The Mystery of Methane on Mars and Titan
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A Stringent Upper Limit of 20 Pptv for Methane on Mars and Constraints on Its Dispersion Outside Gale Crater F
A&A 650, A140 (2021) Astronomy https://doi.org/10.1051/0004-6361/202140389 & © F. Montmessin et al. 2021 Astrophysics A stringent upper limit of 20 pptv for methane on Mars and constraints on its dispersion outside Gale crater F. Montmessin1 , O. I. Korablev2 , A. Trokhimovskiy2 , F. Lefèvre3 , A. A. Fedorova2 , L. Baggio1 , A. Irbah1 , G. Lacombe1, K. S. Olsen4 , A. S. Braude1 , D. A. Belyaev2 , J. Alday4 , F. Forget5 , F. Daerden6, J. Pla-Garcia7,8 , S. Rafkin8 , C. F. Wilson4, A. Patrakeev2, A. Shakun2, and J. L. Bertaux1 1 LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt, France e-mail: [email protected] 2 Space Research Institute (IKI) RAS, Moscow, Russia 3 LATMOS/IPSL, Sorbonne Université, UVSQ Université Paris-Saclay, CNRS, Paris, France 4 AOPP, Oxford University, Oxford, UK 5 Laboratoire de Météorologie Dynamique, Sorbonne Université, Paris, France 6 BIRA-IASB, Bruxelles, Belgium 7 Centro de Astrobiología (CSIC?INTA), Torrejón de Ardoz, Spain 8 Southwest Research Institute, Boulder, CO, USA Received 20 January 2021 / Accepted 23 April 2021 ABSTRACT Context. Reports on the detection of methane in the Martian atmosphere have motivated numerous studies aiming to confirm or explain its presence on a planet where it might imply a biogenic or more likely a geophysical origin. Aims. Our intent is to complement and improve on the previously reported detection attempts by the Atmospheric Chemistry Suite (ACS) on board the ExoMars Trace Gas Orbiter (TGO). This latter study reported the results of a campaign that was a few months in length, and was significantly hindered by a dusty period that impaired detection performances. -
Atmospheric Dust on Mars: a Review
47th International Conference on Environmental Systems ICES-2017-175 16-20 July 2017, Charleston, South Carolina Atmospheric Dust on Mars: A Review François Forget1 Laboratoire de Météorologie Dynamique (LMD/IPSL), Sorbonne Universités, UPMC Univ Paris 06, PSL Research University, Ecole Normale Supérieure, Université Paris-Saclay, Ecole Polytechnique, CNRS, Paris, France Luca Montabone2 Laboratoire de Météorologie Dynamique (LMD/IPSL), Paris, France & Space Science Institute, Boulder, CO, USA The Martian environment is characterized by airborne mineral dust extending between the surface and up to 80 km altitude. This dust plays a key role in the climate system and in the atmospheric variability. It is a significant issue for any system on the surface. The atmospheric dust content is highly variable in space and time. In the past 20 years, many investigations have been conducted to better understand the characteristics of the dust particles, their distribution and their variability. However, many unknowns remain. The occurrence of local, regional and global-scale dust storms are better documented and modeled, but they remain very difficult to predict. The vertical distribution of dust, characterized by detached layers exhibiting large diurnal and seasonal variations, remains quite enigmatic and very poorly modeled. Nomenclature Ls = Solar Longitude (°) MY = Martian year reff = Effective radius τ = Dust optical depth (or dust opacity) CDOD = Column Dust Optical Depth (i.e. τ integrated over the atmospheric column) IR = Infrared LDL = Low Dust Loading (season) HDL = High Dust Loading (season) MGS = Mars Global Surveyor (NASA spacecraft) MRO = Mars Reconnaissance Orbiter (NASA spacecraft) MEX = Mars Express (ESA spacecraft) TES = Thermal Emission Spectrometer (instrument aboard MGS) THEMIS = Thermal Emission Imaging System (instrument aboard NASA Mars Odyssey spacecraft) MCS = Mars Climate Sounder (instrument aboard MRO) PDS = Planetary Data System (NASA data archive) EDL = Entry, Descending, and Landing GCM = Global Climate Model I. -
Environmental Philosophy and the Ethics of Terraforming Mars
