The atmospheres of short-period terrestrial exoplanets

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Degenerecies atm vs inclination dense atmosphere 30° no atmosphere 70° vendredi 10 septembre 2010
- SNR calculations for phasecurve detection based on stellar photon noise only. Main limitations will be stellar variability and instrument stability - the theoretical phase curves are available to anyone who wants to test their observability with a more realistic instrument simulator - if non-transiting planets are observable this way, it increases the number <strong>of</strong> targets by ~10 - new models will include a mixture <strong>of</strong> species (CO2, H2O, CH4,...) and clouds vendredi 10 septembre 2010
Page 1 and 2: The atmospheres of short-period ter
Page 3 and 4: Habitability around M stars • Str
Page 5 and 6: stellar photon noise only instrumen
Page 7 and 8: vendredi 10 septembre 2010 Belu et
Page 9 and 10: The detection and basic characteriz
Page 11 and 12: Animation made with the data from t
Page 13 and 14: vendredi 10 septembre 2010 12
Page 15 and 16: vendredi 10 septembre 2010
Page 17 and 18: vendredi 10 septembre 2010
Page 19 and 20: IR light phase curve curve and clim
Page 21 and 22: vendredi 10 septembre 2010 HZ: Sels
Page 23 and 24: Eccentric planets max max vendredi
Page 25 and 26: IR Earth Vis Palle et al., 2008 ven
Page 27 and 28: Test case for a non-transiting hot
Page 29 and 30: no atmosphere 3.6 µm 4.3 µm 5.9
Page 31 and 32: 1 bar (CO2) 3.6 µm 4.3 µm 5.9 µm
Page 33 and 34: 8.7 µm no atmosphere 0.1 bar (CO2)
Page 35 and 36: 0.1 bar CO2 1 bar CO2 10 bar CO2 ve
Page 37 and 38: Altitude 10 bar (CO2) color = gas t
Page 39 and 40: dayside low-res spectrum of the pla
Page 41 and 42: 0.1 bar CO2 1 bar CO2 10 bar CO2 SN
Page 43: ideal SNR with a 6m telescope integ

The atmospheres of short-period terrestrial exoplanets

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