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The Goldstone
Deep Space Communications Complex, located in California's Mojave
Desert, is one of three complexes in NASA's Deep Space Network
(DSN). |
Marvelous images from such far
away locales as Mars, Jupiter, and Saturn have been made possible
by the engineering and scientific minds at the Jet Propulsion
Laboratory (JPL). Just as impressive are the missions JPL is
flying or planning to take NASA into, what JPL director Dr. Edward
Stone refers to as the "third era of exploration"--a
time of sending probes into deep space often for detailed exploration
or to return samples to Earth.
One of NASA's leaders in the agency's Space Science Enterprise,
JPL is managed by the California Institute of Technology. JPL
is NASA's Center of Excellence in deep space systems. This center
also manages the worldwide Deep Space Network of radio dishes
that are placed in California, Spain, and Australia.
JPL engineers are blueprinting missions for the robotic exploration
of Mars, Jupiter's moon Europa, distant Pluto, the Sun, and numbers
of comets and asteroids. A step-by-step build-up of technological
capability has also started, with the aim of detecting and imaging
Earth-like planets that circle stars light-years away. JPL also
develops and flies instruments and satellites that observe the
environment of Earth. Additionally, the laboratory uses its technological
expertise for many other customers and partners both within and
outside of NASA.
A good example of a recent cutting-edge JPL mission is that
of the Deep Space 1. Launched into space in October 1998, Deep
Space 1 took a host of advanced technologies around the test
track.
Armed with advanced solar arrays, and carrying many other
new technologies, including several in communications, microelectronics,
and spacecraft structures, Deep Space 1 also validated the first-ever
use of an ion propulsion system for primary propulsion in deep
space. Fueled by xenon, the ion engine produces a small, but
constant thrust for hours on end while being 10 times more fuel
efficient than chemical onboard propulsion systems. From late
November through the end of the year, the ion engine chalked
up nearly 720 hours of engine thrusting and was still going strong.
Deep Space 1's validation of its ion engine is viewed by many
to be one of NASA's biggest breakthroughs ever.
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| An artist's
rendering of NASA's Quick Scatterometer (QuikScat) that measures
winds over the ocean surface. |
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JPL teams continue to improve on such technologies as the
Quantum Well Infrared Photodetector, one of the world's most
highly sensitive infrared cameras at long wavelengths. Work on
the Active Pixel Sensor is being furthered, enabling video cameras
to be reduced to the size of a chip coupled with optics, while
using only one-hundredth the power of standard CCD cameras.
Sponsored by JPL's Technology Applications Programs (TAP),
important milestones are being met in projects pursuing "Global
Positioning System on a chip" technology, Millimeter Integrated
Circuit low-noise amplifiers, and a submillimeter sensor to measure
ice. TAP-developed technologies range from sensors to support
far-infrared missions, to electronic components for detection
needs in the microwave and submillimeter wave spectral regions.
These technologies, and others developed at JPL, will enable
such missions as the First Infrared and Submillimeter Space Telescope
(FIRST), and contribute to the European Space Agency's Rosetta
mission to a comet.
TAP is also developing Lithographie Galvanoformung Abformung
(LIGA) grids for NASA's High Energy Solar Spectroscopic Imager
(HESSI) mission to be launched in 2000. HESSI will provide full
Sun spectral images to help discern a number of solar secrets.
LIGA/thick film lithography is a technology with an impressive
future, making possible specialized arrays for miniature mass
spectrometers, miniature ion traps for mass spectroscopy, tunable
miniature inductors and capacitors for power and communications
applications, as well as micro-sized propulsion, power sources,
and pumps. In the case of HESSI, the LIGA microfabrication technique
reduced both spacecraft size and the mission's cost.
As part of its current proof-of-concept phase, the Viewing
Imager Gimbaled Instrumentation Lab & Analog Neural Three-dimensional
processing Experiment (VIGILANTE), has moved to completion phase.
VIGILANTE is a machine vision instrument that combines several
sensors in order to recognize specific targets in real-time,
without the aid of the human eye. The key is a new, JPL-developed,
sugar cube-sized processor built on neural networking principles.
JPL's Space Inflatable Technology Program is moving toward
center stage. This innovative program is bringing closer the
day when huge radar and communication dishes circle the Earth,
enormous solar sails slip through the vacuum of space, and giant
sunshades cool down high-tech infrared sensors that peer deep
into the universe. Accomplishment in this area included the successful
testing of a half-scale model of the inflatable sunshield for
the Next-Generation Space Telescope (NGST). Also constructed
were 42-foot-long inflatable thermoset composite booms for future
applications on solar sails. Inflatable solar arrays are now
part of the JPL's Deep Space 4 mission to land atop a comet.
Be it ultra-miniature instruments or huge inflatable structures,
JPL scientists and engineers have shown technology advancements
come in all shapes and sizes.
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An artist's rendition
of the Mars Polar Lander. |
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