Courtesy of
Sky & Telescope
May 1990 |
S & T Test Report
THE ADVANCED ASTRO MASTER
by Dennis di Cicco
Lest anyone doubt that
the electronic revolution has a firm grip on amateur astronomy, flip through the
advertisements in this issue. The products range from simple electric focusing
motors to sophisticated CCD cameras and autoguiders. And though computers
themselves aren't touted, there's no shortage of companies selling astronomical
software.
This revolution hasn't happened overnight. Indeed, I've
enjoyed watching it develop over the years. When I began reading Sky & Telescope in
the early 1960's, the sole electronic gadget advertised was a transistorized
drive corrector. What has impressed me of late, however, is not the extent of
the revolution, but how rapidly it is gaining speed. No sooner does someone
wonder aloud, "Wouldn't it be nice if?" then the item appears on the
market.
A perfect example is Celestron's Advanced Astro Master.
In the September, 1988, issue, page 258, I reviewed the very impressive digital
setting circles sold by several companies. Not only were they accurate and well
made, but they were also the first to work with altazimuth as well as equatorial
mountings. Furthermore these circles needed no alignment of the mounting. You
just initialized them by pointing the telescope at two bright stars and pressing
a button, and an internal microcontroller made all the necessary coordinate
transformations to provide real-time readouts of right ascension and
declination.
The obvious wouldn't-it-be-nice idea was to couple
these readouts to an electronic catalogue of stars and deep-sky objects, thereby
making an extremely "user-friendly" CAT (computer-aided telescope). Viola,
enter the Advanced Astro Master.
In a nutshell, the Astro Master is a pair of shaft
encoders linked to a 4½-by-3-by-1¼-inch package that weighs 6½ ounces
complete with its 9-volt battery. The unit retains all the features of the
earlier digital setting circles and combines them with four internal catalogues.
It also has a stopwatch-type timer and a computer-assisted method for polar
aligning an equatorial mounting. There is also a simple one-step method for
aligning the Astro Master with the sky. The real power of the unit, however, is
that you can access any object in the catalogues and have the Astro Master
direct you to it regardless of the type of telescope mounting you are using or
whether it is aligned.
ASTRO MASTER AT WORK
Here's an example of how
the Astro Master works when attached to the Celestron Ultima 8-inch Schmidt-Cassegrain
telescope that was reviewed in both the December and January issues. On a cold,
clear winter evening I plunked the tripod and wedge down on sloping ground
behind my house. I completely ignored polar alignment and left the polar axis
pointed about 30º west and somewhat below the celestial pole.
When the Astro Master was turned on, it prompted me to
turn the scope until the declination circle (the mechanical rather than
electronic one) read 0º, after which I hit the "enter" button. This
gave the unit's microcontroller a reference point where the optical and polar
axes were perpendicular to each other. That done, the display automatically
advanced to the "align star" mode. I centered Altair in the scope's
eyepiece and selected Altair from the Astro Master's list of 30 alignment stars
(the names appear on the display as you cycle through the list with the
"up" and "down" buttons). I hit the enter button again. Now
I moved the scope to Aldebaran, rising in the east, and repeated the procedure.
All this took about 1½ minutes, and I was ready to
begin deep-sky observing. Andromeda was nearly overhead, so I switched to the
Astro Master's Messier catalogue, entered the digits 31, and switched to the
"guide" mode. Even though I was new to the Astro Master's operation,
this took maybe 15 seconds. The unit instructed me to swing the scope west and
north until the display's indicators zeroed (they counted down the angle that
each axis had to turn as the scope was moved). Sure enough, the bright glow of
M31 was nearly centered in the 30-mm eyepiece field.
Off to the south I could see one of the companion
galaxies. Pretending that I didn't know whether it was M32 or M110, I centered
the object in the field and switched the Astro Master to the
"identify" mode. Pressing two buttons was all it took to ask what was
the nearest Messier object to where the telescope was pointed. Almost instantly
the display responded with M32. One more button press and words scrolled across
the display telling me that this was an 8.2-magnitude elliptical galaxy in
Andromeda. A few more button pushes and the unit guided me to the other
companion, M110.
