Directed Panspermia Synthetic DNA in Bioforming Planets
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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. -
Analysis of the Absorption of Science Learning in National Examinations in 2019 at the Junior High School Level in Sleman District
INTERNATIONAL JOURNAL OF SCIENTIFIC & TECHNOLOGY RESEARCH VOLUME 9, ISSUE 03, MARCH 2020 ISSN 2277-8616 Analysis Of The Absorption Of Science Learning In National Examinations In 2019 At The Junior High School Level In Sleman District Muhammad Minan Chusni, Sulistyo Saputro, Suranto, Sentot Budi Rahardjo Abstract: This study aims to describe the ability of students in national examinations in science learning in terms of their absorption. The method used in this study was a survey with a quantitative approach. The object of research is 146 junior high schools with a total of 14,983 students in the Sleman district. The data used were the national exam's absorption of science learning provided by the education assessment center of the ministry of education and culture. The results showed that the highest mean of absorption is in the material aspects of mechanics and the solar system of 71.60 which is classified as good category, while the lowest average is in the material aspects of waves, electricity and magnetism at 45.56 which is classified as fewer categories. In addition, the lowest mean on the indicator question about waves, electricity and magnetism is "presenting an illustration of two people with eye defects wearing glasses and then determining the ratio of reading distance between the two people" amounted to 28.39, which is classified as very poor category. From these results it can be concluded that the indicator questions about optical material in the ability to analysis are still very poor. Keyword: Science Learning, National Examination. —————————— —————————— 1. INTRODUCTION As for nationally it is used as a mapping of the quality of Education and progress of a nation are two related things [1]. -
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. -
Representations in Sustainability Science
REPRESENTATIONS IN SUSTAINABILITY SCIENCE TOOLS TO ANALYZE, ENVISION, ENGAGE, AND LEARN BEATRICE JOHN “Representation in Sustainability Science: Tools to Analyze, Envision, Engage, and Learn” Academic dissertation Submitted to the Faculty of Sustainability of Leuphana University for the award of the degree Doctor of Philosophy -Dr. phil.- approved by Beatrice John, born Feb 18, 1985, in Achern Submission: January 7, 2019 Defense: March 25, 2019 Supervisor and first reviewer: Prof. Dr. Daniel J. Lang Second reviewer: Prof. Dr. Henrik von Wehrden Third reviewer: Prof. Dr. John Holmberg The articles included here, which together form this cumulative dissertation, have been or will be published in the formats listed below. Chapters 1-3 and 5-6 framing of this thesis may be published in future. John, B., Lang, D.J., von Wehrden, H., John, R., Wiek, A., n.d. Advancing Decision-Visualization Environments-empirically informed Design Guidelines. doi:10.13140/RG.2.2.26933.32486 John, B., Luederitz, C., Lang, D.J., von Wehrden, H., 2019. Toward Sustainable Urban Metabolisms. From System Understanding to System Transformation. Ecol. Econ. 157, 402–414. doi:10.1016/j.ecolecon.2018.12.007 John, B., Withycombe Keeler, L., Wiek, A., Lang, D.J., 2015. How much sustainability substance is in urban visions? – An analysis of visioning projects in urban planning. Cities 48, 86–98. doi:10.1016/j.cities.2015.06.001 Caniglia, G., John, B., Kohler, M., Bellina, L., Wiek, A., Rojas, C., Laubichler, M.D., Lang, D., 2016. An experience-based learning framework. Activities for the initial development of sustainability competencies. Int. J. Sustain. High. -
INTEGRATION of SCIENCE and LANGUAGE with a FOCUS on MULTILINGUAL LEARNERS: SHARED OPPORTUNITIES and RESPONSIBILITIES Okhee Lee* New York University
Keynote Conference Address INTEGRATION OF SCIENCE AND LANGUAGE WITH A FOCUS ON MULTILINGUAL LEARNERS: SHARED OPPORTUNITIES AND RESPONSIBILITIES Okhee Lee* New York University This article highlights the importance of promoting science and language learning for all students, especially multilingual learners. In recent years, there have been parallel instructional shifts in science and language with multilingual learners, which enables integration of science and language in mutually supportive ways. These instructional shifts have resulted in new opportunities for collaboration between language educators and science educators as well as development of new instructional resources. Such collaboration and resources are essential for creating equity for multilingual learners. In this article, I describe contemporary perspectives on integrating science and language