Companion Q&A Fact Sheet: What Mars Reveals About Life in Our
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Review of the MEPAG Report on Mars Special Regions
THE NATIONAL ACADEMIES PRESS This PDF is available at http://nap.edu/21816 SHARE Review of the MEPAG Report on Mars Special Regions DETAILS 80 pages | 8.5 x 11 | PAPERBACK ISBN 978-0-309-37904-5 | DOI 10.17226/21816 CONTRIBUTORS GET THIS BOOK Committee to Review the MEPAG Report on Mars Special Regions; Space Studies Board; Division on Engineering and Physical Sciences; National Academies of Sciences, Engineering, and Medicine; European Space Sciences Committee; FIND RELATED TITLES European Science Foundation Visit the National Academies Press at NAP.edu and login or register to get: – Access to free PDF downloads of thousands of scientific reports – 10% off the price of print titles – Email or social media notifications of new titles related to your interests – Special offers and discounts Distribution, posting, or copying of this PDF is strictly prohibited without written permission of the National Academies Press. (Request Permission) Unless otherwise indicated, all materials in this PDF are copyrighted by the National Academy of Sciences. Copyright © National Academy of Sciences. All rights reserved. Review of the MEPAG Report on Mars Special Regions Committee to Review the MEPAG Report on Mars Special Regions Space Studies Board Division on Engineering and Physical Sciences European Space Sciences Committee European Science Foundation Strasbourg, France Copyright National Academy of Sciences. All rights reserved. Review of the MEPAG Report on Mars Special Regions THE NATIONAL ACADEMIES PRESS 500 Fifth Street, NW Washington, DC 20001 This study is based on work supported by the Contract NNH11CD57B between the National Academy of Sciences and the National Aeronautics and Space Administration and work supported by the Contract RFP/IPL-PTM/PA/fg/306.2014 between the European Science Foundation and the European Space Agency. -
PUTTING LIFE on MARS: Using Computer Graphics to Render a Living Mars
InSight: RIVIER ACADEMIC JOURNAL, VOLUME 9, NUMBER 1, SPRING 2013 PUTTING LIFE ON MARS: Using Computer Graphics to Render a Living Mars Kevin M. Gill ‘11G* Senior Software Engineer, Thunderhead.com, Manchester, NH Keywords: Computer Graphics, Mars, Life, Planetary Science, OpenGL Abstract This article describes the software, algorithms & decisions that went into the development of the Living Mars image project. This includes topics related to computer graphics, software development, astronomy, & planetary science. The purpose of the project was to create a visualization of the planet Mars as could look with a living biosphere. This makes no distinction as to whether this biosphere would represent an ancient or future, possibly terraformed planet. 1 Background Mars, named for the Roman god of war. Ancient civilizations have forever associated the planet with fear, war, and destruction. It is the color of blood, and “one of a handful of planets visible to the naked eye, and the only one of marked color, so the planet demanded attention (Pyle, 2012).” Ever since man has noticed it, there have been dreams and visions of life on Mars, from Giovanni Schiaparelli and Percival Lowell describing channels and canals to Robert A. Heinlein’s science fiction. Lowell, in particular famous for fantastic writings of Mars, asked “are physical forces alone at work there, or has evolution begotten something more complex, something not unakin to what we know on Earth as life?” (Lowell, 1895) Even more recent discoveries by NASA’s Curiosity rover have found proof that liquid water once flowed billions of years ago positing an environment that could have served host to life (Brown, 2013). -
Prospects for Life on Mars Without Doubt, Mars Is the Planet That Has Inspired the Most Speculation About Life Outside Earth. It
