NASA Composite Manufacturing Initiative Gains Two New Members

NASA Composite Manufacturing Initiative Gains Two New Members

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Automated fiber placement machine on an industrial robot
An automated fiber placement machine on an industrial robot is seen at Fives Machining Systems Inc. Fives is one of the new partners joining a NASA project that explores ways to speed up the production of composite aircraft.
Fives Machining Systems Inc.

Gulfstream Aerospace Corporation and Fives Machining Systems Inc. have joined 20 other organizations to support NASA’s Hi-Rate Composite Aircraft Manufacturing (HiCAM) project.

The project is addressing industry’s needs to meet growing demand for air travel, replace aging airliners, and secure U.S. competitiveness in the commercial aircraft industry.  

NASA and its partners are collaborating and sharing costs to increase the manufacturing rate for aircraft components made from composite (nonmetallic) materials. Gulfstream and Fives are the newest members in a public-private partnership called the Advanced Composites Consortium

Advanced Composites Consortium

Members of the Consortium have significant and unique expertise in aircraft design, manufacturing, certification, testing, and tool development, with the new members bringing important new insights and capabilities to the team.   

“By partnering with U.S. industry, academia, and regulators, we’ll increase the likelihood of impacting the next generation of transports,” said Richard Young, manager for NASA’s HiCAM project, which oversees the consortium.

The team is currently competing concepts to determine which technologies will have the greatest impact on manufacturing rates. Once the most promising concepts are selected, they’ll be demonstrated at full scale.

The project and Advanced Composites Consortium contribute to NASA’s Sustainable Flight National Partnership by enabling broader use of lightweight composite airframes, which will reduce fuel consumption and carbon emissions, improving air quality and the environment.

 HiCAM is managed under NASA’s Advanced Air Vehicles Program.

Powered by WPeMatico

Get The Details…
Jim Banke

Beyond the Textbook: DC-8 Aircraft Inspires Students in Retirement

Beyond the Textbook: DC-8 Aircraft Inspires Students in Retirement

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A group of 22 students pose on a stairway descending from an aircraft door. The plane and stairway are white, on a sunny tarmac.
Idaho State University class of 2025 poses with their new hands-on learning tool, the DC-8 aircraft, after it was retired from NASA in May 2024 and arrived in Pocatello, Idaho. The university will use the aircraft to provide a hands-on learning experience for students in the university’s aircraft maintenance technology program.
Idaho State University

In May 2024, Idaho State University’s class of 2025 received a new learning tool from NASA. The DC-8 aircraft served the world’s scientific community for decades as a platform under NASA’s Airborne Science Program before retiring to Idaho State University (ISU) to provide a hands-on learning experience for students in the university’s aircraft maintenance technology program. 

“The DC-8 has quickly become a cornerstone of our Aircraft Maintenance Technology program at ISU,” said Jake Dixon, Director of Marketing and Recruitment at the ISU College of Technology. “It has already enhanced our summer classes ahead of its full integration with the start of the new school year this fall.” 

The DC-8 flew its final flight from NASA’s Armstrong Flight Research Center in Edwards, California to Idaho State University in Pocatello, Idaho in May 2024. That flight represented the retirement of the aircraft after 37 years of supporting airborne science missions as a NASA aircraft. 

“The opportunity for students to interact firsthand with the aircraft’s systems and features significantly extends their learning beyond what theory or textbooks can provide,” Dixon said.

A large white plane and smaller chase plane fly over the top of a building with a NASA logo on the front. A sunny blue sky is behind the building and planes.
The DC-8 flies low for the last time over NASA’s Armstrong Flight Research Center in Edwards, California, before it retires to Idaho State University in Pocatello, Idaho. The DC-8 is providing real-world experience to train future aircraft technicians at the college’s Aircraft Maintenance Technology Program.
NASA/Genaro Vavuris

The DC-8 served as an educational platform for years. Beginning in 2009, the DC-8 functioned as an airborne science laboratory for NASA’s Student Airborne Research Program (SARP), where rising-senior undergraduates were selected to participate in a real science campaign and acquire hands-on research experience. The educational impact of the DC-8 is evident in the professional growth of scientists who have experienced it. 

“Almost everything I’ve learned about using an airplane to collect scientific data can be linked back to my time flying projects on the DC-8.” says Jonathan Zawislak, Flight Director with the Aircraft Operations Center at the National Oceanic and Atmospheric Administration (NOAA). “It has left an indelible mark on the Earth science community and no doubt paved the way for a new generation of scientists, as it did for me and my career as a science aviator.”

