Our James Webb Space Telescope is the most ambitious and complex space science observatory ever built. It will study every phase in the history of our universe, ranging from the first luminous glows after the Big Bang, to the formation of solar systems capable of supporting life on planets like Earth, to the evolution of our own Solar System.
In order to carry out such a daring mission, many innovative and powerful new technologies were developed specifically to enable Webb to achieve its primary mission.
Here are 5 technologies that were developed to help Webb push the boundaries of space exploration and discovery:
Microshutters are basically tiny windows with shutters that each measure 100 by 200 microns, or about the size of a bundle of only a few human hairs.
The microshutter device will record the spectra of light from distant objects (spectroscopy is simply the science of measuring the intensity of light at different wavelengths. The graphical representations of these measurements are called spectra.)
Other spectroscopic instruments have flown in space before but none have had the capability to enable high-resolution observation of up to 100 objects simultaneously, which means much more scientific investigating can get done in less time.
Read more about how the microshutters work HERE.
Webb’s backplane is the large structure that holds and supports the big hexagonal mirrors of the telescope, you can think of it as the telescope’s “spine”. The backplane has an important job as it must carry not only the 6.5 m (over 21 foot) diameter primary mirror plus other telescope optics, but also the entire module of scientific instruments. It also needs to be essentially motionless while the mirrors move to see far into deep space. All told, the backplane carries more than 2400kg (2.5 tons) of hardware.
This structure is also designed to provide unprecedented thermal stability performance at temperatures colder than -400°F (-240°C). At these temperatures, the backplane was engineered to be steady down to 32 nanometers, which is 1/10,000 the diameter of a human hair!
Read more about the backplane HERE.
One of the Webb Space Telescope’s science goals is to look back through time to when galaxies were first forming. Webb will do this by observing galaxies that are very distant, at over 13 billion light years away from us. To see such far-off and faint objects, Webb needs a large mirror.
Webb’s scientists and engineers determined that a primary mirror 6.5 meters across is what was needed to measure the light from these distant galaxies. Building a mirror this large is challenging, even for use on the ground. Plus, a mirror this large has never been launched into space before!
If the Hubble Space Telescope’s 2.4-meter mirror were scaled to be large enough for Webb, it would be too heavy to launch into orbit. The Webb team had to find new ways to build the mirror so that it would be light enough - only 1/10 of the mass of Hubble’s mirror per unit area - yet very strong.
Read more about how we designed and created Webb’s unique mirrors HERE.
Wavefront sensing and control is a technical term used to describe the subsystem that was required to sense and correct any errors in the telescope’s optics. This is especially necessary because all 18 segments have to work together as a single giant mirror.
The work performed on the telescope optics resulted in a NASA tech spinoff for diagnosing eye conditions and accurate mapping of the eye. This spinoff supports research in cataracts, keratoconus (an eye condition that causes reduced vision), and eye movement – and improvements in the LASIK procedure.
Read more about the tech spinoff HERE.
Webb’s primary science comes from infrared light, which is essentially heat energy. To detect the extremely faint heat signals of astronomical objects that are incredibly far away, the telescope itself has to be very cold and stable. This means we not only have to protect Webb from external sources of light and heat (like the Sun and the Earth), but we also have to make all the telescope elements very cold so they don’t emit their own heat energy that could swamp the sensitive instruments. The temperature also must be kept constant so that materials aren’t shrinking and expanding, which would throw off the precise alignment of the optics.
Each of the five layers of the sunshield is incredibly thin. Despite the thin layers, they will keep the cold side of the telescope at around -400°F (-240°C), while the Sun-facing side will be 185°F (85°C). This means you could actually freeze nitrogen on the cold side (not just liquify it), and almost boil water on the hot side. The sunshield gives the telescope the equivalent protection of a sunscreen with SPF 1 million!
Read more about Webb’s incredible sunshield HERE.
Learn more about the Webb Space Telescope and other complex technologies that have been created for the first time by visiting THIS page.
