Boeing’s Starliner spacecraft is pictured docked to the International Space Station. This long-duration photograph was taken at night from the orbital complex as it soared 258 miles above western China.
Credit: NASA
NASA will host a media teleconference at 1 p.m. EDT, Wednesday, Aug. 14, to provide an update on the agency’s Boeing Crew Flight Test. Mission managers continue to evaluate the Starliner spacecraft’s readiness in advance of decisional meetings no earlier than next week regarding the return of NASA astronauts Butch Wilmore and Suni Williams.
Audio of the teleconference will stream live on the agency’s website at:
To ask questions during the teleconference, media must RSVP no later than two hours prior to the start of the call to Jimi Russell at: james.j.russell@nasa.gov. NASA’s media accreditation policy is available online.
NASA’s Boeing Crew Flight Test launched on June 5 on a ULA (United Launch Alliance) Atlas V rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station in Florida. It is an end-to-end test of the Starliner system as part of the agency’s Commercial Crew Program. Through partnership with American private industry, NASA is opening access to low Earth orbit and the space station to more people, science, and commercial opportunities.
For NASA’s blog and more information about the mission, visit:
NASA Challenge Seeks ‘Cooler’ Solutions for Deep Space Exploration
NASA’s Human Lander Challenge, or HuLC, is now open and accepting submissions for its second year. As NASA aims to return astronauts to the Moon through its Artemis campaign in preparation for future missions to Mars, the agency is seeking ideas from college and university students for evolved supercold, or cryogenic, propellant applications for human landing systems.
As part of the 2025 HuLC competition, teams will aim to develop innovative solutions and technology developments for in-space cryogenic liquid storage and transfer systems as part of future long-duration missions beyond low Earth orbit.
“The HuLC competition represents a unique opportunity for Artemis Generation engineers and scientists to contribute to groundbreaking advancements in space technology,” said Esther Lee, an aerospace engineer leading the navigation sensors technology assessment capability team at NASA’s Langley Research Center in Hampton, Virginia. “NASA’s Human Lander Challenge is more than just a competition – it is a collaborative effort to bridge the gap between academic innovation and practical space technology. By involving students in the early stages of technology development, NASA aims to foster a new generation of aerospace professionals and innovators.”
The Goal
Through Artemis, NASA is working to send the first woman, first person of color, and first international partner astronaut to the Moon to establish long-term lunar exploration and science opportunities. Artemis astronauts will descend to the lunar surface in a commercial Human Landing System. The Human Landing System Program is managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama.
Cryogenic, or super-chilled, propellants like liquid hydrogen and liquid oxygen are integral to NASA’s future exploration and science efforts. The temperatures must stay extremely cold to maintain a liquid state. Current state-of-the-art systems can only keep these substances stable for a matter of hours, which makes long-term storage particularly problematic. For NASA’s HLS mission architecture, extending storage duration from hours to several months will help ensure mission success.
“NASA’s cryogenics work for HLS focuses on several key development areas, many of which we are asking proposing teams to address,” said Juan Valenzuela, a HuLC technical advisor and aerospace engineer specializing in cryogenic fuel management at NASA Marshall. “By focusing research in these key areas, we can explore new avenues to mature advanced cryogenic fluid technologies and discover new approaches to understand and mitigate potential problems.”
The Competition
Interested teams from U.S.-based colleges and universities should submit a non-binding Notice of Intent (NOI) by Oct. 6, 2024, and submit a proposal package by March 3, 2025. Based on proposal package evaluations, up to 12 finalist teams will be selected to receive a $9,250 stipend to further develop and present their concepts to a panel of NASA and industry judges at the 2025 HuLC Forum in Huntsville, Alabama, near NASA Marshall, in June 2025. The top three placing teams will share a prize purse of $18,000.
Teams’ potential solutions should focus on one of the following categories: On-Orbit Cryogenic Propellant Transfer, Microgravity Mass Tracking of Cryogenics, Large Surface Area Radiative Insulation, Advanced Structural Supports for Heat Reduction, Automated Cryo-Couplers for Propellant Transfer, or Low Leakage Cryogenic Components.
This view of the Earth’s crest over the lunar horizon was taken on July 29, 1971, during the Apollo 15 lunar landing mission. Astronauts David Scott, Alfred Worden, and James Irwin launched from NASA’s Kennedy Space Center in Florida aboard a Saturn V launch vehicle.