NASA Armstrong’s Student Airborne Research Program celebrated 15 years of success in 2023. An eight-week summer internship program, SARP offered upper-level undergraduate students the opportunity to acquire hands-on research experience as part of a scientific campaign using NASA Airborne Science Program flying science laboratories – aircraft outfitted specifically for research projects.
NASA/Carla Thomas

Real-life platforms like the DC-8 are an exciting and meaningful learning tool that enable college students to go beyond the textbook, and they make a lasting impact on communities adjacent to its activities. 

“We have seen so much enthusiasm surrounding the DC-8’s arrival that we are organizing an open house in the future to allow the community and aviation enthusiasts alike to explore this historic aircraft,” said Dixon. “Doing so will help preserve the remarkable legacy of the DC-8, ensuring it continues to inspire and educate for years to come.” 

Whether as a science platform or as a unique aircraft, the DC-8 has a legacy that continues to inspire and educate generations of scientists, engineers, and aviators. 

Learn more about NASA’s SARP program 

Learn more about the retired DC-8 aircraft Learn more about NASA’s Armstrong Flight Research Center

Share

Details

Last Updated

Aug 22, 2024

Powered by WPeMatico

Get The Details…
Dede Dinius

NASA’s EXCITE Mission Prepared for Scientific Balloon Flight

NASA’s EXCITE Mission Prepared for Scientific Balloon Flight

5 min read

NASA’s EXCITE Mission Prepared for Scientific Balloon Flight

Scientists and engineers are ready to fly an infrared mission called EXCITE (EXoplanet Climate Infrared TElescope) to the edge of space. 

EXCITE is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during circumpolar long-duration scientific balloon flights. But first, it must complete a test flight during NASA’s fall 2024 scientific ballooning campaign from Fort Sumner, New Mexico. 

“EXCITE can give us a three-dimensional picture of a planet’s atmosphere and temperature by collecting data the whole time the world orbits its star,” said Peter Nagler, the mission’s principal investigator at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Only a handful of these types of measurements have been done before. They require a very stable telescope in a position to track a planet for several days at a time.”

Photo of a telescope in a hanger.
EXCITE (EXoplanet Climate Infrared TElescope) hangs from a ceiling at the Columbia Scientific Balloon Facility’s location in Fort Sumner, New Mexico. The mission team practiced taking observations ahead of flight by looking out the hanger doors at night.
NASA/Jeanette Kazmierczak

EXCITE will study hot Jupiters, giant gas exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees. The worlds are tidally locked, which means the same side always faces the star.

The telescope will observe how heat is distributed across the planet, from the scalding hemisphere facing the star to the relatively cooler nightside. 

It will also determine how molecules in a world’s atmosphere absorb and emit light over the entire orbit, a process called phase-resolved spectroscopy. Not only can this data reveal the presence of compounds — like water, methane, carbon dioxide, and others — but also how they circulate globally as the planet orbits its star.

NASA’s HubbleJames Webb, and retired Spitzer space telescopes have collected a handful of these measurements between them. 

In 2014, for example, Hubble and Spitzer observed an exoplanet called WASP-43 b. To collect data over the world’s 22-hour day, scientists needed 60 hours of Hubble time and 46 hours from Spitzer. Resource-intensive studies like this on space-based observatories are difficult. Time is a limited resource, and studies must compete with hundreds of other requests for that time.  

“During its first science flight, EXCITE aims to fly for over a dozen days from the Columbia Scientific Balloon Facility’s site in Antarctica,” said Kyle Helson, an EXCITE team member and a research scientist at the University of Maryland, Baltimore County and NASA Goddard. “And at the pole, the stars we’ll study don’t set, so our observations won’t be interrupted. We hope that the mission will effectively double the number of phase-resolved spectra available to the science community.”

EXCITE will fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, the telescope will be able to observe multiple infrared wavelengths with little interference. 

“The telescope collects the infrared light and beams it into the spectrometer, where it kind of goes through a little obstacle course,” said Lee Bernard, an EXCITE team member and a graduate research assistant at Arizona State University in Tempe. “It bounces off mirrors and through a prism before reaching the detector. Everything must be aligned very precisely — just a few millimeters off center and the light won’t make it.”

