S81-29031 (Feb 1981) --- Astronaut Karl G. Henize, PhD.
S67-47941 (1967) --- Astronaut Karl G. Henize.
![This image from NASA Spitzer Space Telescope, shows the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera IRAC. The LMC is a small satellite galaxy gravitationally bound to our own Milky Way. Yet the gravitational effects are tearing the companion to shreds in a long-playing drama of 'intergalactic cannibalism.' These disruptions lead to a recurring cycle of star birth and star death. Astronomers are particularly interested in the LMC because its fractional content of heavy metals is two to five times lower than is seen in our solar neighborhood. [In this context, 'heavy elements' refer to those elements not present in the primordial universe. Such elements as carbon, oxygen and others are produced by nucleosynthesis and are ejected into the interstellar medium via mass loss by stars, including supernova explosions.] As such, the LMC provides a nearby cosmic laboratory that may resemble the distant universe in its chemical composition. The primary Spitzer image, showing the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera (IRAC) at near-infrared wavelengths and the mid-infrared data from a multiband imaging photometer (MIPS). Blue represents invisible infrared light at wavelengths of 3.6 and 4.5 microns. Note that most of the stars in the field of view radiate primarily at these short infrared wavelengths. Cyan denotes emission at 5.8 microns, green depicts the 8.0 micron light, and red is used to trace the thermal emission from dust at 24 microns. The separate instrument images are included as insets to the main composite. An inclined ring of emission dominates the central and upper regions of the image. This delineates a bubble of hot, x-ray emitting gas that was blown into space when a massive star died in a supernova explosion millions of years ago. The shock waves from that explosion impacted a cloud of nearby hydrogen gas, compressed it, and started a new generation of star formation. The death of one star led to the birth of many new stars. This is particularly evident in the MIPS inset, where the 24-micron emission peaks correspond to newly formed stars. The ultraviolet and visible-light photons from the new stars are absorbed by surrounding dust and re-radiated at longer infrared wavelengths, where it is detected by Spitzer. This emission nebula was cataloged by Karl Henize (HEN-eyes) while spending 1948-1951 in South Africa doing research for his Ph.D. dissertation at the University of Michigan. Henize later became a NASA astronaut and, at age 59, became the oldest rookie to fly on the Space Shuttle during an eight-day flight of the Challenger in 1985. He died just short of his 67th birthday in 1993 while attempting to climb the north face of Mount Everest, the world's highest peak. http://photojournal.jpl.nasa.gov/catalog/PIA05517](https://images-assets.nasa.gov/image/PIA05517/PIA05517~medium.jpg)
This image from NASA Spitzer Space Telescope, shows the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera IRAC. The LMC is a small satellite galaxy gravitationally bound to our own Milky Way. Yet the gravitational effects are tearing the companion to shreds in a long-playing drama of 'intergalactic cannibalism.' These disruptions lead to a recurring cycle of star birth and star death. Astronomers are particularly interested in the LMC because its fractional content of heavy metals is two to five times lower than is seen in our solar neighborhood. [In this context, 'heavy elements' refer to those elements not present in the primordial universe. Such elements as carbon, oxygen and others are produced by nucleosynthesis and are ejected into the interstellar medium via mass loss by stars, including supernova explosions.] As such, the LMC provides a nearby cosmic laboratory that may resemble the distant universe in its chemical composition. The primary Spitzer image, showing the wispy filamentary structure of Henize 206, is a four-color composite mosaic created by combining data from an infrared array camera (IRAC) at near-infrared wavelengths and the mid-infrared data from a multiband imaging photometer (MIPS). Blue represents invisible infrared light at wavelengths of 3.6 and 4.5 microns. Note that most of the stars in the field of view radiate primarily at these short infrared wavelengths. Cyan denotes emission at 5.8 microns, green depicts the 8.0 micron light, and red is used to trace the thermal emission from dust at 24 microns. The separate instrument images are included as insets to the main composite. An inclined ring of emission dominates the central and upper regions of the image. This delineates a bubble of hot, x-ray emitting gas that was blown into space when a massive star died in a supernova explosion millions of years ago. The shock waves from that explosion impacted a cloud of nearby hydrogen gas, compressed it, and started a new generation of star formation. The death of one star led to the birth of many new stars. This is particularly evident in the MIPS inset, where the 24-micron emission peaks correspond to newly formed stars. The ultraviolet and visible-light photons from the new stars are absorbed by surrounding dust and re-radiated at longer infrared wavelengths, where it is detected by Spitzer. This emission nebula was cataloged by Karl Henize (HEN-eyes) while spending 1948-1951 in South Africa doing research for his Ph.D. dissertation at the University of Michigan. Henize later became a NASA astronaut and, at age 59, became the oldest rookie to fly on the Space Shuttle during an eight-day flight of the Challenger in 1985. He died just short of his 67th birthday in 1993 while attempting to climb the north face of Mount Everest, the world's highest peak. http://photojournal.jpl.nasa.gov/catalog/PIA05517
The crew assigned to the STS-51F mission included (kneeling left to right) Gordon Fullerton, commander; and Roy D. Bridges, pilot. Standing, left to right, are mission specialists Anthony W. England, Karl J. Henize, and F. Story Musgrave; and payload specialists Loren W. Acton, and John-David F. Bartoe. Launched aboard the Space Shuttle Challenger on July 29, 1985 at 5:00:00 pm (EDT), the STS-51F mission’s primary payload was the Spacelab-2.
