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Astronautics and Aeronautics, 1967 - NASA's History Office

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ASTRONAUTICS AND AERONAUTICS, <strong>1967</strong> August 2231<br />

three times as many craters on Mars as preliminary photos transmitted<br />

in 1965 by Mariner IV spacecraft indicated. Citing data from two-year<br />

study of photos using new computer-enhancement technique, Dr. Leigh-<br />

ton said pictures showed 300 clearly defined craters <strong>and</strong> more than 300<br />

additional possible craters. Original estimate from unprocessed pictures<br />

was less than 100. Mars appeared to be about as densely pitted as the<br />

moon but its craters were smoother because of more effective erosion<br />

processes. Several photos showed a number of linear features similar<br />

to lines formed by rifts <strong>and</strong> faults on the moon. These features were not<br />

the ‘cmuch-discussed” canals of Mars because they were too narrow to<br />

be visible from earth, Dr. Leighton said, but they might be related to<br />

some of the markings identified earlier as canals. (NASA Release 67-225)<br />

Dr. <strong>and</strong> Mrs. Pierre Connes of Haute Provence Observatory <strong>and</strong><br />

Meudon Observatory, France, respectively, reported evidence that might<br />

indicate Venusian clouds are not formed by water. Observation tech-<br />

nique which greatly increased precision with which planets’ spectra<br />

could be analyzed showed spectral lines of hydrogen chloride <strong>and</strong> hydro-<br />

gen fluoride in the light reflected from Venus. When hydrogen fluoride<br />

combines with water it creates hydrochloric acid which absorbs radar<br />

waves; yet radar waves are known to penetrate Venutian clouds, re-<br />

turning echoes to the surface of the earth. (Sullivan, NYT, 8/24/67)<br />

The “mysterium phenomenon”-peculiar radio emissions from the<br />

Milky Way which display almost all the characteristics of artificial<br />

interstellar communication-was the subject of a report by Dr. T. K.<br />

Menon, National Astronomy Observatory, Green Bank, W. Va., <strong>and</strong> a<br />

later panel discussion. Dr. Menon said most recent observations of<br />

the emissions in the nearby part of the galaxy had been made simulta-<br />

neously from California, Massachusetts, <strong>and</strong> U.K., using almost the<br />

entire width of earth as a baseline for measurement. They had identi-<br />

fied sources of emissions which were smaller than the smallest star<br />

as seen by the human eye <strong>and</strong> discovered some of these emissions were<br />

fluctuating on time scales measured in hours or even less. Panel raised<br />

the possibility that emissions might be from stars in the process of<br />

formation. They were being transmitted at four closely spaced wave-<br />

lengths associated with hydroxyl, a molecule formed of a single oxygen<br />

<strong>and</strong> hydrogen atom, <strong>and</strong> were being given off when such molecules shed<br />

energy. Emissions also appeared to have various properties associated<br />

with a maser-man-made device in which a radio or light wave is beamed<br />

through certain atoms whose energy has been raised, enormously ampli-<br />

fying original wave <strong>and</strong>, if wave is confined to a single axis, producing<br />

a beam of extreme intensity. (Sullivan, NYT, 8/26/67,1,10; 8/28/67,<br />

22)<br />

Lunar Committee postponed naming of surface features on moon’s<br />

far side pending the results of Lunar Orbiter V mission. A list of 228<br />

names for approximately 500 major features had been submitted by<br />

Soviet scientists, but US. delegates cited errors in their designations<br />

<strong>and</strong> asked that features be assigned numbers until a more definitive map<br />

could be prepared using Lunar Orbiter V photos. Commission agreed to<br />

interim number designations <strong>and</strong> accepted US. map temporarily, assign-<br />

ing study group to report on specific names at next assembly. (Sullivan,<br />

NYT, 8/25/67, 13; NASNRC-NAE News Report, 10/67, 6-7)<br />

IAU president Dr. Pol Swings of Belgium confirmed an observation<br />

made by two obscure Irish astronomers in 1882. Astronomers Lohse <strong>and</strong><br />

251

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