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Pinhole Photography<br />

Landschaft von der Sonne beleuchtet wird and man bringt auf der<br />

gegenüberliegenden Seite in der Wand einer nicht von der Sonne<br />

gotr<strong>of</strong>fenen Wohnung ein kleines Löchlein an, so werden alle erleuchteten<br />

Gegenstände ihr Bild durch diese Öffnung senden und werden umgekehrt<br />

erscheinen". [1]<br />

In 1475 the Renaissance mathematician and astronomer Paolo Toscanelli<br />

placed a bronze ring with an aperture in a window in the Cathedral <strong>of</strong><br />

Florence, still in use today. On sunny days a solar image is projected<br />

through the hole onto the cathedral's floor. At noon, the solar image bisects<br />

a "noon-mark" on the floor. The image and noon-mark were used for telling<br />

time (Renner 1995:6).<br />

In 1580 papal astronomers used a pinhole and a similar noon-mark in the<br />

Vatican Observatory in Rome to prove to Pope Gregory XIII that the spring<br />

equinox fell incorrectly on 11 March rather than on 21 March. Two years<br />

later, after careful consideration, Pope Gregory XIII corrected the Julian<br />

calendar by 10 days, thus creating the Gregorian calendar (Renner 1995:7).<br />

Giovanni Battista della Porta (1538–1615), a scientist from Naples, was<br />

long regarded as the inventor <strong>of</strong> the camera obscura because <strong>of</strong> his<br />

description <strong>of</strong> the pinhole (lensless) camera obscura in the first edition <strong>of</strong> his<br />

Magia naturalis (1558). His description has received much publicity, as did<br />

his camera obscura shows, but he was by no means the inventor.<br />

The first published picture <strong>of</strong> a pinhole camera obscura is apparently a<br />

drawing in Gemma Frisius' De Radio Astronomica et Geometrica (1545).<br />

Gemma Frisius, an astronomer, had used the pinhole in his darkened room<br />

to study the solar eclipse <strong>of</strong> 1544. The very term camera obscura ("dark<br />

room") was coined by Johannes Kepler (1571–1630). At his time, the term<br />

had come to mean a room, tent or box with a lens aperture used by artists to<br />

draw a landscape. The lens made the image brighter and focused at a certain<br />

distance. Thus this type <strong>of</strong> camera differed from the pinhole camera obscura<br />

used by Frisius in 1544. In the 1620s Johannes Kepler invented a portable<br />

camera obscura. Camera obscuras as drawing aids were soon found in many<br />

shapes and sizes. They were used by both artists and amateur painters.<br />

During the 19th century several large scale camera obscuras were built as<br />

places <strong>of</strong> education and entertainment. The meniscus lens, superior to the biconvex<br />

lens, improved the quality <strong>of</strong> the the projected images. Several<br />

buildings or towers with camera obscuras remain today: The Camera<br />

Obscura at Royal Mile, Edinburgh; the Great Union Camera at Douglas, Isle<br />

http://www.photo.net/photo/pinhole/pinhole (4 <strong>of</strong> 28)7/3/2005 2:15:39 AM

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