Back to Home

ATM Forum Message

Forums: Atm · Astrophotography · Blackholes · Blackholes2 · CCD · Celestron · Domes · Education
Eyepieces · Meade · Misc. · God and Science · SETI · Software · UFO · XEphem
RSS Button

Home | Discussion Forums | Amateur Telescope Making | Post
Login

Be the first pioneers to continue the Astronomy Discussions at our new Astronomy meeting place...
The Space and Astronomy Agora
Re: How Does Grinding Work?!?

Forum List | Follow Ups | Post Message | Back to Thread Topics | In Response To
Posted by Tom on June 19, 1999 17:13:17 UTC

: I do know how to grind a mirror, but I don't know how it can grind out the concave shape in the glass? This is not that important, but I would like to know for my own sake. Also, is a ronchi test better than a focault test? And lastly, is a ten inch mirror a good start? : I apreciate all of your help!!!! THANK YOU!!!!

John:

Lets see if I can paint a mental picture of how grinding works. If you are to watch the two disks move back and forth over each other you would see - the closer you get to the center of the upper disk, the more time that glass is in grinding contact with the bottom disk so it gets ground out more. Away from the center, that glass progressivly spends more time "hanging" out in thin air. (I know, I know, you could say the same for the bottom disk but..) Now, for the bottom disk, picture you're pushing down with 10lbs of pressure as you grind. As the top disk progressivly overhangs the bottom, that 10lbs is being concentrated more and more on the edge of the bottom disk and the center of the top disk. These forces combined with the fact you are not doing anything to hold the two faces parallel as they grind has a natural tendancy to hollow out the upper disk. If you could mount the disks in a machine that held them rigidly (so the pressure is exactly even with no "rocking" tendancy and you ground them back and forth, they would not hollow out. You may not think you are trying (trying is the key word here) to rock the disks when grinding, but if you picture the pressure "curve" across the stroke it would be a curve, less pressure when the two are centered, and more as they overhang. Combine the two and you see as the pressure/time grinding is greatest for the center of the top disk and edge of the bottom disk.

Phew! hope that helped instead of confusing. Translating the picture in my mind to words that will paint the same picture in yours...

It was a great question, and one that has been asked by many before you - myself included.

Tom

Follow Ups:

    Login to Post
    Additional Information
    Google
     
    Web www.astronomy.net
    DayNightLine
    About Astronomy Net | Advertise on Astronomy Net | Contact & Comments | Privacy Policy
    Unless otherwise specified, web site content Copyright 1994-2024 John Huggins All Rights Reserved
    Forum posts are Copyright their authors as specified in the heading above the post.
    "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET"
    are trademarks of John Huggins