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Mars, the Nearest Habitable World – a Comprehensive Program for Future Mars Exploration
Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Report by the NASA Mars Architecture Strategy Working Group (MASWG) November 2020 Front Cover: Artist Concepts Top (Artist concepts, left to right): Early Mars1; Molecules in Space2; Astronaut and Rover on Mars1; Exo-Planet System1. Bottom: Pillinger Point, Endeavour Crater, as imaged by the Opportunity rover1. Credits: 1NASA; 2Discovery Magazine Citation: Mars Architecture Strategy Working Group (MASWG), Jakosky, B. M., et al. (2020). Mars, the Nearest Habitable World—A Comprehensive Program for Future Mars Exploration. MASWG Members • Bruce Jakosky, University of Colorado (chair) • Richard Zurek, Mars Program Office, JPL (co-chair) • Shane Byrne, University of Arizona • Wendy Calvin, University of Nevada, Reno • Shannon Curry, University of California, Berkeley • Bethany Ehlmann, California Institute of Technology • Jennifer Eigenbrode, NASA/Goddard Space Flight Center • Tori Hoehler, NASA/Ames Research Center • Briony Horgan, Purdue University • Scott Hubbard, Stanford University • Tom McCollom, University of Colorado • John Mustard, Brown University • Nathaniel Putzig, Planetary Science Institute • Michelle Rucker, NASA/JSC • Michael Wolff, Space Science Institute • Robin Wordsworth, Harvard University Ex Officio • Michael Meyer, NASA Headquarters ii Mars, the Nearest Habitable World October 2020 MASWG Table of Contents Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Table of Contents EXECUTIVE SUMMARY .......................................................................................................................... -
Prebiotic Chemistry, Origin, and Early Evolution of Life
Say what you are going to say, say it, say what you said Guiding theory Richard Feynman Polyelectrolytes with uniform structure are universal for Darwinism A specific hypothesis to provide context The polyelectrolyte that supported Earth’s first Darwinism was RNA Focus on paradoxes to constrain human self-deception "Settled science" says that RNA is impossible to form prebiotically Strategies for paradox resolution Mineral-guided processes allow RNA to form nonetheless Natural history context The needed chemistry-mineral combination was transient on Earth Your reward A relatively simple path to form RNA prebiotically A relatively narrow date when life on Earth originated prebiotically A clear statement of the next round of paradoxes Elisa Biondi, Hyo-Joong Kim, Daniel Hutter, Clemens Richert, Stephen Mojzsis, Ramon Brasser, Dustin Trail, Kevin Zahnle, David Catling, Rob Lavinsky Say what you are going to say, say it, say what you said Guiding theory Richard Feynman Polyelectrolytes with uniform structure are universal for Darwinism A specific hypothesis to provide context The polyelectrolyte that supported Earth’s first Darwinism was RNA Focus on paradoxes to constrain human self-deception "Settled science" says that RNA is impossible to form prebiotically Strategies for paradox resolution Mineral-guided processes allow RNA to form nonetheless Natural history context The needed chemistry-mineral combination was transient on Earth Your reward A relatively simple path to form RNA prebiotically A relatively narrow date when life on Earth originated prebiotically A clear statement of the next round of paradoxes Elisa Biondi, Hyo-Joong Kim, Daniel Hutter, Clemens Richert, Stephen Mojzsis, Ramon Brasser, Dustin Trail, Kevin Zahnle, David Catling, Rob Lavinsky What does a repeating backbone charge do for informational molecule? O 1. -
Snowball Earth: a Thin-Ice Solution with Flowing Sea Glaciers’’ by David Pollard and James F
