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Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
Recurring Slope Lineae: Evidence of Liquid Water on Mars Today?
Recurring Slope Lineae: Evidence of liquid water on Mars today? The High Resolution Imaging Science Experiment (HiRISE) on Mars Reconnaissance Orbiter (MRO) has monitored surface feature changes over several Mars years. One of the more intriguing observations has been of the seasonal occurrence of numerous (multi-thousand) dark streak features advancing down equator-facing slopes in several mid-latitude and equatorial regions of the southern hemisphere. Termed Recurring Slope Lineae (RSL), the streak behavior resembles that of a fluid mobilized by increasing surface temperatures – initiating in spring, incrementally extending downslope through summer, and then fading in the fall and winter seasons. The phenomenon is then seen to repeat the following spring. RSLs are narrow in width (meter-scale), requiring our best resolution imaging to see them, but may extend down-slope for hundreds of meters before terminating. Science teams involved in the discovery of RSL have been cautious in concluding a water-based origin since most of the RSL locations are found in environments well outside the pressure-temperature stability field for liquid water. However, the presence of salts such as perchlorate can depress freezing points by tens of degrees. MRO Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) observations of multiple RSL locations show hydrated mineral absorption signals most consistent with magnesium perchlorate, magnesium chlorate and sodium perchlorate. That raises the possibility of a Mg-, Na-, Cl-rich brine that would also leave these minerals as a kind of evaporite deposit. However, the amount of water, if present, has been constrained at one location by independent Thermal Emission Imaging System (THEMIS; Mars Odyssey) data analysis and a numerical heat transfer model to 0 wt.%, and up to 3 wt.% given observational uncertainties, unlikely to support a sustained flow. -
Optical Timeline by Tony Oursler
Optical Timeline by Tony Oursler 1 Iris is thought to be derived from the RED Symyaz leads the fallen angels. Archimedes (c. 287212 b.c.) is said to Greek word for speaker or messenger. According to Enoch, they came to earth have used a large magnifying lens or Seth, the Egyptian god most associated of their own free will at Mount Hermon, burning-glass, which focused the suns Fifth century b.c. Chinese philosopher with evil, is depicted in many guises: descending like stars. This description rays, to set fire to Roman ships off Mo Ti, in the first description of the gives rise to the name Lucifer, “giver of Syracuse. camera obscura, refers to the pinhole as a black pig, a tall, double-headed figure light.” “collection place” and “locked treasure with a snout, and a serpent. Sometimes And now there is no longer any “I have seen Satan fall like lightning room.” he is black, a positive color for the difficulty in understanding the images in from heaven.” (Luke 10:1820) Egyptians, symbolic of the deep tones of mirrors and in all smooth and bright Platos Cave depicts the dilemma of fertile river deposits; at other times he is surfaces. The fires from within and from the uneducated in a graphic tableau of red, a negative color reflected by the without communicate about the smooth light and shadow. The shackled masses parched sands that encroach upon the surface, and from one image which is are kept in shadow, unable to move crops. Jeffrey Burton Russell suggests variously refracted. -
How Doc Draper Became the Father of Inertial Guidance
(Preprint) AAS 18-121 HOW DOC DRAPER BECAME THE FATHER OF INERTIAL GUIDANCE Philip D. Hattis* With Missouri roots, a Stanford Psychology degree, and a variety of MIT de- grees, Charles Stark “Doc” Draper formulated the basis for reliable and accurate gyro-based sensing technology that enabled the first and many subsequent iner- tial navigation systems. Working with colleagues and students, he created an Instrumentation Laboratory that developed bombsights that changed the balance of World War II in the Pacific. His engineering teams then went on to develop ever smaller and more accurate inertial navigation for aircraft, submarines, stra- tegic missiles, and spaceflight. The resulting inertial navigation systems enable national security, took humans to the Moon, and continue to find new applica- tions. This paper discusses the history of Draper’s path to becoming known as the “Father of Inertial Guidance.” FROM DRAPER’S MISSOURI ROOTS TO MIT ENGINEERING Charles Stark Draper was born in 1901 in Windsor Missouri. His father was a dentist and his mother (nee Stark) was a school teacher. The Stark family developed the Stark apple that was popular in the Midwest and raised the family to prominence1 including a cousin, Lloyd Stark, who became governor of Missouri in 1937. Draper was known to his family and friends as Stark (Figure 1), and later in life was known by colleagues as Doc. During his teenage years, Draper enjoyed tinkering with automobiles. He also worked as an electric linesman (Figure 2), and at age 15 began a liberal arts education at the University of Mis- souri in Rolla. -
