DOCSLIB.ORG

Oil Team Is Off to the Moon BULLETIN the Rocket and Spacecraft, Are to Detach the Fragile, Spi- You-Very Much

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Oil Team Is Off to the Moon BULLETIN the Rocket and Spacecraft, Are to Detach the Fragile, Spi- You-Very Much Change of Command Set at Ft. Monmouth SEE STORY BEL0F Hot and Humid Sunny, hot and humid "today. FINAL Clear, warm tonight. Sunny Red Bank, Freehold and humid tomorrow. 7 Long Branch EDITION (Sea Details, Page 31 ' Monmouth County's Home Newspaper for 92 Years VOL. 93, NO. 13 RED BANK, N. J., WEDNESDAY, JULY 16, 1969 24'PAGES 10 CENTS iiiiiiniiiiiiliiiliiiiiiliiiiiiiiiiii iiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiiii Oil Team Is Off to the Moon BULLETIN The rocket and spacecraft, are to detach the fragile, spi- you-very much. We know it- When the computer sensed CAPE KENNEDY, Fla. 363 feet tall on the launch der-like lunar module from will be a good flight." . all was right, it commanded (AP)—Reaching for a dream, pad, lifted off from a space- the command ship and ride Pushing Apollo 11 • toward four 40,000-pound steel re- the Apollo 11 astronauts port area jammed with hun- it to the moon's surface. Ear-.. earth'orbit, the 3,817-ton Sat-a straining arms to flip back rocketed from earth today to dreds of thousands of visitors ly the nekt day, they are to „ urn 5 roared to. life, punish- * to the pulsating giant. - . make man's first attempt to eager for a glimpse of the ad- walk on the moon, fulfilling ing its launch pedestal,-with With agonizing •<. slown.ess land on the moon. venture's blazing start. a centuries-old dream, of a dazzling sheet of flame. the Saturn 5 climbed on a For three .days, the- astro- mankind.' The rocket screamed on its wide pillar of fire, gradually ^ A. Armstrong, Air nauts will soar outward on a Paul' Donley, test con- pad for 8-9 seconds as a. picking, up speed as its hun- Force Col. Edwin 13: Aldrin quarter-million-mile voyage ductor, told the astronauts computer system made cer- gry powerplant gulped fuel Jr. and Air Force Lt. Col. Mi- through space and then fire tain' all five booster engines' at the rate of 15 tons a sec- just before launch, "Good chael Collins rode a Saturn 5 themselves into orbit 69 miles reached full thrust of 7.7 ond. rocket into space at 9:32 a.m. above the lunar surface. luck and Godspeed from the million pounds T more pow- After 12 seconds, the guid- EDT to start the epic jour- On Sunday afternoon, Arm- launch crew." • erful than 92,000 locomo- ance system tipped the rock- ney. ' • strong and "Buzz" Aldrin Armstrong replied! "Thank tives or 500,000 automobiles. (See APOLLO, Pg. 3, Col. 3) LBJ Among 500 VIPs AIMING FOR THE MOON — Three U. S. astronauts who started their historic flight to the moon today are shown in their space suits. They ara, from left, Edwin 'Like First Baby' Aldrin, Michaj>JL^ollrnjjand_jj<jLArmstr<)ng. ' (AP Wirephoto) -CAPE -KENNEDY-r—Ha,—flational-^Aeranautics and high spwuting on space ex- . (AP) - "It's kind of like Space Administration. ploration compared to anti- standing around the hospital Ngt all the VIPs had hous- poverty programs. room before your first baby ing in the immediate vicinity Paine promised Abernathy is bom," fprmer President of this Cape midway down 10 VIP passes and said if it es Buzz Lyndon B. Johnson said.as he • Florida's east coast. Dr. Lee would solve the problems of and 500 other special guests A. Dubridge,; President Nix- of the poor by withholding marked time.before the Apol- on's science adviser, stayed. the Apollo 11 shot no button lo 11 launching. overnight in Orlando, SO miles would be pushed, but it "You must be prepared to away. wasn't.that simple. ' accept the worst, but you Sixty-nine ambassadors of President Nixon wasn't hope for the best," Johnson foreign governments fly in here to join the 40 mayors, 19 explained. this morning, as do manyv governors and 275 U.S. busi- BRIELLE r- The father seen him in months." said ifo his son when he saw Vice President Spiro Ag- other visitors. ness leaders on the VIP list, ARTIST'S CONCEPTION OF ASTRONAUT ON MOON of .astronaut Edwin "Buzz" Col. Edwin E. Aldrin Sn, him for lunch at Cape Ken- new, like Johnson, arrived in Ten representatives