Jump to content

A Look Through Time with NASA’s Lead Photographer for the James Webb Space Telescope


Recommended Posts

  • Publishers
Posted
2 Min Read

A Look Through Time with NASA’s Lead Photographer for the James Webb Space Telescope

header.jpg?w=1536
This self portrait of Chris Gunn, standing in front of NASA’s James Webb Space Telescope from inside the Goddard Space Flight Center cleanroom, was captured November 10, 2016.
Credits:
NASA/Chris Gunn

Nearly two years ago in the early morning hours of Dec. 25, NASA’s James Webb Space Telescope successfully took flight from the jungle-encircled ELA-3 launch complex at Europe’s Spaceport near Kourou, French Guiana. Following a successful deployment in space, and the precise alignment of the telescope’s mirrors and instruments, Webb began science operations nearly six months after liftoff. As the two-year anniversary of the launch aboard ESA’s (European Space Agency) Ariane 5 rocket approaches, Webb’s lead photographer Chris Gunn has remastered a selection of his favorite images from his career, including one previously unreleased image. 

The opportunity to be the visual spokesperson for a mission of this magnitude was the experience of a lifetime

Chris GUNN

Chris GUNN

NASA/GSFC Lead Photographer for Webb Telescope

 

Since the fall of 2009, Gunn has routinely worked through holidays and weekends, and has spent much of these years on the road, ensuring that the Webb telescope’s progress is visually chronicled and shared with the world. As the various parts and components of Webb began to be assembled and tested throughout the country, Gunn and his camera followed along, capturing the historic development of NASA’s premier space telescope. Though Gunn’s images display the complex nature of the telescope aesthetically, these images also serve as critical engineering bookmarks that the team routinely relied on to document that Webb’s construction was sound before launch.   

Following the launch of Webb, Gunn is now chronicling NASA’s next flagship space telescope, the Nancy Grace Roman Space Telescope.

All images below, credit NASA/Chris Gunn.  

A diverse group of people in white cleanroom suits carefully inspect a single golden faced, hexagonal mirror from the James Webb Space Telescope. Many faces all stare intently, some using flashlights, to examine the mirror surface. Reflected on the surface is the face and intense eye contact from one engineer, and the bright reflection of his flashlight shining directly at the viewer. Behind this engineer, a stainless-steel lens cap used to safely transport the mirror, nearly the size of a human body, rests on scaffolding, still attached by ropes to the crane that lifted it off the mirror moments before. In the background, gray and light blue walls lay behind several other components of Webb scattered around the cleanroom floor. To the right of the frame, a structure made of long overlapping black struts that appear like scaffolding sits on top of a lift table that is meant to safely move the structure up and down.
On Nov. 6, 2012, engineers and technicians inspected one of the first of Webb’s 18 hexagonal mirrors to arrive at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
NASA/Chris Gunn

002-mirror-cover-removal.jpg?w=2048
Inside a clean room at NASA’s Goddard Space Flight Center, on the afternoon of April 25, 2016, the James Webb Space Telescope primary mirrors were uncovered in preparation for installation of its scientific instruments.
NASA/Chris Gunn

Traveling alongside Webb as it grew and evolved, and to be able to add my signature to each photograph captured, was of course an honor, but also an immense challenge. With each image, I wanted to express the awe that I felt seeing Webb integrated right before my eyes, knowing what it was destined to shed new light on the mysteries of the cosmos.

CHRIS GUNN

CHRIS GUNN

NASA/GSFC Lead Photographer for Webb Telescope

002a-wing-folding.jpg?w=1364
NASA’s James Webb Space Telescope is shown with one of its two “wings” folded. Each wing holds three of its primary mirror segments. During this operation in the clean room at NASA Goddard, the telescope was also rotated in preparation for the folding back of the other wing. When Webb launched, both wings were stowed in this position, which enabled the mirror to fit into the launch vehicle. This image was captured July 17, 2016.
NASA/Chris Gunn

003-isim-in-ses.jpg?w=2048
Dressed in a clean room suit, NASA photographer Desiree Stover shines a light on the Space Environment Simulator’s integration frame inside the thermal vacuum chamber at NASA’s Goddard Space Flight Center in Greenbelt, Md. This image was captured Aug. 29, 2013.

004-isim-integration.jpg?w=1526
On May 19, 2016, inside a massive clean room at NASA’s Goddard Space Flight Center, Webb’s Integrated Science Instrument Module was lowered into the Optical Telescope Element.

