Title: EXTRA-SOLAR PLANETS
1EXTRA-SOLAR PLANETS
- Dr. Z. E. Musielak
- Department of Physics
- University of Texas at Arlington
2OUTLINE
- Detection of Extra-Solar Planets
- Planets around Nearby Stars
- Stellar Habitable Zones
- Research at UTA
- Conclusions
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3The host star wobbles as a result of moving planet
4Doppler Detection Technique
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7Planetary Transition
8Change in Stellar Brightness Due to Planet
Transition
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10Discoveries of Extrasolar Planets
- First planetary system was discovered by
- Wolszczan Frail (1992)
- around a pulsar PSR 125712
- First planets around solar-type stars were
discovered by - Mayor Queloz (1995)
- Butler Marcy (1996)
- Marcy Butler (1996)
11McDonald Observatory
12Current Status
- As of today (February 20, 2008)
- Doppler technique 260 planets
- Photometric technique 35 planets
- Microlensing method 6 planets
- Pulsar planets 4 planets
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14Orbits of Some Extrasolar Planets
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21 Observational Results
- The discovered planets are more massive than
Jupiter giant planets! - Massive planets are located at small orbits.
- Some giant planets have highly eccentric orbits.
22Stellar Habitable Zones
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25Milky Way Habitable Zone
26 RESEARCH AT UTA
- (1) Star Planet Interactions
- (2) Orbital Stability in Habitable Zones
- (a) Single Stars
- (b) Binary Stars
- (c) Multiple Stellar Systems
27 Stellar Activity and Exoplanets
- Enhancement of stellar activity by exoplanets
(e.g., Ca II HK and X-rays) - Interaction between the stellar and planetary
magnetic fields
Cuntz, Saar Musielak (2000)
Orbital modulations of Ca II in 3 systems
Hot spot following the planet in HD179949
Shkolnik, Walker Bohlender (2003)
28Orbital Stability in Habitable Zone of 51 Peg
29Orbital Stability in Habitable Zone of 47 UMa
Noble, Musielak and Cuntz (2002)
30Orbital Stability in Habitable Zone of HD 210277
Noble, Musielak and Cuntz (2002)
31Orbital Stabilty in Binary Systems
Musielak, Cuntz, Marshall and Stuit (2003)
32 CONCLUSIONS
- As of today, 276 extra-solar planets orbiting
solar-type stars have been discovered. - The discovered planets have masses comparable to
or larger than Jupiter and most of them orbit
near their host stars. - Some of these giant planets have highly eccentric
orbits.
33 FUTURE OBSERVATIONS
- The Keck Interferometer
- Space Interferometry Mission (SIM)
- Terrestrial Planet Finder (TPF)
- The Kepler Photometer
- The Darwin Mission
- Gaia Space Observatory
- The StarLight Mission