51F-06-017 (29 July-6 Aug. 1985) --- Crew portrait with sunglasses. C. Gordon Fullerton's head is at center. Others (bottom, l.-r.) are Roy D. Bridges, F. Story Musgrave and John David Bartoe; and (top) Karl J. Henize, Loren W. Acton and Anthony W. England.
S66-45615 (23 Sept. 1966) --- Discussing the S-13, Ultraviolet Astronomical Camera Experiment, during the postflight experiments briefing at the Manned Spacecraft Center, Houston, Texas, are (left to right) astronauts Charles Conrad Jr., Gemini-11 command pilot; Richard F. Gordon Jr., Gemini-11 pilot; and Dr. Karl Henize, Dearborn Observatory, Northwestern University. Photo credit: NASA
51F-S-161 (6 Aug 1985) --- The Space Shuttle Challenger, with its seven member crew and battery of scientific experiments aboard, eases its rear landing gear onto the dry lake bed at Edwards Air Force Base in California. Onboard for the eight-day mission were C. Gordon Fullerton, Roy D. Bridges Jr., F. Story Musgrave, Karl J. Henize, Anthony W. England, Loren W. Acton and John-David Bartoe.
S85-36655 (24 June 1985) --- The seven crewmembers for STS 51-F/Spacelab 2 pose for photographers following their pre-flight press conference in the Johnson Space Center's public affairs facility. Standing, l.-r., are Karl J. Henize, mission specialist; Roy D. Bridges, pilot; C. Gordon Fullerton, mission commander; F. Story Musgrave, mission specialist; John-David Bartoe, payload specialist; and Anthony W. England, mission specialist. Loren W. Acton, payload specialist, is seated. Launch is scheduled for July of this year.
S85-29307 (May 1985) --- The seven crew members for the Space Shuttle STS-51F/Spacelab 2 mission take a pause from a KSC training session to pose for a pre-flight crew portrait. Astronauts C. Gordon Fullerton (kneeling center), mission commander; and Roy D. Bridges (kneeling right), pilot; are flanked by the payload specialists and mission specialists for the mission. Standing (left to right) are astronauts Anthony W. England, Karl J. Henize and Story Musgrave - all mission specialists; and payload specialist Loren Acton and John-David Bartoe.
51F-S-162 (6 Aug 1985) ---Mission Operations Director George W.S. Abbey, right, shakes hands with Astronaut C. Gordon Fullerton, as the seven-member 51F crew descends from its "home" for eight days. Other Challenger crewmembers egressing the spacecraft are, left to right, F. Story Musgrave, mission specialist; John-David Bartoe, payload specialist; Roy D. Bridges, Jr., Karl J. Henize, mission specialist; Loren W. Acton, payload specialist; and Anthony W. England, mission specicalist. Fullerton, commander, earlier successfully landed Challenger on a Mojave desert dry lake bed. Three years ago, Fullerton was pilot of STS-3, on which the Columbia's scheduled Edwards landing was moved to New Mexico because of weather and runway conditions here.
S85-29498 (June 1985) --- The crew members of space shuttle mission STS-51F have chosen as their insignia this design by Houston artist Skip Bradley. The space shuttle Challenger is depicted ascending toward the heavens in search of new knowledge in the field of solar and stellar astronomy, with its Spacelab 2 payload. The constellations Leo and Orion are in the positions they will be in, relative to the sun during the flight. The nineteen stars signify that this will be the 19th STS flight. Crew members for the mission are astronauts C. Gordon Fullerton, commander; Roy D. Bridges, pilot; F. Story Musgrave, Anthony W. England and Karl J. Henize, mission specialist; and payload specialists Loren W. Acton and John David Bartoe. The NASA insignia design for space shuttle flights is reserved for use by the astronauts and for other official use as the NASA Administrator may authorize. Public availability has been approved only in the forms of illustrations by the various news media. When and if there is any change in this policy, which is not anticipated, the change will be publicly announced. Photo credit: NASA
Image release June 22, 2010 A spectacular new NASA/ESA Hubble Space Telescope image — one of the largest ever released of a star-forming region — highlights N11, part of a complex network of gas clouds and star clusters within our neighbouring galaxy, the Large Magellanic Cloud. This region of energetic star formation is one of the most active in the nearby Universe. The Large Magellanic Cloud contains many bright bubbles of glowing gas. One of the largest and most spectacular has the name LHA 120-N 11, from its listing in a catalogue compiled by the American astronomer and astronaut Karl Henize in 1956, and is informally known as N11. Close up, the billowing pink clouds of glowing gas make N11 resemble a puffy swirl of fairground candy floss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features visible in the nebula are the telltale signs of star formation. N11 is a well-studied region that extends over 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known. It is the process of star formation that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image. Beans are not the only terrestrial shapes to be found in this spectacular high resolution image from the NASA/ESA Hubble Space Telescope. In the upper left is the red bloom of nebula LHA 120-N 11A. Its rose-like petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region. Other star clusters abound in N11, including NGC 1761 at the bottom of the image, which is a group of massive hot young stars busily pouring intense ultraviolet radiation out into space. Although it is much smaller than our own galaxy, the Large Magellanic Cloud is a very vigorous region of star formation. Studying these stellar nurseries helps astronomers understand a lot more about how stars are born and their ultimate development and lifespan. Both the Large Magellanic Cloud and its small companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud in 964 and 1503 respectively. Credit: NASA, ESA and Jesús Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain) To learn more about Hubble go to: <a href="http://www.nasa.gov/mission_pages/hubble/main/index.html" rel="nofollow">www.nasa.gov/mission_pages/hubble/main/index.html</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe.