Our first task was to estimate the planet's radius and mid-transit time by creating a light curve based on this data in the Allesfitter program. The program evaluated our curve and determined how accurate we were and we obtained the correct value to compare with our result. We saw that our estimate of the transit depth had 2,6% deflection from Allesfitter, that was not bad for beginners. From the Allesfitter program we also received more data - the mass of the planet, temperature and time period… (see attached pictures). Radius A light curve shows percentage values of light coming from the star in time. The difference between the smallest measured value and the maximum is called transit depth. It’s approximately the ratio of the area of the planet's disc and the area of the star's disc. With this ratio, we determined the planet radius (see calculation below) Volume, density The planet's radius is ca. 2.45 larger than of our planet Earth, which means its volume is appro...
Welcome to the blog about our amazing journey through space! Within the scope of the project Hack an exoplanet organized by ESA we turned into space detectives - astrophysicists - and we analysed real data from ESA's satellite Cheops. On this blog, you can read about every step we made to explore the exoplanet TOI-560 c. We recommend reading this blog from the first article to the last, so you can fully enjoy our discoveries! Good luck, detective!