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Appendix b: basic astronomy – Meade Instruments LX80 User Manual

Page 59

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Planets change positions in the sky as they orbit

around the Sun. To locate the planets on a given day

or month, consult a monthly astronomy magazine,

such as Sky and Telescope or Astronomy. You can

also consult LX80 for information about planets. Scroll

to the “Object: Solar System” menu and scroll through

the lists of planets. When a planet you are interested

in displays, press “ENTER”. Use the Scroll keys to

display information about the planet, such as the

planet’s coordinates, and the rise and set times (Tip:

enter a date in the Date menu and you can determine

if a planet) will be visible during the night of the entered

date by checking its rise and set times). Listed below

are the best planets for viewing through the LX80.

Mars is about half the diameter of Earth, and appears

through the telescope as a tiny reddish-orange disk.

It may be possible to see a hint of white at one of the

planet’s polar ice caps. Approximately every two years,

when Mars is closest to Earth in its orbit, additional

detail and coloring on the planet’s surface may

be visible.

Jupiter is the largest planet

in our solar system and is 11

times the diameter of Earth.

The planet appears as a disk

with dark lines stretching

across the surface. These

lines are cloud bands in

the atmosphere. Four of

Jupiter’s 16 moons (Io,

Europa, Ganymede and

Callisto) can be seen as

“star-like” points of light

when using even the lowest

magnifi cation. These moons orbit Jupiter so that the

number of moons visible on any given night changes

as they circle around the giant planet.

Saturn is nine times the diameter of Earth and appears

as a small, round disk with rings extending out from

either side. In 1610, Galileo, the fi rst person to observe

Saturn through a telescope, did not understand that

what he was seeing were rings. Instead, he believed

that Saturn had “ears.” Saturn’s rings are composed of

billions of ice particles ranging in size from a speck of

dust to the size of a house. The major division in Saturn’s

rings, called the Cassini Division, is occasionally

visible through the LX80. Titan, the largest of Saturn’s

18 moons can also be seen

as a bright, star-like object

near the planet.

Deep-Sky Objects

Star charts can be used

to locate constellations,

individual stars and deep-

sky objects.

Examples of various

deep-sky objects are

given below:

Stars are large gaseous

objects that are self-

illuminated by nuclear fusion in their core. Because

of their vast distances from our solar system, all stars

appear as pinpoints of light, irrespective of the size of

the telescope used.

Nebulae are vast interstellar clouds of gas and dust

where stars are formed. Most impressive of these is

the Great Nebula in Orion (M42), a diffuse nebula that

appears as a faint wispy gray cloud. M42 is 1600 light

years from Earth.

Open Clusters are loose groupings of young stars,

all recently formed from the same diffuse nebula.

The Pleiades is an open cluster 410 light years away.

Through the LX80, numerous stars are visible.

Constellations are large, imaginary patterns of stars

believed by ancient civilizations to be the celestial

equivalent of objects, animals, people or gods. These

patterns are too large to be seen through a telescope.

To learn the constellations, start with an easy grouping

of stars, such as the Big Dipper in Ursa Major. Then,

use a star chart to explore across the sky.

Galaxies are large assemblies of stars, nebulae and

star clusters that are bound by gravity. The most

common shape is spiral (such as our own Milky Way),

but galaxies can also be elliptical or even irregular

blobs. The Andromeda Galaxy (M31) is the closest

spiral-type galaxy to our own. This galaxy appears

fuzzy and cigar-shaped. It is 2.2 million light years

away in the constellation Andromeda, located between

the large “W” of Cassiopeia and the great square

of Pegasus.

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Appendix B:

Basic

Astronomy