Nitrogen-enhanced greenhouse warming on early Earth
By C. Goldblatt, M. Claire, T. Lenton, A. Matthews, A. Watson, K. Zahnle. 2009
265 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science, Paleontology
View Paper: https://www.semanticscholar.org/paper/48af7ed9c2f96fceaa0626ac59a3d7f542f5a5d0
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In Astronomy and Astrophysics
- R. Wordsworth
- Francois Forget
- Ehouarn Millour
- F. Selsis
- B. Charnay
- Jean-Baptiste Madeleine
- K. Zahnle
- Benjamin W. Johnson
In Atmospheric Science
- R. Wordsworth
- Ehouarn Millour
- Jean-Baptiste Madeleine
- F. Selsis
- Francois Forget
- T. Robinson
- K. Zahnle
- David Crisp
In Paleontology
Citations in the corpus
- Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “The current amount of nitrogen in Earth’s crust and mantle is highly uncertain and estimated between surface partial pressures of 0.32 - 5.6 bar (e.g., Goldblatt et al. 2009, Johnson and Goldblatt 2015; Marty 1995; Marty and Dauphas 2003).”
- The Nitrogen Budget of Earth (2015, methodology): “Our work not only suggests a higher N mass in the BSE than previous work (Goldblatt et al., 2009), but also arrives at approximately the same value from two independent tactics.”
- Low simulated radiation limit for runaway greenhouse climates (2013, background): “Earth’s atmospheric nitrogen inventory has likely changed with time[29].”
- The faint young Sun problem (2012, background): “Although nitrogen is not a greenhouse gas in itself, a higher partial pressure of atmospheric nitrogen during the Archean would amplify the greenhouse impact of other gases by broadening of absorption lines [Goldblatt et al., 2009].”
- THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES (2012, unknown): “Figure 4(b) represents a first-order improvement on this correction by factors ranging up to 2 in the near-UV and a few percent in the visible, the latter of which affects calculations of paleo-temperatures by ∼1 ◦C (Goldblatt et al. 2009).”
- WATER LOSS FROM TERRESTRIAL PLANETS WITH CO2-RICH ATMOSPHERES (2013, unknown): “ared and Rayleigh scattering in the visible. These eects tend to partially cancel out, with the result that the eect of doubling atmospheric N 2 on Earth is a small increase in surface temperature (Goldblatt et al. 2009). Hydrogen-nitrogen CIA can cause ecient warming in cases when the hydrogen cont”
- GLIESE 581D IS THE FIRST DISCOVERED TERRESTRIAL-MASS EXOPLANET IN THE HABITABLE ZONE (2011, background): “the warming due to other greenhouse gases like CH4 or buffer gases like N2 or Ar (von Paris et al. 2010; Goldblatt et al. 2009; Li et al. 2009).”
- Nitrogen Isotopes and Mantle Geodynamics: The Emergence of Life and the Atmosphere–Crust–Mantle Connection (2013, background): “Mass balance considerations also support massive exchange between the Earth’s surface and the mantle, with an inferred decrease in atmospheric N pressure by a factor of ~2–3 (Goldblatt et al. 2009).”