of the but he telephoned best wishes — This drawing from Grumman Aerospace Corp. de- Aldrin Jr., scheduled to take 73, a retired Air Force pio- nedy, Fla., Sunday, were the jam-packed Cape Ken- "Poor Peoples Campaign" of to astronauts Neil Armstrong, part to the Apollo 11 moon neer, said he plans to watch "God bless you." He saiijie nedy area on the eve of the the Rev. Ralph' David Aber- Michael Collins and Edwin picts Apollo 11 astronaut Neil Armstrong taking his shot, Said yesterday the last the launch on television at does not plan to -talk to his flight to the moon and at- nathy were added to the VIP Aldrin Jr. first step on the moon after descending by ladder time he saw his son he was his home or at a friend's. son again until after the Apol- tended a private dinner party list after a .meeting with. Nixon originally was to from the lunar module. In the background is tbe "more relaxed than I have He Said the-last words he lo 11 flight. given by Dr., Thomas O. Paine. —Irave^ined-with-the Apolk>4i ~fartrn (AP Wirepihoto DrawingL The elder Aldrin told a Paine, administrator of the £hey protested the nation's (See VIP'S, Pg. 2, Col. 4 news conference that he wiH not be worried about most of the mission, only the descent NqtJhing Prepares to the moon's surface and the Latta and Lotz Swapping Commands return to the command mod- ule. , A Wife for This "From there it should be like taking a taxi .back By HARRY F. ROSENTHAL the space-made communities home," he said. SPACE CENTER, Houston of Nassau Bay and Seabrook Aldrin and astronaut Neil (AP) — Nothing ever pre- and Clear Lake and El Lago. .A. Armstrong are scheduled FT. MONMOUTH - Two of uation from the U.S. Military Lotz served in Vietnam as pared a wife for a time such And as an electronic clock to set foot on the moon while the Army's top communica- Academy, serving in that as- Assistant Chief of Staff for as this. 1,040 miles away at Cape astronaut Michael Collins re- tors will swap jobs in early signment from September, Communications - Electronics, Not Jan Armstrong, who Kennedy, Fla., strangely mains in the command mod- September, the Department 1938 to September, 1939. Gen. U.S. Military Assisfance Com- understood that "Neil wanted counts backward to zero, ule. of the Army announced yes- Lotz is a former deputy com- mand. tojflevaUfhis life Jo what he's there'suddenly are no kids on The elder Aldrin added.that terday. manding general of ECOM. He is the former deputy doing now." the street and no housewives afterHie Apollo 11 flight, U.S. Maj. Gen.-William B.iat- Gen_JLotz, .ene of _ the Ar- . commander of the Army Not Jean Aldrin, who going for the paper or a officials will have to decide ta, commanding generaLof. my's, highest educated com- pe^rc^cJ^ov|ng_Ground at whether, they want to "slide learned on the amateur stage street chat, and newsmen the Army Electronics Com- munications specialists, hold's Ft Huachuca, assuming his back and let someone else be to lose her own identity. wait outside three homes to mand and Ft. Monmouth, a master's degree in commu- duties there in 1959 following the .number one'space power nications engineering and a service in Korea and Hawaii, Not Pat Collins, when she hear what the wives have to in the world.'! ' will become the commanding say when the clock-Smarts go- doctorate in physics. He where he was the Signal Of- promised, like women the Aldrin, adding that there general of the Strategic Com- world over, "to have and to ing forward and everything munications Command earned his master's degree at ficer for the 8th U.S. Army was no "generation gap" be- the University of Illinois and and the U.S. Army Forces hold from this day forward is well. tween himself and his son, (STRATCOM) and Ft. Hua- the doctorate from the Uni- Pacific, respectively. • • • Jan and Jean and Pat all said he did not know if his chuca, Ariz., replacing Maj. versity of Virginia. They have lived with it for have gone through it before. son and Armstrong planned Gen. Walter E. Lotz Jr., who At Ft. Huachuca, he served ' years, this fantasy that one But nothing ever prepared a to say anything special upon will take command of ECOM A native of Pennsylvania, for three years as Chief of day man will go to the moon. • wife for