For the latest updates and news on the Webb Space Telescope, follow the mission on Twitter, Facebook and Instagram.
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One brother is a facts-and-figures guy, the other an adventurer.
They're both deeply fascinated by all things space.
Mikey and Robbie Rouse, 15 and 16, are from Salem, Virginia, and both have Duchenne Muscular Dystrophy, a progressive condition that affects nearly all their voluntary muscles.
On a recent trip to Hampton, Virginia, they visited one of the birthplaces of the American space program — NASA's Langley Research Center.
Mikey, the adventurer, wants to be the first wheelchair astronaut. "And I want to go to Mars," he said during his visit.
Robbie, the facts-and-figures guy, is always thinking of safety first — a quality held sacred by all at NASA.
The brothers' visit to Langley included a tour of the center's hangar, a stop at the Flight Mission Support Center for the ozone-monitoring Stratospheric Aerosol and Gas Experiment III, and presentations on the Hypersonic Inflatable Aerodynamic Decelerator, autonomous technologies, and tests at the Landing and Impact Research Facility.
Deputy Center Director Clayton Turner and Associate Director Cathy Mangum presented Mikey and Robbie with commemorative coins and copies of "A Century at Langley," a pictoral history of the center.
No subject raised during the visit failed to spark the boys' curiosity.
Steve Velotas, associate director for intelligent flight systems, talked with Mikey and Robbie about the ways in which Langley researchers are studying autonmous technologies. Autonomous systems could be used in unmanned aerial vehicles, in-space assembly robots, or even wheelchairs to help those with disabilities navigate more easily.
"I don't trust robots completely," Mikey said.
"We don't either," said Velotas, who then explained that part of the reason Langley scientists are studying autonomous systems is to make sure they work like people want them to.
Evan Horowitz, structures and mechanical systems airworthiness engineer, showed the brothers Langley's historic hangar and talked about some of the past and present missions the facility has supported.
Gemini and Apollo astronauts trained in the hangar's Rendezvous Docking Simulator, and aircraft used for airborne science studies and autonomous flight research are based there.
Mikey and Robbie peppered Horowitz, who often takes tour groups through the hangar, with questions about air pollution and habitable exoplanets.
"This is great," said Horowitz. "Best interaction I've had in months."
The previous day, Mikey and Robbie visited the Virginia Air & Space Center, Langley's official visitors center.
The brothers live with their great-grandmother in Salem and receive daily assistance from a nonprofit called Lutheran Family Services of Virginia. The trip to Hampton was organized by Julie's Abundance Project, a program of Lutheran Family Services of Virginia.
Image Credits: NASA/David C. Bowman
Joe AtkinsonJoe Atkinson NASA Langley Research Center
In many ways, the military and NASA couldn’t be different. Frank Batts has managed to navigate both worlds with precision, grace and just a bit of humor. After serving as a major general in the Army National Guard, he made the transition to working on computers as an engineer at NASA’s Langley Research Center in Hampton, Virginia.
“They’re opposites, but that keeps me balanced,” Batts said. “In the Army, you’re out there blowing things up in the field. Here, you’re trying to build electronic computer components.”
Batts is a senior data-systems engineer with the Advanced Measurement and Data Systems Branch at NASA’s Langley Research Center in Hampton, Virginia. He has been at Langley for 34 years and has seen the tools of the job change.
“Technology has changed tremendously,” said the 63-year-old Batts. “When we started out in the eighties, we were all using proprietary operating systems on real-time computers that were not widely used or understood. Now we’re pretty much using PCs for our work.”
In addition to his NASA career, Batts served his country with distinction in the armed forces – and made history along the way. He retired from the Army National Guard in 2012 as a major general and commander of the 29th Infantry Division in Fort Belvoir, Virginia - the first African-American to hold that post. He also served in the West Virginia and Tennessee national guards.
The adventure begins
Batts’ journey started in 1976, when he was accepted at North Carolina Agricultural and Technical State University in Greensboro and joined the Army Reserve Officer Training Corps (ROTC) there.
