Ozturk, O.Erdem, A.2025-01-272025-01-272018978-0-7354-1627-70094-243Xhttps://doi.org/10.1063/1.5025961https://hdl.handle.net/20.500.12428/2793733rd International Physics Congress of the Turkish-Physical-Society (TPS) -- SEP 06-10, 2017 -- Bodrum, TURKEYWe reexamine the classification of transiting exoplanets proposed by Hansen & Barman (2007) based on equilibrium temperatures and Safronov numbers. We used more sensitive data, namely, photometric and spectroscopic orbital solutions, of 263 well-known planets given in The Exoplanet Data Explorer, while Hansen & Barman (2007) used data on 18 transiting planets. Diagrams of the planet gravity vs. orbital period, planet gravity vs. equilibrium temperature, and Safronov number vs. equilibrium temperature of the 263 transiting planets show that the division of planets into two classes is indistinct.eninfo:eu-repo/semantics/closedAccessConference Object193510.1063/1.5025961N/AWOS:0004459561000072-s2.0-85043980297Q4