1. F F
F F F F F F F
F F F F F F
F F (Murray Gellmann) F FF F
F6 F F F F F F F 12
F F F
F F F F 6 F F (up, down, bottom, top, strange,
charmed) F F3 F 3
F F F F
. .1932 F F F F (particle)
F F F F
F F F F F
F F F F F
F F F F F F F F F
F F F F
F F F
F F
F F F F
F F F F F F F F F
F F F F
F (quark) F Finnegans Wake James Joice three quarks for
muster mask!
F F F big bang
1) F E. Hubble F F F F
2) F F F A. Penzias R. Wilson F
F
3) F F F F F
F big bang F F
FF big bang F big bang
F F F
F F F
F F F F F F F F

2. F F F F F
F
F F F
F F F F F F Hubble F F FF F F F
F F Hipparcos W. Freedman F
Carnegie F F F Hubble F F 72 F F 9,000-12,000 F
F A. Sandage F Carnegie F Hubble F F 56 F F
12,000-16,000 F F F F F F F F F
Hubble F F F Hubble F
3. F F F
F F F F F
F
F 6 1) 2) 3) F 4) 5)
6) F
F
F
F F F F F F F F
FF FF F F
F F F F F F
F F
1. (Georges Louis Leclere Buffon) F
. . 2288 F F F F F F F F F
F F
2. F (Fred Hoyle) F (Hans Alphen) F
. . 2493 F F F (interstellar cloud theory) F F F
F F F F F F F F F
F F
3. ( Nebular Hypothesis) F (Pierre Simon Laplace)
F F F . .1796 F F
F F F F F F F
F F F
(angular momentum) F F F
F F F F F F
F F F F F F

3. F F F
F F F F
F F F F F F F F F F
F F F
F F F F F
F F F F
F F F F
98 F F F
0.14 F F F F F F
F F F 745 F F
2 F F F
4. planetesimal Tidal F (F. R. Moulton) F F
(Thomas Chomberlin) F . .1900 F F F F
F F F F F F F
F F F F F F F F encounter theory
F F F (Sir James Jeans) F . . 2444 F F F
(tidal theory two-star) F F F F F F
F F
F F F F F F F F
F tidal F F
F F F
F F F F F F
F F F F F F F
F F F F F F F
F F F F F
F F F F (Ruscell) F F F
F F F F F F F F
F F F F F
5. F F double sun (R.A. Lyttleton)
(R.A. Lyttleton) F planetesimal F F
F F F (double star) F F F F
F F F
F F F F F F F
F F F F F

4. F F (Hill) (Luyten) F F F F
F F F F
F 95 F F 5 F F F F
F F F F F F
F F F
F (Spitzer) F F F F F F F
F F F F F
F
6. F F F (Coral Von Weizsacker) . .1945 F
F F F F F F F
F F F F F F F F
F F F F F F F
F F F F F F F F F F
F F F F F
F F F F F
(vortexes) F
F F F F F F F F
F F F F 5 F
F 5 F F F F
F F F F F
F F F
F F F F F
F
F F F F
F F F F F
F F F F
7. F F
F F F (Kant : 1755) ( Laplace : 1796) F
F (W.H Mc Crea) F F F F
F F F F F (protosun)
F F F F F
F F F F
F F F F F F F F F F F
F F F F

5. F F F F F (floccules) F
F F F F F F F F F
F F F F F F
F F F F F F F F F F F F
F
F F F F F F F F F
F 4 F F 2 F F F F 75 F F
25 F F F F F
F F F F F F
F F
F F F F F
F F (protosun) F F F
F F F F F F F
F F F F F F F F
F F F F F F F F F F F
F F F F F F F F F
F F F F F FF (protoplanet)
F F F
F F F F F F
(tidal force) F F F F F F F
F F F F F F F F F F
F F F F F F F F F F
F F F F F F
F F F
F
F F F F F
F F F F F F F F F F
F F
F F F F F F F F F
F F F F
F F F
1) F
2) F F
3) F F F F F

6. 4) F F F F F F F
F F F F F F F
F F F
F F F FF F F
F F F F F F F F
F F F F
F F F FF F
F F
1) F F F F F 2
1.1 F F F F F F F F F
F F F F
F F F
F F F F F F F F F F F
F F
1.2 F F
. .1938 F (H.Bethe) F (C.F von Weizacker) F F F
F F F F (fusion reaction)
F F F F F F F E = mc2
m
E
c F 3 x 108 F
F 1 F F F F
E = 1x ( 3x1010 )2
= 9 x 1020 F F 25 F F F
( 1 H) 4
1
( 4 He) F
2
1
1H 4 1.0078 x 4 = 4.0312 F
4
2 He 1 = 4.0026 F
= 0.0286 F
-24
1 F F 1.66 x 10

7. E = mc2
= (0.0286) x (1.66 x 10-24 ) x ( 3x1010)2
= 4.3 x 10-5 F
F F F 3.9 x 1033 F F FF F F
F F (1.28/3.9) x 1018 F F F F F
5 F F
2) F
F F F (sunspot groups) F
F F
F F F
F F F
F
F (sidereal rotation)
F F F F (ecliptic)
F F F F 7
15 F F
F F F F F
F F F F F
F F
F F
F F
F F (synodic rotation) F F F
0 0
F F 0.9856 F (360 F 365.256 )
3) F
F F F F F F
F F F F F F F F F
F F F
F F F
F F F F F F
F F
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