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The anthropic principle and its implications for biological evolution
Abstract
In the form in which it was originally expounded, the anthropic principle was presented as a warning to astrophysical and cosmological theorists of the risk of error in the interpretation of astronomical and cosmological information unless due account is taken of the biological restraints under which the information was acquired. However, the converse message is also valid: biological theorists also run the risk of error in the interpretation of the evolutionary record unless they take due heed of the astrophysical restraints under which evolution took place. After an introductory discussion of the ordinary (‘weak’) anthropic principle and of its more contestable (‘strong’) analogue, a new application of the former to the problem of the evolution of terrestrial life is presented. It is shown that the evidence suggests that the evolutionary chain included at least one but probably not more than two links that were highly improbable (a priori) in the available time interval.
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“Since there are more centers in glorious-future worlds than doomsday worlds by a factor of billions, the posterior probability of the doomsday hypothesis is boosted from one in a million to close to one.”
From Multiple Universes and Self-Locating Evidence (2022) · cites this paper as Carter 1983
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Carter, G. R., Modrak, N., Willis, S., Tions, A., Development, Houtz, J., Martin, K., Nasr, S., Kalyan, M., Matheson, B., et al. (2018) · Indianizing Film · doi:10.7591/9781501722035-016 · Cited by 1,385
The fundamental constants and their variation: observational and theoretical status
Uzan, J. (2003) · Reviews of Modern Physics · doi:10.1103/revmodphys.75.403 · Cited by 1,214
“Carter (1974, 1976, 1983), who actually coined the term “anthropic principle”, showed that the numerological coincidence found by Dirac can be derived from physical models of stars and the competition between the weakness of gravity with respect to nuclear fusion.”
BackgroundVarying Constants, Gravitation and Cosmology
Uzan, J. (2011) · Living Reviews in Relativity · doi:10.12942/lrr-2011-2 · Cited by 880
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Predictions from Quantum Cosmology
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Implications of the Copernican principle for our future prospects
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The Galactic Habitable Zone and the Age Distribution of Complex Life in the Milky Way
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Exoplanet Biosignatures: A Framework for Their Assessment
Catling, D. C., Krissansen-Totton, J., Kiang, N. Y., Crisp, D., Robinson, T. D., DasSarma, S., Rushby, A. J., Del Genio, A., Bains, W., & Domagal-Goldman, S. (2018) · Astrobiology · doi:10.1089/ast.2017.1737 · Cited by 225
“Nonetheless, given the present stage of understanding and lack of data, the possibilities for P(life jEarth-like) range from life being very common to very rare, as has been much discussed in the literature (e.g., Carter, 1983; Spiegel and Turner, 2012; Scharf and Cronin, 2016; Walker, 2017).”
BackgroundVaidman, L. (1998) · International Studies in the Philosophy of Science · doi:10.1080/02698599808573600 · Cited by 199
Maudlin, T. (2012) · Princeton University Press eBooks · doi:10.1515/9780691190679 · Cited by 155
Astrobiology: The Study of the Living Universe
Chyba, C. F., & Hand, K. P. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.051804.102202 · Cited by 176
Garriga, J., & Vilenkin, A. (1998) · Physical Review D · doi:10.1103/physrevd.57.2230 · Cited by 154
Constraining the Time Interval for the Origin of Life on Earth
Pearce, B. K. D., Tupper, A. S., Pudritz, R. E., & Higgs, P. G. (2018) · Astrobiology · doi:10.1089/ast.2017.1674 · Cited by 140
“Indeed, it has been argued that if intelligent life requires a great deal of time to evolve, Earth may be a rare planet, on which life got started unusually early (Carter, 1983).”
Habitable Zone Lifetimes of Exoplanets around Main Sequence Stars
Rushby, A. J., Claire, M. W., Osborn, H., & Watson, A. J. (2013) · Astrobiology · doi:10.1089/ast.2012.0938 · Cited by 138
“The probabilistic anthropic model of Watson (2008), which draws on the theory of critical evolutionary transitions advanced by Szathma´ry and Maynard-Smith (1995) and the ‘‘critical steps’’ model of Carter (1983), proposes that complex biology becomes increasingly probable with longer HZ life-times.”
