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Orion XT-12 Intelliscope;
Newtonian Reflector
on a
Dobsonian mount:
The Intelliscope Controller
The Orion Intelliscope family of Dobsonian telescopes consists of 6-, 8-,
10-, and 12-inch scopes. They are exactly alike except for the size of the
Optical Tube Assembly (OTA) with the 6-inch being the smallest and the 12-inch
being the largest. This article is my description of the operation of the
Intelliscope controller.
How to find things in the sky
The main challenge facing an astronomer -- professional or amateur -- is
finding things in the sky. If you want to look at a certain star, nebula,
globular cluster, planet, or what have you, how do you find it? How do you
know which of the zillion or so spots of light in the sky is the one you want to
look at?
The sky
Complicating the problem of finding what you want to observe is the fact that
it's all moving -- that is, the Earth revolves on its axis once every 24 hours
and the Earth revolves around the Sun, making one circuit every 365 days.
Where an object is in the sky is determined by three elements: rotation of
the Earth around its axis; rotation of the Earth around the Sun, and, observer's
location on Earth.
- Rotation of the Earth around its axis. The stars and other
objects in the universe are fixed in position -- they don't move (well,
really they DO move, it's just that their motion is so slow and so complex
in relation to each other and to us that they appear to be fixed). As
the Earth revolves on its axis, objects move into and out of view -- step
outside one night and look for a bright star, mark where it is. Then,
step outside a couple of hours later and notice that the star is not where
it was earlier. Actually, the star has not moved -- you have -- the
Earth has rotated through a few degrees around its axis and the star has
appeared to move. This is how the Sun moves across the sky from
morning to night -- we rotate, the sun sits still.
- Rotation of the Earth around the Sun. As the Earth revolves
around the Sun, our view of the universe changes. That is, some
objects are visible only in the winter, others in the summer, etc. One
of my favorite constellations is Orion, The Hunter. Orion dominates
the winter sky, usually appearing in early fall and remaining visible until
early spring. In the fall, Orion rises early in the morning, rising
earlier and earlier each day until in the middle of winter Orion rises
around sunset and is visible all night.
- Observer's location on Earth. Another factor that
determines where objects are in the sky is your location. An observer
standing in Alaska will see a star in one position while an observer on the
Equator looking at the same star, same date, same time, will see the star in
a different location because each observer is looking at the star from a
different point.
Manually locating astronomical objects
The traditional, manual method of finding objects involves, "learning the
sky," then using various observation aids, mainly a sky chart or a sky atlas.
We have all seen sky charts and some of us have seen sky atlases. A sky
chart shows a view of the night sky at a particular date and time and shows
where the stars are at that date, time, and observing location. Here's an
example of a star chart that shows the positions of stars and constellations in
winter as seen from the mid-latitudes of the Northern Hemisphere.

The constellation Orion is in the center of the southern sky, with its
brightest stars, Betelgeuse and Rigel shining brightly. Sirius, the Dog
Star, is the brightest object in the night sky. This chart is good for
midnight, late December. Two months earlier, this chart would be good but
for earlier in the morning -- around 0400 -- because the Earth is moving around
the Sun, causing the angle at which we see these objects to change. If you
look directly overhead at midnight, late December, you'll spot the bright star
Capella. Polaris -- the North Star -- is in the center of the northern
sky.
Armed with a sky chart and a pair of binoculars, you can see a lot of objects
in the sky. Just compare the sky chart to the sky and refer to the chart
to identify objects in the sky. If you do this 3-4 days a week for a year,
you will have gone a long way toward "learning the sky" -- you'll be able to
pick out the major constellations, the bright stars, and other objects in the
sky without the aid of a chart.
A more sophisticated method of locating objects in the sky is "star-hopping."
This requires a fairly good knowledge of the sky and a sky atlas. Here's
how it works:
- Find a known object in your telescope.
- Consult your star chart and find the known object that's in the
telescope field of view and the object you want to see.
- Consult your star atlas and determine how far and in what direction is
the object you want to see.
- Note any prominent objects between where you are looking and where you
want to look.
- Now, move the telescope in the direction and for the distance you
determined from the atlas until you find the object you are looking
for. You may have to move from one object to the next and the next and
so on until you get to where you are going -- hence the name "star-hopping,"
because you are hopping from star to star to find what you want.
- Do a Google search for star-hopping for a better explanation and
examples.
