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55 Years Ago: Star Trek Final Episode Airs, Relationship with NASA Endures

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The voyages of the Starship Enterprise came to a sudden and premature end on June 3, 1969, with the airing of the final episode of the Star Trek original television series. Ironically, the show’s cancellation came just six weeks before humanity embarked on its first voyage to land on another celestial body. Although the show ran for only three seasons, it generated a devoted fan base disappointed by the cancellation despite their write-in campaign to keep it on the air. But as things turned out, over the decades Star Trek evolved into a global phenomenon, first with the original episodes replayed in syndication, followed by a series of full-length motion pictures, and eventually a multitude of spin-off series. With its primary focus on space exploration, along with themes of diversity, inclusion, and innovation, the Star Trek fictional universe formed a natural association with NASA’s real life activities.

A scene from “The Man Trap,” the premiere episode of Star Trek The cast of the original Star Trek series from a promotional ad for the 1968-9 season A scene from “Turnabout Intruder,” the final episode of the original series
Left:  A scene from “The Man Trap,” the premiere episode of Star Trek. Middle: The cast of the original Star Trek series from a promotional ad for the 1968-9 season. Right: A scene from “Turnabout Intruder,” the final episode of the original series. Image credits: courtesy NBC-TV.

Star Trek creator Gene Roddenberry first had the idea for a science fiction television series in 1964. He presented his idea, a show set in the 23rd century aboard a starship with a crew dedicated to exploring the galaxy, to Desilu Productions, an independent television production company headed by Lucille Ball. They produced a pilot titled “The Cage,” selling it to the National Broadcasting Corporation (NBC) network that then bought a second pilot titled “Where No Man Has Gone Before.” NBC introduced the show to its fall 1966 lineup, with the first episode “The Man Trap” airing on Sep. 8. To put that date in perspective, NASA launched Gemini XI four days later, one of the missions that helped the agency achieve the Moon landing nearly three years later. Meanwhile, Star Trek’s Starship Enterprise continued its fictional five-year mission through the galaxy to “seek out new life and new civilizations.” The makeup of the Enterprise’s crew made the show particularly attractive to late 1960s television audiences. The major characters included an African American woman communications officer, an Asian American helmsman, and a half-human half-Vulcan science officer, later joined by a Russian-born ensign. While the show enjoyed good ratings during its first two seasons, cuts to its production budget resulted in lower quality episodes during its third season leading to lower ratings and, despite a concerted letter-writing campaign from its dedicated fans, eventual cancellation.

NASA Administrator James C. Fletcher, left, with the creator and cast members of Star Trek at the September 1976 rollout of space shuttle Enterprise The cast members give the Vulcan salute
Left: NASA Administrator James C. Fletcher, left, with the creator and cast members of Star Trek at the September 1976 rollout of space shuttle Enterprise. Right: The cast members give the Vulcan salute.

Despite the show’s cancellation, Star Trek lived on and prospered in syndication and attracted an ever-growing fan base, turning into a worldwide sensation. Often dubbed “trekkies,” these fans held the first of many Star Trek conventions in 1972. When in 1976 NASA announced that it would name its first space shuttle orbiter Constitution, in honor of its unveiling on the anniversary of the U. S. Constitution’s ratification, trekkies engaged in a dedicated letter writing campaign to have the orbiter named Enterprise, after the starship in the television series. This time the fans’ letter writing campaign succeeded. President Gerald R. Ford agreed with the trekkies and directed NASA to rechristen the first space shuttle. When on Sept. 17, 1976, it rolled out of its manufacturing plant in Palmdale, California, appropriately accompanied by a band playing the show’s theme song, it bore the name Enterprise. Many of the original cast members of the show as well as its creator Rodenberry participated in the rollout ceremony, hosted by NASA Administrator James C. Fletcher. Thus began a lengthy relationship between the space agency and the Star Trek brand.

Star Trek cast member Nichelle Nichols, left, in the shuttle simulator with astronaut Alan L. Bean at NASA’s Johnson Space Center (JSC) in Houston Nichols at the controls of the shuttle simulator Nichols, left, in JSC’s Mission Control Center during filming of the recruiting video
Left: Star Trek cast member Nichelle Nichols, left, in the shuttle simulator with astronaut Alan L. Bean at NASA’s Johnson Space Center (JSC) in Houston. Middle: Nichols at the controls of the shuttle simulator. Right: Nichols, left, in JSC’s Mission Control Center during filming of the recruiting video.