The spectrometer rests inside a vessel called a cryostat situated behind the telescope. The cryostat cools the spectrometer’s detector — once a flight candidate from Webb’sNIRSpec (Near InfraRed Spectrograph)— to about 350 degrees below zero Fahrenheit (minus 210 degrees Celsius) so it can measure tiny intensity changes in the infrared light. 

Photo of EXCITE’s infrared detector on a lab bench.
The EXCITE infrared detector, shown here, was once a flight candidate from NASA’s James Webb Space Telescope’s NIRSpec (Near InfraRed Spectrograph) instrument. Before being added to the mission’s spectrometer assembly, it was mounted to a copper base and topped with a protective black case. The detector allows EXCITE to collect spectroscopic measurements from 1 to 4 microns — the near-infrared portion of the electromagnetic spectrum.
NASA/Sophia Roberts

The entire telescope and cryostat assembly rests in a rowboat-shaped base where it can rotate along three axes to maintain stable pointing down to 50 milliarcseconds. That’s like holding a steady gaze on a U.S. quarter coin from 65 miles away. 

“Several different institutions contributed to EXCITE’s subsystems,” said Tim Rehm, an EXCITE team member and a graduate research assistant at Brown University in Providence, Rhode Island. “It’s great to see them all assembled and working together. We’re excited to do this test flight, and we’re looking forward to all the future science flights we hope to have.”

The EXCITE instrument was primarily built by NASA Goddard, Brown, Arizona State University, and StarSpec Technologies in Ontario, with additional support from collaborators in the U.S., Canada, Italy, and the United Kingdom.

NASA’s scientific balloons offer frequent, low-cost access to near-space to conduct scientific investigations and technology maturation in fields such as astrophysics, heliophysics, and atmospheric research, as well as training for the next generation of leaders in engineering and science. To follow the missions in the 2024 Fort Sumner fall campaign, visit NASA’s CSBF (Columbia Scientific Balloon Facility) website for real-time updates of a balloon’s altitude and GPS location during flight. 

NASA’s Wallops Flight Facility in Virginia manages the agency’s scientific balloon flight program with 10 to 15 flights each year from launch sites worldwide. Peraton, which operates CSBF in Texas, provides mission planning, engineering services, and field operations for NASA’s scientific balloon program. The CSBF team has launched more than 1,700 scientific balloons over some 40 years of operations. NASA’s balloons are fabricated by Aerostar. The NASA Scientific Balloon Program is funded by the NASA Headquarters Science Mission Directorate Astrophysics Division.

By Jeanette Kazmierczak
NASA’s Goddard Space Flight Center, Greenbelt, Md. 

Media Contact:
Claire Andreoli
301-286-1940
claire.andreoli@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Share

Details

Last Updated
Aug 22, 2024
Editor
Jeanette Kazmierczak

Powered by WPeMatico

Get The Details…

NASA Selects Three New Venture-Class Launch Service Providers

NASA Selects Three New Venture-Class Launch Service Providers

Image of the NASA logo
Credit: NASA

NASA has selected three additional companies to provide launch services for future agency missions through its VADR (Venture-Class Acquisition of Dedicated and Rideshare) contract.

The companies awarded are:

  • Arrow Science and Technology LLC of Webster, Texas
  • Impulse Space Inc. of Redondo Beach, California
  • Momentus Space LLC of San Jose, California

The VADR contract is a firm-fixed-price, indefinite-delivery/indefinite-quantity instrument with an ordering period through Feb. 3, 2027 and a maximum total value of $300 million across all VADR contracts. NASA selected the new launch providers in accordance with VADR’s on-ramp provision, allowing the agency to add new capabilities not available or identified at the time of the initial award. NASA will issue firm-fixed-price task orders for launch services as needed for future agency and agency-sponsored missions.

The VADR contract builds on NASA’s previous procurement efforts, such as the VCLS (Venture Class Launch Services) and VCLS Demo 2, providing a broad range of Federal Aviation Administration-licensed commercial launch services capable of delivering Class D, CubeSats, and higher risk-tolerant payloads to a variety of orbits. By using a lower level of mission assurance and commercial best practices for launching rockets, these highly flexible contracts help broaden access to space through lower launch costs and serve as an ideal platform for contributing to NASA’s science research and technology development.

