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Newtonian Basics

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Newtonian Telescope Basics

This site describes the features of the Newtonian, one of the simplest and cheapest telescope designs made for astronomy.

I admit I'm partial to this inexpensive and capable design. Given its capabilities versus its price, it provides the best overall seeing for the dollar.

My 6 inch f/5 Newtonian is similar to the Celestron Advanced Series C6-NGT - Telescope - 150 mm - f/5.0 - Newtonian reflector. I purchased my model from Discovery telescopes some years ago. My equatorial Newtonian, reviewed here is overall my favorite telescope. It's a good general purpose work horse. Portable, great for wide star views, and capable of delivering decent planetary images.

I also have a 6 inch f/10 Newtonian designed especially for lunar and planetary observing, and it is reviewed here.

If you want to know more about Newtonians, read on.





Newtonian Diagram

The Newtonian Reflector Design

After the refractor, the next telescope design that came along was the Newtonian, named after, you guessed it, Isaac Newton. This design uses a parabolic curved mirror (left side of picture) for the objective instead of a lens. The curved surface of the mirror reflects the light to create the image for the eyepiece. Newtonian telescopes of long focal ratio (f/10 for a 4.25 inch or 6 inch for example) need not have parabolic mirrors to produce good images.

Because light entering the open end of the telescope tube (right side of picture) is reflected back through the tube, a flat diagonal mirror is needed to deliver the image out the side of the tube to an eyepiece.



The Modern Amateur Astronomy Newtonian

Since all wavelengths of light reflect off of the surface of a mirror in the same way, the reflecting telescope is not plagued with the color problems of the refractor. The only trouble with the reflectors of old was that the mirrors of the day were made of speculum metal. It provided a smooth reflecting surface, but one whose reflectivity deteriorated rapidly. So a given diameter reflector would provide much dimmer images than the same sized refractor.

That's not nearly as true today. Most mirrors of today are made of glass with a thin aluminum coating. Aluminum is very reflective, above 90%. So today's reflectors are good performers. The parabolic curve on the mirrors surface is necessary, especially in focal ratios less than f/10, in order to cause light striking the entire mirror surface to be focused to the same point.

As it turns out, in longer f ratios the difference between a sphere and a parabola is insignificant. So longer focus Newtonian reflectors, common in the 4.25 inch and 4.5 inch diameters, need not be parabolic to give very good performance, and are often sold with spherical mirrors. Just don't buy a short focus reflector with a spherical mirror and expect good performance.

The Newtonian has it's own advantages that appeal to observers. First and foremost, they give the most seeing per dollar. That is, for a given diameter of instrument, they are the cheapest.

Does that mean they are inferior in any way? Not at all. They are just a simple design that is inexpensive to make.

Since the Newtonian has no chromatic distortion, it can be made to a wider range of focal ratios without problem. Very large instruments (12 inch diameter and larger) can be made at focal ratios of f/4 or f/5, making them still usable by the amateur astronomer at only about 4 to 5 feet long. Shorter focus Newtonians do, however, suffer from coma. This aberration causes objects near the edge of the field of view a comet shaped distortion. Collimation of short focus Newtonians must also be more precise.

Align Secondary
Animation
Mouse Over For Animation

A very quick alignment guide is illustrated by the animated image at left. One easy way to do alignment is with a Cheshire eyepiece, a handy alignment tool. The illustration at left is a depiction of what you see looking into a Cheshire eyepiece inserted into a Newtonian telescope focuser. The colored rings represent as follows: Cheshire eyepiece and cross hair (black), secondary mirror (purple), primary mirror (green), and cross hair reflection (red). The initial image is what you typically see, a primary that doesn't appear to be centered, and a reflection of the Cheshire that's not centered.

The procedures are to first make adjustments to the secondary adjustment screws to make the primary appear to be centered. The process is aided considerably if you paint a dot on the very center of your primary. The secondary blocks off the center of the primary anyway, so a dot on the center does not harm your primary mirror.

Then, adjust the primary alignment screws to move the reflection of the Cheshire cross hair to also be centered on the directly seen cross hair. Walla, you've achieved alignment. A more detailed collimation instruction can be found at Newtonian Collimation. These same instructions apply to Dobsonian telescopes also.

The features that compromise the design are less to do with observing and more to do with maintenance. Newtonians expose all optical components to the elements when they are in use. So delicate first-surface mirrors occasionally must be cleaned, and this takes care. To be cleaned, they must be removed from the telescope. This means a complete realignment of the optics will have to be performed when all elements are reassembled. In fact, alignment tweaking needs to be done routinely for best performance. Once learned, this is not a difficult procedure, but a number of observers would rather avoid this issue.

If you don't mind learning how to carefully clean your optics and realign them, a Newtonian is a excellent choice. I've been using Newtonians since I was about 16, so it's not a big deal. I've owned a number of them, and find them my personal favorite for a general use telescope.

If you think a Newtonian might be what you're interested in, I suggest you give a moment to the following table. It shows which types of telescopes are most often used for different types of observing, including provision for larger, moderate, or small portable telescopes.

Telescope/Observing Preference Table

Telescope Usage Chart

Use this astro-customized search to browse some excellent telescope vendors.

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Personal Notes

I've owned a number of Newtonian reflecting telescopes over the years, some in the Dobsonian configuration. My first was a Gilbert 2.5 inch Newtonian -- anyone else ever have one of those? Then I obtained a 6 inch f/12 Newtonian in sort of a kit, I had to assemble it. It was great, but so long I had to use a small step ladder to look through it much of the time.

Then I decided to make one of my own -- from scratch. Allyn J. Thompson's book Making Your Own Telescope gave me the inspiration, and the guidance of what to build. I was first thinking an 8 inch, but Allyn stated that the perfect match to a 6 inch f/12 was a 6 inch Richest Field Telescope (RFT). That was it, I went for a 6 inch f/4.5. It turns out that short focus telescopes aren't the easiest to construct, but I managed it. So for a time there, I had a great combination. Then I got aperture fever, going to an 8 inch, then a 10 inch behemoth. In the fray I sold my 6 inchers.

Now after all these years I'm almost back where Allyn said I should be, I have a 6 inch f/10 telescope for planetary viewing, and a 6 inch f/5 telescope for stellar work. It is still a great combination, as he wrote in his book. Allyn's books is still available at used book stores, if you want an inspirational telescope making book.