Five or six step scenario for evolution?
arXiv:0711.1985 · doi:10.1017/S1473550408004023
Abstract
The prediction that (due to the limited amount of hydrogen available as fuel in the Sun) the future duration of our favourable terrestrial environment will be short (compared with the present age of the Earth) has been interpreted as evidence for a hard step scenario. This means that some of the essential steps (such as the development of eukaryotes) in the evolution process leading to the ultimate emergence of intelligent life would have been hard, in the sense of being against the odds in the available time, so that they are unlikely to have been achieved in most of the earth-like planets that may one day be discovered in nearby extra-solar systems. It was originally estimated that only one or two of the essential evolutionary steps had to have been hard in this sense, but it has become apparent that this figure may need upward revision, because recent studies of climatic instability suggest that the possible future duration of our biologically favourable environment may be shorter than had been supposed, only about one Giga year rather than five. On the basis of the statistical requirement of roughly equal spacing between hard steps, it is argued that the best fit with the fossil record is now obtainable by postulating the number of hard steps to be five, if our evolution was exclusively terrestrial, or six if, as now seems very plausible, the first step occurred on Mars.
11 pages Latex
References in corpus (4)
- Spectral signatures of photosynthesis II: coevolution with other stars and the atmosphere on extrasolar worlds
- A test for the search for life on extrasolar planets: Looking for the terrestrial vegetation signature in the Earthshine spectrum
- Does the rapid appearance of life on Earth suggest that life is common in the Universe?
- Does life's rapid appearance imply a Martian origin?
Cited by in corpus (28)
- Exoplanet Biosignatures: Future Directions
- The Degree of Fine-Tuning in our Universe -- and Others
- A Numerical Testbed for Hypotheses of Extraterrestrial Life and Intelligence
- Physical constraints on the likelihood of life on exoplanets
- Effect of Metallicity on the Evolution of the Habitable Zone from the Pre-Main Sequence to the Asymptotic Giant Branch and the Search for Life
- An Objective Bayesian Analysis of Life's Early Start and Our Late Arrival
- Subsurface Exolife
- On the Origin and Evolution of Life in the Galaxy
- Dependence of Biological Activity on the Surface Water Fraction of Planets
- A Statistical Estimation of the Occurrence of Extraterrestrial Intelligence in the Milky Way Galaxy
- Numerical Testing of The Rare Earth Hypothesis using Monte Carlo Realisation Techniques
- On the probability of habitable planets
- Constraints on Alternate Universes: Stars and habitable planets with different fundamental constants
- Role of stellar physics in regulating the critical steps for life
- Astrobiological Complexity with Probabilistic Cellular Automata
- Observational Constraints on the Great Filter
- If Loud Aliens Explain Human Earliness, Quiet Aliens Are Also Rare
- Optimal Target Stars in the Search for Life
- Triggering A Climate Change Dominated "Anthropocene": Is It Common Among Exocivilizations?
- The Impact of Stellar Abundance Variations on Stellar Habitable Zone Evolution
- Prospects for Life on Temperate Planets Around Brown Dwarfs
- The Galactic Club, or Galactic Cliques? Exploring the limits of interstellar hegemony and the Zoo Hypothesis
- Formulation and Resolutions of the Red Sky Paradox
- Hominid evolution: genetics versus memetics
- A reassessment of the "hard-steps" model for the evolution of intelligent life
- The longevity of habitable planets and the development of intelligent life
- The Entropy Principle and the Influence of Sociological Pressures on SETI
- Seafloor Weathering and Stochastic Outgassing Unlikely to Significantly Shorten the Future Lifespan of Earth's Terrestrial Biosphere