1960s had received personal letters from the head of life sciences at NASA asking them to be part of a privately funded program to include women as astronauts. They had accepted the challenge and undergone the same grueling physical tests required of NASA’s first astronauts. Although the women performed as well as or better than the Mercury 7 astronauts on the selection tests, which many of them had made sacrifices even to pursue, the program was abruptly shut down just days before they were scheduled to start the next phase of testing. It would be almost two decades before NASA selected its first female astronauts. 

Never had I felt more acutely aware of being part of that lineage of brave and boundary-breaking women than I did that day, standing among those pioneers, watching Eileen make history. I can’t know what the Mercury 13 were thinking as they watched Eileen’s launch, but I sensed that they knew how much it meant to Eileen to be carrying their legacy with her in the pilot seat of that space shuttle.

Missions and malfunctions

Acouple of years after I had added my name to the still-too-short list of women who had flown in space, Eileen called again. This time she told me that I would be joining her on her next mission, ­STS-93, scheduled to launch in July 1999. Our Mercury 13 heroes would attend that launch too, and Eileen would be making history once again, this time as NASA’s first female space shuttle commander. I would be the lead mission specialist for delivering the shuttle’s precious payload, the Chandra X-ray Observatory, to orbit. I’d also be one of the EVA (extravehicular activity) crew members, if any spacewalking repairs were needed.  

Our mission to launch the world’s most powerful x-ray telescope would change the world of astrophysics. With eight times the resolution of its predecessors and the ability to observe sources that were fainter by a factor of more than 20, Chandra was designed to detect x-rays from exploding stars, black holes, clusters of galaxies, and other high-energy sources throughout the universe. Because cosmic x-rays are absorbed by our atmosphere, we can’t study them from Earth, so an x-ray telescope must operate from well above our atmosphere. Chandra wouldlaunch into low Earth orbit on the shuttle and then require additional propulsion to achieve its final orbit, a third of the way to the moon.

I was thrilled by the idea that my team and I would be launching a telescope whose work would continue long after we were back on Earth. Preparation for launch was intense. As Chandra’s shepherd, I needed to be able to perform what we called the deploy sequence in my sleep. And I had to have a close relationship with the folks at the Chandra Mission Control, which was separate from NASA Mission Control, and make sure the two groups were working together. In a very real sense, Chandra represented the future of astrophysics—a window that promised a deeper understanding of the universe. When the moment came for the telescope to be deployed, all of this would be, quite literally, in my hands.

But first it was in the hands of the launch team at the Kennedy Space Center, whose job it was to get us off the ground and into orbit. And we almost didn’t make it.

Our first launch attempt was aborted eight seconds before liftoff. There we were, waiting for the solid rocket boosters to ignite and the bolts holding us to the launchpad to explode. Instead, we heard “Abort for a hydrogen leak” from Launch Control. Later it was revealed that a faulty sensor had been the issue.  

For our second attempt, we were confidently told we were “one hundred percent GO for weather.” In other words, there was not even a hint of bad weather to delay us. And then there were lightning strikes at the launchpad. Really.

For our third launch attempt, under a bright moon on a cool, clear night, we strapped in and the countdown began. This time I was determined I wouldn’t take anything for granted—even in those final 30 seconds after control switched over to the shuttle’s internal computers. Even when the engines kicked in and I felt the twang of the nose tipping forward and then back. Only when the solid rockets ignited did I let myself believe that we were actually heading back to space. As a seasoned second-time flyer, I kept my excitement contained, but inside I was whooping and hollering. And then, as Columbia rolled to the heads-down position just seconds after liftoff, my joyful inner celebration was drowned out by an angry alert tone and Eileen’s voice on the radio:

Houston: Columbia is in the roll and we have a fuel cell pH number one.

Almost immediately, we got a response from the flight controllers in Houston: 

Columbia, Houston: We’d like AC bus sensors to OFF. We see a transient short on AC1.

It was incomprehensible to be hearing these words less than 30 seconds into our actual flight. An electrical short had taken out two of our six main engine controllers.

