The Moon Map

Total Page:16

File Type:pdf, Size:1020Kb

The Moon Map The Moon map The image shows the side of the moon visible from Earth with its most prominent features: Mare Frigoris • = Mare (lat. seas) Platog fAristoteles Maria (plural) are large, dark areas on the Valley ine lunar surface. These are huge ancient impact lp A s craters which were filled by escaping lava Sinus s t Sinus iridum t during the primitive age of the moon. Today M M the moon has completely cooled down and Roris Mare Imbrium s f contains no more liquid layers. u Posidonius ▲ 15 s 17 a Lacus c 21 = Montes (lat. Mountains) u * • a Somniorum These are mountain ranges that were formed C * when the moon was still geologically active. s ▲ 17 The names are based on the names of the f t Mare Aristarchus M mountains of the earth (Alps, Appenin, ine Crisium Caucasus...). nn Ape Mare Vaporum 13 Mare 23 24 = Crater Copernicusg * Tranquillitatis * The• many craters on the surface of the * 20 moon originate for the most part from the g ▲ 11 Kepler Sinus Medii  1 formation time of the solar system. Since the * 16 9 moon has no atmosphere, these have never Sinus aestum  3 Py Mare* weathered and are still fully preserved. The * re  6 n Fecunditatis craters are marked with the names of famous Oceanus 14 ▲  7 e 12 Theophilus e astronomers and scientists according to ▲ s Procellarum 16 international agreement. ▲ i M Ptolemaeusg i t fGrimaldi f s • = Sinus (lat. bay) Albategnius Mare These are parts of Maria, partly also craters, Nectaris which overlap with the edges of Maria. Mare f f ▲ = Apollo Missions (USA) Gassendi Fracastorius These are the landing sites of the American Nubium Apollo missions of the 60s and 70s with the mission number. fPiccolomini  = Unmanned NASA probes (USA) These are the landing sites of the American Surveyor probes (60s) with the mission number fStofler f = Unmanned RAKA Probes Tycho Rheita Valley * fSchickard (former USSR) g These are the landing sites of the Soviet Luna Mare Australe probes (60s and 70s) with the mission number. fClavins Leibnitz Mts --HOLD--Poster_Moon-map-A2_en_BRESSER_v022021a.indd 1 18.03.2021 08:40:27.
Recommended publications
  • Location #1: Peary/Whipple Crater
    Location, Location, Location A Lunar Investment Strategy Hoyt Davidson Near Earth LLC June 2017 ISU's International Institute of Space Commerce Lunar Economic Action Plan (LEAP) Space and Questions from 1960 Still Relevant Today Economic Development • How can we utilize our dynamic system of competitive private enterprise in space, as on earth, to make newly discovered resources useful to man? • How can private enterprise and private capital make their maximum contribution? Philosophy and Policy The ultimate goal is not to impress others, or merely to explore our planetary system, but to use accessible space for the benefit of humankind. It is a goal that is not confined to a decade or a century. Nor is it confined to a single nearby destination, or to a fleeting dash to plant a flag. The idea is to begin preparing now for a future in which the material trapped in the Sun's vicinity is available for incorporation into our way of life. Dr. John Marburger, Head of the Office of Science and Technology Policy 2006 3 The Investment Premise • Just as on Earth, lunar real estate “value” is driven by location, location, location Rank Location Why Valuable 1 Peary Crater Best 1st industrial base and settlement 2 Sinus Medii Good cargo port & space elevator site 3 Largest skylights / lava tubes Best large scale settlements 4 Tsiolkovskiy crater, dark side Prime radio astronomy site 5 High helium-3 concentrations Potential high value mining 6 Lipsky Crater Space elevator site for Earth-Moon L2 7 Aristillus High Thorium concentrations • Lunar real
