NASA
A Midsummer Red Sprite Seen from Space
A Midsummer Red Sprite Seen from Space
NASA astronaut Matthew Dominick photographed red sprites in Earth’s upper atmosphere from the International Space Station on June 3, 2024. The bright red flashes (more easily seen by clicking on the photo to see a larger version) are a less understood phenomena associated with powerful lightning events and appear high above the clouds in the mesosphere. Transient Luminous Events (TLEs), including red sprites, are colorful bursts of energy that appear above storms as a result of lightning activity occurring in and below storms on Earth.
Crew members typically capture TLEs with wide focal lengths during Earth timelapses. Instruments mounted outside station, like Atmosphere-Space Interactions Monitor (ASIM), can capture a range of data for researchers on Earth using cameras, photometers, X-ray and gamma-ray detectors. Learn more about seeing storms from space.
While space station crew hunt for TLEs from space, you can help right here on Earth: send your photographs of sprites and other TLEs to NASA’s citizen science project, Spritacular, to contribute to a crowdsourced database that professional scientists can use for research.
Image Credit: NASA/Matthew Dominick
NASA Deputy Administrator Strengthens Ties in Japan, Republic of Korea
NASA Deputy Administrator Pam Melroy will visit Japan and the Republic of Korea beginning Thursday, July 11, to underscore the critical role of international cooperation in advancing space exploration and technology development.
During her week-long visit to the region, Melroy will engage with ministers and other senior government officials in both countries, including leaders from JAXA (Japan Aerospace Exploration Agency) and KASA (Korea AeroSpace Administration) to strengthen partnerships and highlight civil space cooperation.
In Tokyo, Melroy will participate in the Secure World Foundation’s 6th Summit for Space Sustainability, highlighting NASA’s leadership in responsible and sustainable operations amid rapid technological advancements, many of them championed by the agency.
NASA and JAXA are working to advance sustainable human exploration of the Moon. NASA announced in April that Japan will design, develop, and operate a pressurized rover for exploration of the lunar surface. The activity is part of a shared goal for a Japanese national to be the first non-American to land on the Moon as part of a future Artemis mission, assuming important benchmarks are achieved. In addition, NASA and JAXA are advancing goals in climate research and space science missions to benefit humanity.
Melroy also will speak alongside other space agency leaders at the 45th Scientific Assembly of the Committee on Space Research in Busan, Korea, emphasizing opportunities for international and commercial collaboration in space research.
The visit to Korea coincides with the recent establishment of KASA and builds upon decades of collaboration with NASA in exploration, Earth and space science, and aeronautics.
For more information about NASA’s international partnerships, visit:
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Amber Jacobson
Headquarters, Washington
202-358-1600
amber.c.jacobson@nasa.gov
Sols 4239-4240: ‘Vuggin’ Out’
- Curiosity
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Sols 4239-4240: ‘Vuggin’ Out’ NASA’s Mars rover Curiosity acquired this image of a target named “Glacier Notch” on July 6, 2024, Sol 4236 of the Mars Science Laboratory Mission, at 16:55:06 UTC. Curiosity used its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, capturing the image from 32 centimeters (about 13 inches) away.Earth planning date: Monday, July 8, 2024
And just like we planned, Curiosity successfully drove about 11 meters (about 36 feet) after a 27-sol drill campaign at Mammoth Lakes! Not so fast, though, these rocks are just too interesting to leave behind so quickly. Instead of high-tailing it uphill like we usually do after a drill campaign, we’re staying put for another plan to get as much contact science on these diversely-toned rocks with mysterious origins and vugs (geologic term for the cavities in the rock) galore. It’s been a high priority to get as much color documentation of the clasts in the area, so a plan like this has kept my team busy commanding the Mastcams!
The first sol of this plan includes a long, 90-minute remote science block including about 50 minutes of ChemCam LIBS and RMI, about 32 minutes of Mastcam images, and a six-minute dust devil movie taken by Navcam. ChemCam is using its one-LIBS-per-sol on a conglomeratic block target named “Mount Baxter,” and an RMI of Echo Ridge to the south. Mastcam is taking a 12-image mosaic of Mount Baxter after the LIBS work is done, and a huge 54-image mosaic to the east of Echo Ridge called “Stubblefield Canyon.” After the mast instruments are done, our rover will take about a four-hour long nap and wake up to unstow our arm. Arm activities this plan include two vug-tastic targets named “Lake Dorothy” and “Palisade Glacier,” both imaged by MAHLI and investigated by APXS. Curiosity is back to sleep by about 22:50, which sounds like my perfect sleep schedule.
The second sol of this plan includes a 60-minute remote science block containing about 45 minutes of ChemCam LIBS and RMI, only about six minutes of Mastcam images, and a whopping two hours of dust devil and environmental monitoring by Navcam. With 27 sols at our last location, we noticed significant wind motion between repeated images, and Navcam monitoring helps us keep track of how windy it is. Our rover will take another midday nap and wake up in the evening for a bonus APXS integration on Lake Dorothy, helping raise the signal-to-noise ratio and uncover more secrets (and questions) these Martian rocks have been keeping for millions of years.
Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems
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NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri
ESA/Hubble, NASA, Maximilian Häberle (MPIA)
Most known black holes are either extremely massive, like the supermassive black holes that lie at the cores of large galaxies, or relatively lightweight, with a mass of under 100 times that of the Sun. Intermediate-mass black holes (IMBHs) are scarce, however, and are considered rare “missing links” in black hole evolution.
Now, an international team of astronomers has used more than 500 images from NASA’s Hubble Space Telescope — spanning two decades of observations — to search for evidence of an intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri.
Omega Centauri is about 10 times as massive as other big globular clusters – almost as massive as a small galaxy – and consists of roughly 10 million stars that are gravitationally bound. ESA/Hubble, NASA, Maximilian Häberle (MPIA)Download this image
These stars provide new compelling evidence for the presence of the gravitational pull from an intermediate-mass black hole tugging on them. Only a few other IMBH candidates have been found to date.
