Fermi Paradox Special Issue

Total Page:16

File Type:pdf, Size:1020Kb

Fermi Paradox Special Issue Journal of the British Interplanetary Society VOLUME 71 NO.6 JUNE 2018 Fermi Paradox Special Issue THE ORIGIN OF THE “FERMI PARADOX” Anthony R. Martin FERMI AND LOTKA: the Long Odds of Survival in a Dangerous Universe Kent A. Peacock SCENARIO BLOCK DIAGRAM ANALYSIS of the Galactic Evolution of Life Stephen Ashworth EXTREMOPHILES: The Resilience of Life under “Adverse” Conditions Robert O. J. Weinzierl LIFE BEFORE FERMI – Back to the Solar System David L. Clements ALIEN AIRCRAFT: Have they been observed on Earth? Alan Bond www.bis-space.com ISSN 0007-084X PUBLICATION DATE: 6 DECEMBER 2018 Submitting papers International Advisory Board to JBIS JBIS welcomes the submission of technical Rachel Armstrong, Newcastle University, UK papers for publication dealing with technical Peter Bainum, Howard University, USA reviews, research, technology and engineering in astronautics and related fields. Stephen Baxter, Science & Science Fiction Writer, UK James Benford, Microwave Sciences, California, USA Text should be: James Biggs, The University of Strathclyde, UK ■ As concise as the content allows – typically 5,000 to 6,000 words. Shorter papers (Technical Notes) Anu Bowman, Foundation for Enterprise Development, California, USA will also be considered; longer papers will only Gerald Cleaver, Baylor University, USA be considered in exceptional circumstances – for Charles Cockell, University of Edinburgh, UK example, in the case of a major subject review. Ian A. Crawford, Birkbeck College London, UK ■ Source references should be inserted in the text in square brackets – [1] – and then listed at the Adam Crowl, Icarus Interstellar, Australia end of the paper. Eric W. Davis, Institute for Advanced Studies at Austin, USA ■ Illustration references should be cited in Kathryn Denning, York University, Toronto, Canada numerical order in the text; those not cited in the Martyn Fogg, Probability Research Group, UK text risk omission. Raghavan Gopalaswami, Aerospace Researcher, India ■ Captions must be labelled with their Fig. number and should be as short as possible. Lamartine Guimarães, Institute for Advanced Studies, Brazil Mark Hempsell, Hempsell Astronautics Ltd, UK Illustrations should be: Takuto Ishimatsu, Massachusetts Institute of Technology, USA ■ Colour or mono, but should be as close to print Les Johnson, Marshall Space Flight Center, USA resolution (300 dpi) as possible. Poor-quality illustrations may compromise the acceptance of Terry Kammash, University of Michigan, USA paper for publication. Images embedded in Word Kelvin F. Long, Initiative for Interstellar Studies documents may be acceptable, but JBIS reserves Inoue Makoto, Institute of Astronomy & Astrophysics Academia Sinica, Taiwan the right to request separate higher-resolution Gregory L. Matloff, City University New York, USA image files from the author prior to publication. Koichi Mori, Nagoya University, Japan ■ Responsibility for copyright clearance of images rests entirely with the author. Richard Obousy, Richard Obousy Consulting LLC, USA Robert Parkinson, BIS, Aylesbury, UK Submission of papers George Schmidt, NASA John H Glenn Research Center, Ohio, USA ■ Papers for consideration should be sent by Paul Schuch, The SETI League Inc, USA email to [email protected] as both a Word document and as a Word PDF file (in order to Tabitha Smith, Bifrost, USA check for font anomalies), together with any Andreas Tziolas, Variance Dynamical Corporation, USA separate image files. Chris Welch, The International Space University, Strasbourg, France ■ If a paper is accepted for publication, the Friedwardt Winterberg, University of Nevada, Reno, USA author will be asked to sign a License to Publish form. This can be downloaded at www.bis- space.com/wp-content/uploads/2012/08/ WebsiteLicense.pdf. ■ Authors will receive a complimentary copy of the issue in which their paper appears. Editor Roger Longstaff Deputy Editor Duncan Law-Green Associate Editors Stephen Ashworth, We respectfully ask authors to adhere to these Keith Cooper, Stephen Gamble, Paul Gilster, Rob Swinney, Production MP3 Media guidelines. Failure to do so will result in the Promotion Gill Norman JBIS Office British Interplanetary Society, Arthur C. Clarke House, delay of acceptable papers for publication. 