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The Clementine UVVIS camera returned over half a million images while in orbit around the Moon in 1994. Since the Clementinemission, our knowledge of lunar topography, gravity, and the location of features on the surface has vastly improved with the successof the Gravity Recovery and Interior Laboratory (GRAIL) mission and ongoing Lunar Reconnaissance Orbiter (LRO) mission. Inparticular, the Lunar Reconnaissance Orbiter Camera (LROC) has returned over a million images of the Moon since entering orbit in2009. With the aid of improved ephemeris and on-orbit calibration, the LROC team created a series of precise and accurate globalmaps. With the updated reference frame, older lunar maps, such as those generated from Clementine UVVIS images, are misalignedmaking cross-mission analysis difficult. In this study, we use feature-based matching routines to refine and recalibrate the interiorand exterior orientation parameters of the Clementine UVVIS camera. After applying these updates and rigorous orthorectification,we are able generate precise and accurate maps from UVVIS images to help support lunar science and future cross-missioninvestigations

the international archives of the photogrammetry, remote sensing and spatial information sciences/international archives of the photogrammetry, remote sensing and spatial information sciences

GEOMETRIC CALIBRATION OF THE CLEMENTINE UVVIS CAMERA USING IMAGES ACQUIRED BY THE LUNAR RECONNAISSANCE ORBITER