Ways to Improve a Newtonian Telescope


The Quest for an Optimal Telescope

It's been several years since I purchased my 6 inch f/5 Newtonian from Discovery telescopes. No longer available from Discovery, virtually the same model is the Orion 9827 AstroView 6 Equatorial Reflector Telescope .

The 6 inch f/5 Newtonian is classified as a Richest Field telescope. A Richest or Rich Field telescope is designed to reveal the maximum number of stars to the observers eye. Short focus telescopes of moderate aperture are designed to do this, and the f/5 Newtonian is one of the more popular and capable options for this type of telescope.

It turns out that the mount and telescope I purchased were made in Taiwan. Discovery imported the mechanical parts and added their own optics. In my case, a lime-glass mirror objective.

I chose the unit after months of shopping. I'd always used telescopes I constructed myself (usually with purchased optics), but I'd never owned a sizable commercial instrument. This wasn't a matter of ego, but originally because I didn't have much money to put into telescopes, then later because making my own telescopes had become a matter of habit.


6 Inch Newtonian on EQ Mount

I found that Discovery at the time had two instruments with prices and features that caught my eye. Those were an 8 inch f/5 Newtonian and a 6 inch f/5 Newtonian, both delivered with an equatorial mount. The difference in price at the time was only about $100. Calling Discovery, I found that both telescopes shipped with the same mount.

I'm sure a lot of people would question my decision to go for the 6 inch (shown here) over the 8 inch. A lot of experienced amateur astronomers think one should always go for the greater aperture. But my reasoning was tempered by several considerations.



The Reasoning Behind the Purchase

First, I figured that if the 8 inch unit was even barely adequately supported with the equatorial mount, the 6 inch should be very stable. Second, I'd found during the previous couple of years that I really did a lot more observing when I gave away my old 8 inch DOB and all I had left was a small Jaegers refractor. It seemed that portability translated to more viewing, for me at least.

So what I wanted was the maximum aperture I could use in a portable package. I considered an 8 inch SCT, but I remember watching a friend of mine set up his Celestron C8, and could see that while the 8 inch SCT telescope is compact, scope and tripod together aren't that portable.

Looking at the combined weight of the Discovery 6 inch Newtonian and the mount (total of 35 lbs), I thought I'd be able to move the unit around my yard while the scope was fully assembled. If so, it would save me a lot of time and give me a good combination of portability and power.

I'm happy to say that my expectations were met on both fronts. The mount is very stable and easy to use with the 6 inch on it, and I can move the entire unit without disassembly.



Considering Scope and Mount Combination

The decision I made considered the mounted telescope as well as the telescope itself. I chose a more moderate telescope because I knew that the mount that came with it would be sturdy, given that it was also used on bigger telescopes.

Interestingly, I've read a number of articles where amateur astronomers have been making the same calculation when considering a couple of other very popular telescopes. It turns out that the Celestron NexStar 6 SE Telescope and the Celestron NexStar 8 SE Telescope both use the same mount. While most people go for the legendary 8 inch version of the Celestron SCT, a lot of people, thinking about steadiness of mount, have gone with the 6 inch version. For their decision they save a few bucks, get a more portable telescope (as I did with my f/5 Newtonian), and get a telescope and mount combination that is more sturdy.



The Flies in the Ointment

For a time, I did find some things I didn't like. First views through the telescope were disappointing. While views of star objects have always been spectacular through the instrument, planetary images were especially poor. Images in my 2 inch Jaegers refractor were at least as good.

I determined that while well packed when shipped, the unit had arrived in poor alignment. It took me some time to re-learn how to align a short focal ratio telescope.

Sadly, even when properly aligned, the telescope performed poorer on planetary images than I expected. Looking into the problem a bit further, I found that the cause was the barely adequate tube size. The diameter of the thin-walled metal tube that housed the optics was only 7 inches. General ATM guidelines would recommend an 8 inch tube.

The problem this caused was that with short focus eyepieces, the eyepiece focuser extended into the optical path as shown below. Notice that the illustration shows the focuser extending past the edge of the primary mirror, thus blocking off some of the mirror and creating a more complicated and destructive diffraction pattern. This noticeably reduced the quality of the resulting images.



Rehab Step 1: Adjusted The Tube Length

Focuser FOV Intrusion

In the diagram above, a simulated view into the open end of the telescope is presented. The white disk represents the mirror. In this example, the focuser tube is racked in to where typical short focal length eyepieces come to focus. As the illustration shows, this results in the focuser tube extending into the light path. This causes a more complex diffraction pattern and thus lower contrast and resolution images.

