Barbicane, however, lost not one moment amid all the enthusiasm of which he had become the object. His first care was to reassemble his colleagues in the board-room of the Gun Club. There, after some discussion, it was agreed to consult the astronomers1 regarding the astronomical2 part of the enterprise. Their reply once ascertained3, they could then discuss the mechanical means, and nothing should be wanting to ensure the success of this great experiment.
A note couched in precise terms, containing special interrogatories, was then drawn4 up and addressed to the Observatory5 of Cambridge in Massachusetts. This city, where the first university of the United States was founded, is justly celebrated6 for its astronomical staff. There are to be found assembled all the most eminent7 men of science. Here is to be seen at work that powerful telescope which enabled Bond to resolve the nebula8 of Andromeda, and Clarke to discover the satellite of Sirius. This celebrated institution fully9 justified10 on all points the confidence reposed11 in it by the Gun Club. So, after two days, the reply so impatiently awaited was placed in the hands of President Barbicane.
It was couched in the following terms:
The Director of the Cambridge Observatory to the President
of the Gun Club at Baltimore.
CAMBRIDGE, October 7.
On the receipt of your favor of the 6th instant, addressed to
the Observatory of Cambridge in the name of the members of the
Baltimore Gun Club, our staff was immediately called together,
and it was judged expedient12 to reply as follows:
The questions which have been proposed to it are these —
“1. Is it possible to transmit a projectile13 up to the moon?
“2. What is the exact distance which separates the earth from its satellite?
“3. What will be the period of transit14 of the projectile when endowed with sufficient initial velocity15? and, consequently, at what moment ought it to be discharged in order that it may touch the moon at a particular point?
“4. At what precise moment will the moon present herself in the most favorable position to be reached by the projectile?
“5. What point in the heavens ought the cannon16 to be aimed at which is intended to discharge the projectile?
“6. What place will the moon occupy in the heavens at the moment of the projectile’s departure?”
Regarding the first question, “Is it possible to transmit a projectile up to the moon?”
Answer.— Yes; provided it possess an initial velocity of 1,200 yards per second; calculations prove that to be sufficient. In proportion as we recede17 from the earth the action of gravitation diminishes in the inverse18 ratio of the square of the distance; that is to say, at three times a given distance the action is nine times less. Consequently, the weight of a shot will decrease, and will become reduced to zero at the instant that the attraction of the moon exactly counterpoises that of the earth; that is to say at 4752 of its passage. At that instant the projectile will have no weight whatever; and, if it passes that point, it will fall into the moon by the sole effect of the lunar attraction. The theoretical possibility of the experiment is therefore absolutely demonstrated; its success must depend upon the power of the engine employed.
As to the second question, “What is the exact distance which separates the earth from its satellite?”
Answer.— The moon does not describe a circle round the earth, but rather an ellipse, of which our earth occupies one of the foci; the consequence, therefore, is, that at certain times it approaches nearer to, and at others it recedes19 farther from, the earth; in astronomical language, it is at one time in apogee20, at another in perigee21. Now the difference between its greatest and its least distance is too considerable to be left out of consideration. In point of fact, in its apogee the moon is 247,552 miles, and in its perigee, 218,657 miles only distant; a fact which makes a difference of 28,895 miles, or more than one-ninth of the entire distance. The perigee distance, therefore, is that which ought to serve as the basis of all calculations.
To the third question.
Answer.— If the shot should preserve continuously its initial velocity of 12,000 yards per second, it would require little more than nine hours to reach its destination; but, inasmuch as that initial velocity will be continually decreasing, it will occupy 300,000 seconds, that is 83hrs. 20m. in reaching the point where the attraction of the earth and moon will be in equilibrio. From this point it will fall into the moon in 50,000 seconds, or 13hrs. 53m. 20sec. It will be desirable, therefore, to discharge it 97hrs. 13m. 20sec. before the arrival of the moon at the point aimed at.
Regarding question four, “At what precise moment will the moon present herself in the most favorable position, etc.?”
Answer.— After what has been said above, it will be necessary, first of all, to choose the period when the moon will be in perigee, and also the moment when she will be crossing the zenith, which latter event will further diminish the entire distance by a length equal to the radius22 of the earth, i. e. 3,919 miles; the result of which will be that the final passage remaining to be accomplished23 will be 214,976 miles. But although the moon passes her perigee every month, she does not reach the zenith always at exactly the same moment. She does not appear under these two conditions simultaneously24, except at long intervals25 of time. It will be necessary, therefore, to wait for the moment when her passage in perigee shall coincide with that in the zenith. Now, by a fortunate circumstance, on the 4th of December in the ensuing year the moon will present these two conditions. At midnight she will be in perigee, that is, at her shortest distance from the earth, and at the same moment she will be crossing the zenith.
On the fifth question, “At what point in the heavens ought the cannon to be aimed?”
Answer.— The preceding remarks being admitted, the cannon ought to be pointed26 to the zenith of the place. Its fire, therefore, will be perpendicular27 to the plane of the horizon; and the projectile will soonest pass beyond the range of the terrestrial attraction. But, in order that the moon should reach the zenith of a given place, it is necessary that the place should not exceed in latitude28 the declination of the luminary29; in other words, it must be comprised within the degrees 0° and 28° of lat. N. or S. In every other spot the fire must necessarily be oblique30, which would seriously militate against the success of the experiment.
