D RR Delta 1000 Achromatic Refractor Telescope Instruction Manual
- June 10, 2024
- D RR
Table of Contents
- D RR Delta 1000 Achromatic Refractor Telescope
- SAFETY INSTRUCTIONS
- NOMENCLATURE WEGA 1000
- NOMENCLATURE DELTA 1000 / SATURN 900
- ASSEMBLY INSTRUCTIONS DELTA 1000 WITH EQ1-MOUNT
- ASSEMBLY INSTRUCTIONS WEGA 1000 / SATURN 900 WITH EQ2-MOUNT
- OPERATING YOUR TELESCOPE
- CHOOSING THE APPROPRIATE EYEPIECE
- OBSERVING THE SKY
- CARE AND MAINTENANCE OF YOUR TELESCOPE
- TECHNICAL SPECIFICATIONS
- CLEANING YOUR TELESCOPE
- References
- Read User Manual Online (PDF format)
- Download This Manual (PDF format)
D RR Delta 1000 Achromatic Refractor Telescope
THANK YOU: very much for choosing a quality product from DÖRR. Please
read the instruction manual and the safety instructions carefully before using
the device for the first time. Keep this instruction manual together with the
device for later use. If other people use this device, provide them with this
instruction manual. If you sell the device, the instruction manual is part of
the device and must be supplied with it.
DÖRR: is not liable for damage caused by improper use or failure to
observe the instruction manual and safety instructions. In the event of damage
caused by improper handling or by external influence, the guarantee or
warranty becomes void. Manipulation, structural alteration of the product, as
well as the opening of the housing by the user or unauthorized third parties,
is considered improper handling.
SAFETY INSTRUCTIONS
ATTENTION! The following safety instructions must be observed before use.
- NEVER look directly at or near the sun through this telescope or through the viewfinder! There is a risk of blindness!
- The telescope is not a toy! Children must not use the telescope without adult supervision. Keep the telescope,
- accessories, and packaging materials away from children and pets to prevent accidents and suffocation.
- People with physical or cognitive disabilities should operate the telescope under guidance and supervision.
- Please note that the light shining through the eyepiece is highly focused and can generate a great deal of heat.
- Therefore, make sure that the telescope is not pointed at easily flammable materials. After use, please attach the protective eyepiece cap.
- Protect the telescope from rain, moisture, direct sunlight, and extreme temperatures.
- Make sure that the telescope is placed on a solid surface so that it cannot tip over.
- Protect the telescope from impacts. Do not use the telescope if it has been dropped.
- If the telescope is defective or damaged, do not attempt to disassemble or repair the telescope yourself. Please contact your specialist dealer.
- Protect the telescope from dirt. Do not clean the telescope with petrol or harsh cleaning agents. We recommend using a lint-free, slightly damp microfibre cloth to clean the outer components of the telescope.
- Store the device in a dust-free, cool, dry place.
- This telescope is for private use only and is designed for observing nature and the sky.
- Respect the privacy of others: do not use this telescope to look into other people‘s homes.
DISPOSAL
Please dispose of old appliances and packaging in an environmentally friendly
manner and according to type. Sorting waste for separate collection and
sensible recycling of packaging waste helps to use natural resources more
sparingly. Furthermore, recycling is a contribution to preserving our
environment and thus also people‘s health. Further information on the current
legal regulations, proper disposal, recycling and collection points can be
obtained from local authorities, waste disposal companies, and specialized
retailers.
NOMENCLATURE WEGA 1000
WEGA 1000
- A Dust Cap/Mask (Remove before Viewing)
- B Dew Cap/Sun Shade
- C Objective Lens
- D Telescope Main Tube
- E Piggyback Bracket
- F Finderscope
- G Finderscope Bracket
- H Finderscope Alignment Screws
- I Focus on Locking the Screw
- J Eyepiece
- K Diagonal
- L Focus Tube
- M Focus Knob
- 1 DEC. Flexible Control Cable
- 2 R.A. Flexible Control Cable
- 3 Altitude Adjustable T-Bolt
- 4 Azimuth Lock Knob
- 5 Counterweight
- 6 Counterweight Locking
- 7 Counterweight Rod
- 8 R.A. Axis Scale
- 9 DEC. Scale
- 10 DEC. Lock Knob
- 11 Tube Ring Mounting Plate
- 12 Tube Rings
- a Accessory Tray
- b Tripod Legs
NOMENCLATURE DELTA 1000 / SATURN 900
DELTA 1000
- A Secondary Mirror Position
- B Dust Cap/Mask (Remove before Viewing)
- C Focus Tube
- D Finderscope Bracket
- E Finderscope
- F Finderscope Alignment Screws
- G Eyepiece
- H Focus Knob
- I Piggyback Bracket
- J Telescope Main Tube
- K Primary Mirror Position
- 1 DEC. Flexible Control Cable
- 2 R.A. Flexible Control Cable
- 3 Altitude Adjustment T-bolt
- 4 Azimuth Lock Knob
- 5 Counterweight
- 6 Counterweight Locking Thumb Screw
- 7 Counterweight Rod
- 8 R.A. Scale
- 9 DEC. Scale
- 10 DEC. Lock Knob
- 11 Tube Rings
- a Accessory Tray
- b Tripod Legs
SATURN 900
- A Secondary Mirror Position
- B Dust Cap/Mask (Remove before Viewing)
- C Focus Tube
- D Finderscope Bracket
- E Finderscope
- F Finderscope Alignment Screws
- G Eyepiece
- H Focus Knob
- I Piggyback Bracket
- J Telescope Main Tube
- K Primary Mirror Position
- 1 R.A. Scale
- 2 DEC. Flexible Control Cable
- 3 Altitude Adjustment T-bolt
- 4 Azimuth Lock Knob
- 5 R.A. Flexible Control Cable
- 6 Counterweight
- 7 Counterweight Locking Thumb Screw
- 8 Counterweight Rod
- 9 R.A. Scale
- 10 DEC. Scale
- 11 DEC. Lock Knob
- 12 Tube Rings
- a Accessory Tray
- b Tripod Legs
ASSEMBLY INSTRUCTIONS DELTA 1000 WITH EQ1-MOUNT
TRIPOD SET UP
Adjusting tripod legs (Fig.1)
- Slowly loosen the height adjustment clamp and gently pull out the lower section of each tripod leg. Tighten the clamps to hold the legs in place.