Bayesian analysis of the astrobiological implications of life’s early emergence on Earth
Spiegel, D. S., & Turner, E. L. (2012) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1111694108 · Cited by 132
“We note several previous quantitative attempts to address this issue in the literature, of which one [8] found, as we do, that early abiogenesis is consistent with life being rare, and the other [9] found that Earth’s early abiogenesis points strongly to life being common on Earth-like planets (we compare our approach…”
ResultDoes the Rapid Appearance of Life on Earth Suggest that Life Is Common in the Universe?
Lineweaver, C. H., & Davis, T. M. (2002) · Astrobiology · doi:10.1089/153110702762027871 · Cited by 123
“Carter (1983) has pointed out that the time scale for the evolution of intelligence on the Earth ( , 5 Gyr) is comparable to the main sequence lifetime of the Sun ( , 10 Gyr).”
InfluentialExoplanet Biosignatures: Future Directions
Walker, S. I., Bains, W., Cronin, L., DasSarma, S., Danielache, S. O., Domagal-Goldman, S. D., Kaçar, B., Kiang, N. Y.-L., Lenardic, A., Reinhard, C. T., et al. (2018) · Astrobiology · doi:10.1089/ast.2017.1738 · Cited by 137
“Attempts have been made to estimate P(life) within a Bayesian framework by Carter and McCrea (Carter and McCrea, 1983) and more recently by Spiegel and Turner (Spiegel and Turner, 2012).”
BackgroundMethodInfluentialHabitability of Exoplanet Waterworlds
Kite, E. S., & Ford, E. B. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aad6e0 · Cited by 124
“Maximum τhab is greatly increased (Carter 1983).”
BackgroundThe Temporal Aspect of the Drake Equation and SETI
Ćirković, M. (2003) · Astrobiology · doi:10.1089/153110704323175160 · Cited by 95
“In addition (1983) suggested an independent life on Earth in the galactic context generally recognized that “contact pes-simists” a strong position.”
Origins of life: a problem for physics, a key issues review
Walker, S. I. (2017) · Reports on Progress in Physics · doi:10.1088/1361-6633/aa7804 · Cited by 94
Selection for Gaia across Multiple Scales
Lenton, T. M., Daines, S. J., Dyke, J. G., Nicholson, A., Wilkinson, D. M., & Williams, H. T. P. (2018) · Trends in Ecology & Evolution · doi:10.1016/j.tree.2018.05.006 · Cited by 117
Relative likelihood for life as a function of cosmic time
Loeb, A., Batista, R. A., & Sloan, D. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/08/040 · Cited by 71
“Our results provide a new perspective on the so-called “coincidence problem”, why do we observe Ωm ∼ ΩΛ? [37] The answer comes naturally if we consider the history of Sun-like star formation, as the number of habitable planets peaks around present time for m ∼ 1M .”
ResultGalactic Gradients, Postbiological Evolution and the Apparent Failure of SETI
Ćirković, M., & Bradbury, R. J. (2005) · arXiv.org · doi:10.1016/j.newast.2006.04.003 · Cited by 69
“In addition, we have witnessed substantial research leading to a decrease in confidence in the so-called Carter’s (1983) ”anthropic” argument, the other mainstay of SETI scepticism (Wilson 1994; Livio 1999; Ćirković and Dragićević 2006, preprint).”
BackgroundTestable anthropic predictions for dark energy
Garriga, J., & Vilenkin, A. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.043503 · Cited by 78
The hidden simplicity of biology
Davies, P. C. W., & Walker, S. I. (2016) · Reports on Progress in Physics · doi:10.1088/0034-4885/79/10/102601 · Cited by 62
Conditions for the emergence of life on the early Earth: summary and reflections
Jortner, J. (2006) · Philosophical Transactions of the Royal Society B Biological Sciences · doi:10.1098/rstb.2006.1909 · Cited by 65
“The distinction between the ‘hard’ and the ‘easy’ formation of early life can be highlighted by the adaptation of the Carter formula (Carter 1983; Barrow & Tiepler 1988) and its slight extension ( Jortner 2006, unpublished results).”
BackgroundThe degree of fine-tuning in our universe — and others
Adams, F. C. (2019) · Physics Reports · doi:10.1016/j.physrep.2019.02.001 · Cited by 62
“Although anthropic arguments have been put forth with a range of definitions (classic references include [61, 122, 131, 132]), the basic consideration is that the universe must have the proper version of physical law in order to develop observers.”
