Telescope mirrors under tension.



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Topic: Science > Physics
User: "Robert Clark"
Date: 12 Mar 2005 04:58:12 PM
Object: Telescope mirrors under tension.
In this article Geoffrey Landis proposes builing a space tower using
pressurized structures:
THE TSIOLKOVSKI TOWER RE-EXAMINED
Journal of The British Interplanetary Society, Vol 52, pp. 175-180,
1999.
http://www.aeiveos.com/~bradbury/Authors/Engineering/Landis-GA/TTTR.html
He notes that typically materials have higher failure or ultimate
strength in tension than in compression so this would allow higher
towers to be built by using pressurized towers that translate the
vertical compressional forces into tensional forces that tend to expand
the pressurized structure outwards. See section 4.3 and Fig. 3.
I wanted to use a similar idea for creating large telescope mirrors.
However, the formula for deflection of a mirror due to self-weight
depends on Young's modulus, not ultimate strength and Young's modulus
is about the same in tension and compression.
Still it may be possible to create larger mirrors because the
deflection formula also is dependent on density which will be much less
with a gas filled structure:
Deflection ~ Density*(1-Poisson's ratio^2)/Young's Modulus
However, all three of these quantities will likely change for a two
material structure as with a pressurized mirror.
(BTW, perhaps someone can answer this for me, in the Landis article he
just calculates the tensional outward force that would need to be
supported, but surely the outside walls would still need to support
some vertical compression force. Is this just a minor component and can
be neglected?)
Some proposals for inflatable membrane mirrors for use with space
telescopes are given in this conference report:
Ultra Light Space Optics Challenge: Presentations.
http://origins.jpl.nasa.gov/meetings/ulsoc/presentations.html
Another possibility for a mirror under tension is given by this
surprising fact:
Parabolas and Bridges.
"If you hang a flexible chain loosely between two supports, the curve
formed by the chain looks like a parabola, but isn't. It is a catenary,
a more glamorous curve which can be represented algebraically by
hyperbolic functions [y = A (cosh kx - 1)]. In this case, the vertical
load on the chain is uniform with respect to arc length. A whirling
skipping rope is another example of a catenary.
"The load on a suspension bridge is (approximately) uniform with
respect to the horizontal distance. In this case, the curve is a
parabola ..."
http://www.du.edu/~jcalvert/math/parabola.htm
Shape of a suspension bridge cable.
http://aemes.mae.ufl.edu/~uhk/SUSPCAB.jpg
Hanging With Galileo.
"Take a flexible chain of uniform linear mass density. Suspend it from
the two ends. What is the curve formed by the chain? Galileo Galilei
said that it was a parabola, and perhaps you made the same guess. This
time Galileo was not correct. The curve is called a catenary. However,
it is easy to see how he could arrive at this answer through casual
observation and incomplete deduction.
....
"We can get back to the chain solution later. First consider this
extension. What about the curve formed by the cables of a suspension
bridge? Is it too a catenary? No, it is a parabola. So, what gives? How
can this be a parabola while the other one is not?"
http://whistleralley.com/hanging/hanging.htm
Then to form a parabolic surface you could have the suspension cables
arranged in concentric circles hanging from the mirror supporting a
weight. In this case gravity would be working to *form* the surface
shape.
A problem is that just with liquid mirrors you might need to keep the
mirror horizontal so it would have to be zenith-pointing. However, it
may be that by varying the cable lengths you could maintain the
parabolic shape.
Bob Clark
.

User: "redbelly"

Title: Re: Telescope mirrors under tension. 13 Mar 2005 09:33:15 AM
Robert Clark wrote:

In this article Geoffrey Landis proposes builing a space tower using
pressurized structures:

THE TSIOLKOVSKI TOWER RE-EXAMINED
Journal of The British Interplanetary Society, Vol 52, pp. 175-180,
1999.

http://www.aeiveos.com/~bradbury/Authors/Engineering/Landis-GA/TTTR.html


He notes that typically materials have higher failure or ultimate
strength in tension than in compression ...

Funny, I could have sworn it was the other way around.
Fused silica glass is about 20x stronger in compression than in tension
(1100 MPa vs. 50 MPa). See
http://www.sciner.com/Opticsland/FS.htm
and look at "compressive" and "tensile" strength on that page.
Mark
.
User: "Lady Chatterly"

Title: Re: Telescope mirrors under tension. 13 Mar 2005 10:41:40 AM
In article <1110727995.928238.93710@z14g2000cwz.googlegroups.com>
redbelly <redbelly98@yahoo.com> wrote:


Funny, I could have sworn it was the other way around.