Prospects for Life on Mars Without doubt, Mars is the planet that has inspired the most speculation about life outside Earth. It has also starred in more science fiction stories than all other non-Earth planets put together. In this lecture we will have some fun exploring the history of these notions, as well as the entirely serious pursuit of life on Mars that is an ongoing focus of NASA. Lowell and the canals Fascination with Mars has probably occurred since the dawn of humans. Its bright red aspect draws attention, and it is probably no accident that multiple civilizations identified it with the god of war. We take our tradition in this respect from the Romans. Mars, the fourth planet from the Sun, is the second smallest of the terrestrial planets. It has about 1/10 of the mass of the Earth and 1/3 of Earth’s surface gravity, with the consequence that it has difficulty holding onto gases and thus has an atmosphere with only about 1% of the density of Earth’s. The atmosphere itself is mostly carbon dioxide; the oxygen that was in the atmosphere has combined with the iron in the crust to make rust, which is why the planet is red. Mars has no detectable magnetic field, which suggests to some people that it is solid throughout: for comparison, the Earth’s molten interior combined with its rotation (which is similar to that of Mars) generates our magnetic field. Nonetheless, Mars has some spectacular surface features including the largest volcano in the Solar System, Olympus Mons, which rises an amazing 25 km above the surface and is 600 km wide at its base. -
Magnetite Biomineralization and Ancient Life on Mars Richard B Frankel* and Peter R Buseckt
Magnetite biomineralization and ancient life on Mars Richard B Frankel* and Peter R Buseckt Certain chemical and mineral features of the Martian meteorite with a mass distribution unlike terrestrial PAHs or those from ALH84001 were reported in 1996 to be probable evidence of other meteorites; thirdly, bacterium-shaped objects (BSOs) ancient life on Mars. In spite of new observations and up to several hundred nanometers long that resemble fos interpretations, the question of ancient life on Mars remains silized terrestrial microorganisms; and lastly, 10-100 nm unresolved. Putative biogenic, nanometer magnetite has now magnetite (Fe304), pyrrhotite (Fel_xS), and greigite (Fe3S4) become a leading focus in the debate. crystals. These minerals were cited as evidence because of their similarity to biogenic magnetic minerals in terrestrial Addresses magnetotactic bacteria. *Department of Physics, California Polytechnic State University, San Luis Obispo, California 93407, USA; e-mail: [email protected] The ancient life on Mars hypothesis has been extensively tDepartments of Geology and Chemistry/Biochemistry, Arizona State challenged, and alternative non-biological processes have University, Tempe, Arizona 85287-1404, USA; e-mail: [email protected] been proposed for each of the four features cited by McKay et al. [4]. In this paper we review the current situa tion regarding their proposed evidence, focusing on the Abbreviations putative biogenic magnetite crystals. BCM biologically controlled mineralization BIM biologically induced mineralization BSO bacterium-shaped object Evidence for and against ancient Martian life PAH polycyclic aromatic hydrocarbon PAHs and BSOs Reports of contamination by terrestrial organic materials [5°,6°] and the similarity of ALH84001 PAHs to non-bio genic PAHs in carbonaceous chondrites [7,8] make it Introduction difficult to positively identify PAHs of non-terrestrial, bio A 2 kg carbonaceous stony meteorite, designated genic origin. -
Physical Changes
How Matter Changes By Cindy Grigg Changes in matter happen around you every day. Some changes make matter look different. Other changes make one kind of matter become another kind of matter. When you scrunch a sheet of paper up into a ball, it is still paper. It only changed shape. You can cut a large, rectangular piece of paper into many small triangles. It changed shape and size, but it is still paper. These kinds of changes are called physical changes. Physical changes are changes in the way matter looks. Changes in size and shape, like the changes in the cut pieces of paper, are physical changes. Physical changes are changes in the size, shape, state, or appearance of matter. Another kind of physical change happens when matter changes from one state to another state. When water freezes and makes ice, it is still water. It has only changed its state of matter from a liquid to a solid. It has changed its appearance and shape, but it is still water. You can change the ice back into water by letting it melt. Matter looks different when it changes states, but it stays the same kind of matter. Solids like ice can change into liquids. Heat speeds up the moving particles in ice. The particles move apart. Heat melts ice and changes it to liquid water. Metals can be changed from a solid to a liquid state also. Metals must be heated to a high temperature to melt. Melting is changing from a solid state to a liquid state. -