- Spread the tripod legs apart to stand the tripod upright.
- Adjust the height of each tripod leg until the tripod head is properly leveled. Note that the tripod legs may not be at the same length when the equatorial mount is level.
Attaching the accessory tray (Fig.2)
- Place the accessory tray on top of the bracket, and secure it with the locking knob from underneath.
Attaching mount to tripod legs (Fig.3)
- Place the equatorial mount inside the tripod mounting platform
- Push the azimuth lock knob/locking shaft up and thread the screw into the hole in the bottom of the mount.
PREPARING THE MOUNT FOR ASSEMBLY
Repositioning the mount head (Fig.4.1 – 4.5). Follow the diagrams to place the
mount into an upright position.
- Fig 4.1: Unlock the DEC. lock knob. Swivel 180°
- Fig 4.2: Unlock the R.A. lock knob on the other side. Swivel 180°
- Fig4.3: Unlock the altitude lock knob. Set the angle to the local altitude
- Fig4.4: Swivel 180°
- Fig4.5: Tighten altitude, DEC. and R.A. knobs
TELESCOPE ASSEMBLY
Installing counterweight (Fig.5)
- Slide the counterweight halfway onto the rod. Hold the counterweight with one hand and insert the counterweight rod into the threaded hole one mount with the other hand. Tighten the counterweight rod onto the mount.
- Tighten the thumbscrew to lock the counterweight in place.
Installing control cables (Fig.6)
- Slide the sleeve end of the cable over the nipple on the end of the worm gear. Tighten the cable using the set screw against the flat surface on the nipple.
Attaching the tube rings to mount (Fig.7)
- Remove the tube rings from the telescope by releasing their thumb nuts and opening their hinges.
- Place the tube rings on top of the tube ring mounting plate and bolt the tube rings to the mount using the wench provided.
Attaching the telescope main tube to tube rings (Fig.8)
- Remove the telescope tube from the paper covering.
- Find the center of balance of the telescope tube. Place this point between the two tube rings. Close the hinges around the telescope and fasten it securely by tightening the thumb nuts. Do not over-tighten.
FINDERSCOPE ASSEMBLY
Attaching the finderscope (Fig.10, 11)
- Locate the finderscope optical assembly.
- Remove the two knurled thumbscrews near the end of the telescope’s main body. (near the front of the telescope’s main body for the reflector).
- Position the finderscope bracket over the screws in the telescope’s main body.
- Secure the finderscope bracket with the two knurled thumbscrews.
ASSEMBLY INSTRUCTIONS WEGA 1000 / SATURN 900 WITH EQ2-MOUNT
TRIPOD SET UP
Adjusting tripod legs (Fig.15)
- Slowly loosen the height adjustment clamp and gently pull out the lower section of each tripod leg.
- Spread the tripod legs apart to stand the tripod upright.
- Adjust the height of each tripod leg until the tripod head is properly leveled. Note that the tripod legs may not be at the same length when the equatorial mount is level.
Attaching the accessory tray (Fig.16)
- Place the accessory tray on top of the bracket, and secure it with the locking knob from underneath.
Attaching mount to tripod legs (Fig.17)
- Place the equatorial mount inside the tripod mounting platform.
- Push the azimuth lock knob/locking shaft up and thread the screw into the hole in the bottom of the mount.
TELESCOPE ASSEMBLY
Installing counterweight (Fig.18)
- Slide the counterweight halfway onto the rod. Hold the counterweight with one hand and insert the counterweight rod into the threaded hole on the mount with the other hand. Tighten the counterweight rod onto the mount.
- Tighten the thumbscrew to lock the counterweight in place.
Installing control cables (Fig.19)
- Locate the control cables. The control cables have two different lengths. Although you can mount either cable to each direction axis, it is recommended that you mount the longer cable to the declination axis and the shorter cable to the right ascension axis (setting circle).
- To install the control cables, slide the sleeve end of the cable over the nipple on the end of the worm gear. Tighten the cable using the set screw against the flat surface of the nipple.
Attaching the tube rings to mount (Fig.20)
- Remove the tube rings from the telescope by releasing their thumb nuts and opening their hinges.
- Place the tube rings on top of the tube ring mounting plate and bolt the tube rings to the mount using the wench provided.