While at the university, Batts entered a cooperative program with the Union Carbide Corp., working in a gaseous diffusion plant in the nuclear division. After graduating from North Carolina A&T, Batts worked fulltime as an electrical engineer with Union Carbide, and as an engineering officer in the West Virginia National Guard.
“Initially when you get out of college, you’re competing with engineers from other schools,” Batts said. “I found out pretty soon that regardless of what school you came from, it got down to who can really deliver projects on time and on budget.”
Batts was pursuing a master’s degree in electronics engineering at North Carolina A&T around the time IBM introduced personal computers. He was told PCs were a fad and not worth investing in, but he glimpsed the future and got on board.
“It looked like to me it was the way to go,” he said.
But then in 1979, the Three Mile Island nuclear power plant in Pennsylvania experienced a partial core meltdown, releasing radioactive gas into the atmosphere.
The incident changed his professional trajectory, as the Union Carbide-run K-25 facility in Oak Ridge, Tennessee, where Batts was working, enriched uranium for nuclear power plants.
“Prior to Three Mile Island there were plans to construct nuclear plants all over the country, and K-25’s future was secure,” Batts said. “After Three Mile Island, all of those plans were dropped; we had more enriched uranium than was needed and K-25 was slated for closure.”
That meant he needed another job. While looking to move on, Batts found that NASA Langley was using a computing system similar to the one he used while he was with Union Carbide. He sets his sights on Langley, and has been on center as an electronic engineer since 1984 .
Two worlds in one
Batts’ military and NASA worlds were peacefully cohabitating until the Sept. 11, 2001, terrorist attacks. Batts was soon activated and from May 2004 through April 2005, served with the 54th Field Artillery Brigade Headquarters as the mobile liaison team chief in Kabul, Afghanistan as part of Operation Enduring Freedom.
“With the Army comes the leadership responsibilities. I managed a few thousand troops, and that’s no fun. I make an effort in my career at NASA to stay on the technical side rather than on the administrative side of things,” he said with a laugh.
What is fun for Batts, besides getting in more rounds at the golf course in his spare time, is serving as an example for engineering students though NASA’s outreach programs.
Batts, as the first engineer in his family, said he realizes the importance of recognizing those who blazed the trail for others.
“I have to pay homage to the people who came before me,” he said. “Before I was able to command a battalion, there was some else who commanded one, and did a credible enough job so that I had an opportunity.”
Batts also enjoys the reaction of people when they learn he works for NASA.
“There’s a lot of prestige that goes with working at NASA,” he said. “When people find out you work at NASA, they seem to look at you a bit differently.”
Eric Gillard NASA Langley Research Center
Vibration test at 80% power of the European Structural Test Article conducted at NASA Glenn’s Space Power Facility at Plum Brook Station, Sandusky, Ohio.
Throughout Women’s History Month, we’ve been presenting profiles of the women who are leading the way in deep space exploration.
+ Meet some of them
Our Juno spacecraft made its fifth close flyby over giant Jupiter’s mysterious cloud tops.
+ See the latest from the King of Planets
A routine check of the aluminum wheels on our Curiosity Mars rover has found two small breaks on the rover’s left middle wheel tread–the latest sign of wear and tear as the rover continues its journey, now approaching the 10-mile (16 kilometer) mark. But there’s no sign the robotic geologist won’t keep roving right through its ongoing mission.
+ Get the full report
Our research reveals that volcanic activity at the giant Martian volcano Arsia Mons ceased about 50 million years ago, around the time of Earth’s Cretaceous-Paleogene extinction, when large numbers of plant and animal species (including dinosaurs) went extinct. However, there’s no reason to think the two events were more than a cosmic coincidence.
+ Learn how scientists pieced together the past
Images returned from the European Space Agency’s Rosetta mission indicate that during its most recent trip through the inner solar system, the surface of comet 67P/Churyumov-Gerasimenko was a very active place – full of growing fractures, collapsing cliffs and massive rolling boulders.
