Planet Mars Images: Nov. 13-21, 2025 | NASA's Curiosity & Perseverance Rovers
Friends of NASA (FoN) is an independent non-governmental organization (NGO) dedicated to building international support for peaceful space exploration, commerce, scientific discovery, and STEM education.
Saturday, November 22, 2025
Planet Mars Images: Nov. 13-21, 2025 | NASA's Curiosity & Perseverance Rovers
NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center
NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center
NASA’s X-59 quiet supersonic research aircraft took to the skies for the first time Tuesday, Oct. 28, 2025, departing from Lockheed Martin’s Skunk Works facility in Palmdale, California, and arriving at NASA’s Armstrong Flight Research Center in Edwards, California. The milestone marks a major step for NASA’s Quesst mission and its goal of enabling quiet supersonic flight over land.
The X-59 aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.” Follow the X-59 team as they take on the exciting journey of building the X-59 and working toward quiet supersonic flight.
The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.
For more information about the X-59 and NASA's Quesst mission, visit www.nasa.gov/quesst
Image Credit: NASA's Armstrong Flight Research Center (AFRC)
Image Date: Oct. 28, 2025
#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #Palmdale #Edwards #California #UnitedStates #STEM #Education
Friday, November 21, 2025
The Wandering Tail of Comet C/2025 A6 (Lemmon): View from Spain
The Wandering Tail of Comet C/2025 A6 (Lemmon): View from Spain
What has happened to Comet Lemmon's tail?
The answer is blowing in the wind—the wind from the Sun in this case. This continuous outflow of charged particles from the Sun has been quite variable of late. As the Sun emits bursts of energy via what are called coronal mass ejections (CMEs), this pushes out and deflects charged particles emitted by the comet itself. The result is a blue hued ion tail for Comet C/2025 A6 (Lemmon) that is impressively intricate.
This long-duration composite image was taken from Alfacar, Spain last month. Comet Lemmon is now fading as it heads out away from the Earth and Sun and back into the outer Solar System. Comet Lemmon was discovered early this year. It rounded the Sun on November 8, 2025. Comet Lemmon passed nearest to the Earth—about half the Earth-Sun distance—on October 21.
Image Description: A starfield is shown above a mountain peak. Just above the mountain and extending up toward the upper right is a blue-tinted tail of a comet. The comet's head is just to the left of the peak.
Release Date: Nov. 17, 2025
#NASA #Astronomy #Space #Science #Comets #CometC2025A6Lemmon #Coma #CometaryTails #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #IgnacioFernández #Astrophotographers #Alfacar #Spain #España #STEM #Education #APoD
Chinese Scientists Make First Achievement in Detecting Neutrinos with JUNO
Chinese Scientists Make First Achievement in Detecting Neutrinos with JUNO
The world's largest transparent spherical neutrino detector in south China's Guangdong province reported its first achievement on November 19, 2025, marking a major step of its decade-long construction.
In a press conference held in Guangdong's Jiangmen by the Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences (CAS), IHEP deputy director Wen Liangjian presented the first physics result by the Jiangmen Underground Neutrino Observatory (JUNO).
Using 59 days of effective data after the start of operation on Aug. 26 this year, JUNO has already measured two of the solar neutrino oscillation parameters with a factor of 1.5 to 1.8 better precision than previous experiments, said Wen, also the physics analysis coordinator of the JUNO Collaboration.
The two parameters, originally determined by solar neutrinos, can also be precisely measured by reactor antineutrinos. Earlier results from the two approaches showed a mild 1.5-sigma discrepancy, known as the solar neutrino tension, hinting at a possible new physics theory.
Achieving such precision within only two months of operation shows that JUNO is performing exactly as designed, said Wang Yifang, JUNO project manager and spokesperson.
With this level of accuracy, JUNO will soon determine the neutrino mass ordering, test the three-flavour oscillation framework, and search for new physics beyond it, Wang added.
Since neutrinos rarely interact with ordinary matter, they can easily zip through human bodies, buildings, or even the entire Earth without being felt, earning them the nickname "ghost particles." Due to their elusive nature, neutrinos are the least understood fundamental particles, requiring massive detectors to capture their faintest traces.