One option to fix the focuser intrusion into the light path was to remount the optics into a larger diameter tube. However, I feared that this may destroy some of the portability that I'd purchased the telescope to achieve. In addition, the primary mirror mount was designed to also serve as an end cap for the telescope, and it would be difficult remove the mirror from the existing mount, as it was glued to the mount. I was afraid I might break the mirror if I tried to remove it from the mount.


It seemed that the better option was to modify the existing tube, which is what I chose to do, as shown in the above diagram. This consisted of removing the optics and cutting off some of the rear end of the tube to move the mirror cell forward. I determined how much by observing some distant targets in hills a few miles away with each of my eyepiece and Barlow lens configurations. When I found the maximum intrusion, I measured the amount of intrusion and used this as the measure of how much tube to remove. This moved the focus further out from the side of the tube, and once done the eyepiece tube no longer extended into the optical path. Fortunately, the eyepiece tube had enough travel to accommodate this extended focal point.



Rehab Step 2: Eliminated The Clock Drive Vibration

No sooner had the focuser problem been solved than I discovered I had another design issue that was limiting the quality of planetary views. The clock drive had a vibration (more like a hum) that was enough to obscure details smaller than perhaps 5 to 10 arc-seconds. I could see the planetary images become sharper just by turning off the motor.

German Equatorial Mount w/Clock Drive

Looking on line, I found that JMI had a clock drive that was a direct replacement, so I ordered it. The JMI drive doesn't have the electronic control that my old drive had. It has a slip clutch built in. But it has a synchronous motor that doesn't cause any discernible vibration.

You can see the small clock drive that I was able to obtain from JMI in the image above. It has worked perfectly for years, and with the built-in clutch I can make small RA adjustments with the slow motion controls without loosening the RA clamp. As you can also see, the equatorial mount that came with the telescope has a small polar axis telescope I can use to get good polar alignment.



Rehab Step 3: Got The Bugs Out Of The Spider

3 Vane Secondary Holder (Spider)


With the new, vibration-less clock drive, images got better, but were still not spectacular. During a Mars opposition I noticed that the spikes caused by the secondary spider vanes, shown above, were causing a very distracting amount of light extending from the limb of the bright planet. With six broad spikes bleeding away, details near the limb of the planet were hardly discernible. There was also potential of missing dim components associated with bright stars, because the bright star may throw obscuring spikes.

The 3 element spider on the secondary was part of a plastic fitting that also stabilized the end of the thin-walled telescope tube. Being plastic, the spider vanes were excessively thick in order to have the necessary strength. The vanes were in fact nearly 1/4 inch thick.

I needed, as a minimum, to replace the spider with thinner vanes. I decided to make a more aggressive modification.

Thin Curved Secondary Holder

I removed the thick spider elements, leaving the supporting ring, and fabricated a thin metal curved secondary holder, as shown above. The new secondary mount makes a 180 degree loop and evenly scatters light throughout the field of view, eliminating spikes. The old spider had such thick vanes that nearly 8 pct of the light entering the telescope was being blocked. With the thin metal curved spider, only about 1.5 pct of the light is blocked. So in addition to eliminating spikes, the curved spider increased by a few percent the brightness of the images.

The total length of the curved vane is about the same as the sum of the lengths of the original 3 vanes, so no additional diffraction surface had been introduced. In fact, since the new vane is only about 1/16 inch in thickness, the total diffraction surface is reduced, as well as curved to eliminate spikes.



Rehab Step 4: Trapped Those Unwanted Photons

After all of the previous steps were completed, I found the images finally approaching what I'd anticipated. But in looking at the smooth interior finish of the metal tube that held the optics, I realized I still had another factor limiting performance.

While the inside of the tube was painted flat black, the smoothness of the finish still allowed some specular reflection of unwanted light to make it through to the eyepiece, raising the brightness of the background. Since I view primarily from my backyard, there are occasions when neighbors' porch lights are on, providing stray light that impacted my DSO views.

The problem was exacerbated by the shortness of the telescope tube beyond the eyepiece. An old ATM guideline suggested having the telescope tube extend past the secondary by the diameter of the tube. So the suggested amount of tube extension beyond the secondary for my f/5 telescope was 6.5 inches. The actual extension is about 2 inches. This allows unwanted light from sources several degrees from the target to still enter the tube.

