Subsurface Exolife
arXiv:1711.09908 · doi:10.1017/S1473550418000083
Abstract
We study the prospects for life on planets with subsurface oceans, and find that a wide range of planets can exist in diverse habitats with ice envelopes of moderate thickness. We quantify the energy sources available to these worlds, the rate of production of prebiotic compounds, and assess their potential for hosting biospheres. Life on these planets is likely to face challenges, which could be overcome through a combination of different mechanisms. We estimate the number of such worlds, and find that they may outnumber rocky planets in the habitable zone of stars by a few orders of magnitude.
Published in the International Journal of Astrobiology; 64 pages; 2 figures
References in corpus (61)
- Cosmic Star Formation History
- Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
- Mass-Radius Relationships for Solid Exoplanets
- 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
- Photochemistry and astrochemistry: photochemical pathways to interstellar complex organic molecules
- Ice structures, patterns, and processes: A view across the ice-fields
- Three regimes of extrasolar planets inferred from host star metallicities
- Detailed Models of super-Earths: How well can we infer bulk properties?
- The ancient heritage of water ice in the solar system
- The pH of Enceladus' ocean
- How to Characterize Habitable Worlds and Signs of Life
- Probing for Evidence of Plumes on Europa with HST/STIS
- The largest oxigen bearing organic molecule repository
- A decreased probability of habitable planet formation around low-mass stars
- Interstellar Interloper 1I/2017 U1: Observations from the NOT and WIYN Telescopes
- Is Proxima Centauri b habitable? -- A study of atmospheric loss
- The Habitable Zones of Pre-Main-Sequence Stars
- An Observational Upper Limit on the Interstellar Number Density of Asteroids and Comets
- The MUSCLES Treasury Survey IV: Scaling Relations for Ultraviolet, Ca II K, and Energetic Particle Fluxes from M Dwarfs
- Interstellar Interlopers: Number Density and Origins of 'Oumuamua-like Objects
- Volatile Delivery to Planets from Water-rich Planetesimals around Low Mass Stars
- Transit surveys for Earths in the habitable zones of white dwarfs
- Habitability of Exoplanet Waterworlds
- Astrophysical Ionizing Radiation and the Earth: A Brief Review and Census of Intermittent Intense Sources
- A Search for Propylene Oxide and Glycine in Sagittarius B2 (LMH) and Orion
- 1I/2017 U1 (`Oumuamua) is Hot: Imaging, Spectroscopy and Search of Meteor Activity
- Col-OSSOS: Colors of the Interstellar Planetesimal 1I/`Oumuamua
- On the "Galactic Habitable Zone"
- Risks for life on habitable planets from superflares of their host stars
- The origin of interstellar asteroidal objects like 1I/2017 U1 'Oumuamua
- APO Time Resolved Color Photometry of Highly-Elongated Interstellar Object 1I/'Oumuamua
- Can habitable planets form in clustered environments?
- Implications of the interstellar object 1I/'Oumuamua for planetary dynamics and planetesimal formation
- A Review of Exoplanetary Biosignatures
- Implications for planetary system formation from interstellar object 1I/2017 U1 (`Oumuamua)
- The occurrence of planets and other substellar bodies around white dwarfs using K2
- The Survival Rate of Ejected Terrestrial Planets with Moons
- Realistic Detectability of Close Interstellar Comets
- 1I/`Oumuamua as a Tidal Disruption Fragment From a Binary Star System
- `Oumuamua as a messenger from the Local Association
- The Demographics of Rocky Free-Floating Planets and their Detectability by WFIRST
- Relative Likelihood for Life as a Function of Cosmic Time
- The dehydration of water worlds via atmospheric losses
- Ejection of rocky and icy material from binary star systems: Implications for the origin and composition of 1I/`Oumuamua
- On the Possible Properties of Small and Cold Extrasolar Planets: Is OGLE-2005-BLG-390Lb Entirely Frozen?
- The Resilience of Life to Astrophysical Events
- On the Origin and Evolution of Life in the Galaxy
- Probing Planets in Extragalactic Galaxies Using Quasar Microlensing
- The language of exoplanet ranking metrics needs to change
- Polymerization of building blocks of life on Europa and other icy moons
- The Propitious Role of Solar Energetic Particles in the Origin of Life
- The habitability of the Milky Way during the active phase of its central supermassive black hole
- Is Life Most Likely Around Sun-like Stars?
- Habitable Evaporated Cores and the Occurrence of Panspermia near the Galactic Center
- Why do we find ourselves around a yellow star instead of a red star?
- Implications of Captured Interstellar Objects for Panspermia and Extraterrestrial Life
- Reduced Diversity of Life Around Proxima Centauri and TRAPPIST-1
- Water Formation During the Epoch of First Metal Enrichment
- Capture of free-floating planets by stellar systems
- Are extrasolar oceans common throughout the Galaxy?
Cited by in corpus (32)
- Physical constraints for the evolution of life on exoplanets
- Galactic Panspermia
- Dependence of Biological Activity on the Surface Water Fraction of Planets
- Is Extraterrestrial Life Suppressed on Subsurface Ocean Worlds due to the Paucity of Bioessential Elements?
- Is Life Most Likely Around Sun-like Stars?
- Implications of Captured Interstellar Objects for Panspermia and Extraterrestrial Life
- Active Galactic Nuclei: Boon or Bane for Biota?
- Brown Dwarf Atmospheres as the Potentially Most Detectable and Abundant Sites for Life
- The Habitability of the Galactic Bulge
- Interstellar communication network. I. Overview and assumptions
- The Impact of Tidal Disruption Events on Galactic Habitability
- The impact of AGN outflows on the surface habitability of terrestrial planets in the Milky Way
- If Loud Aliens Explain Human Earliness, Quiet Aliens Are Also Rare
- The GALAH Survey: Using Galactic Archaeology to Refine our Knowledge of TESS Target Stars
- A Bayesian Analysis of Technological Intelligence in Land and Oceans
- Optimal Target Stars in the Search for Life
- On the Habitable Lifetime of Terrestrial Worlds with High Radionuclide Abundances
- Different is More: The Value of Finding an Inhabited Planet that is Far From Earth 2.0
- Potential For Liquid Water Biochemistry Deep Under The Surfaces Of The Moon, Mars And Beyond
- Theoretical constraints imposed by gradient detection and dispersal on microbial size in astrobiological environments
- Characteristics of aquatic biospheres on temperate planets around Sun-like stars and M-dwarfs
- A light sail astrobiology precursor mission to Enceladus and Europa
- Beyond Mediocrity: How Common is Life?
- Chasing Nomadic Worlds: A New Class of Deep Space Missions
- Spaceflight from Super-Earths is difficult
- Utilizing a Database of Simulated Geometric Albedo Spectra for Photometric Characterization of Rocky Exoplanet Atmospheres
- Physical Constraints on Motility with Applications to Possible Life on Mars and Enceladus
- Upper limit on the fraction of alien civilizations that develop communication technology
- Habitability on local, Galactic and cosmological scales
- Super-Earths in need for Extremly Big Rockets
- Artificial versus Biological Intelligence in the Cosmos: Clues from a Stochastic Analysis of the Drake Equation
- Necessary Conditions for Earthly Life Floating in the Venusian Atmosphere