DOCSLIB.ORG

Millions Abroad Watch Millions Abroad U

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Millions Abroad Watch Millions Abroad U A lto n E vening t e l e g r a p h Serving Madison, Jersey, Maeounin, Greeneane' (.alhoun (.aunties 4.' j * ______________________________________________________________________________________________________________________________________________________________________________________________________________________ _ - 22 PAGES P ric e IQC Merrier Associated P r e s s Est Jan. 15, 1836 © ATP Co. 1969 Vol. CXXXIV, No. 159 ALTON. IL L ., MONDAY, JULY 21, 1969 Starts After Spacem on Moon IU HOWARD BENEDICT 'after their target, the command earth earlyTuesday, ending a AP Aerospace Writer ship, flashes overhead. space odysseywhich in they SPACE CENTER, Houston Mission control awakenedthe (etched their names beside those (AP) — Neil A. Armstrong and moonmen shortly after ll ofa.m. history’s greatexplorers, Co­ Edwin E. Aldrin Jr. blastedoff following a six-hour rest period,lumbus, Balboa. Magellan, da safely from the moon and into Instruments which monitoredGama and Byrd. lunar orbit today, beginning the Armstrong during the nightThrough in the magic of televi­ complex maneuvers to link up (Heated he slept fitfully.There sion, an estimated 500 million with their mother ship Theyis only one set of biomedical peoplein­ around the world had a left behind their footprintsstruments in in the cabin so Aldrin ringside seat to man’sgreatest the lunar dust and in the history was not monitored. 'adventure. of man. Sleeping in the cramped quar- it was unforgettable. Their liftoff began ti!) seconds tei's of the LM is difficult and Armstrongclimbed through after the command ship, with Aldrin reported: “ Neil has beenLM hatchthe and startedback- Michael Collins its lone passen- lying on the engine coverI ing anddown a nine-rungladder. On ger, passed 69 miles abovecurled up on the floor.” the secondfrom rung the bot- Tranquillity Base. Seven min­Checking of systems and tom, he opened a compartment, utes later, they entered orbitswitch settings for the criticalexposing j a television camera, and a 3V2 hour chase began. liftoff was the No.I priority aft- The picture was black and lf all went well, the two shipser wakeup. whiteand somewhat jerky, but would link up at 5:32 p.m. EDT.A successful liftoff wouldit recorded history, and head for home at 12:57 a m.shoot them into lunar orbitAmong to scientists, there was Tuesday. chase down Michael Collins,or- 1 elation that the crew had landed Their thrust lander, which set­ biting some 65 miles overhead *n an area w*tha variety of tled them onto the surface Sun­in the Apolloll command ship.rocks, I a treasure that held at day for a2114 hour stay, served Once linked up, they planto leastthe hopeof a rich payoff in them, too, at liftoff. They left fire themselves back toward!Continued «n Page 2, Col. 4 behind the spindly-legged lower stage, their launching platform, as a permanent memento of July 20,1969—the day man land­ ed on the moon. Touchdown • It was the first time a rocket had lifted anything from the moon. Armstrong anc! Aldrin staked their lives on single engine which was to lift the cabin sec­On Moon by tion of Eagle off the surface. The bottom half of the raft. with the landing legs, were to I serve as a launching pad and will be left on the moon. Reds ’ Luna The firing was to be the first piloted by Astronaut .Michael Collins, and the Apollo I! mission will be ready lo ON THE WAV TO A KEM ) EX VO! S— This NASA drawing shows how thlunar e for the ascent engine on the By ANDREU TORCHIA module ap|*©ared when ii blasted oil flu* moon’s surface. Hie modulewill carry begin its long journey back to Earth. (AI* Wirephoto) Apollo ll mission. J OR DELL BANK, England (AP) — Russia landed Luna 15 on I .s. V >nuu s , iI \rms.roug and Edwin Aldrin Jr. to the command module, As they prepared for liftoff. Armstrong provided a descrip­the moon’s surface today,500 miles from where America’s tion of the boulder field in whichApollo astronauts were preparing to take onoff their journey Eagle had landed. back to earth, Jordell Bank Observatory reported. As Men Stride Upon The Moon “ Some of the boulders look asSignals picked up at the giant!tempt a remote-controlled lunar if they’re basalt, and someradio-telescope here indicatedlanding to retrieve a sample of seem to have crystals,” he said.that after four daysof moon or­moon soil—a task already per­ “We’re in a boulder field withbit the unmanned proble landedformed by the American astro­ rocks ranging up to two feet,on the moon’s Sea of Crises.nauts. some on top of the surface andJodrell Observatory, headedBut in the absence of signals, some partially buried.Working I by 55-year-old Sir BernardI ov- therewas noimmediate indica- Millions Abroad Watch with the scoop