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Mercury and Venus: A Comparative Study of Planetary Features

This chapter explores the unique characteristics of Mercury and Venus, including their surface features, rotations, and compositions. The chapter includes detailed figures and maps to illustrate these features.

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Mercury and Venus: A Comparative Study of Planetary Features

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  1. Mercury and Venus Chapter 10

  2. Fig. 10.1

  3. Fig. 10.2 Maximum elongation

  4. Fig. 10.3 Mercury’s rotation: 2 Mercury years

  5. Fig. 10.4

  6. Fig. 10.5

  7. Fig. 10.6 Carolis Planitia Basin

  8. Fig. 10.7 Intercrater plains

  9. Fig. 10.8 Smooth plains

  10. Fig. 10.9 Scarps

  11. Fig. 10.10

  12. Fig. 10.11 Broken Terrain Diametrically opposite To Carolis Basin

  13. Fig. 10.12

  14. Fig. 10.13 Mercury is denser than Earth (Larger size Metallic core)

  15. Venus

  16. Fig. 10.15

  17. Fig. 10.16 Venus’ rotation clockwise

  18. Tab. 10.4

  19. Fig. 10.17

  20. Fig. 10.18

  21. Fig. 10.20 Map of surface elevations of Venus

  22. Fig. 10.21 Ishtar Terra Red=high Blue = low

  23. Fig. 10.22 Radar Reflectivity Map of Venus

  24. Fig. 10.23 Network of fractures

  25. Fig. 10.24 30 Km crater on Venus

  26. Fig. 10.25 Dark Splotches On Venus

  27. Fig. 10.26 Triple-crater on Venus

  28. Fig. 10.27 Venusian Volcano Maat Mons

  29. Fig. 10.28

  30. Fig. 10.29 Pancake Domes (25 km in diameter 1-2 km high)

  31. Fig. 10.30 Arachnoids (from magma pushed the surface, fracturing it)

  32. Fig. 10.31 Fotla Corona (volcanic domes)

  33. Fig. 10.32 Intersecting Ridges and Troughs in Ishtar Terra

  34. Tab. 10.1

  35. Tab. 10.2

  36. Tab. 10.3

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