Jump to content

55 Years Ago: Five Months Until the Moon Landing


Recommended Posts

  • Publishers
Posted

Following the success of the Apollo 8 circumlunar mission, NASA believed that it could achieve a Moon landing by the summer of 1969 and meet President John F. Kennedy’s goal. Much work remained to accomplish that objective. Three crews and their backups trained for the next three Apollo missions while workers at NASA’s Kennedy Space Center (KSC) in Florida prepared the spacecraft and rockets for those flights. With Apollo 9 in the home stretch to test the Lunar Module (LM) in Earth orbit in early March, preparations also continued for Apollo 10 in May, a lunar orbit test of the LM that served as a dress rehearsal for the Moon landing, and for Apollo 11, the landing mission itself planned for July.

Apollo 8

Apollo 8 astronaut Frank Borman and his wife Susan, at left, meet the Royal family at Buckingham Palace during the London stop of their European tour Borman, left, meets with French President Charles de Gaulle and U.S. Ambassador to France R. Sargent Shriver during the Paris stop of the tour In Den Haag, The Netherlands, Apollo 8 astronaut Borman, right, describes the Lunar Module to Queen Juliana
Left: Apollo 8 astronaut Frank Borman and his wife Susan, at left, meet the Royal family at Buckingham Palace during the London stop of their European tour. Middle: Borman, left, meets with French President Charles de Gaulle and U.S. Ambassador to France R. Sargent Shriver during the Paris stop of the tour. Right: In Brussels, Borman, left, presents a model of the Saturn V rocket to Jean Rey, president of the European Commission.

In Den Haag, The Netherlands, Apollo 8 astronaut Borman, right, describes the Lunar Module to Queen Juliana At The Vatican, Borman, left, presents a photograph of the Moon from Apollo 8 to Pope Paul VI The Bormans, Frank, left, Susan, and sons Edwin and Frederick, hold a press conference in Lisbon, the last stop of their European tour
Left: In Den Haag, The Netherlands, Apollo 8 astronaut Borman, right, describes the Lunar Module to Queen Juliana. Middle: At The Vatican, Borman, left, presents a photograph of the Moon from Apollo 8 to Pope Paul VI. Right: The Bormans, Frank, left, Susan, and sons Edwin and Frederick, hold a press conference in Lisbon, the last stop of their European tour.

As President Richard M. Nixon announced on Jan. 30, Apollo 8 astronaut Frank Borman, his wife Susan, and their two children Frederick and Edwin, set off on their European goodwill tour on Feb. 2, flying aboard a presidential Air Force jet. Borman’s Apollo 8 crewmates James A. Lovell and William A. Anders could not participate in the tour because they had already begun training as part of the Apollo 11 backup crew. The Bormans’ 19-day tour took them to London, Paris, Brussels, Den Haag, Bonn, West Berlin, Rome, Madrid, and Lisbon. They met with royalty, politicians, scientists, and Pope Paul VI, gave lectures during which Borman narrated a film from his flight, and held numerous press conferences.

Apollo 9

Apollo 9 astronauts Russell L. Schweickart, left, James A. McDivitt, and David R. Scott pose in front of the control panel for the spacecraft simulators Fisheye lens view of Schweickart, left, and McDivitt in the Lunar Module simulator A technician poses in the Apollo A7L spacesuit, including the Portable Life Support System backpack used for the first time during Apollo 9
Left: Apollo 9 astronauts Russell L. Schweickart, left, James A. McDivitt, and David R. Scott pose in front of the control panel for the spacecraft simulators. Middle: Fisheye lens view of Schweickart, left, and McDivitt in the Lunar Module simulator. Right: A technician poses in the Apollo A7L spacesuit, including the Portable Life Support System backpack used for the first time during Apollo 9.

Apollo 9 astronauts James A. McDivitt, David R. Scott, and Russell L. Schweickart planned to conduct the first crewed test of the LM during their 10-day Earth orbital mission. They and their backups Charles “Pete” Conrad, Richard F. Gordon, and Alan L. Bean spent many hours in the spacecraft simulators and training for the spacewalk component of the mission. The planned spacewalk, the first and only one before the Moon landing mission, would not only test the spacesuit and its Portable Life Support System but also demonstrate an external crew transfer should a problem arise with the internal transfer tunnel or hatches. McDivitt, Scott, and Schweickart provided details of their mission to reporters during a press conference on Feb. 8 at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. They explained that during the mission phase when the two vehicles fly separately, they will use the call signs Spider for the LM and Gumdrop for the Command Module (CM), lighthearted references to the shapes of the respective spacecraft.

