The Astrophotography reference article from the English Wikipedia on 24-Apr-2004 (provided by Fixed Reference: snapshots of Wikipedia from wikipedia.org)

Astrophotography

Astrophotography involves taking photographss of astronomical objects such as the planets, stars , galaxies and nebulae.

Since the photographic emulsion accumulates light throughout its exposure, astrophotography is used to reveal objects which are too faint to observe with the naked eye.

Astrophotography poses challenges which are distinct from normal photography in that the subject is usually extremely faint. Effective astrophotography requires the use of many of the following techniques;

• Mounting the camera at the focal point of a large telescope
• Emulsions designed for low light sensitivity
• Very long exposure times (one hour or more is common)
• Tracking the subject to compensate for the rotation of the Earth during the exposure
• Gas Hypersensitizing of emulsions
• Use of filters to reduce background fogging due to light pollution of the night sky.

Since the early 1990 most professional observatories switched to using CCD devices for astronomical imaging. They have numerous advantages with increased sensitivity and more linear response. The principle disadvantage being a significant reduction in the field of view. Again CCDs require specific modifications for best effect in the low light conditions of astronomy

• Cryogenic cooling to reduce thermal noise
• compensation for non-uniform pixel sensitivity
• biasing

Emulsion based astrophotography remains popular with amateur astronomers, but even here CCD imaging is becoming relatively cheap and is starting to replace wet photography.

See Also

• Photographic plate
• Palomar Observatory Sky Survey
• David Malin

External Links

• History of Astrophotography

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