Explore Scientific Truss Tube Dobsonian Series User Manual Download Page 12

 

 

Astronomical observations 

The first observations should be performed during dusk  so that you get familiar with your new telescope quickly. 

Always 

remember never to look at or near the sun! 

Choose a land object that is easy to find and far away, such as a mountain top. 

Roughly point the telescope at the object. Now look through the finder scope and move the telescope until the red dot of light 
appears centered onto the object. If your are looking through an eyepiece with low magnification, you should now be able to see 
the object in the telescope. Focus the image carefully, center it in the field of view and fine tune the alignment of the finder if 
necessary. Now that you are getting more familiar with the telescope you can try to watch the Moon (if visible). It  should be 
possible to use the telescope without additional light now without problems. The Moon can be observed best during the periods 
where less than 50% of its surface is bright. So you can see the detailed shadows that the sun is causing when the light hits the 
craters from the side angle – creating a 3D-like experience. We recommend using a neutral density filter for the Moon that reduces 
the glare. During a Full Moon, the surface appears evenly bright without contrast and prominent structures. 
If you are spending a few successive nights watching the Moon you will notice the change in the appearance of the mountains, 
craters and maria due to the change of the phase of the Moon – a very interesting effect! 

The planets 

During their orbit around the sun the planets are continuously changing their position on the sky. When they are visible, the 
following planets are especially suited for observations with your telescope: 

Venus: 

The diameter of Venus is about 9/10 the diameter of the Earth, and it is the third brightest object in the sky (after the Sun and the 
Moon). As Venus orbits the Sun, you can observe the change of the light phases — sickle, half Venus, full Venus — very much 
like the phases of the moon. The planetary disc of Venus appears white because the sunlight is reflected by a compact layer of 
clouds that covers all surface details.  

Mars: 

The diameter of Mars is about half of the Earth’s diameter. In a telescope, Mars will appear as a tiny red-orange disk. You may 
see a tiny white patch when you look at the polar regions that are covered in ice. About every two years, when Mars and Earth 
reach their closest distance you can discover new features. 

Jupiter: 

The biggest planet in our solar system is Jupiter. In a telescope, the gas giant appears as a disk that is covered in dark lines. 
Those lines are cloud bands in the atmosphere of Jupiter. Even with low magnification, 4 of the 67 moons of Jupiter are often 
visible. These are the Galilean moons (Io, Ganymed, Europa and Callisto). Because those moons are orbiting Jupiter the visible 
number and position changes. Sometimes a moon passes above the planetary disc of Jupiter – then the shadow of the moon can 
be spotted on the planet as a sharp dark spot. 

Saturn: 

Saturn has a diameter about nine times the Earth’s diameter and appears as small roundish disc with a distinct set of rings that 
bulge out from the edges of the planetary disc. Galileo, who was the first human observer of this planet in 1610, couldn´t know 
that the planet had rings. Instead, he described Saturn as having “ears“. The rings of Saturn mainly consist of billions of icy 
particles – ranging from tiny dust to the size of a house. The biggest division in the rings, the so called “Cassini division” should 
be easily seen with your telescope in nights of steady air. Titan, the biggest of the 62 moons of Saturn, is also visible as a bright, 
starlike object in the vicinity of the planet. Up to six moons may be detected in your telescope. 

Deep-Sky-Objects 

To locate constellations, stars or other deep-sky-objects, it makes sense to use a star chart. We will list a selection of deep sky 
objects here: 

Stars

 are giant objects that mainly consist of gas. Due to the nuclear fusion in their core they radiate energy and shine. The stars 

are extremely far away. Because of this vast distance they appear as tiny spots of light in your telescope, despite their size – no 
matter how big your telescope is. 