BackgroundIndifference principle and anthropic principle in cosmology
McMullin, E. (1993) · Studies in History and Philosophy of Science Part A · doi:10.1016/0039-3681(93)90034-h · Cited by 75
Fermi's Paradox - The Last Challenge For Copernicanism?
Ćirković, M. (2009) · Serbian Astronomical Journal · doi:10.2298/saj0978001c · Cited by 60
T HE F UTURE OF H UMAN E VOLUTION
Templeton, A. R. (2001) · doi:10.2307/j.ctv7h0s6j.27 · Cited by 60
“3 But see e.g. (Carter 1983, 1989; Bostrom 2002a; Hanson 1998b). extinction of the human species.”
Implications of an Anthropic Model of Evolution for Emergence of Complex Life and Intelligence
Watson, A. J. (2008) · Astrobiology · doi:10.1089/ast.2006.0115 · Cited by 53
“One reason for this may be the conclusion originally reached by Carter (1983), that there was only 1 such step or, at most, 2, based on the assumption that we are presently only midway through the life span of the biosphere.”
InfluentialHarrison, T. M. (2020) · doi:10.1007/978-3-030-46687-9 · Cited by 53
“Lastly, some believe that tens to hundreds of millions of years would be needed for nature to survey nonfunctional biopolymer sequence space in order to form macromolecules on prebiotic Earth (e.g., Carter 1983; Neveu et al. 2013; Adamala et al. 2014).”
BackgroundIs our universe decaying at an astronomical rate?
Page, D. N. (2008) · Physics Letters B · doi:10.1016/j.physletb.2008.08.039 · Cited by 50
The Doomsday Argument and the Number of Possible Observers
Olum, K. D. (2002) · The Philosophical Quarterly · doi:10.1111/1467-9213.00260 · Cited by 50
“ar X iv :g rqc /0 00 90 81 v2 1 3 O ct 2 00 0 If the human race comes to an end relatively shortly, then we have been born at a fairly typical time in history of humanity.”
BackgroundFive- or six-step scenario for evolution?
Carter, B. (2007) · International Journal of Astrobiology · doi:10.1017/s1473550408004023 · Cited by 49
“The aim of the present discussion is to clarify the problem of identifying which of the essential steps may have been hard in the sense Carter (1983) of depending on the fortuitous occurrence of some combination of random events that would automatically happen sooner or later if unlimited time were…”
BackgroundMethodInfluentialSelf-citationTERRESTRIAL PLANETS ACROSS SPACE AND TIME
Zackrisson, E., Calissendorff, P., González, J., Benson, A., Johansen, A., & Janson, M. (2016) · The Astrophysical Journal · doi:10.3847/1538-4357/833/2/214 · Cited by 51
“…assumes that it typically takes several billion years for intelligent life to arise (some 4.5 Gyr in the case of humans,and please note that the Carter (1983) argument suggests that the typical timescale may be much longer than this), then only the z 2 part of the universe becomes relevant.”
BackgroundInfluentialThe astrobiological landscape : philosophical foundations of the study of cosmic life
Ćirković, M. (2012) · doi:10.1017/cbo9780511667404 · Cited by 48
Gott, J. (1994) · Nature · doi:10.1038/368108a0 · Cited by 47
Quantifying the origins of life on a planetary scale
Scharf, C. A., & Cronin, L. (2016) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1523233113 · Cited by 49
Astrobiological Phase Transition: Towards Resolution of Fermi’s Paradox
Ćirković, M., & Vukotić, B. (2008) · Origins of Life and Evolution of Biospheres · doi:10.1007/s11084-008-9149-y · Cited by 46
Ćirković, M. (2008) · doi:10.4324/9781003000655 · Cited by 46
The Timing of Evolutionary Transitions Suggests Intelligent Life is Rare
Snyder-Beattie, A. E., Sandberg, A., Drexler, K. E., & Bonsall, M. B. (2020) · Astrobiology · doi:10.1089/ast.2019.2149 · Cited by 62
“Carter (1983) noticed this coincidence and proposed a resolution to the puzzle based on observation selection effects.”
BackgroundMethodPopulation growth, energy use, and the implications for the search for extraterrestrial intelligence
Mullan, B., & Haqq-Misra, J. D. (2018) · Futures · doi:10.1016/j.futures.2018.06.009 · Cited by 38
“A more recent version known as the “doomsday argument” implies that we might be much closer to the end of civilization than to its beginning due to the probabilistic implications of this growth (Carter and McCrea 1983; Bostrom 2013) or more broadly from the Copernican principle (Gott 1993).”