    [Show full text]
  • Surveyor 1 Space- Craft on June 2, 1966 As Seen by the Narrow Angle Camera of the Lunar Re- Connaissance Orbiter Taken on July 17, 2009 (Also See Fig
    i “Project Surveyor, in particular, removed any doubt that it was possible for Americans to land on the Moon and explore its surface.” — Harrison H. Schmitt, Apollo 17 Scientist-Astronaut ii Frontispiece: Landing site of the Surveyor 1 space- craft on June 2, 1966 as seen by the narrow angle camera of the Lunar Re- connaissance Orbiter taken on July 17, 2009 (also see Fig. 13). The white square in the upper photo outlines the area of the enlarged view below. The spacecraft is ca. 3.3 m tall and is casting a 15 m shadow to the East. (NASA/LROC/ ASU/GSFC photos) iii iv Surveyor I: America’s First Moon Landing by William F. Mellberg v © 2014, 2015 William F. Mellberg vi About the author: William Mellberg was a marketing and public relations representative with Fokker Aircraft. He is also an aerospace historian, having published many articles on both the development of airplanes and space vehicles in various magazines. He is the author of Famous Airliners and Moon Missions. He also serves as co-Editor of Harrison H. Schmitt’s website: http://americasuncommonsense.com Acknowledgments: The support and recollections of Frank Mellberg, Harrison Schmitt, Justin Rennilson, Alexander Gurshstein, Paul Spudis, Ronald Wells, Colin Mackellar and Dwight Steven- Boniecki is gratefully acknowledged. vii Surveyor I: America’s First Moon Landing by William F. Mellberg A Journey of 250,000 Miles . December 14, 2013. China’s Chang’e 3 spacecraft successfully touched down on the Moon at 1311 GMT (2111 Beijing Time). The landing site was in Mare Imbrium, the Sea of Rains, about 25 miles (40 km) south of the small crater, Laplace F, and roughly 100 miles (160 km) east of its original target in Sinus Iridum, the Bay of Rainbows.
    [Show full text]
  • Guide to Observing the Moon
    Your guide to The Moonby Robert Burnham A supplement to 618128 Astronomy magazine 4 days after New Moon south is up to match the view in a the crescent moon telescope, and east lies to the left. f you look into the western sky a few evenings after New Moon, you’ll spot a bright crescent I glowing in the twilight. The Moon is nearly everyone’s first sight with a telescope, and there’s no better time to start watching it than early in the lunar cycle, which begins every month when the Moon passes between the Sun and Earth. Langrenus Each evening thereafter, as the Moon makes its orbit around Earth, the part of it that’s lit by the Sun grows larger. If you look closely at the crescent Mare Fecunditatis zona I Moon, you can see the unlit part of it glows with a r a ghostly, soft radiance. This is “the old Moon in the L/U. p New Moon’s arms,” and the light comes from sun- /L tlas Messier Messier A a light reflecting off the land, clouds, and oceans of unar Earth. Just as we experience moonlight, the Moon l experiences earthlight. (Earthlight is much brighter, however.) At this point in the lunar cycle, the illuminated Consolidated portion of the Moon is fairly small. Nonetheless, “COMET TAILS” EXTENDING from Messier and Messier A resulted from a two lunar “seas” are visible: Mare Crisium and nearly horizontal impact by a meteorite traveling westward. The big crater Mare Fecunditatis. Both are flat expanses of dark Langrenus (82 miles across) is rich in telescopic features to explore at medium lava whose appearance led early telescopic observ- and high magnification: wall terraces, central peaks, and rays.