In the world.

Fused silica glass is about 20x stronger in compression than in tension
(1100 MPa vs. 50 MPa). See

Under such conditions of awareness, but I know that.

and look at "compressive" and "tensile" strength on that page.

The biggest difference is in the reliability of the hardware and
software. You can look forward to very stringent manufacturing
parameters and programming discipline.

Mark

You are not a Jew hands, organs, dimensions, senses, affections,
passions.
--
Lady Chatterly
"BTW, how long are you going to keep doing this dance with the bot?"
-- Dr.Postman
.

User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 18 Mar 2005 12:12:03 PM
redbelly wrote:

Robert Clark wrote:

In this article Geoffrey Landis proposes builing a space tower

using

pressurized structures:

THE TSIOLKOVSKI TOWER RE-EXAMINED
Journal of The British Interplanetary Society, Vol 52, pp.

175-180,

1999.


http://www.aeiveos.com/~bradbury/Authors/Engineering/Landis-GA/TTTR.html


He notes that typically materials have higher failure or ultimate
strength in tension than in compression ...


Funny, I could have sworn it was the other way around.

Fused silica glass is about 20x stronger in compression than in

tension

(1100 MPa vs. 50 MPa). See

http://www.sciner.com/Opticsland/FS.htm

and look at "compressive" and "tensile" strength on that page.

Mark

Yes, for brittle materials such as concrete or glass the compressive
strength is usually greater than the tensile strength. This is the
reason why steel is used to reinforce concrete, to give it greater
tensile strength. Perhaps Landis is considering the materials that
might be used for a space cable such as steel or carbon fibers for
instance, where the tensile strength is larger, since he makes a
comparison to the lengths that could be achieved with current materials
for a space cable.
BTW, I received an answer to my question of why Landis did not have to
consider the compressive strength of the sides of the pressurized
structure. The situation is analogous to for example a beachball. It
can support significant compression due to the tensile strength of the
material, but the material itself has little compressive strength.
Here's another interesting question to ponder. The formula for
deflection of a mirror due to its self-weight is:
Deflection ~ Density *(1-Poisson's ratio^2)/Young's Modulus
Usually for constructing large mirrors it has only been the Young's
modulus and density that has been considered since the Poisson is
usually about 1/3 for most materials.
But I thought what if you could find a material with a Poisson of 1?
Then the deflection would be 0.
Honeycombed structures in 2-dimensions can have Poisson equal to +1:
Properties of a chiral honeycomb with a Poisson's ratio -1.
D. Prall and Roderic Lakes (University of Wisconsin), Int. J. of
Mechanical Sciences, 39, 305-314, (1996).
"Two dimensional honeycombs with regular hexagonal cells (Fig. 1a)
exhibit a Poisson's ratio of +1 in the honeycomb plane; the
out-of-plane properties differ due to anisotropy. The cell walls have
120 deg. angles between walls and all walls must be of equal thickness
and composition. In contrast honeycombs with inverted cells (Fig. 1b)
give rise to negative Poisson's ratios in the honeycomb plane [2-5]."
http://silver.neep.wisc.edu/~lakes/PoissonChiral.html
Is it believed the Poisson ratio can not be +1 in 3-dimensions or is
this still an open question? Note that this Poisson ratio might not
have to be isotropic. It might be sufficient for example if when the
applied stress is in one direction say the vertical the expansion in
the horizontal direction is 1.

Bob Clark
.
User: "jbuch"

Title: Re: Telescope mirrors under tension. 19 Mar 2005 09:14:36 AM
Landis says:

Fewer references are available about the ultimate compressive strengths of materials than tensile strength.

Long compression members have to contend with buckling as a failure
mode. That is one of the reasons there is less attention paid to
compressive strength of structural materials, as a practical matter.
Buckling is ignored in the Landis paper you cite.
You can do an experiment with a toy long balloon, and readily
demonstrate axial compressive buckling failure in a long length at
really low axial loads.......
I wouldn't ignore buckling as a failure mode in postulating these
structures.
Rather than admiring the nuances of a formula.... (and the predicted
wonders of a magic value of a materials pareameter such as Poisson ratio
of +1) it might be really useful to think of the meaning of the formula.
The formula is based on bending of a (uniform) beam/disk under self
loading and probably has the boundary condition of fixed edges. I must
admit to laziness in not going to my bookcase and dragging out Roark, or
not reading the original
You are encouraged to look at a different formula, one for the boundary
condition of a controlled line bending moment.... which will tend to
counteract the gravity induced bending.
The goal is to reduce the bending to useful levels, not to find perfection.
It is long been said that one of the problems with the Roark compilation
of mechanics of materials equations is that too often the user does not
understand the derivation and assumptions of the example, and therefore
cannot appreciate the limitations.
Robert Clark wrote:

redbelly wrote:

Robert Clark wrote:

In this article Geoffrey Landis proposes builing a space tower


using

pressurized structures:

THE TSIOLKOVSKI TOWER RE-EXAMINED
Journal of The British Interplanetary Society, Vol 52, pp.


175-180,

1999.


http://www.aeiveos.com/~bradbury/Authors/Engineering/Landis-GA/TTTR.html

He notes that typically materials have higher failure or ultimate
strength in tension than in compression ...


Funny, I could have sworn it was the other way around.

Fused silica glass is about 20x stronger in compression than in


tension

(1100 MPa vs. 50 MPa). See

http://www.sciner.com/Opticsland/FS.htm

and look at "compressive" and "tensile" strength on that page.

Mark



Yes, for brittle materials such as concrete or glass the compressive
strength is usually greater than the tensile strength. This is the
reason why steel is used to reinforce concrete, to give it greater
tensile strength. Perhaps Landis is considering the materials that
might be used for a space cable such as steel or carbon fibers for
instance, where the tensile strength is larger, since he makes a
comparison to the lengths that could be achieved with current materials
for a space cable.
BTW, I received an answer to my question of why Landis did not have to
consider the compressive strength of the sides of the pressurized
structure. The situation is analogous to for example a beachball. It
can support significant compression due to the tensile strength of the
material, but the material itself has little compressive strength.
Here's another interesting question to ponder. The formula for
deflection of a mirror due to its self-weight is:

Deflection ~ Density *(1-Poisson's ratio^2)/Young's Modulus

Usually for constructing large mirrors it has only been the Young's
modulus and density that has been considered since the Poisson is
usually about 1/3 for most materials.
But I thought what if you could find a material with a Poisson of 1?
Then the deflection would be 0.
Honeycombed structures in 2-dimensions can have Poisson equal to +1:

Properties of a chiral honeycomb with a Poisson's ratio -1.
D. Prall and Roderic Lakes (University of Wisconsin), Int. J. of
Mechanical Sciences, 39, 305-314, (1996).
"Two dimensional honeycombs with regular hexagonal cells (Fig. 1a)
exhibit a Poisson's ratio of +1 in the honeycomb plane; the
out-of-plane properties differ due to anisotropy. The cell walls have
120 deg. angles between walls and all walls must be of equal thickness
and composition. In contrast honeycombs with inverted cells (Fig. 1b)
give rise to negative Poisson's ratios in the honeycomb plane [2-5]."
http://silver.neep.wisc.edu/~lakes/PoissonChiral.html

Is it believed the Poisson ratio can not be +1 in 3-dimensions or is
this still an open question? Note that this Poisson ratio might not
have to be isotropic. It might be sufficient for example if when the
applied stress is in one direction say the vertical the expansion in
the horizontal direction is 1.


Bob Clark

--
................................
Keepsake gift for young girls.
Unique and personal one-of-a-kind.
Builds strong minds 12 ways.
Guaranteed satisfaction
- courteous money back
- keep bonus gifts
http://www.alicebook.com
.
User: "Geoffrey"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 08:07:44 AM
Pretty good discussion; I'm not sure I have much to add.
Indeed, it turns out that theoretical ultimate compression strength is
greater than tensile strength; it's the opposite in the real world.
Mark wrote:

Fused silica glass is about 20x stronger in compression than in

tension
Glass is a special case. Glass fails in tension due to surface
irregulaties; glass fails by cracking from the surface inward. This
is, in fact, the secret behind the strength of "Tempered glass;" the
thermal treatment puts the surface in compression and the interior in
tension, so surface irregularities won't cause failure, because they're
in tension.
In a different post, Mark wrote:

The force in a typical atomic bond gets ever stronger as the atoms
are compressed together.

But if the atoms are pulled apart, the force will eventually get

weaker

(after initially getting stronger for small tensile displacement of

the

atoms). Unless there is something unusual about the bonding, that
would mean tensile strength is weaker than compressive strength in

most

materials.

