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: Creencia, Erwin, Sy, Gemma P.
Format: text
Language:English
Published: Animo Repository 1996
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Online Access:https://animorepository.dlsu.edu.ph/etd_bachelors/8212
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Institution: De La Salle University
Language: English
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spelling oai:animorepository.dlsu.edu.ph:etd_bachelors-88572021-08-10T05:37:17Z Photography of selected lunar features and the depth measurement of selected craters Creencia, Erwin Sy, Gemma P. 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. 1996-01-01T08:00:00Z text https://animorepository.dlsu.edu.ph/etd_bachelors/8212 Bachelor's Theses English Animo Repository Lunar craters--Measurement Moon--Surface Lunar photography Computer programs Moon--Photographs
institution De La Salle University
building De La Salle University Library
continent Asia
country Philippines
Philippines
content_provider De La Salle University Library
collection DLSU Institutional Repository
language English
topic Lunar craters--Measurement
Moon--Surface
Lunar photography
Computer programs
Moon--Photographs
spellingShingle Lunar craters--Measurement
Moon--Surface
Lunar photography
Computer programs
Moon--Photographs
Creencia, Erwin
Sy, Gemma P.
Photography of selected lunar features and the depth measurement of selected craters
description 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.
format text
author Creencia, Erwin
Sy, Gemma P.
author_facet Creencia, Erwin
Sy, Gemma P.
author_sort Creencia, Erwin
title Photography of selected lunar features and the depth measurement of selected craters
title_short Photography of selected lunar features and the depth measurement of selected craters
title_full Photography of selected lunar features and the depth measurement of selected craters
title_fullStr Photography of selected lunar features and the depth measurement of selected craters
title_full_unstemmed Photography of selected lunar features and the depth measurement of selected craters
title_sort photography of selected lunar features and the depth measurement of selected craters
publisher Animo Repository
publishDate 1996
url https://animorepository.dlsu.edu.ph/etd_bachelors/8212
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