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Just seen some pictures of Hubble, and The "Very Large Telescope"
(original name) in Chile. It made me think. With a reasonable space based industry, moon mining, metal working, aluminium and glass production, precision engineering, how big an optical telescope could be built in zero-g? What are the limits? Could a 100m diameter optical telescope be built? what would it see? As for radio telescopes, what are the limits are baseline inferometry? what would a few telescopes, each say 3km across, in solar orbit, say 1 billion km apart be able to achieve? |
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wrote:
Just seen some pictures of Hubble, and The "Very Large Telescope" (original name) in Chile. It made me think. With a reasonable space based industry, moon mining, metal working, aluminium and glass production, precision engineering, how big an optical telescope could be built in zero-g? What are the limits? Could a 100m diameter optical telescope be built? what would it see? Heck, they are seriously looking at doing this on the ground, including exactly the studies you describe: http://www.eso.org/projects/owl/publ..._Messenger.htm Several times larger, at the very least, should be possible in space. As for radio telescopes, what are the limits are baseline inferometry? what would a few telescopes, each say 3km across, in solar orbit, say 1 billion km apart be able to achieve? Good question. We know from pulsar studies that coherence is maintained at the microsecond level all the way around the earth's orbit. We can't measure any better now, but there is no obvious reason why a humongous interferometer would not give resolution roughly equal to wavelength/spacing (in radians). We have done correlation from high orbit to earth, and it works as expected, so single dishes up to 36,000 km diameter (!) would work. Two of these on opposite sides of the sun would be a rather powerful facility. Lou Scheffer |
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wrote in news:1108941878.780319.37180
@z14g2000cwz.googlegroups.com: What are the limits? Could a 100m diameter optical telescope be built? what would it see? Here's a project for a ground-based 100 meter telescope (that's about 328 feet!). http://www.eso.org/projects/owl/ High angular resolution can be, and is being, achieved with arrays of optical telescopes. This is probably more practical than a mirror of some arbitrary maximum size. The OWL barely looks practical at all. --Damon |
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In article ,
Rand Simberg wrote: What are the limits? Could a 100m diameter optical telescope be built? Possibly, but there'd be little point, since you can get equivalent resolution with multiple-mirror systems. Actually, there are groups working on concepts for a 100m ground-based telescope, notably the European OWL project. The main mirror *is* segmented, but apparently there are practical advantages in having a single filled aperture rather than a wide scattering of smaller mirrors. There's no reason why you couldn't build an OWL in space, although it would be an expensive project if it used current infrastructure. -- "Think outside the box -- the box isn't our friend." | Henry Spencer -- George Herbert | |
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In article . com,
wrote: What are the limits? Could a 100m diameter optical telescope be built? what would it see? Look into the OWL, the OverWhelmingly Large telescope, a 100 meter ground-based telescope. http://www.eso.org/projects/owl/ -- David M. Palmer (formerly @clark.net, @ematic.com) |
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Damon Hill wrote:
High angular resolution can be, and is being, achieved with arrays of optical telescopes. This is probably more practical than a mirror of some arbitrary maximum size. The OWL barely looks practical at all. There's a 30 meter telescope project (a kind of a small OWL) that would cost about $600 M to build. Hey, that's less than one shuttle launch. Paul |
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wrote in message
ups.com... With a reasonable space based industry, moon mining, metal working, aluminium and glass production, precision engineering, how big an optical telescope could be built in zero-g? What are the limits? Could a 100m diameter optical telescope be built? what would it see? I remember Gerard O'Neill (of High Frontier fame) once wrote a paper on such a concept. He suggested a vast array of multiple mirror segments 1 meter across each. He recommended an independent RCS on each segment. It might seem tempting to just attach them all to some kind of framework, but he insisted that with temperature differences, etc. that would be the last thing you'd want to do. I forget now what size array he was talking about, but I remember him saying you would not only be spotting extrasolar planets, you'd be charting weather systems on them. -- Regards, Mike Combs ---------------------------------------------------------------------- Member of the National Non-sequitur Society. We may not make much sense, but we do like pizza. |
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Henry Spencer wrote:
Actually, there are groups working on concepts for a 100m ground-based telescope, notably the European OWL project. The main mirror *is* segmented, but apparently there are practical advantages in having a single filled aperture rather than a wide scattering of smaller mirrors. Light buckets on Earth have historically been spectrometry workhorses. Two excellent cases in point being extra-solar planet hunting and high-Z supernova searches (both of which have produced ground breaking science within the last decade). For that you very much want a whole heck of a lot of light gathering area and you really don't want to mess around with futzy issues like nulling and whatnot. With adaptive optics and the bleeding edge of interferometry it has become possible to compete at the high end (with space based observatories) in more than just spectrometry, but that's still their bread and butter. There's no reason why you couldn't build an OWL in space, although it would be an expensive project if it used current infrastructure. However, there is a realm of space access cost where constructing something like a 100m telescope in space would actually be cheaper than doing so on Earth. Probably somewhere around an order of magnitude cheaper than today's launch costs, though that's just a SWAG. |
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