My first thought: We know how to deal with this. We did it last week in the simulator. But we weren’t in the simulator anymore. This was a real, no-shit emergency. After we returned to Earth we realized just how close we’d come to several actual life-or-death situations. No matter how much you train for just such a moment, you can’t really anticipate what it will mean to find yourself in one. I was relieved that it wasn’t long before I heard the steady voice of Jeff Ashby, our pilot, confirming that he had successfully flipped the bus sensor switches, reducing our exposure to the potential catastrophe of additional engine shutdowns.

An image of the Space Shuttle taking off.
The Space Shuttle Columbia lifted off from Kennedy Space Center on July 23, 1999, for a five-day mission that would include releasing the Chandra X-ray Observatory.
NASA

We were still headed to space, but with the loss of some of our backup capabilities, we were vulnerable. We carefully monitored the milestones that would tell us which options we still had. I tried not to hold my breath as the shuttle continued to climb and we listened for updates from Houston:

Columbia, Houston: Two Engine Ben. Translation: We could lose an engine and still safely abort the mission and make it to our transatlantic landing site in Ben Guerir, Morocco.

Columbia, Houston: Negative return. Translation: We were too far along to perform an RTLS (return to launch site) and head back to Florida.

Then finally, the call we’d been wishing and waiting for: 

Columbia, Houston: PRESS TO MECO. Translation: We would make it to orbit and main engine cutoff even if one of our engines failed in the next few minutes.

Now, assured of a safe orbit as we hurtled through space, we could turn our attention to our mission: sending Chandra off to its new home.

An electrical short is a serious problem. After our mission landed, the shuttle fleet would be grounded for months after inspections revealed multiple cases of wire chafing on the other shuttles. Some would call us lucky, but listening to the audio from our cockpit and from Mission Control, I credit the well-trained teams that worked their way patiently through multiple failures catalyzed by the short and by a separate, equally dangerous issue: a slow leak in one of our three engines used during launch. 

Our STS-93 launch would go down in the history books as the most dangerous ascent of the shuttle program that didn’t result in an accident. Even in the midst of it, my sense of mission helped anchor me.

The Chandra X-ray Observatory was deployed from the space shuttle Columbia’s payload bay on July 23, 1999, just a few hours after the shuttle’s arrival in Earth orbit.
NASA

The plan in 1999 had been that Chandra would last five years. But as of this writing, Chandra is 25 and still sending valuable data back from space. Each year, on its “birthday,” the crew from STS-93 and the teams who worked on the ground connect via email, or in person for the big ones. We’ll always share a bond from that mission and its continuing legacy. And what a legacy it is. Young astronomers who were still toddlers when I pulled that deploy switch are now making discoveries based on the data it’s produced. Chandra is responsible for almost everything that we now know about black holes, and it’s still advancing our understanding of the universe by giant leaps. But these are difficult times. Sadly, budget cuts proposed in 2025 would eliminate Chandra, with no replacements planned. 

Suiting up and making change 

People often wonder what would possess any sane person to strap themself on top of a rocket. And by now you’re probably wondering why, after the harrowing malfunctions during the STS-93 launch, I was eager not only to return to space again but to spend six months living and working aboard the International Space Station. It comes back to mission. I don’t consider myself to be braver than most people, though I may be more optimistic than many. I take the risks associated with my job because I believe in what we’re doing together, and I trust my crew and our team to do all that’s humanly possible to keep us safe.

But the odds were stacked against me in my quest to serve on the space station. 

The world of space exploration, like so many others, is slow to change. Long-standing inequities were still evident when I joined NASA in 1992, and many endured during my time there. But it can be difficult to know when to fight for change at the outset and when to adapt to unfair circumstances to get your foot in the door.

The first trained astronauts tended to be tall, athletic, and male—and the biases and assumptions that led to that preference were built into our equipment, especially our space suits. Our one-piece orange “pumpkin suits” worn for launching and landing weren’t designed for people with boobs or hips, so many of us wound up in baggy suits that made fitting a parachute harness tricky and uncomfortable. But fit issues with our 300-pound white spacewalking suits proved to be a much bigger problem, especially for the smaller-framed astronauts—including some men. 