Attaching the telescope main tube to tube rings (Fig.21)
- Remove the telescope tube from the paper covering.
- Find the center of balance of the telescope tube. Place this point between the two tube rings. Close the hinges around the telescope and fasten it securely by tightening the thumb nuts. Do not over-tighten.
FINDERSCOPE ASSEMBLY
Attaching the finderscope (small finderscope) (Fig.23)
- Locate the finderscope optical assembly.
- Remove the two knurled thumbscrews near the front of the telescope main body (near the end of the telescope main body for the refractor).
- Position the finderscope bracket over the screws in the telescope’s main body.
- Secure the finderscope assembly with the two knurled thumb screws.
Attaching the finderscope bracket (large finderscope) (Fig.24)
- Locate the finderscope optical assembly.
- Slide the finderscope bracket into the rectangular slot and tighten the screw to hold the mount in place.
RED DOT FINDER ASSEMBLY (OPTIONAL)
Attaching the Red Dot Finder (Fig.25)
- Slide the red dot finder bracket into the rectangular slot and tighten the screw to hold the red dot finder in place (DÖRR-No. 566310)
EYEPIECE ASSEMBLY
Inserting eyepiece into reflector (Fig.26)
- Unscrew the thumbscrews on the end of the focus tube to remove the black plastic end cap.
- Insert the desired eyepiece then re-tighten the thumb screws to hold the eyepiece in place.
Inserting eyepiece into refractor (Fig.27)
- Loosen the thumbscrews on the end of the focus tube.
- Insert the diagonal into the focus tube and re-tighten the thumbscrews to hold the diagonal in place.
- Loosen the thumbscrews on the diagonal.
- Insert the desired eyepiece into the diagonal and secure by re-tightening thumbscrews.
OPERATING YOUR TELESCOPE
ALIGNING THE FINDERSCOPE
These fixed magnification scopes mounted on the optical tube are very useful
accessories. When they are correctly aligned with the telescope, objects can
be quickly located and brought to the center of the field. Alignment is best
done outdoors in day light when it’s easier to locate objects. If it is
necessary to refocus your finderscope, sight on an object that is at least 500
yards (meters) away.
- For 5×24 finderscope: twist the end of the finderscope until focus is reached (Fig.a).
- For 6×30 finderscope: loosen the locking ring by unscrewing it back towards the bracket. The front lens holder can now be turned in and out to focus.
When focus is reached, lock it in position with the locking ring (Fig.a1).
- Choose a distant object that is at least 500 yards away and point the main telescope at the object. Adjust the telescope so that the object is in the centre of the view in your eyepiece.
- Check the finderscope to see if the object centred in the main telescope view is centred on the crosshairs.
- For the 5×24 finderscope, use the three alignment screws to centre the finderscope crosshairs on the object (Fig.a2). For the 6×30 finderscope with spring loading, adjust only the two small screws (Fig.a3).
USING THE RED DOT FINDER (OPTIONAL)
The Red Dot Finder is a zero magnification pointing tool that uses a coated
glass window to superimpose the image of a small red dot onto the night sky.
The Red Dot Finder is equipped with a variable brightness control, azimuth
adjustment control, and altitude adjustment control (Fig.b). The Red Dot
Finder is powered by a 3-volt lithium battery located under-neath at the
front. To use the Finder, simply look through the sight tube and move your
telescope until the red dot merges with the object. Make sure to keep both
eyes open when sighting.
Aligning the Red Dot Finder
Like all finderscopes, the Red Dot Finder must be properly aligned with the
main telescope before use. This is a simple process using the azimuth and
altitude control knobs.
- Open the battery cover by pulling it down (you can gently pry at the 2 small slots) and remove the plastic shipping cover over the battery (Fig.b1).
- Turn on the Red Dot Finder by rotating the variable brightness control clockwise until you hear a “click”. Continue rotating the control knob to increase the brightness level.
- Insert a low power eyepiece into the telescope’s focuser. Locate a bright object and position the telescope so that the object is in the centre of the field of view. With both eyes open, look through the sight tube at the object. If the red dot overlaps the object, your Red Dot Finder is perfectly aligned. If not, turn its azimuth and altitude adjustment controls until the red dot is merged with the object.
BALANCING THE TELESCOPE
The telescope should be balanced before each observing session. Balancing
reduces stress on the mount and allows precise micro-adjustment control. A
balanced telescope is especially critical when using the optional clock drive
for astro-photography. The telescope should be balanced after all accessories
(eyepiece, camera, etc.) have been attached. Before balancing your telescope,
make sure that your tripod is in a balanced level and on a stable surface. For
photography, point the telescope in the direction you will be taking photos
before performing the balancing steps. R.A. Balancing
- For best result, adjust the altitude of the mount to between 15° and 30° if possible by using the altitude adjustment T-bolt.
- Slowly unlock the R.A. and DEC. lock knobs. Rotate the telescope until both the optical tube and counterweight rod is horizontal to the ground, and the telescope tube is to the side of the mount. (Fig.c)
- Tighten the DEC. lock knob.
- Move the counterweight along the counterweight rod until the telescope is balanced and remains sta-tionary when released.
- Tighten the counterweight thumb screw to hold the counterweight in its new position.
DEC. Balancing
All accessories should be attached to the telescope before balancing around
the declination axis. The R.A. balancing should be done before proceeding with
DEC. balancing.
- For best results, adjust altitude of the mount to between 60° and 75° if possible.
- Release the R.A. lock knob and rotate around the R.A. axis so that the counterweight rod is in a horizontal position. Tighten the R.A. thumbscrew.
- Unlock the DEC. thumbscrew and rotate the telescope tube until it is paralleled to the ground.
- Slowly release the telescope and determine in which direction it rotates. Loosen the telescope tube rings and slide the telescope tube forward or backward in the clamps until it is balanced.
- Once the telescope no longer rotates from its parallel starting position, re-tighten tube rings and the DEC. lock knob. Reset altitude axis to your local latitude.
Operating the EQ1-Mount Delta 1000
The EQ1 mount has controls for both conventional altitude (up-down) and
azimuth (left-right) directions of motion.These two adjustments are suggested
for large direction changes and for terrestrial viewing. Use the large knurled
knob located underneath for azimuth adjustments. Loosen the knob and rotate
the mount head around the azimuth axis. Use the altitude adjustment T-bolts
for altitude adjustments (Fig.d). In addition, this mount has Right Ascension
(hour angle) and declination direction controls for polar-aligned astronomical
observing. Loosen the lock knobs to make large direction changes. Use the
control cables for fine adjustment after the lock knobs have both been locked
(Fig.d1). An additional scale is included for the altitude axis. This allows
polar alignment for your local latitude. (Fig.d2)
Operating the EQ2-Mount Wega 1000 / Saturn 900
The EQ2 mount has controls for both conventional altitude (up-down) and
azimuth (left-right) directions of motion. These two adjustments are suggested
for large direction changes and for terrestrial viewing. Use the large knurled
knob located underneath for azimuth adjustments. Loosen the knob and rotate
the mount head around the azimuth axis. Use the altitude adjustment T-bolts
for altitude adjustments (Fig.e). In addition, this mount has Right Ascension
(hour angle) and declination direction controls for polar-aligned astronomical
observing. Loosen the lock knobs to make large direction changes. Use the
control cables for fine adjustment after the lock knobs have both been locked
(Fig.e1). An additional scale is included for the altitude axis. This allows
polar alignment for your local latitude (Fig.d2).
CAUTION: Observations of the sun are extremely dangerous. Do not use this
telescope for sun observation. The optical elements have the effects of a
burning glass and will blind you! The ideal way to make safe sun observations
is the usage of a special sun filter foil, which is fixed at the front end of
the telescope. The foil absorbs 99.9% of the sunlight.
USING THE OPTIONAL BARLOW LENS
A Barlow is a negative lens which increases the magnifying power of an
eyepiece, while reducing the field of view. It expands the cone of the
focussed light before it reaches the focal point, so that the telescope’s
focal length appears longer to the eyepiece. The Barlow is inserted between
the focuser and the eyepiece in a reflector, and usually between the diagonal
and the eyepiece in a refractor or a catadioptric (Fig.f). With some
telescopes, it can also be inserted between the focuser and the diagonal, and
in this position it gives even greater magnification. For example, a 2x Barlow
when inserted after the diagonal can become 3x when placed in front of the
diagonal. In addition to increasing magnification, the benefits of using a
Barlow lens include improved eye relief, and reduced spherical aberration in
the eyepiece. For this reason, a Barlow plus a lens often outperform a single
lens producing the same magnification. However, its greatest value may be that
a Barlow can potentially double the number of eyepiece in your collection.
FOCUSING
Slowly turn the focus knobs under the focuser, one way or the other, until the
image in the eyepiece is sharp (Fig.g). The image usually has to be finely
refocused over time, due to small variations caused by temperature changes,
flexures, etc. This often happens with short focal ratio telescopes,
particularly when they haven’t yet reached outside temperature. Refocusing is
almost always necessary when you change an eyepiece or add or remove a Barlow
lens.
POLAR ALIGNMENT
In order for your telescope to track objects in the sky you have to align your
mount. This means tilting the head over so that it points to the North (or
South) celestial pole. For people in the Northern Hemisphere this is rather
easy as there is a bright star very near the spot Polaris. For casual
observing, rough polar alignment is adequate. Make sure your equatorial mount
is in level and the red dot finder or finderscope is aligned with the
telescope before beginning. Look up your latitude on a map, road maps are good
for this purpose. Now look at the side of your mount head, there you will see
a scale running from 0-90 degrees. Unlock the hinge of the mount by gently
pulling on the lock lever counterclockwise. At the bottom of the head is a
screw that pushes on a tongue under the hinge, changing the angle. Spin this
until your latitude is shown on the scale by the indicator pin, then lock the
hinge (Fig.h). “Pole Star” is less than one degree from the North Celestial
Pole (NCP). Because it is not exactly at the NCP, Polaris appears to trace a
small circle around it as the Earth rotates. Polaris is offset from the NCP,
toward Cassiopeia and away from the end of the handle of the Big Dipper
(Fig.i).
EQ1 Delta 1000
Unlock the DEC. lock knob and rotate the telescope tube until the pointer on
the setting circle reads 90°. Retighten the DEC. lock knob. At the top of the
main shaft is a white line with “R”and”A” on either side of it. Loosen the a
zimuth lock knob and rotate the mount until the white line points roughly at
Polaris. Retighten the azimuth lock knob. Look through the finderscope and
centre Polaris on the crosshairs by adjusting the azimuth and latitude
settings if a more accurate polar alignment is desired.
