Clim. Past, 10, 697–713, 2014 Open Access www.clim-past.net/10/697/2014/ Climate doi:10.5194/cp-10-697-2014 © Author(s) 2014. CC Attribution 3.0 License. of the Past The faint young Sun problem revisited with a 3-D climate–carbon model – Part 1 G. Le Hir1, Y. Teitler1,*, F. Fluteau1, Y. Donnadieu2, and P. Philippot1 1IPGP, Institut de Physique du Globe de Paris, Sorbonne Paris cité, Université Paris Diderot, UMR7154, 75005, France 2LSCE, CNRS-CEA-UVSQ, 91191 Gif-sur-Yvette, France *now at: Centre for Exploration Targeting, University of Western Australia, Crawley, Australia Correspondence to: G. Le Hir (
[email protected]) Received: 6 February 2013 – Published in Clim. Past Discuss.: 22 March 2013 Revised: 17 February 2014 – Accepted: 18 February 2014 – Published: 3 April 2014 Abstract. During the Archaean, the Sun’s luminosity was 18 1 Introduction to 25 % lower than the present day. One-dimensional radia- tive convective models (RCM) generally infer that high con- Sagan and Mullen (1972) argued from solar models that, in centrations of greenhouse gases (CO , CH ) are required to 2 4 the early Archaean, the young Sun’s luminosity was 25 % prevent the early Earth’s surface temperature from dropping lower compared to now. According to climate models, the below the freezing point of liquid water and satisfying the weakness of the young Sun’s brightness would have implied faint young Sun paradox (FYSP, an Earth temperature at least that Earth’s surface temperature was well below the freezing as warm as today). Using a one-dimensional (1-D) model, point of water during the first two billion years of its history.