Remembering that there is a rather nice planetary
nebula somewhere about a dozen degrees west of M31, I swung the scope to its
approximate location and switched to the identify mode. This time the display
replied that the nearest NGC object to where I was pointed was NGC 7640. That
number didn't rind a bell, and, sure enough, one button press informed me this
was an 11.5-magnitude barred spiral galaxy. It seemed interesting, however, so I
switched to the guide mode and moved the scope as indicated. What an unusual
splinter of light! I couldn't recall having seen it before, but it was certainly
worth noting.
I nudged the scope a little northward to where I
thought the planetary would be and tried the process again. Success! NGC 7662
was a bit to the southeast, so I moved the scope as instructed and found the
planetary almost smack in the middle of the field. All this was pretty
impressive, especially since the scope wasn't anywhere near polar aligned and
the motor drive wasn't even running. During the next hour or so I hunted down
several dozen objects, including some old friends and a few new ones.
INSTALLATION
The Advanced Astro
Master I tested was one of the first off the production line. It arrived in
June, 1989, but was soon followed by a new read-only-memory (ROM) chip. This was
the version 1.38 update of the unit's software. The 28-pin ROM contains half a
megabyte of memory (including some 6,000 lines of computer code that form the
operating instructions). I took 5 minutes and a small screw/driver to swap the
ROM chips.
This also offered an interesting perspective on the
Astro Master. Because there are bound to be mistakes in such a complex piece of
electronic razzle-dazzle (not to mention the huge electronic data base), the
fact that updates are so easily made is comforting to anyone worried that the
unit will soon become obsolete. I've been told that another ROM version with
enhanced user features is in the works. These upgrades will be available to
existing Astro Master owners at a reasonable cost (probably around $30).
In addition to the tiny optical encoders that attach to
each axis of the telescope mounting, the Astro Master arrived accompanied by
brackets, gears, screws, bolts, and metal covers. These were the materials
needed to fit the unit to all but the earliest Celestron 8 fork mountings as
well as the Super Polaris German equatorial mounting. Because I installing it on
the newer Ultima, most of this hardware was unnecessary.
That's not to say installation was a snap, even though
the Ultima appears to be the first Celestron telescope manufactured with the
Astro Master in mind. I still had to swap the left and right fork arms — a job
decidedly more complicated than you might deduce from the one-sentence
instruction in the Astro Master's manual. Furthermore, I had to drill a hole in
the fork arm to attach one bracket. Installing the Astro Master on other
Celestron telescopes requires additional drilling or disassembly. While none of
this is especially demanding work, it will intimidate the mechanically faint of
heart.
Telescope makers should note that it would be rather
easy to attach the Astro Master to just about any homemade mounting I've ever
seen, whether altazimuth or equatorial. The encoder can be driven directly (1:1
drive ratio) by the telescope axes or connected with gears and the like as long
as the drive ratio remains between 1:1 and 1:4. (This ratio is specified by the
user during the one-time setup of the Astro Master's software.)
ACCURACY
Each optical encoder
resolves 2,048 steps, or slightly better than 0º.18. The right ascension is
displayed to 1 minute of time, while the declination counts "1, 2,
3,..." which stands for 10', 20', 30', and so on. In addition to the tests
mentioned earlier, I also set up the scope as an altazimuth and then used it
precisely polar aligned. The Astro Master's microcontroller handled all three
modes with ease, putting almost every object I searched for well within the
field of a low-power eyepiece.
The unit seemed slightly more accurate when the
mounting was polar aligned. Rick McWilliams of Tangent Instruments, who designed
and manufactures the Astro Master for Celestron, explained that the improved
accuracy is the result of the simpler internal calculations needed for a
polar-aligned mounting. This, in turn, allows using the maximum accuracy
available from the shaft encoders.
Overall, I suspect that the greatest source of error
will not be the Astro Master's encoders or calculations but rather the
mechanical limits of the telescope it is attached to. The mountings must have
their axes precisely perpendicular to each other for the Astro Master to give
optimum performance. Furthermore, especially with German equatorial mountings,
it is important to have the telescope's optical axis perpendicular to the
declination axis. Errors that arise from a failure to meet theses conditions are
relatively small if the telescope is sweeping only one part of the sky on which
the Astro Master is "aligned." They appear magnified when moving the
scope across a large expanse of the heavens as when moving from the western to
eastern sky.