NASA’s Launch Services Program, based at the agency’s Kennedy Space Center in Florida, manages the VADR contracts. The program also works with private industry, spacecraft projects, and international partners to launch science payloads ranging from small satellites with colleges and universities to NASA’s highest priority missions.

For more information about NASA’s launch services, visit:

https://go.nasa.gov/46SorXk

-end-

Josh Finch / Julian Coltre
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / julian.n.coltre@nasa.gov

Patti Bielling / Amanda Griffin
Kennedy Space Center, Florida
321-501-7575 / 321-593-6244
patricia.a.bielling@nasa.gov / amanda.griffin@nasa.gov

Powered by WPeMatico

Get The Details…
Tiernan P. Doyle

Into The Field With NASA: Valley Of Ten Thousand Smokes

Into The Field With NASA: Valley Of Ten Thousand Smokes

4 Min Read

Into The Field With NASA: Valley Of Ten Thousand Smokes

Three people, wearing large backpacks, trek across a snow field between hills of dark rubble. In the background: steep, snow-covered mountains under a blue sky.
NASA scientists begin a day’s field research in Katmai National Park.
Credits:
NASA/Patrick Whelley

In June 2024, the Goddard Instrument Field Team (GIFT) hiked deep into the backcountry of Alaska’s Katmai National Park to study the Valley of Ten Thousand Smokes, site of the largest volcanic eruption of the twentieth century. The team’s task: traverse a vast volcanic debris field layered with glacier ice, gathering data and samples to help us better understand this place on Earth and similar terrain on other worlds.

Composite of two images. Top: Aerial image of a grayscale landscape. In the middle, a dominant dark streak has some areas highlighted in purple. A scale bar shows that this feature is a few hundred meters long. Bottom: Ground-level view of an ice cliff face on an ashy, barren landscape. The ice is partially covered in beige dirt. In the foreground is a black, rounded device on a tripod. The ground is rocky with patches of snow.
Buried glaciers on Mars and Earth. Top: Orbital view of partially-exposed ice beneath an eroding deposit on Mars, from HiRISE. Bottom: Edge-on view of a partially buried glacier in Alaska with a LiDAR (Light Detection and Ranging) device in the foreground, from the Goddard Instrument Field Team.

Novarupta, the volcano that erupted here in 1912, ejected more than three cubic miles of ash from Earth’s subsurface. The ice nearby is now insulated by, and mixed with, thick layers of geologically “young” volcanic debris. (For comparison, many of the eruption sites NASA teams study are tens of thousands to millions of years old.) Mars, too, has glaciers and ice sheets covered in layers of airfall materials, including dust and volcanic ash.

On Mars, as on Earth, some of the planet’s history is in disguise. Ancient volcanic materials are buried underneath newer deposits of ashy debris. Patterns in these layers (think thickness or thinness, color and texture, chemical and mineral signatures) hold a lot of information, but the message isn’t always clear. Erosion and other surface processes hide evidence of past eruptions, even enormous ones. Since relatively fresh volcanic material blankets the Valley of Ten Thousand Smokes, it’s an ideal place to observe the early stages of these changes.

Three people on a barren, rocky landscape with hills of grey ash and snow-covered mountains in the background. The researcher on the left kneels and raises a rock hammer, about to collect a sample. Nearby, another scientist props a portable spectrometer up on her shoulder in between uses-- the spectrometer resembles a large, orange and grey blow dryer. The third scientist holds a bag of rock samples and looks at the camera. She has a large pack on her back and hiking poles under her arm.
Cherie Achilles raises a rock hammer as Alexandra Matiella Novak stands by with a hand-held spectrometer and Alice Baldridge holds a container of rock samples. The hand-held spectrometer gives on-the-spot information about what its targets are made of, helping the team decide which samples to collect and bring back to the lab.

In three days of violent eruption, Novarupta blasted an uncommonly wide variety of clays, minerals, and volcanic rocks throughout the surrounding valley. Since then, hot, sulfurous gases have filtered up through underground channels and escaped into the air via countless fumaroles (a.k.a. the “ten thousand smokes”). Fumaroles, together with erosion and other alteration processes, affect how minerals near Novarupta move and change. Research here can help us understand mineral movement and alteration on Mars and other worlds, too. The range of starting materials and alteration patterns in this valley, all from a single eruption, is difficult to match anywhere else.

