Calibration of ShadowCam

• Published in: Journal of astronomy and space sciences Vol. 40; no. 4; pp. 173 - 197
• Main Authors: Humm, David Carl, Kinczyk, Mallory Janet, Brylow, Scott Michael, Wagner, Robert Vernon, Speyerer, Emerson Jacob, Estes, Nicholas Michael, Mahanti, Prasun, Boyd, Aaron Kyle, Robinson, Mark Southwick
• Format: Journal Article
• Language: English
• Published: 한국우주과학회 01.12.2023
• Subjects: 천문학
• ISSN: 2093-5587; 2093-1409
• DOI: 10.5140/JASS.2023.40.4.173

ShadowCam is a high-sensitivity, high-resolution imager provided by NASA for the Danuri (KPLO) lunar mission. ShadowCam calibration shows that it is well suited for its purpose, to image permanently shadowed regions (PSRs) that occur near the lunar poles. It is 205 times as sensitive as the Lunar Reconnaissance Orbiter Camera (LROC) Narrow Angle Camera (NAC). The signal to noise ratio (SNR) is greater than 100 over a large part of the dynamic range, and the top of the dynamic range is high enough to accommodate most brighter PSR pixels. The optical performance is good enough to take full advantage of the 1.7 meter/pixel image scale, and calibrated images have uniform response. We describe some instrument artifacts that are amenable to future corrections, making it possible to improve performance further. Stray light control is very challenging for this mission. In many cases, ShadowCam can image shadowed areas with directly illuminated terrain in or near the field of view (FOV). We include thorough qualitative descriptions of circumstances under which lunar brightness levels far higher than the top of the dynamic range cause detector or stray light artifacts and the size and extent of the artifact signal under those circumstances.