The bulky EVA suits, which allow astronauts who venture outside a spacecraft to breathe and communicate while regulating our temperature and protecting us from radiation, are essentially human-shaped spaceships. But while they came in small, medium, large, and extra-large, those suits were designed for (male) astronauts of the Apollo era with no thought to how they might work for different body types. Given that ill-fitting equipment would affect performance, astronauts like me—who weren’t shaped like Neil Armstrong, Buzz Aldrin, and their compatriots—were often negatively prejudged before we even started training. As a result, NASA failed for years to leverage the skills of many members of the astronaut corps who physically didn’t fit an institutional template that hadn’t been redesigned for half a century.

Spacewalk training was the most physically difficult thing I did as an astronaut. Training in that way-too-large space suit made it even harder, forcing me to find ways to optimize my ability to function.  

As she prepares to head into the pool for EVA training, Coleman dons glove liners. Next, the bottom of her suit will be attached to the top and her gloves will be attached at the wrist ring, locked, and tested for a solid seal. Coleman qualified as a spacewalker for all of her missions, even when that required doing so in a medium suit that was much too big.
NASA

We practice spacewalking underwater in an enormous swimming pool. If the suit is too big for you—as even the small was for me—the extra volume of air inside drags you up to the surface when you’re trying to work underwater. It’s a profound physical disadvantage. 

Though the fit of the small spacewalking suit wasn’t great, I persevered and adapted, training for many years in that suit with above-average spacewalking grades. And I was chosen to serve as a spacewalker for both of my shuttle missions, should the need arise. Not long before my first mission, Tom Akers, one of the experienced spacewalkers, came up to me and said, “Cady, I can see that you have a real aptitude for spacewalking and also a head that thinks like a spacewalker.” But then he told me that to cut costs, NASA had decided not to use the small suits on the space station. “People are going to look at you and think you’re too small, but I think someone like you could learn to function inside a medium suit,” he said. “So my advice is this: If you are interested in flying on the space station, then when someone asks you what size suit you wear, you tell them a medium will be no problem.” 

Sure enough, after my second shuttle flight, NASA announced that the small suit would be eliminated. I’ve never forgotten the wording of the rationale: “We’ve looked ahead at the manifest, and we have all of the spacewalkers that we need.” Implied was that they wouldn’t miss the smaller astronauts—not a bit. 

I think people might not have understood at the time what it meant to get rid of those small space suits. You could not live and work on the space station unless you were space-suit qualified. And because NASA was about to shut down the shuttle program, soon missions to the space station would be the only ones there were. NASA’s decision to eliminate the small suit effectively grounded more than a third of female astronauts. It also meant that few women would have the experience needed to serve in positions where they could have a say in important decisions about everything from prioritizing missions and choosing crews to making changes in NASA’s culture.    

To me, eliminating the small space suit indicated that the organization didn’t understand the value of having teams whose members contribute a wide range of experiences and viewpoints. When team members are too much alike—in background, ways of thinking and seeing the world, and, yes, gender—the teams are often less effective at finding innovative solutions to complex problems. 

Determined to contribute to the important scientific work being done on the space station, I had no choice but to qualify in the medium suit. But it would be a tall order because for the instructors, the gear is seldom at fault. You just need to get used to it, understand it better, or practice more. I did all three—but it wasn’t enough. So I also adapted everywhere I could, and I recruited a lot of great help. Kathy Thornton, one of the first female spacewalkers, recommended that I buy a waterskiing vest at Walmart to wear inside the suit. The space-suit team was horrified at the thought of using nonregulation materials, but it got them thinking. Together, we settled on having me wear a large girdle—left over from the Apollo guys—and stuffing it with NASA-approved foam to center me in the suit. This kept the air pockets more evenly distributed and allowed me to practice the required tasks, showing that I could work effectively in a medium.