Omega Centauri consists of roughly 10 million stars that are gravitationally bound. The cluster is about 10 times as massive as other big globular clusters — almost as massive as a small galaxy.
Among the many questions scientists want to answer: Are there any IMBHs, and if so, how common are they? Does a supermassive black hole grow from an IMBH? How do IMBHs themselves form? Are dense star clusters their favored home?
The astronomers have now created an enormous catalog for the motions of these stars, measuring the velocities for 1.4 million stars gleaned from the Hubble images of the cluster. Most of these observations were intended to calibrate Hubble’s instruments rather than for scientific use, but they turned out to be an ideal database for the team’s research efforts.
This image shows the central region of the Omega Centauri globular cluster, where NASA’s Hubble Space Telescope found strong evidence for an intermediate-mass black hole candidate. ESA/Hubble, NASA, Maximilian Häberle (MPIA)Download this image
“We discovered seven stars that should not be there,” explained Maximilian Häberle of the Max Planck Institute for Astronomy in Germany, who led this investigation. “They are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the center. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our Sun.”
Several studies have suggested the presence of an IMBH in Omega Centauri. However, other studies proposed the mass could be contributed by a central cluster of stellar-mass black holes, and had suggested the lack of fast-moving stars above the necessary escape velocity made an IMBH less likely in comparison.
An international team of astronomers used more than 500 images from NASA’s Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date. This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole. This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster. ESA/Hubble, NASA, Maximilian Häberle (MPIA)Download this image
“This discovery is the most direct evidence so far of an IMBH in Omega Centauri,” added team lead Nadine Neumayer of the Max Planck Institute for Astronomy in Germany, who initiated the study, together with Anil Seth from the University of Utah, Salt Lake City. “This is exciting because there are only very few other black holes known with a similar mass. The black hole in Omega Centauri may be the best example of an IMBH in our cosmic neighborhood.”
If confirmed, at a distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, located 26,000 light-years away.
Omega Centauri is visible from Earth with the naked eye and is one of the favorite celestial objects for stargazers living in the southern hemisphere. Located just above the plane of the Milky Way, the cluster appears almost as large as the full Moon when seen from a dark rural area. It was first listed in Ptolemy’s catalog nearly 2,000 years ago as a single star. Edmond Halley reported it as a nebula in 1677. In the 1830s the English astronomer John Herschel was the first to recognize it as a globular cluster.
The discovery paper led by Häberle et al. is published online today in the journal Nature.
Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. Credit: NASA’s Goddard Space Flight Center, Lead Producer: Paul MorrisDownload this video
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubbleMedia Contacts:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Ray Villard
Space Telescope Science Institute, Baltimore, MD
Bethany Downer
ESA/Hubble.org
Science Contact:
Maximilian Häberle
Max Planck Institute for Astronomy, Heidelberg, Germany
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Monster Black Holes Are Everywhere
Hubble’s Star Clusters
Time Travel: Observing Cosmic History
NASA Administrator, Leaders to Discuss Space-Based Cancer Research
As part of the Biden Cancer Moonshot, NASA will virtually host an event at 2 p.m. EDT Thursday, July 11, to highlight how the agency is working to end cancer for the benefit of humanity by conducting research aboard the International Space Station.
The event will stream on NASA Television and the agency’s website. Learn how to stream NASA TV through a variety of platforms, including social media.
Additional participants include:
- Dr. Michael Roberts, chief scientific officer, International Space Station National Laboratory
- Dr. Catriona Jamieson, director, Sanford Stem Cell Institute at the University of California San Diego
As a member of the Cancer Cabinet, NASA is working with agencies and researchers across the federal government to reduce the nation’s cancer death rate by at least 50% in the next 25 years, one of the ambitious but achievable goals of the Cancer Moonshot.
Learn more about the Biden Cancer Moonshot at:
https://www.whitehouse.gov/cancermoonshot/
-end-
Faith McKie
Headquarters, Washington
202-358-1600
faith.d.mckie@nasa.gov
First Mars Crew Completes Yearlong Simulated Red Planet NASA Mission
The inaugural CHAPEA (Crew Health and Performance Exploration Analog) crew is “back on Earth” after walking out of their simulated Martian habitat at NASA’s Johnson Space Center in Houston on July 6. The first of three simulated missions, CHAPEA Mission 1 was designed to help scientists, engineers, and mission planners better understand how living on another world could affect human health and performance.
Kelly Haston, commander, Ross Brockwell, flight engineer, Nathan Jones, medical officer, and Anca Selariu, science officer, lived and worked in an isolated 1,700-square-foot, 3D-printed habitat to support human health and performance research to prepare for future missions to Mars.
“Congratulations to the crew of CHAPEA Mission 1 on their completion of a year in a Mars-simulated environment,” said NASA Administrator Bill Nelson. “Through the Artemis missions, we will use what we learn on and around the Moon to take the next giant leap: sending the first astronauts to Mars. The CHAPEA missions are critical to developing the knowledge and tools needed for humans to one day live and work on the Red Planet.”
The crew stepped out of the habitat and back into the arms of family and friends after a 378-day simulated Mars surface mission that began June 25, 2023.
This high-fidelity simulation involved the crew carrying out different types of mission objectives, including simulated “marswalks,” robotic operations, habitat maintenance, exercise, and crop growth. The crew also faced intentional environmental stressors in their habitat such as resource limitations, isolation, and confinement. For the next two weeks, the volunteers will complete post-mission data collection activities before returning home.
“We planned the last 378 days with many of the challenges crews could face on Mars and this crew dedicated their lives over that time to achieve these unprecedented operational objectives,” said CHAPEA Principal Investigator Grace Douglas. “I am looking forward to diving into the data we have gathered, preparing for CHAPEA Mission 2 and eventually, a human presence on Mars.”