a time, such as this. setting foot on the moon. and this fort. he had served as Chief of the the Electronic Warfare De- This was the day. The men "Gemini was the end of He said they may have Maj. Gen. Latta and Maj. Army's Communications- partment, director of the Sys- were their men. something," said Jean Al- planned to say something, Gen. Lotz were classmates in Electronics in the Pentagon. tems Development Director- Astronaut homes cluster drin, whose. "Buzz" was on but joked, "Well, I made the 1938 at the U.S. Military He has been the. commander ate and deputy commander. around the Lakeland area* the last flight of that series remark that he might say Aaademy. Both joined the of STRATCOM since Jan.
Load more

Recommended publications
  • Columbus Crater HLS2 Hangout: Exploration Zone Briefing
    Columbus Crater HLS2 Hangout: Exploration Zone Briefing Kennda Lynch1,2, Angela Dapremont2, Lauren Kimbrough2, Alex Sessa2, and James Wray2 1Lunar and Planetary Institute/Universities Space Research Association 2Georgia Institute of Technology Columbus Crater: An Overview • Groundwater-fed paleolake located in northwest region of Terra Sirenum • ~110 km in diameter • Diversity of Noachian & Hesperian aged deposits and outcrops • High diversity of aqueous mineral deposits • Estimated 1.5 km depth of sedimentary and/or volcanic infill • High Habitability and Biosignature Preservation Potential LZ & Field Station Latitude: 194.0194 E Longitude: 29.2058 S Altitude: +910 m SROI #1 RROI #1 LZ/HZ SROI #4 SROI #2 SROI #5 22 KM HiRISE Digital Terrain Model (DTM) • HiRISE DTMs are made from two images of the same area on the ground, taken from different look angles (known as a stereo-pair) • DTM’s are powerful research tools that allow researchers to take terrain measurements and model geological processes • For our traversability analysis of Columbus: • The HiRISE DTM was processed and completed by the University of Arizona HiRISE Operations Center. • DTM data were imported into ArcMap 10.5 software and traverses were acquired and analyzed using the 3D analyst tool. • A slope map was created in ArcMap to assess slope values along traverses as a supplement to topography observations. Slope should be ≤30°to meet human mission requirements. Conclusions Traversability • 9 out of the 17 traverses analyzed met the slope criteria for human missions. • This region of Columbus Crater is traversable and allows access to regions of astrobiological interest. It is also a possible access point to other regions of Terra Sirenum.
    [Show full text]
  • Identification of Volcanic Rootless Cones, Ice Mounds, and Impact 3 Craters on Earth and Mars: Using Spatial Distribution As a Remote 4 Sensing Tool
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, XXXXXX, doi:10.1029/2005JE002510, 2006 Click Here for Full Article 2 Identification of volcanic rootless cones, ice mounds, and impact 3 craters on Earth and Mars: Using spatial distribution as a remote 4 sensing tool 1 1 1 2 3 5 B. C. Bruno, S. A. Fagents, C. W. Hamilton, D. M. Burr, and S. M. Baloga 6 Received 16 June 2005; revised 29 March 2006; accepted 10 April 2006; published XX Month 2006. 7 [1] This study aims to quantify the spatial distribution of terrestrial volcanic rootless 8 cones and ice mounds for the purpose of identifying analogous Martian features. Using a 9 nearest neighbor (NN) methodology, we use the statistics R (ratio of the mean NN distance 10 to that expected from a random distribution) and c (a measure of departure from 11 randomness). We interpret R as a measure of clustering and as a diagnostic for 12 discriminating feature types. All terrestrial groups of rootless cones and ice mounds are 13 clustered (R: 0.51–0.94) relative to a random distribution. Applying this same 14 methodology to Martian feature fields of unknown origin similarly yields R of 0.57–0.93, 15 indicating that their spatial distributions are consistent with both ice mound or rootless 16 cone origins, but not impact craters. Each Martian impact crater group has R 1.00 (i.e., 17 the craters are spaced at least as far apart as expected at random). Similar degrees of 18 clustering preclude discrimination between rootless cones and ice mounds based solely on 19 R values.
