The Space Race Documented Through Front Pages of Newspapers from Around North America
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3 f~ ~:~~NEA~yA:=~~~T?c:NA:=~~:c:Q:.,I~~; . }RS:~cN ------------------------RELEASE NO, I FOR RELEASE' January 4, 1971 [ \_ ('. '~ '· APOLLO 14 STATUS REPORT Apollo 14 astronaut crew activities include physical examination at MSC, guidance and navigation system briefing, contingency (one-man) EVA simulation on January 5; lunar descent flight simulations with flight controller participation on January 6; lunar orbit and descent orbit insertion simulations with the flight controllers on January 7; EVA simulation with the flight controllers on January 8; and press interviews on January 9 at MSC Hypergolic propellants-- those which ignite spontaneously when the fuel and oxydizer meet-- will be loaded in the Apollo 14 spacecraft and in the auxiliary propulsion system of the Saturn third stage from January 4 to 8. Then RP-1 fuel will be loaded aboard the Saturn V first stage on January 9. Also during the week, spacecraft pyrotechnics will be installed, Saturn first stage engines will be leak-checked. and flight stowage of the modularized equipment stowage assembly in the lunar module descent stage will be accomplished. Preparations of the Apollo 14 space vehicle continue to proceed satisfactorily for a scheduled launching January 31 from Kennedy Space Center Launch Complex 39. Fifteen potential Skylab astronauts are scheduled to visit Sacramento Peak Observatory, Sunspot. New Mexico for solar telescope training on January ' and 7. The second stage for the 13th Saturn V rocket departed the NASA Mississippi Test Facility December 30 aboard the barge Poseidon for the Kennedy Space Center. The stage is scheduled to arrive January 5 and go into temporary storage in the VAB The stage is planned for use in the Skylab program as part of the Saturn V rocket to place the orbital workshop into Earth orbit in late 1972. -
CENTRIPETAL FORCE from GRAVITY Unit 14 & 8
CENTRIPETAL FORCE FROM GRAVITY Unit 14 & 8 Dr. John P. Cise, Professor of Physics, Austin Com. College, Austin , Tx. [email protected] & New York Times November 7, 2017 by Richard Goldstein. Dedicated to all the American Apollo Astronauts in 1960s & 1970s. -------------------------------------------------------------------------------------------------------------------------------------------------------------- Richard Gordon, Astronaut Who Reached for Moon (1969)and Very Nearly Made It, Dies at 88 INTRODUCTION: Gordon commanded the command module Yankee Clipper from 60 miles above moon surface in 1969. The other 2 Apollo Astronauts went to Lunar surface in lunar lander. The radius of moon is 1079 miles. Gordon did 45 orbits of moon over 89 hrs. (3.7 days). Gravity provides centripetal force. G m M/R2 = m v2/R , v = Rω = 2π R/T, thus Solving for M = [4π2/6.67 X 10-11](R3/T2) , Kepler’s 3rd. Law. Richard Gordon, center, with Charles Conrad, left, QUESTIONS: (a) Find R from center of moon?, (b)Find period T of lunar and Alan Bean, aboard the U.S.S. Hornet, an aircraft orbit?, (c) Find mass of moon? See below for Hints and Answers. carrier, after their spacecraft splashed down. Richard Gordon, who undertook what became a harrowing and abortive spacewalk in a 1966 NASA mission, then orbited the moon three years later, but never achieved his dream of walking on the lunar surface, died on Monday at his home in San Marcos, Calif., near San Diego. He was 88. His death was confirmed by NASA. Mr. Gordon piloted the command module ((Yankee Clipper ))during its orbit of the moon in November 1969 while Mr. -
The History Group's Silver Jubilee
