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88 PAJ 116 Anne Carson Reading Text in STACKS © Michael Hart, 2008
Anne Carson reading text in STACKS © Michael Hart, 2008. Courtesy Jonah Bokaer Choreography. 88 PAJ 116 Downloaded from http://www.mitpressjournals.org/doi/pdf/10.1162/PAJJ_a_00369 by guest on 01 October 2021 Stacks Anne Carson STACK OF THE SEAS OF THE MOON IN ALPHABETICAL ORDER Mare Aliorum Sea of Others Mare Ambulationis Sea of Walking Mare Anguis Snake Sea Mare Australe Sea to the South Mare Crisium Sea of Crises Mare Dormiendi Nuditer Sea of Sleeping Naked Mare Frigoris Sea of Cold Mare Humboldtianum Humboldt’s Sea Mare Humorum Sea of Moistures Mare Imbrium Sea of Rains Mare Lunae Quaestionum Sea of the Problems of the Moon Mare Marginis Border Sea Mare Moscoviense Moscow Sea Mare Nectaris Sea of Nectar Mare Nocte Ambulationis Sea of Walking at Night Mare Nubium Sea of Clouds Mare Orientale Sea to the East Mare Personarum Sea of Masks Mare Phoenici Phoenician Sea Mare Phoenicopterorum Sea of Flamingos Mare Pudoris Sea of Shame Mare Relictum Sea of Detroit Mare Ridens Laughing Sea Mare Smythii Sea of Smyth Mare Spumans Foaming Sea Mare Tempestivitatis Sea of What Frank O’Hara Calls “Cantankerous Filaments of a Larger Faintheartedness Like Loving Summer” Mare Vituperationis Sea of Blaming © 2017 Anne Carson PAJ 116 (2017), pp. 89–108. 89 doi:10.1162/PAJJ _a_00369 Downloaded from http://www.mitpressjournals.org/doi/pdf/10.1162/PAJJ_a_00369 by guest on 01 October 2021 THUNDERSTORM STACK A bird flashed by as if mistaken then it starts. We do not think speed of life. We do not think why hate Jezebel? We think who’s that throwing trees against the house? Jezebel was a Phoenician. -
Radar Remote Sensing of Pyroclastic Deposits in the Southern Mare Serenitatis and Mare Vaporum Regions of the Moon Lynn M
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, E11004, doi:10.1029/2009JE003406, 2009 Click Here for Full Article Radar remote sensing of pyroclastic deposits in the southern Mare Serenitatis and Mare Vaporum regions of the Moon Lynn M. Carter,1 Bruce A. Campbell,1 B. Ray Hawke,2 Donald B. Campbell,3 and Michael C. Nolan4 Received 21 April 2009; revised 12 July 2009; accepted 3 August 2009; published 5 November 2009. [1] We use polarimetric radar observations to study the distribution, depth, and embedded rock abundance of nearside lunar pyroclastic deposits. Radar images were obtained for Mare Vaporum and the southern half of Mare Serenitatis; the imaged areas contain the large Rima Bode, Mare Vaporum, Sulpicius Gallus, and Taurus-Littrow pyroclastic deposits. Potential pyroclastic deposits at Rima Hyginus crater, the Tacquet Formation, and a dome in Mare Vaporum are also included. Data were acquired at S band (12.6 cm wavelength) using Arecibo Observatory and the Green Bank Telescope in a bistatic configuration. The S band images have resolutions between 20 and 100 m/pixel. The pyroclastic deposits appear dark to the radar and have low circular polarization ratios at S band wavelengths because they are smooth, easily penetrable by radar waves, and generally contain few embedded blocks. Changes in circular polarization ratio (CPR) across some of the pyroclastic deposits show areas with increased rock abundance as well as deposits that are shallower. Radar backscatter and CPR maps are used to identify fine-grained mantling deposits in cases where optical and near-infrared data are ambiguous about the presence of pyroclastics. -
10Great Features for Moon Watchers