    [Show full text]
  • Geologic Map of Mars 1: 600 000 Gusev Crater Region M 600K 14.00S/175.50E G
    Geologic Map of Mars 1: 600 000 Gusev Crater Region M 600k 14.00S/175.50E G GEOLOGIC UNITS 188°00’ West 187°30’ 187°00’ 186°30’ 186°00’ 185°30’ 185°00’ 184°30’ 184°00’ 183°30’ 183°00’ 182°30’ 182°00’ 181°30’ 181°00’ West 172°00’ East 172°30’ 173°00’ 173°30’ 174°00’ 174°30’ 175°00’ 175°30’ 176°00’ 176°30’ 177°00’ 177°30’ 178°00’ 178°30’ 179°00’ East -10°00’ -10°00’ Highlands -10°07’ A -10°07’ v Modified Gusev highland formation (MGHf) e r n Durius formation (Df) u -10°30’ -10°30’ s Gusev highland formation (GHf) -10°30’ R -10°30’ Himalaya formation (Hf) u p Lowlands e s A p o l l i n a r i s P a t e r a Suici formation (2) (Sf2) -11°00’ -11°00’ Suici formation (1) (Sf1) -11°00’ Zutphen Galdakao formation (ZGf) Death Valley formation (DVf) A p o l l i n a r i s S u l c i Bermuda formation (Bf) -11°30’ -11°30’ Z e p h y r i a M e n s a e -11°30’ -11°30’ Apollinaris formation (Af) Vaucouleurs formation-mesas (Vfm) Vaucouleurs formation (1) (Vf1) -12°00’ -12°00’ Vaucouleurs formation (2) (Vf2) -12°00’ -12°00’ Gusev Crater Gusev Crivitz formation (GCf) Ma'adim Vallis formation (MVf) -12°30’ -12°30’ Manhattan formation (Mf) -12°30’ -12°30’ Thira formation(Tf) Paris formation (Pf) -13°00’ -13°00’ Zandfoort formation (Zf) Gusev rim formation (Grf) -13°00’ -13°00’ Features G a l d a k a o Groove -13°30’ -1330’ Ridge -13°30’ Channel Crater rim d e V a u c o u l e u r s Degraded, buried crater rim -14°00’ -14°00’ Z u t p h e n Central peak of impact crater -14°00’ -14°00’ Landslide G u s e v Contacts Certain -14°30’ -14°30’ Approximate T h i r a -14°30’
    [Show full text]
  • Sundayiournal
    STANDING STRONG FOR 1,459 DAYS — THE FIGHT'S NOT OVER YET JULY 11-17, 1999 THE DETROIT VOL. 4 NO. 34 75 CENTS S u n d a yIo u r n a l PUBLISHED BY LOCKED-OUT DETROIT NEWSPAPER WORKERS ©TDSJ JIM WEST/Special to the Journal Nicholle Murphy’s support for her grandmother, Teamster Meka Murphy, has been unflagging. Marching fourward Come Tuesday, it will be four yearsstrong and determined. In this editionOwens’ editorial points out the facthave shown up. We hope that we will since the day in July of 1995 that ofour the Sunday Journal, co-editor Susanthat the workers are in this strugglehave contracts before we have to put Detroit newspaper unions were forcedWatson muses on the times of happi­until the end and we are not goingtogether any­ another anniversary edition. to go on strike. Although the compa­ness and joy, in her Strike Diarywhere. on On Pages 19-22 we show offBut four years or 40, with your help, nies tried mightily, they never Pagedid 3. Starting on Page 4, we putmembers the in our annual Family Albumsolidarity and support, we will be here, break us. Four years after pickingevents up of the struggle on the record.and also give you a glimpse of somestanding of strong. our first picket signs, we remainOn Page 10, locked-out worker Keiththe far-flung places where lawn signs— Sunday Journal staff PAGE 10 JULY 11 1999 Co-editors:Susan Watson, Jim McFarlin --------------------- Managing Editor: Emily Everett General Manager: Tom Schram Published by Detroit Sunday Journal Inc.