Evolution of Mars As a Planet, Possible Life on Mars
EVOLUTION OF MARS LECTURE 18 NEEP 533 HARRISON H. SCHMITT NASA HST IMAGE N THARSIS HELLAS S ANDESITE OR WEATHERED SOIL DUST DUST DUST BASALT ~100 KM A C B THEMIS THERMAL IMAGING OF SPIRIT LANDING AREA IN GUSEV CRATER A. SPIRIT LANDING ELLIPSE B. CLOSER VIEW OF SPIRIT LANDING ELLIPSE C. NIGHT IR IMAGE: BRIGHT AREAS ARE MORE ROCKY. ARROW POINTS TO ROCKY SLOPE SPIRIT MOVED TO GUSEV CRATER POSSIBLE LAKE BED IN LARGE BASIN A C B THEMIS THERMAL IMAGING OF OPPORTUNITYLANDING AREA IN MERIDIANI PLANUM A. LANDING ELLIPSE ~120 KM LONG) B. CLOSER VIEW OF LANDING ELLIPSE C. NIGHT IR IMAGE: BRIGHT AREAS ARE MORE ROCKY. ARROW POINTS TO ROCKY SLOPE MAJOR STAGES OF MARS’ EVOLUTION 1 BEGINNING 2 MAGMA OCEAN / CONVECTIVE OVERTURN 3A ? ? CRATERED UPLANDS / VERY LARGE BASINS 3B ? CORE FORMATION/GLOBAL MAGNETIC FIELD 3C 4.5 - 1.3 GLOBAL MAFIC VOLCANISM DENSE WATER / CO2 ATMOSPHERE E ? G 3D EROSION / LAKES / NORTHERN OCEAN A T ? ? S 4 LARGE BASINS CATACLYSM ? THARSIS UPLIFT AND VOLCANISM ? 5 NORTHERN HEMISPHERE BASALTIC / ANDESITIC VOLCANISM ? 1.3 - 0.2 SUBSURFACE HYDROSPHERE / CRYOSPHERE 6 ? PRESENT SURFACE CONDITIONS LUNAR 4.6 4.2? 3.8 ? 5.0 4.0 3.0 2.0 1.0 BILLIONS OF YEARS BEFORE PRESENT ITALICS = SNC DATES RED = MAJOR UNCERTAINTY OLYMPUS TOPOGRAPHY OF MONS THARSIS REGION VALLES MARINERIS THARSIS REGION SHADED RELIEF DETAIL MARS GLOBAL SURVEYOR MOLA OLYMPUS MONS VALLES MARINERIS APOLLO MODEL OF MARS EVOLUTION ELYSIUM MONS ANDESITIC THARSIS EVENTS EXTRUSIONS <3.8 B.Y. THARSIS THICKENING ATMOSPHERE: MAFIC UPPER MANTLE WITH CO2, H20 CRYOSPHERE / INCREASING HYDROSPHERE SI AND FE UPWARDS OLIVINE/ NA- PYROXENE ? ANDESITIC CUMULATE INTRUSIONS? OLIVINE ? CUMULATE RELIC PROTO- GARNET / NA-CPX/ CORE ? NA-BIOTITE?/NA- HORNBLENDE/ ? FExNIySz “RUTILE” (TRANSITION? CORE CUMULATES ? ZONE) RELIC MAGNETIC STRIPING THICKENED SOUTHERN ©Harrison H. -
Cosmic Microwave Background
1 29. Cosmic Microwave Background 29. Cosmic Microwave Background Revised August 2019 by D. Scott (U. of British Columbia) and G.F. Smoot (HKUST; Paris U.; UC Berkeley; LBNL). 29.1 Introduction The energy content in electromagnetic radiation from beyond our Galaxy is dominated by the cosmic microwave background (CMB), discovered in 1965 [1]. The spectrum of the CMB is well described by a blackbody function with T = 2.7255 K. This spectral form is a main supporting pillar of the hot Big Bang model for the Universe. The lack of any observed deviations from a 7 blackbody spectrum constrains physical processes over cosmic history at redshifts z ∼< 10 (see earlier versions of this review). Currently the key CMB observable is the angular variation in temperature (or intensity) corre- lations, and to a growing extent polarization [2–4]. Since the first detection of these anisotropies by the Cosmic Background Explorer (COBE) satellite [5], there has been intense activity to map the sky at increasing levels of sensitivity and angular resolution by ground-based and balloon-borne measurements. These were joined in 2003 by the first results from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP)[6], which were improved upon by analyses of data added every 2 years, culminating in the 9-year results [7]. In 2013 we had the first results [8] from the third generation CMB satellite, ESA’s Planck mission [9,10], which were enhanced by results from the 2015 Planck data release [11, 12], and then the final 2018 Planck data release [13, 14]. Additionally, CMB an- isotropies have been extended to smaller angular scales by ground-based experiments, particularly the Atacama Cosmology Telescope (ACT) [15] and the South Pole Telescope (SPT) [16]. -
Life on Mars- Extracting the Signs for Future Human Habitation on The
