Do You Need a Computerized Telescope?
It's a good question, especially if you are just getting into astronomy. It's even a good question for those who've been in the hobby for awhile but have yet to experience a computerized telescope.
What is a Non-Computerized Telescope?
Before we delve into computerized telescope, perhaps we should first talk about the old standby telescopes of past and present that are not computerized. They exist is all types, in many different types of mounts. The simplest is the telescope on an altazimuth mount. below is an example of a simple, home-made in fact, Pipe Fitting Altazimuth Mount.
This type of mount lets the telescope move around a vertical axis (azimuth) and up and down (elevation). It is the simplest to implement, cheapest to purchase, and generally one of the most steady. The Orion 10105 VersaGo II Altazimuth Telescope Mount is an example of a commercially manufactured altazimuth mount. If you view it, notice that it has setting circles on both axes. The pipe fitting mount I made also has setting circles, shown below:
You can find most any type of telescope available on an altazimuth mount, including refractors, reflectors (like Dobsonian telescopes), and even Cassegrains.
These telescopes are certainly not the only altazimuth mounted telescopes on the market, but represent some examples, from refractor to Maksutov, to Dobsonian. Each has the basic altazimuth function of being moveable in azimuth (left/right) and elevation (up/down). Note in each case the mounts look very simple, and they are. Most any altazimuth mounted telescope is a good bargin if optics is your concern. The reason is that they the mounts in each case are inexpensive to manufacture, yet are generally quite stable. So the bulk of the purchase is in the optics.
So what's the pros and cons of having a telescope on an altazimuth mount?
Altazimuth mount pros:Altazimuth mount cons:
Equatorial Mounts
In the past, one common solution for the inabilty of simple altazimuth mounts to track celestial objects was the equatorial mount. My f/5 Newtonian telescope, shown below, is on such a mount:
You see immediately that this mount looks more complicated. It is basically an altazimuth mount with the vertical axis tilted towards the earth's spin axis. In the northern hemisphere, this basically means that what would be an altazimuth mount's vertical axis is tilted toward Polaris.
In this orientation, the axis aligned with the earth's spin axis is called the Polar axis or Right Ascension (RA) axis. The other axis is called the Declination axis. These axes are analogous to the azimuth and elevation axes of the altazimuth mount, but by being tilted so, the RA axis can compensate for earth's rotation. A clock driven (motorized) equatorial mount just has a motor that rotates the RA axis in the opposite direction of the earth's rotation at earth rate, and thus keeps the telescope pointed at a celestial object.
The implications of this is two-fold.
First, when observing with this type of mount, the user sees an object stay pretty much in the same place in the field of view, and he/she doesn't have keep making adjustments to re-center the object of interest.
Second, the idea of taking pictures of astronomical objects becomes possible. The length of exposures a person can make through a clock driven telescope depends upon the quality of the mount, and the alignment accuracy of course.
The equatorial mount is still sold, most often on 4.5 to 8 inch Newtonians like mine shown above. Below are some examples of what's available with this type mount:
The above examples include common options in the reflector and refractor models. The particular ones displayed give less tedious observing because only the RA axis needs repeated adjustment, and clock drives are available for many models. So what are the pros and cons?
Pros of classical equatorial mounts:Cons of classical equatorial mounts
Fork Mount Telescopes
The advent of short focus Cassegrain telescopes, similar to my ETX 90 Maksutov (shown below) ushered in the fork mount. The image below of my ETX 90 shows the typical fork mount:
The fork mount is in actuality a variation of the equatorial mount. The base is tilted to point the rotational axis at, you guessed it, the earth's spin axis. So the tilted base creates a right ascension and declination axis. Like with the classical equatorial, in this orientation only the polar axis needs to be adjust to remain on a target. The short barrel Cassegrains made possible the very compact fork mount, many with a clock drive mounted in the base. Even this modest Meade ETX 90 telescope has a clock drive and drive gear mounted in the base.
For a time the fork mount in the equatorial orientation was quite popular. It was much easier to implement a clock drive into the base of a compact Cassegrain than to implement a clock drive on a heavier classical equatorial mount hosting a large refractor or Newtonian telescope.
Here are the pros and cons of the fork mount:
Pros of the fork mountCons of the fork mount
Going Modern with Computerized Telescope
The big equatorial mounts and compact fork mounts dominated the amateur telescope world for a number of decades. In the last couple of decades what has come to prominence is the computerized mount. These mounts use a small onboard computer to hold catalogs of thousands of celestial objects, plus do the computations to help align the telescope and track objects. They look like a basic altazimuth mounts in that the telescopes move in azimuth and elevation. An example is my Celestron NexStar 5SE:
Notice the simple straight up and down style, no tilted axis. The magic that makes this design possible is that the mount has two motors instead of the older classical equatorial mounts and fork mounts with their one motor. The reason for two motors is that the earth isn't rotating around the observers local vertical (unless he/she's at one of the earth's poles). So the rotation rates of azimuth and elevation must be constantly adjusted to make up for that.
That's another area where the onboard computer comes in. Once the computer knows the telescope's geographical location and that the mount is aligned, the necessary drive rates are computed and applied by the computer for any pointing angle.
So in practice, one uses a hand controller attached to the mount to align the telescope for the evening, then simply selects objects with the same controller and the computer positions the telescope to the selected targets. Pros of the Computerized Mount
Cons of the COmputerized Mount
So When Do You Need a Computerized Telescope
The cost tradeoff is clear, a more sophisticated mount costs money. So a computerized telescope costs more per aperature than a simpler mounted telescope. For example, at the time of the writing of this article, you could purchase an 8 inch Dobsonian telescope on it's simple wooden mount for about $600, or you could purchase a 5 inch computerized telescope for about the same money.
An 8 inch telescope has a resolution of about 0.56 arc-seconds versus a resolution of about 0.9 arc-seconds for a 5 inch. So you can detect (seeing permitting) lunar and planetary detail of nearly half the size with the 8 inch.
An 8 inch telescope has about 2.5 times the light gathering power of a 5 inch, which reveals another magnitude of stars. So you can see that for the money, optical power is definitely more available with a simple, altazimuth mount.
But on the flip side, a smaller computerized mount may actually let you see more objects, because it will locate objects for you. If you've ever struggled to star-hop a non-computerized telescope to a target that isn't naked eye visible, then you know what I mean.
A smaller computerized telescope will certainly be more compact, lighter, and more portable. Plus, the computerized mount will give you some short-time (30 seconds or shorter) photographic capability.
And most of the modern computerized telescopes can be operated in
an equatorial mode (tipping the vertical axis toward the earth's pole),
allowing photography with longer exposure times. My Celestron NexStar 5SE has a base that has a rod that can
be used to hold the base at the proper equatorial angle. Some other
models require purchase of a wedge
that sits on top of the
tripod, and has the telescope base mounted to it. In that way, the
telescope is in equatorial mode.
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