Sinus Aestuum is a lava pond hemming the Imbrium debris. Mare Orientale is another of the Moon’s large impact basins, Beginning observing On its eastern edge, dark volcanic material erupted explosively and possibly the youngest. Lunar scientists think it formed 170 along a rille. Although this region at first appears featureless, million years after Mare Imbrium. And although “Mare Orien- observe it at several different lunar phases and you’ll see the tale” translates to “Eastern Sea,” in 1961, the International dark area grow more apparent as the Sun climbs higher. Astronomical Union changed the way astronomers denote great features for Occupying a region below and a bit left of the Moon’s dead lunar directions. The result is that Mare Orientale now sits on center, Mare Nubium lies far from many lunar showpiece sites. the Moon’s western limb. From Earth we never see most of it. Look for it as the dark region above magnificent Tycho Crater. When you observe the Cauchy Domes, you’ll be looking at Yet this small region, where lava plains meet highlands, con- shield volcanoes that erupted from lunar vents. The lava cooled Moon watchers tains a variety of interesting geologic features — impact craters, slowly, so it had a chance to spread and form gentle slopes. 10Our natural satellite offers plenty of targets you can spot through any size telescope. lava-flooded plains, tectonic faulting, and debris from distant In a geologic sense, our Moon is now quiet. The only events by Michael E. Bakich impacts — that are great for telescopic exploring. -
List of Targets for the Lunar II Observing Program (PDF File)
Task or Task Description or Target Name Wood's Rükl Target LUNAR # 100 Atlas Catalog (chart) Create a sketch/map of the visible lunar surface: 1 Observe a Full Moon and sketch a large-scale (prominent features) L-1 map depicting the nearside; disk of visible surface should be drawn 2 at L-1 3 least 5-inches in diameter. Sketch itself should be created only by L-1 observing the Moon, but maps or guidebooks may be used when labeling sketched features. Label all maria, prominent craters, and major rays by the crater name they originated from. (Counts as 3 observations (OBSV): #1, #2 & #3) Observe these targets; provide brief descriptions: 4 Alpetragius 55 5 Arago 35 6 Arago Alpha & Arago Beta L-32 35 7 Aristarchus Plateau L-18 18 8 Baco L-55 74 9 Bailly L-37 71 10 Beer, Beer Catena & Feuillée 21 11 Bullialdus, Bullialdus A & Bullialdus B 53 12 Cassini, Cassini A & Cassini B 12 13 Cauchy, Cauchy Omega & Cauchy Tau L-48 36 14 Censorinus 47 15 Crüger 50 16 Dorsae Lister & Smirnov (A.K.A. Serpentine Ridge) L-33 24 17 Grimaldi Basin outer and inner rings L-36 39, etc. 18 Hainzel, Hainzel A & Hainzel C 63 19 Hercules, Hercules G, Hercules E 14 20 Hesiodus A L-81 54, 64 21 Hortensius dome field L-65 30 22 Julius Caesar 34 23 Kies 53 24 Kies Pi L-60 53 25 Lacus Mortis 14 26 Linne 23 27 Lamont L-53 35 28 Mairan 9 29 Mare Australe L-56 76 30 Mare Cognitum 42, etc. -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
Effusive Lunar Domes in Capuanus Crater: Morphometry and Mode of Emplacement
42nd Lunar and Planetary Science Conference (2011) 1443.pdf EFFUSIVE LUNAR DOMES IN CAPUANUS CRATER: MORPHOMETRY AND MODE OF EMPLACEMENT. R. Lena 1, R. Evans 2, S. Lammel 3, J. Phillips 4, C. Wöhler 5 – Geologic Lunar Research (GLR) group. 