HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.
NASA Press Release Feb. 28, 1996
NASA Renames X-Ray Timing Explorer in Honor of Bruno B. Rossi
Don Savage
Headquarters, Washington, DC February 28, 1996
(Phone: 202/358-1547)
Jim Sahli
Goddard Space Flight Center, Greenbelt, MD
(Phone: 301/286-0697)
RELEASE: 96-38
NASA RENAMES X-RAY TIMING EXPLORER IN HONOR OF BRUNO B. ROSSI
NASA will name the X-ray Timing Explorer, placed into
orbit in December 1995, in honor of a pioneer in the field of
X-ray astronomy, Bruno B. Rossi. The new official title of the
6,700-pound observatory is the Bruno B. Rossi X-ray Timing
Explorer (RXTE).
The RXTE is currently in a circular 360-statute-mile
(580-kilometer) orbit with an inclination of 23 degrees. Among
the objects to be studied by RXTE are stellar black holes,
neutron stars and quasars.
Professor Rossi and his colleagues discovered the
first non-solar source of X-rays in a dramatic rocket flight in
1962. This source, Scorpius X-1, was the first of many
collapsed stars that also are a key topic of study for the RXTE.
Rossi, who died in 1993 after a long and distinguished
career, served as professor of Physics and Professor Emeritus
at the Massachusetts Institute of Technology. He can be
described as a pioneer in two separate fields of observational
space astrophysics: X-ray astronomy and space plasma physics.
He was the co-recipient of the prestigious Wolf Prize in
Physics in 1987. The Bruno Rossi Prize, awarded annually by
the American Astronomical Society to a top astrophysicist for
achievements in the field, is named in his honor.
The spacecraft, which is about the size of a telephone
booth, is carrying three science instruments which work together
to increase scientific understanding of cosmic X-rays sources.
Two of these instruments -- the Proportional Counter
Array (PCA) and the High-Energy X-ray Timing Experiment (HEXTE)
-- work in concert as the largest X-ray telescope yet flown,
sensitive to X-rays from 2 to 200 keV.
The third instrument, the All Sky Monitor (ASM),
observes the long-term behavior of X-ray sources. The ASM also
serves as a sentinel which monitors the sky and enables the
spacecraft to swing rapidly to targets of opportunity for the
PCA and the HEXTE.
RXTE is the first mission for which 100 percent of the
observing time will be available to the broad scientific
community. Specific observations will be proposed by
scientists from the United States and abroad. Observations are
planned by scientists at the XTE Science Operations Center at
NASA's Goddard Space Flight Center, Greenbelt, MD.
The RXTE was developed by and is managed and operated by
Goddard for NASA's Office of Space Science, Washington, DC.
For questions about scheduling of RXTE observations please send email to
xteplan@athena.gsfc.nasa.gov
If you have other questions about RXTE, please send email to one of our
help desks.
Responsible NASA Official:
Phil Newman
Web Curator:
Robin Corbet
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