By adapting, which sometimes means staying silent, you may perpetuate a discriminatory system. But if I’d tried to speak the truth from day one, I’d never have made it to the day when I was taken seriously enough to start conversations about the importance of providing all astronauts with equipment that fits. I needed to launch those discussions from a place of strength, where I could be heard and make a difference.

How best to catalyze change is always a personal decision. Sometimes drawing a line in the sand is the most effective strategy. Other times, you have to master the ill-fitting equipment before you get a chance to redesign it. Qualifying in the too-large suit was my only option if I wanted to fly on the International Space Station, since every flight to the ISS needed two spacewalkers and a backup spacewalker—and there were only three seats in the space capsule. The alternative would have been waiting at least 11 years for the newer spacecraft, which would have a fourth seat. I had to play by the unfair rules in order to get to a point where I could change those rules.

With grit and a lot of support from others, I did end up qualifying in the medium suit. And in 2010, I set off for the International Space Station, serving as the lead robotics and science officer for Expedition 26/27 as I traveled 63,345,600 miles in 2,544 orbits over 159 days in space.

Coleman conducts the Capillary Flow Experiment on the International Space Station to study the behavior of liquids at interfaces in microgravity.
NASA/PAOLO NESPOLI

Today, efforts are underway to redesign NASA’s space suits to fit the full range of sizes represented in the astronaut corps. Because of the work I put in to make it possible for a wider range of people to excel as spacewalkers, NASA hung a portrait of me in the row of space-suit photos outside the women’s locker room. And I’m proud to know that my colleagues—women and men—are continuing the work of making change at NASA. Every change has been hard won. The numbers matter. The astronaut corps is now 40% women. Given that, it is harder to make decisions with the potential to leave women out. When a female NASA astronaut walks on the moon for the first time, she will do so in a redesigned space suit. I hope it fits her like a glove.

The crew of spaceship Earth

Contributing to an important mission is a privilege. But who gets to contribute is as important to mission success as it is to the individuals who want to play a part. I can’t emphasize enough how much our incredibly complex NASA missions have benefited from the broad range of people involved. Bringing together people of different backgrounds and skills, with different ways of seeing the world and unique perspectives on opportunities and problems, is what makes space exploration possible.

At the White House Science Fair in 2016, Coleman sits with the “Supergirls” Junior FIRST Lego League Team from Girl Scout Troop 411 in Tulsa, Oklahoma, as they await the arrival of President Barack Obama
NASA/JOEL KOWSKY

Sharing space, to me, means including more people—both in the privilege of going to space and in so many of our endeavors here on Earth. When I applied to be an astronaut, very few women had orbited our planet. Today, that number has grown to 82 of 633 human beings in total, and newer NASA astronaut classes have averaged 50% women. Spaceflight is making progress in terms of including people with a wider range of backgrounds, fields of expertise, and physical abilities. But we have a long way to go. And the same is true in countless fields—the barriers that we struggle with in space exploration seem to be ubiquitous in the working world.

As a planet, we’re facing enormous challenges, in areas from climate change to public health to how to sustainably power our endeavors. If there’s one thing I learned above all else from my time in space, it’s that we’re all sharing Earth. No one else is coming to solve our complex problems. And we won’t find solutions with teams of people who share too much in common. We need everyone to contribute where they can, and so we need to create systems, environments, and equipment that make that possible. And we need to be sure that those making contributions are visible, so they can serve as models for future generations. Our job now is to make sure everyone gets enough support to acquire the skills that we—all of us—need to build collaborative teams and solve problems both on Earth and in space. 

It’s worth repeating: We’re all sharing Earth. Looking down from space, you see very few borders separating humans from one another. You understand—not as an abstract ideal but as a visceral, obvious reality—that we are one family sharing a precious, life-supporting home. It’s so clear from up there that we are all the crew of “Spaceship Earth.” I believe that sharing that perspective, bringing it to life, will help more people see that our differences matter less than what binds us together, and motivate us to combine our efforts to tackle the challenges affecting all of us.


