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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


Vision Description (EN)

Page 120 is a text-only body page containing the continuation of Henry's remarks (marked 'HENRY (CONT'D)' in left margin) in what appears to be a formal NASA Apollo 17 crew debriefing transcript. The page presents a technical scientific discussion of astronomical observations, specifically addressing galactic plane radiation, interstellar dust reflection, Lyman-alpha hydrogen radiation phenomena, and Earth spectrum analysis obtained during the Apollo mission. The text is rendered in monospaced typewriter font, typical of official government transcripts. No redactions, classification markings, signatures, or images are present. The page is clearly readable with no significant degradation.

Descrição Vision (PT-BR)

A página 120 é uma página de corpo contendo apenas texto, com a continuação das observações de Henry (marcada como 'HENRY (CONT'D)' na margem esquerda) em uma transcrição formal de debriefing da tripulação do Apollo 17 da NASA. A página apresenta uma discussão técnica e científica sobre observações astronômicas, abordando especificamente radiação do plano galáctico, reflexão de poeira interestelar, fenômenos de radiação de hidrogênio Lyman-alfa e análise do espectro da Terra obtidos durante a missão Apollo. O texto está em fonte de máquina de escrever monoespaçada, típica de transcritos oficiais governamentais. Não há redações, marcações de classificação, assinaturas ou imagens presentes. A página está claramente legível sem degradação significativa.