History of Meteorology and Physical Oceanography Special Interest Group Newsletter 1, 2010 ANNUAL REPORT CONTENTS We asked in the last two newsletters if you Annual Report ........................................... 1 thought the History Group should hold an Committee members ................................ 2 Annual General Meeting. There is nothing in Mrs Jean Ludlam ...................................... 2 the By-Law s or Standing Orders of the Royal Meteorological Society that requires the The 2010 Summer Meeting ..................... 3 Group to hold one, nor does Charity Law Report of meeting on 18 November .......... 4 require one. Which papers have been cited? .............. 10 Don’t try this at home! ............................. 10 Only one person responded, and that was in More Richard Gregory reminiscences ..... 11 passing during a telephone conversation about something else. He was in favour of Storm warnings for seafarers: Part 2 ....... 13 holding an AGM but only slightly so. He Swedish storm warnings ......................... 17 expressed the view that an AGM provides an Rikitea meteorological station ................. 19 opportunity to put forward ideas for the More on the D-Day forecast .................... 20 Group’s committee to consider. Recent publications ................................ 21 As there has been so little response, the Did you know? ........................................ 22 Group’s committee has decided that there will Date for your diary .................................. 23 not be an AGM this year. Historic picture ........................................ 23 2009 members of the Group ................... 24 CHAIRMAN’S REVIEW OF 2009 by Malcolm Walker year. Sadly, however, two people who have supported the Group for many years died during I begin as I did last year. Without an enthusiastic 2009. David Limbert passed away on 3 M a y, and conscientious committee, there would be no and Jean Ludlam died in October (see page 2). -
Student Worksheets, Assessments, and Answer Keys
Apollo Mission Worksheet Team Names _________________________ Your team has been assigned Apollo Mission _______ Color _________________ 1. Go to google.com/moon and find your mission, click on it and then zoom in. 2. Find # 1, this will give you information to answer the questions below. 3. On your moon map, find the location of the mission landing site and locate this spot on your map. Choose a symbol and the correct color for your mission (each mission has a specific symbol and you can use this if you like or make up your own). In the legend area put your symbol and mission number. 4. Who were the astronauts on the mission? The astronauts on the mission were ______________________________________ ______________________________________________________________________ 5. When did the mission take place? The mission took place from _______________________________________________ 6. How many days did the mission last? The mission lasted ______________________________________________________ 7. Where did the mission land? The mission landed at____________________________________________________ 8. Why did the mission land here? They landed at this location because ________________________________________ ___________________________________________________________________________ _______________________________________________________________________ 9. What was the goal of the mission? The goal of the mission was_______________________________________________ ______________________________________________________________________ ___________________________________________________________________________ -
Planetary Surfaces
Chapter 4 PLANETARY SURFACES 4.1 The Absence of Bedrock A striking and obvious observation is that at full Moon, the lunar surface is bright from limb to limb, with only limited darkening toward the edges. Since this effect is not consistent with the intensity of light reflected from a smooth sphere, pre-Apollo observers concluded that the upper surface was porous on a centimeter scale and had the properties of dust. The thickness of the dust layer was a critical question for landing on the surface. The general view was that a layer a few meters thick of rubble and dust from the meteorite bombardment covered the surface. Alternative views called for kilometer thicknesses of fine dust, filling the maria. The unmanned missions, notably Surveyor, resolved questions about the nature and bearing strength of the surface. However, a somewhat surprising feature of the lunar surface