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Meade Instruments 60AZ-A2 User Manual

Page 12

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Fig. 6

Changing e

yepiec

es changes the

pow

er or magnific

ation of y

our

te

lesc
ope.

By the way, y

ou might hav

e notic

ed

something s

tr

ange when y

ou l

ook

ed thr

ough

your e

yepiec

e. Although the image is right-

side up, it is r

e

ve

rsed. That means r

e

ading

wor

d

s c
an be a pr

obl
em. But it has no aff

ect

on as

tr

onomic

al objects. If y

ou wish t

o

hav

e

a full

y c
orr
ect
ed image, check out Meade’

s

optional Er

ecting Prism in the Optional

Ac
c

e

s

sory section.

Barl

o

w

l

ens

: Y
ou c

an also change

magnific

ation by using a Barl

o

w

. Remo

ve

the

e

yepiec

e fr

om the diagonal mirr

or and slide

in the Barl

o

w

. And then plac

e the e

yepiec

e

int
o the Barl

o

w

. Tight

en the thumbscr

e

ws t

o

secur

e the Barl

o

w

l

ens and the e

yepiec

e in

plac

e. The Barl

o

w

l

ens included with y

our

te

lesc
ope doubl

es the pow

er of y

our

te

lesc
ope. See

Fig. 6

.

Meade off

er
s a c

ompl

et

e line of e

yepiec

es

for y

our t

e

lesc
ope. Mos

t as

tr

onomer

s hav

e

four or fiv

e l
o

w-pow

er and high pow

e

r

e

yepiec

es t

o

view diff

er

ent objects and t

o

c

ope with diff

e

rent viewing c

onditions.

Objects mo

v

e

in the e

y

epiec

e

: If y

ou ar

e

observing an as

tr

onomic

al object (the Moon,

10

ST
AR CHARTS

St

ar charts and planispher

es ar

e useful f

or a v

ariety of

reasons. In particular, the

y ar

e a gr

eat aid in planning a

night of c

e

le

s

tial viewing.

A wide v

ariety of s

tar charts ar

e av

ailabl

e in books, in

magazines, on the int

ernet and on CD

Roms. Meade

off
er
s Aut

o

s

tar Suit

e

softwar

e. Cont

act y

our l

o

c

a

l

Meade deal

er or Meade’

s Cus

tomer Servic

e

department

for mor

e inf

ormation.

Astronomy

and

Sky and Telescope

magazines print s

tar

charts each month f

or up-t

o-the-minut

e maps of the

heav

ens.

a planet, s

tar, et

c.) y

ou will notic

e that the

object will begin t

o

mo

ve

sl
o

w

ly

thr

ough the

te

lesc
opic field of view

. This mo

vement is

c

aused by the r

o

tation of the Earth and

mak

es an object mo

ve

thr

ough the t

e

le

-

sc
ope’

s field of view

. T

o

k

eep as

tr

onomic

al

objects c

ent

er

ed in the field, simpl

y mo

ve

the t

e

lesc
ope on one or both of its ax

es—

vertic

all
y and/or horizont

all
y as needed—try

using the t

e

lesc
opes c

oar

se and fine

adjus

tment c

ontr

ols. At higher power

s

,

as
tr

onomic

al objects will seem t

o

mo

ve

thr
ough the field of view of the e

yepiec

e

mor

e r
apidl

y.

Plac

e the object t

o

be view

ed at the edge of

the field and, without t

ouching the t

e

lesc
ope,

wat

ch it drift thr

ough the field t

o

the other

side bef

or

e r
epositioning the t

e

lesc
ope so

that the object t

o

be view

ed is again plac

ed

at the edge of the field, r

eady t

o

be further

observ

ed.

Vibr

ations

: A

void t

ouching the e

yepiec

e

whil

e observing thr

ough the t

e

lesc
ope.

Vibr

ations r

esulting fr

om such c

ont

act will

c

ause the image t

o

mo

ve. A

void observing

sit
es wher

e vibr

ations c

ause image

mo

vement (f

or e

xampl

e, near r

ailr

oad

e

yepiec

e

barl

o

w

diagonal

mirr

or

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