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Meade Instruments 60AZ-A2 User Manual

Page 10

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Any small t

e

lesc
ope c

an see the f

our

Galil

ean moons of Jupit

er (

Fig. 5

),

plus a f

e

w other

s, but how many

moons does Jupit

er actuall

y hav

e?

No one knows f

or sur

e! Nor ar

e we

sur

e

how many Saturn has either

. At las

t

c

ount, Jupit

er had o

ver 60 moons, and held a

small l

ead o

ver Saturn. Mos

t of these moons

ar

e v
ery small and c

an onl

y be seen with

very lar

ge t

e

lesc
opes.

Pr
obabl

y the mos

t memor

abl
e sight y

ou will

see in y

o

ur t

e

lesc
ope is Saturn. Although y

o

u

may not see many f

eatur

es on the surf

ac
e of

Saturn, its ring s

tructur

e will s

teal y

our

br
eath away

. Y
ou will pr

obabl

y be abl

e t
o

see

a black opening in the rings, known as the

Cas

sini band.

Saturn is not the onl

y planet that has rings,

but it is the onl

y set of rings that c

an be

seen with a small t

e

lesc
ope. Jupit

er’
s rings

c

annot be seen fr

om Earth at all—the

V

o

yager spac

ecr

aft disc

o

ve

red the ring aft

er

it pas

sed Jupit

er and l

ook

ed back at it. It

turns out, onl

y with the sunlight shining

thr
ough them, c

an the rings be seen. Ur

anus

and Neptune also hav

e f
aint rings.

Optional c

o

lor filt

er
s help bring out det

ail

and c

ontr

as
t of the planets. Meade off

er
s a

line of ine

xpensiv

e c
o

lor filt

er
s.

What’

s Ne

xt? Be

y

ond the Solar Sys

tem

:

Onc

e y
o

u hav

e

observ

ed our own sys

tem of

planets, it’

s time t

o

r

eall

y tr

av
el f

ar fr

om

home and l

ook at s

tar
s and other objects.

You c

an observ

e thousands of s

tar
s with

your t

e

lesc
ope. At fir

s

t, y
ou may think s

tar
s

ar

e jus

t pinpoints of light and ar

en’t v

ery

int
er

es
ting. But l

ook again. Ther

e is much

inf
ormation that is r

e

veal
ed in s

tar
s.

The fir

s

t thing y

ou will notic

e is that not all

8

s

tar
s ar

e the same c

o

lo

rs. See if y

ou c

an find

blue, or

ange, y

ell
o

w, whit

e and r

ed s

tar
s.

The c

o

lor of s

tar
s sometimes c

an t

ell y

o

u

about the age of a s

tar and the t

emper

atur

e

that the

y burn at.

Other s

tar
s t
o

l

ook f

or ar

e multipl

e s
tar
s.

V

ery oft

en, y

ou c

an find doubl

e (or binary)

s

tar
s, s

tar
s that ar

e v
ery cl

ose t

ogether

.

These s

tar
s orbit each other

. What do y

o

u

notic

e about these s

tar
s? Ar

e the

y diff

er

ent

c

o

lo

rs? Does one seem bright

er than the

other?

Almos

t all the s

tar
s y
ou c

an see in the sky

ar

e part of our galaxy

. A galaxy is a lar

ge

Fig. 5

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