During the development of the space shuttle in the 1970s, the need arose to recruit a new group of astronauts to fly the vehicle, deploy the satellites, and perform the science experiments. When NASA released the call for the new astronaut selection on July 8, 1976, it specifically encouraged women and minorities to apply. To encourage those applicants, NASA chose Nichelle Nichols, who played communications officer Lt. Uhura on the Starship Enterprise, to record a recruiting video and speak to audiences nationwide. She came to NASA’s Johnson Space Center (JSC) in Houston in March 1977, and accompanied by Apollo 12 and Skylab 3 astronaut Alan L. Bean, toured the center and filmed scenes for the video in Mission Control and other facilities. NASA hoped that her stature and popularity would encourage women and minorities to apply, and indeed they did. In January 1978, when NASA announced the selection of 35 new astronauts from more than 8,000 applicants, for the first time the astronaut class included women and minorities. All distinguished themselves as NASA astronauts and paved the way for others in subsequent astronaut selections. Nichols returned to JSC in September 2010 with the Traveling Space Museum, an organization that partners with schools to promote space studies. She toured Mission Control and the International Space Station trainer accompanied by NASA astronaut B. Alvin Drew. She also flew aboard NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) airborne telescope aircraft managed by NASA’s Ames Research Center in Silicon Valley, California, in September 2015.

Nichols, center, aboard NASA’s Stratospheric Observatory for Infrared Astronomy aircraft Nichols, center, aboard NASA’s Stratospheric Observatory for Infrared Astronomy aircraft
Left: Nichelle Nichols, middle, with NASA astronaut B. Alvin Drew in the space station trainer at NASA’s Johnson Space Center in Houston. Right: Nichols, center, aboard NASA’s Stratospheric Observatory for Infrared Astronomy aircraft.

Meanwhile, the Star Trek brand renewed itself in 1979 as a full-length motion picture with the original TV series cast members reprising their roles. Over the years, several sequels followed this first film. And on the small screen, a reboot of sorts occurred in 1987 with the premiere of Star Trek: The Next Generation, a new series set in the 24th century aboard the Enterprise-D, a next generation starship with a new crew. That series lasted seven seasons, followed by a near-bewildering array of spin-off series, all built on the Star Trek brand, that continue to this day.

Actor James Doohan visits NASA’s Dryden (now Armstrong) Flight Research Center in California in 1967 with NASA pilot Bruce A. Peterson, in front of the M2-F2 lifting body aircraft At NASA’s Johnson Space Center in Houston, Doohan sits in the commander’s seat of the space shuttle simulator, as NASA astronaut Mario Runco looks on Doohan, second from left, during his retirement party with fellow Star Trek stars George Takei, left, and Nichelle Nichols, and Apollo 11 astronaut Neil A. Armstrong
Left: Actor James Doohan visits NASA’s Dryden (now Armstrong) Flight Research Center in California in 1967 with NASA pilot Bruce A. Peterson, in front of the M2-F2 lifting body aircraft. Middle: At NASA’s Johnson Space Center in Houston, Doohan sits in the commander’s seat of the space shuttle simulator, as NASA astronaut Mario Runco looks on. Right: Doohan, second from left, during his retirement party with fellow Star Trek stars George Takei, left, and Nichelle Nichols, and Apollo 11 astronaut Neil A. Armstrong. Credit: Image courtesy Anne Cusack/Los Angeles Times.

James Doohan, the actor who played Lt. Cmdr. Montgomery “Scotty” Scott, the Starship Enterprise’s chief engineer, had early associations with NASA. In April 1967, Doohan visited NASA’s Dryden (now Armstrong) Flight Research Center in California, spending time with NASA test pilot Bruce A. Peterson. A month later, Peterson barely survived a horrific crash of the experimental M2-F2 lifting body aircraft. He inspired the 1970s TV series The Six-Million Dollar Man, and the show’s opening credits include film of the crash. Doohan narrated a documentary film about the space shuttle released shortly before Columbia made its first flight in April 1981. In January 1991, Doohan visited JSC and with NASA astronaut Mario Runco (who sometimes went by the nickname “Spock”) toured the shuttle trainers, Mission Control, and tried his hand at operating the shuttle’s robotic arm in the Manipulator Development Facility. In a unique tribute, astronaut Neil A. Armstrong, the first person to step on the lunar surface, spoke at Doohan’s retirement in 2004, addressing him as “one old engineer to another.”

Takei and Robonaut both give the Vulcan greeting Takei and Robonaut both give the Vulcan greeting
Left: Director of NASA’s Johnson Space Center in Houston Michael L. Coats presents actor George Takei with a commemorative plaque. Right: Takei and Robonaut both give the Vulcan greeting.

George Takei, who played Enterprise helmsman Lt. Hikaru Sulu, and his husband Brad, visited JSC in May 2012. Invited by both Asian American and LGBTQ+ Employee Resource Groups, Takei spoke of leadership and inclusiveness, including overcoming challenges while in Japanese American internment camps during World War II and as a member of the LGBTQ+ community. He noted that Star Trek remained ahead of its time in creating a future when all members of society could equally participate in great undertakings, at a time when the country struggled through the Civil Rights movement and the conflict in Southeast Asia. The inclusiveness that is part of NASA’s culture greatly inspired him. JSC Director Michael L. Coats presented Takei with a plaque including a U.S. flag flown aboard space shuttle Atlantis’ STS-135 mission. He also visited Mission Control and spent some time with Robonaut.