    [Show full text]
  • A Map of the Visible Side of the Moon
    The Near Side of the Moon 108 N 107 106 105 45 104 46 103 47 102 48 101 49 100 24 50 99 51 52 22 53 98 33 35 54 97 34 23 55 96 95 56 36 25 57 94 58 93 2 92 44 15 40 59 91 3 27 37 17 38 60 39 6 19 20 26 28 1 18 4 29 21 11 30 W 12 E 14 5 43 90 10 16 89 7 41 61 8 62 9 42 88 32 63 87 64 86 31 65 66 85 67 84 68 83 69 82 81 70 80 71 79 72 73 78 74 77 75 76 S Maria (Seas) Craters 1 - Oceanus Procellarum (Ocean of Storms) 45 - Aristotles 77 - Tycho 2 - Mare Imbrium (Sea of Showers) 46 - Cassini 78 - Pitatus 3 - Mare Serenitatis (Sea of Serenity) 47 - Eudoxus 79 - Schickard 4 - Mare Tranquillitatis (Sea of Tranquility) 48 - Endymion 80 - Mercator 5 - Mare Fecunditatis (Sea of Fertility) 49 - Hercules 81 - Campanus 6 - Mare Crisium (Sea of Crises) 50 - Atlas 82 - Bulliadus 7 - Mare Nectaris (Sea of Nectar) 51 - Mercurius 83 - Fra Mauro 8 - Mare Nubium (Sea of Clouds) 52 - Posidonius 84 - Gassendi 9 - Mare Humorum (Sea of Moisture) 53 - Zeno 85 - Euclides 10 - Mare Cognitum (Known Sea) 54 - Menelaus 86 - Byrgius 18 - Mare Insularum (Sea of Islands) 55 - Le Monnier 87 - Billy 19 - Sinus Aestuum (Bay of Seething) 56 - Vitruvius 88 - Cruger 20 - Mare Vaporum (Sea of Vapors) 57 - Cleomedes 89 - Grimaldi 21 - Sinus Medii (Bay of the Center) 58 - Plinius 90 - Riccioli 22 - Sinus Roris (Bay of Dew) 59 - Magelhaens 91 - Galilaei 23 - Sinus Iridum (Bay of Rainbows) 60 - Taruntius 92 - Encke T 24 - Mare Frigoris (Sea of Cold) 61 - Langrenus 93 - Eddington 25 - Lacus Somniorum (Lake of Dreams) 62 - Gutenberg 94 - Seleucus 26 - Palus Somni (Marsh of Sleep)
    [Show full text]
  • AL Lunar 100
    AL Lunar 100 The AL Lunar 100 introduces amateur astronomers to that object in the sky that most of us take for granted, and which deep sky observers have come to loathe. But even though deep sky observers search for dark skies (when the moon is down), this list gives them something to do when the moon is up. In other words, it gives us something to observe the rest of the month, and we all know that the sky is always clear when the moon is up. The AL Lunar 100 also allows amateurs in heavily light polluted areas to participate in an observing program of their own. This list is well suited for the young, inexperienced observer as well as the older observer just getting into our hobby since no special observing skills are required. It is well balanced because it develops naked eye, binocular, and telescopic observing skills. The AL Lunar 100 consists of 100 features on the moon. These 100 features are broken down into three groups: 18 naked eye, 46 binocular, and 36 telescopic features. Any pair of binoculars and any telescope may be used for this list. This list does not require expensive equipment. Also, if you have problems with observing the features at one level, you may go up to the next higher level. In other words, if you have trouble with any of the naked eye objects, you may jump up to binoculars. If you have trouble with any of the binocular objects, then you may move up to a telescope. Before moving up to the next higher level, please try to get as many objects as you can with the instrument required at that level.
    [Show full text]
  • Dragon Fire! Copy Subscriber
    SpaceFlight A British Interplanetary Society publication Volume 61 No.5 May 2019 £5.25 Dragon fire! copy Subscriber Apollo feedback 05> Commercial space 634089 Steps back to the Moon 770038 Remembering Apollo 10 9 copy Subscriber CONTENTS Features 16 Return of the Dragon SpaceX has taken a big step forward by successfully launching its Dragon 2 crew- carrying capsule to the International Space Station but how long before astronauts get to ride the latest people-carrier? 2 Letter from the Editor 18 The Impact of Apollo – Part 2 Nick Spall FBIS looks at the technological and The excitement just keeps on inspirational legacy of the Apollo Moon shots growing! No sooner did we have and finds value in the money spent. the first uncrewed landing on the far side of the Moon by China than Israel launched the first privately 22 Apollo 10 – so near, yet so far funded spacecraft to head for a David Baker recalls events 50 years ago when lunar touchdown. Then, NASA three astronauts got closer to the Moon than boss Jim Bridenstine advised ever before and yet left the final descent to glory Congress that its flagship rocket, to the next mission in line, clearing the way for 16 the Space Launch System, may the first landing. not be ready to launch Orion in 2020 as planned, while calling on 32 Commercial Space commercial providers to step up Using a wide range of commercial providers, and fly the mission to fast-track humans back on the Moon in 2028 NASA is building a roadmap to the Moon with (page 2).