    [Show full text]
  • Distribution of Rocks on the Gusev Plains and on Husband Hill, Mars J
    GEOPHYSICAL RESEARCH LETTERS, VOL. 33, L16202, doi:10.1029/2006GL026964, 2006 Click Here for Full Article Distribution of rocks on the Gusev Plains and on Husband Hill, Mars J. A. Grant,1 S. A. Wilson,1 S. W. Ruff,2 M. P. Golombek,3 and D. L. Koestler4 Received 19 May 2006; revised 12 July 2006; accepted 21 July 2006; published 29 August 2006. [1] The population of rocks larger than 15 cm in diameter al., 2000, Greeley et al., 2005], but perhaps Noachian) was measured at 36 locations imaged by the Spirit rover and of uncertain origin [Squyres et al., 2006; Arvidson et al., over 4 km of the traverse across the Gusev plains and 2006]. We examined the rock population of the surfaces at Husband Hill in Gusev crater on Mars. The rock population regular intervals along the traverse of the Spirit rover observed on plains surfaces is consistent with impact (Figure 1) to determine whether there was any significant fragmentation of rubbly/fractured volcanics and reveals variability among presumably different geomorphic surfa- little evidence for modification by secondary processes or ces that might reflect a fluvial/alluvial contribution to the weathering. Interpretation of counts from Husband Hill impact-derived blocks and/or modification by weathering or suggest an influence by bedrock for rocks larger than 0.5 m alternate geomorphic processes. across, but the distribution of smaller rocks is consistent with ejecta possessing contributions from pre-plains impact 2. Measuring the Rock Population events. Results indicate plains surfaces experienced only tens of centimeters of eolian erosion/deposition since the [4] The rock population was characterized by measuring Hesperian, whereas meters rather than tens of meters of the maximum visible axis of all rocks larger than 15 cm at erosion modified Husband Hill since the early Hesperian.
    [Show full text]
  • Geologic Mapping of Gusev Crater, Mars: Gusev Rim and Floor Characteristics
    Planetary Geologic Mappers 2021 (LPI Contrib. No. 2610) 7020.pdf GEOLOGIC MAPPING OF GUSEV CRATER, MARS: GUSEV RIM AND FLOOR CHARACTERISTICS. David A. Crown1, Frank C. Chuang1, James W. Rice1, Steven W. Ruff2, and Stephen P. Scheidt1,3,4, 1Planetary Science Institute, 1700 E. Ft. Lowell Rd., Suite 106, Tucson, AZ 85719 ([email protected]), 2Arizona State University, Tempe, AZ 85287, 3Howard University, Washington, DC 20059, 4Center for Research & Exploration in Space Science and Technology, Greenbelt, MD 20771. Introduction: The geologic complexity of Gusev the crater floor. crater (~160 km diameter; 14.53°S, 175.52°E) and its Gusev Crater Floor: Gusev floor materials have surroundings have been revealed through orbital been attributed to aeolian deposits overlying lava flows remote sensing coupled with in situ exploration of the [11]; mass-wasting and channel deposits [12]; fluvio- Columbia Hills and adjacent volcanic plains by the lacustrine deposits [6-7]; and basaltic lava flows [8, MER Spirit rover [e.g., 1-4]. Gusev crater’s geologic 13-15]. Although Spirit confirmed the presence of history has been attributed to the combined effects of a basalt, questions remain regarding the overall geologic variety of geologic processes that span much of evolution of Gusev. Martian history. We have initiated a new geologic Figure 1 shows our preliminary geologic map of mapping investigation of Gusev crater, designed to Gusev floor materials. Using 5-6 m/pixel CTX images, produce a 1:250K-scale, formal geologic map focused we have identified eight geologic units, including: two on the geologic evolution of the Gusev rim and floor ridged volcanic plains, Ma’adim debris flow, dissected (Figures 1-3).
