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Subject: Re: Stereo of the Moon
- From: P3D john bercovitz <bercov@xxxxxxxxxxx>
- Subject: Subject: Re: Stereo of the Moon
- Date: Wed, 6 Nov 1996 20:15:34 -0800
I just did some back-of-the-envelope figuring and I must agree
with Mugnier now. What I was really basing my earlier statement
on was having looked at an old moon stereo and not seeing any
depth in the craters/mountains. But! The pair was of very poor
resolution. That thought set me to scribbling:
Mugnier says parallax is visible in stereo pairs of the moon.
My question is, "At what magnification?" Using rough guesses:
Moon distance is 238 000 mi ? (+/- 5%?).
Crater wall height ~ 3 mi ?
Mugnier indicates max libration ~ 15 degrees,
the tangent of which is about 1 part in 4
So shift of top of crater wall relative to bottom of crater wall
is 1/4 * 3 = 3/4 mile
At a distance of 238 000 mi, this is
1 part in (238 000/(3/4)) = 320 000
Eyes' sensitivity to parallax is 10" of arc or 1 part in 20 000
So minimum magnification is 320K/20K = 16X !!
Moon subtends 1/2 degree but needs to subtend
16 * 1/2 degree = 8 degrees, the tangent of which is about 1/8
In a 45 mm ocular viewer, 8 degrees would come from an image size
of 45 * (1/8) or 6 mm
The moon subtends 1/2 degree which is 1 part in ~100.
To get a 6 mm image diameter, you would need a 6 * 100 or 600 mm
lens on your camera. And that's to get minimally-detectable
parallax. Probably it would be better to go for some overkill and
use at least a 2000 mm camera lens.
John B
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