was the completeness of the mantle or blanket of debris. Bedrock exposures are extremely rare, the occurrence in the wall of Hadley Rille (Fig. 6.6) being the only one which was observed closely during the Apollo missions. Fragments of rock excavated during meteorite impact are, of course, common, and provided both samples and evidence of co,mpetent rock layers at shallow levels in the mare basins. Freshly exposed surface material (e.g., bright rays from craters such as Tycho) darken with time due mainly to the production of glass during micro- meteorite impacts. Since some magnetic anomalies correlate with unusually bright regions, the solar wind bombardment (which is strongly deflected by the magnetic anomalies) may also be responsible for darkening the surface [I]. -
PEANUTS and SPACE FOUNDATION Apollo and Beyond
Reproducible Master PEANUTS and SPACE FOUNDATION Apollo and Beyond GRADE 4 – 5 OBJECTIVES PAGE 1 Students will: ö Read Snoopy, First Beagle on the Moon! and Shoot for the Moon, Snoopy! ö Learn facts about the Apollo Moon missions. ö Use this information to complete a fill-in-the-blank fact worksheet. ö Create mission objectives for a brand new mission to the moon. SUGGESTED GRADE LEVELS 4 – 5 SUBJECT AREAS Space Science, History TIMELINE 30 – 45 minutes NEXT GENERATION SCIENCE STANDARDS ö 5-ESS1 ESS1.B Earth and the Solar System ö 3-5-ETS1 ETS1.B Developing Possible Solutions 21st CENTURY ESSENTIAL SKILLS Collaboration and Teamwork, Communication, Information Literacy, Flexibility, Leadership, Initiative, Organizing Concepts, Obtaining/Evaluating/Communicating Ideas BACKGROUND ö According to NASA.gov, NASA has proudly shared an association with Charles M. Schulz and his American icon Snoopy since Apollo missions began in the 1960s. Schulz created comic strips depicting Snoopy on the Moon, capturing public excitement about America’s achievements in space. In May 1969, Apollo 10 astronauts traveled to the Moon for a final trial run before the lunar landings took place on later missions. Because that mission required the lunar module to skim within 50,000 feet of the Moon’s surface and “snoop around” to determine the landing site for Apollo 11, the crew named the lunar module Snoopy. The command module was named Charlie Brown, after Snoopy’s loyal owner. These books are a united effort between Peanuts Worldwide, NASA and Simon & Schuster to generate interest in space among today’s younger children. -
Why NASA Consistently Fails at Congress
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 6-2013 The Wrong Right Stuff: Why NASA Consistently Fails at Congress Andrew Follett College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Political Science Commons Recommended Citation Follett, Andrew, "The Wrong Right Stuff: Why NASA Consistently Fails at Congress" (2013). Undergraduate Honors Theses. Paper 584. https://scholarworks.wm.edu/honorstheses/584 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. The Wrong Right Stuff: Why NASA Consistently Fails at Congress A thesis submitted in partial fulfillment of the requirement for the degree of Bachelors of Arts in Government from The College of William and Mary by Andrew Follett Accepted for . John Gilmour, Director . Sophia Hart . Rowan Lockwood Williamsburg, VA May 3, 2013 1 Table of Contents: Acknowledgements 3 Part 1: Introduction and Background 4 Pre Soviet Collapse: Early American Failures in Space 13 Pre Soviet Collapse: The Successful Mercury, Gemini, and Apollo Programs 17 Pre Soviet Collapse: The Quasi-Successful Shuttle Program 22 Part 2: The Thin Years, Repeated Failure in NASA in the Post-Soviet Era 27 The Failure of the Space Exploration Initiative 28 The Failed Vision for Space Exploration 30 The Success of Unmanned Space Flight 32 Part 3: Why NASA Fails 37 Part 4: Putting this to the Test 87 Part 5: Changing the Method. -
A 1 Case-PR/ }*Rciofft.;Is Report
