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65 Years Ago: First Factory Rollout of the X-15 Hypersonic Rocket Plane


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On Oct. 15, 1958, the first X-15 hypersonic rocket-powered aircraft rolled out of its factory. A joint project among NASA, the U.S. Air Force, and the U.S. Navy, the X-15 greatly expanded our knowledge of flight at speeds exceeding Mach 6 and altitudes above 250,000 feet. Between 1959 and 1968, 12 pilots completed 199 missions, achieving ever-higher speeds and altitudes while gathering data on the aerodynamic and thermal performance of the aircraft flying to the edge of space and beyond and returning to Earth. The X-15 served as a platform for a series of experiments studying the unique hypersonic environment. The program experienced several mishaps and one fatal crash. Knowledge gained during X-15 missions influenced the development of future programs such as the space shuttle.

Rollout of the first X-15 hypersonic research rocket plane North American pilot A. Scott Crossfield poses in front of the X-15-1 Rear view of the X-15-1
Left: Rollout of the first X-15 hypersonic research rocket plane at the North American Aviation facility in Los Angeles. Middle: North American pilot A. Scott Crossfield poses in front of the X-15-1. Right: Rear view of the X-15-1, showing the twin XLR-11 rocket engines used on early test flights.

The origins of the X-15 date to 1952, when the Committee on Aerodynamics of the National Advisory Committee for Aeronautics (NACA) adopted a resolution to expand their research portfolio to study flight up to altitudes between 12 and 50 miles and Mach numbers between 4 and 10. The Air Force and Navy agreed and conducted joint feasibility studies at NACA’s field centers. On Dec. 30, 1954, the U.S. Air Force released a Request for Proposals (RPF) for aerospace firms to bid on building the experimental hypersonic aircraft. Four companies submitted proposals with the Air Force selecting North American Aviation, Los Angeles, as the winning bid on Sept. 30, 1955, awarding the contract in November. The Air Force held a separate competition for the aircraft’s XLR-99 rocket engine, a 57,000-pound throttleable single-chamber engine. The process began with release of the RFP on Feb. 4, 1955, and selection in February 1956 of the Reaction Motors Division of Thiokol Chemical Corporation. Delays in the development of the XLR-99 engine required North American to rely on a pair of four-nozzle XLR-11 engines, similar to the one that powered the X-1 on its historic sound-barrier breaking flight in 1947. Providing only 16,000 pounds of thrust, this left the X-15 significantly underpowered for the first 17 months of test flights. On Oct. 1, 1958, the new National Aeronautics and Space Administration (NASA) incorporated the NACA centers and inherited the X-15 project, just two weeks before rollout from the factory of the first flight article.

Crowds gather to admire the first X-15 after its rollout from the North American Aviation plant Workers at Edwards Air Force Base in California lift the first X-15 off its delivery truck
Left: Crowds gather to admire the first X-15 after its rollout from the North American Aviation plant in Los Angeles. Right: Workers at Edwards Air Force Base in California lift the first X-15 off its delivery truck.

On Oct. 15, 1958, the rollout of the first of the three aircraft took place with some fanfare at North American’s Los Angeles facility. Vice President Richard M. Nixon and news media attended the festivities, as did North American X-15 project manager Harrison A. “Stormy” Storms and several of the early X-15 pilots. After the conclusion of the ceremonies, workers wrapped the aircraft, placed it on a flatbed truck, and drove it overnight to the High Speed Flight Station, today NASA’s Armstrong Flight Research Center, at Edwards Air Force Base (AFB) in California’s Mojave Desert. Even before this first aircraft took to the skies, North American rolled out X-15-2 on Feb. 27, 1959. The third aircraft, equipped with the LR-99 engine and a more advanced adaptive flight control system, rounded out the small fleet in 1960.

Diagram showing the two main profiles used by the X-15, either for altitude or speed The twin XLR-11 engines and the more powerful XLR-99 engine used to power the X-15
Left: Diagram showing the two main profiles used by the X-15, either for altitude or speed. Right: The twin XLR-11 engines, left, and the more powerful XLR-99 engine used to power the X-15.

Like earlier X-planes, a carrier aircraft, in this case two modified B-52 Stratofortresses, released the 34,000-pound X-15 at an altitude of 45,000 feet to conserve its fuel for the research mission. Flights took place within the High Range, extending from Wendover AFB in Utah to the Rogers Dry Lake landing zone adjacent to Edwards AFB, with emergency landing zones along the way. Typical missions lasted eight to 12 minutes and followed either a high-altitude or a high-speed profile following launch from the B-52 and ignition of the rocket engine. After burnout of the engine, the pilot guided the aircraft to an unpowered landing on the lakebed runway. To withstand the high temperatures during hypersonic flight and reentry, the X-15’s outer skin consisted of a then-new nickel-chrome alloy called Inconel-X. Because traditional aerodynamic surfaces used for flight control while in the atmosphere do not work in the near vacuum of space, the X-15 used its Ballistic Control System thrusters for attitude control while flying outside the atmosphere. North American pilot A. Scott Crossfield had the primary responsibility for carrying out the initial test flights of the X-15 before handover to NASA and the Air Force.

