What's New on the Moon?"
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Catalogue Pilot Film & Television Productions Ltd
productions 2020 Catalogue Pilot Film & Television Productions Ltd. is a leading international television production company with an outstanding reputation for producing and distributing innovative factual entertainment, history and travel led programmes. The company was set up by Ian Cross in 1988; and it is now one of the longest established independent production companies under continuous ownership in the United Kingdom. Pilot has produced over 500 hours of multi-genre programming covering subjects as diverse as history, food and sport. Its award winning Globe Trekker series, broadcast in over 20 countries, has a global audience of over 20 million. Pilot Productions has offices in London and Los Angeles. CONTENTS Mission Statement 3 In Production 4 New 6 Tough Series 8 Travelling in the 1970’s 10 Specials 11 Empire Builders 12 Ottomans vs Christians 14 History Specials 18 Historic Walks 20 Metropolis 21 Adventure Golf 22 Great Railway Journeys of Europe 23 The Story Of... Food 24 Bazaar 26 Globe Trekker Seasons 1-5 28 Globe Trekker Seasons 6-11 30 Globe Trekker Seasons 12-17 32 Globe Trekker Specials 34 Globe Trekker Around The World 36 Pilot Globe Guides 38 Destination Guides 40 Other Programmes 41 Short Form Content 42 DVDs and music CDs 44 Study Guides 48 Digital 50 Books 51 Contacts 52 Presenters 53 2 PILOT PRODUCTIONS 2020 MISSION STATEMENT Pilot Productions seeks to inspire and educate its audience by creating powerful television programming. We take pride in respecting and promoting social, environmental and personal change, whilst encouraging others to travel and discover the world. Pilot’s programmes have won more than 50 international awards, including six American Cable Ace awards. -
Bibliography
Annotated List of Works Cited Primary Sources Newspapers “Apollo 11 se Vraci na Zemi.” Rude Pravo [Czechoslovakia] 22 July 1969. 1. Print. This was helpful for us because it showed how the U.S. wasn’t the only ones effected by this event. This added more to our project so we had views from outside the US. Barbuor, John. “Alunizaron, Bajaron, Caminaron, Trabajaron: Proeza Lograda.” Excelsior [Mexico] 21 July 1969. 1. Print. The front page of this newspaper was extremely helpful to our project because we used it to see how this event impacted the whole world not just America. Beloff, Nora. “The Space Race: Experts Not Keen on Getting a Man on the Moon.” Age [Melbourne] 24 April 1962. 2. Print. This was an incredibly important article to use in out presentation so that we could see different opinions. This article talked about how some people did not want to go to the moon; we didn’t find many articles like this one. In most everything we have read it talks about the advantages of going to the moon. This is why this article was so unique and important. Canadian Press. “Half-billion Watch the Moon Spectacular.” Gazette [Montreal] 21 July 1969. 4. Print. This source gave us a clear idea about how big this event really was, not only was it a big deal in America, but everywhere else in the world. This article told how Russia and China didn’t have TV’s so they had to find other ways to hear about this event like listening to the radio. -
James Baldwin As a Writer of Short Fiction: an Evaluation
JAMES BALDWIN AS A WRITER OF SHORT FICTION: AN EVALUATION dayton G. Holloway A Dissertation Submitted to the Graduate School of Bowling Green State University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY December 1975 618208 ii Abstract Well known as a brilliant essayist and gifted novelist, James Baldwin has received little critical attention as short story writer. This dissertation analyzes his short fiction, concentrating on character, theme and technique, with some attention to biographical parallels. The first three chapters establish a background for the analysis and criticism sections. Chapter 1 provides a biographi cal sketch and places each story in relation to Baldwin's novels, plays and essays. Chapter 2 summarizes the author's theory of fiction and presents his image of the creative writer. Chapter 3 surveys critical opinions to determine Baldwin's reputation as an artist. The survey concludes that the author is a superior essayist, but is uneven as a creator of imaginative literature. Critics, in general, have not judged Baldwin's fiction by his own aesthetic criteria. The next three chapters provide a close thematic analysis of Baldwin's short stories. Chapter 4 discusses "The Rockpile," "The Outing," "Roy's Wound," and "The Death of the Prophet," a Bi 1 dungsroman about the tension and ambivalence between a black minister-father and his sons. In contrast, Chapter 5 treats the theme of affection between white fathers and sons and their ambivalence toward social outcasts—the white homosexual and black demonstrator—in "The Man Child" and "Going to Meet the Man." Chapter 6 explores the theme of escape from the black community and the conseauences of estrangement and identity crises in "Previous Condition," "Sonny's Blues," "Come Out the Wilderness" and "This Morning, This Evening, So Soon." The last chapter attempts to apply Baldwin's aesthetic principles to his short fiction. -
The Evolution of a Heterogeneous Martian Mantle: Clues from K, P, Ti, Cr, and Ni Variations in Gusev Basalts and Shergottite Meteorites
