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The First Image Of Surface Features On A Sun-Like Star.

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The First Image Of Surface Features On A Sun-Like Star. Robert Clark 06-01-2007
Posted by Robert Clark on June 1, 2007, 7:23 pm
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University Of Michigan Astronomers Capture The First Image Of Surface
Features On A Sun-Like Star.
Ann Arbor MI (SPX) Jun 01, 2007
"University of Michigan astronomers combined light from four widely
separated telescopes to produce the first picture showing surface
details on a sun-like star beyond our solar system. The image of the
rapidly rotating, hot star Altair is the most detailed stellar picture
ever made using an innovative light-combining technique called optical
interferometry, said U-M astronomer John Monnier."
http://www.spacedaily.com/reports/University_Of_Michigan_Astronomers_Capture_The_First_Image_Of_Surface_Features_On_A_Sun_Like_Star_999.html

Then could this mean that rather than needing a single large mirror
you could combine the light from small, widely separated mirrors to
create a single high resolution image, as has been done for radio
astronomy for several years?
This would be especially useful for space telescopes where you don't
have to worry about using adaptive optics (which works better in the
infrared rather than the optical.)


Bob Clark


Posted by Eric Gisse on June 1, 2007, 8:19 pm
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[...]

Impressive. That means directly imaging extrasolar planets is within
reach.


Posted by robert casey on June 1, 2007, 11:40 pm
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Eric Gisse wrote:
>
> [...]
>
> Impressive. That means directly imaging extrasolar planets is within
> reach.
>

Hope so, but I suspect that the dynamic range of the differing levels of
light may not be good enough. That the glare from the star may wash the
planet out...

Posted by Henry Spencer on June 2, 2007, 5:39 pm
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> Then could this mean that rather than needing a single large mirror
>you could combine the light from small, widely separated mirrors to
>create a single high resolution image, as has been done for radio
>astronomy for several years?

Yes. Various groups have been working on this for the last 10-20 years;
the idea is not new, although it's difficult and practical use of it is
still quite experimental. Interferometry is why the European Southern
Observatory, for example, was built with four huge telescopes rather than
just one.

Huge telescopes? Yes, even with interferometry! It tends to require a
fair amount of light -- you need a substantial number of photons per
second to form detectable interference fringes -- so it does work better
with lots of mirror area.

> This would be especially useful for space telescopes where you don't
>have to worry about using adaptive optics (which works better in the
>infrared rather than the optical.)

Yes and no. The problem in doing it with space telescopes is that the
spacing between the mirrors has to be controlled very tightly indeed, to
a fraction of the wavelength of light, so there are real advantages to
having them firmly anchored to something heavy and solid. People are
working on doing it in space, but the challenges are even greater.

Most "optical" interferometry is likewise done in the near infrared rather
than the visible, for the same reason as for adaptive optics: the longer
wavelength makes all sorts of optical things easier.
--
spsystems.net is temporarily off the air; | Henry Spencer
mail to henry at zoo.utoronto.ca instead. | henry@spsystems.net

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