with multilingual learners across policy, research, and practice. I also provide a classroom example using a unit from the Science And Integrated Language (SAIL) curriculum and a series of webinars and briefs based on the SAIL curriculum for the New York State Education Department. It was an honor to be invited to give a talk at the 50th anniversary of the New York State TESOL conference in 2020. I feel privileged to be included among the group of distinguished speakers invited to address the organization. I am honored again to be invited to write this article for our membership. The purpose of the article is to highlight the importance of promoting science and language learning for multilingual learners. New opportunities for collaboration between language educators and science educators are being forged as well as new instructional resources are being developed. Such collaboration and resources are essential for creating equity for multilingual learners. -
A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System
Space Sci Rev (2020) 216:100 https://doi.org/10.1007/s11214-020-00719-1 A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System Martin Turbet1 · Emeline Bolmont1 · Vincent Bourrier1 · Brice-Olivier Demory2 · Jérémy Leconte3 · James Owen4 · Eric T. Wolf5 Received: 14 January 2020 / Accepted: 4 July 2020 / Published online: 23 July 2020 © The Author(s) 2020 Abstract TRAPPIST-1 is a fantastic nearby (∼39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount of irradiation. To date, this is the most observationally favourable system of po- tentially habitable planets known to exist. Since the announcement of the discovery of the TRAPPIST-1 planetary system in 2016, a growing number of techniques and approaches have been used and proposed to characterize its true nature. Here we have compiled a state- of-the-art overview of all the observational and theoretical constraints that have been ob- tained so far using these techniques and approaches. The goal is to get a better understanding of whether or not TRAPPIST-1 planets can have atmospheres, and if so, what they are made of. For this, we surveyed the literature on TRAPPIST-1 about topics as broad as irradiation environment, planet formation and migration, orbital stability, effects of tides and Transit Timing Variations, transit observations, stellar contamination, density measurements, and numerical climate and escape models. Each of these topics adds a brick to our understand- ing of the likely—or on the contrary unlikely—atmospheres of the seven known planets of the system. -
Materials Challenges for the Starshot Lightsail
PERSPECTIVE https://doi.org/10.1038/s41563-018-0075-8 Materials challenges for the Starshot lightsail Harry A. Atwater 1*, Artur R. Davoyan1, Ognjen Ilic1, Deep Jariwala1, Michelle C. Sherrott 1, Cora M. Went2, William S. Whitney2 and Joeson Wong 1 The Starshot Breakthrough Initiative established in 2016 sets an audacious goal of sending a spacecraft beyond our Solar System to a neighbouring star within the next half-century. Its vision for an ultralight spacecraft that can be accelerated by laser radiation pressure from an Earth-based source to ~20% of the speed of light demands the use of materials with extreme properties. Here we examine stringent criteria for the lightsail design and discuss fundamental materials challenges. We pre- dict that major research advances in photonic design and materials science will enable us to define the pathways needed to realize laser-driven lightsails. he Starshot Breakthrough Initiative has challenged a broad nanocraft, we reveal a balance between the high reflectivity of the and interdisciplinary community of scientists and engineers sail, required for efficient photon momentum transfer; large band- Tto design an ultralight spacecraft or ‘nanocraft’ that can reach width, accounting for the Doppler shift; and the low mass necessary Proxima Centauri b — an exoplanet within the habitable zone of for the spacecraft to accelerate to near-relativistic speeds. We show Proxima Centauri and 4.2 light years away from Earth — in approxi- that nanophotonic structures may be well-suited to meeting such mately -