    [Show full text]
  • Columbus Crater HLS2 Hangout: Exploration Zone Briefing
    Columbus Crater HLS2 Hangout: Exploration Zone Briefing Kennda Lynch1,2, Angela Dapremont2, Lauren Kimbrough2, Alex Sessa2, and James Wray2 1Lunar and Planetary Institute/Universities Space Research Association 2Georgia Institute of Technology Columbus Crater: An Overview • Groundwater-fed paleolake located in northwest region of Terra Sirenum • ~110 km in diameter • Diversity of Noachian & Hesperian aged deposits and outcrops • High diversity of aqueous mineral deposits • Estimated 1.5 km depth of sedimentary and/or volcanic infill • High Habitability and Biosignature Preservation Potential LZ & Field Station Latitude: 194.0194 E Longitude: 29.2058 S Altitude: +910 m SROI #1 RROI #1 LZ/HZ SROI #4 SROI #2 SROI #5 22 KM HiRISE Digital Terrain Model (DTM) • HiRISE DTMs are made from two images of the same area on the ground, taken from different look angles (known as a stereo-pair) • DTM’s are powerful research tools that allow researchers to take terrain measurements and model geological processes • For our traversability analysis of Columbus: • The HiRISE DTM was processed and completed by the University of Arizona HiRISE Operations Center. • DTM data were imported into ArcMap 10.5 software and traverses were acquired and analyzed using the 3D analyst tool. • A slope map was created in ArcMap to assess slope values along traverses as a supplement to topography observations. Slope should be ≤30°to meet human mission requirements. Conclusions Traversability • 9 out of the 17 traverses analyzed met the slope criteria for human missions. • This region of Columbus Crater is traversable and allows access to regions of astrobiological interest. It is also a possible access point to other regions of Terra Sirenum.
    [Show full text]
  • Chapter Vi Report of Divisions, Commissions, and Working
    CHAPTER VI REPORT OF DIVISIONS, COMMISSIONS, AND WORKING GROUPS Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.42, on 24 Sep 2021 at 09:23:58, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0251107X00011937 DIVISION I FUNDAMENTAL ASTRONOMY Division I provides a focus for astronomers studying a wide range of problems related to fundamental physical phenomena such as time, the intertial reference frame, positions and proper motions of celestial objects, and precise dynamical computation of the motions of bodies in stellar or planetary systems in the Universe. PRESIDENT: P. Kenneth Seidelmann U.S. Naval Observatory, 3450 Massachusetts Ave NW Washington, DC 20392-5100, US Tel. + 1 202 762 1441 Fax. +1 202 762 1516 E-mail: [email protected] BOARD E.M. Standish President Commission 4 C. Froeschle President Commisison 7 H. Schwan President Commisison 8 D.D. McCarthy President Commisison 19 E. Schilbach President Commisison 24 T. Fukushima President Commisison 31 J. Kovalevsky Past President Division I PARTICIPATING COMMISSIONS: COMMISSION 4 EPHEMERIDES COMMISSION 7 CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY COMMISSION 8 POSITIONAL ASTRONOMY COMMISSION 19 ROTATION OF THE EARTH COMMISSION 24 PHOTOGRAPHIC ASTROMETRY COMMISSION 31 TIME Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.42, on 24 Sep 2021 at 09:23:58, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0251107X00011937 COMMISSION 4: EPHEMERIDES President: H. Kinoshita Secretary: C.Y. Hohenkerk Commission 4 held one business meeting.