27-29 South Lambeth Road, London, SW8 1SZ, United Kingdom tel +44 (0)20 7735 3160 email [email protected] www.bis-space.com Our full Guidelines for Authors can be downloaded DISTRIBUTION from www.bis-space.com JBIS is distributed worldwide by mail and may be received by annual subscription or purchase of single copies. It is available through membership of the British Interplanetary Society at much reduced rates. Subscription details for members, non-members and libraries are available from the above address. JBIS is a publication that promotes the mission of the British Interplanetary Society. Opinions expressed in signed articles are those of the contributors and do not necessarily reflect the views of the Editor or the Council of the British Interplanetary Society. Security clearance, where necessary, is the responsibility of the author. Published by the British Interplanetary Society. Registered Company No: 402498. Registered Charity No: 250556. Printed by Latimer Trend & Company Ltd, Estover Road, Plymouth, PL6 7PY, England. © 2018 British Interplanetary Society. No part of this magazine may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying or recording by any information storage or retrieval system without prior permission from the Publishers. CONTENTS VOLUME 71 NO.6 JUNE 2018 198 Introduction 200 THE ORIGIN OF THE “FERMI PARADOX” Anthony R. Martin 207 FERMI AND LOTKA: the Long Odds of Survival in a Dangerous Universe Kent A. Peacock 212 SCENARIO BLOCK DIAGRAM ANALYSIS of the Galactic Evolution of Life Stephen Ashworth 216 EXTREMOPHILES: The Resilience of Life under “Adverse” Conditions Robert O. J. Weinzierl 222 LIFE BEFORE FERMI – Back to the Solar System David L. Clements 225 ALIEN AIRCRAFT: Have they been observed on Earth? Alan Bond OUR MISSION STATEMENT The British Interplanetary Society promotes the exploration and use of space for the benefit of humanity, connecting people to create, educate and inspire, and advance knowledge in all aspects of astronautics. JBIS Vol 71 No.6 June 2018 197 INTRODUCTION Introduction by GERRY WEBB FBIS, President of the British Interplanetary Society he idea that there are worlds outside Earth which and extremophiles. I therefore thought it useful to return to may be inhabited has existed throughout history. the topic of the Fermi Paradox, review the new and improved However, Enrico Fermi was the first to voice the data and see if the topic can be freshened and tightened in any problem posed by the absence of evidence of intel- way. Accordingly, to test whether this could be done, and ably Tligent aliens on Earth clearly and with some reason. assisted by Alistair Scott I put together a symposium which was Since he had been a major player in bringing about the nu- run on the 28th November 2017. It was generally agreed that clear age, the first time in history that humans could see how this symposium was a success and produced much interesting the power necessary for interstellar travel could be generated, discussion. Four of the papers presented have been prepared it was but a short step for a man of his calibre to spot the vital for publication in this special JBIS issue and others may follow question ‘where is everybody?’ in future editions. The term ‘Fermi Paradox’ was not coined until later when The papers cover a broad range of topics within the Fermi the ‘evidence for absence’ had begun to build and a conven- Paradox envelope and I am pleased to say that Bond and Mar- ient way of referring to the problem was needed. Stated without tin are represented. The first two papers, by Martin and Pea- frills the paradox is: there should be evidence of (intelligent, cock respectively, were not presented at the symposium, but starfaring, communicative) aliens and there is not. Martin’s paper was stimulated by it and provides an excellent, The paradox usually provokes ‘why’ and ‘how’: Why should even necessary, introduction. Peacock’s paper was submitted there be aliens? How do we know there are no aliens? The first when this edition of JBIS was taking shape and fits perfectly is mainly addressed by pointing to human civilization as a typi- into its theme. cal development of intelligent star-faring life and the second by Radio telescopes were evolving at the same time as nucle- the increasing amount of astronomical evidence which, at first ar power but, because it was clearly much simpler to envisage, glance, would seem to indicate that the conditions necessary interstellar communication by signals was discussed (and at- for the development of civilisations such as our own are com- tempted) first, in the 60s and 70s, to a much greater extent than mon throughout the universe. physical transportation. I will not digress on what, in my opin- We cannot say for sure that intelligent technically capable ion, are the limitations and naivety of the former, save to say beings do not exist elsewhere in the universe, but the evidence that I remember arguing against any form of advertising our for their absence increases every year since Fermi first posed presence during the panel discussion at the 1977 BIS confer- the question in 1950. Nearly 70 years of increasingly sophis- ence referred to by our first author, Anthony R Martin, who ticated data on everything from extremophiles to extrasolar fixes very well the evolution and use of the term ‘Fermi-Par- planets has shown nothing so far. adox’ at about this time. The understandable reason for this In the 70s and 80s the BIS published much pioneer work early bias against physical transport is what are perceived as on Interstellar Studies such as ‘Project Daedalus’, World-ships the large timescales required for interstellar transport. How- and the Fermi Paradox. The main inspirers and leaders of this ever, these timescales are large only in terms of human life and work were Alan Bond and Tony Martin.