Earth and Planetary Science Letters 296 (2010) 67–77 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The evolution of a heterogeneous Martian mantle: Clues from K, P, Ti, Cr, and Ni variations in Gusev basalts and shergottite meteorites Mariek E. Schmidt a,⁎, Timothy J. McCoy b a Dept. of Earth Sciences, Brock University, St. Catharines, ON, Canada L2S 3A1 b Dept. of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560-0119, USA article info abstract Article history: Martian basalts represent samples of the interior of the planet, and their composition reflects their source at Received 10 December 2009 the time of extraction as well as later igneous processes that affected them. To better understand the Received in revised form 16 April 2010 composition and evolution of Mars, we compare whole rock compositions of basaltic shergottitic meteorites Accepted 21 April 2010 and basaltic lavas examined by the Spirit Mars Exploration Rover in Gusev Crater. Concentrations range from Available online 2 June 2010 K-poor (as low as 0.02 wt.% K2O) in the shergottites to K-rich (up to 1.2 wt.% K2O) in basalts from the Editor: R.W. Carlson Columbia Hills (CH) of Gusev Crater; the Adirondack basalts from the Gusev Plains have more intermediate concentrations of K2O (0.16 wt.% to below detection limit). The compositional dataset for the Gusev basalts is Keywords: more limited than for the shergottites, but it includes the minor elements K, P, Ti, Cr, and Ni, whose behavior Mars igneous processes during mantle melting varies from very incompatible (prefers melt) to very compatible (remains in the shergottites residuum). -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms. -
Chapter 12 the Moon and Mercury: Comparing Airless Worlds The
11/4/2015 The Moon: The View from Earth From Earth, we always see the same side of the moon. Moon rotates around its axis in the same time that it takes to orbit Chapter 12 around Earth: The Moon and Mercury: Tidal coupling: Earth’s gravitation has Comparing Airless Worlds produced tidal bulges on the moon; Tidal forces have slowed rotation down to same period as orbital period Lunar Surface Features Highlands and Lowlands Two dramatically Sinuous rilles = different kinds of terrain: remains of ancient • Highlands: lava flows Mountainous terrain, scarred by craters May have been lava • Lowlands: ~ 3 km lower than highlands; smooth tubes which later surfaces: collapsed due to Maria (pl. of mare): meteorite bombardment. Basins flooded by Apollo 15 lava flows landing site The Highlands Impact Cratering Saturated with craters Impact craters on the moon can be seen easily even with small telescopes. Older craters partially … or flooded by Ejecta from the impact can be seen as obliterated by more lava flows bright rays originating from young recent impacts craters 1 11/4/2015 History of Impact Cratering Missions to the Moon Rate of impacts due to Major challenges: interplanetary Need to carry enough fuel for: bombardment decreased • in-flight corrections, rapidly after the formation of the solar system. • descent to surface, • re-launch from the surface, • return trip to Earth; Most craters seen on the need to carry enough food and other moon’s (and Mercury’s) life support for ~ 1 week for all surface were formed astronauts on board. Lunar module (LM) of within the first ~ ½ billion Solution: Apollo 12 on descent to the years. -
February 2022
FORECAST OF UPCOMING ANNIVERSARIES -- FEBRUARY 2022 116 Years Ago – 1902 February 4: Charles Lindbergh’s birthday. 90 Years Ago – 1932 February 19: Joseph Kerwin's birthday. 60 Years Ago – 1962 February 8: Tiros 4 launched by Thor Delta, 7:43 a.m., EST, Cape Canaveral, Fla. February 20: Mercury Atlas 6 (MA-6), Friendship 7 launched, with astronaut John H. Glenn, 9:47:39 a.m., first American to orbit the earth, Cape Canaveral, Fla. February 27: Discoverer 38 (Corona Mission 9030) launched by Thor, Vandenberg AFB. The last Discoverer named Corona mission. 55 Years Ago – 1967 February 4: Lunar Orbiter 3 launched by Atlas Agena, 8:17 p.m., EST, Cape Canaveral, Fla. February 8: Diademe 1 launched by Diamant A, Hammaguir, Algeria, French satellite. February 15: Diademe 2 launched by Diamant A, Hammaguir, Algeria, French satellite. 50 Years Ago – 1972 February 14: USSR launches Luna 20 (Lunik 20) at 03:27:59 UTC by Proton K from Baikonur which soft lands on the Moon four days later. A rotary-percussion drill retrieved samples from the surface which were returned to Earth by capsule on February 25. 45 Years Ago -1977 February 7: USSR launches Soyuz-24 from Baikonur. Cosmonauts: Viktor V.Gorbatko and Yuri N.Glazkov. Ferry flight to Salyut-5 space station. February 18: Enterprise, the first space shuttle orbiter, was flight tested at Dryden Flight Research Center. 40 Years Ago – 1982 February 25: Westar IV launched by Delta, 7:04 p.m., EST, Cape Canaveral, Fla. 35 Years Ago – 1987 February 5: Soyuz TM-2 launched from Baikonur, 2138 Moscow time, Yuri V. -