True, but not actually relevant to real materials.
In tension, the radial component of the interatomic force is pretty
much the main thing of interest. You're pulling the bonds between
atoms apart. In compression, though, both the radial and the
directional part of the force is relevant. Real world materials squish
when compressed, and that counts as failure even if the atoms don't
actually get closer together.
(An analogue in tensile failure is necking, actually-- once one part
stretches more than another part, the cross section decreases, the
force per unit area increases, and the failure goes exponentially.
Thus, structures fail catastrophically in tension, while they fail
softly in compression. Except for buckling, of course. qv.)
jbuch wrote:

Long compression members have to contend with buckling as a failure
mode. That is one of the reasons there is less attention paid to
compressive strength of structural materials, as a practical matter.

Buckling is ignored in the Landis paper you cite.

Yep. Buckling is a killer failure mode for structures with the
fineness ratio I considered. But for structures this large, buckling
failure has quite long time scales-- it should, in principle, be very
easy to apply active control to prevent it.
(Of course, in the case of a power failure, the tower goes down.)
--a point nobody's made here is simple scale height of the atmosphere.
When I originally did that analysis, I ignored it on the assumption
that interior walls could make the gradient irrelevant, but a couple of
people arguing that point have made me decide I was handwaving a
serious objection. The pressure gradient in the tower makes
pressurized towers of the height I was looking at pretty much
unrealizable in practice-- there are workarounds, but they're not
terribly practical in the real world.
--
Geoffrey A. Landis
http://www.sff.net/people/geoffrey.landis
.
User: "jbuch"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 09:16:22 AM
Geoffrey wrote:

Pretty good discussion; I'm not sure I have much to add.

Indeed, it turns out that theoretical ultimate compression strength is
greater than tensile strength; it's the opposite in the real world.

Mark wrote:

Fused silica glass is about 20x stronger in compression than in


tension

Glass is a special case. Glass fails in tension due to surface
irregulaties; glass fails by cracking from the surface inward. This
is, in fact, the secret behind the strength of "Tempered glass;" the
thermal treatment puts the surface in compression and the interior in
tension, so surface irregularities won't cause failure, because they're
in tension.

In a different post, Mark wrote:


The force in a typical atomic bond gets ever stronger as the atoms
are compressed together.

But if the atoms are pulled apart, the force will eventually get


weaker

(after initially getting stronger for small tensile displacement of


the

atoms). Unless there is something unusual about the bonding, that
would mean tensile strength is weaker than compressive strength in


most

materials.



True, but not actually relevant to real materials.

In tension, the radial component of the interatomic force is pretty
much the main thing of interest. You're pulling the bonds between
atoms apart. In compression, though, both the radial and the
directional part of the force is relevant. Real world materials squish
when compressed, and that counts as failure even if the atoms don't
actually get closer together.

(An analogue in tensile failure is necking, actually-- once one part
stretches more than another part, the cross section decreases, the
force per unit area increases, and the failure goes exponentially.
Thus, structures fail catastrophically in tension, while they fail
softly in compression. Except for buckling, of course. qv.)


jbuch wrote:


Long compression members have to contend with buckling as a failure
mode. That is one of the reasons there is less attention paid to
compressive strength of structural materials, as a practical matter.

Buckling is ignored in the Landis paper you cite.



Yep. Buckling is a killer failure mode for structures with the
fineness ratio I considered. But for structures this large, buckling
failure has quite long time scales-- it should, in principle, be very
easy to apply active control to prevent it.

(Of course, in the case of a power failure, the tower goes down.)

--a point nobody's made here is simple scale height of the atmosphere.
When I originally did that analysis, I ignored it on the assumption
that interior walls could make the gradient irrelevant, but a couple of
people arguing that point have made me decide I was handwaving a
serious objection. The pressure gradient in the tower makes
pressurized towers of the height I was looking at pretty much
unrealizable in practice-- there are workarounds, but they're not
terribly practical in the real world.

Very nice response. Thanks for the professional reply.
.

User: "redbelly"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 05:15:16 PM
Geoffrey,
Thanks for responding. It seemed the O.P. was interested in how to
build a large telescope mirror, so it seemed quite relevent that glass
is stronger in compression (both theoretically and in practice). But I
suppose the mirror need not be made from glass, as had been my thinking
earlier.
However, as this thread has progressed I am less and less clear on what
is being asked for. It's not clear just how large a mirror the O.P.
has in mind, and whether this is something they actually plan to build
or are just putting the idea forth for discussion.
Mark
p.s. Did you think about the effects of high winds on the tower you
discussed in your paper?
.
User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 09:42:04 PM
redbelly wrote:

Geoffrey,

Thanks for responding. It seemed the O.P. was interested in how to
build a large telescope mirror, so it seemed quite relevent that

glass

is stronger in compression (both theoretically and in practice). But

I

suppose the mirror need not be made from glass, as had been my

thinking

earlier.