A sky atlas is a VERY detailed chart showing the location of thousands of
stars. Sky atlases are many pages long and can be quite detailed -- they
are typically used only by serious amateurs and professionals.
Let the computer find things for you
If you stop and think about this process for a minute, you'll come up with an
obvious solution to the problem of finding objects in the sky. Consider
the following:
- Objects in the sky "move" across our field of view at a steady,
predictable rate because of the rotation of the Earth and because of our
movement around the Sun.
- Objects in the sky appear at the same place, the same time, year after
year.
- Objects in the sky always appear in the same position relative to each
other. That is -- refer to the sky chart above and note the locations
of Procyon, Betelgeuse, Sirius, and Rigel. These four stars are always
in the same relative position, forming a + sign with Betelgeuse at the top,
Sirius at the bottom, and Rigel and Procyon on the right and left wings
respectively.
Throw in the fact that observing location will cause the view to change, and
you come up with the following conditions:
-
If you know where you are on the face of the Earth, the
date, and the time, you will know exactly where to look for a specific
object. For example -- if it's 2345 hours, EST, 23 December (year
does not matter), then the star Betelgeuse will be at one specific location
in the sky -- ditto for everything else in the sky.
OR
- If you know where two objects are in relation to you and to each
other, then you can calculate where every other object is. For
example -- look again at the sky chart. If you can measure precisely
the angle of view from your location to Procyon and Rigel, and the angle
between these two objects, then you can calculate the angle at which you
must look to see Castor (or any other object)-- you don't need to know where
you are, you just need to know the angle to each object you are seeing.
This works because everything in the universe is in a fixed position
relative to everything else.
Because of the regularity of movement and position in the universe relative
to date, time, and observer location, we can program a computer to calculate
where to look in the sky if the computer is told:
- EITHER, observer location, date, and time; OR,
- The location of two known objects.
With this data, the computer can tell you where to look -- or -- better yet,
the computer can control motors that drive your telescope and point it for you.
GOTO vs. PUSHTO
The capability of a computer to calculate where objects are in the sky and
then to move a telescope so it points to that spot has given rise to two types
of automated or semi-automated telescopes -- GOTO scopes and PUSHTO scopes.
- A GOTO scope is driven by a motors that are controlled by a computer --
tell the computer your location, date, and time and it will calculate where
each object is from your vantage point. You then select from the
computer's database the object you want to see, push a button, and the
computer moves the scope so it's pointing at the object. Every
telescope manufacturer makes several models of GOTO scopes. I owned a
Meade ETX-90 GOTO scope until it was destroyed in
Hurricane Katrina. The scope was accurate, provided I fed to it the
exact location, date, and time -- I obtained that information from a GPS
receiver so the input data was accurate. I would set up the scope,
turn it on, tell it the location, date, and time (actually, I had an
application that allowed the scope to read the data from a GPS receiver);
the scope would "beep" when it was ready; it would go to two stars and ask
me to center the stars in the field of view, just to check alignment; then,
I could tell the scope to GOTO a certain object, the motors would grind
away, the scope would move and "beep" to tell me it was at its destination
-- and there would be the object in the middle of the field of view.
- A PUSHTO scope, on the other hand, has a computer that tracks where the
scope is pointed and that will calculate where to move the scope to see any
object -- but -- the PUSHTO scope does not have motors to move it -- you
push or pull the scope in the direction indicated by the computer until the
computer tells you the scope is pointed at the right spot in the sky to see
what you want to see. The XT-12 Intelliscope is a PUSHTO scope.
The following paragraphs describe how it works.
The Orion Intelliscopes
The following information applies to all the Orion Intelliscopes, although I
use my XT-12 as the example.
Remember the earlier discussion in which I said: "If you know
where two objects are in relation to you and to each other, then you can
calculate where every other object is. For example -- look again at
the sky chart. If you can measure precisely the angle of view from your
location to Procyon and Rigel, and the angle between these two objects, then you
can calculate the angle at which you must look to see Castor (or any other
object)-- you don't need to know where you are, you just need to know the angle
to each object you are seeing. This works because everything in the
universe is in a fixed position relative to everything else." Well,
this is how the Intelliscope works -- it measures the angle from you to two
objects and the angle between these two objects, then, when you ask, it tells
you where to go to find any other object.
I will describe how to use the Intelliscope computerized controller and you
will understand how it works.
First, here is a view of the XT-12 with the Intelliscope controller
connected. In this photo, the controller is the small handheld device with
the coiled cord connected between it and the scope base.