005-vibe-prep-gsfc.jpg?w=2048
Taken on Nov. 16, 2016, inside NASA Goddard’s largest clean room Webb’s Optical Telescope Element and Integrated Science Instrument Module – together called “OTIS” – are shrouded with a “clean tent” as the team prepared for Webb’s first vibration testing, which took place just outside the clean room.

To capture Webb in its true beauty, I employed the use of specialized lighting rigs, often setting up lights early before the start of work. Johnson Space Center’s Chamber A was an especially tough subject to shoot once Webb was inside. It required remote lights that had to be adjusted perfectly before I boarded a boom lift to make the photograph from seven stories up. It was all worth it, everyone’s hard work – just look at how well our starship is performing

Chris Gunn

Chris Gunn

NASA/GSFC Lead Photographer for Webb Telescope

006-webb-enters-chamber-a-jsc.jpg?w=1638
On June 20, 2017, Webb’s Optical Telescope Element and science instruments were loaded into the historic thermal vacuum testing facility known as “Chamber A” at NASA’s Johnson Space Center in Houston.

007-first-move-to-horiz.jpg?w=2048
On Sept. 16, 2021, Webb was ready to be shipped to the launch site in French Guiana. Before Webb could be lifted into its shipping container, engineers and technicians at Northrop Grumman in Redondo Beach, California, performed this first horizontal tilt of the fully assembled observatory.
008-last-observatory-lift-fg-.jpg?w=2048
This never-before-seen image shows engineers and technicians disassembling ground hardware after completing one of the final lifts of the Webb observatory, before being placed atop ESA’s (European Space Agency) Ariane 5 rocket in French Guiana. This image was taken Nov. 11, 2021.

009-webb-launch.jpg?w=1638
“Liftoff – from a tropical rainforest to the edge of time itself, James Webb begins a voyage back to the birth of the universe.” Arianespace’s Ariane 5 rocket launched with NASA’s James Webb Space Telescope aboard, Dec. 25, 2021, from the ELA-3 Launch Zone of Europe’s Spaceport at the Guiana Space Centre in Kourou, French Guiana.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.

Downloads

Right click the images in this article to open a version in a new tab/window that can be zoomed or saved.

Media Contacts

Thaddeus Cesari Thaddeus.cesari@nasa.gov, Laura Betzlaura.e.betz@nasa.gov, Rob Gutrorob.gutro@nasa.gov
NASA’s  Goddard Space Flight Center, Greenbelt, Md.