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, C09016, doi:10.1029/2005JC003411, 2006 Click Here for Full Article Comment on ‘‘Snowball Earth: A thin-ice solution with flowing sea glaciers’’ by David Pollard and James F. Kasting Stephen G. Warren1,2 and Richard E. Brandt1 Received 22 November 2005; revised 22 May 2006; accepted 9 June 2006; published 14 September 2006. Citation: Warren, S. G., and R. E. Brandt (2006), Comment on ‘‘Snowball Earth: A thin-ice solution with flowing sea glaciers’’ by David Pollard and James F. Kasting, J. Geophys. Res., 111, C09016, doi:10.1029/2005JC003411. 1. Introduction 2. Choices of Model Variables That Favor [1] Pollard and Kasting [2005] (hereinafter referred to as Thin Ice PK) have coupled an energy-balance climate model to an 2.1. Albedo of Cold Glacier Ice ice-shelf flow model, to investigate the Snowball Earth [2] As sea glaciers flowed equatorward into the tropical episodes of the Neoproterozoic, 600–800 million years region of net sublimation, their surface snow and subsurface ago, when the ocean apparently froze all the way to the firn would sublimate away, exposing bare glacier ice to equator [Hoffman and Schrag, 2002]. PK’s particular con- the atmosphere and solar radiation. This ice would be cern was to investigate the possibility that over a wide freshwater (meteoric) ice, which originated from compres- equatorial band where sublimation exceeded snowfall, the sion of snow, so it would contain numerous bubbles, giving bare ice may have been thin enough to permit transmission a high albedo. The albedo of cold (nonmelting) glacier ice of sunlight to the water below, providing an extensive exposed by sublimation (Antarctic ‘‘blue ice’’) has been refugium for the photosynthetic eukaryotes that survived measured as 0.55–0.65 in four experiments in the Atlantic the Snowball events. -
The First Billion Years: Warm and Wet Or Cold and Icy? Robert M
The First Billion Years: Warm and Wet or Cold and Icy? Robert M. Haberle Space Science and Astrobiology Division NASA/Ames Research Center July 15, 2014 Mars 8 Meeting Acknowledgements: Mike Carr, David Catling, and Kevin Zahnle Haberle, 8th Mars Conference Evidence for a Different Valley Networks Climate Isotopic Heavy Isotopes Aqueous Minerals 14N/15N 170±15 (Viking) 20Ne/22Ne ~10 (Meteorites) 36Ar/38Ar 4.2±0.2 (MSL) δ13C 46±4‰ (MSL) Elmann and Edwards (2014) 129Xe/132Xe ~ 2.5 (Viking) Haberle, 8th Mars Conference The First Billion Years Haberle, 8th Mars Conference Faint Young Sun Problem Noachian Haberle, 8th Mars Conference Atmospheric Redox and Outgassing The oxidation state of volcanic gases (principally H2/H2O) is governed by the oxidation state (fO2) of the upper mantle. During core(a) formation After core(b) formation Since core formation was fast (< 10 My), the mantle was likely weakly reducing and Outgassing products were mostly CO2, H2O, and N2 Haberle, 8th Mars Conference 1-D Calculations of Pollack et al. (1987) Main Conclusion: Early Mars was Continuously Warm and Wet - 5 bars of CO2 maintained against carbonate loss by impact recycling Haberle, 8th Mars Conference Problems With This Model Haberle, 8th Mars Conference 1. CO2 condenses in the atmosphere reducing the greenhouse effect. Latent heat release warms the upper atmosphere Kasting (1991) Haberle, 8th Mars Conference 2. Collision Induced Absorption Overestimated We now have more accurate absorption data based on theoretical and experimental data Old parameterizations overestimated induced-dipole absorption -1 in the 250-500 cm region Haberle, 8th Mars Conference Wordsworth et al. -
Life Beyond the Solar System: Remotely Detectable Biosignatures
Life Beyond the Solar System: Remotely Detectable Biosignatures Shawn Domagal-Goldman 1,NancyY.Kiang2,NikiParenteau3,DavidC.Catling4,Shiladitya DasSarma 5,YukaFujii6,ChesterE.Harman7,AdrianLenardic8,EnricPall´e9,ChristopherT. Reinhard 10,EdwardW.Schwieterman11,JeanSchneider12,HarrisonB.Smith13,Motohide Tamura 14,DanielAngerhausen15,GiadaArney1 ,VladimirS.Airapetian16,NatalieM. Batalha 3 ,CharlesS.Cockell17,LeroyCronin18,RussellDeitrick19,AnthonyDelGenio2 , Theresa Fisher 13 ,DawnM.Gelino20,J.LeeGrenfell21,HilairyE.Hartnett13 ,Siddharth Hegde 22,YasunoriHori23,Bet¨ulKa¸car24,JoshuaKrissansen-Totten4 ,TimothyLyons11 , William B. Moore 25,NorioNarita26,StephanieL.Olson11 Heike Rauer 27,TylerD.Robinson 28,SarahRugheimer29,NickSiegler30,EvgenyaL.Shkolnik13 ,KarlR.Stapelfeldt30 ,Sara Walker 31 1NASA Goddard Space Flight Center,2NASA Goddard Institute