Literature DB >> 25984919

Habitability of waterworlds: runaway greenhouses, atmospheric expansion, and multiple climate states of pure water atmospheres.

Colin Goldblatt1.   

Abstract

There are four different stable climate states for pure water atmospheres, as might exist on so-called "waterworlds." I map these as a function of solar constant for planets ranging in size from Mars-sized to 10 Earth-mass. The states are as follows: globally ice covered (Ts ⪅ 245 K), cold and damp (270 ⪅ Ts ⪅ 290 K), hot and moist (350 ⪅ Ts ⪅ 550 K), and very hot and dry (Tsx2A86;900 K). No stable climate exists for 290 ⪅ T s ⪅ 350 K or 550 ⪅ Ts ⪅ 900 K. The union of hot moist and cold damp climates describes the liquid water habitable zone, the width and location of which depends on planet mass. At each solar constant, two or three different climate states are stable. This is a consequence of strong nonlinearities in both thermal emission and the net absorption of sunlight. Across the range of planet sizes, I account for the atmospheres expanding to high altitudes as they warm. The emitting and absorbing surfaces (optical depth of unity) move to high altitude, making their area larger than the planet surface, so more thermal radiation is emitted and more sunlight absorbed (the former dominates). The atmospheres of small planets expand more due to weaker gravity; the effective runaway greenhouse threshold is about 35 W m(-2) higher for Mars, 10 W m(-2) higher for Earth or Venus, but only a few W m(-2) higher for a 10 Earth-mass planet. There is an underlying (expansion-neglected) trend of increasing runaway greenhouse threshold with planetary size (40 W m(-2) higher for a 10 Earth-mass planet than for Mars). Summing these opposing trends means that Venus-sized (or slightly smaller) planets are most susceptible to a runaway greenhouse. The habitable zone for pure water atmospheres is very narrow, with an insolation range of 0.07 times the solar constant. A wider habitable zone requires background gas and greenhouse gas: N2 and CO2 on Earth, which are biologically controlled. Thus, habitability depends on inhabitance.

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Year:  2015        PMID: 25984919      PMCID: PMC4442573          DOI: 10.1089/ast.2014.1268

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  4 in total

1.  Effects of high CO2 levels on surface temperature and atmospheric oxidation state of the early Earth.

Authors:  J F Kasting; J B Pollack
Journal:  J Atmos Chem       Date:  1984       Impact factor: 2.158

2.  Habitable zone limits for dry planets.

Authors:  Yutaka Abe; Ayako Abe-Ouchi; Norman H Sleep; Kevin J Zahnle
Journal:  Astrobiology       Date:  2011-06       Impact factor: 4.335

3.  The runaway greenhouse: implications for future climate change, geoengineering and planetary atmospheres.

Authors:  Colin Goldblatt; Andrew J Watson
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2012-09-13       Impact factor: 4.226

4.  Runaway and moist greenhouse atmospheres and the evolution of Earth and Venus.

Authors:  J F Kasting
Journal:  Icarus       Date:  1988       Impact factor: 3.508

  4 in total
  2 in total

1.  Dynamics of atmospheres with a non-dilute condensible component.

Authors:  Raymond T Pierrehumbert; Feng Ding
Journal:  Proc Math Phys Eng Sci       Date:  2016-06       Impact factor: 2.704

2.  The Resilience of Life to Astrophysical Events.

Authors:  David Sloan; Rafael Alves Batista; Abraham Loeb
Journal:  Sci Rep       Date:  2017-07-14       Impact factor: 4.379

  2 in total

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