As NASA works to establish a long-term presence for scientific discovery and exploration on the Moon through the Artemis campaign, analog missions like CHAPEA provide scientific data to validate systems and develop technological solutions for future missions to Mars.
Two additional one-year CHAPEA missions are planned, with the next targeted to begin in 2025. The subsequent missions will be nearly identical, allowing researchers to collect data from more participants to expand the dataset and provide a broader perspective on the impacts of Mars-realistic resource limitations, isolation and confinement on human health and performance.
NASA has several other avenues for gathering isolation research, including the Human Exploration Research Analog, Antarctica, and other analogs, as well as human spaceflight missions to the International Space Station to ensure key research goals can be completed to inform future human missions to the Moon and Mars.
The CHAPEA simulated missions are unique because they test the impacts of extended isolation and confinement with the addition of Mars-realistic time delays of communicating to Earth – up to 44-minutes roundtrip – along with resource limitations relevant to Mars, including a more limited food system that can be supported on the space station and in other analogs.
To view the ceremony of crew exiting their habitat, visit here.
Under NASA’s Artemis campaign, the agency will establish the foundation for long-term scientific exploration at the Moon, land the first woman, first person of color, and its first international partner astronaut on the lunar surface, and prepare for human expeditions to Mars for the benefit of all.
Learn more about CHAPEA at:
30 Years Ago: STS-65, the Second International Microgravity Lab Mission
On July 8, 1994, space shuttle Columbia took to the skies on its 17th trip into space, on the second International Microgravity Laboratory (IML-2) mission. Six space agencies sponsored 82 life and microgravity science experiments. The seven-person crew consisted of Commander Robert D. Cabana, Pilot James D. Halsell, Payload Commander Richard J. Hieb, Mission Specialists Carl E. Walz, Leroy Chiao, and Donald A. Thomas, and Payload Specialist Chiaki Mukai representing the National Space Development Agency (NASDA) of Japan, now the Japan Aerospace Exploration Agency. Jean-Jacques H. Favier of the French space agency CNES served as a backup payload specialist. During their then-record setting 15-day shuttle flight, the international team of astronauts successfully completed the science program. They returned to earth on July 23.
Left: The STS-65 crew patch. Middle: Official photo of the STS-65 crew of Richard J. Hieb, seated left, Robert D. Cabana, and Donald A. Thomas; Leroy Chiao, standing left, James D. Halsell, Chiaki Mukai of Japan, and Carl E. Walz. Right: The payload patch for the International Microgravity Laboratory-2.
In August 1973, NASA and the European Space Research Organization, reorganized as the European Space Agency (ESA) in 1975, agreed to build a reusable laboratory called Spacelab to fly in the space shuttle’s cargo bay. As part of the agreement, ESA built two pressurized modules in addition to other supporting hardware. First flying on STS-9 in 1983, the 18-foot-long pressurized Spacelab module made its 10th flight on STS-65. In September 1992 NASA named Hieb as the IML-2 payload commander and Mukai and Favier as prime and backup payload specialists, respectively, adding Chiao and Thomas as mission specialists in October 1992, finally designating Cabana, Halsell, and Walz as the orbiter crew in August 1993. For Cabana and Hieb, both selected as astronauts in 1985, STS-65 marked their third spaceflight. NASA selected Halsell, Walz, Chiao, and Thomas in 1990, in the class nicknamed The Hairballs. Walz would make his second flight, with the other three making their first. NASDA selected Mukai in 1985 and she holds the distinction as the first Japanese woman in space. Chiao and Mukai as part of the STS-65 crew marked the first time that two Asians flew on the shuttle at the same time, and with Kazakh cosmonaut Talgat A. Musbayev aboard Mir, the first time that three people of Asian origins flew in space at the same time.
Left: The STS-65 crew during preflight training at NASA’s Johnson Space Center in Houston. Right: Technicians at NASA’s Kennedy Space Center in Florida prepare the Spacelab module for the STS-65 mission.
Columbia returned to NASA’s Kennedy Space Center (KSC) in Florida following its previous flight, STS-62, in March 1994. Technicians in KSC’s Orbiter Processing Facility (OPF) serviced the orbiter, removed the previous payload, and installed the Spacelab module in the payload bay. Following a successful leak check of the Spacelab module, rollover of Columbia from the OPF to the Vehicle Assembly Building (VAB) took place on June 8, where workers mated it with an external tank (ET) and two solid rocket boosters (SRBs). Following integrated testing, the stack rolled out to Launch Pad 39A seven days later. The crew participated in the Terminal Countdown Demonstration Test on June 22.
Liftoff of space shuttle Columbia on STS-65 carrying the second International Microgravity Laboratory.
On July 8, 1994, precisely on time, Columbia thundered off KSC’s Launch Pad 39A to begin the STS-65 mission. For the first time in shuttle history, a video camera recorded the liftoff from the orbiter’s flight deck, showing the vibrations during the first two minutes while the SRBs fired, smoothing out once the shuttle main engines took over. Mounted inside Columbia’s payload bay, the Spacelab 18-foot-long module provided a shirt-sleeve environment for the astronauts to conduct the scientific experiments. As during many Spacelab missions, the STS-65 crew carried out science operations 24-hours a day, divided into two teams – the red shift comprised Cabana, Halsell, Hieb, and Mukai, while Chiao, Thomas, and Walz made up the blue shift.
Left: Still image from video recorded on the shuttle’s flight deck during powered ascent. Middle: James D. Halsell, left, and Carl E. Walz moments after Columbia reached orbit. Right: View of the Spacelab module in the shuttle’s payload bay.
Left: Richard J. Hieb opens the hatch from the airlock to the tunnel leading to the Spacelab module. Middle: Hieb and Chiaki Mukai begin activating Spacelab and its experiments. Right: The view from the tunnel showing astronauts at work in the Spacelab module.