for Space Studies,3NASA Ames Research Center,4Dept. Earth and Space Sciences / Astrobiology Program, University of Washington,5Institute of Marine and Environmental Technology, University of Maryland School of Medicine, Baltimore, Maryland,6Earth-Life Science Institute, Tokyo Institute of Technology and NASA Goddard Institute for Space Studies,7Columbia University and NASA Goddard Institute for Space Studies,8Rice Univer- sity ,9Instituto de Astrof´ısica de Canaria, Spain,10School of Earth and Atmospheric Sciences, Georgia Institute of Technology,11Dept. Earth Sciences, University of California, Riverside, California,12Paris Observatory,13School of Earth and Space Exploration, Arizona State University,14University -
Astrobiology Fights for Its Life
NEWSFOCUS Astrobiology Fights for Its Life A decade after NASA pledged to create a robust program to find and understand life in the universe, researchers face a debilitating budget crunch and skepticism within their own agency THESE SHOULD BE HEADY TIMES FOR tist on Mars exploration. Researchers are for astrobiology within the space agency and astrobiologists. Reports of recent liquid afraid that the field may go the way of the outside. And the new Congress, which water on Mars and organic matter in the far agency’s life and materials science effort, a includes a more powerful California delega- reaches of the solar system signal that the once-robust $1 billion program now virtually tion, is expected to go to bat for the field in fledgling discipline, which seeks to under- extinct as more pressing needs in the human upcoming budget battles with the White stand the nature of life in the universe, is space flight program have siphoned off funds. House. “We’re going to emerge from this in coming of age. Add an expanding roster of Those fears grew stronger last summer when an even stronger position,” insists Carl newly discovered extrasolar planets and NASA Administrator Michael Griffin told the Pilcher, the new NAI director. But others examples of life flourishing in extreme envi- Mars Society that astrobiology is marginal to aren’t so sanguine. “I feel a pang in my stom- ronments on Earth—amid the high ultra- the agency’s mission. The fiscal downturn has ach,” says Kenneth Nealson, a biologist at the violet of the Andes, in Australian radioactive meant staff cuts at the program’s centerpiece, University of Wisconsin, Madison. -
The Rationale for a Long-Lived Geophysical
THE RATIONALE FOR A LONG-LIVED GEOPHYSICAL NETWORK MISSION TO MARS Submitted to The Mars Panel, NRC Decadal Survey for the Planetary Sciences Division, SMD, NASA Phil Christensen, Chair; Wendy Calvin, Vice Chair Written by Bruce Banerdt JPL Robert Grimm SwRI Franck Montmessin Scot Rafkin SwRI Tilman Spohn DLR Matthias Grott DLR Service Aeronomie Peter Read Oxford Ulli Christensen MPS Bob Haberle NASA-Ames Yosio Nakamura Gerald Schubert UCLA Veronique Dehant ROB Martin Knapmeyer DLR U Texas (ret.) Sue Smrekar JPL Linda Elkins-Tanton MIT Philippe Lognonné IPGP Roger Phillips SwRI Mike Wilson JPL Endorsed by Oded Aharonson Caltech François Forget Kurt Klaus Boeing Thomas Ruedas Carnegie Don Albert CRREL CNRS-LMD Jörg Knollenberg DLR Chris Russell UCLA Carlton Allen NASA-JSC Matt Fouch ASU Naoki Kobayashi JAXA David Sandwell Scripps Robert Anderson JPL Brenda Franklin JPL Ulrich Koehler DLR Nicholas Schmerr Carnegie Scott Anderson SwRI Herbert Frey GSFC Carlos Lange U Alberta Nicole Schmitz DLR Jeff Andrews-Hanna Jeannine Gagnepain- Gary Latham DOE (ret.) Richard Schultz U Nevada Colo. School of Mines Beyneix IPGP Mark Leese Open U Mindi Searls U Colorado Jafar Arkani-Hamed Rafael Garcia Frank Lemoine GSFC Karsten Seiferlin U Bern McGill U Obs. Midi-Pyrenees Robert Lillis UC Berkeley Nikolai Shapiro IPGP Gabriele Arnold U Münster Jim Garvin GSFC John Longhi Charles Shearer UNM Sami Asmar JPL Rebecca Ghent U Toronto Lamont-Doherty Brian Shiro NOAA Lisa Baldwin DLR Domenico Giardini ETH Paul Lundgren JPL Mark Simons Caltech Don Banfield Cornell Lori Glaze GSFC Mioara Mandea GFZ Norman Sleep Stanford Amy Barr SwRI Matthew Golombek JPL Michael Manga John C. -
