The second problem with all telescope mirrors is the gravity sag due to the Earths gravity. Most
all telescope mirrors are supported form the flat back. There are many ways to support the glass to minimize the gravity warping
effects. The rule of thumb is that a mirror with a thickness to diameter radio of 1:8 can use simple support of the back of
the mirror. Mirrors that are thin and have a ratio of 1:10 will need extra support
to help them provide the best images.
For the 6”f5 plate glass mirror we see it is about ¾” thick and 6” in diameter.
Therefore the ratio is .75” to 6” or a ratio of 1:8. So, this is good and the mirror will only
need the simplest support.
The simplest support for a mirror is 3 points at 120 degrees around the center of gravity of the
mirror. There is a radius out from the center of the mirror in which the volume
of glass on the inside of the circle is equal to the volume of glass on the outside of the circle.
Mathematically the equation would look like this where Rin is the inside radius of the circle and
Redge is the outside diameter of the mirror. The relationship of the area of
a circle is Pi times radius squared.
So the area inside Rin equals
= Pi * Rin * Rin,
the area from Rin to Redge equals
= Pi * (Redge –Rin) * (Redge – Rin)
If you solve for Rin you get the equation
Rin = 0.707 Redge = .707
* 3”
So you want to put three small cork dots about ¼”
diameter at 3” * .707 or 2.12” out form the center of the mirror
back.
So, flip the glass mirror over to the uncoated side. Place at 3 places and 120 degrees apart, small
paste on dots of cork out 2.12” from the center of the mirror. These 3
cork pads will support the weight of the mirror equally when the mirror is sitting on its back in the telescope.