Nebulae

 are giant interstellar clouds of gas and dust. Within those clouds new stars are being born. The premier nebula on the 

northern hemisphere is the Great Orion Nebula, a diffuse nebula that looks like a fuzzy patch of light in the sword that branches 
off of Orion’s Belt. Also known as M42, it contains many intriguing features that pop to life in a telescope. 
An 

open cluster

 is a group of young stars that were born in a single diffuse nebula not too long ago (on an astronomical time 

scale). The Pleiades is an open cluster that is relatively young, having formed within the last 100 million years, and lies relatively 
close to Earth at about 440 light years away. Found in the Taurus constellation, it  consists of more than 1,000 confirmed stars, 
although an average of only six are visible to the naked eye. A dark sky free of light pollution can help a dedicated observer see 
around a dozen Pleiades stars, but you telescope will quickly reveal many more of the elusive members of this legendary 
cluster.  

Constellations

  are big patterns of stars that were believed to be celestial representations of men, gods and objects by old 

civilizations. Those patterns are too big to be observed at a single glance through a telescope. If you want to become familiar with 
the constellations, start with a pattern that is easy to find, like the Big Dipper in the constellation Ursa Major. Try to locate the other 
constellations in the neighborhood of this constellation in the second step and move on to even more distant patterns. 

Galaxies

 are gigantic accumulations of stars, nebulae and clusters that are held together by gravity. Most galaxies have a spiral 

shape (like for example our own galaxy, the milky way), but there are also galaxies with elliptical or irregular shapes. The closest 
spiral galaxy is the Andromeda-Galaxy (M31). The core of M31 looks like a bright patch of light in your telescope – under dark 
clear skies you will be able to detect features in this object with your telescope.  
 

 

Summary of Contents for Truss Tube Dobsonian Series

Page 1: ...has occurred until it is too late Take extra care when using the telescope or a finder scope during daylight hours and do not point either at or near the Sun Do not look through either when you are m...

Page 2: ...s and tricks Maintaining the optics Specifications Accessory Explore Scientific service All Explore Scientific telescopes and telescope accessories are subject to constant technical improvement Minor...

Page 3: ...Extension 11 Clutch The revision consists of the clutch and the 4mm hex screw with the plastic sleeve The center rocker knob will be replaced with the hex screw and sleeve Figure 2 This will allow for...

Page 4: ......

Page 5: ...r box Stray light protection 8 Screws 4 short screws with knob to secure the secondary cage to the truss pairs 2 long screws with knob to secure the altitude wheels directly to the main mirror box its...

Page 6: ...other contains the rocker box On the outer left you can see one of the altitude wheels the stray light cover for the secondary cage is visible in the upper part of the box Remove all parts from the b...

Page 7: ...are two sets of holes on both sides of the mirror box Having two sets gives you an additional degree of freedom to balance your telescope If you are just using lightweight eyepieces 1 25 we recommend...

Page 8: ...time you will need a few minutes to get accustomed to the procedure since you have to hold the secondary cage with one hand and align the truss holes and the threaded hole of the secondary unit and i...

Page 9: ...main mirror Practice this until you get a feel of what a turn at one of the collimation screws is doing Fine Collimation During fine collimation locate Polaris and view it with high magnification Note...

Page 10: ...and show tails directed tot he edge of the field of view If you are using cheap eyepieces those star images will be even more distorted because the off axis aberrations of the telescope and the eyepi...

Page 11: ...red dot finder and move your head until you see the red dot of light that is projected onto the glass window Adjust the finder with the two screws until the red dot is on top of the object that is cen...

Page 12: ...turn Saturn has a diameter about nine times the Earth s diameter and appears as small roundish disc with a distinct set of rings that bulge out from the edges of the planetary disc Galileo who was the...

Page 13: ...ins Always remember to bring warm clothing like thick jackets beanies gloves winter shoes and thick socks even if your were sweating during the day It is hard to enjoy even the best night when you are...

Page 14: ...coated aluminum with connectors Secondary spider 4 arm steel Main mirror 12 305 mm parabolic BK 7 like glass aluminum coated with protective layer Focal length 1524 mm Focal ratio f 5 Resolving power...

Page 15: ...b If cleaning the optics is necessary it is best to brush away the dust with a fine camel hair brush as it is used for photographic equipment Please do NOT use optical lens cleaning tissues as many c...

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