Habitability Models for Astrobiology
Astrobiology, 21, 8. (August, 2021) DOI: 10.1089/ast.2020.2342 Habitability Models for Astrobiology Abel Méndez, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Edgard G. Rivera-Valentín, Lunar and Planetary Institute, USRA, Houston, Texas, USA Dirk Schulze-Makuch, Center for Astronomy and Astrophysics, Technische Universität Berlin, Berlin, Germany; German Research Centre for Geosciences, Section Geomicrobiology, Potsdam, Germany; Leibniz-Institute of Freshwater Ecology and Inland Fisheries, Stechlin, Germany. Justin Filiberto, Lunar and Planetary Institute, USRA, Houston, Texas, USA Ramses M. Ramírez, University of Central Florida, Department of Physics, Orlando, Florida, USA; Space Science Institute, Boulder, Colorado, USA. Tana E. Wood, USDA Forest Service International Institute of Tropical Forestry, San Juan, Puerto Rico, USA Alfonso Dávila, NASA Ames Research Center, Moffett Field, California, USA Chris McKay, NASA Ames Research Center, Moffett Field, California, USA Kevin N. Ortiz Ceballos, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Marcos Jusino-Maldonado, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Nicole J. Torres-Santiago, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Guillermo Nery, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA René Heller, Max Planck Institute for Solar System Research; Institute for Astrophysics, -
Valles Marineris Landslides: Evidence for a Strength Limit to Martian Relief? ⁎ Florence Bigot-Cormier , David R
Earth and Planetary Science Letters 260 (2007) 179–186 www.elsevier.com/locate/epsl Valles Marineris landslides: Evidence for a strength limit to Martian relief? ⁎ Florence Bigot-Cormier , David R. Montgomery Quaternary Research Center and Department of Earth & Space Sciences, University of Washington, Seattle, WA 098195, United States Received 16 March 2007; received in revised form 11 May 2007; accepted 19 May 2007 Available online 26 May 2007 Editor: T. Spohn Abstract Unresolved controversies in Martian geology surround the role of active tectonics and a wetter climate early in Mars history, and particularly the history and amount of liquid water at or near the surface. Among the various lines of evidence brought into such debates are the massive landslides along the walls of Valles Marineris, which generally have been interpreted as resulting from marsquakes, and therefore necessitating active tectonics, under either wet or dry conditions. We analyze Valles Marineris landslides using digital elevation data from the Mars Orbiter Laser Altimeter (MOLA) and find that a relief limit consistent with the intact strength of evaporites or other weak sedimentary rock defines an upper bound to the length and relief of unfailed slopes, as would material with the strength properties of basalt lithology subjected to ground accelerations of about 0.2 g. In contrast to prior interpretations of Valles Marineris landslides, we propose an alternative, complementary hypothesis that does not require significant pore-water pressures or ground acceleration based on the close correspondence between back-calculated material strength properties and values consistent with portions of the chasm walls at least locally being composed of relatively weak materials, such as potentially frozen evaporites and/or mixtures of ash fall or flow deposits, ice, hydrated salts and lava flows. -
Waiting for O2
Downloaded from specialpapers.gsapubs.org on May 11, 2015 The Geological Society of America Special Paper 504 2014 Waiting for O2 Kevin Zahnle* Space Science Division, National Aeronautics and Space Administration Ames Research Center, MS 245-3, Moffett Field, California 94035, USA David Catling Department of Earth and Space Sciences/Astrobiology Program, University of Washington, Seattle, Washington 98195, USA ABSTRACT Oxygenic photosynthesis appears to be necessary for an oxygen-rich atmosphere like Earth’s. However, available geological and geochemical evidence suggests that at least 200 m.y., and possibly as many as 700 m.y., elapsed between the advent of oxygenic photosynthesis and the establishment