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- Newsgroups: sci.astro
- Path: sparky!uunet!zaphod.mps.ohio-state.edu!darwin.sura.net!cs.ucf.edu!news
- From: clarke@acme.ucf.edu (Thomas Clarke)
- Subject: Re: Binoculars, exit pupil size, etc...
- Message-ID: <1992Dec29.205842.17543@cs.ucf.edu>
- Sender: news@cs.ucf.edu (News system)
- Organization: University of Central Florida
- References: <1992Dec29.144420.1@stsci.edu>
- Distribution: na
- Date: Tue, 29 Dec 1992 20:58:42 GMT
- Lines: 74
-
- In article <1992Dec29.144420.1@stsci.edu> gawne@stsci.edu writes:
- > Concerning the ongoing discussion of binoculars, image brightness, etc...
- > I went to the library and looked at the recent issue of Astronomy which
- > included the binocular buyer's guide. While the guide is overall well
- > written it does seem to have suffered from not having been proofread by
- > an optics expert.
- >
- > Specifically, the guide claims that larger exit pupils (up to 7 mm)
- > produce brighter images. As someone else has recently pointed out this
- > just is not the case. Image brightness depends only on:
- >
- > 1. The area of the objective lenses.
- > 2. The quality of the anti-reflective coatings.
- > 3. The effective focal ratio of the binoculars.
- >
- > The first gathers photons over a given area. The larger that area the more
- > photons gathered. The second gets as many photons as possible from the
- > front of the binoculars to your eyes. The third factor (focal length)
- > governs how well you'll be able to see dim extended objects, with image
- > brightness for extended objects dropping off as f squared.
- > .....
- I beg to differ. If a film or CCD sensor were located at the binocular
- objective's focal plane, then the brightness of extended objects
- would depend on the objective focal ratio.
-
- Binoculars produce virtual images, however, so that the real image
- is formed on the retina of the person looking through the binocular.
- The important focal ratio is thus that of the viewer's eye. I don't
- have exact figures, but this would be something like f/3 or 4 depending
- on the individual. This results from the approximately 7 mm entrance
- pupil of the eye and the 2-odd cm focal length of the eye.
-
- When using a binocular the focal ratio is determined by the
- combination of objective, eyepiece and eye-optics of the viewer.
- Maximum brightness is determined by the structure of the individual's
- eye. If the binocular exit pupil fills the eye's pupil, and the
- binocular has 100% transmission efficiency, then the brighntess is
- at the physiological maximum for extended objects.
-
- For extended objects - there's the rub. For point objects, the image
- size is to a large extent independent of magnification or anything else,
- so that brightness is determined by the effective aperture of the binocular.
- That is, it is detemrined by how much light focuses into the eye's
- resolution patch.
-
- > BUT if instead of 11x80's you were to use 20x80's with a 5mm exit pupil
- > then the person with 6mm dark adapted pupils would see 1.56 times brighter
- > images than with the 10x70's! A person with 5 mm dark adapted pupils would
- > see images 2.25x brighter!
-
- Under these conditions extended objects would have equal surface
- brightness (I assume you mean 16x80s to get 5mm), although nebulae
- would of course be larger in the 16x's. Stars would be brighter in
- the 16x's since the all the light from the objective gets
- through to the retina.
- >
- > So where is this all going, you ask? My point is that very few people
- > using binoculars for astronomy have pupils that dilate to 7mm. You are
- > much better off getting binoculars with a 5 or 5.5 mm exit pupil and
- > getting ALL the light into your eyes.
- >
- Having differed, I nevertheless agree with your conclusions. The
- eyes entrance pupil is maximum only in very dark conditions, so that
- exit pupils larger than 5 or so waste light under many conditions.
- If the sky is less than perfectly dark, then the contrast of stars
- may be increased with a smaller exit pupil. The brightness of
- the extended sky background is decreased by a smaller exit pupil,
- whereas the stellar brightness remains nearly constant.
-
- --
- Thomas Clarke
- Institute for Simulation and Training, University of Central FL
- 12424 Research Parkway, Suite 300, Orlando, FL 32826
- (407)658-5030, FAX: (407)658-5059, clarke@acme.ucf.edu
-