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Dobsonian telescope

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A Dobsonian telescope is a specialized Newtonian reflector design. It uses an altazimuth mount to allow for easy movement. This design was popularized by John Dobson in 1965. It changed how amateur astronomers access the universe. Most large telescopes are very heavy and expensive. Dobson created a way to build massive tools for a low cost. These telescopes are often called "light buckets." This nickname refers to their ability to gather large amounts of light.

Red dobsonian
Red dobsonian

The mechanism of a Dobsonian relies on a unique altazimuth mount. This mount allows the telescope to move up and down. It also allows the telescope to move left and right. Instead of using complex gears, it uses a simple, stable construction. The base consists of a flat, horizontal ground board. A box called a rocker box sits on top of this board. A loose center-bolt keeps the rocker box centered so it can pivot. The rocker box rests on three support points on the ground board.

Dob
Dob

To move the telescope, the design uses seven specific support points. These points use small blocks made of Teflon, which is a slippery material. The rocker box has semicircular cutouts on its top edges. Four more supports are placed inside these cutouts. The telescope's optical tube assembly, or OTA, has two large round trunnions. These trunnions are also called altitude bearings. They rest directly on the four supports in the rocker box. To change the altitude, a user simply lifts the tube. To change the azimuth, the user pushes the top rim of the tube. This motion causes the rocker box to slide over the ground board.

Dob
Dob

John Dobson pioneered this design to help with "sidewalk astronomy." He wanted to bring deep-sky astronomy to the masses. He used many unconventional and inexpensive materials. For the mirrors, he used glass from surplus ship porthole covers. These mirrors were much thinner than standard mirrors. While a typical mirror has a 1:6 thickness ratio, Dobson used a 1:16 ratio. This means the mirror is very thin compared to its diameter. To prevent these thin mirrors from sagging, he supported them with indoor or outdoor carpet.

Dobsonian rocker wood
Dobsonian rocker wood

Dobson also changed how the telescope tubes were made. He replaced expensive aluminum or fiberglass with Sonotubes. These are thick, compressed paper tubes used in construction to pour concrete. Sonotubes are very rugged and do not dent easily. They are also thermally stable and non-conductive. This helps prevent unwanted air currents inside the tube. These currents can blur the view of stars. By using these common items, Dobson achieved a low cost-to-objective size ratio. This means users get more mirror diameter for every dollar spent.

Two dobsonians
Two dobsonians

The design is specifically optimized for observing deep-sky objects. These include dim objects like nebulae, star clusters, and galaxies. Because these objects are large, they are viewed at low magnification. This makes the simple altazimuth mount sufficient for use. Standard equatorial mounts are often massive and require heavy counterweights. They are also difficult to move and expensive to build. A Dobsonian is much more portable and rugged for travel. This is vital because astronomers must travel to dark locations away from city lights.

Dobson truss
Dobson truss

Over time, the amateur community has created many derivative designs. The original designs were often too large to transport easily. To solve this, designers created collapsible tube assemblies. These allow large telescopes to fit into smaller vehicles like sedans or hatchbacks. Some modern versions use a truss tube design. A truss tube uses a lightweight frame instead of a solid cylinder. This combines the light weight of a truss with the portability of a collapsible design.

Dobson truss
Dobson truss

While highly effective, the Dobsonian has some specific limitations. Because it is an un-driven mount, it does not track the stars automatically. The Earth's rotation will cause objects to move out of view. Users must "nudge" the telescope every few minutes to compensate. This task becomes harder when using high magnification. Additionally, the design is not well suited for astrophotography. It can also be difficult to point the telescope at objects near the zenith. This is because a large movement of the azimuth axis is required for small changes in direction. Despite this, the design remains a cornerstone of amateur astronomy.

Teeter 16 inch telescope
Teeter 16 inch telescope
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🖼️ Images & Media (7)
File:Red dobsonian.jpg
Red dobsonian.jpg
File:Two dobsonians.jpg
Two dobsonians.jpg
File:Dob.png
Dob.png
File:Dobsonian rocker wood.jpg
Dobsonian rocker wood.jpg
File:Dobson truss.jpg
Dobson truss.jpg
File:Dobson-mount.jpg
Dobson-mount.jpg
File:Teeter 16 inch telescope.jpeg
Teeter 16 inch telescope.jpeg
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