At the heart of JUNO is a liquid-scintillator detector with an unprecedented mass of 20,000 tonnes, housed at the center of a 44-meter-deep water pool. A 41.1-meter-diameter stainless steel truss supports the 35.4-meter-diameter acrylic sphere, the liquid scintillator, over 45,000 photo-multiplier tubes (PMTs) and many other key components such as cables, magnetic shielding coils and light baffles.
When passing through the detector, neutrinos have a small chance of bumping into the hydrogen nuclei in the liquid, triggering extremely faint flashes, which can be detected by the surrounded PMTs and then converted into electrical signals.
JUNO is a major international collaboration led by the IHEP. The project involves more than 700 scientists from 75 institutions across 17 countries and regions. Proposed in 2008 and approved by the CAS and Guangdong Province in 2013, JUNO began underground construction in 2015 and started taking data in August 2025.
The CAS vice president Ding Chibiao said at the press conference that JUNO is a major international collaborative project in fundamental scientific research that brings together global expertise. The project demonstrates China's commitment to the principles of openness, cooperation, and mutual benefit for international partnerships.
JUNO is designed to determine the neutrino mass ordering and measure oscillation parameters with sub-percent precision. It will also study solar, atmospheric, supernova and geoneutrinos, and search for physics beyond the standard model of particle physics.
JUNO will continue to produce important results and train new generations of physicists for decades to come, said Cao Jun, director of IHEP and JUNO deputy spokesperson.
Learn more about the Jiangmen Underground Neutrino Observatory:
http://juno.ihep.cas.cn
Duration: 56 seconds
Release Date: Nov. 19, 2025
#NASA #Space #Astronomy #Science #Astrophysics #Physics #Neutrinos #Earth #China #中国 #GuangdongProvince #江门 #Jiangmen #JUNO #UndergroundNeutrinoObservatory #SolarSystem #Stars #Galaxies #BlackHoles #Blazars #Universe #SpaceResearch #InternationalScience #Technology #Engineering #CGTN #STEM #Education #HD #Video
Comet C/2025 A6 (Lemmon): View from Mexico
Comet C/2025 A6 (Lemmon): View from Mexico
Astrophotographer Braulio Guerra Urbiola: "Comet C/2025 A6 (Lemmon) . . . The green coma arises from sunlight exciting diatomic carbon (C₂) and cyanogen (CN). Its dust tail is shaped by radiation pressure and the solar wind as the comet travels at high velocity along its orbit toward perihelion."
Comet Lemmon was discovered early this year. It rounded the Sun on November 8, 2025. Comet Lemmon passed nearest to the Earth—about half the Earth-Sun distance—on October 21.
Braulio's website: https://app.astrobin.com/u/BraulioGuerra
Capture Location: Hidalgo, México
#NASA #Astronomy #Space #Science #Comets #CometC2025A6Lemmon #Coma #CometaryTails #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #BraulioGuerraUrbiola #Astrophotographers #Hidalgo #Mexico #STEM #Education
Russian Cosmonaut Spacewalk: Ryzhikov & Zubritsky | International Space Station
Russian Cosmonaut Spacewalk: Ryzhikov & Zubritsky | International Space Station
On Oct. 16, 2025, members of Expedition 73 and Russian cosmonauts Sergei Ryzhikov (station commander) and Aleksei Zubritsky of Roscosmos ventured onto the exterior of the Russian International Space Station (ISS) segment for more than six hours for the VKD-64 spacewalk. They installed the Ekran-M experiment for the production of semiconductors in the vacuum of space. The duo also removed a high-resolution camera monoblock, cleaned a window on the Zvezda service module, and removed a materials exposure experiment container.
Russian Spacewalker#1 Sergei Ryzhikov, Orlan-MKS No. 7 spacesuit with red stripes
Russian Spacewalker#2 Aleksei Zubritsky, Orlan-MKS No. 6 spacesuit with blue stripes
https://blogs.nasa.gov/spacestation/
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.
