Photography of selected lunar features and the depth measurement of selected craters.
Photographs of Theophillus, Catharina, Piccolomini and other craters were taken using the 16-inch Mishimura telescope. These photographs were then converted into digitized graphics files. A developed computer program measured the depths of the crater images contained in these files. The program meas...
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| Main Authors: | , |
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| Format: | text |
| Language: | English |
| Published: |
Animo Repository
1996
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| Subjects: | |
| Online Access: | https://animorepository.dlsu.edu.ph/etd_bachelors/4131 |
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| Institution: | De La Salle University |
| Language: | English |
| Summary: | Photographs of Theophillus, Catharina, Piccolomini and other craters were taken using the 16-inch Mishimura telescope. These photographs were then converted into digitized graphics files. A developed computer program measured the depths of the crater images contained in these files. The program measured the shadow pixel distances of the craters that were present. Computed depths of Piccolomini, Catharina, Polybius, Rothmann and Stiborius are 14, 512.06 ft, 25,216.06 ft, 10,062.31 ft, 12,886.04 ft. and 10,062.31 ft. respectively. |
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