Again, to replace the tube with a bigger, longer one would impact the portability I wanted to maintain. So I did the next best thing. I covered the interior of the tube with black flock paper. Flock paper has a sticky back on one side, and a fuzzy black surface on the other. Because of the fuzzy surface, there are no longer any specular reflections from stray light. Stray light just gets gobbled up by the black fuzz.



Rehab Step 5: Put Eyepiece Holder in Tray

The tripod for the telescope has a utility tray that is suspended between the tripod legs. This tray acts as a tripod leg brace and as a tray for holding eyepieces, etc. The tray has a lip of about 1/2 inch high around the edge to keep things from rolling off of the tray.

Basic Eyepiece Tray

 
Newtonian Telescope Eyepiece Tray

Above you see the tray in the original configuration. The tray is low enough in the area between tripod legs to make for a sizable tray, and one easy to reach. It works pretty well, but tall eyepieces if sitting on end are easy to bump over. And if tall eyepieces or accessories are laid flat, they tend to roll. So I wanted something that made a more sure stable support for eyepieces and accessories.

 

Inverted Tray Insert


So I made a wooden eyepiece holder that could sit in the tray and provide holes to hold eyepieces and Barlow lenses. The illustration shows the tray not in place but upside down. Notice that at the extremities of the triangular insert are about 1/2 inch thick stand-offs. These, when the tray is inserted with the stand-offs on the bottom, hold the tray up from the bottom of the tray, giving a deep enough hole to hold the eyepieces and Barlows securely.

 

Tray Holder In Place


The picture above shows the eyepiece cutouts inserted. This provides 1.25 inch holes to put several eyepieces. Insterted into place, the simple modification holds eyepieces securely so they can't accidently be bumped and knocked over. Of course, it could have been made to hold 2 inch eyepieces with larger holes, or a combination of 1.25 and 2 inch eyepieces.



Rehab Step 6: Replaced the Finder

Rifle LED Sight

The last improvement is one of a subjective nature. The telescope came with a perfectly fine 6x30 finder telescope. But because the main telescope is rather short, I have the tripod set pretty low so that I can often view objects from a sitting position. I do this by loosening the cradle clamps that hold the telescope to the tripod, rotating the telescope within the cradle to put the eyepiece in a convenient position, and re-tightening the cradle clamps.

But because the tripod was set pretty low to accommodate this comfortable viewing arrangement, the finder was too low to conveniently view through. And the finder being a telescope, I had to position myself close to the eyepiece. So I replaced the finder with an LED rifle sight. It was given to me, so I figured the price was right. The rifle sight is much like many of the LED telescope finders, lacking mainly a potentiometer for adjusting the LED brightness.

The LED finder sits a bit further out from the telescope, and I don't have to be positioned so closely to the finder eyepiece to be able to spot the red LED and use it for pointing the telescope.



Not Perfect -- But Definitely Not Bad

Tycho Through 6 inch f/5 Newtonian

Now I finally see through the telescope what I want to see. Planetary images are quite good for an f/5 instrument, as illustrated in the Tycho crater image taken through the tuned up Newtonian. The spike-less views are reminiscent of those through a Cassegrain. And with the f/5 focal ratio, the telescope is a great performer on stellar objects.

It has been a long road to get the telescope I bought transformed into the telescope I wanted. The optics made by Discovery are excellent. The mount made in Taiwan is smooth and sturdy. The telescope is solidly constructed, but had design issues that kept it from performing up to its potential. I've taken a few lunar and planetary photos with the Newtonian that show good performance. You can see these at 6Inch Newtonian Astrophotos.

In summary, I made the following modifications to fix design limitations and enhance the telescopes performance:

  • Moved the primary forward

  • Replaced the clock drive

  • Replaced the secondary spider

  • Covered the inside of the tube with black flock paper

  • Placed plywood eyepiece holder in tripod tray

  • Replaced 6x30 finder with LED rifle sight

  • What I ended up with is a high performance 6 inch telescope on a very stable mount that is so portable I can move it in and out of the garage and around the yard without it being disassembled.

    It is a good general purpose instrument operating at f/5, which is what I wanted. I also have an SCT and Maksutov, and they too are portable in this size range. But I don't consider telescopes above f/8 in focal ratio to be that great for general use, especially star target hunting. Many star objects and comets benefit considerably from a wider field instrument.