1Via Cartesio 144, sc. D, I-00137 Rome, Italy; [email protected]; 2114 Simonds St., Fitchburg, MA 01420, USA; [email protected]; 326 Amberley Way, Uxbridge, Middlesex, England; [email protected]; 4101 Bull Street, Charleston, SC 29401, USA, [email protected]; 5Image Analysis Group, Dortmund Uni- versity of Technology, Dortmund, Germany; [email protected] Introduction: Recent studies about lunar mare domes 0.16° and 1.27° ± 0.13°, while the edifice volumes are based on the evaluation of their spectrophotometric amount to 1.90 km 3 and 3.17 km 3 for Ca1 and Ca2, re- and morphometric properties, rheologic parameters, and spectively. The recently released global digital elevation their classification based on the spectral properties and map (DEM) obtained with the Lunar Orbiter Laser Alti- three-dimensional shapes of the volcanic edifices [1, 2]. meter (LOLA) on board the Lunar Reconnaissance Orbi- In this contribution we provide an analysis of three domes ter (LRO) spacecraft with its lateral resolution of 1/64 located inside Capuanus, a ruined crater in Palus Epide- degrees or ~500 m in the equatorial regions of the Moon miarum, a small lava plain at the southwestern edge of (http://pds-geosciences.wustl.edu/missions/lro/lola.htm) Mare Nubium. In this region, tectonic features such as was used to render an image of the Capuanus domes the complex rille systems of Rimae Ramsden and the using the LTVT software package [3] (cf. -
Moon Map and Features
Northern Stars Planetarium Teacher Resource Sheets 1 Find more at NorthernStarsPlanetarium.com The Moon and its features This is a guide to the surface features on the Moon which you can see with binoculars or a small telescope. Northern Stars Planetarium Teacher Resource Sheets 2 Find more at NorthernStarsPlanetarium.com The Moon without labels What features can you identify? Seas? Craters? Mountains? Do you know where the astronauts landed? Northern Stars Planetarium Teacher Resource Sheets 3 Find more at NorthernStarsPlanetarium.com The Maria (or seas, oceans, bays and lakes) These do not have any water, nor are they craters, they are ancient hardened lava flows on the surface of the Moon. Listed from west to east (left to right) English name (latin name) • Ocean of Storms (Oceanus Procellarun) • Bay of Dew (Sinus Roris) • Sea of Cold (Mare Frigoris) • Bay of Rainbows (Sinus Iridum) • Sea of Showers (Mare Imbrium) • Sea of Islands (Mare Insularum) • Known Sea (Mare Cognitum) • Sea of Moisture (Mare Humorum) • Marsh of Epidemics (Palus Epidemiarum) • Sea of Clouds (Mare Nubium) • Sea of Vapors (Mare Vaporum) • Sea of Serenity (Mare Serenitatis) • Lake of Dreams (Lacus Somniorum) • Sea of Tranquility (Mare Tranquilitatis) • Bay of Love (Sinus Amoris) • Sea of Nectar (Mare Nectaris) • Southern Sea (Mare Australe) • Sea of Fertility (Mare Fecunditatis) • Sea of Crises (Mare Crisium) • Border Sea (Mare Marginis) Northern Stars Planetarium Teacher Resource Sheets 4 Find more at NorthernStarsPlanetarium.com Craters The Moon’s craters were created by meteoric impacts on the surface. There are over 5000 craters larger than 12 miles in diameter, here are a sampling of them that can be found with a small telescope or binoculars. -
What's Hot on the Moon Tonight?: the Ultimate Guide to Lunar Observing
What’s Hot on the Moon Tonight: The Ultimate Guide to Lunar Observing Copyright © 2015 Andrew Planck All rights reserved. No part of this book may be reproduced in any written, electronic, recording, or photocopying without written permission of the publisher or author. The exception would be in the case of brief quotations embodied in the critical articles or reviews and pages where permission is specifically granted by the publisher or author. Although every precaution has been taken to verify the accuracy of the information contained herein, the publisher and author assume no responsibility for any errors or omissions. No liability is assumed for damages that may result from the use of information contained within. Books may be purchased by contacting the publisher or author through the website below: AndrewPlanck.com Cover and Interior Design: Nick Zelinger (NZ Graphics) Publisher: MoonScape Publishing, LLC Editor: John Maling (Editing By John) Manuscript Consultant: Judith Briles (The Book Shepherd) ISBN: 978-0-9908769-0-8 Library of Congress Catalog Number: 2014918951 1) Science 2) Astronomy 3) Moon Dedicated to my wife, Susan and to my two daughters, Sarah and Stefanie Contents Foreword Acknowledgments How to Use this Guide Map of Major Seas Nightly Guide to Lunar Features DAYS 1 & 2 (T=79°-68° E) DAY 3 (T=59° E) Day 4 (T=45° E) Day 5 (T=24° E.) Day 6 (T=10° E) Day 7 (T=0°) Day 8 (T=12° W) Day 9 (T=21° W) Day 10 (T= 28° W) Day 11 (T=39° W) Day 12 (T=54° W) Day 13 (T=67° W) Day 14 (T=81° W) Day 15 and beyond Day 16 (T=72°) Day 17 (T=60°) FINAL THOUGHTS GLOSSARY Appendix A: Historical Notes Appendix B: Pronunciation Guide About the Author Foreword Andrew Planck first came to my attention when he submitted to Lunar Photo of the Day an image of the lunar crater Pitatus and a photo of a pie he had made. -
Lunar Program Observing List Lunar Observing Program Coordinator: Nina Chevalier 1662 Sand Branch Rd
Lunar Program Observing List Lunar Observing Program Coordinator: Nina Chevalier 1662 Sand Branch Rd. Bigfoot, Texas 78005 210-218-6288 [email protected] The List The 100 features to be observed for the Lunar Program are listed below. At the top of each section is a space to list the instruments used in the program. After that are five columns: CHK, Object, Feature, Date and Time. The "CHK" column should be used to check off the feature as you observe it. The "Object" column lists the features in Naked Eye, Binocular, and Telescopic order, and tells you what you are observing and when the best time is to observe it. The "Feature" column lists the 100 features to be observed. Finally, the "Date" and "Time" columns allow you to log when you observed the objects. In the last section, we have listed the 10 optional activities, and broken them down as to naked eye, binocular, and telescopic. Also on page 4, we have included four illustrations to help with observing four of the naked eye features. We certainly hope that you find the Lunar Program useful in helping you become more familiar with earth's nearest neighbor. If after completing this program you would like to do more work in this area, you may contact The Association of Lunar and Planetary Observers. Julius L. Benton Jr. ALPO Lunar Recorder % Associates in Astronomy 305 Surrey Road Savannah, Ga. 31410 (912) 897-0951 E-mail: [email protected]. Until then, good luck, clear skies, and good observing. Lunar Program Checklist Naked Eye Objects Instruments Used ____________________________ -
Moon Course Section 27-33 V1.0
Around the Moon in 28 Days: Lunar Observing for Beginners Course Notes Section 27 - Lunar Day 22 Section 28 - Lunar Day 23 Section 29 - Lunar Day 24 Section 30 - Lunar Day 25 Section 31 - Lunar Day 26 Section 32 - Lunar Day 27 Section 33 - Lunar Day 28 (The End) Copyright © 2010 Mintaka Publishing Inc. 2 Section 27 - Lunar Day 22 Tonight's late rising Moon might seem impossible to study when you have a daytime work schedule, but why not consider going to bed early and spending the early morning hours contemplating some lunar history and the peace and quiet before the day begins? Let's journey off to the lonely Riphaeus Mountains just southwest of crater Copernicus. Northeast of the range is another smooth floored area on the border of Oceanus Procellarum. It is here that Surveyor 3 landed on April 19, 1967. Figure 27-1: The major features of the Moon on Day 22 Around the Moon in 28 Days: Lunar Observing for Beginners 3 Figure 27-2: Surveyor 3 and Apollo 12 and 14 landing sites (courtesy of NASA) After bouncing three times, the probe came to rest on a smooth slope in a sub-telescopic crater. As its on-board television monitors watched, Surveyor 3 extended its mechanical arm with a "first of its kind" miniature shovel and dug to a depth of 18 inches. The view of sub-soil material and its clean-cut lines allowed scientists to conclude that the loose lunar soil could compact. Watching Surveyor 3 pound its shovel against the surface, the resulting tiny "dents" answered the crucial question. -
