Chapter

 1 II  |         zenith, the mathematical point which it ought to attain
 2 III |          wish to reach, than the point of departure.”~“You are
 3 III |          after having passed the point of neutral attraction) on
 4 IV  |           to attain that neutral point where the terrestrial and
 5 IV  |          for, starting from that point, situated about nine-tenths
 6 IV  |        tell you its speed at any point of its transit.”~“On your
 7 IV  |        Nicholl; “it is from that point that we must calculate the
 8 IV  |     enable it to reach the equal point of attraction, ought to
 9 IV  |        able to reach the neutral point.”~“The deuce!”~“We shall
10 IV  |         if it was already on the point of striking the terrestrial
11 V   |        them to reach the neutral point.~The three friends looked
12 V   |        earth. We have passed the point at which the projectile
13 VII |        she would reach the exact point where her meeting with the
14 VIII|    proportion. There must come a point where these two attractions
15 VIII|   densities had been equal, this point would have been at an equal
16 VIII|         easy to reckon that this point would be situated at 4760ths
17 VIII|          from the earth. At this point, a body having no principle
18 VIII| calculated, it would attain this point without speed, having lost
19 VIII|          of motion, and pass the point of equal attraction, and
20 VIII|          and unable to reach the point of equal attraction, it
21 VIII|          it to reach the neutral point, but not sufficient to pass
22 VIII|         had reached this neutral point situated at that distance,
23 VIII|    projectile passes the neutral point, the lunar attraction will
24 VIII|       and when it has passed the point of equal attraction, its
25 IX  |        question from a practical point of view; they would have
26 IX  |          moon will not be at the point indicated, and later it
27 IX  |      might hope that at a nearer point the weight, predominating,
28 X   |  striking the lunar disc at some point or other. He could not think
29 XI  |      able to attain that unknown point of the terrestrial globe.~
30 XI  |     portion of the globe. But in point of fact, these are not liquid
31 XI  |        map from a very different point of view to that of their
32 XII |        were far from the central point which they would have struck,
33 XII |        appeared like a brilliant point through the cloudy light,
34 XIII|      four miles distant.~At this point, under their feet, rose
35 XIII|          an instant from boiling point to the cold of space.~Another
36 XIII|  projectile could not attain any point whatever of the satellite,
37 XIV |         hours and a half at each point of the disc, a long night
38 XIV |    appear as nothing but a black point upon the sun.~“So,” said
39 XIV |         it could never reach any point of the moon. Whither was
40 XV  |   increased or diminished? Every point of mark was wanting by which
41 XV  |        it might strike some high point on the invisible hemisphere,
42 XV  |    almost concentric curve.~This point of mark was a luminous brightness,
43 XV  |          by the black disc. This point could not be confounded
44 XV  |       was taking it far from the point indicated by the eruption.
45 XV  |     being sighted, this luminous point had disappeared behind the
46 XVII|      elliptical orbit. From this point, had the earth been at the
47 XVII|         to remark this brilliant point of the southern hemisphere.
48 XIX |      earth? That was a difficult point.~In watching the course
49 XIX |        most likely extend to the point of equal attraction, where
50 XIX |        when arrived at this dead point, what will become of us?”
51 XIX |         success from a stomachic point of view. Certainly Michel
52 XIX |         aphelion at the farthest point. Speaking of the moon, she
53 XIX |       aposelene” at its farthest point, and in its “periselene”
54 XIX |        toward its aposelenitical point; and Barbicane had reason
55 XIX |        would decrease up to this point, and then increase by degrees
56 XIX |         even become nil, if this point joined that of equal attraction.
57 XIX |          is probable that at the point of equal attraction, its
58 XIX |        first passage at the dead point, because the projectile
59 XIX |       projectile would reach the point of equal attraction, on
60 XIX |        distance between the dead point and the south pole would
61 XIX |         north pole from the dead point. The hours representing
62 XIX |        Barbicane found that this point would be reached at one
63 XIX |         it would reach the given point in twenty-two hours.~The
64 XIX |           One hour more, and the point of equal attraction would
65 XIX |    utterly annulled on this dead point, a decided movement toward
66 XIX |       were very near the neutral point, if they did not touch it.~“
67 XIX |       projectile beyond the dead point. The explosion of the rockets
68 XIX |         it to pass through every point which it had already gone
69 XXI |        We know the truth on that point.~But on the arrival of Blomsberry’
70 XXII|        so as to reach this exact point.~At forty-seven minutes