    [Show full text]
  • Geologic Maps of Early Apollo Landing Sites of Set C
    UH ITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY .. This report is preliminary and has not been edited or reviewed for conformity with U.S. Geological Survey standards and nomenclature. Prepared by the Geological Survey for the l National Aeronautics and Space Administration LUNAR .. INTERAGENCY REPORT: ASTROGEOLOGY 17 GEOLOGIC MAPS OF EARLY APOLLO LANDING SITES OF SET C By N. J. Trask October 1969 Prepared under NASA Contract T-66353G CONTENTS Page Abstract .. 1 Introduction 1 Acknowledgments 2 Geology of the Moon, general 3 Assignment of materials to time-stratigraphic units 6 Definitions and conventions . 6 Assignment of crater materials 8 Assignment of mare materials 12 Assignment of terra materials 13 Scientific significance of features common to all sites 13 Regolith 14 Craters . 14 Other landfprms 18 Scientific significance of individual sites 18 Site 1 (II P- 2, East Two) 19 Site 2 (II P-6, East One) 20 Site 3 (II P-8. Central One). 21 Site 4 (III P-11, West Two) 22 Site 5 (II P-13, West One). 24 Summary 26 References 26 ILLUSTRATIONS Figure 1. Location of five early Apollo landing sites of set C 4 2. Graph relating craters' morphological characteristics with their diameters and postulated ages .. 10 TABLES Table 1. Authors of geologic maps of Apollo landing sites of set C ..... 5 iii Tables--continued Page 2. Lunar stratigraphic and time divisions as shown on 1:1,000,000-scale maps 7 3. Summary of geologic characteristics of Apollo landing sites of set C . 25 iv GEOLOGIC MAPS OF EARLY APOLLO LANDING SITES OF SET C By N.
    [Show full text]
  • Lunar Club Program
    Lunar Club Program Naked Eye Objects Instruments Used ____________________________ OBJECT FEATURE DATE TIME [ ] (Within 72 Hrs of new) Old Moon in New Moon's Arms _______ ______ [ ] (Within 72 Hrs of new) New Moon in Old Moon's Arms _______ ______ [ ] (Within 40 Hrs of new) Crescent Moon, Waxing _______ ______ [ ] (Within 48 Hrs of New) Crescent Moon, Waning _______ ______ [ ] Man in the Moon _______ ______ [ ] Woman in the Moon _______ ______ [ ] Rabbit in the Moon _______ ______ [ ] Cow Jumping Over the Moon _______ ______ Maria [ ] Crisium _______ ______ [ ] Fecunditatis _______ ______ [ ] Serenitatis _______ ______ [ ] Tranquillitatis _______ ______ [ ] Nectaris _______ ______ [ ] Imbrium _______ ______ [ ] Frigoris _______ ______ [ ] Nubium _______ ______ [ ] Humorum _______ ______ [ ] Oceanus Procellarum _______ ______ Binocular Objects Instruments Used ____________________________ OBJECT FEATURE DATE TIME [ ] Lunar Rays _______ ______ [ ] Sinus Iridum _______ ______ [ ] Sinus Medii _______ ______ [ ] Sinus Roris _______ ______ [ ] Palus Somnii _______ ______ [ ] Palus Epidemiarum _______ ______ [ ] Mare Vaporum _______ ______ Craters [ ] ~4 Days old Langrenus _______ ______ [ ] Vendelinus _______ ______ [ ] Petavius _______ ______ [ ] Cleomedes _______ ______ [ ] Atlas _______ ______ [ ] Hercules _______ ______ [ ] Endymion _______ ______ [ ] Macrobius _______ ______ [ ] ~7 Days old Piccolomini _______ ______ [ ] Theophilus _______ ______ [ ] Cyrillus _______ ______ [ ] Catharina _______ ______ [ ] Posidonius _______ ______ [ ]
    [Show full text]
  • 19710008022.Pdf
