TOI 5747b Transit Simulation With Real Data!

Published: 21 January 2024
on channel: AstroLyn

LCO 1 Meter data showcasing transit coverage of exoplanet candidate TOI 5747b with no limb darkening coefficients..... Possible terrestrial sized exoplanet around TOI 5747 which is a Early Class M Red Dwarf Star with a mass less than 0.42M of the sun and 0.41 less than that of our sun and a Orbital Inclination of 89.9* and Orbital Radius of 0.015 AU with a 22.7hr orbital period and 55:58 minute transit duration ! Initial observation done and made by Dr. Collins team of CFA Harvard, data reduction made by me via LCO archive

Theories:

1. Possible Tidal Locking due to gravitational tug from host star

2. Super Earth Category as predicted mass is 2.85 maybe higher as more observations come in

3. Internal day side maybe 988 kelvin or 712* Celsius/ 1350*F, while nightside maybe cooler than 700 kelvin or 412* Celsius/ 800.33*F or lower, just an initial guess!

NOT MY MUSIC ALL CREDIT GOES TO ‪@HansZimmer‬

#astronomy #exoplanets #coding #hanszimmer #mountains

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