This collection consists of publications and memoranda from JPL relating to Newburn's work with the Laboratory, as well as correspondence with colleagues, including Marcia Neugebauer and H.C. Urey.
Biographical / Historical:
Ray Leon Newburn (1933-), noted lunar and planetary scientist, first came to the Jet Propulsion Laboratory (JPL) as a summer employee, after pursuing graduate study in astronomy at the California Institute of Technology. In his long tenure with JPL, he participated in the development of plans for lunar and planetary exploration and planetary models for mission design, served as JPL representative to NASA's Space Sciences Steering Committee's Astronomy Subcommittee and help establish the Table Mountain Observatory in 1962.
Joseph Tatarewicz, David DeVorkin, Division of Space History, NASM, transfer, 1998, 1998-0058, unknown
No restrictions on access
82.13 cu. ft. (80 record storage boxes) (2 document boxes) (1 16x20 box) (1 blueprint storage box)
Atacama Desert (Chile)
Scorpius X-1 (Star)
These records document Riccardo Giacconi's professional career, and consist of papers illustrating his scientific work and administrative records relating to the institutions
at which he worked.
There is extensive documentation of Giacconi's professional activities, including meetings attended, papers presented (and published), his services as officer or board
member of professional societies; grants, proposals, and contracts, mainly with NASA; correspondence with colleagues; slides and photographs of many facilities with which
Giacconi was associated (some unlabeled); news clippings and press releases; appointment books and journals; and files documenting his association with Montedison S.p.A.
Series 1 provides biographical information about Giacconi. Series 2 through 12 offer a roughly chronological overview of the institutions and major scientific projects
with which Giacconi has been associated during his professional career. The institutions are American Science and Engineering (Series 2), Harvard-Smithsonian Center for Astrophysics
(Series 4), Harvard University (Series 5), Space Telescope Science Institute (Series 11) and European Southern Observatory (Series 12).
Although all the institutional series mentioned contain both scientific and administrative records, there is a noticeable decline in scientific content when Giacconi moves
from the Center for Astrophysics to the Space Telescope Science Institute. Interspersed amongst institutional series are series covering major scientific projects that spanned
more than one institution, including the High Energy Astronomy Observatory (HEAO) series of satellites (Series 6-9), particularly HEAO-B also known as Einstein, Uhuru (Series
3), and the Advanced X-Ray Astronomical Facility (AXAF), later known as the Chandra X-Ray Observatory (Series 10).
Series 13 through 17 illustrate Giacconi's tenure on various committees having to do, primarily, with space science. Series 18 and 19 detail his involvement with professional
scientific societies. Series 20 documents Giacconi's involvement in professional scientific meetings. Series 21 illustrates his involvement with Italian company Montedison
and its efforts to found a scientific research institute. Series 22 contains Giacconi's general correspondence, much of it from his time at STSI. Series 23 consists of publications
that did not match with any specific institute or project. Many of these publications are directed toward a lay audience. Series 24 contains generic materials relating to
x-ray astronomy including newspaper clippings and articles. Series 25 consists of Giacconi's appointment books. Series 26 contains materials that relate to Giacconi's personal
life, including receipts, pamphlets, announcements, and videotapes. Series 27 consists of awards that Giacconi received for his scientific accomplishments. The Nobel Prize
is not included in this collection. The total volume of the collection is approximately 95 cubic feet.
Riccardo Giacconi (1931-2018), an astrophysicist, was born in Genoa, Italy. He attended the University of Milan, receiving the PhD in 1954. From 1954 to 1956, he served
as an Assistant Professor of Physics at the University, then became Research Associate (Fulbright Fellow) at Indiana University. From 1958 to 1959, he was a Research Associate
in the Cosmic Ray Laboratory at Princeton University. In 1959 he took the post of Senior Scientist, vice president in charge of the Space Research and Systems Division, at
American Science and Engineering (ASE), a private research corporation in Cambridge, Massachusetts. He stayed at ASE, serving as Executive Vice President and a member of the
Board of Directors, until 1973, when he left to become Associate Director of the High Energy Astrophysics Division of the Harvard-Smithsonian Center for Astrophysics (CFA)
and Professor of Astronomy at Harvard University. He remained at the CFA until 1981 when he was appointed first Director of the Space Telescope Science Institute (STSI) and
Professor of Physics and Astronomy at The Johns Hopkins University. In 1991 he was also appointed Professor of Physics at the University of Milan.