    INTERAGENCY REPORT: ASTROGEOLOGY 17 GEOLOGIC MAPS OF EARLY APOLLO LANDING SITES OF SET C N. J. Trask October 1969 Prepared under NASA Contract T-66353G CONTENTS Page Abstract .......................... k Introduction ......................... 1 Acknowledgments ...................... 2 Geology of the Moon. general ..............., 3 Assignment of materials to time-stratigraphic units .... 6 Definitions and conventions .............. 6 Assignment of crater materials ............ 8 Assignment of mare materials ............. 12 Assignment of terra materials ............. 13 Scientific significance of features common to all sites . 13 Regolith ....................... 14 Craters ........................ 14 Other landforms .................... 18 Scientific significance of individual sites ........ kt3 Site 1 (I1 P-2. East Two) ............... 19 Site 2 (I1 P-6. East One) ............... 20 Site 3 (I1 P-8 . Central One) .............. 21 Site 4 (111 P-11. West Two) .............. 22 Site 5 (I1 P-13. West One) ............... 24 Summary .......................... 26 References ......................... 26 ILLUSTRATIONS Figure 1. Location of five early Apollo landing sites ofsetC ................... 4 2 . Graph relating craters' morphological characteristics with their diameters and postulated ages .............. 10 TABLES Table 1. Authors of geologic maps of Apollo landing sites of set C ................. 5 iii Tables--continued Page 2, Lunar stratigraphic and time divisions as shown on 1:1,000,000-scale maps . 7 3, Summary of geologic characteristics of Apollo landing sites of set C . 25 GEOLOGIC MASS OF EARLY APOLLO ING SITES OF SET C By N. J. Trask ABSTRACT Comparison of the five potential early Apollo landing sites of set C reveals significant geologic similarities and differences, No two sites are identical; the geology of each should be consid- ered in the interpretation of returned lunar samples and observa- tions.
    [Show full text]
  • APOLLO 11 PRELIMINARY SCIENCE REPORT Landing Sites
    NASA SP-214 Prelin1l[nary Science lleport NATIONAL AERONAUTICS AND SPACE ADMINISTRATION ACKNOWLEDGMENT The material submitted for the Lunar Surface Scien­ tific Mission of Apollo ll was reviewed by a NASA Manned Spacecraft Center Technical Review Board consisting of the following members: J. M. \Vest (Chair­ man), P. R. Bell, A. J. Calia, J. W. Harris, H. H. Schmitt, S. H. Simpkinson, W. K. Stephenson, and D. G. Wiseman. For sale by the Clearinghouse for Federal Scientific and Technical Information, Springfield, Virginia 22151 CFSTI price $3.00 Library of Congress Catalog Card Number 77-603770 Foreword OuR FJRST JOURNEY to the Jvloon ushered in a new era in which man will no longer be confined to his home planet. The concept of traveling across the vastness of space to new worlds has stirred the imagination of men everywhere. One-sixth of the Earth's population watched as the Apollo 11 astronauts walked and worked a quarter of a million miles away. The success of this mission has opened new fields of exploration and research - research which will lead to a greater understanding of our planet and provide a new insight into the origin and history of the solar system. The Apollo 11 mission was only a beginning, however. Subsequent missions will reflect more ambitious scientific objectives and will include more comprehensive observations and measurements at a variety of lunar sites. This document is a preliminary report of the initial scientific observations resulting from the Apollo 11 mission. We expect that further significant results will come from more detailed analysis of the returned samples of lunar material, and from additional study of the photographs and data obtained from the emplaced experiments.