The first captive flight of the X-15-1 rocket plane takes off under the wing of its B-52 Stratofortress carrier aircraft X-15-1 begins its first unpowered glide flight
Left: With North American Aviation pilot A. Scott Crossfield in the cockpit, the first captive flight of the X-15-1 rocket plane takes off under the wing of its B-52 Stratofortress carrier aircraft. Right: Seconds after release from the B-52, with Crossfield at the controls, the X-15-1 begins its first unpowered glide flight.

With Crossfield at the controls of X-15-1, the first captive flight during which the X-15 remained attached to the B-52’s wing, took place on March 10, 1959. Crossfield completed the first unpowered glide flight of an X-15 on June 8, the flight lasting just five minutes. On Sept. 17, at the controls of X-15-2, Crossfield completed the first powered flight of an X-15, reaching a speed of Mach 2.11 and an altitude of 52,000 feet. Overcoming a few hardware problems, he brought the aircraft to a successful landing after a flight lasting nine minutes. During 12 more flights, Crossfield expanded the aircraft’s flight envelope to Mach 2.97 and 88,116 feet while gathering important data on its flying characteristics. All except his last three flights used the lower thrust LR-11 engines, limiting the aircraft’s speed and altitude. The last three used the powerful LR-99 engine, the one the aircraft was designed for. Crossfield’s 14th flight on Dec. 6, 1960, marked the end of North American’s contracted testing program, turning the X-15 over to the Air Force and NASA.

Chief NASA X-15 pilot Joseph A. “Joe” Walker launches from the B-52 carrier aircraft to begin his first flight Walker following his altitude record-setting flight in 1963 Walker at the controls of the Lunar Landing Research Vehicle in 1964
Left: Chief NASA X-15 pilot Joseph A. “Joe” Walker launches from the B-52 carrier aircraft to begin his first flight. Middle: Walker following his altitude record-setting flight in 1963. Right: Walker at the controls of the Lunar Landing Research Vehicle in 1964.

On March 25, 1960, NASA’s chief X-15 pilot Joseph A. “Joe” Walker, completed the agency’s first flight aboard X-15-1. Walker, one of five NASA pilots to fly the X-15, completed 25 flights aboard the aircraft. On May 12, 1960, Walker took X-15-1 above Mach 3 for the first time. On two of his flights, Walker exceeded the Von Karman line, the internationally recognized boundary of space of 100 kilometers, or 62 miles, earning him astronaut wings. On a third flight, he flew above 50 miles, the altitude the Air Force considered the boundary of space. By that standard, 13 flights by eight X-15 pilots qualified them for Air Force astronaut wings. On Walker’s final flight on Aug. 22, 1963, he flew X-15-3 to an altitude of 354,200 feet, or 67.1 miles, the highest achieved in the X-15 program, and a record for piloted aircraft that stood until surpassed during the final flight of SpaceShipOne on Oct. 4, 2004. After leaving the X-15 program, Walker conducted 35 test flights of the Lunar Landing Research Vehicle (LLRV) between 1964 and 1966, the precursor to the Lunar Landing Training Vehicle that Apollo commanders used to simulate the final several hundred feet of the Lunar Module’s descent to the lunar surface. Tragically, Walker died in a mid-air collision on June 8, 1966, when his F-104 Starfighter struck an XB-70 Valkyrie during a demonstration exercise.

NASA X-15 pilot John B. “Jack” McKay poses with X-15-3 after a mission Rollout of X-15A-2 in 1964, repaired and modified following a landing mishap.
Left: NASA X-15 pilot John B. “Jack” McKay poses with X-15-3 after a mission. Middle: Rollout of X-15A-2 in 1964, repaired and modified following a landing mishap.

The second NASA X-15 pilot, John B. “Jack” McKay completed 29 flights, the most of any NASA pilot. He achieved a maximum speed of Mach 5.65 and reached an altitude of 295,600 feet, qualifying him for Air Force astronaut wings. On Nov. 9, 1962, he suffered serious injuries during a landing mishap on his seventh mission but recovered to make 22 more flights. Engineers at North American not only repaired the damaged X-15-2 but redesignated it as X-15A-2. They extended its fuselage by more than two feet and added two external fuel tanks to enable longer engine burns. McKay made another emergency landing on his 25th flight on May 6, 1966, when the X-15-1’s LR-99 engine shut down prematurely. The aircraft did not incur any damage and McKay suffered no injuries.

NASA pilot Neil A. Armstrong stands next to an X-15 Armstrong sits in Gemini VIII prior to liftoff Armstrong in the Apollo 11 Lunar Module Eagle following his historic Moon walk
Left: NASA pilot Neil A. Armstrong stands next to an X-15. Middle: Armstrong sits in Gemini VIII prior to liftoff. Right: Armstrong in the Apollo 11 Lunar Module Eagle following his historic Moon walk.