Recommended publications
  • Modelling Panspermia in the TRAPPIST-1 System
    October 13, 2017 Modelling panspermia in the TRAPPIST-1 system James A. Blake1,2*, David J. Armstrong1,2, Dimitri Veras1,2 Abstract The recent ground-breaking discovery of seven temperate planets within the TRAPPIST-1 system has been hailed as a milestone in the development of exoplanetary science. Centred on an ultra-cool dwarf star, the planets all orbit within a sixth of the distance from Mercury to the Sun. This remarkably compact nature makes the system an ideal testbed for the modelling of rapid lithopanspermia, the idea that micro-organisms can be distributed throughout the Universe via fragments of rock ejected during a meteoric impact event. We perform N-body simulations to investigate the timescale and success-rate of lithopanspermia within TRAPPIST-1. In each simulation, test particles are ejected from one of the three planets thought to lie within the so-called ‘habitable zone’ of the star into a range of allowed orbits, constrained by the ejection velocity and coplanarity of the case in question. The irradiance received by the test particles is tracked throughout the simulation, allowing the overall radiant exposure to be calculated for each one at the close of its journey. A simultaneous in-depth review of space microbiological literature has enabled inferences to be made regarding the potential survivability of lithopanspermia in compact exoplanetary systems. 1Department of Physics, University of Warwick, Coventry, CV4 7AL 2Centre for Exoplanets and Habitability, University of Warwick, Coventry, CV4 7AL *Corresponding author: [email protected] Contents Universe, and can propagate from one location to another. This interpretation owes itself predominantly to the works of William 1 Introduction1 Thompson (Lord Kelvin) and Hermann von Helmholtz in the 1.1 Mechanisms for panspermia...............2 latter half of the 19th Century.
    [Show full text]
  • Far Side of the Moore by Sean Grundy
    Far Side Of The Moore By Sean Grundy CHARACTERS PATRICK MOORE (early 30s)...eccentric amateur astronomer PAUL JOHNSTONE (mid 30s)...BBC science producer DR HENRY KING (40s) ...soon-to-be head of the BAA PERCY WILKINS (60s) ...Moore’s mentor EILEEN WILKINS (early 20s) ...Percy’s daughter ARTHUR C CLARKE (late 30s)...Moore’s friend GERTRUDE MOORE (60s)...Moore’s mother LEONARD MIALL (40s)...BBC Head of Talks ANNOUNCER; STUDIO FM; TRANSMISSION CONTROL; HENRY KING’S SECRETARY; NEWS REPORTER; GEORGE ADAMSKI; BAA PRESIDENT Set in mid-1950s at BBC TV, BAA meeting room and Patrick’s home, East Grinstead. (Draft 4 - 27/01/15) SCENE 1.INTRO. SFX SPACEY FX/MUSIC ANNOUNCER The following drama is based on the true story of Patrick Moore and the making of ‘The Sky At Night’. PATRICK MOORE (OLDER) All true, even the stuff I exaggerated to jolly up the proceedings. However, I do apologise for my restraint on more colourful opinions: PC-brigade, female producers, Europhiles and all that. Damn irritating.. (FADE) SFX SPACEY MUSIC – MIX TO – RADIO DIAL REWINDING BACK IN TIME TO: SCENE 2.INT. BBC STUDIO. 1957 ARCHIVE (OR MOCK-UP) CYRIL STAPLETON’S PARADE MUSIC PLAYS PAUL JOHNSTONE ..Countdown to live in 90..Ident, please.. STUDIO FM (ON TALKBACK) Sky At Night. Programme 1. 24/4/57. 10.30pm. Transmission, do you have a feed? TRANSMISSION CONTROL (ON TALKBACK) Hello, studio. Rolling credits on ‘Cyril Stapleton Parade’. I see your slate: (READS) ‘Producer, Paul Johnstone. Host, Patrick Meere.’ STUDIO FM (ON TALKBACK) ‘Moore’. TRANSMISSION CONTROL Correction, ‘Moore’. STUDIO FM (ON TALKBACK) Live in 60.