Star Trek cast member Leonard Nimoy gives the Vulcan greeting in front of space shuttle Enterprise after its arrival in New York in 2012 Expedition 43 crew member European Space Agency astronaut Samantha Cristoforetti gives the Vulcan salute to honor the late actor Nimoy
Left: Star Trek cast member Leonard Nimoy gives the Vulcan greeting in front of space shuttle Enterprise after its arrival in New York in 2012. Right: Expedition 43 crew member European Space Agency astronaut Samantha Cristoforetti gives the Vulcan salute to honor the late actor Nimoy. 

Leonard Nimoy played the science officer aboard the Starship Enterprise, the half-human, half-Vulcan Mr. Spock. The actor watched in September 2012 when space shuttle Enterprise arrived at John F. Kennedy International Airport in New York, on the last leg of its journey to the Intrepid Sea, Air and Space Museum, where it currently resides. “This is a reunion for me,” observed Nimoy. “Thirty-five years ago, I met the Enterprise for the first time.” As noted earlier, the Star Trek cast attended the first space shuttle’s rollout in 1976. Following his death in 2015, European Space Agency astronaut Samantha Cristoforetti paid tribute to Nimoy aboard the International Space Station by wearing a Star Trek science officer uniform, giving the Vulcan greeting, and proclaiming, “Of all the souls I have encountered … his was the most human.”

Star Trek cast member William Shatner, left, receives the Distinguished Public Service Medal from NASA Deputy Associate Administrator for Communications Robert N. Jacobs in 2014 Shatner, upper left, moderates a virtual panel at the 2020 San Diego Comic-Con with NASA spacesuit engineer Lindsay T. Aitchison, upper right, NASA astronauts Nicole A. Mann, lower left, and Kjell N. Lindgren, and NASA technology expert LaNetra C. Tate Shatner experiences weightlessness during his suborbital trip to the edge of space aboard a New Shepard vehicle
Left: Star Trek cast member William Shatner, left, receives the Distinguished Public Service Medal from NASA Deputy Associate Administrator for Communications Robert N. Jacobs in 2014. Middle: Shatner, upper left, moderates a virtual panel at the 2020 San Diego Comic-Con with NASA spacesuit engineer Lindsay T. Aitchison, upper right, NASA astronauts Nicole A. Mann, lower left, and Kjell N. Lindgren, and NASA technology expert LaNetra C. Tate. Image credit: courtesy Comic-Con International. Right: Shatner experiences weightlessness during his suborbital trip to the edge of space aboard a New Shepard vehicle. Image credit: courtesy Blue Origin.

Captain James T. Kirk, played by actor William Shatner, a life-long advocate of science and space exploration, served at the helm of the Starship Enterprise. His relationship with NASA began during the original series, with references to the space agency incorporated into several story lines. In 2011, Shatner hosted and narrated a NASA documentary celebrating the 30th anniversary of the Space Shuttle program, and gave his time and voice to other NASA documentaries. NASA recognized Shatner’s contributions in 2014 with a Distinguished Public Service Medal, the highest award NASA bestows on non-government individuals. NASA Deputy Associate Administrator for Communications Robert “Bob” N. Jacobs presented the medal to Shatner. The award’s citation read, “For outstanding generosity and dedication to inspiring new generations of explorers around the world, and for unwavering support for NASA and its missions of discovery.” In 2019, Shatner narrated the NASA video We Are Going, about NASA’s plans to return astronauts to the Moon. He has spoken at numerous NASA-themed events and moderated panels about NASA’s future plans. On Oct. 13, 2021, at the age of 90, Shatner reached the edge of space during the NS-18 suborbital flight of Blue Origin’s New Shepard vehicle, experiencing three minutes of weightlessness.

Patch for the Window Observational Research Facility (WORF), including the Klingon writing just below the letters “WORF.” Astronaut Naoki Yamazaki of the Japan Aerospace Exploration Agency and the WORF rack after its installation aboard the space station during STS-131 The STS-54 crew dressed as Starfleet officers
Left: Patch for the Window Observational Research Facility (WORF), including the Klingon writing just below the letters “WORF.” Middle: Astronaut Naoki Yamazaki of the Japan Aerospace Exploration Agency and the WORF rack after its installation aboard the space station during STS-131. Right: The STS-54 crew dressed as Starfleet officers.

The Space Flight Awareness (SFA) poster for the Expedition 21 crew The SFA poster for the STS-134 crew
Left: The Space Flight Awareness (SFA) poster for the Expedition 21 crew. Right: The SFA poster for the STS-134 crew.

Elements of the Star Trek universe have made their way not only into popular culture but also into NASA culture. As noted above, Star Trek fans had a hand in naming the first space shuttle Enterprise. NASA’s Earth observation facility aboard the space station that makes use of its optical quality window bears the name the Window Observational Research Facility (WORF). The connection between that acronym and the name of a Klingon officer aboard the Enterprise in the Star Trek: The Next Generation TV series seemed like an opportunity not to be missed – the facility’s official patch bears its name in English and in Klingon. Several astronaut crews have embraced Star Trek themes for their unofficial photographs. The STS-54 crew dressed in the uniforms of Starship Enterprise officers from Star Trek II: The Wrath of Kahn, the second full-length feature motion picture of the series. Space shuttle and space station crews created Space Flight Awareness (SFA) posters for their missions, and more than one embraced Star Trek themes. The Expedition 21 crew dressed in uniforms from the original series, while the STS-134 crew chose as their motif the 2009 reboot motion picture Star Trek.

