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First results from CoRoT. C. Karoff H. Kjeldsen , T. Arentoft, J. Christensen-Dalsgaard Danish AsteroSeismology Centre, University of Aarhus, Department of Physics and Astronomy, Denmark Instrument Center for Danish Astrophysic, Denmark. Convection, Rotation & planetary Transits.
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First results from CoRoT C. Karoff H. Kjeldsen , T. Arentoft, J. Christensen-Dalsgaard Danish AsteroSeismology Centre, University of Aarhus, Department of Physics and Astronomy, Denmark Instrument Center for Danish Astrophysic, Denmark
Convection, Rotation & planetary Transits CoRoT has two scientific objectives: • Stellar Seismology • Search for Exoplanets. Proteus platform • 27 cm afocal telescope • 4 2kx4k frame transfer CCDs • Colors provided by a prism in front of two of the CCDs
27th of December 2006 • CoRoT was launched with a Soyuz rocket from Baikonur on the 27th of December 2006. • Precision for Asteroseismology: 0.74 ppm in 5 days. • Precision for Planets: 0.075 % i one hour.
Corot-Exo-1b Period: 1.5 d Mass: 1.3 MJ Radius: 1.78 RJ
M(v): 3.39 • L/Lsun: 3.5 • Teff: 6457 K • Vsin(i): 10.9 km/s • R/Rsun: 1.5 • /Sun: 0.388 • Prot: 7.0 d
Intensity and Sunspots Intensity from the GOLF instrument on the SOHO satellite (green channel). Intensitygram from the MDI instrument on SOHO.
Sunspots and Rotation Period Solar rotation period at equator: 24 d
Sunspots and Rotation Period Solar rotation period at equator: 24 d
Sunspots and Rotation Period Solar rotation period at equator: 24 d
Sunspots and Rotation Period Solar rotation period at equator: 24 d Typical spot size: 0.001 Large spots: 0.002
Sunspots and Rotation Period Rotation period: 24 d Typical spot size: 0.001% (D ~ 44.000 km) Large spots: 0.002% (D ~ 76.000 km) Spot lifetime: 7-24 days (0.3-1.0 rot)
HD49933Spots and Rotation Period Rotation period: 3.5 d
HD49933Spots and Rotation Period Rotation period: 3.5 d
HD49933Spots and Rotation Period Rotation period: 3.5 d Typical spot size: 0.0005 (D ~ 46.000 km) Large spots: 0.0015 (D ~ 80.000 km) Spot lifetime: 5-10 d (1.5-3 rot) Inclination: 30o
Oscillations in The Sun ∆ν0 = 134.5 μHz
HD49933The Large Separation l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 ∆ν0 = 85.6 μHz
HD49933The Large Separation l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 ∆ν0 = 85.6 μHz
The SunThe Small Separation ν02~ 10 μHz
HD49933The Small Separation l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 ν02 = 6 μHz
The SunThe Rotation Splitting Period ~ 24 d ~ 0.5 μHz
HD49933The Rotation Splitting l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 l=0 l=1 Periode ~ 3.5 d ~ 3.3 μHz