From the Earth to the Moon, Direct in Ninety-Seven Hours and Twenty Minutes: and a Trip Round ItVerne, Jules
Science
From the Earth to the Moon, Direct in Ninety-Seven Hours and Twenty Minutes: and a Trip Round It
Verne, Jules
Manned space flight -- Fiction; Moon -- Fiction; Science fiction; Space flight to the moon -- Fiction; Space ships -- Fiction
At the time that the projectile was as high as the tenth parallel,
north latitude, it seemed rigidly to follow the twentieth degree, east
longitude. We must here make one important remark with regard to the map
by which they were taking observations. In the selenographical maps where,
on account of the reversing of the objects by the glasses, the south
is above and the north below, it would seem natural that, on account of
that inversion, the east should be to the left hand, and the west to the
right. But it is not so. If the map were turned upside down, showing the
moon as we see her, the east would be to the _left_, and the west to the
_right_, contrary to that which exists on terrestrial maps. The following
is the reason of this anomaly. Observers in the northern hemisphere
(say in Europe) see the moon in the south,— according to them. When
they take observations, they turn their backs to the north, the reverse
position to that which they occupy when they study a terrestrial map. As
they turn their backs to the north, the east is on their left, and the
west to their right. To observers in the southern hemisphere (Patagonia
for example), the moon's west would be quite to their left, and the east
to their right, as the south is behind them. Such is the reason of the
apparent reversing of these two cardinal points, and we must bear it in
mind in order to be able to follow President Barbicane's
observations.
With the help of Bœer and Moedler's _Mappa Selenographica_, the travellers
were able at once to recognise that portion of the disc enclosed within
the field of their glasses.
"What are we looking at, at this moment?" asked Michel.
"At the northern part of the 'Sea of Clouds,'" answered Barbicane. "We
are too far off to recognize its nature. Are these plains composed of
arid sand, as the first astronomer maintained? Or are they nothing but
immense forests, according to M. Warren de la Rue's opinion, who gives
the moon an atmosphere, though a very low and a very dense one? That we
shall know by and by. We must affirm nothing until we are in a position
to do so."
This "Sea of Clouds" is rather doubtfully marked out upon the maps. It
is supposed that these vast plains are strewn with blocks of lava from
the neighbouring volcanoes on its right, Ptolemy, Purbach, Arzachel.
But the projectile was advancing, and sensibly nearing it. Soon there
appeared the heights which bound this sea at this northern limit. Before
them rose a mountain radiant with beauty, the top of which seemed lost
in an eruption of solar rays.
"That is—?" asked Michel.
"Copernicus," replied Barbicane.
"Let us see Copernicus."
Public-domain text, read in full here on John Shaqi.
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