Picture of the Gemini VI launch in the background in the 1967 Star Trek episode “Court Martial.” NASA astronaut Mae C. Jemison, left, and actor LeVar Burton in a 1993 episode of Star Trek: The Next Generation NASA astronauts Terry W. Virts, left, and E. Michael Fincke, right, flank actor Scott Bakula on the set of Star Trek: Enterprise in 2005
Left: Picture of the Gemini VI launch in the background in the 1967 Star Trek episode “Court Martial.” Credit: Image courtesy of Collectspace.com. Middle: NASA astronaut Mae C. Jemison, left, and actor LeVar Burton in a 1993 episode of Star Trek: The Next Generation. Credit: Image courtesy CBS. Right: NASA astronauts Terry W. Virts, left, and E. Michael Fincke, right, flank actor Scott Bakula on the set of Star Trek: Enterprise in 2005. Credit: Image courtesy CBS.

As much as Star Trek has influenced NASA, in turn the agency has left its mark on the franchise, from episodes referencing actual and future spaceflight events to NASA astronauts making cameo appearances on the show. The first-season episode “Court Martial” that aired in February 1967 featured a photograph of the December 1965 Gemini VI launch adorning a wall aboard a star base. In the second-season episode “Return to Tomorrow,” airing in February 1968, Captain Kirk in a dialogue about risk-taking remarks, “Do you wish that the first Apollo mission hadn’t reached the Moon?” a prescient reference to the first Apollo mission to reach the Moon more than 10 months after the episode aired. Astronaut Mae C. Jemison, who credits Nichelle Nichols as her inspiration to become an astronaut, appeared in the 1993 episode “Second Chances” of Star Trek: The Next Generation, eight months after her actual spaceflight aboard space shuttle Endeavour. In May 2005, two other NASA astronauts, Terry W. Virts and E. Michael Fincke, appeared in “These are the Voyages…,” the final episode of the series Star Trek: Enterprise.

NASA astronaut Victor J. Glover, host of the 2016 documentary “NASA on the Edge of Forever: Science in Space.” Actress Nichelle Nichols appearing in the documentary “NASA on the Edge of Forever: Science in Space.”
Left: NASA astronaut Victor J. Glover, host of the 2016 documentary “NASA on the Edge of Forever: Science in Space.” Right: Actress Nichelle Nichols appearing in the documentary “NASA on the Edge of Forever: Science in Space.”

In the 2016 documentary “NASA on the Edge of Forever: Science in Space,” host NASA astronaut Victor J. Glover states, “Science and Star Trek go hand-in-hand.” The film explores how for 50 years, Star Trek influenced scientists, engineers, and even astronauts to reach beyond their potential. While the space station doesn’t speed through the galaxy like the Starship Enterprise, much of the research conducted aboard the orbiting facility can make the fiction of Star Trek come a little closer to reality. Several of the cast members from the original TV series share their viewpoints in the documentary, along with those of NASA managers and scientists. Over the years, NASA has created several videos highlighting the relationship between the agency and the Star Trek franchise. In 2016, NASA Administrator Charles F. Bolden led a video tribute to celebrate the 50th anniversary of the first Star Trek episode.

In a tribute to Star Trek creator Gene Roddenberry on the 100th anniversary of his birth, his son Rod, upper left, hosts a virtual panel discussion about diversity and inspiration
In a tribute to Star Trek creator Gene Roddenberry on the 100th anniversary of his birth, his son Rod, upper left, hosts a virtual panel discussion about diversity and inspiration.

In 2021, on the 100th anniversary of Gene Roddenberry’s birth, his son Rod hosted a virtual panel discussion, introduced by NASA Administrator C. William “Bill” Nelson, about diversity and inspiration, two ideals the Star Trek creator infused into the series. Panelists included Star Trek actor Takei, Tracy D. Drain, flight systems engineer for the Europa Clipper spacecraft at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, NASA astronaut Jonny Kim, Swati Mohan, guidance and operations lead for the Mars 2020 rover at JPL, and Hortense B. Diggs, Director of the Office of Communication and Public Engagement at NASA’s Kennedy Space Center in Florida.

The mutual attraction between NASA and Star Trek stems from, to paraphrase the opening voiceover from the TV series, that both seek to explore and discover new worlds, and to boldly go where no one has gone before. The diversity, inclusion, and inspiration involved in these endeavors ensure that they will live long and prosper.

