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Apollo 17·科学汇报(1973)

Apollo 17 Crew Debriefing For Science (1973)
机构NASA
日期1973年
标签1973
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1973年,NASA阿波罗17号任务科学汇报记录
The Apollo 17 mission science debriefing record from 1973

摘要 Summary

这份文件记录了1973年1月8日,NASA国家航空航天局在休斯顿,德克萨斯州进行的阿波罗17号任务科学汇报。文件由科学需求分支行星和地球科学部门准备,记录了任务的相关科学数据。

This document records the science debriefing for the Apollo 17 mission, conducted by the National Aeronautics and Space Administration on January 8, 1973, in Houston, Texas. The document was prepared by the Science Requirements Branch of the Planetary and Earth Sciences Division.

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从 PDF 内提取,最多 3 张代表性页面/影像。完整内容请下载原档。

关键段落对照 Bilingual Excerpts

EXCERPT · 01
C/B/R.A.PARKER MSC-07632 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION * APOLLO 17 CREW DEBRIEFING FOR SCIENCE JANUARY 8, 1973
译文 · 01
C/B/R.A.PARKER MSC-07632 美国国家航空航天局 * 阿波罗17号任务科学汇报 1973年1月8日
EXCERPT · 02
PREPARED BY SCIENCE REQUIREMENTS BRANCH PLANETARY AND EARTH SCIENCES DIVISION
译文 · 02
由科学需求分支行星和地球科学部门准备
EXCERPT · 03
INDEXING DATA DATE OPR # T PGM SUBJECT SIGNATORI LOC
译文 · 03
索引数据日期操作员编号任务主题签署人位置
EXCERPT · 04
1-8-73 MSC MSC-07632 B APO NS 080-44F MANNED SPACECRAFT CENTER HOUSTON, TEXAS
译文 · 04
1-8-73 MSC MSC-07632 B APO NS 080-44F 指令航天器中心 休斯顿,德克萨斯州

标签 Tags

#NASA#Apollo 17#Science Debriefing#1973#Houston
展开原文抽取(pdftotext,未翻译) · Show extracted source
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 ll9

 HENRY gravitationally holding it together° We though it might be
 (CONT 'D)
 in the form of ionized hydrogen. We looked for Lyman-alpha

 radiation, red shifted from the ionized hydrogen, and we

 didn't see any. We set a lower limit, which certainly ex-

 cludes the possibility that the Coma cluster is held together
J
 by this ionized hydrogen. I think that may leave a real

 mystery as to what is holding the thing together.

 The fourth point may turn out to be the most interesting

 thing of all. When you look in the Milky Way, you see a

 lot of UV coming from the stars, but the question is, what

 do you see when you look up to the North Galactic Pole or

 down to the South Galactic Pole. One of the most exciting

 results of X-ray astronomy was the fact that an X-ray back-

 ground was observed over the sky that nobody had expected,

 and part of this is the gamma-ray background that Dr. Trombka

 talked about. In the UV, nobody knows, but you never know

 until you look. You do have to deal with this background

 of stars that we know is there. So we did look at a large

 number of different points at high galactic latitudes, both

. north and south. The spectrum that we see is above this

 dark count. In other words, this abnormally high dark

 current did not, in fact, interfere with that experiment.

 The spectrum that we see looks like the spectrum of the hot
120

HENRY star; however, we know that there were no hot stars within
(CONT'D)
 our field of view. Therefore, the most conservative inter-

 pretation, I think, is that what we're seeing is light from

 hot stars in the galactic plane going up out of the plane

 and reflecting off interstellar dust. There are certain

 characteristics of the spectrum, though, that don't fit that

 theory, and it's at least possible that this is extragalactic

 radiation. I'm looking forward very much to the detailed

 computer study of this, but it's going to take a long time.

 Fifth point: Lyman-alpha hydrogen radiation is a completely

 separate problem, and Gary Thomas at the University of

 Colorado and Charles Barthum [?] observed this from OGO-5.

 We obtained Just an enormous amount of data on the Apollo

 that's going to straighten out this picture and clarify it

 considerably. This is hydrogen that is inside our solar

 system. It's sunlight reflecting off this. The hydrogen,

 Gary Thomas thinks, is hydrogen from interstellar space

 streaming through the solar system, and he is looking for-

 ward with great anticipation to getting detailed analyses

 of that.

 One more thing: the spectrum of the Earth. I keep saying

 "we ? " but these were the guys that were there. We looked

 at the Earth from outside. A lot of people have observed