After reaching orbit, the crew opened the payload bay doors and deployed the shuttle’s radiators, and removed their bulky launch and entry suits, stowing them for the remainder of the flight. Shortly after, Hieb opened the hatch to the transfer tunnel and translated through it to enter the Spacelab module for the first time. He and Mukai activated the module and turned on the first experiments. For the next 14 days, the astronauts worked round the clock, with Cabana, Halsell, and Walz managing the shuttle’s systems while Hieb, Chiao, Thomas, and Mukai conducted the bulk of the research. The astronauts commemorated the 25th anniversary of the Apollo 11 launch on July 16 and the Moon landing four days later, recalling that their spacecraft and the Command Module shared the name Columbia.
Left: Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, talks to students in Japan using the shuttle’s amateur radio. Middle: Richard J. Hieb, left, and Robert D. Cabana take an air sample from an experiment. Right: Hieb in the Lower Body Negative Pressure device.
Left: Donald A. Thomas, left, Leroy Chiao, Richard J. Hieb, and Chiaki Mukai at work in the Spacelab module. Middle: Chiao, left, and Thomas work on the Biorack instruments. Right: Goldfish swim in the Aquatic Animal Experiment Unit.
Left: Robert D. Cabana uses the shuttle’s amateur radio. Middle: Leroy Chiao looks out at the Earth. Right: Carl E. Walz working on the shuttle’s flight deck.
Left: Carl E. Walz flies through the Spacelab module. Middle: Donald A. Thomas gives two thumbs up for the crew’s performance during the mission. Right: Thomas, left, Walz, and Leroy Chiao pay tribute to Apollo 11 on the 25th anniversary of the Moon landing mission.
Left: The first time two Asians fly on the shuttle at the same time – Chiaki Mukai, left, of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, left, and NASA astronaut Leroy Chiao. Middle: Donald A. Thomas, left, James D. Halsell, Carl E. Walz, and Chiao, all selected in 1990 as part of astronaut class 13, nicknamed The Hairballs. Right: Inflight photograph of the STS-65 crew.
A selection of the STS-65 crew Earth observation photographs. Left: Rio de Janeiro. Middle: Barrier islands in Papua New Guinea. Right: Hurricane Emilia in the central Pacific Ocean.
Left: James D. Halsell uses the laptop-based PILOT to train for the entry and landing. Middle: The astronauts close Columbia’s payload bay doors prior to entry. Right: Flash of plasma seen through Columbia’s overhead window during reentry.
At the end of 13 days, the astronauts finished the last of the experiments and deactivated the Spacelab module. Managers waved off the planned landing on July 22 due to cloudy weather at KSC. On July 23, the astronauts closed the hatch to the Spacelab module for the final time, closed Columbia’s payload bay doors, donned their launch and entry suits, and strapped themselves into their seats for entry and landing. Cabana piloted Columbia to a smooth landing on KSC’s Shuttle Landing Facility, completing 236 orbits around the Earth in 14 days, 17 hours, and 55 minutes, at the time the longest shuttle flight. Mukai set a then-record for the longest single flight by a woman. In October 1994, Columbia returned to its manufacturer, Rockwell International in Palmdale, California, for scheduled modification and refurbishment before its next mission, STS-73, in October 1995.
Left: Robert D. Cabana pilots Columbia during the final approach to NASA’s Kennedy Space Center (KSC) in Florida, with the Vehicle Assembly Building visible through the window. Middle: Columbia touches down on KSC’s Shuttle Landing Facility to end the STS-65 mission. Right: Donald A. Thomas, left, and Cabana give a thumbs up after the successful mission.
The two Spacelab modules flew a total of 16 times, the last one during the STS-90 Neurolab mission in April 1998. Visitors can view the module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia. The other module resides at the Airbus Defence and Space plant in Bremen, Germany, and not accessible to the public.
The Spacelab long module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia.
Enjoy the crew narrate a video about the STS-65 mission. Read Cabana’s and Chiao’s recollections of the STS-65 mission in their oral histories with the JSC History Office.
Explore More 11 min read Fourth of July Holidays in Space Article 1 week ago 9 min read 40 Years Ago: STS-41D – First Space Shuttle Launch Pad Abort Article 2 weeks ago 5 min read The 1998 Florida Firestorm and NASA’s Kennedy Space Center Article 2 weeks agoNASA Marshall Researchers Battle Biofilm in Space
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The biofilm mitigation research team at NASA’s Marshall Space Flight Center assembled its own test stand to undertake a multi-month assessment of a variety of natural and chemical compounds and strategies for eradicating biofilm accretion caused by bacteria and fungi in the wastewater tank assembly on the International Space Station. Testing will help NASA extend the lifecycle of water reclamation and recycling hardware and ensure astronauts can sustain clean, healthy water supplies on long-duration missions in space and on other worlds.NASA/Eric BeitleA small group of scientists on the biofilm mitigation team at NASA’s Marshall Space Center in Huntsville, Alabama, study solutions to combat fast-growing colonies of bacteria or fungi, known as biofilm, for future space missions.
Biofilm occurs when a cluster of bacteria or fungi generates a slimy matrix of “extracellular polymeric substances” to protect itself from adverse environmental factors. Biofilm can be found nearly anywhere, from the gray-green scum floating on stagnant pond water to the pinkish ring of residue in a dirty bathtub.
For medical, food production, and wastewater processing industries, biofilm is often a costly issue. But offworld, biofilm proves to be even more resilient.
“Bacteria shrug off many of the challenges humans deal with in space, including microgravity, pressure changes, ultraviolet light, nutrient levels, even radiation,” said Yo-Ann Velez-Justiniano, a microbiologist and environmental control systems engineer at Marshall.
Biofilm is icky, sticky – and hard to kill.Liezel Koellner
Chemical Engineer and NASA Pathways Intern
“Biofilm is icky, sticky – and hard to kill,” said Liezel Koellner, a chemical engineer and NASA Pathways intern from North Carolina State University in Raleigh. Koellner used sophisticated epifluorescence microscopy, 3D visualizations of 2D images captured at different focal planes, to fine-tune the team’s studies.