of an oxygen atmosphere. The inter- regnum implies that at least one other necessary condition for O2 needed to be met. Here, we argue that the second condition was the oxidation of the surface and crust to the point where free O2 became more stable than competing reduced gases such as CH4, and that the cause of Earth’s surface oxidation was the same cause as it is for other planets with oxidized surfaces: hydrogen escape to space. The duration of the interregnum was determined by the rate of hydrogen escape and by the size of the reduced reservoir that needed to be oxidized before O2 became favored. We speculate that hydrogen escape determined the history of continental growth, and we are confi - dent that hydrogen escape provided a progressive bias to biological evolution. INTRODUCTION atmosphere, a state that is more widespread in the solar system. Oxygen and oxidation are different things and refl ect different This volume addresses Earth from its beginnings in the processes acting on different time scales, although it is plausible Hadean ca. -
BRUCE M. JAKOSKY Laboratory for Atmospheric and Space Physics
BRUCE M. JAKOSKY Laboratory for Atmospheric and Space Physics Department of Geological Sciences 3665 Discovery Dr. Campus Box 399 University of Colorado University of Colorado Boulder, CO 80303 Boulder, CO 80309-0399 Telephone: 303-492-8004 Fax: 303-492-6444 email: [email protected] EDUCATION: B.S., 1977, University of California at Los Angeles M.S., 1980, California Institute of Technology Ph.D., 1982, California Institute of Technology (in Planetary Science and Geophysics; Dissertation: The Seasonal Behavior of Water Vapor in the Mars Atmosphere) POSITIONS HELD: Associate Director for Science, Laboratory for Atmospheric and Space Physics, University of Colorado (2005 - present) Director, Center for Astrobiology, University of Colorado (1998 - 2012) Professor of Geology, Department of Geological Sciences, University of Colorado (1999- present; Associate Professor, 1992-1999; Assistant Professor, 1988-1992) Faculty Research Associate, Laboratory for Atmospheric and Space Physics, University of Colorado (1988-present; Research Associate 1982-1988) Lecturer, Dept. of Astrophysical, Planetary, and Atmospheric Sciences, University of Colorado (1983-1988) PROFESSIONAL ACTIVITIES: Spacecraft Participation: Emirates Mars Mission, Co-Investigator Mars Atmosphere and Volatile Evolution Mission (MAVEN), Principal Investigator Lunar Reconnaissance Orbiter, DIVINER investigation, Co-Investigator Mars Science Laboratory, Sample Analysis at Mars investigation, Co-Investigator Mars Odyssey, Thermal Emission Imaging System, Co-Investigator -
Habitability Models for Planetary Sciences
White Paper for the Planetary Science and Astrobiology Decadal Survey 2023–2032 (July 14, 2020) Habitability Models for Planetary Sciences Abel Méndez, ([email protected]) Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, USA 1 2 1 3 4 Edgard G. Rivera-Valentín , Dirk Schulze-Makuch , Justin Filiberto , Ramses Ramírez , Tana E. Wood , Alfonso 5 5 6 6 6 7 8 Dávila , Chris McKay , Kevin Ortiz Ceballos , Marcos Jusino-Maldonado , Guillermo Nery , René Heller , Paul Byrne , 9 10 11 11 12 Michael J. Malaska , Erica Nathan , Marta Filipa Simões , André Antunes , Jesús Martínez-Frías , Ludmila 13 14 15 16 17 Carone , Noam R. Izenberg , Dimitra Atri , Humberto Itic Carvajal Chitty , Priscilla Nowajewski-Barra , Frances 18 19 1 20 21 22 Rivera-Hernández , Corine Brown , Kennda Lynch , David Catling , Jorge I. Zuluaga , Juan F. Salazar , Howard 23 4 24 25 26 27 Chen , Grizelle González , Madhu Kashyap Jagadeesh , Rory Barnes , Charles S. Cockell , Jacob Haqq-Misra 1 2 3 4 L unar and Planetary Institute, USRA, USA; T echnical University Berlin, Germany; E arth-Life Science Institute, Japan; I nternational Institute of 5 6 Tropical Forestry, USDA Forest Service, Puerto Rico, USA; N ASA Ames Research Center, USA; P lanetary Habitability Laboratory, University of 7 8 9 Puerto Rico at Arecibo, Puerto Rico, USA; M ax Planck Institute for Solar System Research, Germany, N orth Carolina State University, USA;