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"Спустившись на лунную поверхность и выйдя из тени модуля, я достал этот значок и с силой бросил. Серебряная звездочка ярко сверкнула на солнце, и это была единственная звезда, которую я видел, находясь на лунной поверхности".
(Алан Бин Аполло-12)
QUERY: I have two brief questions that I would like to ask, if I may. When you were carrying out that incredible Moon walk, did you find that the surface was equally firm everywhere or were there harder and softer spots that you could detect? And secondly, when you looked up at the sky, could you actually see the stars in the solar corona in spite of the glare?
ALDRIN: The first part of your question, the surface did vary in its thickness of penetration somewhere in flat regions. [...]
ARMSTRONG: We were never able to see stars from the lunar surface or on the daylight side of the Moon by eye without looking through the optics [i.e., the lunar module's navigation telescope]. I don't recall during the period of time that we were photographing the solar corona what stars we could see.
ALDRIN [actually Collins]: I don't remember seeing any.
(The First Lunar Landing As Told By The Astronauts: Armstrong, Aldrin, and Collins in a Post-flight Press Conference, NASA EP-73, 1989 pt. VI)
Collins' response is a followup to Armstrong's reference to solar corona photography (Fig. 3) which had been taken from the command module during the translunar coast, in which all three astronauts participated. (Apollo 11 Preliminary Science Report NASA SP-214, 1969, p. 39). The reporter's question is a bit confusing since the solar corona cannot be seen from the lunar surface except when the earth eclipses the sun. Or, of course, from a spaceship positioned such that the earth is between the spaceship and the sun. Apollo 11's course provided just such an opportunity. It appears Neil Armstrong interpreted the reporter's phrase "solar corona" to refer to this data.
SCIENTIFIC STUDY OF
UNIDENTIFIED FLYING OBJECTS
Conducted by the University of Colorado
Under contract No. 44620-67-C-0035 With the United States Air Force
Dr. Edward U. Condon, Scientific Director
Copyright © 1968 by The Regents of The University of Colorado
Electronic edition © 1999 by National Capital Area Skeptics (NCAS)
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Chapter 6
Visual Observations Made by U. S. Astronauts
Franklin E. Roach
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The Visibility of Stars
Satellite orbits are at a minimum height of about 160 km. where the "sky" above is not the familiar blue as it is from the earth's surface. Since the small fraction of the atmosphere above the space-craft produces a very low amount of scattering, even in full sunlight, it was anticipated that the day sky from a spacecraft would therefore display the full astronomical panoply. This was decidedly notthe case. All the American astronauts have expressed themselves most forcefully that during satellite daytime, i.e., when the sun is above the horizon, they could not see the stars, even the brighter ones. Only on a few occasions, if the low sun was completely occulted by the spacecraft were some bright stars noted. The inability to observe the stars as anticipated is ascribed to two reasons; (1) the satellite window surfaces scattered light from the oblique sun or even from the earth sufficiently to destroy the visibility of stars, just as does the scattered light of our daytime sky at the earth's surface; and (2) the astronauts are generally not well dark-adapted, as mentioned in section 5 of this Chapter.
Mention has already been made of the dispersion in star visibility during satellite night because of the smudging of the windows. Under the best window conditions the astronomical sky is reported to be similar to that from an aircraft at 40,000 ft. Under the particularly poor conditions of Mercury 8, astronaut Schirra, who is very familiar with the constellations, could not distinguish the Milky Way.