    [Show full text]
  • Lecture-29 (PDF)
    Life in the Universe Orin Harris and Greg Anderson Department of Physics & Astronomy Northeastern Illinois University Spring 2021 c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 1 / 95 Overview Dating Rocks Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 2 / 95 Dating Rocks Zircon Dating Sedimentary Grand Canyon Life on Earth How Did Life Arise? Life in the Solar System Life Around Dating Rocks Other Stars Interstellar Travel SETI Review c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 3 / 95 Zircon Dating Zircon, (ZrSiO4), minerals incorporate trace amounts of uranium but reject lead. Naturally occuring uranium: • U-238: 99.27% • U-235: 0.72% Decay chains: • 238U −→ 206Pb, τ =4.47 Gyrs. • 235U −→ 207Pb, τ = 704 Myrs. 1956, Clair Camron Patterson dated the Canyon Diablo meteorite: τ =4.55 Gyrs. c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 4 / 95 Dating Sedimentary Rocks • Relative ages: Deeper layers were deposited earlier • Absolute ages: Decay of radioactive isotopes old (deposited last) oldest (depositedolder first) c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 5 / 95 Grand Canyon: Earth History from 200 million - 2 billion yrs ago. Dating Rocks Life on Earth Earth History Timeline Late Heavy Bombardment Hadean Shark Bay Stromatolites Cyanobacteria Q: Earliest Fossils? Life on Earth O2 History Q: Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2021 G.
    [Show full text]
  • Biosignatures Search in Habitable Planets
    galaxies Review Biosignatures Search in Habitable Planets Riccardo Claudi 1,* and Eleonora Alei 1,2 1 INAF-Astronomical Observatory of Padova, Vicolo Osservatorio, 5, 35122 Padova, Italy 2 Physics and Astronomy Department, Padova University, 35131 Padova, Italy * Correspondence: [email protected] Received: 2 August 2019; Accepted: 25 September 2019; Published: 29 September 2019 Abstract: The search for life has had a new enthusiastic restart in the last two decades thanks to the large number of new worlds discovered. The about 4100 exoplanets found so far, show a large diversity of planets, from hot giants to rocky planets orbiting small and cold stars. Most of them are very different from those of the Solar System and one of the striking case is that of the super-Earths, rocky planets with masses ranging between 1 and 10 M⊕ with dimensions up to twice those of Earth. In the right environment, these planets could be the cradle of alien life that could modify the chemical composition of their atmospheres. So, the search for life signatures requires as the first step the knowledge of planet atmospheres, the main objective of future exoplanetary space explorations. Indeed, the quest for the determination of the chemical composition of those planetary atmospheres rises also more general interest than that given by the mere directory of the atmospheric compounds. It opens out to the more general speculation on what such detection might tell us about the presence of life on those planets. As, for now, we have only one example of life in the universe, we are bound to study terrestrial organisms to assess possibilities of life on other planets and guide our search for possible extinct or extant life on other planetary bodies.