Neil A. Armstrong joined NACA as an experimental test pilot in January 1952, and gained experience flying the X-1B supersonic rocket plane. NACA selected him as its third X-15 pilot, and he flew the aircraft seven times. After his first two checkout flights in December 1960, Armstrong spent a year as a consultant on the X-20 Dyna-Soar program before returning to fly his remaining five X-15 missions. Because he helped to develop the adaptive flight control system, on Dec. 20, 1961, Armstrong completed the first flight of X-15-3, rebuilt after an explosion in June 1960 of the LR-99 engine on a test stand destroyed the back of the aircraft. On his sixth flight on April 20, 1962, while trying to maintain a constant g-load during reentry, the aircraft’s attitude caused it to skip out of the atmosphere. This resulted in an overshoot of the landing zone, requiring a high-altitude U-turn, with Armstrong just barely reaching the lakebed runway. Armstrong left the X-15 program when NASA selected him as an astronaut on Sept. 17, 1962. In March 1966, as the Gemini VIII Command Pilot, he executed the first docking in space and then guided the spacecraft back to Earth after the first in-space emergency. On July 20, 1969, during Apollo 11, Armstrong took humanity’s first step on the Moon.

NASA pilot Milton O. Thompson poses in front of X-15-3 Thompson poses in front of the M2-F2 lifting body aircraft after his first flight in 1966
Left: NASA pilot Milton O. Thompson poses in front of X-15-3. Right: Thompson poses in front of the M2-F2 lifting body aircraft after his first flight in 1966.

In June 1963, NASA selected Milton O. “Milt” Thompson as an X-15 pilot, and he completed 14 flights. Although he achieved a maximum speed of Mach 5.48 and reached 214,100 feet, more than half his flights remained at relatively low altitude but high speed to gather data on the effects of high temperatures on the skin of the X-15. Thompson transferred to test fly the experimental M2-F2 lifting body aircraft before giving up flying to manage advanced research projects for NASA, including influencing the design of the space shuttle orbiter. His X-15 experience convinced him that the orbiter did not need jet engines to assist in the landing. Thompson served as the chief engineer at NASA’s Dryden Flight Reseach Center, now Armstrong Flight Research Center, from 1975 until his death in 1993.

NASA pilot William “Bill” Dana poses in front of X-15-3 Dana after the final rocket powered aircraft flight, aboard the X-24B, at Edwards Air Force Base in 1975.
Left: NASA pilot William “Bill” Dana poses in front of X-15-3. Right: Dana after the final rocket powered aircraft flight, aboard the X-24B, at Edwards Air Force Base in 1975.

In May 1965, NASA selected William “Bill” H. Dana, already involved in the program as a chase pilot and simulation engineer, to backfill Thompson as an X-15 pilot. Dana completed 16 flights including what turned out to be the final flight of the X-15 program on Oct. 24, 1968. He reached a maximum speed of Mach 5.53 and an altitude of 306,900 feet, high enough to qualify him for Air Force astronaut wings. With the program sufficiently mature, in addition to gathering flight characteristics data, several experiments flew aboard Dana’s flights. On the last mission, Dana observed a Minuteman missile launch from Vandenberg Air Force Base. Following the end of the X-15 program, between April 1969 and December 1972, Dana piloted experimental lifting body aircraft like the HL-10 and M2-F3, and in September 1975, he flew the X-24B twice, including the final flight of a rocket-powered aircraft at Edwards. After test flying other aircraft, he served as Dryden’s chief engineer between 1993 and 1998, taking over from Thompson.

U.S. Air Force pilot Robert M. White after the last flight of an X-15 with the LR-11 engines White inside the X-15 about to launch on the first flight above Mach 6
Left: U.S. Air Force pilot Robert M. White after the last flight of an X-15 with the LR-11 engines. Right: White inside the X-15 about to launch on the first flight above Mach 6.

Five U.S. Air Force and one U.S. Navy pilot made history flying the X-15. The U.S. Air Force selected Iven C. “Kinch” Kincheloe as their first X-15 pilot, but tragically he died in an aircraft accident on July 26, 1958, before making a flight. His backup, Robert M. White, stepped in as the first Air Force pilot to fly the X-15, completing 16 missions. Over the course of these missions, White’s achievements included the first flight of an X-15 above 100,000 feet, then 200,000 feet, and eventually to 314,750 feet. That earned White U.S. Air Force astronaut wings on his July 17, 1962, flight. He also broke speed records, as the first person to fly faster than Mach 4, then Mach 5, and finally reaching Mach 6.04 – more than doubling the speed record in just eight months. After leaving the X-15 program, White flew combat missions in southeast Asia, the only X-15 pilot to see active duty in World War II, Korea, and Vietnam. He retired as a major general in 1981.

U.S. Navy pilot Forrest S. “Pete” Petersen poses next to an X-15 The B-52 carrier aircraft flies overhead to salute Petersen’s highest and fastest flight
Left: U.S. Navy pilot Forrest S. “Pete” Petersen poses next to an X-15. Right: The B-52 carrier aircraft flies overhead to salute Petersen’s highest and fastest flight.