    [Show full text]
  • APP Notes Programs
    Blue iPods are 6th Generation, iOS 11.3 VR Resources Detailed List- TEACHERS Silver iPods are 5th Generation, iOS 9.1 updated 10/27/2017 APP Notes Operating Programs systems Bosch VR Paintings- Hieronymus Bosch iOS 8.0; Go inside the “Garden of Earthly Delights.” Android Note: the other paintings are fee-based. Brastours Ancient Rome tours iOS 8.0 or later; Tour ancient Rome- uses a map of Rome with icons to launch the Android VR. Includes the Forum, the Coliseum, Circus Maximus & Palatine Hill; Navigate using device, select VR mode at the locations. Cardboard Introductory VRs iOS 8.0 or later; Launch Cardboard demos. Includes: Android Tutorial Explorer- toggle through a series of 360 photospheres, Exhibit – toggle through a series of sculpted masks Urban Hike- toggle through 360 photospheres of major cities Kaleidoscope – colorful kaleidoscopic patterns Arctic Journey- Fly through the arctic like a bird. Cardboard Create your own 360 iOS 9.0 or later; Document your location in a 360 photosphere. photospheres. Android camera Discovery VR Many different VR shows iOS 9.1 or later; See Appendix A Available in 360 Android Eon Short, CG VRs, many with iOS 7.0 or later; Education Tab computer narration; Android Magi Chapel (voice okay) Some are available in 360. King Tut (computer voice) Neferititi (computer voice) Machu Picchu (computer voice) Edutainment tab: Egypt 360 Expeditions Teacher driven field trips. iOS 8.0 or later; Inclusive of many curricula; Available in 360. Android See Appendix B 1 Blue iPods are 6th Generation, iOS 11.3 VR Resources Detailed List- TEACHERS Silver iPods are 5th Generation, iOS 9.1 updated 10/27/2017 Google Street Works adequately in VR; iOS 9.0 or later; “Walk” through the streets of cities and towns around the View Works best in 360.
    [Show full text]
  • Ebook < Impact Craters on Mars # Download
    7QJ1F2HIVR # Impact craters on Mars « Doc Impact craters on Mars By - Reference Series Books LLC Mrz 2012, 2012. Taschenbuch. Book Condition: Neu. 254x192x10 mm. This item is printed on demand - Print on Demand Neuware - Source: Wikipedia. Pages: 50. Chapters: List of craters on Mars: A-L, List of craters on Mars: M-Z, Ross Crater, Hellas Planitia, Victoria, Endurance, Eberswalde, Eagle, Endeavour, Gusev, Mariner, Hale, Tooting, Zunil, Yuty, Miyamoto, Holden, Oudemans, Lyot, Becquerel, Aram Chaos, Nicholson, Columbus, Henry, Erebus, Schiaparelli, Jezero, Bonneville, Gale, Rampart crater, Ptolemaeus, Nereus, Zumba, Huygens, Moreux, Galle, Antoniadi, Vostok, Wislicenus, Penticton, Russell, Tikhonravov, Newton, Dinorwic, Airy-0, Mojave, Virrat, Vernal, Koga, Secchi, Pedestal crater, Beagle, List of catenae on Mars, Santa Maria, Denning, Caxias, Sripur, Llanesco, Tugaske, Heimdal, Nhill, Beer, Brashear Crater, Cassini, Mädler, Terby, Vishniac, Asimov, Emma Dean, Iazu, Lomonosov, Fram, Lowell, Ritchey, Dawes, Atlantis basin, Bouguer Crater, Hutton, Reuyl, Porter, Molesworth, Cerulli, Heinlein, Lockyer, Kepler, Kunowsky, Milankovic, Korolev, Canso, Herschel, Escalante, Proctor, Davies, Boeddicker, Flaugergues, Persbo, Crivitz, Saheki, Crommlin, Sibu, Bernard, Gold, Kinkora, Trouvelot, Orson Welles, Dromore, Philips, Tractus Catena, Lod, Bok, Stokes, Pickering, Eddie, Curie, Bonestell, Hartwig, Schaeberle, Bond, Pettit, Fesenkov, Púnsk, Dejnev, Maunder, Mohawk, Green, Tycho Brahe, Arandas, Pangboche, Arago, Semeykin, Pasteur, Rabe, Sagan, Thira, Gilbert, Arkhangelsky, Burroughs, Kaiser, Spallanzani, Galdakao, Baltisk, Bacolor, Timbuktu,... READ ONLINE [ 7.66 MB ] Reviews If you need to adding benefit, a must buy book. Better then never, though i am quite late in start reading this one. I discovered this publication from my i and dad advised this pdf to find out. -- Mrs. Glenda Rodriguez A brand new e-book with a new viewpoint.