In her 24 years at NASA, Cady Coleman ’83, a scientist, musician, and mother of two, flew on two space shuttle missions and began her 159-day mission aboard the International Space Station the day after turning 50. Today, as a public speaker and consultant, she shares her insights on leadership and teamwork gleaned from the high-stakes world of space exploration.

Sharing Space cover

This excerpt is adapted from her book, Sharing Space: An Astronaut’s Guide to Mission, Wonder, and Making Change, published by Viking, an imprint of Penguin Random House. © 2024 by Catherine Coleman.  

Travels with Rambax

KAOLACK, Senegal – The MIT students have just finished dinner and are crumpling soda cans into trash bins when they get the summons: “Grab your drums, grab your drums, grab your drums …” 

It is time for the tanibeer, a nighttime drum and dance party, in Kaolack, a town amid salt plains and peanut farms located 220 kilometers southeast of Dakar, Senegal’s capital. For the members of Rambax MIT, the Institute’s Senegalese drumming ensemble, the excitement is palpable as they fetch their drums and make their way up the road. Their destination is a small field on the family land of their director, Lamine Touré, who comes from a long line of griots, the musicians and oral historians of the Wolof people.

Lamine Touré, director of Rambax MIT, leads drum practice in Grand Mbao
NIKO ODHIAMBO ’25

Touré, a Senegalese master drummer and an MIT lecturer in world music, cofounded Rambax in 2001 with Patricia Tang, an associate professor and ethnomusicologist who specializes in West African music. It began as an extracurricular group to teach students and other members of the MIT community the art of sabar, a vibrant West African drumming and dance tradition. Today, Rambax is a credit-bearing class (21M.460) enrolling as many as 50 students a semester, and its ensemble’s performances draw audiences from MIT and the wider Boston community.  

During Independent Activities Period (IAP), 16 members of the ensemble joined Touré and Tang on a two-week study tour in Senegal, the birthplace of the music that inspires Rambax. In addition to performing, the students attended drumming classes and dance workshops taught by expert Senegalese drummers, and they experienced sabar drumming within its traditional and cultural context in Dakar and Kaolack.

A sabar celebration, known as a tanibeer when held at night, is a lavish display of dance music, a great neighborhood carnival.

“Rambax is unique,” says Touré, whose family of prominent griot percussionists had him drumming from the age of four. Traveling to Senegal allowed the students to experience the cultural significance of the music—and Touré says their Senegalese audiences were really impressed with their playing.

Poster for the tanibeer in Kaolack, Senegal, featuring Rambax MIT.
COURTESY OF RAMBAX

A sabar celebration, also known as a tanibeer when held at night, is a lavish display of dance music: a great neighborhood carnival, jammed with lights, blaring speakers, griots, costumed dancers, drums and drums and ever more drums, and—of course—dancing.

On the night of the Rambax tanibeer in January, the sky is clear and chilly breezes waft across the field, where throngs of people, some dressed in colorful Senegalese traditional garb, gather under fluorescent lights perched on lampposts, chatting and gesticulating while waiting to watch the performance.

As the MIT students walk in, wearing their bright yellow, green, and red knee-length dashikis, the crowd erupts into applause. 

Standing in front of his hometown audience, long dark dreadlocks spilling to his shoulders, Touré takes a microphone and introduces the ensemble in his native Wolof. He explains that his students are lovers of African music and, under his tutelage at MIT, have been learning the art of sabar. He pauses for a moment and leans in close to start conducting. 

Then Rambax begins to play.

Local musicians join MIT students as they play their sabar drums at the Grand Mbao practice session.
NIKO ODHIAMBO ’25

The audience cheers and dances, forming a large circle in front of the musicians. Before long, women take turns at the center of the circle, matching the energetic rhythms of the drumming in the exuberant hip twists, arm swings, jumps, and impossibly high knee kicks of sabar dancing. The high-spirited drumming and dancing continue until the early hours of the morning.   

