NASA’s Dragonfly Tunnel Visions

NASA’s Dragonfly Tunnel Visions

5 min read

NASA’s Dragonfly Tunnel Visions

Dragonfly Team Utilizes Unique NASA Facilities to Shape Its Innovative Titan-bound Rotorcraft 

Dragonfly team members review the half-scale lander model
Dragonfly team members review the half-scale lander model after it underwent wind tunnel testing at NASA Langley Research Center in Hampton, Virginia. Pictured are (from left) Art Azarbarzin, Juan Cruz, Wayne Dellinger, Zibi Turtle, Chuck Hebert, Ken Hibbard, Bernadine Juliano and Bruce Owens.
Johns Hopkins APL/Ed Whitman

With its dense atmosphere and low gravity, Saturn’s moon Titan is a great place to fly. 

But well before NASA’s Dragonfly rotorcraft lander soars through Titan’s skies, researchers on Earth – led by the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland – are making sure their designs and models for the nuclear-powered, car-sized drone will work in a truly unique environment.

Artist’s impression of the Dragonfly rotorcraft lander on the surface of Titan, Saturn’s largest moon
Artist’s impression of the Dragonfly rotorcraft lander on the surface of Titan, Saturn’s largest moon and a major target in NASA’s quest to assess habitability and search for potential signs of life beyond Earth on worlds across the solar system.
NASA/Johns Hopkins APL/Steve Gribben

Dragonfly, NASA’s only mission to the surface of another ocean world, is designed to investigate the complex chemistry that is the precursor to life. The vehicle, which APL will build and operate, will be equipped with cameras, sensors and samplers to examine swaths of Titan known to contain organic materials that may, at some point in Titan’s complex history, have come in contact with liquid water beneath the organic-rich, icy surface. 

To transport those science instruments across the moon, Dragonfly’s four pairs of coaxial rotors (meaning one rotor is stacked above the other) will need to slice through Titan’s dense, nitrogen-rich atmosphere. Four times in the past three years, the mission team has headed to Virginia to test its flight systems in one-of-a-kind facilities at NASA’s Langley Research Center in Hampton, Virginia. 

Mission engineers have conducted two test campaigns in NASA Langley’s 14-by-22-foot Subsonic Tunnel, and two in the 16-foot Transonic Dynamics Tunnel (TDT).  They use the Subsonic Tunnel to validate computational fluid dynamics models and data gathered from integrated test platforms – terrestrial drones outfitted with Dragonfly-designed flight electronics. They use the variable-density heavy gas capabilities of the TDT to validate its models under simulated Titan atmospheric conditions — one aerodynamic stability test of the aeroshell that is used to deliver the Lander to a release point above Titan’s surface and one to model the Lander’s rotors aerodynamics. 

“All of these tests feed into our Dragonfly Titan simulations and performance predictions,” said Ken Hibbard, Dragonfly mission systems engineer at APL. 

On its latest trip to NASA Langley, in June, the team set up a half-scale Dragonfly lander model, complete with eight rotors, in the 14-by-22 Subsonic Tunnel. Test lead Bernadine Juliano of APL said the campaign focused on two flight configurations: Dragonfly’s descent and transition to powered flight upon arrival at Titan, and forward flight over Titan’s surface. 

“We tested conditions across the expected flight envelope at a variety of wind speeds, rotor speeds, and flight angles to assess the aerodynamic performance of the vehicle,” she said. “We completed more than 700 total runs, encompassing over 4,000 individual data points. All test objectives were successfully accomplished and the data will help increase confidence in our simulation models on Earth before extrapolating to Titan conditions.”

APL engineers are analyzing the 14-by-22 test data with mission flight team partners at the University of Central Florida, Penn State University, Lockheed Martin Sikorsky, NASA Langley and NASA Ames Research Center in Silicon Valley, California. Rick Heisler, the Dragonfly wind tunnel test lead from APL who heads the TDT test campaigns, said each trip to NASA Langley has given the team a chance to hone its technical models and designs and, specifically in the TDT, gain a better idea of how Dragonfly’s rotors will perform in Titan’s exotic atmosphere.  

“The heavy gas environment in the TDT has a density three-and-a-half times higher than air while operating at sea level ambient pressure and temperature,” Heisler said, “This allows the rotors to operate at near-Titan conditions and better replicate the lift and dynamic loading the actual lander will experience. The data we acquire are used to validate predictions of the lander aerodynamics, aero-structural performance and rotor fatigue life in the harsh cryogenic environment on Titan.”