If you find that objects are not falling near the
center of the eyepiece field, there is a simple solution. Center the telescope
on any known object called up from the Astro Master's catalogues, switch to the
"align" mode, and hit the enter button. The unit is now initialized on
that part of the sky.
THE CATALOGUES
The heart of the Astro
Master is its data base stored in four catalogues. The first contains 363 stars,
including multiples and noteworthy colored stars. Accessing objects from this
catalogue isn't easy since it's done by a star number you have to look up in the
manual. For example, you can only access the beautiful, colored double star
Gamma Andromedae by calling for star 29. Once you call this number, however, a
single button press will scroll information across the display telling you that
the star is 2.2-magnitude Almach and a colorful double.
Another of the Astro Master's catalogues contains all
110 Messier objects and correctly lists M40 and M73 as asterisms, M102 as a
duplicate observation of M101, and M91 as the spiral galaxy NGC 4548 in Coma
Berenices, which is the widely accepted candidate for this once-missing Messier
object. The largest of the Astro Master's catalogues contains 7,840 deep-sky
entries from the Revised New General Catalogue of Nonstellar Astronomical
Objects by J. Sulentic and W. Tifft.
Lastly there is a "user" catalogue that holds
up to 25 objects. These could be positions of planets, asteroids, comets, or
perhaps selected variable stars. To make optimum use of this catalogue the user
must enter the positions in equinox 2000.0 coordinates. The information is
stored in a special nonvolatile memory that is retained when the power is turned
off and even when the battery is removed. McWilliams says that this memory can
be over-written (changed) at least 4,000 times without damage and, by one
estimate, can be changed 100,000 times.
It was impossible to check the accuracy of every entry
in the Astro Master's catalogues, but only a fool would expect them to be free
of errors, especially in early versions, of the software. Indeed, as Murphy's
law would have it, the very first object I tried to find with the unit, NGC 246
in Cetus, had the wrong sign on the declination.
The only other outright error I found was that the
nebulous knot NGC 604 in the outer arm of M33 was listed as a galaxy. But there
were also inconsistencies. such as the descriptions of M32 and M110 being very
different depending on whether they were called from the Messier catalogue or
from the corresponding entries in the NGC catalogue. Little things like this
ought to be ironed out in later releases of the software. I certainly don't feel
these error should delay a purchase of the unit.
The instructions that were shipped with the Astro
Master were pretty good, especially considering this was an early model. Some
seemed a bit confusing, but a few minutes of pressing buttons while reading the
instructions cleared up any questions I had.
At first I was leery of having only four buttons to
control all the Astro Master's features. I thought this would be especially
annoying when entering numbers, since it means you would have to scroll through
the digits 0 to 9 to get to the number you want. I assumed that entering a
four-digit NGC number would be a pain. But in practice, the scroll up and down
buttons make this task very efficient, especially in the dark. Once I got the
hang of it, it took only seconds to enter any number. Furthermore, the large,
well-separated buttons were easy to operate even while wearing mittens!
Both Jim's Mobile Industries and Lumicon sell
variations of the Astro Master with mounting hardware to fit telescopes other
than Celestron's. These include the fork-mounted Schmidt-Cassegrains by Meade
and most Dobsonian designs. Both companies also have versions of the device that
use shaft encoders with twice the resolution of those I tested. My guess is that
these would have the most noticeable improvement only on telescopes with
extremely accurate mountings as mentioned above.
Ever since the first CAT was introduced a few years
ago, I've listened to countless arguments for and against computer-aided
telescopes. No doubt the debate will continue. I see valid points on both sides,
but people always seem to take extreme positions. Where are the moderates in
this debate?
I look at CAT's as electronic catalogues to be used
right at the telescope. They have given me a chance to check out objects that
I'm sure I would have ignored while I was sitting at a desk planning my night's
observing with conventional charts and catalogues because they seemed too small,
too faint, or too far from an easy guide star. And every time that little voice
in my head gets too loud telling me I'm not being a "real" amateur,
well, I just reach down and turn off the Astro Master. It's that easy to go back
to the one-on-one relationship I've had with the stars for nearly 30 years now.
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