    It took some time and effort, but in the end I have a pretty nice telescope. In fact, a great telescope. Good but not great as originally shipped, but being the simple design of a Newtonian, it lent itself well to modification by even someone like me. The only issues with the telescope being a Newtonian is the mirror cleaning (once every few years), and the critical alignment. I now use a Cheshire eyepiece to do the alignment, which you can read about on the Collimation web page.




    Addendum


    I've used the telescope described in this page for many years and it has been a good performer. My main take is that it can even deliver quite fine planetary performance, but only if accurately collimated. In my efforts to collimate the mirrors over the years, I confess to forgetting that on a short focus Newtonian like this one, collimation is somewhat difficult. I finally accepted that and ordered a Cheshire Eyepiece collimation aid, which has greatly reduced the difficulty of collimating this instrument.

    But in those same years, I've grown older. Old enough that moving the assembled equatorial mount and telescope has become difficult for me, though when I was younger it was pretty easy. In addition, aligning the mount with Polaris, a must for effective use of the clock drive or using the setting circles, has also been made difficult by my advancing age. Alignment is done with the equatorial mount by making use of a built in polar alignment telescope mounted in the polar axis. Its much harder for the current (old) me to get down on my knees to see through that alignment telescope.

    So after thinking about my new preferences, which are relatively portable telescopes that are easy to set up and use and viewing from a sitting position, I decided to do a major reconfiguration of my old trusty f/5 Newtonian. I made a Dobsonian mount for the telescope useing plans from the Stellefane web site: Stellefane Dobsonian Plans .

    The result of my efforts at following those plans is the following new configuration of my f/5 Newtonian. Notice that an eyepiece rack for 4 eyepieces is mounted on the side of the rocker box.

    Newtonian on Dobsonian Mount



    This configuration workes well for me. I can easily lift the telescope off the cradle by the handle on the cradle box, and then move it and the rocker box to my observing location. The combination is much lighter than the same telescope on the equatorial mount. Observing is done from a sitting position, a real plus for me.

    This arrangement uses a needle level (the red apparatus on top of the cradle box}, and azimuth markings on the large base. The advantage of the needle level is that it really doesn't matter if the base of the mount is level or not.

    Needle Level used for Elevation Indication




    Azimuth Indication on Base

     


     




    I find that using the Star Pointer utility with this mount makes locating targets pretty easy. It's difficult to get the base jostled to the position where Polaris appears at a reading of zero azimuth. So I modified the Star Pointer app to allow an azimuth bias entry to make alignment of Dobsonian mounts easier. If I get the mount within plus or minus 10 degrees of north, I can enter the resulting reading when pointing at Polaris as a bias in the Star Pointer app. From then on the listed azimuth values have the initial bias inherent.

    Star Pointer Sample View



    The Star Pointer app offers a selection of the Messier, Caldwell, Herschell 400, and Double Star catalogs to chose from. It will then list all of the objects of the chosen catalog that are currently visible. It lists them from west to east so that the items at the top of the list are ones that may be setting soon. It handily displays the items, their magnitude, and their current azimuth and elevation. Azimuth is listed in both 0 to 360 and +/- 180. It updates the azimuth and elevation every 30 seconds.

    If you have a telescope on an altazimuth mount, and either have or can add setting circles to the mount, I suggest you  give Star Pointer a try.

    Recommendations

    I don't know if the other models similar to this have the issues this one had, but there are models much like this still available. There seem to be more 5 inch options than 6 inch.

    You can find models similar to my Discovery, which would deliver the same combination of significant aperture and portability that I find very conducive to frequent observing.

    You can also get a similar design with a computerized mounting in at least the 5 inch range. That wasn't available when I was shopping, but it certainly is now.

    Telescope Mounts Explained


    The Basic Astronomical Telescope Mounts

    There are many different types of telescopes used for astronomy. But for amateur astronomy, these can broadly be divided into refractor telescopes and reflecting telescopes. Within each of these categories are short versions (short focal length or catadioptric), and long versions. You choose a short focus telescope if you want to view wide star fields, or need a portable instrument, or both. You might choose a long focus telescope if you want to look at high resolution targets like planets, double stars, and the moon, though there are short reflector designs that can do this well.

    As to refractor telescopes, the short ones now available use newer types of glass in the objectives that allow short focal lengths with much less chromatic (color) distortion than older designs. The long refractor telescopes are still made pretty much with crown and flint glass objectives, as these work quite well in long focus designs.

