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The Kepler telescope is discovering many planets by searching for changes in a star's brightness when a planet transits across the face of a star. However, with that method of observing planets, we cannot see any of the details of the planet. While Kepler may not be powerful enough to see details of the planet, maybe future telescopes, such as James Webb will. To see the details it will have to see the bright side of the planet, so it will have to see the planets while they are on the far side of the star. To do that they can use solar occlusion so that the light from the star will not interfere with the light from the planet. The diagram below shows how it could work.
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In article ,
Elassoto writes: The Kepler telescope is discovering many planets by searching for changes in a star's brightness when a planet transits across the face of a star. However, with that method of observing planets, we cannot see any of the details of the planet. Kepler gives the planet's orbital parameters, its diameter, and sometimes information on the mass if there are multiple planets. While Kepler may not be powerful enough to see details of the planet, maybe future telescopes, such as James Webb will. If you are talking about resolving the planet's disk, I don't think so. To see the details it will have to see the bright side of the planet, so it will have to see the planets while they are on the far side of the star. More generally, one would like to track the brightness of the planet around its orbit. The Spitzer Space Telescope has already done some of that. It has also observed secondary transits for quite a few planets now. This gives the infrared emission of the day side of the planet, which can tell something about the planet's composition or atmosphere. To do that they can use solar occlusion You seem to be talking about a coronagraph, which JWST will have: http://www.stsci.edu/jwst/instrument.../#coronagraphy It's actually quite a bit trickier than just putting a black spot in the focal plane. A very few exoplanets have already been directly imaged by ground- based telescopes. -- Help keep our newsgroup healthy; please don't feed the trolls. Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA |
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Thank you for that excellent information and article. I hope that JWST makes some nice discoveries for us.
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On 13/01/2012 10:39 AM, Elassoto wrote:
The Kepler telescope is discovering many planets by searching for changes in a star's brightness when a planet transits across the face of a star. However, with that method of observing planets, we cannot see any of the details of the planet. While Kepler may not be powerful enough to see details of the planet, maybe future telescopes, such as James Webb will. To see the details it will have to see the bright side of the planet, so it will have to see the planets while they are on the far side of the star. To do that they can use solar occlusion so that the light from the star will not interfere with the light from the planet. The diagram below shows how it could work. Some exoplanets have already been imaged by the Hubble and various terrestrial telescopes. But of course, they are all gas giants, and pretty far away from their stars. And even still, the images are really nothing more than fuzzy pixels. Astronomers Capture First Exoplanet Images : Discovery Space http://dsc.discovery.com/space/im/ex...ra-seager.html Yousuf Khan |
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On Jan 13, 7:39*am, Elassoto wrote:
The Kepler telescope is discovering many planets by searching for changes in a star's brightness when a planet transits across the face of a star. However, with that method of observing planets, we cannot see any of the details of the planet. While Kepler may not be powerful enough to see details of the planet, maybe future telescopes, such as James Webb will. To see the details it will have to see the bright side of the planet, so it will have to see the planets while they are on the far side of the star. To do that they can use solar occlusion so that the light from the star will not interfere with the light from the planet. The diagram below shows how it could work. +-------------------------------------------------------------------+ |Filename: solarocclusion.jpg * * * * * * * * * * * * * * * * * * * | |Download:http://www.spacebanter.com/attachment.php?attachmentid=3905| +-------------------------------------------------------------------+ -- Elassoto Yes, we need those remote starshades (solar occlusion) to assist all forms of astronomy. http://translate.google.com/# Brad Guth, Brad_Guth, Brad.Guth, BradGuth, BG / “Guth Usenet” |
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On Jan 19, 8:09*am, Elassoto wrote:
Thank you for that excellent information and article. I hope that JWST makes some nice discoveries for us. +-------------------------------------------------------------------+ +-------------------------------------------------------------------+ -- Elassoto Most of us well be quite dead or at least bankrupt by the time it gets going. Are you happy now? |
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Space telescopes are having trouble seeing planets next to brighter stars. It sounds like stellar coronagraphs can only help so much, but why? Is light still getting around the the stellar corongraphs?
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