Air Force pilot Robert A. Rushworth following a flight aboard X-15-3 photograph of two B-52s preparing to launch two X-15s in November 1960
Left: Air Force pilot Robert A. Rushworth following a flight aboard X-15-3. Right: Unusual photograph of two B-52s preparing to launch two X-15s in November 1960 – X-15-1 prepares to taxi for Rushworth’s first flight, left, and X-15-2 for A. Scott Crossfield and the first flight of the XLR-99 rocket engine. Image credit: courtesy mach25media.com.

The pilot with the most X-15 missions, the Air Force’s Robert A. Rushworth completed 34 flights. For the first time, flight surgeons could monitor a pilot’s electrocardiogram in real time thanks to a new biomonitoring system and did so during Rushworth’s seventh flight. On his 14th flight, Rushworth reached an altitude of 285,000 feet, high enough to earn him U.S. Air Force astronaut wings. Rushworth flew his fastest flight on Dec. 5, 1963, when he reached a top speed of Mach 6.06. On June 25, on his 21st mission, Rushworth completed the first flight of X-15A-2, rebuilt and upgraded following its November 1962 crash. He piloted it to Mach 4.59, the first time the aircraft flew faster than Mach 4. On his next flight, he took the aircraft past Mach 5. On his 34th and final mission, Rushworth tested one of the significant upgrades to X-15A-2, the addition of disposable external fuel and oxidizer tanks to increase the rocket engine’s burn time. He encountered some difficulties when he jettisoned the tanks at the half-full stage, a condition that planners had not anticipated, but successfully landed the aircraft. As previously planned, Rushworth left the X-15 program five days later, attending the National War College before flying 189 combat missions in Vietnam. He retired as a major general in 1981.

Air Force pilot Joe H. Engle following a flight aboard X-15A-2 NASA astronaut Engle poses in front of space shuttle Enterprise during its first rollout in 1976 Engle during Columbia’s STS-2 mission in November 198
Left: Air Force pilot Joe H. Engle following a flight aboard X-15A-2. Middle: NASA astronaut Engle poses in front of space shuttle Enterprise during its first rollout in 1976. Right: Engle during Columbia’s STS-2 mission in November 1981.

Air Force pilot Joe H. Engle joined the X-15 program in June 1963, completing 16 missions. He achieved his highest speed, Mach 5.71, on his 10th flight, and earned his U.S. Air Force astronaut wings at 33 years of age, the youngest X-15 pilot to do so, on his 14th flight. Within less than four months, Engle surpassed the 50-mile mark two more times on his final two X-15 flights in August and October 1965. Engle left the X-15 program when NASA selected him as an astronaut on April 4, 1966. Putting his X-15 experience to good use, he commanded two of the five Approach and Landing Tests with space shuttle Enterprise in 1977. In 1982, he commanded STS-2, the second orbital flight of Columbia, and in 1985 he commanded STS-51I, the sixth flight of Discovery. Comparing the X-15 and the space shuttle, the only person to have piloted both said, “From a pilot-task standpoint, the entry and landing are very similar, performance wise. You fly roughly the same glide speed and the same glide slope angle. The float and touchdown were very similar.” Engle retired from NASA and the Air Force as a major general in 1986 but remained active in an advisory capacity into the 2010s.

Air Force pilot William J. “Pete” Knight poses with X-15A-2 with its unusual white outer paint over an ablative coating Knight, right, following his speed record-setting flight in October 1967
Left: Air Force pilot William J. “Pete” Knight poses with X-15A-2 with its unusual white outer paint over an ablative coating. Right: Knight, right, following his speed record-setting flight in October 1967.

The Air Force selected William J. “Pete” Knight as an X-15 pilot in 1965, and he completed 16 flights in two years. On his eighth flight on Nov. 18, 1966, Knight took X-15A-2 to above Mach 6, with the fully fueled external tanks operating as expected. In an attempt to protect the X-15’s skin during sustained flight at Mach 6, or proposed future flights at Mach 7 and 8, engineers coated X-15A-2 with an ablative material. Since the color of the material resembled the pink of a pencil eraser, workers painted it a gleaming white. On Oct. 3, 1967, Knight flew X-15A-2, with fully fueled external tanks, to an unofficial speed record of Mach 6.70, or 4,520 miles per hour, for a piloted winged vehicle. The mark stood until surpassed during the reentry of space shuttle Columbia on April 14, 1981. While the flight appeared to have gone well, hypersonic shock waves, especially around a model scramjet attached to the bottom rear of the aircraft, caused such heating that it burned through the ablative material, exposing the skin of the aircraft to 2,400 degrees, twice its design limit. Postflight inspection revealed significant damage to the aircraft that would have ended catastrophically had the heating continued for a few more seconds. A previous flight to Mach 6.33 showed similar, although less, severe damage, but engineers did not consider it as a warning sign. Due to the damage, X-15A-2 never flew again. In 2003, space shuttle Columbia suffered similar burn, caused by damage to its thermal protection system, leading to loss of the vehicle and its seven-member crew. When the X-15 program ended at the end of 1968, Knight returned to active duty, flying 253 combat missions in Vietnam in 1969 and 1970. He eventually returned to Edwards as its vice commander before retiring in 1982 and entering politics.