    As to reflector telescopes, they can be further divided into Cassegrain (catadioptric) or Newtonian styles. The oldest design is the Newtonian, invented by -- you guessed it -- Isaac Newton. It uses a parabolic mirror at the bottom end of the telescope as the main light collector and image maker, and a small diagonal mirror at the observing end of the telescope that reflects the image out to the eyepiece. The Newtonian telescope, like the refractor telescope, can be made as either short focus or long focus. However, the performance characteristics vary quite a bit with the different focal ratios.

    Interestingly, the Cassegrain type reflecting telescopes, though very short in physical design, provide more the performance of a long telescope in that they actually have long effective focal lengths.Having a convex secondary mirror on back of the corrector plate considerable reduces the focusing convergence angle, effectively extending the focal length.

    The reason for considering the style of telescope you might most enjoy is that telescope design can have a lot to do with the optimal mounting type for the telescope you choose. As there are different telescope types, there are also different types of telescope mounts. This web page will take you through some of the most common telescope mount types used in amateur astronomy.

    Telescopes used for astronomy, whether Newtonian, Dobsonian, Cassegrain, or Refractor, have two basic types of mounts, with variations of each. The simplest telescope mount is called an altazimuth mount, and the more complex one is called the equatorial mount.

    The altazimuth telescope mount is certainly the simplest, allowing the telescope to be pointed up and down (elevation), and around (azimuth). This telescope mount type is easy to make, can be very sturdy, and works nicely for visual work.

    The more complicated equatorial telescope mount designs are made to facilitate easier tracking of celestial objects, especially for motorized tracking. Each of these come with variations to allow for telescope size and weight, and slow motion or motor control. I'll show here a few of the most common configurations. Incidentally, if you have an altazimuth or equatorial mount with setting circles, the freely available web page utility Star Pointer will also show you where to point your altazimuth or equatorial mounted telescope.

    It is common today for modern telescopes to include not only motor driven mounts, but computerized motor drives that allow you to simply select objects via computer or hand-held controller. After selection, the telescope's computer moves the telescope to point at your selected target. These smart altazimuth mounts also allow automatic tracking, something that could only be done with the more complicated equatorial telescope mounts that were more common before the invention of computerized telescope mounts.

    These modern telescopes use the computer and drive do the work and locate objects and track them for you. You can buy some pretty incredible computerized mounts for even small telescopes in today's market. Look at this iOptron 9502B-A SmartStar-R80 Computerized Telescope - Astro Blue with Carry Bag for example. And you could always mount something like that to a pipe-fitting base for stability.

    If you happen to have, or are only interested in, non-computer driven telescopes, this site has something to offer you. As long as you have setting circles, either in altazimuth or equatorial modes (or are willing to add setting circles), then you can use the Star Pointer utility. Star Pointer is a web page utility designed to list all objects that are above 25 degrees in elevation at your observing location (if you will allow it to keep your location in a cookie). If you want to make some setting circles, you can download the Setting Circle PDF file for a template. Just use a graphic program or copy machine to adjust the size.

    Star Pointer presents any one of three popular target catalogs, and provides a periodically updating coordinate table for the objects visible in your location, with their current pointing angles for either altazimuth or equatorial type mounts. Available catalogs include the Messier, the Caldwell, and the Herschel 400. It might really save you time in finding objects, as it tells you precisely where to point your North-aligned telescope. I use it with my Android smart phone and its web browser.


    The Altazimuth Mount

    Pictured here is a simple configuration of the classic altazimuth telescope mount. The Celestron Heavy-Duty Altazimuth Tripod is a mount of this type -- relatively inexpensive and easy to use.

    The altazimuth type telescope mount has a vertical axis (Labeled Az) that is perpendicular to the ground, and a horizontal axis (Labeled Elev) that is parallel to the ground. Movement of the telescope in the elevation axis points the telescope up or down, with a zero angle being level with the ground. Rotation in the azimuth direction moves the telescope around between the cardinal directions, with zero being North.

    As shown with the 50mm refractor in this picture, such a mount in combination with a small telescope often doesn't even need a counter weight. If you happened to observe from the North or South Pole, the vertical axis would be aligned with the Earth's spin axis. The nice thing about that would be that when you found an object to observe, rotation around only the vertical axis would be needed to keep the object in the field of view. Rotating at the Earth's spin rate in the opposite direction as the Earth's rotation would keep and object motionless in the eyepiece.