ENVIRONMENTAL PHILOSOPHY AND THE ETHICS OF TERRAFORMING MARS: ADDING THE VOICES OF ENVIRONMENTAL JUSTICE AND ECOFEMINISM TO THE ONGOING DEBATE Robert Heath French Thesis Prepared for the Degree of MASTER OF ARTS UNIVERSITY OF NORTH TEXAS August 2013 APPROVED: Robert Figueroa, Committee Chair Eugene Hargrove, Committee Member Adam Briggle, Committee Member Patricia Glazebrook, Chair of the Department of Philosophy and Religion Studies Mark Wardell, Dean of the Toulouse Graduate School French, Robert Heath. Environmental Philosophy and the Ethics of Terraforming Mars: Adding the Voices of Environmental Justice and Ecofeminism to the Ongoing Debate. Master of Arts (Philosophy), August 2013, 133 pp., 1 table, bibliography, 78 titles. Questions concerning the ethics of terraforming Mars have received some attention from both philosophers and scientists during recent decades. A variety of theoretical approaches have been supplied by a number of authors, however research pursuant to this thesis has indicated at least two major blindspots in the published literature on the topic. First, a broad category of human considerations involving risks, dangers, and social, political, and economic inequalities that would likely be associated with efforts to terraform Mars have been woefully overlooked in the published literature to date. I attempt to rectify that oversight by employing the interpretive lens of environmental justice to address questions of environmental colonialism, equality in terms of political participation and inclusion in decision making structures, risks associated with technological progressivism, and responses to anthropogenic climate change. Only by including the historically marginalized and politically disenfranchised “voices,” of both humans and nonhumans, can any future plan to terraform Mars be deemed ethical, moral or just according to the framework provided by environmental justice. -
TIME Space Newsletter September 10, 2019
TIME Space Newsletter September 10, 2019 Dear readers, Not a lot of people would want to go back to the Paleocene Epoch. For one thing, the dinosaurs were only beginning to die out, and while they'd be nifty to see, they were murder on mammals. It would be a good 65 million years before humans got a literal toe-hold on the world. The Eocene wouldn't be much better. It was around that time that what is now the Indian subcontinent crashed into Asia, and while all that produced some lovely mountains, there was a lot of slo-mo violence of clashing plates before things settled down. As far as epochs go, the Holocene is everyone's favorite. It started close to 12,000 years ago, as the last Ice Age was ending, and produced the conditions that allowed all the species we love best—ourselves, and charismatic megafauna like the bald eagle, the panda and the tiger—to thrive. From humanity's perspective, it would be perfectly fine if the Holocene went on forever. But it won't. It's ending now—it may have already ended in the 1950s, according to some scientists—to be replaced by the Anthropocene. The name says it all: it's an epoch in which one species—ours, anthro—became the leading driver of the state of the planet, more powerful, at least in the short-term, than the larger forces of geology, meteorology, even biology. We have, of course, abused that power, fouling the air, annihilating species, wiping out forests and distorting the climate. -
Evidence for Methane in Martian Meteorites
Blamey, N. J. F., Parnell, J., McMahon, S., Mark, D. F., Tomkinson, T., Lee, M., Shivak, J., Izawa, M. R. M., Banerjee, N. R., & Flemming, R. L. (2015). Evidence for methane in Martian meteorites. Nature Communications, 6, [7399]. https://doi.org/10.1038/ncomms8399 Publisher's PDF, also known as Version of record License (if available): CC BY Link to published version (if available): 10.1038/ncomms8399 Link to publication record in Explore Bristol Research PDF-document This is the final published version of the article (version of record). It first appeared online via Nature Publishing Group at doi:10.1038/ncomms8399. Please refer to any applicable terms of use of the publisher. University of Bristol - Explore Bristol Research General rights This document is made available in accordance with publisher policies. Please cite only the published version using the reference above. Full terms of use are