    [Show full text]
  • Exploring Biogenic Dispersion Inside Star Clusters with System Dynamics Modeling
    Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 12 October 2020 doi:10.20944/preprints202010.0232.v1 Exploring Biogenic Dispersion Inside Star Clusters with System Dynamics Modeling Authors Javier D. Burgos. Corporación para la Investigacion e Innovación -CIINAS. Contact: [email protected] Diana C. Sierra. Corporación para la Investigacion e Innovación -CIINAS; Bogotá, Colombia. Contact: [email protected] Abstract The discovery of a growing number of exoplanets and even extrasolar systems supports the scientific consensus that it is possible to find other signs of life in the universe. The present work proposes for the first time, an explicit mechanism inspired by the dynamics of biological dispersion, widely used in ecology and epidemiology, to study the dispersion of biogenic units, interpreted as complex organic molecules, between rocky or water exoplanets (habitats) located inside star clusters. The 3 results of the dynamic simulation suggest that for clusters with populations lower than 4 M/ly it is not possible to obtain biogenic worlds after 5 Gyr. Above this population size, biogenic dispersion seems to follow a power law, the larger the density of worlds lesser will be the impact rate (훽.) value to obtain at least one viable biogenic Carrier habitat after 5 Gyr. Finally, when we investigate scenarios by varying β, a well-defined set of density intervals can be defined in accordance to its characteristic β value, suggesting that biogenic dispersion has a behavior of “minimal infective dose” of “minimal biogenic effective” events by interval i.e. once this dose has been achieved, doesn’t matter if additional biogenic impact events occur on the habitat.
    [Show full text]
  • A Theoretical Astro-Biological Solution for Femi's Paradox
    2019 International Conference on Social Science, Economics and Management Research (SSEMR 2019) ISBN: 978-1-60595-638-1 A Theoretical Astro-biological Solution for Femi’s Paradox Xiang-rui LUO* and Wei WANG University of North Carolina at Chapel Hill, NC, USA Guiyang University, Guizhou, China *Corresponding author Keywords: Astrophysics, Femi’s paradox, Extraterrestrial civilizations. Abstract. The Great Filter Theory is a commonly accepted solution for Fermi’s Paradox, indicating that there is a huge wall preventing the intelligent species from achieving Level III Civilization, Galactic Civilization, which has the ability to control the energy on the scale its entire galaxy. There are many forms of hypothesis about what the Great Filter is, such as unbreakable light speed limit. Here we analyze the hypothesis that the Great Filter is the irreconcilable predicament between advanced technology and limited lifespan, which inevitably leads to stagnation in technology development. Introduction The Fermi paradox, or Fermi's paradox is the apparent contradiction between the lack of evidence and high probability estimates for the existence of extraterrestrial civilizations. The basic reasoning line, made by physicists Enrico Fermi (1901–1954) and Michael H. Hart (born 1932), are: There are at least 100 billion planets in our Galaxy alone (Cassan et al. 2012), and about 20% are of habitable zone (Petigura et al. 2013). With high probability, some of these stars have Earth-like planets, and if the Earth is typical, some may have developed intelligent life. Some of these civilizations may have developed interstellar travel, a step the Earth is investigating now. Even at the slow pace of currently envisioned interstellar travel, the Milky Way galaxy could be completely traversed in a few million years.
    [Show full text]
  • God and Design: the Teleological Argument and Modern Science
    GOD AND DESIGN Is there reason to think a supernatural designer made our world? Recent discoveries in physics, cosmology, and biochemistry have captured the public imagination and made the design argument—the theory that God created the world according to a specific plan—the object of renewed scientific and philosophical interest. Terms such as “cosmic fine-tuning,” the “anthropic principle,” and “irreducible complexity” have seeped into public consciousness, increasingly appearing within discussion about the existence and nature of God. This accessible and serious introduction to the design problem brings together both sympathetic and critical new perspectives from prominent scientists and philosophers including Paul Davies, Richard Swinburne, Sir Martin Rees, Michael Behe, Elliott Sober, and Peter van Inwagen. Questions raised include: • What is the logical structure of the design argument? • How can intelligent design be detected in the Universe? • What evidence is there for the claim that the Universe is divinely fine-tuned for life? • Does the possible existence of other universes refute the design argument? • Is evolutionary theory compatible with the belief that God designed the world? God and Design probes the relationship between modern science and religious belief, considering their points of conflict and their many points of similarity. Is God the “master clockmaker” who sets the world’s mechanism on a perfectly enduring course, or a miraculous presence continually intervening in and altering the world we know? Are science and faith, or evolution and creation, really in conflict at all? Expanding the parameters of a lively and urgent contemporary debate, God and Design considers the ways in which perennial questions of origin continue to fascinate and disturb us.