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      Aquila, The Eagle
      From July and into August, is a great time to observe the constellation Aquila, the eagle.
      Sky chart showing the shape and orientation of the constellation Aquila in the July evening sky. Aquila’s brightest star, Altair, is part of the Summer Triangle star pattern. NASA/JPL-Caltech This time of year, it soars high into the sky in the first half of the night. Aquila represents the mythical eagle that was a powerful servant and messenger of the Greek god Zeus. The eagle carried his lightning bolts and was a symbol of his power as king of the gods.
      To find Aquila in the sky, start by locating its brightest star, Altair. It’s one the three bright stars in the Summer Triangle, which is super easy to pick out during summer months in the Northern Hemisphere. Altair is the second brightest of the three, and sits at the southernmost corner of the triangle.
      The other stars in Aquila aren’t as bright as Altair, which can make observing the constellation challenging if you live in an area with a lot of light pollution. It’s easier, though, if you know how the eagle is oriented on the sky. Imagine it’s flying toward the north with its wings spread wide, its right wing pointed toward Vega. If you can find Altair, and Aquila’s next brightest star, you can usually trace out the rest of the spread-eagle shape from there. ​​The second half of July is the best time of the month to observe Aquila, as the Moon doesn’t rise until later then, making it easier to pick out the constellation’s fainter stars.
      Observing the constellation Aquila makes for a worthy challenge in the July night sky. And once you’re familiar with its shape, it’s hard not to see the mythical eagle soaring overhead among the summertime stars.
      Here are the phases of the Moon for July.
      The phases of the Moon for July 2025. NASA/JPL-Caltech You can stay up to date on all of NASA’s missions exploring the solar system and beyond at science.nasa.gov. I’m Preston Dyches from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.
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    • NASA
      Discovery Alert: Flaring Star, Toasted Planet
      By NASA
      Artist’s concept of the star HIP 67522 with a flare erupting toward an orbiting planet, HIP 67522 b. A second planet, HIP 67522 c, is shown in the background. Janine Fohlmeister, Leibniz Institute for Astrophysics Potsdam The Discovery
      A giant planet some 400 light-years away, HIP 67522 b, orbits its parent star so tightly that it appears to cause frequent flares from the star’s surface, heating and inflating the planet’s atmosphere.
      Key Facts
      On planet Earth, “space weather” caused by solar flares might disrupt radio communications, or even damage satellites. But Earth’s atmosphere protects us from truly harmful effects, and we orbit the Sun at a respectable distance, out of reach of the flares themselves.
      Not so for planet HIP 67522 b. A gas giant in a young star system – just 17 million years old – the planet takes only seven days to complete one orbit around its star. A “year,” in other words, lasts barely as long as a week on Earth. That places the planet perilously close to the star. Worse, the star is of a type known to flare – especially in their youth.
      In this case, the proximity of the planet appears to result in fairly frequent flaring.
      Details
      The star and the planet form a powerful but likely a destructive bond. In a manner not yet fully understood, the planet hooks into the star’s magnetic field, triggering flares on the star’s surface; the flares whiplash energy back to the planet. Combined with other high-energy radiation from the star, the flare-induced heating appears to have increased the already steep inflation of the planet’s atmosphere, giving HIP 67522 b a diameter comparable to our own planet Jupiter despite having just 5% of Jupiter’s mass.
      This might well mean that the planet won’t stay in the Jupiter size-range for long. One effect of being continually pummeled with intense radiation could be a loss of atmosphere over time. In another 100 million years, that could shrink the planet to the status of a “hot Neptune,” or, with a more radical loss of atmosphere, even a “sub-Neptune,” a planet type smaller than Neptune that is common in our galaxy but lacking in our solar system.
      Fun Facts
      Four hundred light-years is much too far away to capture images of stellar flares striking orbiting planets. So how did a science team led by Netherlands astronomer Ekaterina Ilin discover this was happening? They used space-borne telescopes, NASA’s TESS (Transiting Exoplanet Survey Satellite) and the European Space Agency’s CHEOPS (CHaracterising ExoPlanets Telescope), to track flares on the star, and also to trace the path of the planet’s orbit.
      Both telescopes use the “transit” method to determine the diameter of a planet and the time it takes to orbit its star. The transit is a kind of mini-eclipse. As the planet crosses the star’s face, it causes a tiny dip in starlight reaching the telescope. But the same observation method also picks up sudden stabs of brightness from the star – the stellar flares. Combining these observations over five years’ time and applying rigorous statistical analysis, the science team revealed that the planet is zapped with six times more flares than it would be without that magnetic connection.   
      The Discoverers
      A team of scientists from the Netherlands, Germany, Sweden, and Switzerland, led by Ekaterina Ilin of the Netherlands Institute for Radio Astronomy, published their paper on the planet-star connection, “Close-in planet induces flares on its host star,” in the journal Nature on July 2, 2025.