available: http://www.bristol.ac.uk/red/research-policy/pure/user-guides/ebr-terms/ ARTICLE Received 19 Sep 2014 | Accepted 1 May 2015 | Published 16 Jun 2015 DOI: 10.1038/ncomms8399 OPEN Evidence for methane in Martian meteorites Nigel J.F. Blamey1,2, John Parnell2, Sean McMahon2, Darren F. Mark3, Tim Tomkinson3,4, Martin Lee4, Jared Shivak5, Matthew R.M. Izawa5, Neil R. Banerjee5 & Roberta L. Flemming5 The putative occurrence of methane in the Martian atmosphere has had a major influence on the exploration of Mars, especially by the implication of active biology. The occurrence has not been borne out by measurements of atmosphere by the MSL rover Curiosity but, as on Earth, methane on Mars is most likely in the subsurface of the crust. -
Astrobiology for a General Reader
Astrobiology for a General Reader Astrobiology for a General Reader: A Questions and Answers Approach By Vera M. Kolb and Benton C. Clark III Astrobiology for a General Reader: A Questions and Answers Approach By Vera M. Kolb and Benton C. Clark III This book first published 2020 Cambridge Scholars Publishing Lady Stephenson Library, Newcastle upon Tyne, NE6 2PA, UK British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library Copyright © 2020 by Vera M. Kolb and Benton C. Clark III All rights for this book reserved. No part of this book may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the copyright owner. ISBN (10): 1-5275-5502-X ISBN (13): 978-1-5275-5502-0 V. M. K. dedicates this book to the memory of her dear brother, Vladimir Kolb. B. C. C. dedicates this book to the memory of his beloved wife, Johanna. TABLE OF CONTENTS Preface ....................................................................................................... ix Acknowledgments ..................................................................................... xi Chapter 1 .................................................................................................... 1 What is astrobiology? Chapter 2 .................................................................................................... 5 Understanding the concept of life within the astrobiology framework: -
The Science of Astrobiology
The Science of Astrobiology Cellular Origin, Life in Extreme Habitats and Astrobiology ________________________________________________________________ Volume 20 (Second Edition) ________________________________________________________________ Julian Chela-Flores The Science of Astrobiology A Personal View on Learning to Read the Book of Life Julian Chela-Flores The Abdus Salam International Centre for Theoretical Physics P.O. Box 586 34014 Trieste Italy [email protected] ISSN 1566-0400 ISBN 978-94-007-1626-1 e-ISBN 978-94-007-1627-8 DOI 10.1007/978-94-007-1627-8 Springer Dordrecht Heidelberg London New York Library of Congress Control Number: 2011934255 © Springer Science+Business Media B.V. 2011 No part of this work may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, microfilming, recording or otherwise, without written permission from the Publisher, with the exception of any material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) The cupola in the West Atrium of St. Mark's Basilica in Venice, Italy representing the biblical interpretation of Genesis (Cf., also pp. 215-216 at the beginning of Part 4: The destiny of life in the universe. With kind permission of the Procuratoria of St. Mark's Basilica.) For Sarah Catherine Mary Table of contents Table of contents vii Preface xvii Acknowledgements xxi Recommendations to the readers xxiii INTRODUCTION The cultural and scientific context of astrobiology I.1 Early attempts to read the Book of Life 3 ARISTARCHUS OF SAMOS AND HIPPARCHUS 4 NICHOLAS OF CUSA (CUSANUS) 4 NICHOLAS COPERNICUS 4 GIORDANO BRUNO 5 CHARLES DARWIN 6 I.2 Some pioneers of the science of astrobiology 8 ALEXANDER OPARIN 8 STANLEY MILLER 10 SIDNEY W. -
Planetary Science
