Galactic Observer December 2012
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Geologic Structure of Shallow Maria
NASA CR. Photo Data Analysis S-221 NASA Contract NAS 9-13196 GEOLOGIC STRUCTURE OF SHALLOW MARIA Rene' A. De Hon, Principal Investigator John A. Waskom, Co-Investigator (NASA-CR-lq7qoo GEOLOGIC STahJCTUnF OF N76-17001 ISBALOW M1BIA-'(Arkansas Uni.v., mHiticelio.) 96 p BC $5.00' CSCL O3B Unclas G3/91, 09970- University of Arkansas at Monticello Monticello, Arkansas December 1975 Photo Data Analysis S-221 NASA Contract NAS 9-13196 GEOLOGIC STRUCTURE OF SHALLOW MARIA Rene' A. De Hon, Principal Investigator I John A. Waskom, Co-Investigator Un-iversity-of Arkansas-:at-.Monticl o Monticello, Arkansas December 1975 ABSTRACT Isopach maps and structural contour maps of the 0 0 eastern mare basins (30 N to 30 OS; 00 to 100 E) are constructed from measurements of partially buried craters. The data, which are sufficiently scattered to yield gross thickness variations, are restricted to shallow maria with less than 1500-2000 m of mare basalts. The average thickness of b-asalt in the irregular maria is between 200 and 400 m. Multiringed mascon basins are filled to various levels. The Serenitatis and Crisium basins have deeply flooded interiors and extensively flooded shelves. Mare basalts in the Nectaris basin fill only the innermost basin, and mare basalts in the Smythii basin occupy a small portion of the basin floor. Sinus Amoris, Mare Spumans, and Mare Undarum are partially filled troughs concentric to large circular basins. The Tranquillitatis and Fecunditatis are composite depressions containing basalts which flood degraded circular basins and adjacent terrain modified by the formation of nearby cir cular basins. -
Go for Lunar Landing Conference Report
CONFERENCE REPORT Sponsored by: REPORT OF THE GO FOR LUNAR LANDING: FROM TERMINAL DESCENT TO TOUCHDOWN CONFERENCE March 4-5, 2008 Fiesta Inn, Tempe, AZ Sponsors: Arizona State University Lunar and Planetary Institute University of Arizona Report Editors: William Gregory Wayne Ottinger Mark Robinson Harrison Schmitt Samuel J. Lawrence, Executive Editor Organizing Committee: William Gregory, Co-Chair, Honeywell International Wayne Ottinger, Co-Chair, NASA and Bell Aerosystems, retired Roberto Fufaro, University of Arizona Kip Hodges, Arizona State University Samuel J. Lawrence, Arizona State University Wendell Mendell, NASA Lyndon B. Johnson Space Center Clive Neal, University of Notre Dame Charles Oman, Massachusetts Institute of Technology James Rice, Arizona State University Mark Robinson, Arizona State University Cindy Ryan, Arizona State University Harrison H. Schmitt, NASA, retired Rick Shangraw, Arizona State University Camelia Skiba, Arizona State University Nicolé A. Staab, Arizona State University i Table of Contents EXECUTIVE SUMMARY..................................................................................................1 INTRODUCTION...............................................................................................................2 Notes...............................................................................................................................3 THE APOLLO EXPERIENCE............................................................................................4 Panelists...........................................................................................................................4 -
Through Astronaut Eyes: Photographing Early Human Spaceflight
Purdue University Purdue e-Pubs Purdue University Press Book Previews Purdue University Press 6-2020 Through Astronaut Eyes: Photographing Early Human Spaceflight Jennifer K. Levasseur Follow this and additional works at: https://docs.lib.purdue.edu/purduepress_previews This document has been made available through Purdue e-Pubs, a service of the Purdue University Libraries. Please contact [email protected] for additional information. THROUGH ASTRONAUT EYES PURDUE STUDIES IN AERONAUTICS AND ASTRONAUTICS James R. Hansen, Series Editor Purdue Studies in Aeronautics and Astronautics builds on Purdue’s leadership in aeronautic and astronautic engineering, as well as the historic accomplishments of many of its luminary alums. Works in the series will explore cutting-edge topics in aeronautics and astronautics enterprises, tell unique stories from the history of flight and space travel, and contemplate the future of human space exploration and colonization. RECENT BOOKS IN THE SERIES British Imperial Air Power: The Royal Air Forces and the Defense of Australia and New Zealand Between the World Wars by Alex M Spencer A Reluctant Icon: Letters to Neil Armstrong by James R. Hansen John Houbolt: The Unsung Hero of the Apollo Moon Landings by William F. Causey Dear Neil Armstrong: Letters to the First Man from All Mankind by James R. Hansen Piercing the Horizon: The Story of Visionary NASA Chief Tom Paine by Sunny Tsiao Calculated Risk: The Supersonic Life and Times of Gus Grissom by George Leopold Spacewalker: My Journey in Space and Faith as NASA’s Record-Setting Frequent Flyer by Jerry L. Ross THROUGH ASTRONAUT EYES Photographing Early Human Spaceflight Jennifer K. -