+ See the many faces of Comet #67P
The next rovers to explore another planet might bring along a scout. The Pop-Up Flat Folding Explorer Robot (PUFFER) in development at the Jet Propulsion Laboratory was inspired by origami. Its lightweight design is capable of flattening itself, tucking in its wheels and crawling into places rovers can’t fit.
+ Meet PUFFER
According to data from our Dawn mission to Ceres, shadowed craters on the dwarf planet may be linked to the history of how the small world has been tilted over time by the gravity of planets like Jupiter.
+ Find out how understanding “cycles of obliquity” might solve solar system mysteries
We’re developing a long-term technology demonstration project of what could become the high-speed internet of the sky. The Laser Communications Relay Demonstration (LCRD) will help engineers understand the best ways to operate laser communications systems, which could enable much higher data rates for connections between spacecraft and Earth, such as scientific data downlink and astronaut communications.
+ See how it will work
We selected 10 studies to develop mission concepts using CubeSats and other kinds of very small satellites to investigate Venus, Earth’s moon, asteroids, Mars and the outer planets. “These small but mighty satellites have the potential to enable transformational science,” said Jim Green, director of NASA’s Planetary Science Division.
+ Get the small details
It’s possible that one of our closest neighbors had rings at one point – and may have them again someday. At least, that’s the theory put forth by NASA-funded scientists at Purdue University.
+ See more details about the once and future rings of Mars
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Voyager 2 Photograph of Jupiter
A photo of Jupiter. Took by Voyager with VGISS on July 02, 1979 at 06:01:35. Detail page on OPUS database.
From its perch on the International Space Station, SAGE III is measuring stratospheric ozone as well as other gases and aerosols.
An orbiting science instrument whose legacy dates back 34 years continues to beam back data on Earth’s protective ozone layer – this time, from a perch on the hull of the International Space Station.
The Stratospheric Aerosol and Gas Experiment III (SAGE III), a NASA Langley Research Center-led mission, was launched on Feb. 19, 2017 and installed on the International Space Station during a 10-day robotic operation.
Since March 2017, the instrument has been measuring and collecting data on Earth’s sunscreen, stratospheric ozone, as well as other gases and aerosols, which are tiny particles in the atmosphere at all altitudes.
The SAGE III instrument makes these measurements through occultation, which involves looking at the light from the Sun or the Moon as it passes through Earth’s atmosphere at the edge, or limb, of the planet. The initial set of atmospheric data collected from the SAGE III instrument was released publicly in October 2017, and the first lunar data was released in January 2018.
Because the SAGE III instrument makes measurements through remote sensing - collecting data from some distance away - the science validation team cannot be sure if the data they are receiving is accurate without first validating it.
To do that, SAGE III science data must be compared to in-situ measurements, or measurements made by other instruments or systems that come in direct contact with the ozone, aerosol, or gas data being collected. These in-situ measurements are collected by the Network for Detection of Atmospheric Composition Change (NDACC), an international group, part of the National Oceanic and Atmospheric Administration, composed of research sites across the world collecting data on the Earth’s atmosphere.
“These sites have been vetted, validated, and have a long statistical history of making science measurements with their instruments,” said SAGE III Science Manager Marilee Roell.
The NDACC will collect these validated measurements through various methods, with two primary methods being through lidar - light detection and ranging - and sondes. Lidar is a ground-based measurement technique that uses a laser to shoot a beam into the Earth’s atmosphere, causing light to scatter by the atmospheric gases and particles. Being able to detect the distance to these gases and particles, the lidar can gather data on the Earth’s atmospheric composition.
Sondes are lightweight, balloon-borne instruments that are flown thousands of feet into the Earth’s atmosphere. As the instrument ascends, it transmits measurements of particle and gas concentrations by radio to a ground-based receiving station. Sondes are used daily across the globe to capture meteorological data, allowing people to check weather conditions each morning.