Apollo 9 astronauts Russell L. Schweickart, left, James A. McDivitt, and David R. Scott during the preflight crew press conference at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston Senior NASA management assembled for the Apollo 9 Flight Readiness Review at NASA’s Kennedy Space Center (KSC): Associate Administrator for Manned Flight George E. Mueller, left, Apollo Program Director Samuel C. Phillips, KSC Director Kurt H. Debus, MSC Director Robert R. Gilruth, and Marshall Space Flight Center Director Wernher von Braun
Left: Apollo 9 astronauts Russell L. Schweickart, left, James A. McDivitt, and David R. Scott during the preflight crew press conference at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. Right: Senior NASA management assembled for the Apollo 9 Flight Readiness Review at NASA’s Kennedy Space Center (KSC): Associate Administrator for Manned Flight George E. Mueller, left, Apollo Program Director Samuel C. Phillips, KSC Director Kurt H. Debus, MSC Director Robert R. Gilruth, and Marshall Space Flight Center Director Wernher von Braun.

Senior NASA managers met at NASA’s Kennedy Space Center (KSC) in Florida for Apollo 9’s Flight Readiness Review the first week of February. At the end of the meeting, they set the launch date for Feb. 28. The following week, engineers in Firing Room 2 of KSC’s Launch Control Center conducted the Countdown Demonstration Test (CDDT), essentially a dress rehearsal for the actual countdown. On Feb. 12, McDivitt, Scott, and Schweickart participated in the final portion of the CDDT, as they would on launch day, by donning their spacesuits and climbing aboard their spacecraft for the final two hours of the test. Engineers began the countdown to launch on Feb. 26 but had to halt it the next day when the astronauts developed head colds. Managers reset the launch date to March 3, and the countdown restarted on March 1.

The Apollo 9 Saturn V at Launch Pad 39A at NASA’s Kennedy Space Center in Florida during the Countdown Demonstration Test (CDDT) Engineers in the Launch Control Center’s Firing Room 2 monitor the rocket and spacecraft during the CDDT Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt pose in front of their Saturn V following the CDDT
Left: The Apollo 9 Saturn V at Launch Pad 39A at NASA’s Kennedy Space Center in Florida during the Countdown Demonstration Test (CDDT). Middle: Engineers in the Launch Control Center’s Firing Room 2 monitor the rocket and spacecraft during the CDDT. Right: Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt pose in front of their Saturn V following the CDDT.

Apollo 10

The three stages of the Saturn V stacked on Mobile Launcher-3 The Apollo 10 spacecraft, the Command and Service Modules and the Lunar Module (LM) encased in the Spacecraft LM Adapter, arrives from the Manned Spacecraft Operations Building Workers lift the spacecraft for stacking onto the rocket, the footpads of the LM’s folded landing gear visible Workers lower the spacecraft onto the Saturn V rocket’s third stage
Stacking of the Apollo 10 vehicle in High Bay 2 of the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. Left: The three stages of the Saturn V stacked on Mobile Launcher-3. Middle left: The Apollo 10 spacecraft, the Command and Service Modules and the Lunar Module (LM) encased in the Spacecraft LM Adapter, arrives from the Manned Spacecraft Operations Building. Middle right: Workers lift the spacecraft for stacking onto the rocket, the footpads of the LM’s folded landing gear visible. Right: Workers lower the spacecraft onto the Saturn V rocket’s third stage.

With Apollo 9 on Launch Pad 39A and almost ready to launch, workers in High Bay 2 of KSC’s Vehicle Assembly Building (VAB) completed stacking of the Apollo 10 launch vehicle. The spacecraft, consisting of the Command and Service Modules atop the LM encased in the Spacecraft LM Adapter, arrived from the Manned Spacecraft Operations Building (MSOB) on Feb. 6 and VAB workers stacked it on the Saturn V rocket the same day. Engineers began to conduct integrated tests on the launch vehicle in preparation for rollout to Launch Pad 39B in mid-March. Apollo 10 astronauts Thomas P. Stafford, John W. Young, and Eugene A. Cernan and their backups L. Gordon Cooper, Donn F. Eisele, and Edgar D. Mitchell spent much time in spacecraft simulators and testing their spacesuits in vacuum chambers.

