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NASA-UAP-D5,阿波羅 17 號船員科學簡報,1973

NASA-UAP-D5, Apollo 17 Crew Debriefing for Science, 1973

機關

NASA

類型

PDF 文件

日期

1973

NASA-UAP-D5,阿波羅 17 號船員科學簡報,1973
NASA-UAP-D5,阿波羅 17 號船員科學簡報,1973 / 原檔縮圖

阿波羅 17 號是美國第九次載人登月任務,也是第六次成功將太空人送上月球表面的任務。本文件摘錄自 1973 年 1 月 8 日的阿波羅 17 號任務組科學簡報會紀錄。紫外線實驗的共同研究員迪克・亨利(Dick Henry)在會上討論了一些出乎意料的實驗結果。

• 第 119-120 頁。「X 射線天文學最令人興奮的成果之一,就是發現了一種沒有人預期過的全天 X 射線背景輻射,其中一部分就是崔姆卡博士談過的伽馬射線背景。在紫外線方面,沒有人知道,但你不試著看就永遠不會知道。你確實必須處理我們已知存在的星光背景。所以我們觀測了高銀緯地區的許多不同位置,包括北緯和南緯。我們看到的光譜高於這個暗計數。換句話說,這個異常高的暗電流實際上並未干擾該實驗。我們看到的光譜看起來像是熱星的光譜;然而,我們知道我們的視場內沒有熱星。因此,我認為最保守的解釋是,我們看到的是來自銀河平面熱星的光向上射出平面,並被星際塵埃反射的光。光譜的某些特徵雖然不符合該理論,但至少有可能這是河外輻射。我非常期待對此進行詳細的電腦研究,但這將需要很長時間。」


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查看英文原文摘要

Apollo 17 was the ninth crewed U.S. mission to the Moon, and the sixth to land Astronauts on the lunar surface. This document is an excerpt from the Apollo 17 Crew Debriefing for Science on January 8, 1973, in which Dick Henry, co-investigator on the ultraviolet experiment on Apollo 17, discusses seeing results that were unexpected. • Pages 119-120. “One of the most exciting results of X-ray astronomy was the fact that an X-ray background 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 star; however, we know that there were no hot stars within our field of view. Therefore, the most conservative interpretation, 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.”