Designed to explore the Moon over longer periods, greater ranges, and with more instruments for the collection of scientific data than before, Apollo 15 included the introduction of a $40 million lunar roving vehicle (LRV) that reached a top speed of 10 mph (16 kph) across the Moon’s surface.
Upon landing on the Moon at the Hadley-Apennine site, Scott and Irwin conducted four spacewalks, including three excursions using the LRV, for a combined total of 19 hours. Worden remained in orbit aboard the command module Endeavour.
Primary Instrument for Roman Space Telescope Arrives at NASA Goddard
This photo shows the Wide Field Instrument for NASA’s Nancy Grace Roman Space Telescope arriving at the big clean room at NASA’s Goddard Space Flight Center. About the size of a commercial refrigerator, this instrument will help astronomers explore the universe’s evolution and the characteristics of worlds outside our solar system. Unlocking these cosmic mysteries and more will offer a better understanding of the nature of the universe and our place within it.
NASA/Chris Gunn
The primary instrument for NASA’s Nancy Grace Roman Space Telescope is a sophisticated camera that will survey the cosmos from the outskirts of our solar system all the way out to the edge of the observable universe. Called the Wide Field Instrument, it was recently delivered to the agency’s Goddard Space Flight Center in Greenbelt, Maryland.
The camera’s large field of view, sharp resolution, and sensitivity from visible to near-infrared wavelengths will give Roman a deep, panoramic view of the universe. Scanning much larger portions of the sky than astronomers can with NASA’s Hubble or James Webb space telescopes will open new avenues of cosmic exploration. Roman is designed to study dark energy (a mysterious cosmic pressure thought to accelerate the universe’s expansion), dark matter (invisible matter seen only via its gravitational influence), and exoplanets (worlds beyond our solar system).
“This instrument will turn signals from space into a new understanding of how our universe works,” said Julie McEnery, the Roman senior project scientist at Goddard. “To achieve its main goals, the mission will precisely measure hundreds of millions of galaxies. That’s quite a dataset for all kinds of researchers to pull from, so there will be a flood of results on a vast array of science.”
Technicians inspect NASA’s Nancy Grace Roman Space Telescope’s Wide Field Instrument upon delivery to the big clean room at NASA’s Goddard Space Flight Center.
NASA/Chris Gunn
About 1,000 people contributed to the Wide Field Instrument’s development, from the initial design phase to assembling it from around a million individual components. The WFI’s design was a collaborative effort between Goddard and BAE Systems in Boulder, Colorado. Teledyne Imaging Sensors, Hawaii Aerospace Corporation, Applied Aerospace Structures Corporation, Northrop Grumman, Honeybee Robotics, CDA Intercorp, Alluxa, and JenOptik provided critical components. Those parts and many more, made by other vendors, were delivered to Goddard and BAE Systems, where they were assembled and tested prior to the instrument’s delivery to Goddard this month.
“I am so happy to be delivering this amazing instrument,” said Mary Walker, Roman’s Wide Field Instrument manager at Goddard. “All the years of hard work and the team’s dedication have brought us to this exciting moment.”
NASA’s Nancy Grace Roman Space Telescope is a next-generation observatory that will survey the infrared universe from beyond the orbit of the Moon. The spacecraft’s giant camera, the Wide Field Instrument, will be fundamental to this exploration. Data it gathers will enable scientists to discover new and uniquely detailed information about planetary systems around other stars. The instrument will also map how matter is structured and distributed throughout the cosmos, which could ultimately allow scientists to discover the fate of the universe. Watch this video to see a simplified version of how the Wide Field Instrument works. NASA’s Goddard Space Flight Center
Seeing the Bigger Picture
After Roman launches by May 2027, each of the Wide Field Instrument’s 300-million-pixel images will capture a patch of the sky bigger than the apparent size of a full moon. The instrument’s large field of view will enable sweeping celestial surveys, revealing billions of cosmic objects across vast stretches of time and space. Astronomers will conduct research that could take hundreds of years using other telescopes.
And by observing from space, Roman’s camera will be very sensitive to infrared light –– light with longer wavelengths than our eyes can see –– from far across the cosmos. This ancient cosmic light will help scientists address some of the biggest cosmic mysteries, one of which is how the universe evolved to its present state.
From the telescope, light’s path through the instrument begins by passing through one of several optical elements in a large wheel. These elements include filters, which allow specific wavelengths of light to pass through, and a grism and prism, which split light into all of its individual colors. These detailed patterns, called spectra, reveal information about the object that emitted the light.