Release Date: Nov. 18-19, 2025
#NASA #Space #Astronomy #Science #Earth #ISS #Spacewalk #EVA #VKD64 #Cosmonauts #SergeiRyzhikov #AlekseiZubritsky #Russia #Россия #Roscosmos #Роскосмос #Astronauts #AstronautPhotography #UnitedStates #Japan #JAXA #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education
World's Most Sensitive Cosmic-ray Observatory: LHAASO
World's Most Sensitive Cosmic-ray Observatory: LHAASO
At over 4,400 meters above sea level on the Qinghai-Xizang Plateau in Daocheng, southwest China's Sichuan Province, stands the world's most advanced cosmic-ray observatory—the Large High Altitude Air Shower Observatory (LHAASO). Since its completion in 2021, it remains the world's highest, largest and most sensitive observatory for detecting high-energy cosmic rays and gamma rays. CGTN's Liu Jiaxin takes us inside this mega-facility, where scientists are tracing particles from the universe's high-energy frontiers.
https://lssf.cas.cn/en/facilities/pnp/lhaaso/
Video Credit: CGTN
Duration: 6 minutes, 46 seconds
Release Date: Nov. 16, 2025
#NASA #Space #Astronomy #Science #Earth #Astrophysics #Physics #CosmicRays #GammaRays #China #中国 #LHAASO #AstronomicalObservatory #QinghaiXizangPlateau #Daocheng #Sichuan #SolarSystem #Stars #Galaxies #BlackHoles #Universe #SpaceResearch #InternationalScience #Technology #Engineering #STEM #Education #HD #Video
Planting an Artemis I Moon Tree | NASA Goddard
Planting an Artemis I Moon Tree | NASA Goddard
On Nov. 16, 2022, NASA launched the Artemis I test flight, sending an uncrewed Orion capsule beyond the Moon and back. On board were seeds from five species of trees, to be planted after returning to Earth. On Nov. 7, 2024, a seedling from the Artemis I flight was planted at the NASA Goddard Visitor Center by Artemis I Mission Manager Mike Sarafin, Artemis II Camera Lead Marie Henderson, Artemis III Project Scientist Noah Petro, Artemis IV Project Scientist Barbara Cohen, and others. In commemorating the event, Dr. Petro noted that planting a seedling is, like space exploration, an act of hope intended to bring fruit to future generations.
Learn more: https://www.nasa.gov/learning-resources/nasa-stem-artemis-moon-trees/
Dan Gallagher: Producer/Editor
Noah Petro: Scientist
John D. Philyaw: Videographer
Lonnie Shekhtman: Public Affairs
Caela Barry: Support
Staci Horvath: Support
Kathryn Mersmann: Support
Derrol Nail: Launch Commentator
Aaron E. Lepsch: Technical Support
Duration: 1 minute, 33 seconds
Release Date: Nov. 20, 2025
#NASA #Space #Science #Moon #ArtemisProgram #ArtemisI #OrionSpacecraft #TreeSeeds #NASASLS #SpaceLaunchSystem #DeepSpace #MoonToMars #SpaceEngineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAGoddard #GSFC #Greenbelt #Maryland #UnitedStates #STEM #Education #HD #Video
Celestial Lightsabers: Stellar Jets in Herbig-Haro Object 24 | Hubble Visualization
Celestial Lightsabers: Stellar Jets in Herbig-Haro Object 24 | Hubble Visualization
This sequence combines a two-dimensional zoom and a three-dimensional flight to explore Hubble’s striking image of the Herbig-Haro object known as HH24. This video starts with a night sky view of the Orion constellation and zooms in. Located above the left side of Orion’s Belt is the vast dark nebula called the Orion B molecular cloud complex. Within this molecular cloud are many bright regions where stars are forming. This video closes in toward one particularly energetic example.
The video then switches to an envisioned three-dimensional perspective. As the virtual camera flies into the dark nebula, the stars pass off-screen and the details of the forming stars and their jets of emission are revealed. The central star is hidden by gas and dust, but its prominent twin jets of emission resemble a cosmic, double-bladed lightsaber. These jets have carved an hourglass-shaped cavity in the near side of the nebula. The jet from another stellar newborn in this region has created a cylindrical tunnel through the gas extending to the left. Careful study of the Hubble data reveals a few other jets heating and displacing the gas and dust around them. The nebula provides a vivid example of a gas cloud shaped by stellar emission.
