Atmospheric circulations of terrestrial planets orbiting low-mass stars

By Adam R. Edson, Sukyoung Lee, P. R. Bannon, J. Kasting, David D. Pollard. 2011

138 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/f53418f23c6998e413a4c7624b8653a6f5e8cad1

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In Astronomy and Astrophysics

Citations in the corpus

STABILIZING CLOUD FEEDBACK DRAMATICALLY EXPANDS THE HABITABLE ZONE OF TIDALLY LOCKED PLANETS (2013, background): “Furthermore, simulations in a different GCM, GENESIS (Edson et al. 2011, 2012), also show a high albedo for tidally locked planets.”
The Habitability of Planets Orbiting M-dwarf Stars (2016, background): “…is fixed is subject to enhanced radiative cooling (Heng & Kopparla, 2012), weakened low-latitude zonal winds (which also cool a planet), and increased atmospheric latent and oceanic diffusive heat transport, which could reduce day-night temperature differences on the planet (Edson et al., 2011).”
HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: DEPENDENCE ON PLANETARY MASS (2014, background): “For cool stars (Teff ≤ 4500 K), the inner HZ is a function of tidal locking radius (Edson et al. (2011), dashed and solid black line in Fig.”
How to Characterize Habitable Worlds and Signs of Life (2017, background): “…of the HZ (see, e.g., Forget & Pierrehumbert 1997, Lorenz et al. 1997, Joshi 2003, Williams & Pollard 2002, Lopez et al. 2005, Selsis et al. 2007, Edson et al. 2011, Zsom et al. 2012, Goldblatt et al. 2013, Leconte et al. 2013a,b, 2015, Vladilo et al. 2013, Wordsworth & Pierrehumbert 2014, Yang…”
Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets (2017, background): “TRAPPIST-1f, g and h planets have rotation periods ∼ 101 Earth days and they lie thus near the transition between slow and fast rotating regimes (Edson et al. 2011; Carone et al. 2015, 2016).”
THE INNER EDGE OF THE HABITABLE ZONE FOR SYNCHRONOUSLY ROTATING PLANETS AROUND LOW-MASS STARS USING GENERAL CIRCULATION MODELS (2016, background): “Whether atmospheric circulation of one planet is in the rapidly rotating or slowly ro- tating regime mainly depends on the ratio of Rossby deformation radius to the planetary radius (Edson et al. 2011; Showman et al. 2013; Carone2014).”
A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone (2013, background): “Considerable work has shown that thicker atmospheres are able to redistribute dayside heat to produce clement conditi s (Joshi et al. 1997; Joshi 2003; Edson et al. 2011; Pierrehumbert 2011; Wordsworth et al. 2011).”