Apollo 11

Apollo 11 astronaut Edwin E. “Buzz” Aldrin, left, confers with support astronauts Ronald E. Evans and Harrison H. “Jack” Schmitt, the only geologist in the astronaut corps at the time, during training for deployment of the Early Apollo Science Experiment Package (EASEP) Astronaut Don L. Lind, suited, practices deploying the EASEP instruments as Aldrin, in white shirt behind the dish antenna, oberves
Left: Apollo 11 astronaut Edwin E. “Buzz” Aldrin, left, confers with support astronauts Ronald E. Evans and Harrison H. “Jack” Schmitt, the only geologist in the astronaut corps at the time, during training for deployment of the Early Apollo Science Experiment Package (EASEP). Right: Astronaut Don L. Lind, suited, practices deploying the EASEP instruments as Aldrin, in white shirt behind the dish antenna, oberves.

With their historic mission only five months away, the Apollo 11 prime crew of Neil A. Armstrong, Michael Collins, and Edwin E. “Buzz” Aldrin and their backups James A. Lovell, William A. Anders, and Fred W. Haise busied themselves training for the Moon landing. Although the primary goal of the first Moon landing mission centered on demonstrating that the Apollo spacecraft systems could safely land two astronauts on the surface and return them safely to Earth, the surface operations also included collecting lunar samples and deploying experiments. During their two-and-a-half-hour surface excursion, Armstrong and Aldrin planned to deploy three instruments comprising the Early Apollo Surface Experiment Package (EASEP) – a passive seismometer, a laser ranging retro-reflector, and a solar wind composition experiment. On Jan. 21, 1969, astronauts Harrison H. “Jack” Schmitt, the only geologist in the astronaut corps, and Don L. Lind conducted a simulation of the EASEP deployment in MSC’s Building 9. Aldrin observed the simulation, obviously with great interest.

Apollo 11 astronauts Edwin E. “Buzz” Aldrin, left, and Neil A. Armstrong during geology training at Sierra Blanco, Texas Apollo 11 backup astronauts Fred W. Haise, left, and James A. Lovell at the Sierra Blanco geology training session
Left: Apollo 11 astronauts Edwin E. “Buzz” Aldrin, left, and Neil A. Armstrong during geology training at Sierra Blanco, Texas. Right: Apollo 11 backup astronauts Fred W. Haise, left, and James A. Lovell at the Sierra Blanco geology training session.

Generic instruction in geology, including classroom work and field trips, became part of overall NASA astronaut training beginning in 1964. Once assigned to a crew that had a very good chance of actually walking on the lunar surface and collecting rock and soil samples, those astronauts received specialized instruction in geology. On Feb. 24, 1969, the two prime moonwalkers Armstrong and Aldrin, along with their backups Lovell and Haise, participated in their only trip specifically dedicated to geology training. The field exercise in west Texas took place near Sierra Blanca and the ruins of Fort Quitman, about 90 miles southeast of El Paso. Accompanied by a team from MSC’s Geology Branch, the astronauts practiced sampling the variety of rocks present at the site to obtain a representative collection, skills needed to choose the best sample candidates during their brief excursion on the lunar surface. 

Workers mount the S-IC first stage on its Mobile Launcher in the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida Neil A. Armstrong stands in front of the Lunar Module simulator at the Lunar Landing Research Facility (LLRF) at NASA’s Langley Research Center in Hampton, Virginia Aerial view of the LLRF at Langley
Left: Workers mount the S-IC first stage on its Mobile Launcher in the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. Middle: Neil A. Armstrong stands in front of the Lunar Module simulator at the Lunar Landing Research Facility (LLRF) at NASA’s Langley Research Center in Hampton, Virginia. Right: Aerial view of the LLRF at Langley.

By mid-February, all three stages of the Apollo 11 Saturn V had arrived in the VAB, and on Feb. 21, workers stacked the S-IC first stage on its Mobile Launcher in High Bay 1. They finished assembling the rocket in March. In an altitude chamber in the nearby MSOB, on Feb. 10, engineers conducted a docking test between the CM and the LM. Five days later, they mated the ascent and descent stages of the LM for further testing. With the Lunar Landing Training Vehicle (LLTV) still grounded following its December 1968 crash, the Lunar Landing Research Facility (LLRF) at NASA’s Langley Research Center in Hampton, Virginia, remained as the only high-fidelity trainer for the descent and landing of the LM on the Moon. Armstrong practiced landings in the LLRF on Feb 12.