“With Dragonfly, we’re turning science fiction into exploration fact,” Hibbard said. “The mission is coming together piece by piece, and we’re excited for every next step toward sending this revolutionary rotorcraft across the skies and surface of Titan.” 

Part of NASA’s New Frontiers Program, Dragonfly is scheduled to launch no earlier than 2027 and arrive at Titan in the mid-2030s. Principal Investigator Elizabeth Turtle of APL leads a mission team that includes engineers, scientists and specialists from APL as well as NASA’s Goddard Space Flight Center in Greenbelt, Maryland; Lockheed Martin Space in Littleton, Colorado; NASA’s Ames Research Center in Silicon Valley, California; NASA’s Langley Research Center in Hampton, Virginia; Penn State University in State College, Pennsylvania; University of Central Florida in Orlando, Florida; Lockheed Martin Sikorsky in Stratford, Connecticut; Malin Space Science Systems in San Diego; Honeybee Robotics in Pasadena, California; NASA’s Jet Propulsion Laboratory in Southern California;  CNES (Centre National d’Etudes Spatiales) in Paris; the German Aerospace Center (DLR) in Cologne, Germany; and JAXA (Japan Aerospace Exploration Agency) in Tokyo. 

Learn more at www.nasa.gov/dragonfly

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Tricia Talbert

NASA Test Piloting Legends Reunite

NASA Test Piloting Legends Reunite

1 min read

NASA Test Piloting Legends Reunite

Nils Larson, X59 pilot and Astronaut Victor Glover walking side-by-side.
Former flight test instructor and current NASA test pilot Nils Larson reunited with former student and current astronaut Victor Glover on Oct. 21 during an open house at NASA’s Langley Research Center in Hampton, Virginia.
NASA / Dave Bowman

Nils Larson, aerospace engineer and test pilot for NASA’s X-59 aircraft, met up with his former student, Artemis II astronaut Victor Glover, on Saturday, Oct. 21 during an open house held at NASA’s Langley Research Center in Hampton, Virginia. The pilots originally met more than two decades ago when Larson was an instructor at the U.S. Air Force Test Pilot School. Larson trained students – including Glover – using the T-38 aircraft.  

“I always knew Victor would go far. It’s cool to think that far means the Moon,” said Larson, whose current test piloting work is critical to NASA’s Quesst mission. “I was excited to see him picked up as an astronaut, then get to fly to the International Space Station, and now he gets to go to the Moon as part of Artemis II. The sky’s not the limit anymore!” 

Nearly 40,000 people attended the NASA Langley open house. Larson and Glover reunited at Langley’s hangar where other NASA legends, such as astronauts Neil Armstrong and Alan Shepard, trained on its historic Rendezvous Docking Simulator. The simulator remains a permanent fixture at the hangar. 

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Lillian Gipson

New York Students to Hear from Astronaut Aboard Space Station

New York Students to Hear from Astronaut Aboard Space Station

NASA astronaut and Expedition 70 Flight Engineer Jasmin Moghbeli works with the Advanced Resistive Exercise Device, or ARED, removing and replacing cables. The device uses adjustable resistive mechanisms to provide crew members a weight load while exercising to maintain muscle strength and mass in microgravity.

Students from Baldwin Union Free School District in Baldwin, New York, will have an opportunity this week to hear from an astronaut aboard the International Space Station. The Earth-to-space call will air live at 11 a.m. EDT Friday, Oct. 27, on NASA Television, the NASA app, and the agency’s website.

NASA astronaut Jasmin Moghbeli, an alumnus of Baldwin Union Free School District, will answer prerecorded questions from students.

Media interested in covering the event should RSVP no later than 5 p.m. on Wednesday, Oct. 25, to Mary Furcht at furchtm@baldwinschools.org or 516-434-6012.

These educational opportunities for students to speak with astronauts living and working on the space station are provided by the Office of STEM Engagement’s Next Gen STEM project.

For almost 23 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing the skills needed to explore farther from Earth. Astronauts living in space aboard the orbiting laboratory communicate with NASA’s Mission Control Center in Houston 24 hours a day through the Space Communications and Navigation (SCaN) Near Space Network.

Important research and technology investigations taking place aboard the International Space Station benefits people on Earth and lays the groundwork for future exploration.

As part of Artemis, NASA will send astronauts to the Moon to prepare for future human exploration of Mars. Inspiring the next generation of explorers – the Artemis Generation – ensures America will continue to lead in space exploration and discovery.

