Low simulated radiation limit for runaway greenhouse climates

By C. Goldblatt, T. Robinson, K. Zahnle, David Crisp. 2013

159 citations recorded by the source corpus.

Subfields: Atmospheric Science, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/4be39d2e4114f1347569d81029f59005e141befe

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Citations in the corpus

Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs (2017, background): “While numerical limitations of the model prevent us from exploring the end state of the runway process where ~T 1600 Ks (Goldblatt et al. 2013), still we can mark where the energy imbalance grows large and temperatures begin to rise uncontrollably.”
High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations (2023, background): “…by impacts from small, icy bodies (Zahnle et al. 1988) or outgassed depending on the mantle composition (Tian & Heng 2023) but would be quickly lost via the runaway greenhouse effect (Goldblatt et al. 2013), as well as being disfavored by high-resolution observations (Ridden-Harper et al. 2022).”
Transient reducing greenhouse warming on early Mars (2016, unknown): “…, 1965; Clough et al. , 1992; Rothman et al. , 2013; Murphy and Koop , 2005; Gruszka and Borysow , 1997; Baranov et al. , 2004; Wordsworth et al. , 2010; Pierrehumbert , 2011; Hansen and Travis , 1974; Claire et al. , 2012; Béguier et al. , 2015; Goldblatt et al. , 2013; Schaefer et al. , 2016].”
WATER LOSS FROM TERRESTRIAL PLANETS WITH CO2-RICH ATMOSPHERES (2013, unknown): “at the planet has always been in a runaway state. Indeed, our clear-sky calculations suggest Earth itself receives close to the limiting runaway ux at present, in agreement with the recent results of Goldblatt et al. (2013) and Kopparapu et al. (2013). When the Solar System formed, Venus received a ”
The Cosmic Shoreline: The Evidence that Escape Determines which Planets Have Atmospheres, and what this May Mean for Proxima Centauri B (2017, background): “This was very important for Earth and Venus because they likely accreted on a 30-100 Myr timespan, and the added energy of accretion pushed both planets above their runaway greenhouse limits (Matsui and Abe 1986; Abe and Matsui 1988; Zahnle et al. 1988; Hamano et al. 2013).”
How to Characterize Habitable Worlds and Signs of Life (2017, background): “…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 et al. 2013, 2014, Fereira et al.…”
Moist Heat Stress on a Hotter Earth (2020, background): “These scaling relationships constrain the limits of planetary habitability (Sherwood & Huber 2010, Goldblatt et al. 2013).”