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      Explore This Section Exoplanets Home Exoplanets Overview Exoplanets Facts Types of Exoplanets Stars What is the Universe Search for Life The Big Questions Are We Alone? Can We Find Life? The Habitable Zone Why We Search Target Star Catalog Discoveries Discoveries Dashboard How We Find and Characterize Missions People Exoplanet Catalog Immersive The Exoplaneteers Exoplanet Travel Bureau 5 Ways to Find a Planet Strange New Worlds Universe of Monsters Galaxy of Horrors News Stories Blog Resources Get Involved Glossary Eyes on Exoplanets Exoplanet Watch More Multimedia ExEP View the full article
    • NASA
      3 Years of Science: 10 Cosmic Surprises from NASA’s Webb Telescope
      By NASA
      Explore Webb Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Webb’s First Images Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning Since July 2022, NASA’s James Webb Space Telescope has been unwaveringly focused on our universe. With its unprecedented power to detect and analyze otherwise invisible infrared light, Webb is making observations that were once impossible, changing our view of the cosmos from the most distant galaxies to our own solar system.
      Webb was built with the promise of revolutionizing astronomy, of rewriting the textbooks. And by any measure, it has more than lived up to the hype — exceeding expectations to a degree that scientists had not dared imagine. Since science operations began, Webb has completed more than 860 scientific programs, with one-quarter of its time dedicated to imaging and three-quarters to spectroscopy. In just three years, it has collected nearly 550 terabytes of data, yielding more than 1,600 research papers, with intriguing results too numerous to list and a host of new questions to answer.
      Here are just a few noteworthy examples.
      1. The universe evolved significantly faster than we previously thought.
      Webb was specifically designed to observe “cosmic dawn,” a time during the first billion years of the universe when the first stars and galaxies were forming. What we expected to see were a few faint galaxies, hints of what would become the galaxies we see nearby.
      Instead, Webb has revealed surprisingly bright galaxies that developed within 300 million years of the big bang; galaxies with black holes that seem far too massive for their age; and an infant Milky Way-type galaxy that existed when the universe was just 600 million years old. Webb has observed galaxies that already “turned off” and stopped forming stars within a billion years of the big bang, as well as those that developed quickly into modern-looking “grand design” spirals within 1.5 billion years.
      Hundreds of millions of years might not seem quick for a growth spurt, but keep in mind that the universe formed in the big bang roughly 13.8 billion years ago. If you were to cram all of cosmic time into one year, the most distant of these galaxies would have matured within the first couple of weeks, rapidly forming multiple generations of stars and enriching the universe with the elements we see today.
      Image: JADES deep field
      A near-infrared image from NASA’s James Webb Space Telescope shows a region known as the JADES Deep Field. Tens of thousands of galaxies are visible in this tiny patch of sky, including Little Red Dots and hundreds of galaxies that existed more than 13.2 billion years ago, when the universe was less than 600 million years old. Webb also spotted roughly 80 ancient supernovae, many of which exploded when the universe was less than 2 billion years old. This is ten times more supernovae than had ever been discovered before in the early universe. Comparing these supernovae from the distant past with those in the more recent, nearby universe helps us understand how stars in these early times formed, lived, and died, seeding space with the elements for new generations of stars and their planets. NASA, ESA, CSA, STScI, JADES Collaboration 2. Deep space is scattered with enigmatic “Little Red Dots.”
      Webb has revealed a new type of galaxy: a distant population of mysteriously compact, bright, red galaxies dubbed Little Red Dots. What makes Little Red Dots so bright and so red? Are they lit up by dense groupings of unusually bright stars or by gas spiraling into a supermassive black hole, or both? And whatever happened to them? Little Red Dots seem to have appeared in the universe around 600 million years after the big bang (13.2 billion years ago), and rapidly declined in number less than a billion years later. Did they evolve into something else? If so, how? Webb is probing Little Red Dots in more detail to answer these questions.
      3. Pulsating stars and a triply lensed supernova are further evidence that the “Hubble Tension” is real.
      How fast is the universe expanding? It’s hard to say because different ways of calculating the current expansion rate yield different results — a dilemma known as the Hubble Tension. Are these differences just a result of measurement errors, or is there something weird going on in the universe? So far, Webb data indicates that the Hubble Tension is not caused by measurement errors. Webb was able to distinguish pulsating stars from nearby stars in a crowded field, ensuring that the measurements weren’t contaminated by extra light. Webb also discovered a distant, gravitationally lensed supernova whose image appears in three different locations and at three different times during its explosion. Calculating the expansion rate based on the brightness of the supernova at these three different times provides an independent check on measurements made using other techniques. Until the matter of the Hubble Tension is settled, Webb will continue measuring different objects and exploring new methods.
      4. Webb has found surprisingly rich and varied atmospheres on gas giants orbiting distant stars.