    [Show full text]
  • Meter-Scale Slopes of Candidate MER Landing Sites from Point Photoclinometry Ross A
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 108, NO. E12, 8085, doi:10.1029/2003JE002120, 2003 Meter-scale slopes of candidate MER landing sites from point photoclinometry Ross A. Beyer and Alfred S. McEwen Department of Planetary Sciences, University of Arizona, Tucson, Arizona, USA Randolph L. Kirk Astrogeology Team, U.S. Geological Survey, Flagstaff, Arizona, USA Received 13 May 2003; revised 16 July 2003; accepted 22 August 2003; published 4 December 2003. [1] Photoclinometry was used to analyze the small-scale roughness of areas that fall within the proposed Mars Exploration Rover (MER) 2003 landing ellipses. The landing ellipses presented in this study were those in Athabasca Valles, Elysium Planitia, Eos Chasma, Gusev Crater, Isidis Planitia, Melas Chasma, and Meridiani Planum. We were able to constrain surface slopes on length scales comparable to the image resolution (1.5 to 12 m/pixel). The MER 2003 mission has various engineering constraints that each candidate landing ellipse must satisfy. These constraints indicate that the statistical slope values at 5 m baselines are an important criterion. We used our technique to constrain maximum surface slopes across large swaths of each image, and built up slope statistics for the images in each landing ellipse. We are confident that all MER 2003 landing site ellipses in this study, with the exception of the Melas Chasma ellipse, are within the small-scale roughness constraints. Our results have provided input into the landing hazard assessment process. In addition to evaluating the safety of the landing sites, our mapping of small-scale roughnesses can also be used to better define and map morphologic units.
    [Show full text]
  • Collection of Research Materials for the HBO Television Series, from the Earth to the Moon, 1940-1997, Bulk 1958-1997
    http://oac.cdlib.org/findaid/ark:/13030/kt8290214d No online items Finding Aid for the Collection of Research Materials for the HBO Television Series, From the Earth to the Moon, 1940-1997, bulk 1958-1997 Processed by Manuscripts Division staff; machine-readable finding aid created by Caroline Cubé © 2004 The Regents of the University of California. All rights reserved. 561 1 Finding Aid for the Collection of Research Materials for the HBO Television Series, From the Earth to the Moon, 1940-1997, bulk 1958-1997 Collection number: 561 UCLA Library, Department of Special Collections Manuscripts Division Los Angeles, CA Processed by: Manuscripts Division staff, 2004 Encoded by: Caroline Cubé © 2004 The Regents of the University of California. All rights reserved. Descriptive Summary Title: Collection of Research Materials for the HBO Television Series, From the Earth to the Moon, Date (inclusive): 1940-1997, bulk 1958-1997 Collection number: 561 Creator: Home Box Office (Firm) Extent: 86 boxes (43 linear ft.) Repository: University of California, Los Angeles. Library. Dept. of Special Collections. Los Angeles, California 90095-1575 Abstract: From the earth to the moon was a Clavius Base/Imagine Entertainment production that followed the experiences of the Apollo astronauts in their mission to place a man on the moon. The collection covers a variety of subjects related to events and issues of the United States manned space flight program through Project Apollo and the history of the decades it covered, primarily the 1960s and the early 1970s. The collection contains books, magazines, unidentified excerpts from books and magazines, photographs, videorecordings, glass slides and audiotapes.
    [Show full text]