Keenly aware of the potential hurdles biofilm could pose in future Artemis-era spacecraft and lunar habitats, NASA tasked engineers and chemists at Marshall to study mitigation techniques. Marshall built and maintains the International Space Station’s ECLSS (Environment Control and Life Support System) and is developing next-generation air and water reclamation and recycling technologies, including the system’s wastewater tank assembly.
“The wastewater tank is ‘upstream’ from most of our built-in water purification methods. Because it’s a wastewater feed tank, bacteria and fungus grow well there, generating enough biofilm to clog flow paths and pipes along the route,” said Eric Beitle, ECLSS test engineer at Marshall.
To date, the solution has been to pull and replace old hardware once parts become choked with biofilm. But engineers want to avoid the need for such tactics.
“Even with the ability to 3D-print spare parts on the Moon or Mars, it makes sense to find strategies that prevent biofilm buildup in the first place,” said Velez-Justiniano.
The team took the first step in June 2023 by publishing the complete genome sequence of several strains of bacteria isolated from the space station’s water reclamation system, all of which cultivate biofilm formation.
They next designed a test stand simulating conditions in the wastewater tank about 250 miles overhead, which permits simultaneous study of multiple mitigation options. The rig housed eight Centers for Disease Control and Prevention biofilm reactors – cylindrical devices roughly the size of a runner’s water bottle – each 1/60th the size of the actual tank.
Yo-Ann Velez-Justiniano, left, and Connor Murphy, right, both Environmental Control and Life Support Systems engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, prepare slides for study of cultured bacterial biofilm in the center’s test facility NASA/Eric BeitleEach bioreactor holds up to 21 unique test samples on slides, bathed continuously in a flow of real or ersatz wastewater, timed and measured by the automated system, and closely monitored by the team. Because of the compact bioreactor size, the test stand required 2.1 gallons of ersatz flow per week, continuously trickling 0.1 milliliters per minute into each of the eight bioreactors.
“Essentially, we built a collection of tiny systems that all had to permit minute changes to temperature and pressure, maintain a sterile environment, provide autoclave functionality, and run in harmony for weeks at a time with minimal human intervention,” said Beitle. “One phase of the test series ran nonstop for 65 days, and another lasted 77 days. It was a unique challenge from an engineering perspective.”
Different surface mitigation strategies, upstream counteragents, antimicrobial coatings, and temperature levels were introduced in each bioreactor. One promising test involved duckweed, a plant already recognized as a natural water purification system and for its ability to capture toxins and control wastewater odor. By devouring nutrients upstream of the bioreactor, the duckweed denied the bacteria what it needs to thrive, reducing biofilm growth by up to 99.9%.
Over the course of the three-month testing period, teams removed samples from each bioreactor at regular intervals and prepared for study under a microscope to make a detailed count of the biofilm colony-forming units on each plate.
“Bacteria and fungi are smart,” said Velez-Justiniano. “They adapt. We recognize that it is going to take a mix of effective biofilm mitigation methods to overcome this challenge.”
Biofilm poses as an obstacle to long-duration spaceflight and extended missions on other worlds where replacement parts may be costly or difficult to obtain. The biofilm mitigation team continues to assess and publish findings, alongside academic and industry partners, and will further their research with a full-scale tank experiment at Marshall. They hope to progress to flight tests, experimenting with various mitigation methods in real microgravity conditions in orbit to find solutions to keep surfaces clean, water potable, and future explorers healthy.
Joel Wallace
Marshall Space Flight Center, Huntsville, Ala.
256-786-0117
joel.w.wallace@nasa.gov
Gateway: Illuminating the Future
An interplay of light and shadows cast the docking ports for Gateway, humanity’s first space station around the Moon, into sharp relief.
Built by NASA commercial partner Northrup Grumman, HALO (Habitation and Logistics Outpost), is one of four modules where international teams of astronauts will live, conduct science, and prepare for missions to the lunar South Pole region. The module’s main structure is currently undergoing testing in Turin, Italy. One docking port seen inside HALO, image right, is where a cargo spacecraft and Gateway’s Lunar View module, provided by ESA (European Space Agency), will dock. The docking port shown outside of HALO, image left, is where the SpaceX Starship and the Blue Origin Blue Moon Human Landing Systems will dock during the Artemis IV and V missions, respectively.
Gateway will launch to lunar orbit with the Power and Propulsion Element, provided by Maxar Space Systems, and later expand with ESA’s Lunar I-Hab and Lunar View modules, the Crew and Science Airlock provided by the Mohammed Bin Rashid Space Centre, advanced external robotics provided by CSA (Canadian Space Agency), and critical hardware from JAXA (Japan Aerospace Exploration Agency).
NASA and its international partners will explore the scientific mysteries of deep space with Gateway. The space station is central to the Artemis architecture that will return humans to lunar surface for scientific discovery and chart a path for the first humans to Mars.
An artist’s concept image of a docking port on Gateway’s HALO module.NASA/Alberto Bertolin, Bradley Reynolds An artist’s concept image of the Gateway space station showing ESA’s Lunar View module and a government-reference Human Landing System docked to HALO.NASA Learn More About Gateway Facebook logo @NASAGateway @NASA_Gateway Instagram logo @nasaartemis Share Details Last Updated Jul 10, 2024 EditorBriana R. ZamoraContactBriana R. Zamorabriana.r.zamora@nasa.gov Related Terms Explore More 5 min read From Polar Peaks to Celestial Heights: Christy Hansen’s Unique Path to Leading NASA’s Commercial Low Earth Orbit Development Program Article 1 day ago 2 min read NextSTEP Q: CIS Capability Studies III – Lunar User Terminals & Network Orchestration and Management System Article 2 days ago 2 min read NASA Shares Use Requirements with Commercial Destination Partners Article 1 week ago Keep Exploring Discover More Topics From NASA GatewayBuilt with international and commercial partners, Gateway will be humanity’s first space station around the Moon as a vital component…
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NASA Inspires at 2024 ESSENCE Fest in New Orleans
NASA joined the self-designated “party with a purpose” to let participants in the 30th ESSENCE Festival of Culture in New Orleans know there is space for everybody at the space agency.
