Celestron Omni XLT AZ 102 Instruction Manual - Page 42

Collimation of a Newtonian, Aligning the Prim, g the Secondary Mirror, M rror

Page 42 highlights

Perfect collimation will yield a star image very symmetrical just inside and outside of focus. In addition, perfect collimation delivers the optimal optical performance specifications that your telescope is built to achieve. If seeing (i.e., air steadiness) is turbulent, collimation is difficult to judge. Wait until a better night if it is turbulent or aim to a steadier part of the sky. A steadier part of the sky is judged by steady versus twinkling stars. Collimation of a Newtonian The optical performance of most Newtonian reflecting telescopes can be optimized by re-collimating (aligning) the telescope's optics, as needed. To collimate the telescope simply means to bring its optical elements into balance. Poor collimation will result in optical aberrations and distortions. Before collimating your telescope, take time to familiarize yourself with all its components. The primary mirror is the large mirror at the back end of the telescope tube. This mirror is adjusted by loosening and tightening the three screws, placed 120 degrees apart, at the end of the telescope tube. The secondary mirror (the small, elliptical mirror under the focuser, in the front of the tube) also has three adjustment screws. To determine if your telescope needs collimation first point your telescope toward a bright wall or blue sky outside. Never look directly at the sun with the naked eye or with a telescope (unless you have the proper solar filter). Permanent and irreversible eye damage may result. Aligning the Secondary Mirror The following describes the procedure for daytime collimation of your telescope using the optional Newtonian Collimation Tool (#94183) offered by Celestron. To collimate the telescope without the Collimation Tool, read the following section on night time star collimation. For very precise collimation, the optional Collimation Eyepiece 1 ¼" (# 94182) is offered. If you have an eyepiece in the focuser, remove it. Rack the focuser tube in completely, using the focusing knobs, until its silver tube is no longer visible. You will be looking through the focuser at a reflection of the secondary mirror, projected from the primary mirror. During this step, ignore the silhouetted reflection from the primary mirror. Insert the collimating cap into the focuser and look through it. With the focus pulled in all the way, you should be able to see the entire primary mirror reflected in the secondary mirror. If the primary mirror is not centered in the secondary mirror, adjust the secondary mirror screws by alternately tightening and loosening them until the periphery of the primary mirror is centered in your view. DO NOT loosen or tighten the center screw in the secondary mirror support, because it maintains proper mirror position. Aligning the Primary Mirror Now adjust the primary mirror screws to re-center the reflection of the small secondary mirror, so it's silhouetted against the view of the primary. As you look into the focuser, silhouettes of the mirrors should look concentric. Repeat steps one and two until you have achieved this. Remove the collimating cap and look into the focuser, where you should see the reflection of your eye in the secondary mirror. 42

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42
C
The
ng) the
ce.
Poo
rror is
th
e three
rews, placed 120 degrees apart, at the end of the telescope tube.
The secondary mirror (the small, elliptical mirror
nder the focuser, in the front of the tube) also has three adjustment screws.
To determine if your telescope needs
ollimation first point your telescope toward a bright wall or blue sky outside.
eye damage may result.
Ali
n
he
lo
Coll
ti
followin
1 ¼” (# 9
o
a
until its s
mirror, p
gnore the silhouetted reflection from the primary
irror.
Insert the collimating cap into the focuser and look through it.
With the focus pulled in all the way, you
shou
b
entered
r screws by alternately tightening and loosening them
e primar
screw in the secondary mirror su
Aligning the Prim
ry
i
Now adjust the primary mirror s
dary mirror, so it’s
silhouetted against the
ew of the primary.
As you look into the focuser, silhouettes of the mirrors should
look concentric.
Repeat ste
o
Remove the collimating cap and
the secondary mirror.
Perfect collimation will yield a star image very symmetrical just inside and outside of focus.
In addition, perfect collimation
delivers the optimal optical performance specifications that your telescope is built to achieve.
If seeing (i.e., air steadiness) is turbulent, collimation is difficult to judge.
Wait until a better night if it is turbulent or aim to a
steadier part of the sky.
A steadier part of the sky is judged by steady versus twinkling stars.
ollimation of a Newtonian
optical performance of most Newtonian reflecting telescopes can be optimized by re-collimating (aligni
telescope's optics, as needed.
To collimate the telescope simply means to bring its optical elements into balan
r collimation will result in optical aberrations and distortions.
Before collimating your telescope, take time to familiarize yourself with all its components.
The primary mi
e large mirror at the back end of the telescope tube.
This mirror is adjusted by loosening and tightening th
sc
u
c
Never look directly at the sun with the naked eye or with a telescope (unless you have the proper solar filter).
Permanent and irreversible
gni
g the Secondary Mirror
T
fol
wing describes the procedure for daytime collimation of your telescope using the optional Newtonian
ima
on Tool (#94183) offered by Celestron. To collimate the telescope without the Collimation Tool, read the
g section on night time star collimation. For very precise collimation, the optional Collimation Eyepiece
4182) is offered.
If y
u h
ve an eyepiece in the focuser, remove it.
Rack the focuser tube in completely, using the focusing knobs,
ilver tube is no longer visible.
You will be looking through the focuser at a reflection of the secondary
rojected from the primary mirror.
During this step, i
m
ld
e able to see the entire primary mirror reflected in the secondary mirror.
If the primary mirror is not
in the secondary mirror, adjust the secondary mirro
c
y mirror is centered in your view.
DO NOT loosen or tighten the center
pport, because it maintains proper mirror position.
until the periphery of th
a
M rror
crews to re-center the reflection of the small secon
vi
ps
ne and two until you have achieved this.
look into the focuser, where you should see the reflection of your eye in