Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995spie.2475..393p&link_type=abstract
Proc. SPIE Vol. 2475, p. 393-404, Infrared Detectors and Instrumentation for Astronomy, Albert M. Fowler; Ed.
Astronomy and Astrophysics
Astronomy
2
Scientific paper
The Clementine mission provided the first ever complete, systematic surface mapping of the moon from the ultra-violet to the near-infrared regions. More than 1.7 million images of the moon, earth, and space were returned from this mission. The near-infrared (NIR) multi- spectral camera, one of two workhorse lunar mapping cameras (the other being the UV/visible camera), provided approximately 200 m spatial resolution at 400 km periselene, and a 39 km across-track swath. This 1.9 kg infrared camera using a 256 X 256 InSb FPA viewed reflected solar illumination from the lunar surface and lunar horizon in the 1 to 3 micrometers wavelength region, extending lunar imagery and mineralogy studies into the near infrared. A description of this lightweight, low power NIR camera along with a summary of lessons learned is presented. Design goals and preliminary on-orbit performance estimates are addressed in terms of meeting the mission's primary objective for flight qualifying the sensors for future Department of Defense flights.
Ledebuhr Arno G.
Lewis Isabella T.
Massie Mark A.
Metschuleit Karen
Park Hye-Sook
No associations
LandOfFree
Near-infrared camera for the Clementine mission does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Near-infrared camera for the Clementine mission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-infrared camera for the Clementine mission will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-761082