NASA MEO Lunar Impact Candidates
NASA Marshall Space Flight Center (MSFC) - Automated Lunar and Meteor Observatory (ALaMO) - Candidate lunar impact observation database NASA Meteoroid Environment Office (MEO) Last Updated: 9-Mar-2009 By: D. Moser PRELIMINARY # of video Lunar Lunar Effective Peak Time Probable Lunar Lunar frames illum. Lunar elevation Aperture focal length MEO Flash # Date (UT) (UT) Type longitude latitude Region (1/30 sec) fraction phase (deg) (cm) Optical config. (cm) Camera Digitizer Location Observers Press release links 1 7-Nov-05 23:40:53.0 Taurid 39.5 W 31.9 N Gruithuisen 5 0.38 wax 28.9 25.4 Newtonian T 119 StellaCam EX Sony GV-D800 MSFC 4487 Suggs and Swift http://science.nasa.gov/headlines/y2005/22dec_lunartaurid.htm 2 2-May-06 02:34:39.0 Sporadic 19.6 W 24.3 S Bullialdus 14 0.21 wax 26.5 25.4 Newtonian T 119 StellaCam EX Sony GV-D800 MSFC ALAMO Moser and McNamara http://science.nasa.gov/headlines/y2006/13jun_lunarsporadic.htm 3 4-Jun-06 04:48:35.4 Sporadic 35.8 W 11.8 S Rima Herigonius 1.5 0.52 wax 19.1 25.4 Newtonian T 119 StellaCam EX Sony GV-D800 MSFC ALAMO Swift, Hollon, & Altstatt 105 21-Jun-06 08:35:45.0 Sporadic 22.7 E 2.1 N Central Mare Tranquillitatus 2 0.20 wan 15.6 25.4 Newtonian T 119 StellaCam EX Sony GV-D800 MSFC ALAMO Moser and McNamara 4 21-Jun-06 08:57:17.5 Sporadic 62.9 E 13.9 N Mare Crisium 2.5 0.21 wan 19.9 25.4 Newtonian T 119 StellaCam EX Sony GV-D800 MSFC ALAMO Moser and McNamara 4 21-Jun-06 08:57:17.5 Sporadic 62.9 E 13.9 N Mare Crisium 1.5 0.21 wan 19.9 35.5 Rit Chret SD 94 StellaCam EX Sony GV-D800 MSFC ALAMO Suggs -
Planetológiai Helyesírási Tanácsadó
Planetológiai helyesírási tanácsadó GEOLÓGIA Kőzetrétegtani egységek ridged member = gerinces tagozat Heveliusi Formáció, Hold Geokronológia (idő) imbriumi időszak kora-imbriumi kor noachi időszak Kronosztratigráfia (időrétegtani)(kőzettestek) imbriumi rendszer alsó-imbriumi sorozat noachi rendszer Az egyes egységek magyar elnevezései MERKÚR kuiperi mansuri calorisi tolsztoji pretolsztoji VÉNUSZ aureliai atlai guinevrai ruszalkai laviniai sigrúni fortunai prefortunai HOLD kopernikuszi eratoszthenészi imbriumi nektári prenektári (procellárumi: elavult) MARS amazoni heszperiai noachi prenoachi MARS - geokémiai sideriki theiiki phylloci (ejtsd: filloszi) GEOGRÁFIA Bolygófelszíni alakzatok elnevezései Köznévi taggal (az alábbiakat mindig kötőjellel kapcsoljuk, kivéve birtokos esetben: Cassini-régió, de: Válságok tengere) Megjegyzések: • Az itt felsorolt alakok: latin alak egyes szám, többes szám [latin alak latinos kiejtése], magyar megfelelő • A ¯ jel az előtte álló u-n vagy e-n lévő vonalékezet • A toldalékok a (magyar vagy latin) nevekhez általában közvetlenül kapcsolódnak, a szükséges hasonulások vagy a szóvégi magánhangzó nyúlásának a jelölésével: Caloris Montesszal, Lavinia Planitián, Ión. • A két különírt tagból álló latin elnevezésekhez az -i/-beli képzô kötôjellel kapcsolódik; az eredeti kis- és nagybetûket megtartjuk: Caloris Planitia-i, Sinus Meridiani-beli stb. (vö. AkH. 1984: 217. b) pont). A két különírt tagból álló magyar elnevezéseknél az -i képzôs forma: Halál tavabeli, Méz tengerebeli, Rothadás mocsarabeli, Szivárvány öblebeli