Michael J. Adams, left, selected in the first group of astronauts for the U.S. Air Force’s Manned Orbiting Laboratory in 1965 Adams following a mission aboard X-15-1
Left: Michael J. Adams, left, selected in the first group of astronauts for the U.S. Air Force’s Manned Orbiting Laboratory in 1965. Right: Adams following a mission aboard X-15-1.

The U.S. Air Force first selected Michael J. Adams as an astronaut for the Manned Orbiting Laboratory program in November 1965 before transferring him to the X-15 program in July 1966 as its 12th and final pilot. He flew the X-15 seven times and on his third flight reached his highest speed of Mach 5.59. Adams took off on his seventh flight on Nov. 15, 1967, a mission using X-15-3 with its advanced flight control system, to reach 250,000 feet and Mach 6 to conduct several experiments. After overshooting to a peak altitude of 266,000 feet and beginning the descent but sill well outside the atmosphere, the X-15-3 entered into a hypersonic spin traveling at more than 3,000 miles per hour, at one point flying tail first. Adams and the aircraft’s systems recovered from the spin, but now the aircraft began serious pitch oscillations as it continued to fall. At 62,000 feet, the g-loads from the oscillations overcame the structural limits of the aircraft and it broke apart. The X-15-3 crashed, killing Adams. The accident investigation identified proximate causes as a short-circuit from one of the experiments that had not been tested at low atmospheric pressures or high temperatures, causing both the aircraft’s computer and its flight control system to repeatedly fail. Adams became distracted and did not realize his aircraft’s attitude was increasingly off nominal. In addition, an attitude indicator switch had been set at the wrong setting, providing Adams with confusing information. Telemetry to the ground did not include attitude information, so controllers did not know the problems Adams faced and could not provide any helpful direction. Adams may have suffered from vertigo, a condition for which he had previously tested positive, a fact not known to his flight surgeon. Two major changes from the accident included adding attitude information to the telemetry and ensuring that all pilots received thorough vestibular screening to identify cases of vertigo. With the loss of X-15-3 and the retirement of the damaged X-15A-2 following Knight’s October flight, only one aircraft, the original X-15-1, remained to close out the program until funding ran out in December 1968. The Air Force posthumously honored Adams with astronaut wings.

The Edwards Air Force Base ground crew poses in front of the B-52 with X-15-1 mounted under its wing during a rare snowstorm that thwarted a final attempt at a 200th flight
The Edwards Air Force Base ground crew poses in front of the B-52 with X-15-1 mounted under its wing during a rare snowstorm that thwarted a final attempt at a 200th flight.

NASA pilot Dana flew what turned out to be the 199th and final X-15 mission on Oct. 24, 1968. Managers tried to fly a 200th mission before funding ran out on Dec. 31. Eight attempts between Nov. 27 and Dec. 20 for Air Force pilot Knight to take X-15-1 on a final mission failed for a variety of reasons. Due to the delays, the initial mission plan of flying to 250,000 feet at Mach 4.9 in an attempt to visualize a missile launch from Vandenberg AFB had to change to a more modest altitude goal of 162,000 feet and reduced speed of Mach 3.9 to test a new experiment. On Dec. 20, with Knight suited up and ready to board the X-15, a rare snowstorm put an end to any plans to fly, and so the program ended. The next morning, on the other side of the continent, a Saturn V lifted off from NASA’s Kennedy Space Center in Florida to take Apollo 8 astronauts on the first voyage to the Moon. Seven months later, former NASA X-15 pilot Armstrong took humanity’s first steps on the Moon.

Summary of X-15 pilots’ accomplishments.
Summary of X-15 pilots’ accomplishments.

A grateful nation recognized the accomplishments of the X-15 pilots. On Nov. 28, 1961, in a White House ceremony President John F. Kennedy presented Crossfield, Walker, and White with the Harmon International Trophy for Aviators. On July 18, 1962, President Kennedy presented the prestigious Robert J. Collier Trophy to Crossfield, Walker, White, and Petersen for their pioneering hypersonic flights. On Dec. 3, 1968, President Lyndon B. Johnson presented the Harmon Trophy to Knight for his Mach 6.70 record-setting flight.

President John F. Kennedy, left, presents the Harmon Trophy to X-15 pilots A. Scott Crossfield of North American Aviation, Joseph A. Walker of NASA, and Robert White of the U.S. Air Force President Kennedy presents the Collier Trophy to X-15 pilots Crossfield, White, Walker, and Forrest S. Petersen of the U.S. Navy President Lyndon B. Johnson presents the Harmon Trophy to U.S. Air Force X-15 pilot William J. “Pete” Knight
Left: President John F. Kennedy, left, presents the Harmon Trophy to X-15 pilots A. Scott Crossfield of North American Aviation, Joseph A. Walker of NASA, and Robert White of the U.S. Air Force. Middle: President Kennedy presents the Collier Trophy to X-15 pilots Crossfield, White, Walker, and Forrest S. Petersen of the U.S. Navy. Right: President Lyndon B. Johnson presents the Harmon Trophy to U.S. Air Force X-15 pilot William J. “Pete” Knight.