Much of Giacconi's pioneering work in x-ray astronomy took place during his tenure at ASE, and he was a major force in the development of the company. In 1962 Giacconi's
group succeeded in detecting the first extrasolar x-ray source. In 1963 the same group obtained the first solar x-ray picture by use of an x-ray telescope, which had been
conceived, advocated, designed, and fabricated by them. In that same year Giacconi proposed an x-ray astronomy satellite, Explorer. The proposal led to a program of construction
in 1966-1970, followed by a successful launch in 1970. The satellite became known as Uhuru, and represented a major qualitative step in x-ray astronomy's observational capability.
Following this early work on solar x-ray studies, a major program, initiated in 1968, culminated in the flight of the SO-54 x-ray telescope on the Apollo Telescope Mount's
Skylab mission. In 1970 a program for construction of a 1.2 meter x-ray telescope for study of extrasolar sources was initiated. The program was modified in 1973, and finally
led to the Einstein Observatory mission, successfully launched in 1978. Giacconi had responsibility for the scientific direction and administrative management of all these
Giacconi went to the CFA as Director of the High Energy Astrophysics Division in 1973. He oversaw the conception, fabrication, and design of the Einstein Observatory, preparation
of the software and hardware for data reduction for Einstein, and the establishment and implementation of the Guest Observer Program.
In 1981 Giacconi became Director of the new Space Telescope Science Institute, managed by the Association of Universities for Research in Astronomy for the National Aeronautics
and Space Administration (NASA).When fully operational, the STSI was to be the center of operations and research for the Hubble Space Telescope, which was launched in 1990.
From 1987 to 1988, Giacconi served as a consultant to Montedison S.p.A., an Italian chemical conglomerate, with the title of Chairman of the Board, Instituto Donegani, the
research arm of the parent corporation. This activity, which was an attempt to elevate Instituto Donegani to a world class center for chemistry, was soon abandoned.
In 1993, Giacconi left STSI to head the European Southern Observatory (ESO). ESO is an intergovernmental European organization for astronomical research. ESO coordinates
the activities of the La Silla and Paranal observatories in the Atacama Desert in Chile. One of the major scientific achievements of ESO under Giacconi's leadership was the
installation of the Very Large Telescope (VLT) at the Paranal Observatory.
Giacconi left ESO in 1999 and is currently the President of Associated Universities, Inc., which manages the National Radio Astronomy Observatory under a grant from the
National Science Foundation.
Giacconi is the author of over 300 articles on x-ray astronomy. He has been awarded numerous prizes for his scientific research, including the 2002 Nobel Prize in Physics
for the discovery of cosmic x-ray sources.
This video history consists of original, master and reference videos documenting a children's lecture program by George R. Carruthers, a physicist and inventor. Carruthers invented the Far Ultra-Violet Camera (FUVCAM).
Scope and Contents note:
This collection contains original, master, and reference videos documenting Dr. George Carruthers. Dr. Carruthers discusses his invention, the Far Ultra-Violet Camera (FUVCAM), as well his background, and experience working with the space program.
Divided into 3 series: 1) Original Videos; 2) Master Videos; 3) Reference Videos.
Biographical / Historical:
Dr. George Carruthers was born in 1939 and grew up in Milford, Ohio and Chicago's South Side. Carruthers received his B.S. in Physics from the University of Illinois in 1961, M.S. Physics in 1962, and his Ph.D in aeronautical and astronomical engineering in 1964. After receiving his Ph.D in 1964, Carruthers joined the Naval Research Laboratory (NRL), Space Science Division where he is now Senior Astrophysicist. Along with William Conway, another scientist, Carruthers developed the lunar surface ultraviolet camera and spectrograph used on the moon by Apollo 16 in 1972. The camera was used to take ultraviolet pictures of the Earth during the Apollo 16 space mission. It was the first camera to take pictures of the upper levels of the earth's atmosphere and to show that hydrogen exists in outer space.
This videohistory was created by the Innovative Lives Program of The Jerome and Dorothy Lemelson Center for the Study of Invention and Innovation on February 22, 1996. The Innovative Lives series brings young people and American inventors together to discuss inventions and the creative process and to experiment and play with hands-on activities related to each inventor's product.
Collection is open for research.
Collection items available for reproduction, but the Archives Center makes no guarantees concerning copyright restrictions. Other intellectual property rights may apply. Archives Center cost-recovery and use fees may apply when requesting reproductions.