.A 1 case-PR/ }*rciofft.;is Report (a) This eruption site on Mauna Loa Volcano was the main source of the voluminous lavas that flowed two- thirds of the distance to the town of Hilo (20 km). In the interior of the lava fountains, the white-orange color indicates maximum temperatures of about 1120°C; deeper orange in both the fountains and flows reflects decreasing temperatures (<1100°C) at edges and the surface. (b) High winds swept the exposed ridges, and the filter cannister was changed in the shelter of a p^hoehoc (lava) ridge to protect the sample from gas contamination. (c) Because of the high temperatures and acid gases, special clothing and equipment was necessary to protect the eyes. nose, lungs, and skin. Safety features included military flight suits of nonflammable fabric, fuil-face respirators that are equipped with dual acidic gas filters (purple attachments), hard hats, heavy, thick-soled boots, and protective gloves. We used portable radios to keep in touch with the Hawaii Volcano Observatory, where the area's seismic activity was monitored continuously. (d) Spatter activity in the Pu'u O Vent during the January 1984 eruption of Kilauea Volcano. Magma visible in the circular conduit oscillated in a piston-like fashion; spatter was ejected to heights of 1 to 10 m. During this activity, we sampled gases continuously for 5 hours at the west edge. Cover photo: This aerial view of Kilauea Volcano was taken in April 1984 during overflights to collect gas samples from the plume. The bluish portion of the gas plume contained a far higher density of fine-grained scoria (ash). -
The Newsletter of the Barnard-Seyfert Astronomical Society
June TheECLIPSE 2020 The Newsletter of the Barnard-Seyfert Astronomical Society From the President It’s been another long, strange month. Lots of things have been happening that aren’t in the Next Membership Meeting: realm of astronomy and I have been distracted by Stay tuned to the BSAS Google Group it all. As you know, we haven’t had a meeting in a or Night Sky Network email for couple of months, and I am really starting to miss information about future meetings. the meetings. It is nice to get out of the house and socialize with people that share a common interest. Hopefully this month is the month that we can come together as a group and get back into a new normal routine. Watch for emails and Facebook updates regarding the monthly meeting. Last month did have a big space event with the In this Issue: launch of the SpaceX Crew Dragon capsule to the Happy Birthday Pete Conrad ISS late in the month. It marks a return to U.S. byRobinByrne 3 spaceflight and NASA working with private corporations to get astronauts into space. I hope Summer Triangle Corner: Vega you had a chance to watch the launch on TV or by David Prosper and VivianWhite 8 the Internet, it was very exciting to see. I have not been around long enough to remember the Apollo BSAS Board Minutes launch days, but it did bring back memories of the May6,2020 10 shuttle launches for me. I hope this gets America excited about space travel again and brings back Membership Information 13 talk of getting people to the moon. -
Colonel Gordon Cooper, US Air Force Leroy Gordon
Colonel Gordon Cooper, U.S. Air Force Leroy Gordon "Gordo" Cooper Jr. was an American aerospace engineer, U.S. Air Force pilot, test pilot, and one of the seven original astronauts in Project Mercury, the first manned space program of the U.S. Cooper piloted the longest and final Mercury spaceflight in 1963. He was the first American to sleep in space during that 34-hour mission and was the last American to be launched alone to conduct an entirely solo orbital mission. In 1965, Cooper flew as Command Pilot of Gemini 5. Early life and education: Cooper was born on 6 March 1927 in Shawnee, OK to Leroy Gordon Cooper Sr. (Colonel, USAF, Ret.) and Hattie Lee Cooper. He was active in the Boy Scouts where he achieved its second highest rank, Life Scout. Cooper attended Jefferson Elementary School and Shawnee High School and was involved in football and track. He moved to Murray, KY about two months before graduating with his class in 1945 when his father, Leroy Cooper Sr., a World War I veteran, was called back into service. He graduated from Murray High School in 1945. Cooper married his first wife Trudy B. Olson (1927– 1994) in 1947. She was a Seattle native and flight instructor where he was training. Together, they had two daughters: Camala and Janita Lee. The couple divorced in 1971. Cooper married Suzan Taylor in 1972. Together, they had two daughters: Elizabeth and Colleen. The couple remained married until his death in 2004. After he learned that the Army and Navy flying schools were not taking any candidates the year he graduated from high school, he decided to enlist in the Marine Corps. -