we alsofound cli, stood by for any sign tionthat that Luna 15 was operating !some completely buried in the Luna itself might be preparingon “live” themoon’s surface. By THE Assot JATI I) PRESS stuffed the lunar dust, it was lieveit is taking place as one In Venezuela, today is a na- In a more prominent place at the two astronauts. powder.” I to return toearth. Asked about the possibility LONDON ( XI*) — 1 uplanders lust before sunrise in most of sees it. t Iona I holiday, and the bells of the top of the page was a larger Thousands of Europeans with- He said he suspected the j Prof. Johnthat G. the Davies. probe couldLovell’sstill lift off pasturingtheir remde r lisp nod Europe and a crowd of 2,000 still Crowds in front of TV screens1hundreds of churchespealed story on the shift of Luna 15, thetv outsets spent the night at rocks camefrom a crater which aide. said at 12:05 p.m. EDT: |with a lunar sample for a round on transistor radio Japanese clustered around a giant1- telexat Paris sidewalk cafes and during the walk. \ ’Japanese!unmanned Soviet spacecraft, friends’ houses to followj they the narrowly lu- avoided duringI “ Luna has landed ” trip to earth ahead of Apollo ll. staved up a1! nutr lo watch on sion screen in London’s Trafal- bars in Rome cheeredgirl asin Arm- Tokyo said as she closer to the moon. Pravda still nar adventure. 'the descent to the moon yester- The last signalsDavies received said: from “It is now possible television. Millions around the gar Square. strong bounded over thewatched moon a s streetside monitor gave no hint what Lunajn 15’s Fife. Scotland, a boy born (day. Luna were “appropriatea that to the Russian probe will be world hung on ever- word from \t the Jodrell Bank radio ob- surface and Buzz Aldrin“ It s beganlike a dream, although I mission was. Sunday night was to be named The firing of the ascentsoft landing.” en- he added. I back faster than the Americans, i nofficial sources in Moscow There may be savings in time the two I s.astronauts walking senator Sir Bernard Lovell, his descent. know ifs not a dream.” \\ headquarters bases and;Neil Edwin Michael—the second gine, scheduled to last more on the moon Britain’s leading space expert. There was no word fromOne the Yugoslav teen-ager other rear areas in Vietnam child rn Britain to be named aft- fhan seven minuteswas set for had predicted when Luna 15 with an unmanned craft with no In some countries nany re -stopped tracking the progress of1 Vatican on whether Popesounded Paul a dissent: “They have Americans gathered around ra- er all three astronauts. 11:54 p.m. EDT. just took69 secondsoff July 13 that it would ut- docking procedures." mamed in. v u . i rn inn oust the Soviet craft Luna15 overVI stay cd up to watch the walk.stolen the romance out of the dios at midmorning to hear the Clima, with onequarter of the the moon to watch Armstrong, but when the astronautsmoon landed and it will never be the broadcast of the walk as did the world’s pope I on. did not ‘T m just speechless with the 71-year-old pontiff samehailed again. Now the moon is staff at the U.S. Embassy in broadcast news about \|iollo amazement,”ll Lovell said. them as “conquerors of real,the and lovers won't have it Saigon. nor didNorth Vietnam or North “There is nothing more I can moon.” He said man facesfor themselves“the alone anymore.”1 in the war-torn Middle East Korea say than that it is absolutely expanse of endless space Inand arctic a Norway where the Cairo Radio broadcast news As Neil A. V mstron ’s boots fantastic. One can scarcely be- new destiny.” midnight sun kept skies bright about the first steps before re- through the night, Laplanders viewing Sunday’s fierce air bat- ★ ★★★ ★★★★ sat around their campfires com- tie with Israel, posing sing-song folk poems; One night club owner in Bei- about the astronauts as they lis- ’ rut stopped a striptease act to tened to their transistors. tell the audience. “We’ve made Crowds Ignore AreaPoles jammed the lobby of the it.” U'.S. Embassy in Warsaw while In Australia it was lunchtime hundreds applauded outside. So- when the astronauts stepped wet media repeated the landing onto the moon. From the cities without fanfare, but many RUS- to the lonely cattle stations iii Activities for TV sians undoubtedly staved up to the moon-like Outback, Austral- listen to Western broadcasts ians regarded the lunar explora- about the exploration. tion w7ith awe. Australian news- By ART THOMASON pleasure seekers, were “I was surprised that Pravda, the Soviet Union’s papers highlighted their “kan- Telegraph Staff Writer mute witness to only an there were that manyIleading newspaper, gave the garoo” movements.
Load more

Recommended publications
  • Geoscience and a Lunar Base
    " t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • 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.