NASA representatives from the agency’s Headquarters in Washington participated in a panel conversation about Black women in the aerospace industry and diversity in science, technology, engineering, and mathematics (STEM). NASA Assistant Deputy Associate Administrator for the Moon to Mars Program Office Lakiesha Hawkins and NASA Director of Engagement Aya Collins spoke to fest participants during the Take Up Space (Literally) presentation on July 5.
On both July 5-6, representatives from NASA Headquarters and NASA’s Stennis Space Center near Bay St. Louis, Mississippi, also hosted an informational/interactive booth at the Audubon Aquarium near the festival meeting site. The representatives shared about NASA’s Artemis campaign, and NASA Stennis’ role as America’s largest rocket propulsion test site. With the Artemis campaign, NASA will land the first woman and first person of color on the Moon, using innovative technologies to explore more of the lunar surface than ever before.
NASA representatives at the Audubon Aquarium provided attendees with memorabilia and an immersive experience to the International Space Station, which serves as the world’s leading space laboratory. Astronauts aboard the space station are conducting cutting-edge research and technology development to support human and robotic exploration of destinations beyond low Earth orbit, including the Moon and Mars.
The annual ESSENCE Fest attracts hundreds of thousands of people to New Orleans during the Fourth of July weekend to celebrate the Black community. The NASA outreach and engagement effort continues the agency’s commitment to advance equity and reach deeper into underrepresented and underserved segments of society as NASA explores the secrets of the universe for the benefit of all.
Explore the Essence Fest Gallery Share Details Last Updated Jul 09, 2024 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms Keep Exploring Discover More Topics From NASA StennisAbout NASA Stennis
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NASA Invites Media to 65th Birthday Celebration for Iconic Logo
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Preparations for Next Moonwalk Simulations Underway (and Underwater) In Orbiter Processing Facility-2 at NASA’s Kennedy Space Center in Florida, Michael Williams of United Space Alliance paints the NASA logo — known as the “meatball” — on the left wing of space shuttle Endeavour in 2012.Credit: NASA/Dimitri GerondidakisNASA’s logo turns 65 on Monday, July 15, and media are invited to its birthday celebration in Cleveland, the city where the iconic symbol was designed.
To mark the logo’s birthday, NASA’s Glenn Research Center in Cleveland will host a series of activities celebrating the city’s connection to one of the most recognized logos in the world from 10 a.m. to 5 p.m. ET on July 15 at Great Lakes Science Center, home of Glenn’s visitor center. Admission to the Science Center will be free, and the event is open to the public.
A birthday celebration and cake-cutting ceremony will begin at 10:30 a.m. and feature remarks from center leadership, a visit from the logo designer’s family, and special presentations from the city and state. Other activities include:
- History and Symbolism of NASA Insignia Presentation, noon and 2 p.m.
- NASA Creatives Presentation featuring Glenn’s award-winning photographers and videographers, 1 p.m.
- Coloring contest, 10 a.m. to 1:30 p.m.
- Coloring contest winners announced, 2 p.m.
- Eva the Astronaut mascot appearance and photo ops, 1 to 2:30 p.m. and 3:30 to 4:30 p.m.
- NASA Creatives Presentation featuring retired NASA Glenn photographer Marv Smith, 3 p.m.
The round blue, white, and red logo affectionately nicknamed the “meatball” became official in 1959 and was designed by the late James Modarelli, a Cleveland Institute of Art graduate and employee of Lewis Research Center (now NASA Glenn).
Media interested in covering the event should contact Jacqueline Minerd at jacqueline.minerd@nasa.gov.
For more information on NASA Glenn events, visit:
https:www.nasa.gov/glenn-communityengagement/
-end-
Jacqueline Minerd
Glenn Research Center, Cleveland
216-433-6036
jacqueline.minerd@nasa.gov
NASA Technology Soars at Selfridge Air Show
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Tim Campbell, a NASA solar system ambassador, shares highlights of a moon rock with visitors inside the Journey to Tomorrow traveling exhibit. Credit: NASA/Christopher HartenstineNASA’s Glenn Research Center staff traveled to Michigan for the Selfridge Air National Guard Base air show, open house, and STEAM Expo, June 8 and 9. NASA’s Journey to Tomorrow, a 53-foot traveling exhibit, was a popular feature that showcased exploration in air and space. Additionally, experts from NASA’s Fission Surface Power project shared information on the agency’s current and future work in this area.
Lindsay Kaldon, project manager for the Fission Surface Power project, left, joined the air show’s broadcast to discuss NASA’s Technology Demonstration Missions portfolio and pathways to STEAM careers at NASA. Credit: NASA/Christopher HartenstineMembers of NASA’s SLS (Space Launch System) outreach team supported hands-on engagement in the STEAM Expo hangar. Trudy Kortes, director of Technology Demonstrations for NASA’s Space Technology Mission Directorate, and Lindsay Kaldon, project manager for the Fission Surface Power project, joined the air show’s broadcast to discuss NASA’s Technology Demonstration Missions portfolio and pathways to STEAM careers at NASA.
Return to Newsletter Explore More 1 min read NASA Glenn Welcomes Summer Student Interns Article 23 hours ago 7 min read Spectral Energies developed a NASA SBIR/STTR-Funded Tech that Could Change the Way We Fly Article 24 hours ago 3 min read Happy Birthday, Meatball! NASA’s Iconic Logo Turns 65 Article 2 days agoInternational and Space Law
The International and Space Law Practice Group (ISLPG) is responsible for providing legal advice and counsel regarding international matters at Headquarters and all NASA Centers. Some of the legal issues for which ISLPG is responsible include: international law, including space law; domestic law which may impact NASA’s international cooperation; issues involving the United Nations or other multilateral organizations; international trade; telecommunications and use of the radiofrequency spectrum; international aspects of commercialization; export control; and national security. ISLPG advises on negotiating, drafting, executing, and interpreting agreements, understandings, treaties and exchanges with all types of foreign entities (both commercial and governmental), including international organizations.
