Home |Previous Page|Next Page
Chapter 1  1.12 Animation 2.55 Mb The retrograde movement of Mars |
 1.25 Animation 581.09 Kb Ptolemy's model of motion of a planet |
 E1.4 Animation 2.05 Mb A time exposure of the northern sky |
 1.29 Animation 1686.91 Kb Kepler's laws |
 1.13 Animation 959.27 Kb The phases of the Moon |
Chapter 3
 3.12 Animation 919.38 Kb A model of a hydrogen atom |
 3.9 Animation 1422.84 Kb Absorption |
 3.1 Animation 430.33 Kb An electromagnetic wave |
Chapter 4
 Chapter 4 Animation 1353.67 Kb A Foucault pendulum |
 4.22 Animation 1816.29 Kb The position of the Sun against the backdrop of stars throughout the year |
 4.6 Animation 3.42 Mb S and p waves generated by earthquakes |
 Chapter 4 Animation 15.12 Mb The number of remaining 13n nuclei declines with time |
 4.24 Animation 8.62 Mb The Coriolis effect |
Chapter 6
 Chapter 6 Animation 4.14 Mb The movement of the Moon's nodes |
 6.11 Animation 3.74 Mb The rotation of the Moon |
 6.22 Animation 3.46 Mb Tidal forces |
Chapter 8
 8.9 Animation 1754.62 Kb The rotation of Mercury during 2 Mercury years |
Chapter 9
 9.1 Animation 1615.73 Kb The rotation of Jupiter |
 9.22 Animation 1202.25 Kb The seasons of Uranus |
Chapter 10
 10.15 Animation 3.26 Mb The orientation of comet tails |
 10.16 Animation 2.19 Mb A meteor shower |
Chapter 11
 11.11 Animation 1839.68 Kb The reactions of the proton-proton chain |
Chapter 12
 Chapter 12 Animation 4.76 Mb The position and Doppler shift of a star orbiting its common center of mass with a planet |
 12.14 Animation 14.60 Mb Orbital motion reflected in the shifting spectral lines of a spectroscopic binary |
Chapter 13
 Chapter 13 Animation 7.78 Mb An H-R diagram showing the evolutionary track of a one-solar-mass star |
 13.10 Animation 1867.50 Kb The structure of a star when hydrogen shell burning begins |
Chapter 14
 14.3 Animation 8.07 Mb Stages in the evolution of a low-mass binary |
 Chapter 14 Animation 3.28 Mb The paths of light rays from the collapsing core of a star |
Chapter 15
Chapter 16
 16.12 Animation 2.16 Mb Galaxies with tails |
 Chapter 16 Animation 6.97 Mb The pancake model of the formation of clusters of galaxies |
Chapter 17
 17.9 Animation 1374.77 Kb The steady-state theory |
 Chapter 17 Animation 4.57 Mb The future of expansion |
 17.8 Animation 1383.97 Kb The expansion of the universe |