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects NASA Grant No. NNX17AE81G First Year Report Prepared by: Marc G. Millis, Jeff Greason, Rhonda Stevenson Tau Zero Foundation Business Office: 1053 East Third Avenue Broomfield, CO 80020 Prepared for: NASA Headquarters, Space Technology Mission Directorate (STMD) and NASA Innovative Advanced Concepts (NIAC) Washington, DC 20546 June 2018 Millis 2018 Grant NNX17AE81G_for_CR.docx pg 1 of 69 ABSTRACT Progress toward developing an evaluation process for interstellar propulsion and power options is described. The goal is to contrast the challenges, mission choices, and emerging prospects for propulsion and power, to identify which prospects might be more advantageous and under what circumstances, and to identify which technology details might have greater impacts. Unlike prior studies, the infrastructure expenses and prospects for breakthrough advances are included. This first year's focus is on determining the key questions to enable the analysis. Accordingly, a work breakdown structure to organize the information and associated list of variables is offered. A flow diagram of the basic analysis is presented, as well as more detailed methods to convert the performance measures of disparate propulsion methods into common measures of energy, mass, time, and power. Other methods for equitable comparisons include evaluating the prospects under the same assumptions of payload, mission trajectory, and available energy. Missions are divided into three eras of readiness (precursors, era of infrastructure, and era of breakthroughs) as a first step before proceeding to include comparisons of technology advancement rates. Final evaluation "figures of merit" are offered. Preliminary lists of mission architectures and propulsion prospects are provided. -
Cometary Panspermia a Radical Theory of Life’S Cosmic Origin and Evolution …And Over 450 Articles, ~ 60 in Nature
35 books: Cosmic origins of life 1976-2020 Physical Sciences︱ Chandra Wickramasinghe Cometary panspermia A radical theory of life’s cosmic origin and evolution …And over 450 articles, ~ 60 in Nature he combined efforts of generations supporting panspermia continues to Prof Wickramasinghe argues that the seeds of all life (bacteria and viruses) Panspermia has been around may have arrived on Earth from space, and may indeed still be raining down some 100 years since the term of experts in multiple fields, accumulate (Wickramasinghe et al., 2018, to affect life on Earth today, a concept known as cometary panspermia. ‘primordial soup’, referring to Tincluding evolutionary biology, 2019; Steele et al., 2018). the primitive ocean of organic paleontology and geology, have painted material not-yet-assembled a fairly good, if far-from-complete, picture COMETARY PANSPERMIA – cultural conceptions of life dating back galactic wanderers are normal features have argued that these could not into living organisms, was first of how the first life on Earth progressed A SOLUTION? to the ideas of Aristotle, and that this of the cosmos. Comets are known to have been lofted from the Earth to a coined. The question of how from simple organisms to what we can The word ‘panspermia’ comes from the may be the source of some of the have significant water content as well height of 400km by any known process. life’s molecular building blocks see today. However, there is a crucial ancient Greek roots ‘sperma’ meaning more hostile resistance the idea of as organics, and their cores, kept warm Bacteria have also been found high in spontaneously assembled gap in mainstream understanding - seed, and ‘pan’, meaning all. -
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. -
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. -
Optimizing a Solar Sailing Polar Mission to the Sun
Optimizing a Solar Sailing Polar Mission to the Sun Development and Application of a New Ant Colony Optimizer Giacomo Acciarini Optimizing a Solar Sailing Polar Mission to the Sun Development and Application of a New Ant Colony Optimizer by Giacomo Acciarini to obtain the degree of Master of Science at the Delft University of Technology, to be defended publicly on Friday November 1, 2019 at 1:30 PM. Student number: 4754883 Project duration: January 4, 2019 – November 1, 2019 Thesis committee: Prof. Dr. P. Visser, TU Delft, chair Dr. ir. E. Mooij, TU Delft, supervisor Dr. F. Oliviero, TU Delft Dr. D. Izzo, European Space Agency This thesis is confidential and cannot be made public until December 31, 2020. An electronic version of this thesis is available at http://repository.tudelft.nl/. Cover image credit: https://www.theguardian.com/science/2015/jun/11/ spacewatch-lightsail-deploys-solar-sail, date of access: August 2019. ii Preface After months of hard work, I am proud to present to you my thesis to obtain the Master of Science degree at the faculty of Aerospace Engineering, at the Delft University of Technology. It has been an amazing experience that allowed me to come in contact with many researchers from all over the world who share my same love and interest in space exploration. I have always felt privileged and honored to be able to study such a marvelous and challenging subject. First of all, I would thus like to thank my parents, Andrea and Manuela, and my sister, Chiara, without your help and support I would have never been able to reach this point.