    [Show full text]
  • Mare Basalt Thickness in Sinus Aestuum and Sinus Medii J
    Journal of the Arkansas Academy of Science Volume 31 Article 43 1977 Mare Basalt Thickness in Sinus Aestuum and Sinus Medii J. B. Sharp University of Arkansas at Monticello N. Gilbert University of Arkansas at Monticello R. A. de Hon University of Arkansas at Monticello Follow this and additional works at: http://scholarworks.uark.edu/jaas Part of the Geology Commons Recommended Citation Sharp, J. B.; Gilbert, N.; and de Hon, R. A. (1977) "Mare Basalt Thickness in Sinus Aestuum and Sinus Medii," Journal of the Arkansas Academy of Science: Vol. 31 , Article 43. Available at: http://scholarworks.uark.edu/jaas/vol31/iss1/43 This article is available for use under the Creative Commons license: Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0). Users are able to read, download, copy, print, distribute, search, link to the full texts of these articles, or use them for any other lawful purpose, without asking prior permission from the publisher or the author. This General Note is brought to you for free and open access by ScholarWorks@UARK. It has been accepted for inclusion in Journal of the Arkansas Academy of Science by an authorized editor of ScholarWorks@UARK. For more information, please contact [email protected], [email protected]. Journal of the Arkansas Academy of Science, Vol. 31 [1977], Art. 43 General Notes Cevatomia hagcni Grote llagen's Sphinx Erinnyis ello (Linnaeus) Ello Sphinx Isoparne aupressi (Boisduval) Cypress Sphinx Erinnyis obscuva (Fabricius) Obscure Sphinx Pavatrea plebeja (Fabricius) Plebeian Sphinx Aellopos titan (Cramer) White-banded DayD, Sphinx Sphinx BfemibUB (Hiibner) Hermit Sphinx Aellopos fadus (Cramer) Fadus Day Sphinx Sphinx ahersis (HiJbner) Chersis Sphinx Hemaris thysbe (Fabricius) Hummingbird Clearwing Sphinx aanadcnsis Boisduval Canadian Sphinx Hemaris diffinis (Boisduval) Snowberry Clearwing Sphinx kalmiae .1.
    [Show full text]
  • Mystery Maria
    exploring the moon by charles a. wood Mystery Maria nearly all the Moon’s big maria (“seas”) are circular because they fi ll ancient impact basins. But Mare Frigoris The Lunar 100 isn’t. Frigoris (L26 in the Lunar 100) is a 1,500-kilometer- L Feature name Significance long (930-mile), 200-km-wide arc of lava that spans from 10 Mare Crisium Mare contained in large circular basin Oceanus Procellarum in the west to the craters Atlas and Hercules in the east. 26 Mare Frigoris Arcuate mare of uncertain origin One characteristic of Mare Frigoris that See Sky & Telescope: April 2004, page 113, or point your Web browser to SkyTonight A few of the .com/lunar100. may help explain its origin is the fact Moon’s biggest that it’s mostly concentric with the Im- features are brium impact basin. But Frigoris isn’t the “basins” typically have two to six concentric rings and are only mare hugging Imbrium’s rim. Mare more accurately referred to as multiring impact basins. also its most Vaporum, Sinus Medii, Sinus Aestuum, This aspect is best illustrated by the far-side basin Orientale puzzling. and Mare Insularum help defi ne a moat — the youngest and least modifi ed lunar basin. of lava that encircles much of Imbrium. Although six rings have been mapped around Orientale, And Imbrium isn’t the only basin surrounded by maria. only three are clearly visible. The most dramatic is the If you look closely outside the main rim of Mare Crisium 930-km-wide Cordillera Mountains ring, which is partially (L10), you’ll notice that it’s surrounded by a similar, but visible when the western edge of the Moon is tilted to- less conspicuous, lava arc.
    [Show full text]