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Rainbow Alliance Advisory Group Showcases NASA at Pride Event in Downtown Cleveland
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Members of NASA Glenn Research Center’s Rainbow Alliance Advisory Group hosted a booth to share information on NASA during the “Pride in the CLE” event. Credit: NASA/Steven LoganFor the second year in a row, NASA Glenn Research Center’s Rainbow Alliance Advisory Group (RAAG), with support from additional Glenn employees, marched in Cleveland’s “Pride in the CLE” festival on June 1. This year, they widened their presence by staffing an exhibit booth, which showcased NASA and inclusion in the workplace.
Throughout the day, RAAG members engaged with more than 1,500 members of the public, distributing NASA stickers and Diversity, Equity, and Inclusion pins. They also shared information on employment and internship opportunities and details of NASA Glenn’s work in aeronautics and aerospace.
NASA’s Glenn Research Center employees march in the “Pride in the CLE” parade in downtown Cleveland. Credit: NASA/Steven LoganThe event was supported by NASA Glenn’s Office of Diversity and Equal Opportunity and the Diversity, Equity, Inclusion, and Accessibility committee.
Return to Newsletter Explore More 1 min read NASA Glenn Welcomes Summer Student Interns Article 3 hours ago 2 min read NASA Prepares for Air Taxi Passenger Comfort Studies Article 2 weeks ago 4 min read NASA Parachute Sensor Testing Could Make EPIC Mars Landings Article 2 weeks agoNASA Glenn Welcomes Summer Student Interns
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Center Director Dr. Jimmy Kenyon talks with a student intern prior to an orientation session. Credit: NASA/Jordan SalkinNASA Glenn Research Center’s Office of STEM Engagement provided a multi-faceted orientation—including a welcome from Center Director Dr. Jimmy Kenyon—for 151 student interns (on-site and virtually) last month. This summer, student interns from across the United States and U.S. territories will gain practical experience while working with scientists, engineers, and individuals from many other professions.
NASA Glenn Research Center’s students interning on-site this summer pose for a group photo at the back of the hangar at Lewis Field in Cleveland. Credit: NASA/Sara Lowthian-HannaEvents included information about NASA Glenn’s various departments, resources, and services, offering interns a comprehensive overview of the center. A special event featured 17 organizations showcasing the various resources and opportunities available to students during their internships. A livestream of the United Launch Alliance Atlas V Boeing Starliner Crewed Flight Test Launch was part of the activities.
Return to Newsletter Explore More 1 min read NASA Technology Soars at Selfridge Air Show Article 3 hours ago 1 min read Rainbow Alliance Advisory Group Showcases NASA at Pride Event in Downtown Cleveland Article 3 hours ago 7 min read Spectral Energies developed a NASA SBIR/STTR-Funded Tech that Could Change the Way We Fly Article 3 hours agoCelebrate the Heliophysics Big Year with Free Heliophysics and Math Webinars from NASA HEAT
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Celebrate the Heliophysics Big Year with Free Heliophysics and Math Webinars from NASA HEATThe Heliophysics Big Year (HBY) is a global celebration of the Sun’s influence on Earth and the entire solar system. It began with the Annular Solar Eclipse on Oct. 14, 2023, continued through the Total Solar Eclipse on Apr. 8, 2024, and will conclude with Parker Solar Probe’s closest approach to the Sun in December 2024.
Challenged by the NASA Heliophysics Division to participate in as many Sun-related activities as possible, the NASA Heliophysics Education Activation Team (NASA HEAT) has been hosting a monthly webinar for formal and informal educators, science communicators, and other heliophysics enthusiasts to promote the understanding of heliophysics in alignment with monthly HBY themes. Each webinar’s content is designed with the Framework of Heliophysics Education in mind and maps directly to the Next Generation Science Standards (NGSS). Using the three main questions that heliophysicists investigate as a foundation, NASA HEAT cross-referenced heliophysics topics with the NGSS Disciplinary Core Ideas to create NGSS-aligned “heliophysics big ideas.” In each webinar, three math problems related to the theme are presented for beginner, intermediate, and advanced level learners. On average, there have been 30 attendees per webinar.
Register for upcoming webinars:
7/16/24 Physical and Mental Health
8/20/24 Back to School
9/17/24 Environment and Sustainability
10/15/24 Solar Cycle and Solar Max
11/19/24 Bonus Science
12/17/24 Parker’s Perihelion
NASA HEAT is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
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Spectral Energies developed a NASA SBIR/STTR-Funded Tech that Could Change the Way We Fly
Editor Note: Article written by Nicholas Mercurio
With $20 million in commercial sales and $15 million in sales to government agencies, minority-owned small business Spectral Energies, based in Beavercreek, Ohio, has found a customer base for its pulse-burst laser systems. NASA has played a significant role in developing the technology through the Small Business Innovation Research (SBIR) / Small Business Technology Transfer (STTR) program. With wide-ranging applications including metrology to support commercial aircraft certification, as well as material processing, this technology could pave the way for new forms of passenger aircraft.
Without the funding from NASA, it would have been impossible for us to push for versatile technological enhancements that significantly broadened the application field.Dr. Sukesh Roy
CEO of Spectral Energies
The High Cost of Aircraft CertificationDid you know that the Boeing 737 first entered service in 1968? Yet there’s a good chance that, if you’ve flown recently, it was on a Boeing 737. That’s due in large part to the cost of certifying new airplanes, which can range in the hundreds of millions of dollars. One place to look for cost savings is the testing process.
When testing a new design for a space vehicle or commercial aircraft, researchers use wind tunnels to simulate flight conditions. The new aircraft or aircraft component—such as a new wing design—is built, put inside the wind tunnel, and evaluated.
