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This study guide provides an overview of the structure and organization of stars and galaxies, as well as the theory of the universe's origin and evolution. It covers the milky way galaxy, other galaxies, and cosmology, and includes study questions for each section. The guide also touches on the possibility of alien life and intelligence.
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In the last section we looked at the stars that surround us. They were many in number and many in type. In this last section we try to organize and relate all of these stars to each other and to us. In doing this we will reach out into space and time as far as we possibly can. In Section A we consider the organization and structure of all the stars and star clusters that are anywhere near us. This group of stars we call the Milky Way Galaxy. In Section B we find that by looking out beyond our own galaxy that there are other separate groups of stars, i.e., other galaxies. In Section C we try to make up a theory that will explain what we have seen in the previous chapters of this part: We try to explain the whole universe as it is now, how it came to be as it is, and how it may change with time. Finally, in Section D we consider all that we've talked about in the whole course and see what we can say about alien life and alien intelligence.
[text: Ch. 14, all] OUTLINE:
[text: Ch. 15, all; Ch. 16, all] OUTLINE:
[text: Ch. 17, all] OUTLINE:
Abundance of elements: (in %) SUN EARTH CRUST ATMOSPHERE BACTERIA HUMANS
H 93.4 O 50 0 47 N 78 H 63 H 61 He 6.5 Fe 17 Si 28 O 21 O 29 O 26 O .06 Si 14 Al 8.1 Ar .93 C 6.4 C 10. C .03 Mg 14 Fe 5.0 C .011 N 1.4 N 2. N .011 S 1.6 Ca 3.6 Ne .0018 P .12 Ca. Ne .010 Ni 1.1 Na 2.8 He .00052 S .06 P. Mg .003 Al 1.1 K 2.6 S. Si .003 Ca .74 Mg 2. Fe .002 Ti. S .001 H. The concentrations of trace elements in bacteria, in fungi, in plants, and in land animals show a strong correlation with the concentrations of these elements in sea water (which is quite different than relative abundances of trace elements on Mars or interstellar dust clouds).