    However, for observing from any other latitude on the planet, the vertical axis is not aligned with the Earth's spin axis. This means that to keep an object in the field of view requires motion in both axes. The motion rates will change over time as the elevation angle changes. Tracking objects near the horizon requires mostly changes in elevation, and tracking objects more North or South requires mostly changes in azimuth.

    The altazimuth telescope mount is the simplest mount to build, and inexpensive telescopes often come with some variation of this type of mount. If you happen to have a telescope that doesn't have a mount, or one with an inadequate mount, you can build a substantial altazimuth mount out of pipe fittings, polishing the threads on the two axes with a bit of valve grinding compound. The total cost can be as low as about $75. A description of such a mount is at Inexpensive DIY Tripod.

    Since the increasing integration of computers into the astronomy hobby, the altazimuth mount is getting more frequent use. By putting a drive motor on both axes of the altazimuth telescope mount and using a computer to calculate the correct drive rate on each motor for any given target, smart altazimuth telescopes like the Celestron NexStar 5 SE Telescope have entered the hobby in a big way, particularly because of their convenience and their surprising affordability.






    The Dobsonian Mount

    The Dobsonian mount is a common mount for Newtonian telescopes. The Dobsonian mount is just another configuration of the altazimuth mount. It has a vertical axis perpendicular to the ground, and an elevation axis that is parallel to the ground. The Dobsonian design can be as compact as on this Orion StarBlast 4.5 Astro Reflector Telescope, or husky enough to easily handle something like the Orion SkyQuest XT8 Classic Dobsonian Telescope. In fact, Dobsonian telescope models up to 15 inch are commercially available, and ATM designs handle up to 30 inch telescopes.

    The image above is an illustration of changes in azimuth. The Dobsonian telescope base usually sits on 3 Teflon pads, making a smooth bearing with a very big diameter. This gives good support for large Newtonian telescopes. Slight nudges are all that's needed to move a Dobsonian mounted telescope around the azimuth axis.

    This image is an illustration of changes in elevation. The elevation axis bearings usually sit on a couple of Teflon pads, again making for simple, stable, and smooth bearings. The larger the telescope, the larger in diameter are the elevation axis shafts. As with azimuth, simple nudges to a properly made Dobsonian telescope are all that's needed to move it smoothly in elevation.

    The advantages of the Dobsonian telescope mount are it's simplicity, low cost, and ability to handle large telescopes. If you can use a saw, you can likely make a fine Dobsonian mount to complete any reflector telescope project. Check out the plans at Making A DobsonianMount. For amazingly low prices, you can buy Dobsonian telescopes ready to use, like the Orion SkyQuest XT6 Classic Dobsonian Telescope.

    6 Inch f/5 DOB


    The above image is my f/5 Newtonian mounted in a DOB mount based on the Stellefane DOB Design. The telescope is the same one that originally came (years ago) mounted on an Equatorial Mount. The Equatorial Mount provided a clock driven mount, and being an equatorial design only required one drive motor. The above DOB design offers an easier to move around and more convenient to use mount, albeit without the clock drive.


    The Equatorial Mount

    Shown above is my f/5 Newtonian reflector telescope on an equatorial mount -- specifically a German equatorial mount. You can see that it looks more complicated than the altazimuth mount. What makes it more complicated is that it has an axis with an adjustable tilt. That adjustable axis is called the polar axis. The Celestron Omni XLT 150 Telescope is a currently available telescope much like my purchase.

    The equatorial mount shown with this telescope is popular because it simplifies the tracking of celestial objects. For any given location on the Earth, the polar axis can be adjusted to align with the Earth's rotational axis, thus properly compensating for Earth rotation at the observer's Latitude. Having this axis tipped to the proper angle necessitates the use of counter weights to keep the telescope in any given position.

    Many equatorial mounted telescopes have an alignment telescope mounted within the polar axis, making alignment easy. The above image shows some of the parts of a typical equatorial mount, including the built in Polar alignment telescope. You merely look through the polar axis telescope and center Polaris (for North hemisphere observers) in the field of view, then lock down the adjustment.

    Why tip one axis, you might ask? I could go into all the geometry, but it stands to reason that if the Earth's rotation about its spin axis is what makes stars move across the night sky, something aligned with the Earth's spin axis would provide a means of compensating for the motion of the Earth around that axis. A mount with one axis aligned with the Earth's spin axis is much easier to motorize. A single motor on the polar axis that rotates in the opposite direction of the Earth's spin at the Earth rotation rate (once per sidereal day) will do the trick. No computer is necessary, in that the motor rate is constant.