The science validation team is using NDACC ozone and aerosol lidar data, as well as ozone and water vapor sonde measurements, to validate science data collected from SAGE III.
“We want to match our vertical science product to an externally validated source. It helps the science community have confidence in our data set,” said Roell.
The team is working towards having an externally validated aerosol sonde to compare to the collected SAGE III data. This effort is in the preliminary stages of validating the aerosol balloon sonde against a suite of aerosol sounders, including lidar.
The team is working to validate science data with NDACC locations in Boulder, Colorado and Lauder, New Zealand, which fall within similar latitude bands in the northern and southern hemispheres. To be precise in validation efforts, the lidar or sonde measurement is taken at the same time and location that SAGE III is passing over and collecting equivalent data.
One of the most recent validation efforts took place in Table Mountain, California, and Haute Provence in France. Both locations include validated lidar systems, with lidar being operated by NASA’s Jet Propulsion Laboratory in Table Mountain, California.
Validation efforts were taken a step further by including a third source of measurements: NASA’s DC-8 aircraft. The aircraft, based out of NASA Armstrong Flight Research Center in Palmdale, California, operates as a flying science laboratory. It helps validate the accuracy of other remote-sensing satellite data, such as SAGE III, and can fly under the satellite’s path to collect the same measurements.
Validating the science data using this method required SAGE III, the NASA DC-8 aircraft, and the lidar system in California or France to be taking measurements at the same time and location. The science validation team worked to have all three systems line up while taking measurements and collected some coinciding science data.
NASA also created a validation website for other NDACC sites to use. The site displays SAGE III overpasses of NDACC sites that are three weeks out or less. These sites can choose to make lidar or sonde measurements at the same time as the instrument overpass, and compare them to SAGE III data collected to see if the two sets coincide. The validation team is pursuing additional NDACC sites to coordinate overpass timeframes when the sites may be taking lidar and sonde measurements.
The SAGE III team will present initial science validation data at the European Geosciences Union conference in Vienna, Austria this April.
SAGE III is the latest in a legacy of Langley instruments that go back to the Stratospheric Aerosol Measurement (SAM), which flew on the 1975 Apollo-Soyuz mission. SAGE II, operational from 1984 to 2005, measured global declines in stratospheric ozone that were later shown to be caused by human-induced increases in atmospheric chlorine. Data from it and other sources led to the development of the Montreal Protocol on Substances that Deplete the Ozone Layer.
After the passage of the protocol, SAGE II data also provided key evidence that the ozone layer was showing signs of recovery.
SAGE III, which launched to the station Feb. 19 from Kennedy Space Center in Florida, will continue to monitor that recovery, but with more of Earth’s atmosphere in its sights. SAGE II monitored only the stratosphere. SAGE III is monitoring both the stratosphere and the mesosphere, which is the layer directly above the stratosphere.
Ozone in the upper atmosphere acts as Earth’s sunscreen, protecting the surface from cancer-causing, crop-damaging ultraviolet rays. Atmospheric aerosols contribute to variability in the climate record.
Allison Leybold NASA Langley Research Center
From enabling astronauts to practice moon landings to aircraft crash testing to drop tests for Orion, NASA's gantry has come full circle.
The gantry, a 240-foot high, 400-foot-long, 265-foot-wide A-frame steel structure located at Langley Research Center in Hampton, Va., was built in 1963 and was used to model lunar gravity. Originally named the Lunar Landing Research Facility (LLRF), the gantry became operational in 1965 and allowed astronauts like Neil Armstrong and Edwin "Buzz" Aldrin to train for Apollo 11's final 150 feet before landing on the moon.
Because the moon's gravity is only 1/6 as strong as Earth's, the gantry had a suspension system that supported 5/6 of the total weight of the Lunar Excursion Module Simulator (LEMS), the device the astronauts used to perform the tests. This supportive suspension system imitated the moon's gravitational environment. Additionally, many of the tests were conducted at night to recreate lighting conditions on the moon.