Controller: Up-close view and the keys
Here is a close-up of the controller.

Most of the keys on the controller have two functions, as shown in this
chart:
Label #1 |
Label #2 |
Functions |
1 |
M |
Enter number 1; Find a Messier Object |
2 |
NGC |
Enter number 2; Find an object in the New General Catalog |
3 |
IC |
Enter number 3; Find an object in the Index Catalog |
4 |
Nebula |
Enter number 4; Find a Nebula by name of constellation in which
it is located |
5 |
Cluster |
Enter number 5; Find a Star Cluster by name of constellation in
which it is located |
6 |
Galaxy |
Enter number 6; Find a Galaxy by name of constellation in which
it is located |
7 |
Planet |
Enter number 7; Find a Planet |
8 |
Star |
Enter number 8; Find a Star -- Named; Double; Variable; or,
Catalog (ST) |
9 |
User |
Enter number 9; Find an object that you, the User, have entered
into the database |
ID |
(none) |
Identify the object at which the scope is pointed |
0 |
Tour |
Enter number 9; take one of the 12 monthly tours of the sky to
see the objects most visible this month |
FCN |
(none) |
Find an object by astronomic coordinates (decl and RA); realign
the scope during an observing session |
Enter |
(none) |
Same as "Enter" button on the computer keyboard |
UP arrow |
(none) |
Scroll up through data on the controller screen |
DOWN arrow |
(none) |
Scroll down through data on the controller screen |
POWER |
(none) |
Turn the controller on or off; change the contrast and
brightness of the screen |
The controller uses a single 9-volt battery. I don't
know how long the battery lasts but it's always smart to have a couple of
spare batteries anytime you are using a device that requires batteries.
How it works
Embedded in the scope base are two encoder disks. These disks rotate as
the scope is moved from left to right -- AZIMUTH, or, az -- and as the OTA (the
long tube that contains the optics) is moved up and down -- ALTITUDE, or, alt.
- Look at the photo of the scope -- see the round part sitting on the
ground? There are actually two parts to this base plate -- upper base
plate and lower base plate. The lower base plate -- not visible in the
photo -- has feet that sit on the ground, it does not move. The upper
and lower base plates are connected by a single bolt that runs through their
center. Sandwiched between these two plates are several Teflon pads,
which are slippery. When you try to move the scope right or left, the
bottom plate will not move but the top base plate slides across the Teflon
pads, allowing the scope to rotate in azimuth around the axis established by
the bolt that connects the two sections of the base plate. Also
between the upper and lower base plates is the azimuth encoder disk -- as
the upper plate moves around the lower plate, the encoder measures how many
degrees the upper plate -- and hence, the scope -- has rotated. This
data is fed to the handheld controller as the azimuth movement data.
- Look at the photo of the scope again. Notice that there is a knob
to the right of the controller -- look at the optical tube assembly (OTA)
behind the knob and you will see the edge of a large round bearing -- the
OTA rides on tow of these bearings that swivel on bumpers set inside the
upright part of the base. There is a close-up and a better explanation
of this on page 2 of the XT-12 article.
Sandwiched between one of the OTA bearings and the upright is another
encoder disk that measures how far out of vertical the OTA has moved; that
data is fed to the controller as altitude data.
- Thus, the scope is now able to tell the controller how many degrees it
has moved right or left and up or down. If the scope knows its
starting point and knows the degree of travel from the starting point to two
known stars, the controller can then calculate where every other star is --
because it knows the direction to two stars and the angular distance between
them.
To use the Intelliscope controller:
- When the scope is assembled, there is a vertical stop that must be
adjusted using a carpenter's level to ensure that when the OTA is against
the stop, it is pointed exactly vertical.
- To use the Intelliscope controller, you must have some familiarity with
the night sky -- that is, you must be able to locate at least the brightest
stars. You can do this with a star chart or a planisphere.
- Set up the scope.
- Identify two prominent stars -- they should be bright enough for you to
find them without difficulty and they should be 60 degrees apart.
Remember their names and where to find them.
- Plug in the controller, turn it on.
- The controller display will show the command PLACE THE SCOPE VERTICAL.
- Move the OTA so it is against the vertical stop, pointing straight up.
- Hit ENTER.
- The display will then tell you to select the first alignment star.
- Using the UP and DOWN arrow buttons, scroll through the list of
alignment stars until you find one of the two stars you have located.