The X-15-1 as it looked in the Milestones of Flight exhibit at the Smithsonian Institute’s National Air and Space Museum in Washington, D.C The X-15A-2 on display at the National Museum of the Air Force at Wright-Patterson Air Force Base (AFB), in Dayton, Ohio A replica of the X-15-3 as it looked on display in 1997 outside the entrance to NASA’s Dryden, now Armstrong, Flight Research Center at Edwards AFB.
Left: The X-15-1 as it looked in the Milestones of Flight exhibit at the Smithsonian Institute’s National Air and Space Museum in Washington, D.C. Image credit: courtesy National Air and Space Museum. Middle: The X-15A-2 on display at the National Museum of the Air Force at Wright-Patterson Air Force Base (AFB), in Dayton, Ohio. Image credit: courtesy National Museum of the Air Force. Right: A replica of the X-15-3 as it looked on display in 1997 outside the entrance to NASA’s Dryden, now Armstrong, Flight Research Center at Edwards AFB.

Following the end of the program, the two surviving X-15 aircraft found permanent homes in prestigious museums. The X-15-1 arrived at the Smithsonian Institution in Washington, D.C., in June 1969. When the new National Air and Space Museum opened in July 1976, the X-15-1 found a place of prominence in the Milestones of Flight exhibit. In 2019, curators placed it in temporary storage while the museum undergoes a major renovation. The X-15A-2 went on display at the Air Force Museum, now the National Museum of the Air Force at Wright-Patterson AFB, in Dayton, Ohio, where it still resides. Although the third aircraft was lost in a crash, North American built replica of X-15-3 that was mounted outside the entrance to Dryden in 1995. Damage from winds required its removal and refurbishment, and it is currently in storage at Armstrong.