See videos and lesson plans highlighting research on the International Space Station at:

https://www.nasa.gov/stemonstation

-end-

Katherine Brown
Headquarters, Washington
202-358-1288
katherine.m.brown@nasa.gov

Sandra Jones 
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov

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Oct 23, 2023

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Abbey A. Donaldson

NASA’s SpaceX CRS-29 Mission Flies Research to the Space Station

NASA’s SpaceX CRS-29 Mission Flies Research to the Space Station

The 29th SpaceX commercial resupply services (CRS) mission for NASA carries scientific experiments and technology demonstrations, including studies of enhanced optical communications and measurement of atmospheric waves. The uncrewed SpaceX Dragon spacecraft is scheduled to launch to the International Space Station from the agency’s Kennedy Space Center in Florida no earlier than Nov. 5.

Download high-resolution photos and videos of the research mentioned in this article.

Here are details on some of the research launching to the orbiting lab:

Laser Communication from Space

NASA’s ILLUMA-T investigation tests technology to provide enhanced data communication capabilities on the space station. A terminal mounted on the station’s exterior uses laser or optical communications to send high-resolution information to the agency’s Laser Communications Relay Demonstration (LCRD) system, which is in geosynchronous orbit around Earth. LCRD then beams the data to optical ground stations in Haleakala, Hawaii, and Table Mountain, California. The system uses invisible infrared light and can send and receive information at higher data rates than traditional radio frequency systems, making it possible to send more images and videos to and from the space station in a single transmission. The ILLUMA-T demonstration also paves the way for placing laser communications terminals on spacecraft orbiting the Moon or Mars.

ILLUMA-T and LCRD create NASA’s first two-way laser communications relay system. Laser communications can supplement the radio frequency systems that most space-based missions currently use to send data to and from Earth. According to acting ILLUMA-T project manager Glenn Jackson at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, laser systems are smaller, more lightweight, and use less power than radio systems. The smaller size frees up more room for science instruments, the lighter weight reduces launch costs, and lower power use results in less drain on spacecraft batteries.

Managed by NASA Goddard in partnership with NASA’s Johnson Space Center in Houston and the Massachusetts Institute of Technology Lincoln Laboratory, ILLUMA-T is funded by the Space Communications and Navigation (SCaN) program at NASA Headquarters in Washington.

Hardware including tangles of large orange cords and smaller white cords connecting various boxes and boards sits on a large, wheeled cart. To the right is a refrigerator-sized blue computer box topped with red and green flashing lights. A power strip runs along the wall behind.
The ILLUMA-T laser communications system being prepared for launch at Goddard Space Flight Center.
NASA/Goddard Space Flight Center

Watching Waves in the Atmosphere

NASA’s Atmospheric Waves Experiment (AWE) uses an infrared imaging instrument to measure the characteristics, distribution, and movement of atmospheric gravity waves (AGWs). These waves roll through Earth’s atmosphere when air is disturbed much like waves created by dropping a stone into water.

“Atmospheric gravity waves are one mechanism for transporting energy and momentum within the climate system and they play a role in defining the climate and its evolution,” says co-investigator Jeff Forbes of the University of Colorado Boulder. He explains that these waves are relatively small at the source but amplified at altitudes, and potentially indicate climate changes not readily observable at lower altitudes. This investigation’s long-term observations of physical processes in atmospheric circulation could increase insight into AGWs and improve understanding of Earth’s atmosphere, weather, and climate.

Researchers also are looking at how AGWs contribute to space weather, which refers to the varying conditions within the Solar System, including solar wind. Space weather affects space- and ground-based communications, navigation, and tracking systems. Scientists know little about exactly how AGWs influence space weather and this investigation could help fill in these knowledge gaps. Results could support development of ways to mitigate the effects of space weather.

The space station provides an ideal platform for the investigation given its altitude and geographic and time coverage.

“AWE is pioneering research, making the first global measurements of gravity waves at the edge of space,” Forbes says. “This is an important step forward in understanding waves in the atmosphere and their contributions to near-Earth space weather.”

The Atmospheric Waves Experiment is managed by Goddard for NASA’s Science Mission Directorate at NASA Headquarters.

Two scientists wearing white lab coats, hoods, and masks work behind a large reflective disc with four camera lenses in its center, part of the assembly for the AWE.
Scientists prepare the optical assembly for AWE for launch in a clean room at Space Dynamics Laboratory facilities.
Space Dynamics Laboratory/Allison Bills

More science going to the space station

Space Flight Induced Ovarian and Estrogen Signaling Dysfunction, Adaptation, and Recovery is a fundamental science investigation sponsored by NASA’s Biological and Physical Sciences Division. It advances previous microgravity studies that seek to better understand the combined effects of spaceflight, nutritional, and environmental stresses on control of ovulation and resulting effects on the skeleton. Results of this study could help identify and treat the effects of stress on ovulation and improve bone health on Earth.