However, as this thread has progressed I am less and less clear on

what

is being asked for. It's not clear just how large a mirror the O.P.
has in mind, and whether this is something they actually plan to

build

or are just putting the idea forth for discussion.

Mark
...

There are three separate methods of construction of ultra-large
mirrors (greater than 20 meter diameter) I wanted to see investigated
and wanted to put forth for discussion:
1.) The use of pressurized structures. I wanted to consider both gases
and liquids. Both would have the advantage of lowering the overall
density of the mirror and could reduce the deflection amount. This has
been investigated in the case of space mirrors as I said in the first
post, but I only recall seeing the use of thin flexible membranes being
used for this purpose, not stiff materials.
Gases would have the advantage of a much lower density, however,
liquids might have an advantage in that they are largely incompressible
and might mimic the strength to be had in the Young's modulus for solid
materials.
Another possibility that occurs to me is a modification to fully
liquid mirrors, i.e., those with no solid cover, which achieve a highly
parabolic surface by rotation. But the largest that can be practically
achieved is about 6 meters because of the wind kicked up by the motion.
Perhaps by putting a thin *fixed* cover over the rotating liquid,
"interaction" between the solid and liquid could cause the solid cover
to follow the parabolic shape of the liquid. I leave open what this
"interaction" might be, interatomic, electromagnetic, surface tension,
etc.
2.) The second method, which I'm really enthusiastic about, is the
possibility that a parabolic surface can be achieved as a parabolic
curve can be achieved by having the surface support a hanging weight by
cables. I suggested in the first post arranging the supporting cables
in concentric circles, but for the surface to be parabolic you want
vertical cross-sections through the center to be parabolic curves. Then
what you might want is for the support cables to be arranged in
straight radial lines though the center.
3.) The possibility of finding materials with Poisson's ratio of 1.
This could be used in combination with the first two or be completely
separate from them. After a web search I found a discussion on this on
an engineering forum in which one of the posters (by name of
"RPstress") seemed to imply this might be possible in 3-dimensions:
Poisson's ratio greater than 1.
http://www.eng-tips.com/viewthread.cfm?qid=68075&page=9
It is interesting that 2-dimensional examples of this are already
known, for example with honeycombed shapes. Then a possibility might
be to use a single molecular layer over the gas or liquid. Then,
presumably, all the forces within the layer would be in tension not
compression and a 2-D Poisson's ratio equaling 1 could be achieved.
Single-molecular layers of graphite, with high tensile strength, have
been achieved, known as graphene:
Discovery Of Two-Dimensional Fabric Denotes Dawn Of New Materials Era.
Chernogolovka, Russia (SPX) Oct 22, 2004
"Researchers at The University of Manchester and Chernogolovka, Russia
have discovered the world's first single-atom-thick fabric, which
reveals the existence of a new class of materials and may lead to
transistors made from a single molecule. The research is to be
published in Science on 22 October."
http://www.spacedaily.com/news/materials-04zzt.html
Bob Clark
.



User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 19 Mar 2005 10:53:26 AM
jbuch wrote:

Landis says:

Fewer references are available about the ultimate compressive

strengths of materials than tensile strength.


Long compression members have to contend with buckling as a failure
mode. That is one of the reasons there is less attention paid to
compressive strength of structural materials, as a practical matter.

Buckling is ignored in the Landis paper you cite.

You can do an experiment with a toy long balloon, and readily
demonstrate axial compressive buckling failure in a long length at
really low axial loads.......

I wouldn't ignore buckling as a failure mode in postulating these
structures.

Rather than admiring the nuances of a formula.... (and the predicted
wonders of a magic value of a materials pareameter such as Poisson

ratio

of +1) it might be really useful to think of the meaning of the

formula.


The formula is based on bending of a (uniform) beam/disk under self
loading and probably has the boundary condition of fixed edges. I

must

admit to laziness in not going to my bookcase and dragging out Roark,

or

not reading the original

You are encouraged to look at a different formula, one for the

boundary

condition of a controlled line bending moment.... which will tend to
counteract the gravity induced bending.

