Observing Deep Sky Objects; Star Hopping - Celestron ASTROMASTER 102AZ Manual De Instrucciones

OBSERVING DEEP-SKY OBJECTS
Deep-sky objects are simply those objects outside the boundaries of our solar system They include star clusters,
planetary nebulae, diffuse nebulae, double stars and other galaxies outside our own Milky Way Most deep-sky objects
have a large angular size Therefore, low-to-moderate power is all you need to see them Visually, they are too faint to
reveal any of the color seen in long exposure photographs Instead, they appear black and white And, because of their
low surface brightness, they should be observed from a dark-sky location Light pollution around large urban areas washes
out most nebulae making them difficult, if not impossible, to observe Light Pollution Reduction filters help reduce the
background sky brightness, thus increasing contrast

STAR HOPPING

One convenient way to find deep-sky objects is by star hopping This technique uses bright stars to "guide" you to an
object For successful star hopping, it is helpful to know the field of view of your telescope If you're using the standard
20 mm eyepiece with the AstroMaster telescope, your field of view is approximately 1º If you know an object is 3º away
from your present location, then you just need to move 3 fields of view If you're using another eyepiece, consult the
section on determining field of view Below, you'll find instructions for locating two popular objects
The Andromeda Galaxy (Figure 4-1), also known as M31, is an easy target
To find M31:
1 Locate the constellation of Pegasus, a large square visible in the fall (in the eastern sky, moving toward the point
overhead) and winter months (overhead, moving toward the west)
2 Start at the star in the northeast corner—Alpha (
3 Move northeast approximately 7° There you will find two stars of equal brightness—Delta (
Andromeda—about 3° apart
4 Continue in the same direction another 8° There you will find two stars—Beta (
3° apart
5 Move 3° northwest—the same distance between the two stars—to the Andromeda galaxy
Fig. 4-1
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α
) Andromedae
δ
) and Pi (π)
β
) and Mu (μ) Andromedae—also about