Related Information

Webb Observatory

More Webb News

More Webb Images

Webb Mission Page

Share

Details

Last Updated
Dec 22, 2023
Editor
Stephen Sabia

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
      4 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Since launching in 2023, NASA’s Tropospheric Emissions: Monitoring of Pollution mission, or TEMPO, has been measuring the quality of the air we breathe from 22,000 miles above the ground. June 19 marked the successful completion of TEMPO’s 20-month-long initial prime mission, and based on the quality of measurements to date, the mission has been extended through at least September 2026. The TEMPO mission is NASA’s first to use a spectrometer to gather hourly air quality data continuously over North America during daytime hours. It can see details down to just a few square miles, a significant advancement over previous satellites.
      “NASA satellites have a long history of missions lasting well beyond the primary mission timeline. While TEMPO has completed its primary mission, the life for TEMPO is far from over,” said Laura Judd, research physical scientist and TEMPO science team member at NASA’s Langley Research Center in Hampton, Virginia. “It is a big jump going from once-daily images prior to this mission to hourly data. We are continually learning how to use this data to interpret how emissions change over time and how to track anomalous events, such as smoggy days in cities or the transport of wildfire smoke.” 
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      By measuring nitrogen dioxide (NO2) and formaldehyde (HCHO), TEMPO can derive the presence of near-surface ozone. On Aug. 2, 2024 over Houston, TEMPO observed exceptionally high ozone levels in the area. On the left, NO2 builds up in the atmosphere over the city and over the Houston Ship Channel. On the right, formaldehyde levels are seen reaching a peak in the early afternoon. Formaldehyde is largely formed through the oxidation of hydrocarbons, an ingredient of ozone production, such as those that can be emitted by petrochemical facilities found in the Houston Ship Channel. Trent Schindler/NASA's Scientific Visualization Studio When air quality is altered by smog, wildfire smoke, dust, or emissions from vehicle traffic and power plants, TEMPO detects the trace gases that come with those effects. These include nitrogen dioxide, ozone, and formaldehyde in the troposphere, the lowest layer of Earth’s atmosphere.
      “A major breakthrough during the primary mission has been the successful test of data delivery in under three hours with the help of NASA’s Satellite Needs Working Group. This information empowers decision-makers and first responders to issue timely air quality warnings and help the public reduce outdoor exposure during times of higher pollution,” said Hazem Mahmoud, lead data scientist at NASA’s Atmospheric Science Data Center located at Langley Research Center.
      …the substantial demand for TEMPO's data underscores its critical role…
      hazem mahmoud
      NASA Data Scientist
      TEMPO data is archived and distributed freely through the Atmospheric Science Data Center. “The TEMPO mission has set a groundbreaking record as the first mission to surpass two petabytes, or 2 million gigabytes, of data downloads within a single year,” said Mahmoud. “With over 800 unique users, the substantial demand for TEMPO’s data underscores its critical role and the immense value it provides to the scientific community and beyond.” Air quality forecasters, atmospheric scientists, and health researchers make up the bulk of the data users so far.
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      On April 14, strong winds triggered the formation of a huge dust storm in the U.S. central plains and fueled the ignition of grassland fires in Oklahoma. On the left, the NO2 plumes originating from the grassland fires are tracked hour-by-hour by TEMPO. Smoke can be discerned from dust as a source since dust is not a source of NO2. The animation on the right shows the ultraviolet (UV) aerosol index, which indicates particulates in the atmosphere that absorb UV light, such as dust and smoke. Trent Schindler/NASA's Scientific Visualization Studio The TEMPO mission is a collaboration between NASA and the Smithsonian Astrophysical Observatory, whose Center for Astrophysics Harvard & Smithsonian oversees daily operations of the TEMPO instrument and produces data products through its Instrument Operations Center.
      Datasets from TEMPO will be expanded through collaborations with partner agencies like the National Oceanic and Atmospheric Administration (NOAA), which is deriving aerosol products that can distinguish between smoke and dust particles and offer insights into their altitude and concentration.
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      On May 5, TEMPO measured NO2 emissions over the Twin Cities in the center of Minnesota during morning rush hour. The NO2 increases seen mid-day through the early evening hours are illustrated by the red and black shaded areas at the Red River Valley along the North Dakota state line. These levels are driven by emissions from the soils in agriculturally rich areas. Agricultural soil emissions are influenced by environmental factors like temperature and moisture as well as fertilizer application. Small fires and enhancements from mining activities can also be seen popping up across the region through the afternoon.Trent Schindler/NASA's Scientific Visualization Studio “These datasets are being used to inform the public of rush-hour pollution, air quality alerts, and the movement of smoke from forest fires,” said Xiong Liu, TEMPO’s principal investigator at the Center for Astrophysics Harvard & Smithsonian. “The library will soon grow with the important addition of aerosol products. Users will be able to use these expanded TEMPO products for air quality monitoring, improving forecast models, deriving pollutant amounts in emissions and many other science applications.”
      The TEMPO mission detects and highlights movement of smoke originating from fires burning in Manitoba on June 2. Seen in purple hues are observations made by TEMPO in the ultraviolet spectrum compared to Advanced Baseline Imagers (ABIs) on NOAA’s GOES-R series of weather satellites that do not have the needed spectral coverage. The NOAA GOES-R data paired with NASA’s TEMPO data enhance state and local agencies’ ability to provide near-real-time smoke and dust impacts in local air quality forecasts.NOAA/NESDIS/Center for Satellite Applications and Research “The TEMPO data validation has truly been a community effort with over 20 agencies at the federal and international level, as well as a community of over 200 scientists at research and academic institutions,” Judd added. “I look forward to seeing how TEMPO data will help close knowledge gaps about the timing, sources, and evolution of air pollution from this unprecedented space-based view.”
      An agency review will take place in the fall to assess TEMPO’s achievements and extended mission goals and identify lessons learned that can be applied to future missions.
      The TEMPO mission is part of NASA’s Earth Venture Instrument program, which includes small, targeted science investigations designed to complement NASA’s larger research missions. The instrument also forms part of a virtual constellation of air quality monitors for the Northern Hemisphere which includes South Korea’s Geostationary Environment Monitoring Spectrometer and ESA’s (European Space Agency) Sentinel-4 satellite. TEMPO was built by BAE Systems Inc., Space & Mission Systems (formerly Ball Aerospace). It flies onboard the Intelsat 40e satellite built by Maxar Technologies. The TEMPO Instrument Operations Center and the Science Data Processing Center are operated by the Smithsonian Astrophysical Observatory, part of the Center for Astrophysics | Harvard & Smithsonian in Cambridge.