NASA has long sought to develop robust modeling and prediction software to significantly reduce the need for wind tunnel testing and expensive flight testing. Such software would allow initial analysis to be done on a computer model to identify performance improvement opportunities and iterate on designs, saving the actual manufacturing and its associated costs for a design much closer to being final. Innovations in laser measurement systems could finally bring this goal within reach.
The Limitations of Traditional Lasers and Early Pulse-Burst Laser SystemsEntering into use in the 1980s and still widely used today, traditional commercial laser systems operate at 10 Hz, meaning they can fire 10 times per second into the air moving around an aircraft in a wind tunnel. This essentially provides a “photograph” of the air flow at that moment.
But a tenth of a second is a long time, especially when NASA wind tunnels can test vehicles at up to ten times the speed of sound. In a tenth of a second, the pocket of air from the previous image has long since moved on, meaning the second image is capturing something completely different than the first and crucial data is lost.
Why is this data crucial? Because when an aircraft has stalled, it’s the air flow—how the air moves over, under, and around the aircraft—that matters. This air flow changes rapidly in time, leading to effects like stall and buffet; measurement techniques need to be able to capture these rapid changes. Without a complete, data-backed understanding of air flow moment to moment, efforts to develop accurate modeling software have stalled.
In the late 1990s, pulse-burst laser systems came onto the scene and delivered a dramatic increase in measurement speed. These systems—developed in part with support from the NASA SBIR program—went from producing a set of photograph-like images to delivering a movie-like sequence of data. However, these early systems were difficult to transport and operate, significantly limiting their use.
NASA SBIR/STTR phasesCredits: NASA SBIR/STTR Enhancing Usability with Air Force SBIR FundingBy providing funding to develop early-stage technologies, the NASA SBIR/STTR program helps de-risk and develop ideas, maturing them to the point where others can continue innovating. More than a decade after helping to fund some of the earliest pulse-burst laser systems, NASA awarded Phase I SBIR funding to Spectral Energies in 2009 for further advancement of the technology.
The firm went on to receive Phase II and Phase III SBIR funding from the U.S. Air Force, leveraging these awards to create a commercial pulse-burst laser system that was smaller, easier to transport, more resilient and reliable, and simpler to operate due to significant software advancements. Air Force funding also enabled Spectral Energies to demonstrate several new applications of the system in combustion environments.
With this foundational work in place, the technology was ready for further innovation to help NASA pursue its long-held goal of more effective air flow measurement and modeling.
Spectral Energies work with the NASA SBIR/STTR programSpectral Energies resumed its work with the NASA SBIR/STTR program in 2014 with multiple Phase I awards. Through continuing program awards, including three Phase II Extended (II-E) and three Phase III contracts, the firm added new capabilities to its pulse-burst laser system, such as high-speed two-color thermometry, demonstrated in 2020.
Previously, two-color thermometry was typically done at 10 Hz speeds with two lasers and two cameras. Spectral Energies worked with NASA to develop this capability at high-speed using their single-laser, single-camera system, thereby enabling three- and four-dimensional (i.e., three spatial coordinates and time) temperature measurement of chemical flows, a critical capability when designing new chemical propulsion systems.
Further collaboration with NASA yielded additional capabilities in high-speed picosecond velocimetry and two-dimensional ultraviolet spectroscopy and imaging. Adding these measurement techniques to its technology allowed Spectral Energies to make commercial inroads into hypersonic wind tunnel testing, material processing, and defense applications. Rather than modifying the pulse-burst laser system to deliver these capabilities, each enhancement took the form of an add-on that could be attached to the system, similar to how you can add apps to your smart phone or attach a new lens to your camera. These NASA SBIR-funded add-ons have increased the return on investment (ROI) for each of Spectral Energies’ customers across federal agencies, research universities, and commercial companies.
Growing a Small BusinessFor small businesses, the hunger to do more is often quelled by the reality of limited resources. As a result, necessity is often the biggest driver of decision-making: What do we need to do today to keep our doors open tomorrow? Funding from the NASA SBIR/STTR program allowed Spectral Energies to move into a different mindset and tap into their creative drive.
“Through the NASA program, we started diversifying in hypersonic test facilities from subsonic combustion facilities,” said Dr. Sukesh Roy, CEO of Spectral Energies, “and that opened many doors for the application of this laser, from detonation to directed energies. Without the funding from NASA, it would have been impossible for us to push for versatile technological enhancements that significantly broadened the application field.” Moving into the research and development of new applications allowed the company to widen its focus and ultimately find a larger customer base.
Spectral Energies’ continued work with the NASA SBIR/STTR program has helped the company further grow and succeed. By providing entry into new industries and new capabilities for existing customers, the add-on technologies developed with NASA SBIR-funding have generated significant commercial revenue for the small business. Additionally, these developments have opened the door for new funding opportunities with the Air Force, Navy, Army, and Missile Defense Agency.
Providing Benefit to NASA and BeyondDr. Paul Danehy, Senior Technologist for Advanced Measurement Systems at NASA’s Langley Research Center, has worked with Spectral Energies on a number of projects through the program. According to Dr. Danehy, not only did NASA SBIR funding aid the company’s technology growth, program funding also made it possible for NASA researchers to make use of this technology.
As Dr. Danehy explains, SBIR/STTR Post Phase II funding vehicles like Phase II-E and Phase III allow other programs within NASA to pool money together, then receive matching funds from the SBIR/STTR program. This matching funding increases the purchasing power of other NASA programs and has allowed the agency to acquire two of Spectral Energies’ pulse-burst laser systems, complete with add-ons.
Agency researchers are using these pulse-burst laser systems to obtain unique quantitative flow field measurements that will allow them to refine software codes to accurately design and evaluate new aerospace vehicles. In time, these software codes could cut hundreds of millions of dollars from the certification of commercial aircraft, allowing new planes to be developed and made available to passengers faster and cheaper.