      While NASA’s Hubble Space Telescope made the first detection of gases in the atmosphere of a gas giant exoplanet (a planet outside our solar system), Webb has taken studies to an entirely new level. Webb has revealed a rich cocktail of chemicals, including hydrogen sulfide, ammonia, carbon dioxide, methane, and sulfur dioxide — none of which had been clearly detected in an atmosphere outside our solar system before. Webb has also been able to examine exotic climates of gas giants as never before, detecting flakes of silica “snow” in the skies of the puffy, searing-hot gas giant WASP-17 b, for example, and measuring differences in temperature and cloud cover between the permanent morning and evening skies of WASP-39 b.
      Image: Spectrum of WASP-107 b
      A transmission spectrum of the “warm Neptune” exoplanet WASP-107 b captured by NASA’s Hubble and Webb space telescopes, shows clear evidence for water, carbon dioxide, carbon monoxide, methane, sulfur dioxide, and ammonia in the planet’s atmosphere. These measurements allowed researchers to estimate the interior temperature and mass of the core of the planet, as well as understand the chemistry and dynamics of the atmosphere. NASA, ESA, CSA, Ralf Crawford (STScI) 5. A rocky planet 40 light-years from Earth may have an atmosphere fed by gas bubbling up from its lava-covered surface.
      Detecting, let alone analyzing, a thin layer of gas surrounding a small rocky planet is no easy feat, but Webb’s extraordinary ability to measure extremely subtle changes in the brightness of infrared light makes it possible. So far, Webb has been able to rule out significant atmosphere on a number of rocky planets, and has found tantalizing signs of carbon monoxide or carbon dioxide on 55 Cancri e, a lava world that orbits a Sun-like star. With findings like these, Webb is laying the groundwork for NASA’s future Habitable Worlds Observatory, which will be the first mission purpose-built to directly image and search for life on Earth-like planets around Sun-like stars.
      6. Webb exposes the skeletal structure of nearby spiral galaxies in mesmerizing detail.
      We already knew that galaxies are collections of stars, planets, dust, gas, dark matter, and black holes: cosmic cities where stars form, live, die, and are recycled into the next generation. But we had never been able to see the structure of a galaxy and the interactions between stars and their environment in such detail. Webb’s infrared vision reveals filaments of dust that trace the spiral arms, old star clusters that make up galactic cores, newly forming stars still encased in dense cocoons of glowing dust and gas, and clusters of hot young stars carving enormous cavities in the dust. It also elucidates how stellar winds and explosions actively reshape their galactic homes.
      Image: PHANGS Phantom Galaxy (M74/NGC 628)
      A near- to mid-infrared image from NASA’s James Webb Space Telescope highlights details in the complex structure of a nearby galaxy that are invisible to other telescopes. The image of NGC 628, also known as the Phantom Galaxy, shows spiral arms with lanes of warm dust (represented in red), knots of glowing gas (orange-yellow), and giant bubbles (black) carved by hot, young stars. The dust-free core of the galaxy is filled with older, cooler stars (blue). NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS team 7. It can be hard to tell the difference between a brown dwarf and a rogue planet.
      Brown dwarfs form like stars, but are not dense or hot enough to fuse hydrogen in their cores like stars do. Rogue planets form like other planets, but have been ejected from their system and no longer orbit a star. Webb has spotted hundreds of brown-dwarf-like objects in the Milky Way, and has even detected some candidates in a neighboring galaxy. But some of these objects are so small — just a few times the mass of Jupiter — that it is hard to figure out how they formed. Are they free-floating gas giant planets instead? What is the least amount of material needed to form a brown dwarf or a star? We’re not sure yet, but thanks to three years of Webb observations, we now know there is a continuum of objects from planets to brown dwarfs to stars.
      8. Some planets might be able to survive the death of their star.
      When a star like our Sun dies, it swells up to form a red giant large enough to engulf nearby planets. It then sheds its outer layers, leaving behind a super-hot core known as a white dwarf. Is there a safe distance that planets can survive this process? Webb might have found some planets orbiting white dwarfs. If these candidates are confirmed, it would mean that it is possible for planets to survive the death of their star, remaining in orbit around the slowly cooling stellar ember.
      9. Saturn’s water supply is fed by a giant fountain of vapor spewing from Enceladus.
      Among the icy “ocean worlds” of our solar system, Saturn’s moon Enceladus might be the most intriguing. NASA’s Cassini mission first detected water plumes coming out of its southern pole. But only Webb could reveal the plume’s true scale as a vast cloud spanning more than 6,000 miles, about 20 times wider than Enceladus itself. This water spreads out into a donut-shaped torus encircling Saturn beyond the rings that are visible in backyard telescopes. While a fraction of the water stays in that ring, the majority of it spreads throughout the Saturnian system, even raining down onto the planet itself. Webb’s unique observations of rings, auroras, clouds, winds, ices, gases, and other materials and phenomena in the solar system are helping us better understand what our cosmic neighborhood is made of and how it has changed over time.
      Video: Water plume and torus from Enceladus
      A combination of images and spectra captured by NASA’s James Webb Space Telescope show a giant plume of water jetting out from the south pole of Saturn’s moon Enceladus, creating a donut-shaped ring of water around the planet.
      Credit: NASA, ESA, CSA, G. Villanueva (NASA’s Goddard Space Flight Center), A. Pagan (STScI), L. Hustak (STScI) 10. Webb can size up asteroids that may be headed for Earth.
      In 2024 astronomers discovered an asteroid that, based on preliminary calculations, had a chance of hitting Earth. Such potentially hazardous asteroids become an immediate focus of attention, and Webb was uniquely able to measure the object, which turned out to be the size of a 15-story building. While this particular asteroid is no longer considered a threat to Earth, the study demonstrated Webb’s ability to assess the hazard.