The goal is to reduce the bending to useful levels, not to find

perfection.


It is long been said that one of the problems with the Roark

compilation

of mechanics of materials equations is that too often the user does

not

understand the derivation and assumptions of the example, and

therefore

cannot appreciate the limitations.

Do you have a reference that might calculate the deflection for a
plate with a multi-component material? This is what would be needed for
pressurized mirror.
Bob Clark
.
User: "jbuch"

Title: Re: Telescope mirrors under tension. 19 Mar 2005 05:26:28 PM
Robert Clark wrote:

jbuch wrote:

Landis says:


Fewer references are available about the ultimate compressive


strengths of materials than tensile strength.

Long compression members have to contend with buckling as a failure
mode. That is one of the reasons there is less attention paid to
compressive strength of structural materials, as a practical matter.

Buckling is ignored in the Landis paper you cite.

You can do an experiment with a toy long balloon, and readily
demonstrate axial compressive buckling failure in a long length at
really low axial loads.......

I wouldn't ignore buckling as a failure mode in postulating these
structures.

Rather than admiring the nuances of a formula.... (and the predicted
wonders of a magic value of a materials pareameter such as Poisson


ratio

of +1) it might be really useful to think of the meaning of the


formula.

The formula is based on bending of a (uniform) beam/disk under self
loading and probably has the boundary condition of fixed edges. I


must

admit to laziness in not going to my bookcase and dragging out Roark,


or

not reading the original

You are encouraged to look at a different formula, one for the


boundary

condition of a controlled line bending moment.... which will tend to
counteract the gravity induced bending.

The goal is to reduce the bending to useful levels, not to find


perfection.

It is long been said that one of the problems with the Roark


compilation

of mechanics of materials equations is that too often the user does


not

understand the derivation and assumptions of the example, and


therefore

cannot appreciate the limitations.



Do you have a reference that might calculate the deflection for a
plate with a multi-component material? This is what would be needed for
pressurized mirror.


Bob Clark

You are to be congratulated on the strength of a one track mind.
I can't see how a multicomponent plate elastic solution corresponds to
"what ould be needed pressurized mirror."
Can you elucidate?
.
User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 05:16:30 AM

You are to be congratulated on the strength of a one track mind.

I can't see how a multicomponent plate elastic solution corresponds

to

"what ould be needed pressurized mirror."

Can you elucidate?

Usually calculations for deflection are for a plate composed of a
single material that is isotropic with a single density, Poisson's
ratio, and Young's modulus.
What I need is a calculation for a plate with one material on the
surface and a different material internally.
Bob Clark
.
User: "jbuch"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 09:15:00 AM
Robert Clark wrote:

You are to be congratulated on the strength of a one track mind.

I can't see how a multicomponent plate elastic solution corresponds


to

"what ould be needed pressurized mirror."

Can you elucidate?



Usually calculations for deflection are for a plate composed of a
single material that is isotropic with a single density, Poisson's
ratio, and Young's modulus.
What I need is a calculation for a plate with one material on the
surface and a different material internally.

Bob Clark

You failed to explain how the bilayer material plate solution is driven
by your desire to have a pressurized mirror.
It seems clear that a pressurized mirror could be handled without a
bilayer elasticity solution.
Why are you claiming that you need the bilayer solution to deal with a
pressurized mirror?
Unles, you are "fishing" for formulas, rather than actually being
responsible for the writing that you do.
I have my impression......
Bye.
--
................................
Keepsake gift for young girls.
Unique and personal one-of-a-kind.
Builds strong minds 12 ways.
Guaranteed satisfaction
- courteous money back
- keep bonus gifts
http://www.alicebook.com
.
User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 20 Mar 2005 09:46:00 PM
jbuch wrote:

Robert Clark wrote:

You are to be congratulated on the strength of a one track mind.

I can't see how a multicomponent plate elastic solution corresponds


to

"what ould be needed pressurized mirror."

Can you elucidate?



Usually calculations for deflection are for a plate composed of a
single material that is isotropic with a single density, Poisson's
ratio, and Young's modulus.
What I need is a calculation for a plate with one material on the
surface and a different material internally.

Bob Clark


You failed to explain how the bilayer material plate solution is

driven

by your desire to have a pressurized mirror.

It seems clear that a pressurized mirror could be handled without a
bilayer elasticity solution.

Why are you claiming that you need the bilayer solution to deal with

a

pressurized mirror?

Unles, you are "fishing" for formulas, rather than actually being
responsible for the writing that you do.

