In the early 17th century Italian Scientist Galileo, using a telescope smaller than your
LX200-ACF, turned it skyward instead of looking at the distant trees and mountains.
What he saw, and what he realized about what he saw, has forever changed the way
mankind thinks about the universe. Imagine what it must have been like being the first
human to see moons revolve around the planet Jupiter or to see the changing phases
of Venus! Because of his observations, Galileo correctly realized Earth’s movement
and position around the Sun, and in doing so, gave birth to modern astronomy. Yet
Galileo’s telescope was so crude, he could not clearly make out the rings
of Saturn.
Galileo’s discoveries laid the foundation for understanding the motion and nature of
the planets, stars, and galaxies. Building on his foundation, Henrietta Leavitt
determined how to measure the distance to stars, Edwin Hubble gave us a glimpse
into the possible origin of the universe, Albert Einstein unraveled the crucial
relationship of time and light, and 21st-century astronomers are currently discovering
planets around stars outside our solar system. Almost daily, using sophisticated
successors to Galileo’s telescope, such as the Hubble Space Telescope and the
Chandra X-Ray Telescope, more and more mysteries of the universe are being
probed and understood. We are living in the golden age of astronomy.
Unlike other sciences, astronomy welcomes contributions from amateurs. Much of the
knowledge we have on subjects such as comets, meteor showers, double and
variable stars, the Moon, and our solar system comes from observations made by
amateur astronomers. So as you look through your Meade
LX200-ACF telescope, keep
in mind Galileo. To him, a telescope was not merely a machine made of glass and
metal, but something far more—a window of incredible discovery.
AutoStar II Glossary
Be sure to make use of AutoStar II’s Glossary feature. The Glossary menu provides
an alphabetical listing of definitions and descriptions of common astronomical terms.
Access directly through the Glossary menu or through hypertext words embedded in
AutoStar II. See
GLOSSARY MENU, page 28, for more information.
Objects in Space
Listed below are some of the many astronomical objects that can be seen with
your LX200-ACF:
The Moon
The Moon is, on average, a distance of 239,000 miles (380,000km) from Earth and is
best observed during its crescent or half phase when Sunlight strikes the Moon’s
surface at an angle. It casts shadows and adds a sense of depth to the view (Fig. 63).
No shadows are seen during a full Moon, causing the overly bright Moon to appear
flat and rather uninteresting through the telescope. Be sure to use a neutral Moon filter
when observing the Moon. Not only does it protect your eyes from the bright glare of
the Moon, but it also helps enhance contrast, providing a more dramatic image.
Using your
LX200-ACF, brilliant detail can be observed on the Moon, including
hundreds of lunar craters and maria, described below.
Craters are round meteor impact sites covering most of the Moon’s surface. With no
atmosphere on the Moon, no weather conditions exist, so the only erosive force is
meteor strikes. Under these conditions, lunar craters can last for millions of years.
Maria (plural for mare) are smooth, dark areas scattered across the lunar surface.
These dark areas are large ancient impact basins that were filled with lava from the
interior of the Moon by the depth and force of a meteor or comet impact.
Twelve Apollo astronauts left their bootprints on the Moon in the late 1960’s and early
1970’s. However, no telescope on Earth is able to see these footprints or any other
artifacts. In fact, the smallest lunar features that may be seen with the largest
telescope on Earth are about one-half mile across.
BASIC ASTRONOMY
Fig. 63: The Moon. Note the deep
shadows in the craters.
Fig. 64: The planet Jupiter. Jupiter’s
four largest moons can be observed
in a different position every night.
Fig. 65: Saturn has the most
extensive ring structure in our Solar
System.
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