Then, the light travels on toward the camera’s set of 18 detectors, which each contain 16 million pixels. The large number of detectors and pixels gives Roman its large field of view. The instrument is designed for accurate, stable images and exquisite precision in measuring the exact amount of light in every pixel of every image, giving Roman unprecedented power to study dark energy. The detectors will be held at about minus 300 degrees Fahrenheit (minus 184 degrees Celsius) to increase sensitivity to the infrared universe.
“When the light reaches the detectors, that marks the end of what may have been a 10-billion-year journey through space,” said Art Whipple, an aerospace engineer at Goddard who has contributed to the Wide Field Instrument’s design and construction for more than a decade.
Once Roman begins observing, its rapid data delivery will require new analysis techniques.
“If we had every astronomer on Earth working on Roman data, there still wouldn’t be nearly enough people to go through it all,” McEnery said. “We’re looking at modern techniques like machine learning and artificial intelligence to help sift through Roman’s observations and find where the most exciting things are.”
Now that the Wide Field Instrument is at Goddard, it will be tested to ensure everything is operating as expected. It will be integrated onto the instrument carrier and mated to the telescope this fall, bringing scientists one step closer to making groundbreaking discoveries for decades to come.
One panel on the Wide Field Instrument for NASA’s Nancy Grace Roman Space Telescope contains hundreds of names of team members who helped design and build the instrument.
BAE Systems
To virtually tour an interactive version of the telescope, visit:
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems, Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
NASA’s X-59 Progresses Through Tests on the Path to Flight
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA Life Support Technician Mathew Sechler provides support as the X-59’s ejection seat is installed into the aircraft at Lockheed Martin Skunk Works’ facilities in Palmdale, California. Completion of the seat’s installation marks an integration milestone for the aircraft as it prepares for final ground tests.
Lockheed Martin
The team preparing NASA’s X-59 continues through testing in preparation for the quiet supersonic aircraft to make its first flight. This includes a trio of important structural tests and critical inspections on the path to flight.
The X-59 is an experimental plane that will fly faster than the speed of sound without a loud sonic boom. It will be the first of its kind to fly, with the goal of gathering sound data for NASA’s Quesst mission, which could open the door to commercial supersonic overland flight in the future.
Because of its unique design, the X-59’s engineering team must do all it can to predict every aspect of it before it ever takes off, including how its fuselage, wings, and the control surfaces will behave together in flight. That means testing on the ground to give the team the data it needs to validate the models they’ve developed.
“The testing not only tells us how structurally sound the aircraft is, but also what kind of forces it can take once it is in the air.
WALT SILVA
Senior Research Scientist at NASA Langley Research Center in Hampton, Virginia, who serves as structures lead for the X-59.
The X-59’s structural tests provide the team with valuable feedback. From 2022 to –2024 the engineers collected data on the forces that the aircraft will experience in flight and the potential effects of vibrations on the plane.
“You do these tests, you get the data, and things compare well in some areas and in other areas you want to improve them,” Silva said. “So, you figure that all out and then you work towards making it better.”
Lockheed Martin technicians temporarily remove the canopy from the X-59 in preparation for final installation of the ejection seat into the aircraft.
Lockheed Martin
Earlier this year, the X-59 underwent structural coupling tests that saw its control surfaces, including its ailerons, flaps and rudder, moved by computer. It was the last of three vital structural tests. In 2023, engineers applied “shakers” to parts of the plane to evaluate its response to vibrations, and in early 2022 they conducted a proof test to ensure the aircraft would absorb the forces it will experience during flight. This year the X-59 ejection seat was installed and passed inspection. The ejection seat is an additional safety measure that is critical for pilot safety during all aspects of flight.
With structural tests and ejection seat installation complete, the aircraft will advance toward a new milestone, starting up its engines for a series of test runs on the ground.
Also ahead for the X-59 is testing the airplane’s avionics and extensive wiring for potential electromagnetic interference, imitating flight conditions in a ground test environment, and finally, completing taxi tests to validate ground mobility before first flight.
“First flights are always very intense,” said Natalie Spivey, aerospace engineer at NASA’s Armstrong Flight Research Center in Edwards, California. “There’s lots of anticipation, but we’re ready to get there and see how the aircraft responds in the air. It’ll be very exciting.”