    The R A in the diagram near the Polar Axis label stands for right ascension. If you look at a star chart, you will see a grid of lines that look much like the latitude and longitude lines on Earth maps. Star coordinates are mapped onto a two dimensional grid much like the grid used to signify Earth object coordinates. The star coordinates have different names, those being right ascension (similar to longitude) and declination (similar to latitude).

    The star grid moves with respect to the Earth grid because of Earth's rotation with respect to the stars. In an evening you'll see the position of any particular star or pattern of stars move though the sky (at 15 degrees per hour as it happens). So while the star grid coordinates of a star are constant, the star grid itself rotates with respect to the Earth system.



    The Fork Mount - Altazimuth Mode

    This image illustrates the popular fork mount. Cassegrain telescopes often use this type of mount because of their short tube length. The fork telescope mount is particularly well suited for the shorter telescope designs.

    In this configuration, the fork mount is sitting in the altazimuth mode, a configuration not useful for astronomical viewing, but handy for viewing daylight targets. Note that like the refractor and Dobsonian illustrations, the telescope shown can move around a vertical axis (azimuth) and a horizontal axis (elevation).

    The telescope shown is my ETX 90M Meade telescope. It is an older model, and only has a drive motor on one axis. Newer versions of fork mount made by Meade, Celestron, and others have computerized mounts with motor drives in both axes, and are most often used in the altazimuth configuration. The modern ETX 90, for example, no longer uses just the single motor drive like my old model, but is modernized into the Meade Instruments ETX90 Observer model. You can still see what looks like a fork mount on the new ETX 90, but it operates in the altazimuth orientation.

    With these computerized instruments, the altazimuth mode is a fully functional star tracking configuration, with the computer adjusting the speed of the two motors to keep the telescope pointed at a particular object.



    The Fork Mount - Equatorial Mode

    This fork mounted telescope image shows my old ETX 90 model in the equatorial configuration. Note that what was the vertical axis is now tipped to the observer's latitude angle. With the tipped (Polar) axis aligned with the Earth's spin axis, the single motor drive of the telescope is sufficient for tracking targets.

    The small black box with the red button that you see in the image is a modification I added to the telescope to give a fast/slow motion slewing control. By pushing the red button, part of the drive circuitry is bypassed which speeds up the motor, providing a slow slewing motion. Pushing the black button stops the motor, allowing Earth's rotation to catch up.

    The equatorial mode fork mount was common on older Cassegrains. It is still a good mode for even the newer ones for long exposure astrophotography.



    Personal Notes

    The telescopes with a computer on board to provide altazimuth tracking include an extensive database of thousands of objects. Before taking advantage of the computerized mount, you must put the telescope through an alignment sequence, then you can simply select objects from the database and the telescope automatically slews to the selections.

    To get the most efficiency in observing sessions with my computer controlled telescope, I still make use of the Star Pointer web utility. Even though the telecope's computer already knows where the star targets are, I have to tell it which ones I want to observe. If I'm unprepared and happen to pick objects scattered around the sky, I'll spend a lot of time waiting as the motors whir as they move from target to target.

    But the Star Pointer utility makes a list of all targets that are above the horizon, and arranges them in azimuth order. So if I select targets from the browser displayed list to enter into my computerized telescope, the telescope will have to travel very little to get from one target to the next. That saves a lot of time.

    The down side of the two-motor, computer driven altazimuth mount is that the field of view through the eyepiece rotates as the telescope tracks. This isn't true for equatorial mounted telescopes. For viewing purposes this slow field rotation is hardly a problem. But if you intend to do long-exposure astrophotography, you need to have a motorized equatorial mount to facilitate tracking without field rotation.

    The good news is that the two motor, computer driven mounts can generally be operated in an equatorial mode as shown in the Nexstar 5SE image above. In fact, the NexStar 5SE has a built in wedge as it is called, that allows use in equatorial mode. Some other such telescopes don't have the wedge built in, but have it available as an accessory.

    Purists will also point out that if you start out with a computer driven telescope, you won't learn nearly as much about the night sky. There is something enjoyable about having the skill to find objects without the aid of a computer.