EQ2 Wega 1000 / Saturn 900
Unlock the DEC. lock knob and rotate the telescope tube until the pointer on
the setting circle reads 90°. Retighten the DEC. lock knob. At the top of the
main shaft is a white line with “R”and”A” on either side of it. Loosen the a
zimuth lock knob and rotate the mount until the white line points roughly at
Polaris. Retighten the azimuth lock knob. Look through the finderscope and
centre Polaris on the crosshairs by adjusting the azimuth and latitude
settings if a more accurate polar alignment is desired. After a while you will
notice your target drifting slowly North or South depending on the direction
of the pole relative to Polaris. To keep the target in the center of the view,
turn only the R.A. slow-motion cable. After your telescope is polar aligned,
no further adjustments in the azimuth and latitude of the mount should be made
in the observing session, nor should you move the tripod. Only movements in
R.A. and DEC. axis should be made in order to keep an object in the field.
Southern Hemisphere
In the Southern Hemisphere you must align the mount to the SCP by locating
it’s position with star patterns, without the convenience of a nearby bright
star. The closest star is the faint 5.5-mag. Sigma Octanis which is about one
degree away. Two sets of pointers that help to locate the SCP are alpha and
beta Crucis (in the Southern Cross) and a pointer running at a right angle to
a line connecting alpha and beta Centauri (Fig.j).
TRACKING CELESTIAL OBJECTS
When observing through a telescope, astronomical objects appear to move slowly
through the telescope’s field of view. When the mount is correctly polar
aligned, you only need to turn the R.A. slow-motion to follow or track objects
as they move through the field. The DEC. slow-motion control is not needed for
tracking. A R.A. motor drive can be added to automatically track celestial
objects by counteracting the rotation of the Earth. The rotation speed of the
R.A. drive matches the Earth’s rotation rate for stars to appear stationary in
the telescope eyepiece. Different tracking speeds are also available in some
models. A second drive can be added to give DEC. control which is very useful
for doing astrophotography.
USING THE SETTING CIRCLES
The quickest way to find objects is to learn the Constellations and use the
Red Dot Finder, but if the object is too faint you may want to use setting
circles on your mount. Setting circles enable you to locate celestial objects
whose celestial coordinates have been determined from star charts. Your
telescope must be polar aligned and the R.A. setting circle must be calibrated
before using the setting circles. The DEC. setting circle was set at the
factory and does not require calibrating the same manner as the R.A. setting
circle.
Reading the R.A. setting circle
The telescope’s R.A. setting circle is scaled in hours, from 1 through 24,
with small lines in between representing 10-minute increments. The upper set
of numbers applies to viewing in the Northern Hemisphere, while the numbers
below them apply to viewing in the Southern Hemisphere (Fig.k).
Setting (calibrating) the R.A. setting circle
In order to set your Right Ascension circle you must first find a star in your
field of view with known coordinates. A good one would be the 0.0 magnitude
star Vega in the Constellation Lyra. From a star chart we know the R.A.
coordinate of Vega is 18h 36m. Loosen the R.A. and DEC. lock knobs on the
mount and adjust the telescope so that Vega is centred in the field of view of
the eyepiece. Tighten the R.A. and DEC. lock knobs to lock the mount in place.
Now rotate the R.A. setting circle until it reads 18h36m. You are now ready to
use the setting circles to find objects in the sky.
Finding objects using the setting circles
Example: Finding the faint planetary nebula M57; “The Ring”
From a star chart, we know the coordinates of the Rings are DEC. 33° and R.A.
18h52m. Unlock the DEC. lock knob and rotate your telescope in DEC. until the
pointer on the DEC. setting circle reads 33°. Re-tighten the DEC. lock knob.
Loosen the R.A. lock knob and rotate the telescope in R.A. until the pointer
on the R.A. setting circle reads 18h52m (do not move the R.A. circle). Re-
tighten the R.A. lock knob. Now look through the Red Dot Finder to see if you
have found M57. Adjust the telescope with R.A. and DEC. flexible cables until
M57 is centred in the Red Dot Finder. Now look through the telescope using a
low-power eyepiece. Centre M57 in the field of view of the eyepiece. The
setting circles will get you close to the object you wish to observe but are
not accurate enough to put it in the centre of your Red Dot
Finder’s/finderscope’s field of view. The accuracy of your setting circles
also depends on how accurately your telescope is polar aligned.
POINTING YOUR TELESCOPE
A German Equatorial mount has an adjustment, sometimes called a wedge, which
tilts the mount’s polar axis so that it points at the appropriate Celestial
Pole (NCP or SCP). Once the mount has been polar aligned, it needs to be
rotated around only the polar axis to keep an object centred. Do not
reposition the mount base or change the latitude setting. The mount has
already been correctly aligned for your geographical location (ie. Latitude),
and all remaining telescope pointing is done by rotating the optical tube
around the polar (R.A.)
and declination axes. A problem for many beginners is recognizing that a
polar-aligned, equatorial mount acts like an alt-azimuth mount that has been
aligned to a celestial pole. The wedge tilts the mount to an angle equal to
the observer’s Latitude, and therefore it swivels around a plane that
parallels the celestial (and Earth’s) equator (Fig.l). This is now its
“horizon”; but remember that part of the new horizon is usually blocked by the
Earth. This new “azimuth” motion is called Right Ascension (R.A). In addition,
the mount swivels North(+) and South(-) from the Celestial Equator towards the
celestial poles. This plus or minus “altitude” from the celestial equator is
called Declination (DEC.).