I have my impression......

Bye.

Any formula for calculating the deformation of a pressurized plate
would do. I believe such calculations have been done because of the
work on membrane space mirrors.
Bob Clark
.
User: "jbuch"

Title: Re: Telescope mirrors under tension. 21 Mar 2005 05:12:49 AM
Robert Clark wrote:

jbuch wrote:

Robert Clark wrote:


You are to be congratulated on the strength of a one track mind.

I can't see how a multicomponent plate elastic solution corresponds


to


"what ould be needed pressurized mirror."

Can you elucidate?



Usually calculations for deflection are for a plate composed of a
single material that is isotropic with a single density, Poisson's
ratio, and Young's modulus.
What I need is a calculation for a plate with one material on the
surface and a different material internally.

Bob Clark


You failed to explain how the bilayer material plate solution is


driven

by your desire to have a pressurized mirror.

It seems clear that a pressurized mirror could be handled without a
bilayer elasticity solution.

Why are you claiming that you need the bilayer solution to deal with


a

pressurized mirror?

Unles, you are "fishing" for formulas, rather than actually being
responsible for the writing that you do.

I have my impression......

Bye.



Any formula for calculating the deformation of a pressurized plate
would do. I believe such calculations have been done because of the
work on membrane space mirrors.


Bob Clark

So, I guess this means that we cannot trust what you write.
First you NEED this formula for a compound bi-materials disk, and now
you will take any formula for calculating the deformation of a
pressurized plate.
Why can't you go to the library and look it up in the classical
handbook, because it is almost surely there.
" Roark's Formulas for Stress and Strain "
This would give it to you accurately without some oversimplifications
one gets from copying a version out of someone else's simplified
representation.
Frankly, there have been a lot of pretty smart peoole in the field of
large telescope mirrors, and you are most likely re-discovering older
work by these prior smart thinkers.
.







User: "redbelly"

Title: Re: Telescope mirrors under tension. 18 Mar 2005 12:58:55 PM
Robert Clark wrote:

... Perhaps Landis is considering the materials that
might be used for a space cable such as steel or carbon fibers for
instance, where the tensile strength is larger, since he makes a
comparison to the lengths that could be achieved with current

materials

for a space cable.

I am surprised by the statement that tensile strength is larger for
steel or carbon. Have you looked up the values?
The force in a typical atomic bond gets ever stronger as the atoms are
compressed together.
But if the atoms are pulled apart, the force will eventually get weaker
(after initially getting stronger for small tensile displacement of the
atoms). Unless there is something unusual about the bonding, that
would mean tensile strength is weaker than compressive strength in most
materials.
Mark
.
User: "Aidan Karley"

Title: Re: Telescope mirrors under tension. 18 Mar 2005 07:00:11 PM
In article <1111172335.638414.292920@l41g2000cwc.googlegroups.com>,
Redbelly wrote:

I am surprised by the statement that tensile strength is larger for
steel or carbon. Have you looked up the values?

Ultimate strengths are different from real-world strengths. The
ultimate tensile strength of the minerals that make up concretes are
comparable with the tensile strength of steel, but in the Real World
(TM) the stresses in a LUMP (bLOODY cAPSlOCK KEY!) of concrete are
amplified at the boundaries of discontinuities in the material, from
where brittle fractures propagate, following the concentrated stress at
the tip of the propagating fracture. Steels (metals in general) however
are ductile, and fail by flowing and increasing the stress as the
cross-sectional area reduces (consequence of conservation of volume).
The ultimate tensile strength of a material is determined by the
strength of the inter- and intra- particular bonds (for molecular
materials; for atomic materials the particles are atoms, for complex
materials, the particles may be molecules, or grains in an aggregate
like concrete. The intra-molecular bonds in a material like carbon
nanotube fibre are very strong, but the technological challenge is to
combine the nanotubes with a binding material with comparable strength,
and which binds tightly to the nanotube. This is a major chemical
challenge (which may not have a solution).
Knotting the fibers is not a productive line to follow - few
knots can retain even 50% of the fibre's strength, which does not give
sufficient pay-off to offset the high cost of the knotting procedures.
("Knotting" includes continuous processes such as braiding.) Gluing the
fibers with a suitably strong matrix is well-managed - look at
glass-fibre-reinforced plastic (to give it it's proper name - sorry,
Dad is a chemist in that industry; Pedants-R-Us) or the rumoured
titanium-fibre composites that the kill-bois are using for their latest
bit of corpse-making machinery.
--
Aidan Karley,
Aberdeen, Scotland,
Location: 57°10'11" N, 02°08'43" W (sub-tropical Aberdeen), 0.021233
.
User: "redbelly"

Title: Re: Telescope mirrors under tension. 19 Mar 2005 07:00:23 AM
Mati, Aidan,
Thanks for your responses.
Mark
.
User: ""

Title: Re: Telescope mirrors under tension. 19 Mar 2005 04:48:42 PM
In article <1111237222.990526.4350@z14g2000cwz.googlegroups.com>, "redbelly" <redbelly98@yahoo.com> writes:

Mati, Aidan,

Thanks for your responses.

