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Home > Science > Astronomy > Extrasolar Planets
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Directory of Web Resources @ Expo Central : Extrasolar Planets
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Science > Astronomy > Extrasolar Planets : Categories
Science > Astronomy > Extrasolar Planets : Web Resources
Science > Astronomy > Extrasolar Planets : Web-Sites
| 11. Extrasolar Planet Detection with the AFOE
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| Extrasolar Planet Detection with the AFOE The Advanced Fiber-Optic Echelle (AFOE) spectrometer is a fiber-fed, bench-mounted echelle spectrograph, located at the 1.5m telescope of the Whipple Observatory, near Tucson, Arizona. |
| http://cfa-www.harvard.edu/afoe/espd.html |
| 13. Full-sky Astrometric Mapping Explorer
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| FAME is an astrometric satellite designed to determine with unprecedented accuracy the positions, distances, and motions of 40 million stars within our galactic neighborhood. It is a collaborative effort between the U.S. Naval Observatory (USNO) and several other institutions. |
| http://www.usno.navy.mil/FAME/ |
| 17. James Webb Space Telescope
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| The James Webb Space Telescope, or JWST, is a large, infrared-optimized space telescope designed to study the formation of the first stars and galaxies, the evolution of galaxies and the production of elements by stars, and the process of star and planet formation. |
| http://www.jwst.nasa.gov/science/Starsandplanets.html |
| 19. Microlensing Observations in Astrophysics (MOA)
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| A joint Japanese/New Zealand project established to carry out astrophysical observations using a gravitational microlensing technique. Applications include research for extra-solar planets, dark matter, stellar atmospheres, and variable stars. Page includes information on imaging processes, the group's telescope, and publications. |
| http://www.physics.auckland.ac.nz/moa/ |
| 20. Microvariability and Oscillations os STars
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| Detection and characterisation of: (1) acoustic oscillations in Sun-like stars, including very old stars (metal-poor subdwarfs) and magnetic stars (roAp), to probe seismically their structures and ages; (2) reflected light from giant exoplanets closely orbiting Sun-like stars, to reveal their sizes and atmospheric compositions; and (3) turbulent variations in massive evolved (Wolf-Rayet) stars to understand how they add gas to the interstellar medium. |
| http://www.astro.ubc.ca/MOST/ |
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Science > Astronomy > Extrasolar Planets : Web Resources
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