- DO NOT PUSH ANY BUTTONS.
- Move the scope until alignment star #1 is in the center of the field of
view through the eyepiece -- take your time, make certain you have the right
star and make certain it's centered in the eyepiece.
- When the first alignment star is centered in the eyepiece, hit ENTER.
- The display will then tell you to select the second alignment star.
- Using the UP and DOWN arrow buttons, scroll through the list of
alignment stars until you find the second of the two stars you have located.
- DO NOT PUSH ANY BUTTONS
- Move the scope until alignment star #2 is in the center of the field of
view through the eyepiece -- take your time, make certain you have the right
star and make certain it's centered in the eyepiece.
- When the second alignment star is centered in the eyepiece, hit ENTER.
- The controller will then display a number between 0.0 and 51.0 -- this
is a measure of the quality of your alignment, it's known as the "warp
factor." You want warp factor to be less than 0.3 or 0.4.
A warp factor of 0.5 and up is not a good alignment -- turn off the
controller, return the scope to vertical, and do it again. On my first
attempt, the warp factor was 0.3; my warp factor is always 0.1 to 0.3, it's
not difficult.
- Now, the controller is ready to find objects. For example:
- If you want to find a STAR, push the 8/STAR button and use the UP or
DOWN arrows to scroll through NAMED, DOUBLE, VARIABLE, or INDEX stars.
Let's say you want to find Arcturus -- scroll through the STAR choices
to NAMED and hit ENTER. Then, scroll through the list of names
until you find Arcturus and hit ENTER.
- If you want to find a MESSIER object, press the 1/M button and the
display shows M001. Press two or three digits corresponding to the
number of the Messier object you want to see -- if you enter two digits,
hit the ENTER key and the controller calculates where to go; if you
enter three digits, no need to hit the ENTER key. For example, to
find Messier M31, just press the 3 key, the 1 key, and the ENTER key.
To find Messier object 101, enter 1, 0, 1 -- don't hit the ENTER key.
- When you select the object you want to find and hit ENTER, the
controller will then display two arrows -- one pointing left or right, one
pointing up or down. Next to each arrow is a number -- the higher the
number, the farther you must move the scope in the indicated direction.
- Move the OTA left/right, up/down, watching the numbers next to the
arrows. When the number drops below 10, it then shows the number to
one decimal place -- e.g., 8.7. Move the scope until both sets of
numbers read 0.0.
- Look through the finder scope and there is the object you were seeking
-- center the object in the finder scope and there you have it.
Here is a photo of the controller moving to the Whirlpool Galaxy (WHIRLPOOL
GA) in the constellation Canes Venatici (CVN). In the photo on the
left, the controller is telling you to move the scope to the right 34 degrees
and up 12 degrees. As the scope is moved, the encoder wheels tell the
controller how far the scope has moved in azimuth and altitude -- as the scope
moves, the distance to be moved decreases -- in the center photo, the scope
still needs to move 7.6 deg right, 5.7 deg up. In the last photo, the
scope is now pointed at the Whirlpool Galaxy -- 0.0 deg right/left, 0.0 deg
up/down. Stop moving the scope and start observing.

If you are looking for a planet -- there is an extra step. When
you hit the 7/PLANET button, the controller asks for the date and year.
Enter this information and the computer calculates where each planet is then you
can find them. Read the instruction manual because the day, month, and
year must be entered in a specific manner.
Why does this work? Because --
- When you point the scope straight up, the encoders tell the controller
the scope is vertical. The controller than sets its internal readings
to 90.0 ALTITUDE and 0.0 AZIMUTH.
- As you move to the first alignment star, the encoder wheels track how
far and in what direction the scope moves, in degrees, up or down, right or
left. When you hit ENTER, the scope knows that the first alignment
star is XX degrees from vertical and YY degrees in azimuth from where it
started.
- As you move the scope to the second alignment star, the encoder wheels
track how far you move up/down, right/left FROM THE FIRST ALIGNMENT STAR.
When you hit ENTER, the controller now knows how many horizontal and
vertical degrees it is between the two alignment stars. The controller
knows where these two stars are in relation to each other and to every other
object in its database -- because it has a star almanac in its memory.
- If the controller knows the azimuth and altitude to two stars, it knows
the angular distance between the two, and it can now calculate the location
of any other object and can tell you which direction and how far to go to
find the object you want to find.
- Think about it and you'll see just how simple this is.