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      How fast is the universe expanding? It’s hard to say because different ways of calculating the current expansion rate yield different results — a dilemma known as the Hubble Tension. Are these differences just a result of measurement errors, or is there something weird going on in the universe? So far, Webb data indicates that the Hubble Tension is not caused by measurement errors. Webb was able to distinguish pulsating stars from nearby stars in a crowded field, ensuring that the measurements weren’t contaminated by extra light. Webb also discovered a distant, gravitationally lensed supernova whose image appears in three different locations and at three different times during its explosion. Calculating the expansion rate based on the brightness of the supernova at these three different times provides an independent check on measurements made using other techniques. Until the matter of the Hubble Tension is settled, Webb will continue measuring different objects and exploring new methods.
      4. Webb has found surprisingly rich and varied atmospheres on gas giants orbiting distant stars.
      While NASA’s Hubble Space Telescope made the first detection of gases in the atmosphere of a gas giant exoplanet (a planet outside our solar system), Webb has taken studies to an entirely new level. Webb has revealed a rich cocktail of chemicals, including hydrogen sulfide, ammonia, carbon dioxide, methane, and sulfur dioxide — none of which had been clearly detected in an atmosphere outside our solar system before. Webb has also been able to examine exotic climates of gas giants as never before, detecting flakes of silica “snow” in the skies of the puffy, searing-hot gas giant WASP-17 b, for example, and measuring differences in temperature and cloud cover between the permanent morning and evening skies of WASP-39 b.
      Image: Spectrum of WASP-107 b
      A transmission spectrum of the “warm Neptune” exoplanet WASP-107 b captured by NASA’s Hubble and Webb space telescopes, shows clear evidence for water, carbon dioxide, carbon monoxide, methane, sulfur dioxide, and ammonia in the planet’s atmosphere. These measurements allowed researchers to estimate the interior temperature and mass of the core of the planet, as well as understand the chemistry and dynamics of the atmosphere. NASA, ESA, CSA, Ralf Crawford (STScI) 5. A rocky planet 40 light-years from Earth may have an atmosphere fed by gas bubbling up from its lava-covered surface.
      Detecting, let alone analyzing, a thin layer of gas surrounding a small rocky planet is no easy feat, but Webb’s extraordinary ability to measure extremely subtle changes in the brightness of infrared light makes it possible. So far, Webb has been able to rule out significant atmosphere on a number of rocky planets, and has found tantalizing signs of carbon monoxide or carbon dioxide on 55 Cancri e, a lava world that orbits a Sun-like star. With findings like these, Webb is laying the groundwork for NASA’s future Habitable Worlds Observatory, which will be the first mission purpose-built to directly image and search for life on Earth-like planets around Sun-like stars.
      6. Webb exposes the skeletal structure of nearby spiral galaxies in mesmerizing detail.
      We already knew that galaxies are collections of stars, planets, dust, gas, dark matter, and black holes: cosmic cities where stars form, live, die, and are recycled into the next generation. But we had never been able to see the structure of a galaxy and the interactions between stars and their environment in such detail. Webb’s infrared vision reveals filaments of dust that trace the spiral arms, old star clusters that make up galactic cores, newly forming stars still encased in dense cocoons of glowing dust and gas, and clusters of hot young stars carving enormous cavities in the dust. It also elucidates how stellar winds and explosions actively reshape their galactic homes.
      Image: PHANGS Phantom Galaxy (M74/NGC 628)
      A near- to mid-infrared image from NASA’s James Webb Space Telescope highlights details in the complex structure of a nearby galaxy that are invisible to other telescopes. The image of NGC 628, also known as the Phantom Galaxy, shows spiral arms with lanes of warm dust (represented in red), knots of glowing gas (orange-yellow), and giant bubbles (black) carved by hot, young stars. The dust-free core of the galaxy is filled with older, cooler stars (blue). NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS team 7. It can be hard to tell the difference between a brown dwarf and a rogue planet.
      Brown dwarfs form like stars, but are not dense or hot enough to fuse hydrogen in their cores like stars do. Rogue planets form like other planets, but have been ejected from their system and no longer orbit a star. Webb has spotted hundreds of brown-dwarf-like objects in the Milky Way, and has even detected some candidates in a neighboring galaxy. But some of these objects are so small — just a few times the mass of Jupiter — that it is hard to figure out how they formed. Are they free-floating gas giant planets instead? What is the least amount of material needed to form a brown dwarf or a star? We’re not sure yet, but thanks to three years of Webb observations, we now know there is a continuum of objects from planets to brown dwarfs to stars.
      8. Some planets might be able to survive the death of their star.
      When a star like our Sun dies, it swells up to form a red giant large enough to engulf nearby planets. It then sheds its outer layers, leaving behind a super-hot core known as a white dwarf. Is there a safe distance that planets can survive this process? Webb might have found some planets orbiting white dwarfs. If these candidates are confirmed, it would mean that it is possible for planets to survive the death of their star, remaining in orbit around the slowly cooling stellar ember.
      9. Saturn’s water supply is fed by a giant fountain of vapor spewing from Enceladus.
      Among the icy “ocean worlds” of our solar system, Saturn’s moon Enceladus might be the most intriguing. NASA’s Cassini mission first detected water plumes coming out of its southern pole. But only Webb could reveal the plume’s true scale as a vast cloud spanning more than 6,000 miles, about 20 times wider than Enceladus itself. This water spreads out into a donut-shaped torus encircling Saturn beyond the rings that are visible in backyard telescopes. While a fraction of the water stays in that ring, the majority of it spreads throughout the Saturnian system, even raining down onto the planet itself. Webb’s unique observations of rings, auroras, clouds, winds, ices, gases, and other materials and phenomena in the solar system are helping us better understand what our cosmic neighborhood is made of and how it has changed over time.
      Video: Water plume and torus from Enceladus
      A combination of images and spectra captured by NASA’s James Webb Space Telescope show a giant plume of water jetting out from the south pole of Saturn’s moon Enceladus, creating a donut-shaped ring of water around the planet.
      Credit: NASA, ESA, CSA, G. Villanueva (NASA’s Goddard Space Flight Center), A. Pagan (STScI), L. Hustak (STScI) 10. Webb can size up asteroids that may be headed for Earth.
      In 2024 astronomers discovered an asteroid that, based on preliminary calculations, had a chance of hitting Earth. Such potentially hazardous asteroids become an immediate focus of attention, and Webb was uniquely able to measure the object, which turned out to be the size of a 15-story building. While this particular asteroid is no longer considered a threat to Earth, the study demonstrated Webb’s ability to assess the hazard.
      Webb also provided support for NASA’s Double Asteroid Redirection Test (DART) mission, which deliberately smashed into the Didymos binary asteroid system, showing that a planned impact could deflect an asteroid on a collision course with Earth. Both Webb and Hubble observed the impact, serving witness to the resulting spray of material that was ejected. Webb’s spectroscopic observations of the system confirmed that the composition of the asteroids is probably typical of those that could threaten Earth.
      —-
      In just three years of operations, Webb has brought the distant universe into focus, revealing unexpectedly bright and numerous galaxies. It has unveiled new stars in their dusty cocoons, remains of exploded stars, and skeletons of entire galaxies. It has studied weather on gas giants, and hunted for atmospheres on rocky planets. And it has provided new insights into the residents of our own solar system.
      But this is only the beginning. Engineers estimate that Webb has enough fuel to continue observing for at least 20 more years, giving us the opportunity to answer additional questions, pursue new mysteries, and put together more pieces of the cosmic puzzle.
      For example: What were the very first stars like? Did stars form differently in the early universe? Do we even know how galaxies form? How do stars, dust, and supermassive black holes affect each other? What can merging galaxy clusters tell us about the nature of dark matter? How do collisions, bursts of stellar radiation, and migration of icy pebbles affect planet-forming disks? Can atmospheres survive on rocky worlds orbiting active red dwarf stars? Is Uranus’s moon Ariel an ocean world?
      As with any scientific endeavor, every answer raises more questions, and Webb has shown that its investigative power is unmatched. Demand for observing time on Webb is at an all-time high, greater than any other telescope in history, on the ground or in space. What new findings await?
      By Dr. Macarena Garcia Marin and Margaret W. Carruthers, Space Telescope Science Institute, Baltimore, Maryland
      Media Contacts
      Laura Betz – laura.e.betz@nasa.gov
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Christine Pulliam – cpulliam@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
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      Last Updated Jul 02, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
      James Webb Space Telescope (JWST) Astrophysics Black Holes Brown Dwarfs Exoplanet Science Exoplanets Galaxies Galaxies, Stars, & Black Holes Goddard Space Flight Center Nebulae Science & Research Star-forming Nebulae Stars Studying Exoplanets The Universe View the full article
    • By NASA
      NASA astronaut Anil Menon poses for a portrait at NASA’s Johnson Space Center in Houston. Credit: NASA/Josh Valcarcel NASA astronaut Anil Menon will embark on his first mission to the International Space Station, serving as a flight engineer and Expedition 75 crew member.
      Menon will launch aboard the Roscosmos Soyuz MS-29 spacecraft in June 2026, accompanied by Roscosmos cosmonauts Pyotr Dubrov and Anna Kikina. After launching from the Baikonur Cosmodrome in Kazakhstan, the trio will spend approximately eight months aboard the orbiting laboratory.
      During his expedition, Menon will conduct scientific investigations and technology demonstrations to help prepare humans for future space missions and benefit humanity.
      Selected as a NASA astronaut in 2021, Menon graduated with the 23rd astronaut class in 2024. After completing initial astronaut candidate training, he began preparing for his first space station flight assignment.
      Menon was born and raised in Minneapolis and is an emergency medicine physician, mechanical engineer, and colonel in the United States Space Force. He holds a bachelor’s degree in neurobiology from Harvard University in Cambridge, Massachusetts, a master’s degree in mechanical engineering, and a medical degree from Stanford University in California. Menon completed his emergency medicine and aerospace medicine residency at Stanford and the University of Texas Medical Branch in Galveston.
      In his spare time, he still practices emergency medicine at Memorial Hermann’s Texas Medical Center and teaches residents at the University of Texas’ residency program. Menon served as SpaceX’s first flight surgeon, helping to launch the first crewed Dragon spacecraft on NASA’s SpaceX Demo-2 mission and building SpaceX’s medical organization to support humans on future missions. He served as a crew flight surgeon for both SpaceX flights and NASA expeditions aboard the space station.
      For nearly 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and conducting critical research for the benefit of humanity and our home planet. Space station research supports the future of human spaceflight as NASA looks toward deep space missions to the Moon under the Artemis campaign and in preparation for future human missions to Mars, as well as expanding commercial opportunities in low Earth orbit and beyond. 
      Learn more about International Space Station at:
      https://www.nasa.gov/station
      -end-
      Joshua Finch / Jimi Russell
      Headquarters, Washington
      202-358-1100
      joshua.a.finch@nasa.gov / james.j.russell@nasa.gov