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. -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Apollo Space Suit
APOLLO SPACE S UIT 1962–1974 Frederica, Delaware A HISTORIC MECHANICAL ENGINEERING LANDMARK SEPTEMBER 20, 2013 DelMarVa Subsection Histor y of the Apollo Space Suit This model would be used on Apollo 7 through Apollo 14 including the first lunar mission of Neil Armstrong and Buzz International Latex Corporation (ILC) was founded in Aldrin on Apollo 11. Further design improvements were made to Dover, Delaware in 1937 by Abram Nathanial Spanel. Mr. Spanel improve mobility for astronauts on Apollo 15 through 17 who was an inventor who became proficient at dipping latex material needed to sit in the lunar rovers and perform more advanced to form bathing caps and other commercial products. He became mobility exercises on the lunar surface. This suit was known as famous for ladies apparel made under the brand name of Playtex the model A7LB. A slightly modified ILC Apollo suit would also go that today is known worldwide. Throughout WWII, Spanel drove on to support the Skylab program and finally the American-Soyuz the development and manufacture of military rubberized products Test Program (ASTP) which concluded in 1975. During the entire to help our troops. In 1947, Spanel used the small group known time the Apollo suit was produced, manufacturing was performed as the Metals Division to develop military products including at both the ILC plant on Pear Street in Dover, Delaware, as well as several popular pressure helmets for the U.S. Air Force. the ILC facility in Frederica, Delaware. In 1975, the Dover facility Based upon the success of the pressure helmets, the Metals was closed and all operations were moved to the Frederica plant. -
APOLLO 15 OBSERVATIONS; Farouk El-Baz, Lunar Explora- Tion Department, Bellcomm, Washington, D.C
APOLLO 15 OBSERVATIONS; Farouk El-Baz, Lunar Explora- tion Department, Bellcomm, Washington, D.C. 20024; A. M. Worden and V. D. Brand, Astronaut Office, Manned Spacecraft Center, Houston, Texas 77058 Visual observations from lunar orbit constitute a signif- icant complement to photography and other remote-sensed data. Utilization of the capabilities of a well-trained observer in lunar orbit is an illustration of the role of man in space flight. This is particularly significant when one considers the special characteristics of the human eye and the interpretive powers of the brain. The unaided eye resolves 20-30 m objects from 110 km orbit. It is also especially equipped, through its wide dynamic range, to distinguish subtle differences in bright- ness levels, color tones, topographic expressions and textural variations. Fifteen lunar surface areas were studied in detail from lunar orbit on Apollo 15. The wide field of view allowed in- vestigation of both the general and local settings at varying sun elevation angles and viewing directions. "On the scene" interpretations were made and later checked and confirmed on successive orbits. In certain cases, features and phenomena were compared to similar occurrences in other parts of the groundtracks. Results of the observation of eight targets are given and an example is provided of the geologic significance of observing cinder cones on the southeastern rim of Mare Serenitatis. The more significant observations were made of the following features starting with the most easterly target: 1) Swirls of light colored markings on the floor of Mare Inginii on the lunar farside. No topographic expressions are associated with these sinuous markings which appear to have been the result of a "bleaching" mechanism. -
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. -
W Numerze: – Wywiad Z Kustoszem Watykańskiej Kolekcji C.D. – Cz¹stki