      Webb also provided support for NASA’s Double Asteroid Redirection Test (DART) mission, which deliberately smashed into the Didymos binary asteroid system, showing that a planned impact could deflect an asteroid on a collision course with Earth. Both Webb and Hubble observed the impact, serving witness to the resulting spray of material that was ejected. Webb’s spectroscopic observations of the system confirmed that the composition of the asteroids is probably typical of those that could threaten Earth.
      —-
      In just three years of operations, Webb has brought the distant universe into focus, revealing unexpectedly bright and numerous galaxies. It has unveiled new stars in their dusty cocoons, remains of exploded stars, and skeletons of entire galaxies. It has studied weather on gas giants, and hunted for atmospheres on rocky planets. And it has provided new insights into the residents of our own solar system.
      But this is only the beginning. Engineers estimate that Webb has enough fuel to continue observing for at least 20 more years, giving us the opportunity to answer additional questions, pursue new mysteries, and put together more pieces of the cosmic puzzle.
      For example: What were the very first stars like? Did stars form differently in the early universe? Do we even know how galaxies form? How do stars, dust, and supermassive black holes affect each other? What can merging galaxy clusters tell us about the nature of dark matter? How do collisions, bursts of stellar radiation, and migration of icy pebbles affect planet-forming disks? Can atmospheres survive on rocky worlds orbiting active red dwarf stars? Is Uranus’s moon Ariel an ocean world?
      As with any scientific endeavor, every answer raises more questions, and Webb has shown that its investigative power is unmatched. Demand for observing time on Webb is at an all-time high, greater than any other telescope in history, on the ground or in space. What new findings await?
      By Dr. Macarena Garcia Marin and Margaret W. Carruthers, Space Telescope Science Institute, Baltimore, Maryland
      Media Contacts
      Laura Betz – laura.e.betz@nasa.gov
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Christine Pulliam – cpulliam@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
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      Last Updated Jul 02, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
      James Webb Space Telescope (JWST) Astrophysics Black Holes Brown Dwarfs Exoplanet Science Exoplanets Galaxies Galaxies, Stars, & Black Holes Goddard Space Flight Center Nebulae Science & Research Star-forming Nebulae Stars Studying Exoplanets The Universe View the full article
    • NASA
      NASA Stennis Engineer Takes Pride in Test Support Work
      By NASA
      Dwayne Lavigne works as a controls engineer at NASA’s Stennis Space Center, where he supports NASA’s Artemis mission by programming specialized computers for engine testing.NASA/Danny Nowlin As a controls engineer at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, Dwayne Lavigne does not just fix problems – he helps put pieces together at America’s largest rocket propulsion test site.
      “There are a lot of interesting problems to solve, and they are never the same,” Lavigne said. “Sometimes, it is like solving a very cool puzzle and can be pretty satisfying.”
      Lavigne programs specialized computers called programmable logic controllers. They are extremely fast and reliable for automating precisely timed operations during rocket engine tests as NASA Stennis supports the agency’s Artemis missions to explore the Moon and build the foundation for the first crewed mission to Mars.
      However, the system will not act unless certain parameters are met in the proper sequence. It can be a complex relationship. Sometimes, 20 or 30 things must be in the correct configuration to perform an operation, such as making a valve open or close, or turning a motor on or off.
      The Picayune, Mississippi, native is responsible for establishing new signal paths between test hardware and the specialized computers.
      He also develops the human machine interface for the controls. The interface is a screen graphic that test engineers use to interact with hardware.
      Lavigne has worked with NASA for more than a decade. One of his proudest work moments came when he contributed to development of an automated test sequencing routine used during all RS-25 engine tests on the Fred Haise Test Stand.
      “We’ve had many successful tests over the years, and each one is a point of pride,” he said.
      When Lavigne works on the test stand, he works with the test hardware and interacts with technicians and engineers who perform different tasks than he does. It provides an appreciation for the group effort it takes to support NASA’s mission.
      “The group of people I work with are driven to get the job done and get it done right,” he said.
      In total, Lavigne has been part of the NASA Stennis federal city for 26 years. He initially worked as a contractor with the Naval Oceanographic Office as a data entry operator and with the Naval Research Laboratory as a software developer.
      September marks 55 years since NASA Stennis became a federal city. NASA, and more than 50 companies, organizations, and agencies located onsite share in operating costs, which allows tenants to direct more of their funding to individual missions. 
      “Stennis has a talented workforce accomplishing many different tasks,” said Lavigne. “The three agencies I’ve worked with at NASA Stennis are all very focused on doing the job correctly and professionally. In all three agencies, people realize that lives could be at risk if mistakes are made or shortcuts are taken.”
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