The Intelliscope controller does not have every single known object in the
universe in its memory. Instead, it has the following in its database:
- 110 Messier objects
- 7,840 New General Catalog objects
- 5,386 Index Catalog objects
- 8 planets
- 99 user-defined objects
Here is a link to a PDF version of the Intelliscope instruction manual -- it
is detailed and easy to use.
http://www.telescope.com/text/content/pdf/IN_229_E_CompObjectLocator.pdf
My impressions after using the Intelliscope
Compliments: I
like the Intelliscope controller; I find it easy to use and accurate.
You don't have to use the Intelliscope controller -- the scope works
just fine without it. If I want to star-hop, or just look at one
or two objects, there is no need to use the controller. Just don't plug it
in -- leave it in the house or in your eyepiece case and use the scope as a
normal Dobsonian scope.
The Intelliscope is accurate and easy to use. The first
time I used the Intelliscope, I used
it for two nights, locating 30 different objects. In every case, after I
had pushed the scope to where the display showed 0.0 and 0.0, the object was in
the finder scope. If I was using a high magnification eyepiece -- over
225X, there were a couple of times when the object was not in the eyepiece but
was just slightly out of the field of view -- I found these with no problem. In
every other case, the object was in the eyepiece
when the controller showed 0.0, 0.0.
Alignment is easy but you do have to pay attention to what you're doing
-- it's sometimes a chore to find the alignment stars but if you choose a bright
star and are competent with your scope, this is not a problem. I use a
Telrad finder and a 9X50 correct angle finder -- this combination
allows me to locate my alignment stars quickly.
Complaints: I
have only two minor complaints.
The Intelliscope controller does not like to get cold.
The two nights I have used the Intelliscope, the outside temperature was in the
low 20's. After about 20 minutes of being very cold, the display dimmed
and the controller responded slowly. It still worked, just noticeably
slower than when it was warm. I am going to try using a hand warmer
strapped to the controller with a couple of rubber bands and see how that works.
The controller did not fail to work when it got cold -- it just ran very slowly.
The labels on the controller buttons are easy to read -- but --
I wear tri-focals which I take off when I am using the telescope.
It's a real chore to put my glasses on to read the buttons, take them off the
look through the scope, put my glasses back on to read the buttons, take them
off again to look through the scope, and back and forth with the glasses -- so, I leave my glasses off.
It's a bit difficult for my old eyes to read the buttons. The buttons are
big enough and the type is big enough -- and they are back lighted -- but be
advised if you wear glasses you might have difficulty reading the labels without
your glasses.
UPDATE: When you assemble the Intelliscope, the instructions
tell you to set the base on a perfectly level surface. Then, you install
the OTA onto the base and stand it vertical -- using a level, check to see that
the tube is vertical. There is an adjustable stop on the base that
you adjust to ensure the OTA is vertical in relationship to the base.
When you use the Intelliscope, you start off with the OTA vertical -- then --
turn on the handheld controller, find two alignment stars, and align the scope.
It is easy to misinterpret the instructions about the OTA being vertical -- read
carefully:
- When you assemble the scope, set the base on a perfectly flat
surface -- check with a level -- install the OTA, stand it vertical, measure
the OTA for plumb, and adjust the stop on the base so that the OTA is
aligned perfectly vertical in relationship to the base.
- When you use the Intelliscope controller -- set the
scope on the ground, plug in the controller, DO NOT TURN THE CONTROLLER ON,
then move the OTA to its vertical position against the stop. This does
not mean that the OTA must be perfectly vertical -- that is, if the scope is
on rough or un-level ground -- which is common -- the OTA will be slightly
out of vertical -- that's fine because the OTA, when it is against the
vertical stop on the base, is vertical in relationship to the base -- the
scope doesn't care if it's not on level ground.
Carefully read the Intelliscope instruction manual and it tells you the
scope does not have to be on level ground after it has been assembled.
- HOWEVER -- sometimes it's not possible to find a good spot to set
up the scope, especially if you are at a viewing location that is on rough
ground. For this reason, I made a leveling platform that I can use in
case the place where I set up the scope is really rough. This article
shows how I built my leveling platform. I rarely use this platform --
just find a patch of ground that's reasonably flat and plunk the scope down
there, but, sometimes I am at a location where the ground is quite rough and
this platform comes in handy to keep the scope sitting on a solid
foundation.
Here is a link to the
first of two pages describing the XT-12 Intelliscope -- complete with photos
and links to the manufacturer's site.
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