Dependence of Biological Activity on the Surface Water Fraction of Planets
arXiv:1809.09118 · doi:10.3847/1538-3881/aaf420
Abstract
One of the unique features associated with the Earth is that the fraction of its surface covered by land is comparable to that spanned by its oceans and other water bodies. Here, we investigate how extraterrestrial biospheres depend on the ratio of the surficial land and water fractions. We find that worlds that are overwhelmingly dominated by landmasses or oceans are likely to have sparse biospheres. Our analysis suggests that major evolutionary events such as the buildup of O in the atmosphere and the emergence of technological intelligence might be relatively feasible only on a small subset of worlds with surface water fractions ranging approximately between and . We also discuss how our predictions can be evaluated by future observations, and the implications for the prevalence of microbial and technological species in the Universe.
Published in The Astronomical Journal; 14 pages; 3 figures
References in corpus (31)
- Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
- Most 1.6 Earth-Radius Planets are not Rocky
- Extreme Water Loss and Abiotic O Buildup On Planets Throughout the Habitable Zones of M Dwarfs
- A Re-appraisal of the Habitability of Planets Around M Dwarf Stars
- The nature of the TRAPPIST-1 exoplanets
- Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion
- A decreased probability of habitable planet formation around low-mass stars
- The Origin of RNA Precursors on Exoplanets
- Detecting the Glint of Starlight on the Oceans of Distant Planets
- Is Proxima Centauri b habitable? -- A study of atmospheric loss
- The Habitable Zones of Pre-Main-Sequence Stars
- Volatile Delivery to Planets from Water-rich Planetesimals around Low Mass Stars
- Habitability of Exoplanet Waterworlds
- Formation and composition of planets around very low mass stars
- A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
- Risks for life on habitable planets from superflares of their host stars
- The persistence of oceans on Earth-like planets: insights from the deep-water cycle
- Physical constraints for the evolution of life on exoplanets
- Interior characterization in multiplanetary systems: TRAPPIST-1
- Water and the interior structure of terrestrial planets and icy bodies
- The dehydration of water worlds via atmospheric losses
- Subsurface Exolife
- Relative Likelihood of Success in the Searches for Primitive versus Intelligent Extraterrestrial Life
- On the Origin and Evolution of Life in the Galaxy
- The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds
- Is Extraterrestrial Life Suppressed on Subsurface Ocean Worlds due to the Paucity of Bioessential Elements?
- Is Life Most Likely Around Sun-like Stars?
- Planetary formation and water delivery in the habitable zone around solar-type stars in different dynamical environments
- Dynamical, biological, and anthropic consequences of equal lunar and solar angular radii
- Survival Function Analysis of Planet Size Distribution with GAIA Data Release 2 Updates
- A New Desalination Pump Help Define the pH of Ocean Worlds
Cited by in corpus (24)
- Habitability and Spectroscopic Observability of Warm M-dwarf Exoplanets Evaluated with a 3D Chemistry-Climate Model
- Oceanographic Considerations for Exoplanet Life Detection
- Physical constraints for the evolution of life on exoplanets
- Photosynthesis on habitable planets around low-mass stars
- Active Galactic Nuclei: Boon or Bane for Biota?
- Role of stellar physics in regulating the critical steps for life
- Brown Dwarf Atmospheres as the Potentially Most Detectable and Abundant Sites for Life
- Land Fraction Diversity on Earth-like Planets and Implications for their Habitability
- Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
- Water shielding in the terrestrial planet-forming zone: Implication for inner disk organics
- Photosynthesis on Exoplanets and Exomoons from Reflected Light
- Reimagining the water snowline
- A Bayesian Analysis of Technological Intelligence in Land and Oceans
- Prospects for Life on Temperate Planets Around Brown Dwarfs
- Constraints on Aquatic Photosynthesis for Terrestrial Planets Around Other Stars
- Water versus land on temperate rocky planets
- Characteristics of aquatic biospheres on temperate planets around Sun-like stars and M-dwarfs
- Theoretical constraints imposed by gradient detection and dispersal on microbial size in astrobiological environments
- Multiverse Predictions for Habitability: Planetary Characteristics
- Implications of Abiotic Oxygen Buildup for Earth-like Complex Life
- Beyond Mediocrity: How Common is Life?
- Exo-Geoscience Perspectives Beyond Habitability
- The Most Common Habitable Planets II -- Salty Oceans in Low Mass Habitable Planets and Global Climate Evolution
- Habitable zone predictions and how to test them