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Tranzit exoplanety - detail
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Rp: |
1.264 +/- 0.071 RJup |
1.383 -0.030+0.030 RJup |
R*: |
1.096 +/- 0.056 RSun |
fixed, errors included in i |
A: |
0.0238 +/- 0.0004 AU |
fixed, errors included in i |
Per: |
1.327347 days |
fixed |
i : |
86 +/- 1.3 ° |
82.61
-0.36|1.87+0.39|2.28 °
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> Zpět na seznam seznam pozorování
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> Předpověď minim < > Tranzity exoplanet <
Nová data MEDÚZA:
CCD: P. Dubovský: NOVACas2020 Cas, NOVAPer2020 Per, NOVACas2020 Cas, NOVAPer2020 Per, NOVACas2020 Cas, NOVAPer2020 Per, NOVACas2020 Cas, NOVAPer2020 Per, NOVACas2020 Cas, NOVAPer2020 Per, VIZ: P. Dubovský: BB Aur, NSV 16874 Aur, VW Aur, SY Cam, XX Cam, BX Cas, KS Cas, NSV 332 Cas, NSV 650 Cas, ST Cas, UY Cas, V 365 Cas, V 465 Cas, V 764 Cas, VY Cas, TZ Cep, V 730 Cep, AG Dra, Alpha Ori, EV Ori,
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Komentář
objektu HAT-P-36 b
I discovered that the star TYC 3020-2195-1, usually adopted as reference for HAT-P-36, is a variable with amplitude 0.015 magn. and a period of 1h (probably a delta Scuti): www of the light curves of the transit of HAT-P-36b present in ETD were obtained using that star. Giuseppe Marino.
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This observation is in error and can be removed. Correct data is re-imported. Petri Kehusmaa