BackgroundSearching for alien artifacts on the moon
Davies, P., & Wagner, R. V. (2011) · Acta Astronautica · doi:10.1016/j.actaastro.2011.10.022 · Cited by 46
Doomsday--Or: The Dangers of Statistics
Dieks, D. (1992) · doi:10.2307/2220450 · Cited by 43
Multiple Universes and Self-Locating Evidence
Isaacs, Y., Hawthorne, J., & Sanford Russell, J. (2022) · The Philosophical Review · doi:10.1215/00318108-9743809 · Cited by 42
“One objection is the famous “Doomsday argument” (Carter 1983; Leslie 1990; see also Bostrom 2002, pp. 89ff. and references therein).”
BackgroundThe New Astronomy: Opening the Electromagnetic Window and Expanding Our View of Planet Earth
Orchiston, W. (2005) · Springer eBooks · doi:10.1007/1-4020-3724-4 · Cited by 39
Dark energy equation of state and anthropic selection
Garriga, J., Linde, A. D., & Vilenkin, A. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.69.063521 · Cited by 57
On the history and future of cosmic planet formation
Behroozi, P., & Peeples, M. S. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1817 · Cited by 63
“…just “civilisations”) is famously uncertain, with estimates of the civilisation incidence per habitable planet ranging from 10−5 (Sagan 1963) to arbitrarily small values (e.g., < 10−30, combining pessimistic estimates from Carter 1983; Ward & Brownlee 2000; Schermer 2002; Spiegel & Turner 2012).”
BackgroundRelative Likelihood of Success in the Search for Primitive versus Intelligent Extraterrestrial Life
Lingam, M., & Loeb, A. (2018) · Astrobiology · doi:10.1089/ast.2018.1936 · Cited by 47
Fundamental constants: from measurement to the universe, a window on gravitation and cosmology
Uzan, J.-P. (2025) · Living Reviews in Relativity · doi:10.1007/s41114-025-00059-y · Cited by 36
Footprints of alien technology
Davies, P. (2010) · Acta Astronautica · doi:10.1016/j.actaastro.2011.06.022 · Cited by 36
Dissolving the Fermi ParadoxPreprint
Sandberg, A., Drexler, E., & Ord, T. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1806.02404 · Cited by 55
“As noted by Carter and McCrea [10] the evidential power of the early emergence of life on Earth is weakened by observer selection effects, allowing for deep uncertainty about what the natural timescale of life formation is.”
Background“Not Only Defended But Also Applied”: The Perceived Absurdity of Bayesian Inference
Gelman, A., & Robert, C. P. (2013) · The American Statistician · doi:10.1080/00031305.2013.760987 · Cited by 54
“An example is the so-called doomsday argument (Carter and McCrea 1983), which holds that there is a high probability that humanity will be extinct (or will drastically reduced in population) soon, because if this were not true—if, for example, humanity were to continue with 10 billion people or so for the next few tho…”
BackgroundInfluentialThe Doomsday Argument Adam & Eve, UN++, and Quantum Joe
Bostrom, N. (2001) · Synthese · doi:10.1023/a:1010350925053 · Cited by 35
“These other forms of reasoning include methods of deriving observational consequences from cosmological models (Leslie 1989; Bostrom 2000b; Bostrom 2001a), arguments concerning how improbable was the evolution of intelligent life on Earth (Carter 1983; Carter 1989), and game theoretic problems involving imperfect reca…”
InfluentialDependence of Biological Activity on the Surface Water Fraction of Planets
Lingam, M., & Loeb, A. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/aaf420 · Cited by 35
A Comprehensive Comparison of the Sun to Other Stars: Searching for Self-Selection Effects
Robles, J., Lineweaver, C., Grether, D., Flynn, C., Egan, C. A., Pracy, M., Holmberg, J., & Gardner, E. (2008) · The Astrophysical Journal · doi:10.1086/589985 · Cited by 33
“Age If the evolution of observers like ourselves takes on average many billions of years, we might expect the Sun to be anomalously old (Carter 1983).”
BackgroundLingam, M., & Loeb, A. (2018) · International Journal of Astrobiology · doi:10.1017/s1473550418000083 · Cited by 42
“The likelihood of epoch (21)The number of these transitions that led to noogenesis (the emergence of intelligence) on Earth remains unsettled, but has been suggested to lie between 4 and 7 by several authors (Carter, 1983; Watson, 2008; Carter, 2008; McCabe and Lucas, 2010); see also: http://mason.”