Pointing to the NCP
For the following examples, it is assumed that the observing site is in the
Northern Hemisphere. In the first case (Fig.m2), the optical tube is pointing
to the NCP. This is its probable position following the polar-alignment step.
Since the telescope is pointing parallel to the polar axis, it still points to
the NCP as it is rotated around that axis counter-clockwise, (Fig.m1) or
clockwise (Fig.m3).
Pointing toward the western or eastern horizon
Now, consider pointing the telescope to the western (Fig.n1) or eastern
(Fig.n2) horizon. If the counterweight is pointing North, the telescope can be
swiveled from one horizon to the other around the DEC. axis in an arc that
passes through the NCP (any DEC. arc will pass through the NCP if the mount is
polar-aligned). It can be seen then that if the optical tube needs to be
pointed at an object north or south of this arc, it has to be also rotated
around the R.A axis.
Pointing to directions other than due North
Pointing in any direction other than due North requires a combination of R.A.
and DEC. positions (Fig.o). This can be visualized as a series of DEC. arcs,
each resulting from the position of rotation of the R.A. axis. In practice
however, the telescope is usually pointed, with the aid of a finderscope, by
loosening both the R.A. and DEC. locks and swiveling the mount around both
axes until the object is centered in the eyepiece field. The swivelling is
best done by placing one hand on the optical tube and the other on the
counter-weight bar, so that the movement around both axes is smooth, and no
extra lateral force is applied to the axis bearings. When the object is
centered, make sure the R.A and DEC. locks are both retightened to hold the
object in the field and allow tracking by adjusting only in R.A.
Pointing at an object
Pointing at an object, for example to the South (Fig.p), can often be achieved
with the optical tube positioned on either side of the mount. When there is a
choice of sides, particularly when there could be a long observing period, the
East side (Fig. p2) should be chosen in the Northern Hemisphere because
tracking in R.A. will move it away from the mount’s legs. This is particularly
important when using an R.A motor, because if the optical tube jambs against
the mount’s legs, it can result in damage to the motor and/or the gears.
Telescopes with long focal lengths often have a “blind spot” when pointing
near the zenith, because the eyepiece-end of the optical tube bumps into the
mount’s legs (Fig.q1). To adapt for this, the optical tube can be very
carefully slipped up inside the tube rings (Fig.q2). This can be done safely
because the tube is pointing almost vertically, and therefore moving it does
not cause a DEC.-balance problem. It is very important to move the tube back
to the DEC.-balanced position before observing other sky areas. Something
which can be a problem is that the optical tube often rotates so that the
eyepiece, finderscope and the focussing knobs are in less convenient
positions. The diagonal can be rotated to adjust the eyepiece. However, to
adjust the positions of the finderscope and focussing knobs, loosen the tube
rings holding the optical tube and gently rotate it. Do this when you are
going to view an area for while, but it is inconvenient to do every time you
briefly go to a new area. Finally, there are a few things to consider to
ensure that you are comfortable during the viewing session. First is setting
the height of the mount above the ground by adjusting the tripod legs. You
must consider the height that you want your eyepiece to be, and if possible
plan on sitting on a comfortable chair or stool. Very long optical tubes need
to be mounted higher or you will end up crouching or lying on the ground when
looking at objects near the zenith. On the other hand, a short optical tube
can be mounted lower so that there is less movement due to vibration sources,
such as wind. This is something that should be decided before going through
the effort of polar aligning the mount.
CHOOSING THE APPROPRIATE EYEPIECE
CALCULATING THE MAGNIFICATION (POWER)
The magnification produced by a telescope is determined by the focal length of
the eyepiece that is used with it. To determine a magnification for your
telescope, divide its focal length by the focal length of the eyepieces you
are going to use. For example, a 10mm focal length eyepiece will give 80x
magnification with an 800mm focal length telescope.
When you are looking at astronomical objects, you are looking through a column
of air that reaches to the edge of space and that column seldom stays still.
Similarly, when viewing over land you are often looking through heat waves
radiating from the ground, house, buildings, etc. Your telescope may be able
to give very high magnification but what you end up magnifying is all the
turbulence between the telescope and the subject. A good rule of thumb is that
the usable magnification of a telescope is about 2x per mm of aperture under
good conditions.
CALCULATING THE FIELD OF VIEW
The size of the view that you see through your telescope is called the true
(or actual) field of view and it is determined by the design of the eyepiece.
Every eyepiece has a value, called the apparent field of view, which is
supplied by the manufacturer. Field of view is usually measured in degrees
and/or arc-minutes (there are 60 arc-minutes in a degree). The true field of
view produced by your telescope is calculated by dividing the eyepiece’s
apparent field of view by the magnification that you previously calculated for
the combination. Using the figures in the previous magnification example, if
your 10mm eyepiece has an apparent field of view of 52 degrees, then the true
field of view is 0.65 degrees or 39 arc-minutes.
