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Feb S&T article on interferometry to determine planet shapes
Seems like about 30 years ago, I remember an article about a speckle
interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? |
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Sorry, title should have said "star" shapes
Rich wrote: Seems like about 30 years ago, I remember an article about a speckle interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? |
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Sorry, title should have said "star" shapes
Rich wrote:
Rich wrote: Seems like about 30 years ago, I remember an article about a speckle interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? HST was also capable of imaging Betelgeuse (and, even more impressive, measurnig differentia Doppler shifts from its rotation from side to side - the bright spot is around the north ple). The big deal is that there were only a literal handful of stars (actually, only Betelgeuse and R Doradus come to mind immediately) for which either speckle or HST could see structure on the disk. For a few other stars, speckle data could give an effective diameter. What's new is that they can now go to stars with more than a factor of 10 smaller apparent size, with enough preccision for not only diameyter but shape measurements. Betelgeuse has a diameter (depending on wavelength) of around 0.05". Regulus is something like 0.0016". (For that matter, we've been able to image the surface of one star in considerable detail for many years...) Bill Keel |
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Feb S&T article on interferometry to determine planet shapes
On 18 Jan 2007 14:57:42 -0800, Rich wrote:
Seems like about 30 years ago, I remember an article about a speckle interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? The author of the article on speckle interferometry you refer to in S&T in the 1970s is also the principal investigator of the CHARA Array on Mt. Wilson that's described in the current issue of S&T. I can guarantee you he didn't raise millions to build the CHARA Array just so he could duplicate the work he did decades ago. The work described in the current article is new and groundbreaking. Interestingly, much of the speckle interferometry described in the 1970s article was done on the Hooker 100" telescope on Mt. Wilson, which is located right next to the CHARA Array. The 100" was where astronomical interferometry research was first done (Michelson did some testing at Lick Observatory first). The full-page photo in the current article showing them both is not the closest point between the two but was the best vantage point to get both a CHARA scope and the 100" in the photo (I know -- I took the photo, and I spent a lot of time trapsing around the mountain trying different angles). The CHARA beam-combining facility is just a few meters from the 100" dome. In one early design there were light tubes passing *through* the 100" dome but fortunately that turned out to be unecessary and it now passes harmlessly by about 5 meters from the 100" dome's outer wall. Mike Simmons |
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Feb S&T article on interferometry to determine planet shapes
"Mike Simmons" wrote
The author of the article on speckle interferometry you refer to in S&T in the 1970s is also the principal investigator of the CHARA Array on Mt. Wilson that's described in the current issue of S&T. Nice photos of the array in there. Finally an outfit like CHARA gets a photographer with "professional" skills! ;-) |
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Feb S&T article on interferometry to determine planet shapes
On Fri, 19 Jan 2007 09:04:21 -0700, Howard Lester wrote:
"Mike Simmons" wrote The author of the article on speckle interferometry you refer to in S&T in the 1970s is also the principal investigator of the CHARA Array on Mt. Wilson that's described in the current issue of S&T. Nice photos of the array in there. Finally an outfit like CHARA gets a photographer with "professional" skills! ;-) HA! "Professional" indeed. Have you seen the sunset picture of the MMTO on their web site? Now THAT'S a professional shot. :-) Thanks Howard. Mike Simmons |
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Feb S&T article on interferometry to determine planet shapes
"Mike Simmons" wrote Nice photos of the array in there. Finally an outfit like CHARA gets a photographer with "professional" skills! ;-) HA! "Professional" indeed. Have you seen the sunset picture of the MMTO on their web site? Now THAT'S a professional shot. :-) Thanks Howard. Mike Simmons Thank you, Mike, and you're welcome! You even take good photos of goofy looking guys holding mirror-casting refractory materials. ;-) |
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Feb S&T article on interferometry to determine planet shapes
On Fri, 19 Jan 2007 11:47:54 -0700, Howard Lester wrote:
Thank you, Mike, and you're welcome! You even take good photos of goofy looking guys holding mirror-casting refractory materials. ;-) Some subjects are too good to mess up. Watch yourself or I'll post something like that for all of SAA to see. Mike Simmons |
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Feb S&T article on interferometry to determine planet shapes
Rich wrote: Seems like about 30 years ago, I remember an article about a speckle interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? Very likely you have missunderstood the article, in your zeal to missunderstand and confuse and lie to yourself and everyone? .. . . |
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Feb S&T article on interferometry to determine planet shapes
Frog Crossing wrote:
Rich wrote: Seems like about 30 years ago, I remember an article about a speckle interferometry project in Sky & Tel that supposedly showed actual spots on Betelguese. I'm wondering what the big brag is for only illustrating the shape of a star today (Regulus for e.g.) if they were capable of imaging a star surface years ago? Very likely you have missunderstood the article, in your zeal to missunderstand and confuse and lie to yourself and everyone? . . . Tut, tut... see: http://antwrp.gsfc.nasa.gov/apod/ap990605.html and: http://www.aavso.org/vstar/vsots/1200.shtml and: http://adsabs.harvard.edu/abs/1982A&A...115..253B and: http://www.obs-hp.fr/~dejonghe/page3.htm Hm.. Why dont you both use google instead of calling each other names? You might learn something. |
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