BackgroundEvaluating Methods for Estimating Existential Risks
Tonn, B. E., & Stiefel, D. (2013) · Risk Analysis · doi:10.1111/risa.12039 · Cited by 33
“The Doomsday argument, based on a priori estimates of the total number of humans that will come to be over time, also leads to high belief in human extinction.(45,46) It is not clear that these suppositions support the converse, that human survival is likely, so this element of the frame of discernment received no pro…”
BackgroundDoes Life's Rapid Appearance Imply a Martian Origin?
Davies, P. C. W. (2003) · Astrobiology · doi:10.1089/153110703322736006 · Cited by 31
“This situation was considered by Carter (1983), who used it to explain why, to within a factor of about 2, the time taken for evolution to produce intelligence on Earth is the same as the expected lifetime of the main sequence stage of the sun (alternatively, the duration of habitability of the…”
InfluentialQuark masses: An environmental impact statement
Jaffe, R., Jenkins, A., & Kimchi, I. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.065014 · Cited by 31
Self-Locating Belief in Big Worlds: Cosmology’s Missing Link to Observation
Bostrom, N. (2002) · The Journal of Philosophy · doi:10.5840/jphil2002991211 · Cited by 31
ON THE TIMESCALE FORCING IN ASTROBIOLOGY
Vukotić, B., & Ćirković, M. (2007) · doi:10.2298/saj0775045v · Cited by 29
“We conclude that even the simplest preliminary models show it is too early to draw sceptical conclusions about the abundance of extraterrestrial life and intelligence from our single data point via the ”anthropic” argument of Carter (1983).”
BackgroundA refutation of the doomsday argument
Korb, K., & Oliver, J. J. (1998) · doi:10.1093/mind/107.426.403 · Cited by 28
“The Doomsday Argument was conceived by the astrophysicist Brandon Carter some fifteen years ago [i.e. Carter 1983], and it has since been developed in a Nature article by Richard Gott (1993), and in several papers by philosopher John Leslie and especially in his recent monograph The End of The World (Leslie 1996).”
BackgroundLong-Term Planetary Habitability and the Carbonate-Silicate Cycle
Rushby, A., Johnson, M. T., Mills, B. J. W., Watson, A. J., & Claire, M. W. (2018) · Astrobiology · doi:10.1089/ast.2017.1693 · Cited by 32
“Watson (2008), drawing on the earlier work of Carter (1983) and Szathma´ry and Maynard-Smith (1995), developed a probabilistic model that attempts to quantify the timing and likelihood of several critical (de-fined broadly as only occurring once in Earth’s history) steps in evolution en route to…”
Reduced Diversity of Life around Proxima Centauri and TRAPPIST-1
Lingam, M., & Loeb, A. (2017) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aa8860 · Cited by 29
“Hence, a planet that does not pass through a series of complex evolutionary steps will be incapable of giving rise to intelligence (Carter 1983; Watson 2008).”
Background“The Most Philosophically Important of All the Sciences”: Karl Popper and Physical Cosmology
Kragh, H. (2013) · Perspectives in Science · doi:10.1162/posc_a_00102 · Cited by 27
An anthropic myth: Fred Hoyle’s carbon-12 resonance level
Kragh, H. (2010) · Archive for History of Exact Sciences · doi:10.1007/s00407-010-0068-8 · Cited by 47
Why do we find ourselves around a yellow star instead of a red star?
Haqq-Misra, J., Kopparapu, R. K., & Wolf, E. T. (2017) · International Journal of Astrobiology · doi:10.1017/s1473550417000118 · Cited by 31
Leslie, J. (1992) · doi:10.1007/bf03025214 · Cited by 26
Sverdrup, H., van Allen, O., & Haraldsson, H. (2024) · Natural Resources Research · doi:10.1007/s11053-023-10296-z · Cited by 25
“And, the future generations are many (Brandon Carter, 1983; Leslie, 1998).”