    [Show full text]
  • 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].
    [Show full text]
  • Chester County Marriages Bride Index 1885-1930
    Chester County Marriages Bride Index 1885-1930 Bride's Last Name Bride's First Name Bride's Middle Bride's Date of Birth Bride's Age Groom's First Groom's Last Date of Application Date of Marriage Place of Marriage License # Dabney Ruth 47 Arthur Garner October 16, 1929 West Chester 29675 Dabundo Louise 18 Saverio DiMaio December 10, 1925 West Chester 26115.5 Dadley Fannie K 23 Albert Smith April 12, 1916 Toughkenamon 19118 Dagastina LorenzaFebruary 6, 1889 Michele Mastragiolo March 16, 1908 Norristown 13663 Dagne Eva EJuly 8, 1874 Jesse Downs December 27, 1899 West Chester 7490 Dagostina Philomena 18 Nicholas Tuscano August 2, 1925 Phoenixville 25847 D'Agostino Angelina 28 Gabriele Natale April 19, 1915 Norristown 18401 Dague Anna LSeptember 23, 1884 James Porter December 18, 1907 Parkesburg 13097 Dague CoraNovember 10, 1874 Vernon Powell February 10, 1904 Lionville 10244 Dague Lillie AApril 27, 1873 Frederick Gottier April 7, 1902 West Chester 9034 Dague M KatieJanuary 1, 1872 Charles Gantt April 17, 1900 Downington 7673 Dague Mary J 29 Ralph Young March 5, 1921 Coatesville 22856 Dague Sara Ellen 36 Rees Helms October 4, 1922 Honey Brook 23933 Dague Sarah Emma1858 James Eppihimer January 14, 1886 West Chester 104 Dahl Olga G 23 Claude Prettyman January 24, 1925 West Chester 25559 Dahms Elsie Annie 26 Chester Kirkhoff October 31, 1929 Pottstown 29710 Dailey Agnes1859 John McCarthy January 13, 1886 West Chester 084 Dailey Anna 19 Rhinehart Merkt August 14, 1913 Downingtown 17216 Dailey Anna RApril 29, 1877 18 Thomas Argne January 4, 1896
    [Show full text]
  • Martian Crater Morphology
    ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter.
    [Show full text]
  • Pfizer Vaccine
    Find a Walgreens near you to receive an additional dose of the Pfizer COVID-19 vaccine Vaccines subject to availability, State-, age-, and health-related restrictions may apply. PFIZER STORES State Store Address City Zipcode AK 15092 1470 W NORTHERN LIGHTS BLVD ANCHORAGE 99503 AK 13656 725 E NORTHERN LIGHTS BLVD ANCHORAGE 99503 AK 12680 2197 W DIMOND BLVD ANCHORAGE 99515 AK 15653 4353 LAKE OTIS PARKWAY ANCHORAGE 99508 AK 13449 12405 BRANDON ST ANCHORAGE 99515 AK 15654 2550 E 88TH AVE ANCHORAGE 99507 AK 15362 12051 OLD GLENN HWY EAGLE RIVER 99577 AK 15944 530 OLD STEESE HWY FAIRBANKS 99701 AL 9951 9301 HIGHWAY 119 ALABASTER 35007 AL 11279 7155 US HIGHWAY 431 ALBERTVILLE 35950 AL 11819 1401 GOLDEN SPRINGS RD ANNISTON 36207 AL 19256 2413 HIGHWAY 431 NORTH ANNISTON 36206 AL 7951 800 QUINTARD AVE ANNISTON 36201 AL 11651 4700 HIGHWAY 280 BIRMINGHAM 35242 AL 6034 101 GREEN SPRINGS HWY BIRMINGHAM 35209 AL 7791 101 DOUG BAKER BLVD BIRMINGHAM 35242 AL 7245 668 LOMB AVE SW BIRMINGHAM 35211 AL 7306 4496 VALLEYDALE RD BIRMINGHAM 35242 AL 6035 2101 RICHARD ARRINGTON JR BLVD S BIRMINGHAM 35209 AL 15144 3020 CLAIRMONT AVE S BIRMINGHAM 35205 AL 10333 3150 GREEN VALLEY RD BIRMINGHAM 35243 AL 11469 9325 PARKWAY E BIRMINGHAM 35215 AL 4846 2301 CENTER POINT PKWY BIRMINGHAM 35215 AL 10965 920 US HIGHWAY 431 BOAZ 35957 AL 11531 16468 HIGHWAY 280 CHELSEA 35043 AL 15205 444 2ND AVE NW CULLMAN 35055 AL 11180 1700 2ND AVE SW CULLMAN 35055 AL 5606 3025 US HIGHWAY 98 DAPHNE 36526 AL 9976 1127 6TH AVE SE DECATUR 35601 AL 7404 2041 E MAIN ST DOTHAN 36301 AL 7405 2940
    [Show full text]
  • Analysis of Polarimetric Mini-SAR and Mini-RF Datasets for Surface Characterization and Crater Delineation on Moon †
    Proceeding Paper Analysis of Polarimetric Mini-SAR and Mini-RF Datasets for Surface Characterization and Crater Delineation on Moon † Himanshu Kumari and Ashutosh Bhardwaj * Photogrammetry and Remote Sensing Department, Indian Institute of Remote Sensing, Dehradun 248001, India; [email protected] * Correspondence: [email protected]; Tel.: +91-9410319433 † Presented at the 3rd International Electronic Conference on Atmospheric Sciences, 16–30 November 2020; Available online: https://ecas2020.sciforum.net/. Abstract: The hybrid polarimetric architecture of Mini-SAR and Mini-RF onboard Indian Chan- drayaan-1 and LRO missions were the first to acquire shadowed polar images of the Lunar surface. This study aimed to characterize