    I've used both equatorial and altazimuth mounts. A couple of equatorial mounts were home made, and a couple were commercial. I can tell you that the home made ones were heavy and clumsy, and even at their hefty size were inadequate for the 8 inch and 10 inch telescopes I attempted to mount on them.

    Most of the commercial ones are a bit flimsy also, but the one shown in these pictures (with the 6 inch f/5 Newtonian telescope) is actually quite smooth and sturdy. When I bought my Newtonian telescope from Discovery Telescopes, they admitted to me that the telescope and mount were actually imported (from China I suspect), but the optics were made by Discovery. I've had to do a few tweaks on the instrument and tripod mount to get the best performance, but in the end I'm very happy with the unit.

    As to altazimuth mounts, most of the ones I've used are home made. I constructed a couple of Dobsonian telescope mounts and a couple of pipe fitting telescope mounts. In each case, these mounts performed admirably. I guess the point of the story is that altazimuth mounts are easier to make and use, supporting the fact that Dobs are the most often home constructed telescope. But if photography is your goal, then as some point you'll likely end up with an equatorial mounted telescope.









     

    Drake Equation Statistics


    The Drake Equation

    If you aren't familiar with the Drake Equation, it was formulated by astronomer Frank Drake in 1961. It provides a probabilistic method of estimating the number of technical civilizations that might concurrently exist in our galaxy. It combines 7 parameters that make up the components of the estimate.

    Our dilemma is that we don't know very well what values many of those parameters should have. We can come close to estimating the N* star formation rate, but the original view of the paramater was to estimate the rate of sun-like star formation, as low as a value of 1 star per year. Now Red Dwarfs are being considered as possible life sustaining stars. So that rate of star formation paramater may be bigger than thought.

    We know now that most stars (fp) have planets. Most stars likely even have one or more planets in the life zone, that temperate zone where liquid water may exist. But the number of those planets that may be earth-like is small, just a few percent.

    The values of the remaining parameters are largely unknown, though the percentages for number of planets that will develop life (fl), percentage of those that will develop intelligent life (fi), and percentage of those that will develop technology (fc), are all likely small values.

    We also have no idea how long a civilization, having gotten started, may last (L). We have been a technical civilization a very short time, yet we already have the potential to destroy ourselves. And nature can provide numerous methods of destroying life, such as plagues, massive solar flares, asteroid or even planetary collisions, and nearby super novae. So if we are a typical technical civilization, our predicament may suggest that the length of time a technical society exists could be rather short.

    This post shows a version of the Drake Equation you may have never seen before. Rather that present the equation with the option to pick your own specific parameters for a trial run like the Drake Equation App, it lets you get serious about your study of the equation.

    Instead of selecting specific parameters, this version lets you select ranges of parameter values to express you sense of how well parameters are known. Then the app picks the high, low, and two values within the range for each parameter, and calculates number of civilizations (Nciv) for each parameter combination.

    The program then creates a histogram of Nciv values and turns them into percentages of the total number of estimates. It then creates a sum of percentage array and uses that to determine likely values for the number of concurrent civilizations in our galaxy. It provides the Maximum, Average, 90th percentile, 75th percentile, and 50th percentile values of Nciv estimates. When you see these statistics from thousands of samples, you can get a much better picture in your mind of how isolated we may actually be.

    The statistical version of the Drake equation is presented below. It uses a Monty Carlo simulation to get statistical results. Try out some parameter ranges and see what you can deduce.

    The formulation of the Drake Equation used:

    N = N* . fp . ne . fl . fi . fc . L

    N* Star Formation Rate/Year
    fpPercent of those stars with planets
    neAverage number of life-potential planets per star
    flPercent of those that will harbor life
    fiPercent of those that will develop intelligent life
    fcPercent of those that will develop radio communications
    LNumber of years a civilization will exist

    ParameterMinMax
    N*, Star Formation Rate
    fp, Percent of Stars With Planets
    ne, Avg Number of Life Potential Planets Per Star
    fl, Percent Of Those That Will Develop Life
    fi, Percent Of Those That Will Develop Intelligent Life
    fc, Percent Of Those That Will Develop Radio Communication
    L, Number Of Years A Civilization Will Last
    Click for Results

    Star Pointer Utility

    Finding Stars with Your Cell Phone

    Star Pointer

    Note: Star Pointer needs to know user location (lat/lon)
    to work. It saves the lat/lon in a local cookie for
    user convenience. Please don't use Starpointer if
    this is objectionable.

    Ways to Improve a Newtonian Telescope

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