You're very welcome.
Mati Meron | "When you argue with a fool,
meron@cars.uchicago.edu | chances are he is doing just the same"
.



User: ""

Title: Re: Telescope mirrors under tension. 18 Mar 2005 04:32:12 PM
In article <1111172335.638414.292920@l41g2000cwc.googlegroups.com>, "redbelly" <redbelly98@yahoo.com> writes:

Robert Clark wrote:

... Perhaps Landis is considering the materials that
might be used for a space cable such as steel or carbon fibers for
instance, where the tensile strength is larger, since he makes a
comparison to the lengths that could be achieved with current

materials

for a space cable.


I am surprised by the statement that tensile strength is larger for
steel or carbon. Have you looked up the values?

The force in a typical atomic bond gets ever stronger as the atoms are
compressed together.

But if the atoms are pulled apart, the force will eventually get weaker
(after initially getting stronger for small tensile displacement of the
atoms). Unless there is something unusual about the bonding, that
would mean tensile strength is weaker than compressive strength in most
materials.

Well, a practical reason is not the strength of the bonds but
microcracks. For any practical material that is not a single molecule
(hence the interest in nanotubes) the tensile strength is determined
by the sohesion between the grains, not the strength of atomic bonds,
and is typically some 2 orders of magnitude lower than what you would
expect based on atomic bonds. Now, when you apply significant tension
on a practical material, microcracks start opening in weaker spots
between the grains. This reduces the effective area over which the
tension acts, so stress goes up, more microcracks are opening, and at
some point you get a runaway catastrophic process. Same does not
occur under compression (where, if anything, microcracks are closing,
not opening).
Mati Meron | "When you argue with a fool,
meron@cars.uchicago.edu | chances are he is doing just the same"
.

User: "tj Frazir"

Title: Re: Telescope mirrors under tension. 18 Mar 2005 08:07:19 PM
Its retarded to waist your time on a worthless idia . Nothing that
tall is safe and nothing is going to bend its way into orbit .
If a mass moves up the tower then the tower will speed up .
A cold and then hot tower will snap off , load its self with ice , get
caught on a city or have space junk knock it over.
forget it .
You nead to do something else worth doing and you nead to know when to
stick to a project and when to let go of one.
IF you let go of the stupid thing a better solution will warnt
invesigation just to be used or discarded for the same reasons.
Build a hydroelectric or somthing.
learn to make money in trade leads ad load ships.
go find 4 tons of platinum !!
biuld a spectrometer and image gold from space.
.

User: "Robert Clark"

Title: Re: Telescope mirrors under tension. 19 Mar 2005 10:36:31 AM
redbelly wrote:

Robert Clark wrote:

... Perhaps Landis is considering the materials that
might be used for a space cable such as steel or carbon fibers for
instance, where the tensile strength is larger, since he makes a
comparison to the lengths that could be achieved with current

materials

for a space cable.


I am surprised by the statement that tensile strength is larger for
steel or carbon. Have you looked up the values?

The force in a typical atomic bond gets ever stronger as the atoms

are

compressed together.

But if the atoms are pulled apart, the force will eventually get

weaker

(after initially getting stronger for small tensile displacement of

the

atoms). Unless there is something unusual about the bonding, that
would mean tensile strength is weaker than compressive strength in

most

materials.

Mark

The compressive strengths are given in Table 1 and tensiles in Table
2 in the Landis paper. In these tables the tensile is greater than the
compressive for steel and graphite.
But really for this application this is not the relevant question
since for a telescope mirror you don't want the stresses to be anywhere
near the failure limits. In this case the important strength parameter
is the Young's modulus which measures how great is the linear
deformation by applied pressure. For most materials this is same in
both tension and compression. However, it might be useful as well to
find materials for which the modulus is significantly greater in
tension than in compression.
Bob Clark
.





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