Muhammad Shadab Khan, Department of Aeronautical Engineering, Babu Banarasi Das National Institute of Technology and Management, Lucknow, India CONTENT- Introduction Life on Mars Signs of Life Found on Mars and Similarities with those signs on Earth Utilizing Life Support Resources present on Mars for human habitation INTRODUCTION 1- Rise of Global Warming and it’s alarming consequences which might cause complete loss of life on Earth– Search for an Earth like habitable body in the outer Space 2- Ongoing Exploration of Mars in search of Life on the Red Planet for future human habitation on the planet. 3- Mars is the planet which is very similar to Earth and it’s believed that Life had existed on Mars in the Past– Big support to our quest for life in the future 4- The life supporting features found on Mars are very similar to those found on Earth– Giving a sign of prospective life in the near future on Mars Life on Mars Life on Mars has been a subject of wide discussion from the very early beginning. There has been speculations about the existence of Life on the Red Planet in the Past But still about the presence of an Earth like habitable environment on Mars is a BIG QUESTION ? The first search for Life on Mars was carried out by NASA’s VIKING LANDER in 1976 Gas Chromatograph/Mass Spectrometer Instrument on the Lander detected the possible MICROBIAL LIFE in the soil sample . The question about MICROBIAL LIFE remains unresolved LIQUID WATER ON MARS The speculation about the presence of LIQUID WATER on Mars has been a subject of deep interest to the scientists from the very beginning As it’s believed in order to support LIFE, the need of WATER in LIQUID FORM is MUST. -
Comment on Liquid Water and Life on Mars
obiolog str y & f A O u o l t a r e n Chandra Wickramasinghe, Astrobiol Outreach 2015, 3:5 a r c u h o J Journal of Astrobiology & Outreach DOI: 10.4172/2332-2519.1000e111 ISSN: 2332-2519 Editorial Open Access Comment on Liquid Water and Life on Mars Chandra Wickramasinghe N*,1,2,3 1Buckingham Centre for Astrobiology (BCAB), Buckingham University, UK 2Institute for the Study of Panspermia and Astroeconomics, Gifu, Japan 3University of Peradeniya, Peradeniya, Sri Lanka *Corresponding author: Wickramasinghe NC, Buckingham Centre for Astrobiology (BCAB), Buckingham University, UK, Tel: +44-777-838-9243; E-mail: [email protected] Rec date: October 01, 2015; Acc date: October 05, 2015; Pub date: October 07, 2015 Copyright: © 2015 Chandra Wickramasinghe N, et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. Editorial but it was quickly rejected on grounds of alleged uncertainties of interpretation, as well as the lack of organic molecules detectable at the The announcement this week of the detection of liquid water on landing site. A year later, in1977, a major dust storm enveloped the Mars has come close on 4 decades after the arrival of the first Viking planet and H. Abadi and the present writer reported evidence of landers at the red planet in 1976 [1]. The temperatures at the two absorption properties of the Martian dust that was consistent with the original landing sites of the Viking spacecraft in 1976 ranged between a presence of aromatic hydrocarbons [3]. -
The Temperature of the Cosmic Microwave Background at 10 Ghz D
The Astrophysical Journal, 612:86–95, 2004 September 1 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE TEMPERATURE OF THE COSMIC MICROWAVE BACKGROUND AT 10 GHZ D. J. Fixsen,1 A. Kogut,2 S. Levin,3 M. Limon,1 P. Lubin,4 P. Mirel,1 M. Seiffert,3 and E. Wollack2 Received 2004 February 23; accepted 2004 April 14 ABSTRACT We report the results of an effort to measure the low-frequency portion of the spectrum of the cosmic microwave background (CMB) radiation, using a balloon-borne instrument called the Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE). These measurements are to search for deviations from a thermal spectrum that are expected to exist in the CMB as a result of various processes in the early universe. The radiometric temperature was measured at 10 and 30 GHz using a cryogenic open-aperture instrument with no emissive windows. An external blackbody calibrator provides an in situ reference. Systematic errors were greatly reduced by using differential radiometers and cooling all critical components to physical temperatures approxi- mating the antenna temperature of the sky. A linear model is used to compare the radiometer output to a set of thermometers on the instrument. The unmodeled residualsarelessthan50mKpeaktopeakwithaweightedrms of 6 mK. Small corrections are made for the residual emission from the flight train, atmosphere, and foreground Galactic emission. The measured radiometric temperature of the CMB is 2:721 Æ 0:010 K at 10 GHz and 2:694 Æ 0:032 K at 30 GHz. Subject headinggs: cosmic microwave background — cosmology: observations 1. -