    [Show full text]
  • Monday, November 13, 2017 WHAT DOES IT MEAN to BE HABITABLE? 8:15 A.M. MHRGC Salons ABCD 8:15 A.M. Jang-Condell H. * Welcome C
    Monday, November 13, 2017 WHAT DOES IT MEAN TO BE HABITABLE? 8:15 a.m. MHRGC Salons ABCD 8:15 a.m. Jang-Condell H. * Welcome Chair: Stephen Kane 8:30 a.m. Forget F. * Turbet M. Selsis F. Leconte J. Definition and Characterization of the Habitable Zone [#4057] We review the concept of habitable zone (HZ), why it is useful, and how to characterize it. The HZ could be nicknamed the “Hunting Zone” because its primary objective is now to help astronomers plan observations. This has interesting consequences. 9:00 a.m. Rushby A. J. Johnson M. Mills B. J. W. Watson A. J. Claire M. W. Long Term Planetary Habitability and the Carbonate-Silicate Cycle [#4026] We develop a coupled carbonate-silicate and stellar evolution model to investigate the effect of planet size on the operation of the long-term carbon cycle, and determine that larger planets are generally warmer for a given incident flux. 9:20 a.m. Dong C. F. * Huang Z. G. Jin M. Lingam M. Ma Y. J. Toth G. van der Holst B. Airapetian V. Cohen O. Gombosi T. Are “Habitable” Exoplanets Really Habitable? A Perspective from Atmospheric Loss [#4021] We will discuss the impact of exoplanetary space weather on the climate and habitability, which offers fresh insights concerning the habitability of exoplanets, especially those orbiting M-dwarfs, such as Proxima b and the TRAPPIST-1 system. 9:40 a.m. Fisher T. M. * Walker S. I. Desch S. J. Hartnett H. E. Glaser S. Limitations of Primary Productivity on “Aqua Planets:” Implications for Detectability [#4109] While ocean-covered planets have been considered a strong candidate for the search for life, the lack of surface weathering may lead to phosphorus scarcity and low primary productivity, making aqua planet biospheres difficult to detect.
    [Show full text]
  • Problems with Panspermia Or Extraterrestrial Origin of Life Scenarios As Found on the IDEA Center Website At
    Problems with Panspermia or Extraterrestrial Origin of Life Scenarios As found on the IDEA Center website at http://www.ideacenter.org Panspermia is the theory that microorganisms or biochemical compounds from outer space are responsible for originating life on Earth and possibly in other parts of the universe where suitable atmospheric conditions exist. Essentially, it is a hypothesis which states that life on earth came from outer space. It has been popularized in countless science fiction works, however some scientists, including the discoverer of the structure of DNA, Francis Crick, have advocated panspermia. There are generally about 3 different "flavors" of panspermia: 1. Naturalistic Panspermia where life evolves on another planet, and naturally gets ejected off the planet and come to rest on earth. 2. Directed Panspermia where intelligent life on other planets intentionally seeded other planets with their own form of life. 3. Intelligent Design Panspermia, where intelligent beings from another planet came to earth and designed life here. Each type of panspermia will be briefly discussed below: 1. Naturalistic Panspermia where life evolves on another planet, and naturally gets ejected off the planet and come to rest on earth. Naturalistic panspermia has gained popularity because some have recognized that life on earth appears very soon after the origin of conditions which would allow it to exist. Many scientists believed that if life had originated on earth it would have taken many hundreds of millions, or even billions of years to do so. Life appears perhaps less than 200 million after the origin of conditions at which life could exist.
    [Show full text]
  • Fermi's Paradox Is a Daunting Problem – Under Whatever Label
    Fermi's Paradox Is a Daunting Problem – Under Whatever Label Milan M. Dirkovid1 Astronomical Observatory of Belgrade, Volgina 7, 11000 Belgrade, Serbia 1. Introduction Gray (2015) argued that Fermi's paradox (FP) is a misnomer, and it is not a valid paradox. Gray also speculated that the argument was misattributed to Fermi, whose lunchtime remarks did not pertain to the existence of extraterrestrial intelligence, but to the feasibility of interstellar travel. Instead, the paradox is ascribed to Hart and Tipler, and it is further suggested that the paradox is not a “real” problem or research subject and should not be used in debates about SETI projects. The arguments given are unpersuasive, ahistorical, and, in at least one instance, clearly hinge on literalistic and uncharitable reading of evidence. Instead, I argue the following three points: (i) Contrary to Gray’s assertion, the historical issue of naming of ideas or concepts is completely divorced from their epistemic status. (ii) FP is easily and smoothly generalized into the “Great Silence” paradox, so it makes no sense either theoretically or empirically to separate the two. (iii) In sharp contrast to the main implication of Gray’s paper, FP has become more aggravated lately due to advances in astrobiology. Research that deals with FP has greatly expanded in recent years on both a theoretical and observational stage (Davies 2010, 2012; Vukotid and Dirkovid 2012; Barlow 2013; Hair and Hedman 2013; Davies and Wagner 2013; Armstrong and Sandberg 2013; Lampton 2013; Cartin 2014; Nunn, Guy, and Bell 2014; Wright et al. 2014; Spivey 2015; Griffith et al.
    [Show full text]
  • Arxiv:1910.06396V4 [Physics.Pop-Ph] 12 Jun 2021 ∗ Rmtv Ieeitdi H R-Oa Eua(Vni H C System)
    Nebula-Relay Hypothesis: Primitive Life in Nebula and Origin of Life on Earth Lei Feng1,2, ∗ 1Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023 2Joint Center for Particle, Nuclear Physics and Cosmology, Nanjing University – Purple Mountain Observatory, Nanjing 210093, China Abstract A modified version of panspermia theory, named Nebula-Relay hypothesis or local panspermia, is introduced to explain the origin of life on Earth. Primitive life, acting as the seeds of life on Earth, originated at pre-solar epoch through physicochemical processes and then filled in the pre- solar nebula after the death of pre-solar star. Then the history of life on the Earth can be divided into three epochs: the formation of primitive life in the pre-solar epoch; pre-solar nebula epoch; the formation of solar system and the Earth age of life. The main prediction of our model is that primitive life existed in the pre-solar nebula (even in the current nebulas) and the celestial body formed therein (i.e. solar system). arXiv:1910.06396v4 [physics.pop-ph] 12 Jun 2021 ∗Electronic address: [email protected] 1 I. INTRODUCTION Generally speaking, there are several types of models to interpret the origin of life on Earth. The two most persuasive and popular models are the abiogenesis [1, 2] and pansper- mia theory [3]. The modern version of abiogenesis is also known as chemical origin theory introduced by Oparin in the 1920s [1], and Haldane proposed a similar theory independently [2] at almost the same time. In this theory, the organic compounds are naturally produced from inorganic matters through physicochemical processes and then reassembled into much more complex living creatures.
    [Show full text]
  • Fermi Paradox: a Simulation Solution YU HAIHAN, MARK
    Fermi Paradox: a simulation solution YU HAIHAN, MARK Introduction The paradox was proposed by Fermi in 1950 during a lunch with Edward Teller, Hilbert York and Emil Konopinski. When they were talking about mundane topics, Fermi asked a question:”Where is everybody?”(Webb, 2002) His partners immediately understood what he was talking about: If the extraterrestrial civilization exists, why we have not met them till now? If we believe that there is nothing special about earth and solar system, there should be other civilizations in the universe as its enormous size containing countless probabilities. Under such assumptions, the paradox occurred. To provide a forceful explanation, many efforts have been paid on the analysis on Drake equation. Drake equation: The number of civilization in the universe is represented by N. To estimate it, we need to know the yearly rate R at which stars forms the galaxy; the probability fp of stars that possess planets; the number ne of planets with suitable environment for life; the probability fl of suitable planets on which life actually develops; the probability fi of these planets on which develops intelligence; the probability fc of these intelligence that could communicate with other civilizations and the time L that such a culture would devote to communication (Webb, 2002). Though the equation is complicated as above, it can be just divided into 3 main factors. Consider the following equation: n=Npq This equation is provided by Professor David Aldous, which can be viewed as a simple version of Drake equation. In this equation, N is the number of suitable planets for life; p is the chance that an intelligence species would develop a capability to communicate with others and q the chance that such a species would survive in such a way as to be observable (Aldous, 2010).
    [Show full text]