Thermal and Crustal Evolution of Mars Steven A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. E7, 10.1029/2001JE001801, 2002 Thermal and crustal evolution of Mars Steven A. Hauck II1 and Roger J. Phillips McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, Saint Louis, Missouri, USA Received 11 October 2001; revised 4 February 2002; accepted 11 February 2002; published 16 July 2002. [1] We present a coupled thermal-magmatic model for the evolution of Mars’ mantle and crust that may be consistent with estimates of the average crustal thickness and crustal growth rate. By coupling a simple parameterized model of mantle convection to a batch- melting model for peridotite, we can investigate potential conditions and evolutionary paths of the crust and mantle in a coupled thermal-magmatic system. On the basis of recent geophysical and geochemical studies, we constrain our models to have average crustal thicknesses between 50 and 100 km that were mostly formed by 4 Ga. Our nominal model is an attempt to satisfy these constraints with a relatively simple set of conditions. Key elements of this model are the inclusion of the energetics of melting, a wet (weak) mantle rheology, self-consistent fractionation of heat-producing elements to the crust, and a near- chondritic abundance of those elements. The latent heat of melting mantle material is a small (percent level) contributor to the total planetary energy budget over 4.5 Gyr but is crucial for constraining the thermal and magmatic history of Mars. Our nominal model predicts an average crustal thickness of 62 km that was 73% emplaced by 4 Ga. -
Earthrise- Contents and Chapter 1
EARTHRISE: HOW MAN FIRST SAW THE EARTH Contents 1. Earthrise, seen for the first time by human eyes 2. Apollo 8: from the Moon to the Earth 3. A Short History of the Whole Earth 4. From Landscape to Planet 5. Blue Marble 6. An Astronaut’s View of Earth 7. From Cold War to Open Skies 8. From Spaceship Earth to Mother Earth 9. Gaia 10. The Discovery of the Earth 1. Earthrise, seen for the first time by human eyes On Christmas Eve 1968 three American astronauts were in orbit around the Moon: Frank Borman, James Lovell, and Bill Anders. The crew of Apollo 8 had been declared by the United Nations to be the ‘envoys of mankind in outer space’; they were also its eyes.1 They were already the first people to leave Earth orbit, the first to set eyes on the whole Earth, and the first to see the dark side of the Moon, but the most powerful experience still awaited them. For three orbits they gazed down on the lunar surface through their capsule’s tiny windows as they carried out the checks and observations prescribed for almost every minute of this tightly-planned mission. On the fourth orbit, as they began to emerge from the far side of the Moon, something happened. They were still out of radio contact with the Earth, but the on- board voice recorder captured their excitement. Borman: Oh my God! Look at that picture over there! Here’s the Earth coming up. Wow, that is pretty! Anders: Hey, don’t take that, it’s not scheduled. -
A Journey: the International Space Station an Annotated Storyboard: an Example of How to Create a Digital Story
A Journey: The International Space Station An Annotated Storyboard: An Example of How to Create a Digital Story This was my first attempt to create a digital story, and in fact the first time I had ever done video editing on the computer. As a result, it is not perfect. The original intent had been to create a digital story of no more than about 7 minutes length, that told of some aspect of my life, Work or interests. It was to include a variety of images and videos from several sources, have a soundtrack, and my own narration. One of the first things you are told when you go to build a digital story, is to create a storyboard to lay out your ideas, scenes, script and thoughts, aims and goals for each segment of the story. This was not how I created this story. I think visually. My first steps were to review my extensive image and video collection to identify source material and a list of topics from which I would begin my work, and from that, to select a series of videos and still images which I would try to incorporate in my story, and lay them out in a meaningful order. My original idea was to talk about different spacecraft and how they operate. But during the initial review of a preliminary draft of that story, my mentor asked, “why is this meaningful for you” and, when I showed videos of the interior of the space station, he asked “well I see a bunch of stuff, but what is it?” This set me off in a somewhat different direction from where I had started. -
Physical Characteristics
Physical Characteristics Encyclopedia—moon The study of the moon's surface increased with the invention of the telescope by Galileo in 1610 and culminated in 1969 when the first human actually set foot on the moon's surface. The physical characteristics and surface of the moon thus have been studied telescopically, photographically, and more recently by instruments carried by manned and unmanned spacecraft (see space exploration). The moon's diameter is about 2,160 mi (3,476 km) at the moon's equator, somewhat more than 1/4 the earth's diameter. The moon has about 1/81 the mass of the earth and is 3/5 as dense. On the moon's surface the force of gravitation is about 1/6 that on earth. It has been established that the moon completely lacks an atmosphere and, despite some tantalizing hints that there might be ice under the surface dust in shaded portions of Shackleton Crater (near the moon's south pole), there is no definite evidence of water. The surface temperature rises above 100°C (212°F) at lunar noon and sinks below -155°C (-247°F) at night. The gross surface features of the moon are visible to the unaided eye and were first studied telescopically in 1610 by Galileo. Surface Features The lunar surface is divided into the mountainous highlands and the large, roughly circular plains called maria (sing. mare; from Lat.,=sea) by early astronomers, who erroneously believed them to be bodies of water. The smooth floors of the maria, varying from flat to gently undulating, are covered by a thin layer of powdered rock that darkens them and accounts for the moon's low albedo (only 7% of the incident sunlight is reflected back, the rest being absorbed).