Sustainability and the astrobiological perspective: Framing human futures in a planetary context
Frank, A., & Sullivan, W. T. (2014) · Anthropocene · doi:10.1016/j.ancene.2014.08.002 · Cited by 24
“As shown in Carter (1983), if there are n critical steps leading to some property such as intelligence or technological capability and each kth step has low probability lk (lkth 1), then the expectation for the time at which the kth step will occur is htk=ni ¼ k n þ 1 th (2) Using a more detailed…”
BackgroundRole of stellar physics in regulating the critical steps for life
Lingam, M., & Loeb, A. (2019) · International Journal of Astrobiology · doi:10.1017/s1473550419000016 · Cited by 25
“In this paper, we will therefore use a model originally developed by Carter (1983), where evolution is treated as a succession of critical steps, to assess the likelihood of primitive (microbial) and intelligent (technological) life, and the implications for detecting biosignatures and…”
MethodResultInfluentialGalactic Punctuated Equilibrium: How to Undermine Carter's Anthropic Argument in Astrobiology
Ćirković, M., Vukotić, B., & Dragičević, I. (2009) · Astrobiology · doi:10.1089/ast.2007.0200 · Cited by 24
“We conclude that it is too early to draw skeptical conclusions about the abundance of extraterrestrial life and intelligence from our single data point via the ‘‘anthropic’’ argument of Carter (1983).”
Anthropic principle in cosmology
Carter, B. (2006) · Cambridge University Press eBooks · doi:10.1017/cbo9780511607028.015 · Cited by 28
“The example that seems to me most important was provided by the prediction [9] that the occurrence of anthropic observers would be rare, even on environmentally favorable planets such as ours.”
Self-citationStolzenberg, N. (2019) · The Oxford Handbook of Law and Humanities · doi:10.1093/oxfordhb/9780190695620.013.20 · Cited by 23
“213 The analogy between black hole mechanics and thermodynamics was spelled out in Bardeen, Carter, and Hawking (1973).”
BackgroundBayesian evidence for the prevalence of waterworlds
Simpson, F. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx516 · Cited by 25
Lineweaver, C. H., & Egan, C. A. (2007) · The Astrophysical Journal · doi:10.1086/522197 · Cited by 41
Barnes, L. A., Elahi, P. J., Salcido, J., Bower, R. G., Lewis, G. F., Theuns, T., Schaller, M., Crain, R. A., & Schaye, J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty846 · Cited by 23
NEOCATASTROPHISM AND THE MILKY WAY ASTROBIOLOGICAL LANDSCAPE
Vukotić, B., & Ćirković, M. (2008) · doi:10.2298/saj0876071v · Cited by 22
“Carter’s anthropic argument (Carter 1983, 1993, Livio 1999): If biological and astrophysical timescales determining the evolution of life and intelligence are independent, we have a posteriori Bayesian reasons to believe that the biological timescale is much larger than the astrophysical one, thus…”
BackgroundMethodAstrobiological Complexity with Probabilistic Cellular Automata
Vukotić, B., & Ćirković, M. (2012) · Origins of Life and Evolution of Biospheres · doi:10.1007/s11084-012-9293-2 · Cited by 21
Leslie, J. (1990) · Interchange · doi:10.1007/bf01809610 · Cited by 20
Constraints on alternate universes: stars and habitable planets with different fundamental constants
Adams, F. C. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/02/042 · Cited by 24
“As a result, the fiducial time scale of 1 Gyr, while appropriate for life on Earth, does not represent a definitive limit.”
BackgroundInfluentialDanchi, W., & López, B. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/769/1/27 · Cited by 20
“The number of steps discussed in the literature varies between two (Carter 1983) and ten (Barrow & Tipler 1986), and the mean interval between steps can be interpreted in the context of major evolutionary stages, such as biogenesis, bacterial, eukaryotes, combigenesis, metazoans, and civilization…”
BackgroundResultStandish, R. (2000) · doi:10.1023/b:fopl.0000032475.18334.0e · Cited by 20
“If we assume the self-sampling assumption(7, 8), essentially that we expect to find ourselves in one of the universes with greatest measure, subject to the constraints of the anthropic principle.”
BackgroundOn the Rate of Abiogenesis from a Bayesian Informatics Perspective
Chen, J., & Kipping, D. (2018) · Astrobiology · doi:10.1089/ast.2018.1836 · Cited by 20
“From this observation, there have been numerous efforts to quantify k conditioned upon this datum, with, for example, Carter (1983) concluding that it is compatible with life being rare, whereas the findings of Line-weaver and Davis (2002) point strongly toward life being common on Earth-like worlds.”