Testing Hypotheses for the Origin of Steep Slope of Lunar Size-Frequency Distribution for Small Craters
CORE Metadata, citation and similar papers at core.ac.uk Provided by Springer - Publisher Connector Earth Planets Space, 55, 39–51, 2003 Testing hypotheses for the origin of steep slope of lunar size-frequency distribution for small craters Noriyuki Namiki1 and Chikatoshi Honda2 1Department of Earth and Planetary Sciences, Kyushu University, Hakozaki 6-10-1, Higashi-ku, Fukuoka 812-8581, Japan 2The Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara 229-8510, Japan (Received June 13, 2001; Revised June 24, 2002; Accepted January 6, 2003) The crater size-frequency distribution of lunar maria is characterized by the change in slope of the population between 0.3 and 4 km in crater diameter. The origin of the steep segment in the distribution is not well understood. Nonetheless, craters smaller than a few km in diameter are widely used to estimate the crater retention age for areas so small that the number of larger craters is statistically insufficient. Future missions to the moon, which will obtain high resolution images, will provide a new, large data set of small craters. Thus it is important to review current hypotheses for their distributions before future missions are launched. We examine previous and new arguments and data bearing on the admixture of endogenic and secondary craters, horizontal heterogeneity of the substratum, and the size-frequency distribution of the primary production function. The endogenic crater and heterogeneous substratum hypotheses are seen to have little evidence in their favor, and can be eliminated. The primary production hypothesis fails to explain a wide variation of the size-frequency distribution of Apollo panoramic photographs. -
Apollo 13 Mission Review
APOLLO 13 MISSION REVIEW HEAR& BEFORE THE COMMITTEE ON AERONAUTICAL AND SPACE SCIENCES UNITED STATES SENATE NINETY-FIRST CONGRESS SECOR’D SESSION JUR’E 30, 1970 Printed for the use of the Committee on Aeronautical and Space Sciences U.S. GOVERNMENT PRINTING OFFICE 47476 0 WASHINGTON : 1970 COMMITTEE ON AEROKAUTICAL AND SPACE SCIENCES CLINTON P. ANDERSON, New Mexico, Chairman RICHARD B. RUSSELL, Georgia MARGARET CHASE SMITH, Maine WARREN G. MAGNUSON, Washington CARL T. CURTIS, Nebraska STUART SYMINGTON, bfissouri MARK 0. HATFIELD, Oregon JOHN STENNIS, Mississippi BARRY GOLDWATER, Arizona STEPHEN M.YOUNG, Ohio WILLIAM B. SAXBE, Ohio THOJfAS J. DODD, Connecticut RALPH T. SMITH, Illinois HOWARD W. CANNON, Nevada SPESSARD L. HOLLAND, Florida J4MES J. GEHRIG,Stad Director EVERARDH. SMITH, Jr., Professional staffMember Dr. GLENP. WILSOS,Professional #tad Member CRAIGVOORHEES, Professional Staff Nember WILLIAMPARKER, Professional Staff Member SAMBOUCHARD, Assistant Chief Clerk DONALDH. BRESNAS,Research Assistant (11) CONTENTS Tuesday, June 30, 1970 : Page Opening statement by the chairman, Senator Clinton P. Anderson-__- 1 Review Board Findings, Determinations and Recommendations-----_ 2 Testimony of- Dr. Thomas 0. Paine, Administrator of NASA, accompanied by Edgar M. Cortright, Director, Langley Research Center and Chairman of the dpollo 13 Review Board ; Dr. Charles D. Har- rington, Chairman, Aerospace Safety Advisory Panel ; Dr. Dale D. Myers, Associate Administrator for Manned Space Flight, and Dr. Rocco A. Petrone, hpollo Director -___________ 21, 30 Edgar 11. Cortright, Chairman, hpollo 13 Review Board-------- 21,27 Dr. Dale D. Mvers. Associate Administrator for Manned SDace 68 69 105 109 LIST OF ILLUSTRATIOSS 1. Internal coinponents of oxygen tank So. 2 ---_____-_________________ 22 2.