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In article ,
"smallg" writes: Belelgeuse is a red giant and relatively nearby. Betelgeuse is a supergiant, actually, but indeed nearby. Measuring angular diameter with interferometry is not really "resolving." Astronomers use "resolve" to mean any method that detects finite angular size. Two-element interferometry (as pioneered by Michelson) "resolves" stellar disks but doesn't "image" them. "Speckle interferometry" detects surface features, though one can quibble whether it's really imaging. Lunar occultations also detect surface features. Modern multi-element interferometers do even better. And as someone mentioned, the disk of Betelgeuse has been imaged with HST; no quibbling possible about that. These studies give quite a bit of information on limb darkening and starspots. The general point is correct, though: study of stars other than the Sun is much hindered by lack of angular resolution, and the VLT micro-lensing study is very much to be commended. -- Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA (Please email your reply if you want to be sure I see it; include a valid Reply-To address to receive an acknowledgement. Commercial email may be sent to your ISP.) |
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