As to the sixth question, “What place will the moon occupy in the heavens at the moment of the projectile’s departure?”
Answer.— At the moment when the projectile shall be discharged into space, the moon, which travels daily forward 13° 10’ 35’’, will be distant from the zenith point by four times that quantity, i. e. by 52° 41’ 20’’, a space which corresponds to the path which she will describe during the entire journey of the projectile. But, inasmuch as it is equally necessary to take into account the deviation31 which the rotary32 motion of the earth will impart to the shot, and as the shot cannot reach the moon until after a deviation equal to 16 radii33 of the earth, which, calculated upon the moon’s orbit, are equal to about eleven degrees, it becomes necessary to add these eleven degrees to those which express the retardation34 of the moon just mentioned: that is to say, in round numbers, about sixty-four degrees. Consequently, at the moment of firing the visual radius applied35 to the moon will describe, with the vertical36 line of the place, an angle of sixty-four degrees.
These are our answers to the questions proposed to the Observatory of Cambridge by the members of the Gun Club:
To sum up —
1st. The cannon ought to be planted in a country situated37 between 0° and 28° of N. or S. lat.
2nd. It ought to be pointed directly toward the zenith of the place.
3rd. The projectile ought to be propelled with an initial velocity of 12,000 yards per second.
4th. It ought to be discharged at 10hrs. 46m. 40sec. of the 1st of December of the ensuing year.
5th. It will meet the moon four days after its discharge, precisely38 at midnight on the 4th of December, at the moment of its transit across the zenith.
The members of the Gun Club ought, therefore, without delay, to commence the works necessary for such an experiment, and to be prepared to set to work at the moment determined39 upon; for, if they should suffer this 4th of December to go by, they will not find the moon again under the same conditions of perigee and of zenith until eighteen years and eleven days afterward40.
The staff of the Cambridge Observatory place themselves entirely41 at their disposal in respect of all questions of theoretical astronomy; and herewith add their congratulations to those of all the rest of America.
For the Astronomical Staff,
J. M. BELFAST,
Director of the Observatory of Cambridge.
1 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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2 astronomical | |
adj.天文学的,(数字)极大的 | |
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3 ascertained | |
v.弄清,确定,查明( ascertain的过去式和过去分词 ) | |
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4 drawn | |
v.拖,拉,拔出;adj.憔悴的,紧张的 | |
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5 observatory | |
n.天文台,气象台,瞭望台,观测台 | |
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6 celebrated | |
adj.有名的,声誉卓著的 | |
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7 eminent | |
adj.显赫的,杰出的,有名的,优良的 | |
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8 nebula | |
n.星云,喷雾剂 | |
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9 fully | |
adv.完全地,全部地,彻底地;充分地 | |
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10 justified | |
a.正当的,有理的 | |
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11 reposed | |
v.将(手臂等)靠在某人(某物)上( repose的过去式和过去分词 ) | |
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12 expedient | |
adj.有用的,有利的;n.紧急的办法,权宜之计 | |
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13 projectile | |
n.投射物,发射体;adj.向前开进的;推进的;抛掷的 | |
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14 transit | |
n.经过,运输;vt.穿越,旋转;vi.越过 | |
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15 velocity | |
n.速度,速率 | |
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16 cannon | |
n.大炮,火炮;飞机上的机关炮 | |
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17 recede | |
vi.退(去),渐渐远去;向后倾斜,缩进 | |
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18 inverse | |
adj.相反的,倒转的,反转的;n.相反之物;v.倒转 | |
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19 recedes | |
v.逐渐远离( recede的第三人称单数 );向后倾斜;自原处后退或避开别人的注视;尤指问题 | |
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20 apogee | |
n.远地点;极点;顶点 | |
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21 perigee | |
n.近地点 | |
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22 radius | |
n.半径,半径范围;有效航程,范围,界限 | |
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23 accomplished | |
adj.有才艺的;有造诣的;达到了的 | |
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24 simultaneously | |
adv.同时发生地,同时进行地 | |
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25 intervals | |
n.[军事]间隔( interval的名词复数 );间隔时间;[数学]区间;(戏剧、电影或音乐会的)幕间休息 | |
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26 pointed | |
adj.尖的,直截了当的 | |
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27 perpendicular | |
adj.垂直的,直立的;n.垂直线,垂直的位置 | |
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28 latitude | |
n.纬度,行动或言论的自由(范围),(pl.)地区 | |
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29 luminary | |
n.名人,天体 | |
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30 oblique | |
adj.斜的,倾斜的,无诚意的,不坦率的 | |
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31 deviation | |
n.背离,偏离;偏差,偏向;离题 | |
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32 rotary | |
adj.(运动等)旋转的;轮转的;转动的 | |
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33 radii | |
n.半径;半径(距离)( radius的名词复数 );用半径度量的圆形面积;半径范围;桡骨 | |
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34 retardation | |
n.智力迟钝,精神发育迟缓 | |
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35 applied | |
adj.应用的;v.应用,适用 | |
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36 vertical | |
adj.垂直的,顶点的,纵向的;n.垂直物,垂直的位置 | |
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37 situated | |
adj.坐落在...的,处于某种境地的 | |
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38 precisely | |
adv.恰好,正好,精确地,细致地 | |
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39 determined | |
adj.坚定的;有决心的 | |
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40 afterward | |
adv.后来;以后 | |
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41 entirely | |
ad.全部地,完整地;完全地,彻底地 | |
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