Acknowledgment: NASA, ESA, A. Fujii, Digitized Sky Survey (DSS), STScI/AURA, Palomar/Caltech, UKSTU/AAO, T. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOAO/AURA/NSF, Gemini Observatory/AURA/B. Reipurth, C. Aspin, and T. Rector, the Hubble Heritage (STScI/AURA)/Hubble-Europe (ESA) Collaboration, D. Padgett (GSFC), T. Megeath (University of Toledo), and B. Reipurth (University of Hawaii)
Duration: 1 minute
Release Date: Nov. 20, 2025
Thursday, November 20, 2025
Blue Origin New Glenn-2 Rocket & Reusable Booster: New Pictures
Blue Origin New Glenn-2 Rocket & Reusable Booster: New Pictures
On November 18, 2025, Blue Origin welcomed Jacklyn and its fully reusable New Glenn first stage back to the Space Coast.
A Blue Origin New Glenn-2 rocket successfully launched NASA's ESCAPADE Mars Mission on November 13, 2025. This was the second mission to date for the New Glenn rocket series. Blue Origin also landed its fully reusable New Glenn first stage booster on the drone ship Jacklyn in the Atlantic Ocean.
The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.
ESCAPADE is led by the UC Berkeley Space Sciences Laboratory. It is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron and ion electrostatic analyzers, plus science data processing and archiving.
Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).
https://escapade.ssl.berkeley.edu
Release Dates: Nov. 15-20, 2025
#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlennRocket #NewGlenn2 #Florida #UnitedStates #Infographics #STEM #Education
"Movie Night" | International Space Station
"Movie Night" | International Space Station
Expedition 73 Flight Engineer and NASA Astronaut Jonny Kim: "We work hard on the International Space Station, but we also like to relax together. Sometimes we do movie nights in space."
https://blogs.nasa.gov/spacestation/
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.
Release Date: Nov. 18, 2025
#NASA #Space #Astronomy #Science #Earth #ISS #MovieNights #Films #Entertainment #Astronauts #JonnyKim #AstronautPhotography #UnitedStates #Japan #日本 #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education
NASA's Artemis II Moon Rocket Fully Integrated | Kennedy Space Center
NASA's Artemis II Moon Rocket Fully Integrated | Kennedy Space Center
NASA’s Artemis II Orion crew spacecraft with its launch abort system was recently stacked atop the agency’s Space Launch System (SLS) rocket in High Bay 3 of the Vehicle Assembly Building (VAB) at NASA's Kennedy Space Center (KSC) in Florida. This milestone marks a huge step in the mission that will carry four astronauts on a 10-day mission around the Moon and back in early 2026.
Ahead of rolling out the integrated SLS rocket to the launch pad, teams will be conducting a series of verification tests.
Artemis II will officially launch "no earlier than April 2026."
#NASA #Space #Science #Earth #Moon #Artemis #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrewedMissions #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #LockheedMartin #Florida #UnitedStates #STEM #Education #HD #Video
The Apep Wolf-Rayet Binary Star System | Webb Visualization | STScI
The Apep Wolf-Rayet Binary Star System | Webb Visualization | STScI
This scientific visualization models what three of the four dust shells sent out by two Wolf-Rayet stars in the Apep system look like in 3D based on mid-infrared observations from NASA’s James Webb Space Telescope. Apep is made up of two Wolf-Rayet binary stars that are orbiting together with a third supergiant star. For 25 years during every 190-year orbit, the Wolf-Rayet stars’ winds collide, producing and sending out new waves of amorphous carbon dust. The width of the widest bubble is at least 4.6 light-years across.
Wolf-Rayet stars can be around 20 times as massive as our sun, but seem to be on a mission to shed surplus mass as quickly as possible—they blast substantial winds of particles out into space, causing them to dwindle at a rapid rate. A typical star of this type can lose a mass equal to that of our sun in just 100,000 years!
These massive stars are also incredibly hot, with surface temperatures some 10 to 40 times that of the sun, and very luminous, glowing at tens of thousands to several million times the brightness of the sun. Many of the brightest and most massive stars in the Milky Way are Wolf-Rayet stars.
Because these stars are so intense they do not last very long, burning up their fuel and blasting their bulk out into the cosmos on very short timescale—only a few hundred thousand years.