Tentative Lists Submitted by States Parties As of 15 April 2021, in Conformity with the Operational Guidelines
World Heritage 44 COM WHC/21/44.COM/8A Paris, 4 June 2021 Original: English UNITED NATIONS EDUCATIONAL, SCIENTIFIC AND CULTURAL ORGANIZATION CONVENTION CONCERNING THE PROTECTION OF THE WORLD CULTURAL AND NATURAL HERITAGE WORLD HERITAGE COMMITTEE Extended forty-fourth session Fuzhou (China) / Online meeting 16 – 31 July 2021 Item 8 of the Provisional Agenda: Establishment of the World Heritage List and of the List of World Heritage in Danger 8A. Tentative Lists submitted by States Parties as of 15 April 2021, in conformity with the Operational Guidelines SUMMARY This document presents the Tentative Lists of all States Parties submitted in conformity with the Operational Guidelines as of 15 April 2021. • Annex 1 presents a full list of States Parties indicating the date of the most recent Tentative List submission. • Annex 2 presents new Tentative Lists (or additions to Tentative Lists) submitted by States Parties since 16 April 2019. • Annex 3 presents a list of all sites included in the Tentative Lists of the States Parties to the Convention, in alphabetical order. Draft Decision: 44 COM 8A, see point II I. EXAMINATION OF TENTATIVE LISTS 1. The World Heritage Convention provides that each State Party to the Convention shall submit to the World Heritage Committee an inventory of the cultural and natural sites situated within its territory, which it considers suitable for inscription on the World Heritage List, and which it intends to nominate during the following five to ten years. Over the years, the Committee has repeatedly confirmed the importance of these Lists, also known as Tentative Lists, for planning purposes, comparative analyses of nominations and for facilitating the undertaking of global and thematic studies. -
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 .......................................................................................................................... -
IN-SITU RADIOMETRIC AGE DETERMINATION: a CRITICAL COMPONENT of MARS EXPLORATION. J. B. Plescia1 and T. D. Swindle2, 1Applied
Seventh International Conference on Mars 3278.pdf IN-SITU RADIOMETRIC AGE DETERMINATION: A CRITICAL COMPONENT OF MARS EXPLORATION. J. B. Plescia1 and T. D. Swindle2, 1Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723, [email protected]. 2Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, [email protected]. Introduction: In order to understand the geologic, Bombardment [12-18], although this remains a contro- climatic and possibly the biologic evolution of Mars, versial topic. It has also been suggested that the crater- the absolute timing of events must be established. ing rate over the last several billion years has not been Questions of climate change, glacial processes, avail- uniform, but rather has been punctuated by periodic ability of surface water, recent volcanism, and atmos- spikes in the rate [19-20]. pheric evolution all hinge on determining when those events occurred in absolute time. Resolving the abso- lute timing of events has become even more critical with the suggestions of currently active glacial and perhaps fluvial activity and very young volcanic activ- ity. Background: To date, only the relative chronology of events has been firmly established [1]. This has been accomplished through the use of impact crater counts in which the frequency of impact craters per unit area greater than or equal to some diameter is used as a reference for comparison among surfaces; the higher the frequency, the older the age [2-3]. This technique allows surfaces and events on different parts of a planet to be correlated in time. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
NITROGEN on MARS: INSIGHTS from CURIOSITY. J. C. Stern1 , B. Sutter2, W. A. Jackson3, Rafael Na- Varro-González4, Christopher P
Lunar and Planetary Science XLVIII (2017) 2726.pdf 1 2 3 NITROGEN ON MARS: INSIGHTS FROM CURIOSITY. J. C. Stern , B. Sutter , W. A. Jackson , Rafael Na- varro-González4, Christopher P. McKay5, Douglas W. Ming6, P. Douglas Archer2, D. P. Glavin1, A. G. Fairen7,8 and Paul R. Mahaffy1. 1NASA GSFC, Code 699, Greenbelt, MD 20771, [email protected], 2Jacobs, NASA Johnson Space Center, Houston, TX 77058, 3Texas Tech University, Lubbock, TX 79409, 4Universidad Nacional Autónoma de México, México, D.F. 04510, Mexico, 5NASA Ames Research Center, Moffett Field, CA 94035, 6NASA Johnson Space Center, Houston TX 77058, 7Centro de Astrobiologia, Madrid, Spain, 8Cornell University, Ithaca, NY 14853 Introduction: Recent detection of nitrate on Mars [1] indicates that nitrogen fixation processes occurred in early martian history. Data collected by the Sample Analysis at Mars (SAM) instrument on the Curiosity Rover can be integrated with Mars analog work in order to better understand the fixation and mobility of nitrogen on Mars, and thus its availability to putative biology. In particular, the relationship between nitrate and other soluble salts may help reveal the timing of nitrogen fixation and post-depositional behavior of nitrate on Mars. In addition, in situ measurements of nitrogen abundance and isotopic composition may be used to model atmospheric conditions on early Mars. Methods: The data presented are from analyses of solid Martian drilled and scooped samples by the Sam- ple Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity Rover. SAM performs evolved gas analysis (EGA), in which a 3 Figure 1. -