Neil Armstrong with the LEMS at the Lunar Landing Research Facility. This picture (below) was taken in February 1969 - just five months before Armstrong would become the first person to set foot on the surface of the moon.
Aircraft Crash Test Research
After the Apollo program concluded, a new purpose emerged for the gantry – aircraft crash testing. In 1972, the gantry was converted into the Impact Dynamics Research Facility (IDRF) and was used to investigate the crashworthiness of General Aviation (GA) aircraft and rotorcraft. The facility performed full-scale crash tests of GA aircraft and helicopters, system qualification tests of Army helicopters, vertical drop tests of Boeing 707 and composite fuselage sections and drop tests of the F-111 crew escape capsule.
The gantry was even used to complete a number of component tests in support of the Mars Sample Return Earth Entry Vehicle.
With features including a bridge and a 72-foot vertical drop tower, the gantry was able to support planes that weighed up to 30,000 pounds. Engineers lifted aircraft as high as 200 feet in the air and released them to determine how well the craft endured the crash. Data from the crash tests were used to define a typical acceleration for survivable crashes as well as to establish impact criteria for aircraft seats. The impact criteria are still used today as the Federal Aviation Administration standard for certification.
In 1985, the structure was named a National Historic Landmark based on its considerable contributions to the Apollo program.
Revitalized Space Mission
The gantry provides engineers and astronauts a means to prepare for Orion's return to Earth from such missions. With its new mission, the gantry also received a new name – the Landing and Impact Research (LandIR) Facility.
Although originally capable of supporting only 30,000 pounds, the new bridge can bear up to 64,000 pounds after the summer 2007 renovations. Other renovations include a new elevator, floor repairs and a parallel winch capability that allows an accurate adjustment of the pitch of the test article. The new parallel winch system increases the ability to accurately control impact pitch and pitching rotational rate. The gantry can also perform pendulum swings from as high as 200 feet with resultant velocities of over 70 miles per hour.
The gantry makes researching for the optimal landing alternative for NASA's first attempted, manned dry landing on Earth possible. Orion's return on land rather than water will facilitate reuse of the capsule. A water landing would make reuse difficult due to the corrosiveness of salt water.
The testing process involves lifting the test article by steel cables to a height between 40 and 60 feet and swinging it back to Earth. Although the airbags appear most promising, the gantry has the capability to perform different kinds of tests, including a retro rocket landing system and a scale-model, water landing test using a four-foot-deep circular pool. So far, three types of tests have been conducted in support of the Orion program, each progressing from the previous to more realistic features.
The first test consisted of dropping a boilerplate test article that was half the diameter of what Orion will be. For the second round of testing, engineers added a welded structure to the top, with a shape more comparable to Orion to examine the article's tendency to flip or remain upright.
Hydro-Impact
The on-going tests for Orion continue with impacts on water. This is to ensure astronaut safety during a return to Earth mission. Similar to the Apollo program, Orion will re-enter Earth’s atmosphere at very high speeds and after slowing down, deploy parachutes to further slow the descent into the ocean. At NASA Langley Research Center, engineers use the hydro-impact research to determine the stresses on the vehicle and examine its behavior during a mock splashdown.
It’s incredible what humans can do on and off of our planet. Here is a view from the International Space Station taken by Engineer and NASA Astronaut, Colonel Tim Kopra.
Doha, Bahrain – manmade EarthArt.
February 7, 2016.
Credit: NASA Astronaut Tim Kopra’s Twitter Account
Get a behind-the-scenes look at how test dummies at NASA's Langley Research Center contribute to making the planes we fly on safer and developing space exploration vehicles. Work ranges from next-generation aircraft to water-impact tests that evaluate the splashdown of Orion astronaut crew capsules returning from space.
Credit: NASA/Videographer: Gary Banziger; Writer and Co-Producer: Lily Daniels; Editor and Co-Producer: Kevin Anderson