Magnified image of a slide containing a section of tissue, stained purple, with a variety of large and small shapes inside it. Some look like open space and others are partially or completed filled in.
A section of ovarian tissue prepared for an investigation of ovarian function and bone health in space.
University of Kansas Medical Center

Aquamembrane-3, an investigation from ESA (European Space Agency), continues evaluation of replacing the multi-filtration beds used for water recovery on the space station with a type of membrane known as an Aquaporin Inside Membrane (AIM). These are membranes that incorporate proteins found in biological cells, known as aquaporins, to filter water faster while using less energy. Initial testing of AIM technology in 2015 showed that water filtration by membranes is possible in microgravity, and this follow-up testing could demonstrate how effectively the membranes eliminate contaminants in space station wastewater. Results could advance development of a complete and full-scale membrane-based water recovery system, improving water reclamation and reducing the amount of material that needs to be launched to the space station. This water filtration technology also could have applications in extreme environments on Earth, such as military and emergency settings, and for decentralized water systems in remote locations.

Hardware for Aquamembrane-3, a silver suitcase-sized block with six plastic fluid inputs, with a bright orange sample bag bearing a label sitting on its top.
A pre-launch view of equipment for the Aquamembrane-3 investigation.
ESA

Gaucho Lung, sponsored by the ISS National Lab, studies how mucus lining the respiratory system affects delivery of drugs carried in a small amount of injected liquid, known as a liquid plug. Conducting this research in microgravity makes it possible to isolate the factors involved, including capillary or wicking forces, mucus characteristics, and gravity. Understanding the role of these factors could inform the development and optimization of targeted respiratory treatments. In addition, the work could contribute to new strategies to control contamination in tubing for liquids used in the health care and food industries.

A worker wearing blue coveralls and gloves uses a syringe to place liquid on a glass surface held by a clamp. There is a black camera above the surface on another clamp in the foreground and a bright light and a focusing lens opposite the camera.
An investigator at University of California Santa Barbara prepares the camera and work light for recording images from the Gaucho Lung investigation prior to launch.
BioServe Space Technologies

Search this database of scientific experiments to learn more about those mentioned above.

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Ana Guzman

NASA Sets Coverage for Roscosmos Spacewalk Outside Space Station

NASA Sets Coverage for Roscosmos Spacewalk Outside Space Station

(April 18, 2022) --- Cosmonaut Oleg Artemyev waves to the camera while working outside the Nauka multipurpose laboratory module during a spacewalk that lasted for six hours and 37 minutes to outfit Nauka and configure the European robotic arm on the International Space Station's Russian segment.
(April 18, 2022) — Cosmonaut Oleg Artemyev waves to the camera while working outside the Nauka multipurpose laboratory module during a spacewalk that lasted for six hours and 37 minutes to outfit Nauka and configure the European robotic arm on the International Space Station’s Russian segment.

NASA will provide live coverage as two Roscosmos cosmonauts conduct a spacewalk outside the International Space Station Wednesday, Oct. 25, to install communications hardware and inspect a portion of the orbital complex.  

Coverage begins at 1:45 p.m. EDT on NASA Television, the NASA app, and the agency’s website. The spacewalk is expected to begin at 2:10 p.m. and could last up to seven hours.

Expedition 70 cosmonauts Oleg Kononenko and Nikolai Chub will venture outside of the station’s Poisk module to install a synthetic radar communications system and release a nanosatellite to test solar sail technology. While outside the station, they also will inspect and photograph an external backup radiator on the Nauka multipurpose laboratory module that experienced a coolant leak on Oct. 9.

The spacewalk will be the 268th in support of space station assembly, maintenance, and upgrades. It will be the sixth for Kononenko, who will wear the Orlan spacesuit with red stripes and the first for Chub, who will wear the spacesuit with blue stripes.

Get breaking news, images and features from the space station on the station blog, Instagram, Facebook, and X.

Learn more about International Space Station research and operations at:

https://www.nasa.gov/station

-end-

Julian Coltre / Lora Bleacher
Headquarters, Washington
202-358-1100
julian.n.coltre@nasa.gov / lora.v.bleacher@nasa.gov

Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov

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Roxana Bardan