Fe,Mg)S, the IRON-DOMINANT ANALOGUE of NININGERITE
1687 The Canadian Mineralogist Vol. 40, pp. 1687-1692 (2002) THE NEW MINERAL SPECIES KEILITE, (Fe,Mg)S, THE IRON-DOMINANT ANALOGUE OF NININGERITE MASAAKI SHIMIZU§ Department of Earth Sciences, Faculty of Science, Toyama University, 3190 Gofuku, Toyama 930-8555, Japan § HIDETO YOSHIDA Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan § JOSEPH A. MANDARINO 94 Moore Avenue, Toronto, Ontario M4T 1V3, and Earth Sciences Division, Royal Ontario Museum, 100 Queens’s Park, Toronto, Ontario M5S 2C6, Canada ABSTRACT Keilite, (Fe,Mg)S, is a new mineral species that occurs in several meteorites. The original description of niningerite by Keil & Snetsinger (1967) gave chemical analytical data for “niningerite” in six enstatite chondrites. In three of those six meteorites, namely Abee and Adhi-Kot type EH4 and Saint-Sauveur type EH5, the atomic ratio Fe:Mg has Fe > Mg. Thus this mineral actually represents the iron-dominant analogue of niningerite. By analogy with synthetic MgS and niningerite, keilite is cubic, with space group Fm3m, a 5.20 Å, V 140.6 Å3, Z = 4. Keilite and niningerite occur as grains up to several hundred m across. Because of the small grain-size, most of the usual physical properties could not be determined. Keilite is metallic and opaque; in reflected light, it is isotropic and gray. Point-count analyses of samples of the three meteorites by Keil (1968) gave the following amounts of keilite (in vol.%): Abee 11.2, Adhi-Kot 0.95 and Saint-Sauveur 3.4. -
Thermodynamics of DNA Binding by DNA Polymerase I and Reca
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 2014 Thermodynamics of DNA Binding by DNA Polymerase I and RecA Recombinase from Deinococcus radiodurans Jaycob Dalton Warfel Louisiana State University and Agricultural and Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Recommended Citation Warfel, Jaycob Dalton, "Thermodynamics of DNA Binding by DNA Polymerase I and RecA Recombinase from Deinococcus radiodurans" (2014). LSU Doctoral Dissertations. 2382. https://digitalcommons.lsu.edu/gradschool_dissertations/2382 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. THERMODYNAMICS OF DNA BINDING BY DNA POLYMERASE I AND RECA RECOMBINASE FROM DEINOCOCCUS RADIODURANS A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Biological Sciences by Jaycob Dalton Warfel B.S. Louisiana State University, 2006 May 2015 ACKNOWLEDGEMENTS I would like to express my utmost gratitude to the myriad of individuals who have lent their support during the time it has taken to complete this dissertation. First and foremost is due glory to God, The Father, The Son and The Holy Spirit, through whom all is accomplished. It is with extreme thankfulness for the blessings bestowed upon me, and with vast appreciation for the beauty of God’s creation that I have pursued a scientific education. -
Widespread Excess Ice in Arcadia Planitia, Mars
Widespread Excess Ice in Arcadia Planitia, Mars Ali M. Bramson1, Shane Byrne1, Nathaniel E. Putzig2, Sarah Sutton1, Jeffrey J. Plaut3, T. Charles Brothers4 and John W. Holt4 Corresponding author: A. M. Bramson, Lunar and Planetary Laboratory, University of Arizona, Kuiper Space Science Building, 1629 E. University Blvd. Tucson, AZ, 85721, USA. ([email protected]) Affiliations: 1Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA. 2Southwest Research Institute, Boulder, Colorado, USA. 3Jet Propulsion Laboratory, Pasadena, California, USA. 4Institute for Geophysics, University of Texas at Austin, Austin, Texas, USA. Accepted for publication July 18, 2015 in Geophysical Research Letters. An edited version of this paper was published by AGU on August 26, 2015. Copyright 2015 American Geophysical Union. Citation: Bramson, A. M., S. Byrne, N. E. Putzig, S. Sutton, J. J. Plaut, T. C. Brothers, and J. W. Holt (2015), Widespread excess ice in Arcadia Planitia, Mars, Geophys. Res. Lett., 42, doi:10.1002/2015GL064844. Key points: • Terraced craters: abundant in Arcadia Planitia, indicate subsurface layering • A widespread subsurface interface is also detected by SHARAD • Combining data sets yields dielectric constants consistent with decameters of excess water ice Abstract: The distribution of subsurface water ice on Mars is a key constraint on past climate, while the volumetric concentration of buried ice (pore-filling versus excess) provides information about the process that led to its deposition. We investigate the subsurface of Arcadia Planitia by measuring the depth of terraces in simple impact craters and mapping a widespread subsurface reflection in radar sounding data. Assuming that the contrast in material strengths responsible for the terracing is the same dielectric interface that causes the radar reflection, we can combine these data to estimate the dielectric constant of the overlying material.