Mission Directorate: Science Theme: Planetary Science Theme Overview Planetary Science is a grand human enterprise that seeks to discover the nature and origin of the celestial bodies among which we live, and to explore whether life exists beyond Earth. The scientific imperative for Planetary Science, the quest to understand our origins, is universal. How did we get here? Are we alone? What does the future hold? These overarching questions lead to more focused, fundamental science questions about our solar system: How did the Sun's family of planets, satellites, and minor bodies originate and evolve? What are the characteristics of the solar system that lead to habitable environments? How and where could life begin and evolve in the solar system? What are the characteristics of small bodies and planetary environments and what potential hazards or resources do they hold? To address these science questions, NASA relies on various flight missions, research and analysis (R&A) and technology development. There are seven programs within the Planetary Science Theme: R&A, Lunar Quest, Discovery, New Frontiers, Mars Exploration, Outer Planets, and Technology. R&A supports two operating missions with international partners (Rosetta and Hayabusa), as well as sample curation, data archiving, dissemination and analysis, and Near Earth Object Observations. The Lunar Quest Program consists of small robotic spacecraft missions, Missions of Opportunity, Lunar Science Institute, and R&A. Discovery has two spacecraft in prime mission operations (MESSENGER and Dawn), an instrument operating on an ESA Mars Express mission (ASPERA-3), a mission in its development phase (GRAIL), three Missions of Opportunities (M3, Strofio, and LaRa), and three investigations using re-purposed spacecraft: EPOCh and DIXI hosted on the Deep Impact spacecraft and NExT hosted on the Stardust spacecraft. -
1 National Press Club Headliners Luncheon with Ellen Stofan, Director, National Air and Space Museum Subject: the Future of T
NATIONAL PRESS CLUB HEADLINERS LUNCHEON WITH ELLEN STOFAN, DIRECTOR, NATIONAL AIR AND SPACE MUSEUM SUBJECT: THE FUTURE OF THE MUSEUM MODERATOR: DONNA LEINWAND OF THE NATIONAL PRESS CLUB LOCATION: NATIONAL PRESS CLUB, HOLEMAN LOUNGE, WASHINGTON, D.C. TIME: 1:00 P.M. DATE: MONDAY, OCTOBER 22, 2018 (c) COPYRIGHT 2018, NATIONAL PRESS CLUB, 529 14TH STREET, WASHINGTON, DC - 20045, USA. ALL RIGHTS RESERVED. ANY REPRODUCTION, REDISTRIBUTION OR RETRANSMISSION IS EXPRESSLY PROHIBITED. UNAUTHORIZED REPRODUCTION, REDISTRIBUTION OR RETRANSMISSION CONSTITUTES A MISAPPROPRIATION UNDER APPLICABLE UNFAIR COMPETITION LAW, AND THE NATIONAL PRESS CLUB RESERVES THE RIGHT TO PURSUE ALL REMEDIES AVAILABLE TO IT IN RESPECT TO SUCH MISAPPROPRIATION. FOR INFORMATION ON BECOMING A MEMBER OF THE NATIONAL PRESS CLUB, PLEASE CALL 202-662-7505. ANDREA EDNEY: –Andrea Edney. A couple of really important announcements. The first one is, this is your device. This is your device on mute, vibrate, silence, et cetera. If your phone rings, I'm going to point at you on live television. So please take this opportunity to silence your cell phone now. Also, if you are on Twitter, we do encourage you to tweet during the program. Our hashtag today is #NPCLive. That's #NPCLive. And then also, you have on your table these fabulous cards. If you have questions for our speaker today, please write your questions on these cards. Please print or write as legibly as you can. If you write in cursive, your chance of my reading your question on TV is about the same as the Mega Millions lottery. [laughter] So please print. And then when you've written your question, you can pass it up to the head table, however you want to do it. -
George Lakoff and Mark Johnsen (2003) Metaphors We Live By
George Lakoff and Mark Johnsen (2003) Metaphors we live by. London: The university of Chicago press. Noter om layout: - Sidetall øverst - Et par figurer slettet - Referanser til slutt Innholdsfortegnelse i Word: George Lakoff and Mark Johnsen (2003) Metaphors we live by. London: The university of Chicago press. ......................................................................................................................1 Noter om layout:...................................................................................................................1 Innholdsfortegnelse i Word:.................................................................................................1 