Image Processing: Alyssa Pagan (STScI)
Visualization: Christian Nieves (STScI)
Duration: 41 seconds
Release Date: Nov. 19, 2025
New View: A Pair of Wolf-Rayet Stars Named Apep | James Webb Space Telescope
New View: A Pair of Wolf-Rayet Stars Named Apep | James Webb Space Telescope
This new NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s mid-infrared image shows four coiled shells of dust around a pair of Wolf-Rayet stars known as Apep for the first time. Previous observations by other telescopes showed only one.
Webb’s data, combined with observations from the European Southern Observatory’s Very Large Telescope (VLT) in Chile, confirmed that the two Wolf-Rayet stars sail past one another approximately every 190 years. Over each orbit, they make a close pass for 25 years, producing and spewing amorphous carbon dust.
Wolf-Rayet stars can be around 20 times as massive as our sun, but seem to be on a mission to shed surplus mass as quickly as possible—they blast substantial winds of particles out into space, causing them to dwindle at a rapid rate. A typical star of this type can lose a mass equal to that of our sun in just 100,000 years!
These massive stars are also incredibly hot, with surface temperatures some 10 to 40 times that of the sun, and very luminous, glowing at tens of thousands to several million times the brightness of the sun. Many of the brightest and most massive stars in the Milky Way are Wolf-Rayet stars.
Because these stars are so intense they do not last very long, burning up their fuel and blasting their bulk out into the cosmos on very short timescale—only a few hundred thousand years.
Webb’s new data also confirmed that there are three stars gravitationally bound to one another in this system. Holes are “sliced” into these shells by the third star, a massive supergiant.
https://science.nasa.gov/missions/webb/webb-first-to-show-4-dust-shells-spiraling-apep-limits-long-orbit/
Image description: Four dust shells in Wolf-Rayet Apep expand away from three central stars that appear as a single pinpoint of light. The shells are curved, and the interior shell looks like a backward lowercase e shape.
Release Date: Nov. 19, 2025
#NASA #Astronomy #Space #Science #NASAWebb #Nebula #ApepNebula #BinaryStarSystems #Norma #Constellations #Astrophysics #Cosmos #Universe #UnfoldTheUniverse #JWST #NIRCam #InfraredAstronomy #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education
Wednesday, November 19, 2025
Blue Origin New Glenn-2 Reusable Rocket Booster Arrival Post-launch
Blue Origin New Glenn-2 Reusable Rocket Booster Arrival Post-launch
On November 18, 2025, Blue Origin welcomed Jacklyn and its fully reusable New Glenn first stage back to the Space Coast.
A Blue Origin New Glenn rocket successfully launched NASA's ESCAPADE Mars Mission on November 13, 2025. This was the second mission to date for the New Glenn rocket series. Blue Origin also landed the fully reusable New Glenn first stage booster on the drone ship Jacklyn in the Atlantic Ocean.
The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.
ESCAPADE is led by the UC Berkeley Space Sciences Laboratory. It is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron and ion electrostatic analyzers, plus science data processing and archiving.
Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).
https://escapade.ssl.berkeley.edu
Duration: 50 seconds
Release Date: Nov. 19, 2025
#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlennRocket #NewGlenn2 #Florida #UnitedStates #STEM #Education #HD #Video
NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center
NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center
NASA’s X-59 quiet supersonic research aircraft took to the skies for the first time Tuesday, Oct. 28, 2025, departing from Lockheed Martin’s Skunk Works facility in Palmdale, California, and arriving at NASA’s Armstrong Flight Research Center in Edwards, California. The milestone marks a major step for NASA’s Quesst mission and its goal of enabling quiet supersonic flight over land.
The X-59 aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.” Follow the X-59 team as they take on the exciting journey of building the X-59 and working toward quiet supersonic flight.
The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.
For more information about the X-59 and NASA's Quesst mission, visit www.nasa.gov/quesst
Video Credit: NASA's Armstrong Flight Research Center (AFRC)
Duration: 1 minute, 43 seconds
Release Date: Nov. 19, 2025
#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #Palmdale #Edwards #California #UnitedStates #STEM #Education #HD #Video
















.jpg)
.png)



