Person kneeling on reddish-brown, rocky ground, near a small hole, with a steep, snow-patched mountain in the background. They are wearing purple nitrile gloves and holding a tiny, open vial in one hand while digging with the other. A golden wire stretches across the dirt and into the hole in the ground.
Heather Graham studies a fumarole – a place where volcanic gases escape from underground – using a hydrogen sulfide collector and sampling equipment. Their goal: check the fumarole for encrusted evidence that microscopic organisms once lived here, consuming energy and changing the rocks’ composition. Research on these kinds of biosignatures helps us understand what the search for life could look like on other worlds.

It’s a tough field site to access, especially with heavy science instruments. GIFT worked closely with local collaborators including Katmai National Park to coordinate the expedition. After years of planning and months of training, twelve field team members gathered and geared up in Anchorage, Alaska. Two tiny airplane flights, one all-terrain bus ride, and sixteen hiking miles later, they set up a base camp. From there, small groups hiked out and back each day, gathering data and sample material from throughout the valley.

Seven people, with large backpacks, hiking down a hill of lumpy snow dusted with beige volcanic ash. Behind them is a steep wall of dirt with streaks of fresh green shrubbery. The people appear tiny against the landscape and are all in the left half of the image. On the right are overlapping views of three distinct geological formations: a light-colored slope in the foreground, a tan and orange river gorge in the middle ground, and snow-capped mountains in the background, under a partly cloudy sky.
Left to right: Tabb Prissel, Emileigh Shoemaker, Heather Graham, Andrew Johnson, Justin Hayles, Aditi Pandey, and Patrick Whelley hike out of the Valley of Ten Thousand Smokes.

Scientists teamed up to carry large equipment from place to place and bring each other data from far-flung targets. Some results were predictable, like a new library of samples collected from several different “packages” of differently-composed volcanic debris. Some were surprising–like a core sample that came up containing a pocket of empty space instead of buried glacial ice.

Person holding a bulky computer readout attached via a thick cord to a red plastic box with a push handle, on an expanse of beige volcanic ash, with snowy mountain peaks in the background. A tape measure, anchored to the ground with a trekking pole near the red box, extends over a hill into the distance.
Emileigh Shoemaker and her team use Ground Penetrating Radar (the red box shown here is the GPR antenna) to gather information about long stretches of Earth’s subsurface before physically breaking ground. Here, Shoemaker stands on a huge pile of volcanic ash; hidden beneath the debris is a glacier. GPR data, combined with core samples, soil moisture measurements, and pits dug at strategic locations, can reveal how the glacier is preserved.

Analyzing the samples, processing the data, and putting it all together will take time. This is the beginning of GIFT’s Novarupta research, but it’s a chapter of a science story long in the making. Previous studies of the 1912 eruption and its aftermath influenced this expedition’s science plan. The 2024 data and samples, and the new questions arising from the team’s time in the field, are already shaping ideas about future work. NASA has visited before, too. Apollo astronauts and their geology trainers spent time in the Valley in 1965, finding it an unusually Moon-like place to study.

Fieldwork still plays a role in astronaut training–and in advancing lunar science. For example: Novarupta’s chemistry is partly a result of Earth’s plate tectonics. The Moon has volcanic landscapes with similar chemistry, but no tectonic plates. So, what else could explain the parallel? To help address this question, the 2024 team collected samples and ground-truth data from a range of rock formations comparable to the Moon’s Gruithuisen Domes.

Three people, dressed for outdoor work, on a rocky hill in front of a mountainous landscape under an overcast sky. In the middle distance is a huge, dark-colored pile of rubble, shaped like a low dome.
Tabb Prissel, Aditi Pandey, and Justin Hayles at Novarupta. The dome of dark rubble behind the scientists is what’s left of the volcano itself: in 1912, material erupted from this spot buried miles of glaciated valley.

On Earth, the Moon, Mars, and beyond, geologic processes encode pieces of our solar system’s history. Volcanic deposits store details about a world’s insides at the time of an eruption and evidence of what’s happened at the surface since. Rippling fields of sand dunes, gravel, and ash record the influence of wind where atmospheres exist, like on Venus, Mars, and Titan. Glaciers can tell us about climate history and future–and on Mars, ice research also helps to lay the groundwork for human exploration. It’s much easier to take a close look at these features and processes here on Earth than anywhere else. So, to understand planets (including our own), NASA field scientists start close to home. 

About the Author

Caela Barry

Caela Barry

Keep Exploring

Discover More Topics From NASA

Powered by WPeMatico

Get The Details…