The tanibeer is a chance for Touré “to show what he’s been teaching his American students and that they can really play sabar quite well,” says Tang, who serves as a faculty advisor to Rambax. “And that’s often a surprise to the Senegalese audience.” 

Senegalese drummers Sadda Sene, Mbaye Ndiaga Seck, and Pa Ali Konte load drums onto the Rambax van after drum practice.
PATRICIA TANG
Drum practice on the beach in Grand Mbao.
COURTESY OF RAMBAX

Among the 16 Rambax members on the Senegal trip is Autumn Geil ’21, a researcher and PhD student in the department of mechanical engineering. Initially drawn to music through choir and opera singing in high school, she had never heard of sabar drumming before discovering Rambax through a friend as an undergrad. She joined and has been a member of the ensemble, which she calls “just so incredible,” ever since. 

Rambax MIT students
Eri-ife Olayinka ’25 and Kaelyn Dunnell ’25 by the sea in Grand Mbao.
NIKO ODHIAMBO ’25

For Geil, practicing sabar with custodians of the tradition in Senegal is an opportunity to “observe and learn from the drummers to improve my skills for future performances.” 

Baran Mensah ’24, a Ghanian master’s student in mechanical engineering who minored in music as an undergrad, also joined Rambax after a friend recommended it. He sees it as a way to tap into his African roots while at MIT but says it’s also “a gateway to learn about Senegalese art, music, and culture.” Until the tour, he notes, “I really didn’t know much about my country’s West African neighbor.”   

“Coming on this trip allows us to take a step back, to learn about people and cultures, making us more effective communicators.”

Autumn Geil ’21

Eri-ife Olayinka ’25, a computation and cognition major who took Rambax classes for two semesters, says she finds the learning environment supportive and the cultural insights provided by Touré and Tang rewarding. “You see yourself getting better, becoming comfortable with playing in the class,” she says. After completing the classes to satisfy her art requirements, Olayinka stayed on in the drumming ensemble. “I genuinely enjoy being in Rambax—it’s such a cool thing we get to do as a group,” she says.

Sabar artists Badara Faye, Mbaye Ndiaga Seck, and Pa Ali Konte take the mic at a tanibeer in Grand Mbao
NIKO ODHIAMBO ’25

Visiting Kaolack is more than an opportunity for Rambax members to glimpse the culture that gave rise to sabar. With horse-drawn wagons clip-clopping through its rugged terrain but also massive solar farms, Kaolack is a city where old meets new. Witnessing those contrasts—and getting to perform and to immerse themselves in the performances of local musicians—helps the students enhance what Geil calls the “human connection skills” that all scientists and technologists need. 

“It’s really important for people in STEM to make space for art and music,” she says. “Coming on this trip allows us to take a step back, to learn about people and cultures, making us more effective communicators of our technology.” 

Grad student Natalie Huang ’24 and local musician Badara Faye dance at a tanibeer in Grand Mbao.
NIKO ODHIAMBO ’25
Rambax members watch Sengalese dancers and drummers at the tanibeer in Kaolack.
NIKO ODHIAMBO ’25
Grad student Tina Chen ’24, Neha Basu ’25, Pa Ali Konte, Monique Brewster ’10, and grad student Sandra Huffman ’20, SM ’21, drum at the tanibeer in Kaolack.
PATRICIA TANG

Rambax MIT plays at the tanibeer in Kaolack.
COURTESY OF RAMBAX

Back inside Touré’s family compound, Tang invites the students to gather around so she can introduce them to Touré’s mother, Marie Sow, and his sisters and aunts. Sow showers them with good wishes and they bask in the glow.

It’s important for Rambax members to know the history and culture of the people behind the music they practice, says Tang. “We really want the students to have this sort of cultural immersion—live in a Senegalese house like the Senegalese people do, hang out with Senegalese drummers, and really get a sense of what it’s like in Senegal.”

Abdullahi Tsanni, SM ’23, a former MIT Technology Review fellow, is a science writer based in Dakar, Senegal, who specializes in narrative features.