Contents................................................................................................................................4 Acknowledgments................................................................................................................6 1. Concepts We Live By .....................................................................................................8 2. The Systematicity of Metaphorical Concepts ...............................................................11 3. Metaphorical Systematicity: Highlighting and Hiding.................................................13 4. Orientational Metaphors.................................................................................................16 5. Metaphor and Cultural Coherence .................................................................................21 6 Ontological -
The Search for Extreme Life
BIOCHEMIST_BARUCH S. BLUMBERG The Search for Extreme Life ofile If microorganisms exist on other worlds, the head of NASA’s fledgling Astrobiology Institute plans to find them he relentless heat cooks the the space agency aims to someday find “Technology is available to decipher Pr Badwater region of California’s on other worlds. the intricacies of this cause-and-effect Death Valley so thoroughly that “I always liked the idea of doing field- chain” that wasn’t available even five some expanses are textured like work, exploring, going out and finding years ago, Blumberg notes, citing in par- Tdry serpent skin. At some 284 feet below new things,” Blumberg says back at NAI ticular advances achieved through the sea level—North America’s lowest point— headquarters, which is nestled near Sili- Human Genome Project. The 1996 an- it is perhaps the hottest place on the sur- con Valley at the NASA Ames Research nouncement of potential fossilized life in face of the earth: the temperature once Center at Moffett Field. Out of his desert a Martian meteorite known as ALH84001 peaked at a record 53.01 degrees Celsius garb, the outdoors-loving Blumberg looks boosted enthusiasm worldwide. Even (127.4 degrees Fahrenheit). Out here, a good decade younger than his 75 years. Congress, which had quashed NASA’s blood-pumping mammals are scarce. It At the job only since last September, Blum- search for extraterrestrial intelligence may seem unfitting to find a Nobel Prize berg is trying to marshal gaggles of as- (SETI) program in 1993, became recep- winner, renowned for hepatitis B work, tronomers, chemists, ecologists, geologists, tive. -
Strategies for Detecting Biological Molecules on Titan
ASTROBIOLOGY Volume 18, Number 5, 2018 ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2017.1758 Strategies for Detecting Biological Molecules on Titan Catherine D. Neish,1 Ralph D. Lorenz,2 Elizabeth P. Turtle,2 Jason W. Barnes,3 Melissa G. Trainer,4 Bryan Stiles,5 Randolph Kirk,6 Charles A. Hibbitts,2 and Michael J. Malaska5 Abstract Saturn’s moon Titan has all the ingredients needed to produce ‘‘life as we know it.’’ When exposed to liquid water, organic molecules analogous to those found on Titan produce a range of biomolecules such as amino acids. Titan thus provides a natural laboratory for studying the products of prebiotic chemistry. In this work, we examine the ideal locales to search for evidence of, or progression toward, life on Titan. We determine that the best sites to identify biological molecules are deposits of impact melt on the floors of large, fresh impact craters, specifically Sinlap, Selk, and Menrva craters. We find that it is not possible to identify biomolecules on Titan through remote sensing, but rather through in situ measurements capable of identifying a wide range of biological molecules. Given the nonuniformity of impact melt exposures on the floor of a weathered impact crater, the ideal lander would be capable of precision targeting. This would allow it to identify the locations of fresh impact melt deposits, and/or sites where the melt deposits have been exposed through erosion or mass wasting. Determining the extent of prebiotic chemistry within these melt deposits would help us to understand how life could originate on a world very different from Earth.