the surface properties of Lunar polar and non-polar regions con- taining Haworth, Nobile, Gioja, an unnamed crater, Arago, and Moltke craters and delineate the crater boundaries using a newly emerged approach. The Terrain Mapping Camera (TMC) data of Chandrayaan-1 was found useful for the detection and extraction of precise boundaries of the cra- ters using the ArcGIS Crater tool. The Stokes child parameters estimated from radar backscatter like the degree of polarization (m), the relative phase (δ), Poincare ellipticity (χ) along with the Circular Polarization Ratio (CPR), and decomposition techniques, were used to study the surface attributes of craters. The Eigenvectors and Eigenvalues used to measure entropy and mean alpha showed distinct types of scattering, thus its comparison with m-δ, m-χ gave a profound conclusion to the lunar surface. The dominance of surface scattering confirmed the roughness of rugged material. The results showed the CPR associated with the presence of water ice as well as a dihedral reflection inside the polar craters.
    [Show full text]
  • Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
    Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process
    [Show full text]
  • 11 Get Continuances
    ' 0# triton ti Vo'ume 12, Hum"" 6 University 01 (a'ilornia, San Diego FriJay, January 22, '''' Regent's Meeting UCNewspaper Guidelines Approved With Provisions Carl Neiburger UCSD Vice Chancellor of Student Affairs City Editor George Murphy agreed with Haskins in an The Regents' Committee on Educational interview with the TRITO TIMES . He said Policy approved guidelines for student that before the amendement it was presumed newspapers yesterday. The approval, however, that " the papers would be consistent with the included the understanding that a guidelines" which, he observed, they had helped representative delegated by the chancellor to write. He said that " the reversal (of this review each issue within 24 hours after publication for rule violations. The proposal will come before the full board today for final On Page 3 Interview with approval. WILSON RILES, Supt. of Public Regent John Canaday, who first brought the matter of student papers before the board , Instruction and New UC Regent. introduced the 24 hour provision as one of four provisions he desired to be amended to the guidelines submitted to the Regents. The other presumption ) is what I think is not really three provisions stated that " responsibility for necessary." However, he foresaw no change in the conduct of student publications is vested in administrative policy at UCSD, other than that UCSD Scientists mesmerize media representatives at conference on Tuesday. (story on page 2) the chancellor, that apparent violations of the someone will be required to read the TRfTON
    [Show full text]
  • August 2017 Posidonius P & Luther
    A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – AUGUST 2017 POSIDONIUS P & LUTHER Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 2017 01:28-01:48; UT, 15 cm refl, 170x, seeing 7-8/10. I drew these craters on the evening of March 4/5, 2017 while the moon was hiding some Hyades stars. This area is in northeast Mare Serenitatis west of Posidonius itself. Posidonius P is the largest crater on this sketch. The smaller crater south of P is Posidonius F and Posidonius G is the tiny pit to the north. There is a halo around Posidonius G, but this crater is noticeably north of the halo's center. A very low round swelling is northeast of Posidonius G. Luther is the crater well to the west of Posidonius P. All four of these craters are crisp, symmetric features, differing only in size. There are an assortment of elevations near Luther. The peak Luther alpha is well to the west of Luther, and showed dark shadowing at this time. All of the other features near Luther are more subtle than Luther alpha. One mound is between Luther and Luther alpha. Two more mounds are north of Luther, and a low ridge is just east of this crater. A pair of very low mounds are south of Luther. These are the vaguest features depicted here, and may be too conspicuous on the sketch.
    [Show full text]
  • Appendix I Lunar and Martian Nomenclature
    APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei
    [Show full text]