      Shaneequa Vereen
      Johnson Space Center, Houston
      281-483-5111
      shaneequa.y.vereen@nasa.gov   
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      Last Updated Jul 01, 2025 LocationNASA Headquarters Related Terms
      Astronauts Humans in Space International Space Station (ISS) ISS Research View the full article
    • By European Space Agency
      While satellites have revolutionised our ability to measure sea level with remarkable precision, their data becomes less reliable near coasts – where accurate information is most urgently needed. To address this critical gap, ESA’s Climate Change Initiative Sea Level Project research team has reprocessed almost two decades of satellite data to establish a pioneering network of ‘virtual’ coastal stations. These stations now provide, for the first time, reliable and consistent sea-level measurements along coastlines. 
      View the full article
    • By Space Force
      Col. Nick Hague, the first Guardian to launch into space, visited Vandenberg Space Force Base.

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    • By NASA
      Ozone high in the stratosphere protects us from the Sun’s ultraviolet light. But ozone near the ground is a pollutant that harms people and plants. The San Joaquin Valley has some of the most polluted air in the country, and NASA scientists with the new Ozone Where We Live (OWWL) project are working to measure ozone and other pollutants there. They need your help!  
      Do you live or work in Bakersfield, CA? Sign up to host an ozone sensor! It’s like a big lunch box that you place in your yard, but it’s not packed with tuna and crackers. It’s filled with sensors that measure temperature and humidity and sniff out dangerous gases like methane, carbon monoxide, carbon dioxide, and of course, ozone. 
      Can you fly a plane? Going to the San Joaquin Valley? Sign up to take an ozone sensor on your next flight! You can help measure ozone levels in layers of the atmosphere that are hard for satellites to investigate. Scientists will combine the data you take with data from NASA’s TEMPO satellite to improve air quality models and measurements within the region. Find out more here or email: Emma.l.yates@nasa.gov
      Join the Ozone Where We Live (OWWL) project and help NASA scientists protect the people of the San Joaquin Valley! Credit: Emma Yates Share








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      Last Updated Jun 24, 2025 Related Terms
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