Dawes limit

Dawes limit The maximum resolving power that can be obtained in practice from a telescope of a given aperture. It was established by W. R.Dawes on the basis of tests of the visibility of double stars through various apertures. It states that a pair of sixth-magnitude stars can just be seen as double by a 1-inch (25.4-mm) telescope if they are separated by 4”.56. The table gives the resolving power of various instruments based on the Dawes limit.

dawes limit

Aperture mm

Resolving power ”

25

4.63

50

2.32

75

1.54

100

1.16

125

0.93

150

0.77

175

0.66

200

0.58

250

0.46

300

0.39

400

0.29

500

0.23


Cite this article
Pick a style below, and copy the text for your bibliography.

  • MLA
  • Chicago
  • APA

"Dawes limit." A Dictionary of Astronomy. 1997. Encyclopedia.com. 30 May. 2012 <http://www.encyclopedia.com>.

"Dawes limit." A Dictionary of Astronomy. 1997. Encyclopedia.com. (May 30, 2012). http://www.encyclopedia.com/doc/1O80-Daweslimit.html

"Dawes limit." A Dictionary of Astronomy. 1997. Retrieved May 30, 2012 from Encyclopedia.com: http://www.encyclopedia.com/doc/1O80-Daweslimit.html

Learn more about citation styles

Find thousands of answers for hundreds of subjects at Answers Encyclopedia .

All answers verified by trusted sources at Encyclopedia.com

Try Answers Encyclopedia now!

For students and teachers!

Encyclopedia.com provides students and teachers facts, information, and biographies from verified, citable sources, including:

Encyclopedia.com provides students and teachers facts, information, and biographies from verified, citable sources, including: