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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. -
Lecture 9—Is the Earth Rare?
41st Saas-Fee Course From Planets to Life 3-9 April 2011 Lecture 9—Is the Earth Rare? List of Rare Earth arguments/ Nitrogen abundance/ Frequency of large impacts/ Chaotic obliquity fluctuations J. F. Kasting The Gaia hypothesis First presented in the 1970s by James Lovelock 1979 1988 • Life itself is what stabilizes planetary environments • Corollary: A planet might need to be inhabited in order to remain habitable The Medea and Rare Earth hypotheses Peter Ward 2009 2000 Medea hypothesis: Life is harmful to the Earth! Rare Earth hypothesis: Complex life (animals, including humans) is rare in the universe Additional support for the Rare Earth hypothesis • Lenton and Watson think that complex life (animal life) is rare because it requires a series of unlikely evolutionary events – the origin of life – the origin of the genetic code – the development of oxygenic photosynthesis) – the origin of eukaryotes – the origin of sexuality 2011 Rare Earth/Gaia arguments 1. Plate tectonics is rare --We have dealt with this already. Plate tectonics is not necessarily rare, but it requires liquid water. Thus, a planet needs to be within the habitable zone. 2. Other planets may lack magnetic fields and may therefore have harmful radiation environments and be subject to loss of atmosphere – We have talked about this one also. Venus has retained its atmosphere. The atmosphere itself provides protection against cosmic rays 3. The animal habitable zone (AHZ) is smaller than the habitable zone (HZ) o – AHZ definition: Ts = 0-50 C o – HZ definition: Ts = 0-100 C. But this is wrong! For a 1-bar atmosphere like Earth, o water loss begins when Ts reaches 60 C. -
Livre-Ovni.Pdf
UN MONDE BIZARRE Le livre des étranges Objets Volants Non Identifiés Chapitre 1 Paranormal Le paranormal est un terme utilisé pour qualifier un en- mé n'est pas considéré comme paranormal par les semble de phénomènes dont les causes ou mécanismes neuroscientifiques) ; ne sont apparemment pas explicables par des lois scien- tifiques établies. Le préfixe « para » désignant quelque • Les différents moyens de communication avec les chose qui est à côté de la norme, la norme étant ici le morts : naturels (médiumnité, nécromancie) ou ar- consensus scientifique d'une époque. Un phénomène est tificiels (la transcommunication instrumentale telle qualifié de paranormal lorsqu'il ne semble pas pouvoir que les voix électroniques); être expliqué par les lois naturelles connues, laissant ain- si le champ libre à de nouvelles recherches empiriques, à • Les apparitions de l'au-delà (fantômes, revenants, des interprétations, à des suppositions et à l'imaginaire. ectoplasmes, poltergeists, etc.) ; Les initiateurs de la parapsychologie se sont donné comme objectif d'étudier d'une manière scientifique • la cryptozoologie (qui étudie l'existence d'espèce in- ce qu'ils considèrent comme des perceptions extra- connues) : classification assez injuste, car l'objet de sensorielles et de la psychokinèse. Malgré l'existence de la cryptozoologie est moins de cultiver les mythes laboratoires de parapsychologie dans certaines universi- que de chercher s’il y a ou non une espèce animale tés, notamment en Grande-Bretagne, le paranormal est inconnue réelle derrière une légende ; généralement considéré comme un sujet d'étude peu sé- rieux. Il est en revanche parfois associé a des activités • Le phénomène ovni et ses dérivés (cercle de culture). -
University of Groningen Evaluating Galactic Habitability Using High
University of Groningen Evaluating galactic habitability using high-resolution cosmological simulations of galaxy formation Forgan, Duncan; Dayal, Pratika; Cockell, Charles; Libeskind, Noam Published in: International Journal of Astrobiology DOI: 10.1017/S1473550415000518 IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Final author's version (accepted by publisher, after peer review) Publication date: 2017 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Forgan, D., Dayal, P., Cockell, C., & Libeskind, N. (2017). Evaluating galactic habitability using high- resolution cosmological simulations of galaxy formation. International Journal of Astrobiology, 16(1), 60–73. https://doi.org/10.1017/S1473550415000518 Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). The publication may also be distributed here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne” license. More information can be found on the University of Groningen website: https://www.rug.nl/library/open-access/self-archiving-pure/taverne- amendment. Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
Habitable Zone
How to Find a Habitable Planet James Kasting Department of Geosciences Penn State University The search for other habitable worlds is ancient “There are infinite worlds both like and unlike this world of ours...”--- Epicurus (c. 300 BCE) (died painfully 269 BCE) “… false and "There are countless suns and damnable ...” countless earths …” G. Galilei (b. 1564) Giordano Bruno (b. 1584) in De L'infinito Universo E Mondi From Mike Devirian, (life imprisonment JPL (burned at the stake in Campo 1633) dei Fiore, Rome, 1600) • Even today, opinions differ widely as to whether other Earth-like planets exist… The Gaia hypothesis First presented in the 1970s by James Lovelock 1979 1988 http://www.ecolo.org/lovelock Gaia—The Greek goddess • According to this hypothesis, life creates and maintains conditions for its own existence by stabilizing Earth’s climate and other aspects of the Earth system • If this idea is correct, then only planets that are already inhabited would be habitable http://www.paleothea.com/Majors.html The Medea and Rare Earth hypotheses Peter Ward 2009 2000 Medea hypothesis: Life is harmful to the Earth! Rare Earth hypothesis: Complex life (animals, including humans) is rare in the universe The latest addition to this literature Me My new book (Princeton University Press, 2010) • As you will see, I am more optimistic than either Peter Ward or Jim Lovelock Talk outline • Introduction (which you heard already) • Part 1: What makes Earth unique, and what is life? • Part 2: Can we find Earth-like planets around other stars, and can -
Astrobiology Life in the Universe
Astrobiology Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe. In simplest terms, it is the study of life in the universe–both on Earth and off it. It combines the search for habitable environments in the Solar System and beyond with research into the evolution and adaptability of life here on Earth. By knitting together research in astrophysics, earth science, and heliophysics as well as planetary science, astrobiology seeks to answer fundamental scientific questions about life: how it begins and evolves; what biological, planetary, and cosmic conditions must exist in order for it to take hold; and whether there is/was/can be life elsewhere in the galaxy. Dr. Alka Misra Assistant Professor Department of Mathematics & Astronomy University of Lucknow What is Astrobiology! Astrobiology is the study of life in the Universe – where it is, how it came to be there, what it is like, and where it might be going. As the only life we know about for sure is on Earth, a lot of astrobiology is about trying to predict where we might find life elsewhere. Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe. This interdisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System, the search for evidence of prebiotic chemistry, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in outer space. -
Quantum Chemical Computational Methods Have Proved to Be An
10465 Arnab Shome/ Elixir Space Sci. 50 (2012) 10465 Available online at www.elixirpublishers.com (Elixir International Journal) Space Science Elixir Space Sci. 50 (2012) 10465 Rare Intelligent Life on Universe Arnab Shome 238/A, Sarat Bose Road, Kolkata-700065, India. ARTICLE INFO ABSTRACT Article history: Even though we have advanced tremendously in technology in the 21st century, we still have Received: 30 July 2012; not been able to contact with any extraterrestrial civilizations. There have been many Received in revised form: research and hypothesis on extraterrestrial civilizations such as The Drake Equation, The 5 September 2012; Fermi Paradox, Rare Earth Hypothesis. With the help of previous research and hypothesis on Accepted: 14 September 2012; this subject by others, I have here tried to find out the possible reasons of not been able to contact with any extraterrestrial civilizations till now. Keywords © 2012 Elixir All rights reserved. Drake Equation, Fermi Paradox, Rare Earth Hypothesis. Introduction 2) They exist but have not yet communicated Drake Equation 3) Civilizations only have a limited lifetime. They are all dead. In 1961Dr.Frank Drake was working as a radio astronomer Rare Earth Hypothesis at the National Radio Astronomy Observatory in Green Bank, The Rare Earth Hypothesis proposed by Peter Ward and West Virginia. It was at this time he came up with a equation Don Brownlee in their book Rare Earth: Why Complex Life is involving the number of advanced civilizations in our galaxy. Uncommon in the Universe lists a variety of reasons to conclude The Drake equation states that: that advanced life is extremely rare in the Universe.(3) Broadly, it states: where: Microbial life is common in planetary systems. -
Life Before Its Origin on Earth: Implications of a Late Emergence of Terrestrial Life
LIFE BEFORE ITS ORIGIN ON EARTH: IMPLICATIONS OF A LATE EMERGENCE OF TERRESTRIAL LIFE Julian Chela-Flores*,{ *The Abdus Salam ICTP, Trieste, Italy {IDEA, Caracas, Venezuela CHAPTER OUTLINE 1 Introduction.................................................................................................................................... 343 1.1 Time Available Before the Emergence of Life on Earth...................................................... 344 1.2 Rationalizing Our Origins in Terms of Thermodynamics..................................................... 345 2 How Would We See Ourselves if Early Origins are Identified?............................................................ 345 2.1 Approaching the End of Biocentrism if Life on Earth is a Latecomer .................................. 346 2.2 Anthropocentrism .......................................................................................................... 346 3 Philosophical Comments on An Early “Forest of Life” ........................................................................ 346 3.1 Process Philosophy........................................................................................................ 346 3.2 Stellar Evolution............................................................................................................ 347 3.3 Cultural Comments on An Early forest of Life................................................................... 347 4 Terrestrial Life as a Latecomer in Cosmic Evolution ......................................................................... -
On the Evolution of Galactic Habitability
On the Evolution of Galactic Habitability Master's Thesis in Astromundus by Gerardo Martinez Aviles Submitted to the Faculty of Mathematics, Computer Science and Physics of the University of Innsbruck in Partial Fulfillment of the Requirements for the Degree of Magister / Magistra der Naturwissenschaften Supervisor: Dr. Branislav Vukotic and Univ.-Prof. Dr. Sabine Schindler Innsbruck, August 2013. Abstract The Galactic Habitable Zone is a concept that was introduced for the Milky Way galaxy in order to complete the knowledge of the places in the Universe hospitable for complex life as we know it. In this work we will discuss the concept of Galactic habitability and explore how it behaves using a N-body/SPH simulation of the dynamics and evolution of a spiral galaxy using the GADGET- 2 code. To our knowledge, it is the first time that this approach is taken. We analyse how the different criteria chosen to develop complex life, such as enough metallicity and time to develop complexity, and how the presence of Supernova explosions, Gamma-ray bursts and high stellar density as life threat- ening phenomena affect the temporal and spatial distribution of habitable sites in the Galaxy, working separately and together. The impact that the different life threatening phenomena considered have on Galactic habitability is also quantified. We find that this approach is in good accordance of previous calculations of boundaries of the Galactic Habitable Zone found in literature and is a viable platform to do astrobiological research. 1 Contents 1 Introduction 4 2 Habitability Concepts 9 2.1 Galactic Habitable Zone . 9 2.2 Circumstellar Habitable Zone . -
The Galactic Habitable Zone and the Age Distribution of Complex Life In
R ESEARCH A RTICLES ducing the earliest born CR neurons. To con- during development the progenitor cells lose 23. S. Xuan et al., Neuron 14, 1141 (1995). firm this, we followed the fate of deep-layer their competence to revert to earliest born neu- 24. C. Hanashima, L. Shen, S. C. Li, E. Lai, J. Neurosci. 22, tetO-foxg1 6526 (2002). neurons in Foxg1 -E13Doxy mice. rons in the absence of Foxg1. 25. G. D. Frantz, J. M. Weimann, M. E. Levin, S. K. McConnell, We found that fewer cells expressed ER81, J. Neurosci. 14, 5725 (1994). and those that were generated were not co- References and Notes 26. R. J. Ferland, T. J. Cherry, P. O. Preware, E. E. Morrisey, labeled with BrdU (fig. S6). This suggests 1. T. Isshiki, B. Pearson, S. Holbrook, C. Q. Doe, Cell 106, C. A. Walsh, J. Comp. Neurol. 460, 266 (2003). 511 (2001). 27. Y. Sumi et al., Neurosci. Lett. 320, 13 (2002). that ER81 neurons observed in these animals 2. T. Brody, W. F. Odenwald, Development 129, 3763 (2002). 28. B. Xu et al., Neuron 26, 233 (2000). were born before doxycycline administration. 3. F. J. Livesey, C. L. Cepko, Nature Rev. Neurosci. 2, 109 29. D. M. Weisenhorn, E. W. Prieto, M. R. Celio, Brain Res. In control mice, many ER81 cells were BrdU- (2001). Dev. Brain Res. 82, 293 (1994). 4. T. M. Jessell, Nature Rev. Genet. 1, 20 (2000). 30. R. K. Stumm et al., J. Neurosci. 23, 5123 (2003). positive, showing that under normal condi- 5. S. -
Pos(APCS2016)001 the Impact of the Space Ex- " Published in 2004 by the Kluwer Accretion Processes in Cosmic Sources: † ∗
Accretion Processes in Astrophysics: The State of Art PoS(APCS2016)001 Franco Giovannelli∗† INAF - Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere, 100, 00133 Roma, Italy E-mail: [email protected] Lola Sabau-Graziati INTA- Dpt. Cargas Utiles y Ciencias del Espacio, C/ra de Ajalvir, Km 4 - E28850 Torrejón de Ardoz, Madrid, Spain E-mail: [email protected] In this review paper we will discuss about the accretion processes that regulates the growth and evolution of all objects in the Universe. We will make a short cruise discussing the accretion in Young Stellar Objects (YSOs), in Planets (Pts), in White Dwarfs (WDs), in Neutron Stars (NSs), and in Black Holes (BHs) independent of their masses. In this way we will mark the borders of the arguments discussed during this workshop on Accretion Processes in Cosmic Sources: Young Stellar Objects, Cataclysmic Variables and Related Objects, X-ray Binary Systems, Active Galactic Nuclei. This paper gets information from updated versions of the book "The Impact of the Space Ex- periments on Our Knowledge of the Physics of the Universe" published in 2004 by the Kluwer Academic Publishers, reprinted from the review paper by Giovannelli, F. & Sabau-Graziati, L.: 2004, Space Sci. Rev. 112, 1-443 (GSG2004), and subsequent considered lucubrations. The review is a source of a huge amount of references. Thus, who wants to enter in details in one of the discussed arguments can find an almost exhaustive list of specific references. Accretion Processes in Cosmic Sources "APCS2016" 5-10 September 2016, Saint Petersburg, Russia ∗Speaker.