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To use the
accompanying map, turn it around until it matches the view in your
binoculars. Start your tour by learning the Moon's large, dark plains,
called maria (the Latin plural of mare, "sea"). Early
telescope users and mapmakers in the 17th century thought these dark
markings were similar to Earth's bodies of water and gave them fanciful
names like Mare Nectaris, "Sea of Nectar," and Mare
Nubium, "Sea of Clouds." Today we know that the Moon is an airless,
waterless, and lifeless world. The maria are in fact great lava flows that
filled much of the lunar lowlands billions of years ago.
When the Moon is a slender
crescent in the western sky after dusk, we see the features near the
right-hand edge of the map. As you can see, Mare Crisium and Mare
Fecunditatis are the only major "seas" visible. In the next few days the
retreating terminator gradually unveils Mare Nectaris, Mare
Tranquillitatis, and Mare Serenitatis. At first-quarter phase we see the
entire right half of the map. After first quarter Mare Imbrium and Mare
Nubium appear, and just before full, Oceanus Procellarum and Mare Humorum
come into view.
At full phase the Moon is at
its dazzling brightest. Because the Sun shines onto the Moon from almost
directly behind us at this time, we see no shadows of craters and
mountains. The bright ray system of the craters Tycho, Copernicus, and
Kepler stand out especially prominently. The rays are splash patterns of
debris from the impacts that formed the craters. After full phase the
advancing terminator covers up the surface in the same right-to-left
order.
Unlike astronomical
telescopes, which give inverted (upside-down) and sometimes
mirror-reversed images, binoculars show you right-side-up views that are
never mirror-reversed, making comparison with the lunar map very easy.
Once the map is oriented properly, you will be able to readily identify
the major seas, craters, mountain ranges, and other features. In time the
geography of this alien world will become as familiar to you as that of
our own.
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