Star Masses and Star-Planet Distances for Earth-like Habitability
Waltham, D. (2017) · Astrobiology · doi:10.1089/ast.2016.1518 · Cited by 19
“This author, however, finds his arguments compelling, and interested readers are advised to read the works of Carter (1983) and Watson (2008) if they require further reassurance.”
BackgroundMethodInfluentialSearching for a shadow biosphere on Earth as a test of the ‘cosmic imperative’
Davies, P. (2011) · Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences · doi:10.1098/rsta.2010.0235 · Cited by 17
Space colonization remains the only long-term option for humanity: A reply to Torres
Ćirković, M. (2019) · Futures · doi:10.1016/j.futures.2018.09.006 · Cited by 19
Walker, S. I., & Davies, P. C. W. (2017) · Cambridge University Press eBooks · doi:10.1017/9781316584200.002 · Cited by 43
The Universe as a Cyclic Organized Information System: John Wheeler’s World Revisited
Meijer, D. K. F. (2014) · NeuroQuantology · doi:10.14704/nq.2015.13.1.798 · Cited by 11
“Wheeler thereby evidently became an early advocate of the “Participatory Anthropic Principle” as primarily put forward by Brandon Carter (1983) and later by Robert Dicke (1961), indicating that the laws of physics are fine-tuned to permit the existence of life (see for a review of anthropic factors, Ross, 1989).”
BackgroundCopernicus, Kant, and the anthropic cosmological principles
Roush, S. (2003) · Studies in History and Philosophy of Science Part B Studies in History and Philosophy of Modern Physics · doi:10.1016/s1355-2198(02)00029-1 · Cited by 55
On the origin and evolution of life in the Galaxy
McCabe, M., & Lucas, H. (2010) · International Journal of Astrobiology · doi:10.1017/s1473550410000340 · Cited by 17
“A simple stochastic model, first proposed by Carter (1983) and discussed by Barrow & Tipler (1986), Hanson (1998) and Flambaum (2003), assumes that evolution is governed by a series or critical transitions or bottlenecks, which must be passed to advance from basic molecules to simple, complex and…”
MethodProbability distribution of terrestrial planets in habitable zones around host stars
Guo, J., Zhang, F.-H., Chen, X.-F., & Han, Z.-W. (2009) · Astrophysics and Space Science · doi:10.1007/s10509-009-0081-z · Cited by 17
If Loud Aliens Explain Human Earliness, Quiet Aliens Are Also Rare
Hanson, R. D., Martin, D., McCarter, C., & Paulson, J. (2021) · Astrophysical Journal · doi:10.3847/1538-4357/ac2369 · Cited by 16
“…might arise from simple dead matter, via intermediate steps of simple life, complex life, etc., a model that he and many others have since pursued (Carter 1983; Caldeira & Kasting 1992; Hanson 1998b; Carter 2008; Watson 2008; McCabe & Lucas 2010; Aldous 2012; Simpson 2017; Waltham 2017; Sandora…”
BackgroundMethodSafonova, M., Murthy, J., & Shchekinov, Y. A. (2015) · International Journal of Astrobiology · doi:10.1017/s1473550415000208 · Cited by 25
“Carter (1983) has pointed out that the timescale for the evolution of intelligence on the Earth (*5 Gyr) is comparable with the main sequence lifetime of the Sun (*10 Gyr).”
BackgroundInfluential
Metadata
- Authors
- Carter, B.
- Affiliations
- Observatoire de Paris (FR)
- Corresponding author
- Carter, Brandon
- ORCID
- Carter, Brandon
- Venue
- Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences
- Publisher
- The Royal Society
- Published
- 1983-12-20
- Volume
- 310
- Issue
- 1512
- Pages
- 347-363
- ISSN
- 0080-4614 (ISSN-L)
- 2054-0272
- OpenAlex
- W2122258450
- Cited by
- 375
- References
- 14
- Citations by year
- 2026: 4 · 2025: 17 · 2024: 13 · 2023: 15 · 2022: 15 · 2021: 13 · 2020: 28 · 2019: 32 · 2018: 26 · 2017: 11 · 2016: 17 · 2015: 8 · 2014: 6 · 2013: 11 · 2012: 9
- FWCI
- 4.69
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Origins and Evolution of Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Environmental Science › Global and Planetary Change › Earth Systems and Cosmic Evolution
- Keywords
- anthropic principle, evolution
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