Lunar Receiving Laboratory and Mobile Quarantine Facility

To minimize the risk of back contamination of the Earth with any possible lunar microorganisms, NASA designed and built the 83,000-square-foot Lunar Receiving Laboratory (LRL), residing in MSC’s Building 37. The facility isolated the astronauts, their spacecraft, and lunar samples to prevent any Moon germs from escaping into the environment, and also maintained the lunar samples in as pristine a condition as possible. The Mobile Quarantine Facility (MQF) provided isolation for the returning astronauts from shortly after splashdown until their delivery to the LRL, an activity that required transport of the MQF on a cargo jet aircraft. On Feb. 6, following its return from sea trials, workers placed the MQF inside Chamber A of MSC’s Space Environment Simulation Facility. The test in the large vacuum chamber checked out the MQF’s emergency oxygen supply during a simulated aircraft pressure loss. Three test subjects successfully completed the test.

Workers truck the Mobile Quarantine Facility (MQF) into the Space Environment Simulation Laboratory (SESL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston Workers install the MQF in Chamber A of the SESL for a test of the emergency oxygen system Test subjects inside the MQF prepare for the emergency oxygen system test in the SESL
Left: Workers truck the Mobile Quarantine Facility (MQF) into the Space Environment Simulation Laboratory (SESL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston. Middle: Workers install the MQF in Chamber A of the SESL for a test of the emergency oxygen system. Right: Test subjects inside the MQF prepare for the emergency oxygen system test in the SESL.

To be continued …

News from around the world in February 1969:

Feb. 3 – Ibuprofen launched in the United Kingdom as a prescription anti-inflammatory analgesic.

Feb. 5 – The population of the United States reaches 200 million.

Feb. 7 – British band The Who record their song “Pinball Wizard.”

Feb. 7 – Diane Krump becomes the first woman jockey at a major U.S. racetrack (Hialeah, Florida).

Feb. 8 – The Allende meteorite weighing nearly two tons explodes in mid-air and fragments fall on Pueblito de Allende, Chihuahua, Mexico.

Feb. 9 – First flight of the Boeing 747 Jumbo Jet from Everett, Washington.

Feb. 21 – First launch of U.S.S.R.’s N-1 Moon rocket, not successful.

Feb. 24 – U.S. launches Mariner 6 to fly-by Mars.

Share

Details

Last Updated
Feb 20, 2024

Related Terms

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • 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.
      Related Information
      More Webb News
      More Webb Images
      Webb Science Themes
      Webb Mission Page
      Related For Kids
      What is the Webb Telescope?
      SpacePlace for Kids
      En Español
      Ciencia de la NASA
      NASA en español 
      Space Place para niños
      Keep Exploring Related Topics
      James Webb Space Telescope


      Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…


      Galaxies



      Exoplanets



      Universe


      Share








      Details
      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
    • By Amazing Space
      Backyard Astronomy: LIVE Streaming the Moon 1st July
    • By Amazing Space
      Backyard Astronomy: LIVE Streaming the Moon 1st July
    • By European Space Agency
      Asteroid 2024 YR4 made headlines earlier this year when its probability of impacting Earth in 2032 rose as high as 3%. While an Earth impact has now been ruled out, the asteroid’s story continues.
      The final glimpse of the asteroid as it faded out of view of humankind’s most powerful telescopes left it with a 4% chance of colliding with the Moon on 22 December 2032.
      The likelihood of a lunar impact will now remain stable until the asteroid returns to view in mid-2028. In this FAQ, find out why we are left with this lingering uncertainty and how ESA's planned NEOMIR space telescope will help us avoid similar situations in the future.
      View the full article
    • By NASA
      NASA/Bob Hines NASA astronaut Bob Hines took this picture of the waning crescent moon on May 8, 2022, as the International Space Station flew into an orbital sunrise 260 miles above the Atlantic Ocean off the northwest coast of the United States. Since the station became operational in November 2000, crew members have produced hundreds of thousands of images of our Moon and Earth through Crew Earth Observations.
      Image credit: NASA/Bob Hines
      View the full article
  • Check out these Videos

×
×
  • Create New...