      For more information about the TEMPO instrument and mission, visit:
      https://science.nasa.gov/mission/tempo/

      About the Author
      Charles G. Hatfield
      Science Public Affairs Officer, NASA Langley Research Center
      Share
      Details
      Last Updated Jul 03, 2025 LocationNASA Langley Research Center Related Terms
      Tropospheric Emissions: Monitoring of Pollution (TEMPO) Earth Earth Science Earth Science Division General Langley Research Center Missions Science Mission Directorate Explore More
      2 min read Hubble Observations Give “Missing” Globular Cluster Time to Shine
      A previously unexplored globular cluster glitters with multicolored stars in this NASA Hubble Space Telescope…
      Article 15 minutes ago 5 min read NASA Advances Pressure Sensitive Paint Research Capability
      Article 1 hour ago 5 min read How NASA’s SPHEREx Mission Will Share Its All-Sky Map With the World 
      NASA’s newest astrophysics space telescope launched in March on a mission to create an all-sky…
      Article 1 day ago Keep Exploring Discover More Topics From NASA
      Missions
      Humans in Space
      Climate Change
      Solar System
      View the full article
    • By NASA
      Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Hubble and Artificial Intelligence Explore the Night Sky Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts Multimedia Images Videos Sonifications Podcasts e-Books Online Activities 3D Hubble Models Lithographs Fact Sheets Posters Hubble on the NASA App Glossary News Hubble News Social Media Media Resources More 35th Anniversary Online Activities 2 min read
      Hubble Observations Give “Missing” Globular Cluster Time to Shine
      This NASA Hubble Space Telescope image features a dense and dazzling array of blazing stars that form globular cluster ESO 591-12. NASA, ESA, and D. Massari (INAF — Osservatorio di Astrofisica e Scienza dello Spazio); Processing: Gladys Kober (NASA/Catholic University of America)
      Download this image

      A previously unexplored globular cluster glitters with multicolored stars in this NASA Hubble Space Telescope image. Globular clusters like this one, called ESO 591-12 or Palomar 8, are spherical collections of tens of thousands to millions of stars tightly bound together by gravity. Globular clusters generally form early in the galaxies’ histories in regions rich in gas and dust. Since the stars form from the same cloud of gas as it collapses, they typically hover around the same age. Strewn across this image of ESO 591-12 are a number of red and blue stars. The colors indicate their temperatures; red stars are cooler, while the blue stars are hotter.
      Hubble captured the data used to create this image of ESO 591-12 as part of a study intended to resolve individual stars of the entire globular cluster system of the Milky Way. Hubble revolutionized the study of globular clusters since earthbound telescopes are unable to distinguish individual stars in the compact clusters. The study is part of the Hubble Missing Globular Clusters Survey, which targets 34 confirmed Milky Way globular clusters that Hubble has yet to observe.
      The program aims to provide complete observations of ages and distances for all of the Milky Way’s globular clusters and investigate fundamental properties of still-unexplored clusters in the galactic bulge or halo. The observations will provide key information on the early stages of our galaxy, when globular clusters formed.
      Explore More

      Hubble’s Star Clusters


      Exploring the Birth of Stars

      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
      Claire Andreoli
      NASA’s Goddard Space Flight Center, Greenbelt, MD
      claire.andreoli@nasa.gov
      Share








      Details
      Last Updated Jul 03, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Galaxies, Stars, & Black Holes Globular Clusters Goddard Space Flight Center Star Clusters Stars Keep Exploring Discover More Topics From Hubble
      Hubble Space Telescope


      Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.


      Hubble’s Cosmic Adventure



      Hubble’s Night Sky Challenge



      Hubble’s 35th Anniversary


      View the full article
    • By NASA
      NASA Astronauts Send Fourth of July Wishes From the International Space Station
    • By Space Force
      Space Systems Command laid the groundwork for enhanced weather, research, development and prototyping capabilities with the USSF-178 National Security Space Launch Phase 3 Lane 1 task order.
      View the full article
    • By Amazing Space
      REPLAY 2nd JUly Sun Close up Views/ Backyard Astronomy with Lunt Telescope
  • Check out these Videos

×
×
  • Create New...