KWARTALNIK MI£OŒNIKÓW METEORYTÓW METEORYTMETEORYT Nr 3 (63) Wrzesieñ 2007 ISSN 1642-588X W numerze: – wywiad z kustoszem watykañskiej kolekcji c.d. – cz¹stki ze Stardusta a meteorytry – trawienie meteorytów – utwory sp³ywania na Sikhote-Alinach – pseudometeoryty – konferencja w Tucson METEORYT Od redaktora: kwartalnik dla mi³oœników OpóŸnieniami w wydawaniu kolejnych numerów zaczynamy meteorytów dorównywaæ „Meteorite”, którego sierpniowy numer otrzyma³em Wydawca: w paŸdzierniku. Tym razem g³ówn¹ przyczyn¹ by³y k³opoty z moim Olsztyñskie Planetarium komputerem, ale w koñcowej fazie redagowania okaza³o siê tak¿e, i Obserwatorium Astronomiczne ¿e brak materia³u. Musia³em wiêc poczekaæ na mocno opóŸniony Al. Pi³sudskiego 38 „Meteorite”, z którego dorzuci³em dwa teksty. 10-450 Olsztyn tel. (0-89) 533 4951 Przeskok o jeden numer niezupe³nie siê uda³, a zapowiedzi¹ [email protected] dalszych k³opotów jest mi³y sk¹din¹d fakt, ¿e przep³yw materia³ów zacz¹³ byæ dwukierunkowy. W najnowszym numerze „Meteorite” konto: ukaza³ siê artyku³ Marcina Cima³y o Moss z „Meteorytu” 3/2006, 88 1540 1072 2001 5000 3724 0002 a w kolejnym numerze zapowiedziany jest artyku³ o Morasku BOŒ SA O/Olsztyn z „Meteorytu” 4/2006. W rezultacie jednak bêdzie mniej materia³u do Kwartalnik jest dostêpny g³ównie t³umaczenia i trzeba postaraæ siê o dalsze w³asne teksty. Czy mo¿e ktoœ w prenumeracie. Roczna prenu- merata wynosi w 2007 roku 44 z³. chcia³by coœ napisaæ? Zainteresowanych prosimy o wp³a- Z przyjemnoœci¹ odnotowujê, ¿e nabieraj¹ tempa przygotowania cenie tej kwoty na konto wydawcy do kolejnej konferencji meteorytowej, która planowana jest na 18—20 nie zapominaj¹c o podaniu czytel- nego imienia, nazwiska i adresu do kwietnia 2008 r. -
January 2015 BRAS Newsletter
January, 2015 Next Meeting: January 12th at 7PM at HRPO Artist concept of New Horizons. For more info on it and its mission to Pluto, click on the image. What's In This Issue? President's Message Astro Short: Wild Weather on WASP -43b Secretary's Summary Message From HRPO IYL and 20/20 Vision Campaign Recent BRAS Forum Entries Observing Notes by John Nagle President's Message Welcome to a new year. I can see lots to be excited about this year. First up are the Rockafeller retreat and Hodges Gardens Star Party. Go to our website for details: www.brastro.org Almost like a Christmas present from heaven, Comet Lovejoy C/2014 Q2 underwent a sudden brightening right before Christmas. Initially it was expected to be about magnitude 8 at its brightest but right after Christmas it became visible to the naked eye. At the time of this writing, it may become as bright as magnitude 4.5 or 4. As January progresses, the comet will move farther north, and higher in the sky for us. Now all we need is for these clouds to move out…. If any of you received (or bought yourself) any astronomical related goodies for Christmas and would like to show them off, bring them to the next meeting. Interesting geeky goodies qualify also, like that new drone or 3D printer. BRAS members are invited to a star party hosted by a group called the Lake Charles Free Thinkers. It will be January 24, 2015 from 3:00 PM on, at 5335 Hwy. -
PDF Document Download
“We choose to go to the moon ...” President John F. Kennedy’s commitment to landing an astronaut “on the Moon and returning him back safely to the Earth” was particularly audacious considering when he fi rst voiced the challenge, only one American had been in space for a grand total of 15 minutes and 28 seconds. Here is a look back at some of the milestones NASA and its astronauts reached on their way to the Moon. Learn more by visiting the John F. Kennedy Presidential 2 Library & Museum at www.jfklibrary.org 3 Only in the Sixties The Sixties could be described in words Charles To put President Kennedy’s proclamation in pers- Sadly, Gordon Cooper’s Faith 7 mission was the last Dickens had written just over a century before the pective, it is useful to remember that he made the of NASA’s manned space fl ights to take place in decade began: “It was the best of times, it was the speech only 16 months after America’s fi rst manned President Kennedy’s lifetime. worst of times ... “ space flight and seven months after John Glenn became the fi rst American to orbit the Earth. NASA’s While John F. Kennedy would not live to see his It was a time of stark contrasts. On one hand, it was four manned fl ights had each lasted less than fi ve dream realized, his challenge stimulated the imagi- an era of enormous political and social unrest. On the hours. In fact, NASA had only been established four nations of people from every nation and motivated other, it offered unparalleled scientifi c advancement years earlier. -
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.