To put this in perspective, the moon is about 0.5° or 30 arc-minutes in diameter, so this combination would be fine for viewing the whole moon with a little room to spare. Remember, too much magnification and too small a field of view can make it very hard to find things. It is usually best to start at a lower magnification with its wider field and then increase the magnification when you have found what you are looking for. First find the moon then look at the shadows in the craters!
CALCULATING THE EXIT PUPIL
The Exit Pupil is the diameter (in mm) of the narrowest point of the cone of
light leaving your telescope. Know-ing this value for a telescope-eyepiece
combination tells you whether your eye is receiving all of the light that your
primary lens or mirror is providing. The average person has a fully dilated
pupil diameter of about 7mm. This value varies a bit from person to person, is
less until your eyes become fully dark-adapted and decreases as you get older.
To determine an exit pupil, you divide the diameter of the primary of your
telescope (in mm) by the magnification.
For example, a 200 mm f/5 telescope with a 40mm eyepiece produces a magnification of 25x and an exit pupil of 8 mm. This combination can probably be used by a young person but would not be of much value to a senior citizen. The same telescope used with a 32mm eyepiece gives a magnification of about 31x and an exit pupilof 6.4 mm which should be fine for most dark adapted eyes. In contrast, a 200 mm f/10 telescope with the 40mm eyepiece gives a magnification of 50x and an exit pupil of 4 mm, which is fine for everyone.
OBSERVING THE SKY
SKY CONDITIONS
Sky conditions are usually defined by two atmospheric characteristics, seeing,
or the steadiness of the air, and transparen-cy, light scattering due to the
amount of water vapour and particulate material in the air. When you observe
the Moon and the planets, and they appear as though water is running over
them, you probably have bad “seeing” because you are ob-serving through
turbulent air. In conditions of good “seeing”, the stars appear steady,
without twinkling, when you look at them with unassisted eyes (without a
telescope). Ideal “transparency” is when the sky is inky black and the air is
unpolluted.
SELECTING AN OBSERVING SITE
Travel to the best site that is reasonably accessible. It should be away from
city lights, and upwind from any source of air pollution. Always choose as
high an elevation as possible; this will get you above some of the lights and
pollution and will ensure that you aren’t in any ground fog. Sometimes low fog
banks help to block light pollution if you get above them. Try to have a dark,
unobstructed view of the horizon, especially the southern horizon if you are
in the Northern Hemisphere and vice versa. However, remember that the darkest
sky is usually at the “Zenith”, directly above your head. It is the shortest
path through the atmosphere. Do not try to observe any object when the light
path passes near any protrusion on the ground. Even extremely light winds can
cause major air turbulence as they flow over the top of a building or wall.
Observing through a window is not recommended because the window glass will
distort images considerably. And an open window can be even worse, because
warmer indoor air will escape out the window, causing turbulence which also
affects images. Astronomy is an outdoor activity.
CHOOSING THE BEST TIME TO OBSERVE
The best conditions will have still air, and obviously, a clear view of the
sky. It is not necessary that the sky be cloud-free. Often broken cloud
conditions provide excellent seeing. Do not view immediately after sunset.
After the sun goes down, the Earth is still cooling, causing air turbulence.
As the night goes on, not only will seeing improve, but air pollution and
ground lights will often diminish. Some of the best observing time is often in
the early morning hours. Objects are best observed as they cross the meridian,
which is an imaginary line that runs through the Zenith, due North-South. This
is the point at which objects reach their highest points in the sky. Observing
at this time reduces bad atmospheric effects. When observing near the horizon,
you look through lots of atmosphere, complete with turbulence, dust particles
and increased light pollution.
COOLING THE TELESCOPE & ADAPTING YOUR EYES
Telescopes require at least 10 to 30 minutes to cool down to outside air
temperature. This may take longer if there is a big difference between the
temperature of the telescope and the outside air. This minimizes heat wave
distortion inside telescope tube (tube currents). Allow a longer cooling time
for larger optics. If you are using an equatorial mount, use this time for
polar alignment. Do not expose your eyes to anything except red light for 30
minutes prior to observing. This allows your pupils to expand to their maximum
diameter and build up the levels of optical pigments, which are rapidly lost
if exposed to bright light. It is important to observe with both eyes open.
This avoids fatigue at the eyepiece. If you find this too distracting, cover
the non-used eye with your hand or an eye patch. Use averted vision on faint
objects: The center of your eye is the least sensitive to low light levels.
When viewing a faint object, don’t look directly at it. Instead, look slightly
to the side, and the object will appear brighter.
CARE AND MAINTENANCE OF YOUR TELESCOPE
COLLIMATING A NEWTONIAN
Collimation is the process of aligning the mirrors of your telescope so that
they work in concert with each other to deliver properly focused light to your
eyepiece. By observing out-of-focus star images, you can test whether your
telescope’s op-tics are aligned. Place a star in the centre of the field of
view and move the focuser so that the image is slightly out of focus. If the
seeing conditions are good, you will see a central circle of light (the Airy
disc) surrounded by a number of diffraction rings. If the rings are
symmetrical about the Airy disc, the telescope’s optics are correctly
collimated (Fig.r).
