ASTER will obtain high resolution (15 to 90 m)
images of the Earth in the visible, near-infrared
(VNIR), shortwave-infrared (SWIR), and thermal
infrared (TIR) regions of the spectrum.
ASTER is a cooperative effort between NASA and
Japan's Ministry of International Trade and Industry
(MITI), with the collaboration of scientific and
industrial organizations in both countries. Management of
the ASTER Team is provided by the Japan Resources
Observation System Organization (JAROS). As shown
in the figure, ASTER consists of three distinct
telescope subsystems: VNIR, SWIR, and TIR. It is a high
spatial, spectral, and radiometric resolution, 14-band
imaging radiometer. Spectral separation is
accomplished through discrete bandpass filters and
dichroics. Each subsystem operates in a different
spectral region, has its own telescope(s), and is built
by a different Japanese company.
The VNIR subsystem, built by NEC Corporation,
consists of two telescopesone that looks backward
(along track) and one that looks at nadir. The
nadir-looking telescope is a reflecting-refracting improved
Schmidt design and pairs with the backward looking
telescope to produce same-orbit stereo images. The
VNIR subsystem operates in three visible and
near-infrared bands with 15 m resolution and a 60 km
swath width. The telescope pair is pointable
crosstrack over a ± 24° angle to increase the revisit
frequency of any given Earth location and special targets
of opportunity (e.g., volcanic activity and natural
disasters). Light from either of two onboard halogen
lamps will be used periodically for calibration of this
subsystem.
The SWIR subsystem, built by Mitsubishi Electric
Company (MELCO), operates in six shortwave
infrared channels with 30 m resolution and a 60 km
swath width. It contains a pointing mirror that can
point ± 8.54° from nadir to allow coverage of any
point on Earth over the spacecraft's 16-day cycle.
This mirror is also periodically used to direct light
from either of two onboard calibration lamps into the
subsystem's telescopea fixed, aspheric refracting
telescope.
The TIR subsystem, built by Fujitsu Ltd., operates in
five thermal infrared channels with 90 m resolution
and a 60 km swath width. It contains a scan mirror
that is used for both scanning and pointing up to
± 8.54° from nadir. As in the SWIR, this mirror is also
periodically used to view the onboard blackbody for
calibration. Light from the TIR scan mirror is
reflected into a Newtonian catadioptric telescope system
with an aspheric primary mirror and lens for
aberration correction.
The ASTER instrument operates for a limited time
during the day and night portions of an orbit. The
full configuration (all bands plus stereo) collects data
for an average of 8 minutes per orbit. Reduced
configurations (limited bands, different gains, etc.) can
be implemented as requested by investigators.
The ASTER Team Leaders are Hiroji Tsu in Japan,
and Anne Kahle in the U.S. For more information
about the instrument, see http://asterweb.jpl.nasa.gov.
ASTER is the highest spatial resolution instrument on
the Terra spacecraft, and the only one that does
not acquire data continuously. ASTER data products
include:
- spectral radiances and reflectances of the Earth's surface;
- surface temperature and emissivities;
- digital elevation maps from stereo images;
- surface composition and vegetation maps;
- cloud, sea ice, and polar ice products; and
- observation of natural hazards (volcanoes, etc.).