Extreme Cold Is a Dangerous Situation That Can Bring on Bring Can That Situation Dangerous a Is Cold Extreme
Centers for Disease Control and Prevention and Control Disease for Centers U.S. Department of Health And Human Services Human And Health of Department U.S. U.S. Department of Health And Human Services Centers for Disease Control and Prevention http://www.bt.cdc.gov/disasters/winter/ 1-888-232-6789; [email protected] 1-888-232-6789; 4700 Buford Hwy, Atlanta, GA 30341-3717 GA Atlanta, Hwy, Buford 4700 National Center for Environmental Health, MS F52 MS Health, Environmental for Center National Centers for Disease Control and Prevention and Control Disease for Centers or more information on cold weather conditions and health, please contact: please health, and conditions weather cold on information more or F For more information on hot weather conditions and health, please contact: Centers for Disease Control and Prevention National Center for Environmental Health, MS F52 4700 Buford Hwy, Atlanta, GA 30341-3717 1-888-232-6789; [email protected] http://www.bt.cdc.gov/disasters/extremeheat/ 1 and what to do if a cold-weather health emergency arises. arises. emergency health cold-weather a if do to what and should know how to prevent cold-related health problems health cold-related prevent to how know should that is poorly insulated or without heat. without or insulated poorly is that can be affected. To keep yourself and your family safe, you safe, family your and yourself keep To affected. be can without shelter or who are stranded, or who live in a home a in live who or stranded, are who or shelter without Infants and the elderly are particularly at risk, but anyone but risk, at particularly are elderly the and Infants health emergencies in susceptible people, such as those as such people, susceptible in emergencies health can cause other serious or life-threatening health problems. -
Types of Martian Fan-Shaped Sedimentary Deposits
40th Lunar and Planetary Science Conference (2009) 1901.pdf TYPES OF MARTIAN FAN-SHAPED SEDIMENTARY DEPOSITS. G. de Villiers1, M. Kleinhans1, G. Postma1, E. Hauber2, S. de Jong1 and P.L. de Boer1. 1Faculty of Geosciences, Utrecht University, Utrecht, The Netherlands. g.devilliers(at)geo.uu.nl, 2Institute of Planetary Exploration, German Aerospace Centre (DLR), Berlin, Germany. Introduction: Deltas, fans and channels on Mars Elevation Maps (DEMs). Quantification of shapes, clearly indicate surface water in the past. These dimensions, volumes and DEM derivatives focuses on landforms contain valuable information about the the feeder valleys, the fan terraces and the fan lobes. duration and magnitude of surface-water flow, with We ascertain the lengths and gradients of channels (if obvious implications for potential life on Mars. present), bars, terraces, and lobes. In addition, we Martian fan-shaped deposits such as deltas and alluvial determine the diameter, depth, volume, and maximum fans show architectural elements similar to those of water levels of the crater basins within which most of terrestrial analogs, e.g. lobes, terraces, and incised these deposits are located. Preliminary analyses affirm delta fronts. Pilot experiments demonstrate that delta that the gradients or slopes decrease with increase in morphology is related to flow discharge and duration, fan size (both area and length, see Figure 1). However, sediment properties, and crater size [1]. However, the there is apparently very little relationship between fan important relationships between surface morphology gradient and basin size. Based on the geomorphic and climate remain unquantified and it is difficult to shapes alone, different types of fan-shaped deposits unambiguously relate the architecture of sediment can be distinguished and combined with differences in bodies to certain boundary conditions.