If you do not have a collimating tool, we suggest that you make a “collimating
cap” out of a plastic 35mm film canister (black with gray lid). Drill or punch
a small pinhole in the exact center of the lid and cut off the bottom of the
canister. This device will keep your eye centered of the focuser tube. Insert
the collimating cap into the focuser in place of a regular eyepiece.
Collimation is a painless process and works like this: pull off the lens cap
which covers the front of the telescope and look down the optical tube. At the
bottom you will see the primary mirror held in place by three clips 120º
apart, and at the top the small oval secondary mirror held in a support and
tilted 45º toward the focuser outside the tube wall (Fig.s). The secondary
mirror is aligned by adjusting the central bolt behind it, (which moves the
mirror up and down the tube), and the three smaller screws surrounding the
bolt, (which adjust the angle of the mirror). The primary mirror is adjusted
by the three adjusting screws at the back of your scope. The three locking
screws beside them serve to hold the mirror in place after collimation.
(Fig.t) ALIGNING THE SECONDARY MIRROR
Point the telescope at a lit wall and insert the collimating cap into the
focuser in place of a regular eyepiece. Look into the focuser through your
collimating cap. You may have to twist the focus knob a few turns until the
reflected image of the focuser is out of your view. Note: keep your eye
against the back of the focus tube if collimating without a collimating cap.
Ignore the reflected image of the collimating cap or your eye for now, instead
look for the three clips holding the primary mirror in place. If you can’t see
them (Fig.u), it means that you will have to adjust the three bolts on the top
of the secondary mirror holder, with possibly an Allen wrench or Phillip’s
screwdriver. You will have to alternately or loosen one and then compensate
for the slack by tightening the other two. Stop when you see all three mirror
clips (Fig.v). Make sure that all three small alignment screws are tightened
to secure the secondary mirror in place.
ALIGNING THE PRIMARY MIRROR
- Find the three locking screws at the back of your telescope and loosen them by a few turns.
- If you see 3 large nuts protruding from the back of your telescope and 3 small Phillip’s-head screws besides them, the Phillip’s-head screws are the locking screws and the large nuts are the adjusting screws.
- If you see 6 Phillip’s-head screws but 3 protruding from the back of your telescope, the 3 protruding screws are locking screws and the ones next to them are adjusting screws.
- If you see 3 hex bolts and 3 Phillip’s head screws, the hex bolts are the locking screws and the Phillip’s-head screws are the adjusting screws. You will need an Allen wrench to adjust the locking screws.
Now run your ha d around the front of your telescope keeping your eye to the focuser, you will see the reflected image of your hand. The idea here being to see which way the primary mirror is defected, you do this by stopping at the point where the reflected image of the secondary mirror is closest to the primary mirrors’ edge (Fig.w). When you get to that point, stop and keep your hand there while looking at the back end of your telescope, is there a adjusting screw there? If there is you will want to loosen it (turn the screw to the left) to bring the mirror away from that point. If there isn’t a adjusting screw there, then go across to the other side and tighten the adjusting screw on the other side. This will gradually bring the mirror into line until it looks like Fig.x. (It helps to have a friend to help for primary mirror collimation. Have your partner adjust the adjusting screws according to your directions while you look in the focuser.) After dark go out and point your telescope at Polaris, the North Star. With an eyepiece in the focuser, take the image out of focus. You will see the same image only now, it will be illuminated by starlight. If necessary, repeat the collimating process only keep the star centered while tweaking the mirror
TECHNICAL SPECIFICATIONS
WEGA 1000
Lens diameter | 90 mm |
---|---|
Focal length | 1000 mm |
Focal ratio | 1:11,1 |
Accessory mount | 1 ¹/4“ |
Magnifications eyepieces | *PL6 = 166x (332x) PL10 = 100x (200x*) PL25 = 40x |
(80x*)**
*with achromatic Barlow lens 2-times
Tube length| approx. 97 cm
Weight| approx. 10 kg
DELTA 1000
Lens diameter | 114 mm |
---|---|
Focal length | 1000 mm |
Focal ratio | 1:8,8 |
Accessory mount | 1 ¹/4“ |
Magnifications eyepieces | *SR4 = 250x (500x) H12.5 = 80x (160*) H20 = 50x |
(100x*)**
*with 2-times Barlow lens
Tube length| approx. 46,5 cm
Weight| approx. 6 kg
SATURN 900
Lens diameter | 114 mm |
---|---|
Focal length | 900 mm |
Focal ratio | 1:7,9 |
Accessory mount | 1 ¹/4“ |
Magnifications eyepieces | *SR4 = 225x (450x) H12.5 = 72x (144x*) H20 = |
45x (90x*)**
*with 2-times Barlow lens
Tube length| approx. 90 cm
Weight| approx. 11 kg
CLEANING YOUR TELESCOPE
Replace the dust cap over the end of the telescope whenever not in use. This prevents dust from settling on the mirror or lens surface. Do not clean mirrors or lenses unless you are familiar with optical surfaces. Clean finderscope and eyepieces with special lens paper only. Eyepieces should be handled with care, and avoid touching optical surfaces.
NEVER look at the sun through the telescope or viewfinder! Risk of blindness!
DÖRR GmbH Messerschmittstr
- D-89231 Neu-Ulm
- Fon: +49 731.970 37 69
- info@doerr.gmbh.
- www.doerr-outdoor.de.
- doerr-ou67tdoor.de.