id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
cusj-12468	Bhaumik, Sattik	SEPHI of Exoplanets Kepler-504 b, Kepler-315 b and Kepler-315 c	2025	8	.pdf	application/pdf	3610	158	47	Adopting SEPHI, with respect to ESI, the results for SEPHI values and ESI values for the exoplanets along with planets from our Solar System have been added to give A reference base for understanding SEPHI’s relevance. The calculations conducted in this paper were built on the data used previously such as calculation for relative planetary mass (mp), relative planetary radius (rp), relative escape velocity (ve), stellar luminosity (Ln), relative density (⍴p), Stellar Effective Temperature (Teff), which forms the basis for calculating the four composition criteria used to determine SEPHI values for each of the exoplanets.4 These particular criteria are essential to understand whether those basic conditions are compatible enough to allow Earth-based life (carbon-based life) on that exoplanet.	cache/cusj-12468.pdf	txt/cusj-12468.txt