Philips Atlas of the Universe

THE SOLAR SYSTEM

Name Lat. ° Long. °

1 Apollo 37 S 153 W

2 Avogadro 64 N 165 E

3 Birkhoff 59 N 148 W

4 Boltzmann 55 S 115 W

5 Brianchon 77 N 90 W

6 Campbell 45 N 152 E

7 Cockcroft 30 N 164 W

8 Compton 55 N 104 E

9 Daedalus 6 S 180

10 Dunér 45 N 179 E

11 Fabry 43 N 100 E

12 Fermi 20 S 122 E

13 Fersman 18 N 126 W

14 Fleming 15 N 109 E

15 Fowler 43 N 145 W

16 Gagarin 20 S 150 E

17 Galois 16 S 153 W

18 Heaviside 10 S 167 E

19 Hertzsprung 0 130 W

20 Hirayama 6 S 93 E

21 Icarus 6 S 173 W

22 Joffe 15 S 129 W

23 Jules Verne 36 S 146 E

24 Joliot 26 N 94 E

25 Keeler 10 S 162 E

26 Korolev 5 S 157 W

27 Landau 42 N 119 W

28 Lorentz 34 N 100 W

29 Lowell 13 S 103 W

30 Mach 18 N 149 W

31 Mare Moscoviense 27 N 147 E

32 Mendel 49 S 110 W

33 Mendeléev 6 N 141 E

34 Oppenheimer 35 S 166 W

35 Paschen 14 S 141 W

36 Pasteur 12 S 105 E

37 Planck 57 S 135 E

38 Poincaré 57 S 161 E

39 Rowland 57 N 163 W

40 Schrödinger 75 S 133 E

41 Schwarzschild 71 N 120 E

42 Sommerfeld 65 N 161 W

43 Szilard 34 N 106 E

44 Tsiolkovskii 21 S 129 E

45 Van de Graaff 27 S 172 E

46 H. G. Wells 41 N 122 E

47 Zeeman 75 S 135 W

▼ Tsiolkovskiiis exceptional

in many ways. It is 240 km

(150 miles) in diameter,

with terraced walls and a

massive central mountain

structure. The darkness

is caused by lava; in fact

Tsiolkovskii seems to be

intermediate in type of

lunar feature, falling

somewhere between a

crater and a mare, or sea.

 The far sideof the Moon

• first recorded from the
  Soviet space probe Lunik 3 in
  1959, and now fully mapped.
  10°

10°

E 0°

FAR-SIDE FEATURES

N

W

80°

80°

80°

80°

70°

70°

70°

70°

60°

60°

60°

60°

50°

50°

50°

50°

40°

40°

40°

40°

30°

30°

30°

30°

20°

20°

20°

20°

10°

10°

0°

S

1

(^23)

4

5

6

7

8

9

10

11

12

13

14

15

16

18 17

20 19

21

22

23

24

25 26

(^2728)

29

30

31

32

33

34

(^3635)

37

38

39

40

41

42

43

44 45

46

47

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