NRL Develops Critical Components for Next Generation Gamma-Ray Mission
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The Naval Research Laboratory (NRL) is a member of an international consortium that was recently selected by NASA to develop the primary instrument for the Gamma Ray Large Area Space Telescope (GLAST). GLAST, the next major space mission to study high-energy astrophysics, is planned for launch in 2005 for a minimum five-year mission.
GLAST is the successor to the
Energetic Gamma-Ray Experiment Telescope (EGRET) experiment on
NASA's Compton Gamma Ray Observatory (CGRO), which recently ended
its mission after many years of successful observations. GLAST
will be 50 times more sensitive than EGRET and will detect gamma
rays at high energies ranging from 20 million to 300 billion
electron volts. The study of gamma rays is expected to provide
essential insight into physical processes driving celestial objects.
Gamma rays are the most penetrating type of electromagnetic radiation, and allow a direct view of the high-energy processes acting in the innermost regions of cosmic accelerators such as pulsars, black holes, and supernova remnants. GLAST will precisely locate hundreds of mysterious gamma-ray bursts, recently shown to be the most powerful and distant explosions in the Universe since the Big Bang. It will be sensitive enough to detect several dozen gamma-ray pulsars, which, scientists say, will reveal new details about the life cycle of massive stars in our Galaxy.
NRL's Gamma and Cosmic Ray Astrophysics Branch is responsible for the design, development and test of the massive calorimeter for GLAST. The principal function of the calorimeter is to measure the energy of incoming gamma rays.
The main GLAST instrument is a wide field-of-view imaging telescope, which consists of a tracker that determines the trajectory of the gamma ray being measured, and the NRL-developed cesium-iodide calorimeter. A charged-particle anti-coincidence shield helps filter out unwanted signals, such as those produced by background particles.
Once a gamma ray penetrates the shield, it interacts in the tracker and is converted into electron-positron pairs pairs of matter and antimatter that multiply and cascade into a "shower" of charged particles and photons (also known as an electromagnetic shower). The calorimeter collects and measures the energy from these showers to determine how much energy is in each gamma ray.
The passage of these particles through the cesium-iodide crystals produce flashes of scintillation light that are photoelectrically converted to voltages, or electrical signals. These signals are then digitized, recorded and relayed to Earth by the spacecraft's onboard computer and telemetry system. Cesium-iodide blocks are arranged in two perpendicular directions, to provide additional positional information about the shower.
The accuracy of the energy measurement is largely determined by the calorimeter's ability to collect all the energy from the shower of particles created by the interaction of the gamma ray with the GLAST instrument, notes NRL investigator, Dr. Neil Johnson. The penetrating nature of these particles requires a massive calorimeter to stop or capture them. In GLAST, the calorimeter is about 60% of the weight of the experiment. GLAST uses 1350 kg of thallium-doped cesium iodide, CsI(Tl), scintillation crystals to form the calorimeter. These crystals, known for their durability and high resistance to thermal and mechanical shock, look much like rock salt, but are polished like lead glass and emit light when gamma rays or charged particles interact with them. GLAST uses over 1500 CsI crystals.
NRL's X-ray Astronomy Branch is responsible for building the computers used to discriminate gamma rays from background cosmic rays in the events seen by GLAST. Investigator, Dr. Kent Wood, says, "The problem is challenging because background events are several thousand times more numerous than the gamma rays. The gamma rays must be distinguished from the cosmic rays by differences in patterns produced by energy deposited in the tracker and calorimeter." Crucial first stages of this pattern recognition are done in the onboard computers. The high data volumes and event rates call for a high throughput computing system, able to operate reliably in the space radiation environment. NRL has built a prototype processor, using the PowerPC 603e chip. The same NRL group is also flying DoD's first flight testbed for space-based computing systems on the ARGOS satellite, results from which are being applied to the GLAST design.
The GLAST collaboration is headed by Dr. Peter Michelson of Stanford University's Linear Accelerator Center (SLAC). NRL and SLAC recently worked together to build the USA X-ray timing experiment, onboard the ARGOS satellite. Dr. Wood is principal investigator on the USA Experiment. Both USA and GLAST are part of a long collaboration between NRL and Stanford, started by Wood and Michelson in the 1980s, on the study of neutron stars and black holes. NRL was also responsible for the Oriented Scintillation Spectrometer Experiment (OSSE) on CGRO, which employs scintillating crystal and readout technologies that are forerunners of those used in GLAST. During its flight on CGRO, OSSE was able to solve a longstanding puzzle of the active galaxy origin of a background of diffuse gamma rays seen from all parts of the sky at energies up to at least one million electron volts. GLAST will study the continuation of that puzzle up to energies roughly a thousand times higher.
About the U.S. Naval Research Laboratory
The U.S. Naval Research Laboratory is the Navy's full-spectrum corporate laboratory, conducting a broadly based multidisciplinary program of scientific research and advanced technological development. The Laboratory, with a total complement of approximately 2,500 personnel, is located in southwest Washington, D.C., with other major sites at the Stennis Space Center, Miss., and Monterey, Calif. NRL has served the Navy and the nation for over 90 years and continues to meet the complex technological challenges of today's world. For more information, visit the NRL homepage or join the conversation on Twitter, Facebook, and YouTube.
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