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between  the  dark  and  light  portions  of  the  disk  (called  the 
“terminator”). A full Moon is too bright and devoid of surface 
shadows to yield a pleasing view. Make sure to observe the 
Moon when it is well above the horizon to get the sharpest 
images. 
Use an optional Moon filter to dim the Moon when it is very 
bright.  It  simply  threads  onto  the  bottom  of  the  eyepieces 
(you  must  first  remove  the  eyepiece  from  the  focuser  to 
attach a filter). You’ll find that the Moon filter improves view-
ing  comfort,  and  also  helps  to  bring  out  subtle  features  on 
the lunar surface.

B. the Sun

You can change your nighttime telescope into a daytime Sun 
viewer  by  installing  an  optional  full-aperture  solar  filter  over 
the front opening of the SpaceProbe 130mm EQ. The prima-
ry attraction is sunspots, which change shape, appearance, 
and location daily. Sunspots are directly related to magnetic 
activity  in  the  Sun.  Many  observers  like  to  make  drawings 
of sunspots to monitor how the Sun is changing from day to 
day.

Important Note: Do not look at the Sun with any optical 
instrument without a professionally made solar filter, or 
permanent  eye  damage  could  result.  Leave  the  cover 
caps on the finder scope, or better yet, remove the finder 
scope from the telescope tube when solar viewing.

C. the Planets

The  planets  don’t  stay  put  like  the  stars,  so  to  find  them 
you should refer to Sky Calendar at our website (telescope.
com),  or  to  charts  published  monthly  in  Astronomy,  Sky  & 
Telescope
,  or  other  astronomy  magazines. Venus,  Mars, 
Jupiter,  and  Saturn  are  the  brightest  objects  in  the  sky 
after  the  Sun  and  the  Moon. Your  SpaceProbe  130mm  EQ 
is  capable  of  showing  you  these  planets  in  some  detail. 
Other  planets  may  be  visible  but  will  likely  appear  star-like. 
Because  planets  are  quite  small  in  apparent  size,  optional 
higher-power  eyepieces  are  recommended  and  often  need-
ed for detailed observations. Not all the planets are generally 
visible at any one time.

JUPITER 

The  largest  planet,  Jupiter,  is  a  great  subject  for 

observation. You  can  see  the  disk  of  the  giant  planet  and 
watch the ever-changing positions of its four largest moons—
Io, Callisto, Europa, and Ganymede. higher-power eyepieces 
should bring out the cloud bands on the planet’s disk.

SATURN 

The ringed planet is a breathtaking sight when it is 

well positioned. The tilt angle of the rings varies over a peri-
od of many years; sometimes they are seen edge-on, while 
at  other  times  they  are  broadside  and  look  like  giant “ears” 
on  each  side  of  Saturn’s  disk.  A  steady  atmosphere  (good 
seeing) is necessary for a good view. You will probably see a 
bright “star” close by, which is Saturn’s brightest moon, Titan.

VENUS 

At its brightest, Venus is the most luminous object in 

the sky, excluding the Sun and the Moon. It is so bright that 
sometimes it is visible to the naked eye during full daylight! 
Ironically, Venus  appears  as  a  thin  crescent,  not  a  full  disk, 
when  at  its  peak  brightness.  Because  it  is  so  close  to  the 

Sun,  it  never  wanders  too  far  from  the  morning  or  evening 
horizon. No surface markings can be seen on Venus, which 
is always shrouded in dense clouds.

MARS 

The Red Planet makes its closest approach to Earth 

every  two  years.  During  close  approaches  you’ll  see  a  red 
disk, and may be able to see the polar ice cap. To see sur-
face detail on Mars, you will need a high-power eyepiece and 
very steady air!

E. the Stars

Stars will appear like twinkling points of light. Even powerful 
telescopes  cannot  magnify  stars  to  appear  as  more  than  a 
point of light! You can, however, enjoy the different colors of 
the  stars  and  locate  many  pretty  double  and  multiple  stars. 
The  famous  “Double-Double”  in  the  constellation  Lyra  and 
the  gorgeous  two-color  double  star  Albireo  in  Cygnus  are 
favorites.  Defocusing  a  star  slightly  can  help  bring  out  its 
color.

F. Deep-Sky Objects

Under  dark  skies,  you  can  observe  a  wealth  of  fascinating 
deep-sky  objects,  including  gaseous  nebulas,  open  and 
globular star clusters, and a variety of different types of gal-
axies. Most deep-sky objects are very faint, so it is important 
that you find an observing site well away from light pollution. 
Take  plenty  of  time  to  let  your  eyes  adjust  to  the  darkness. 
Do not expect these subjects to appear like the photographs 
you see in books and magazines; most will look like dim gray 
smudges. Our eyes are not sensitive enough to see color in 
deep-sky  objects  except  in  a  few  of  the  brightest  ones.  But 
as you become more experienced and your observing skills 
get  sharper,  you  will  be  able  to  ferret  out  more  and  more 
subtle details and structure. 

How to Find Deep-Sky Objects: Star Hopping

Star hopping, as it is called by astronomers, is perhaps the 
simplest  way  to  hunt  down  deep-sky  objects  to  view  in  the 
night sky. It entails first pointing the telescope at a star close 
to  the  object  you  wish  to  observe,  and  then  progressing  to 
other  stars  closer  and  closer  to  the  object  until  it  is  in  the 
field  of  view  of  the  eyepiece.  It  is  a  very  intuitive  technique 
that has been employed for hundreds of years by profession-
al and amateur astronomers alike. Keep in mind, as with any 
new  task,  that  star  hopping  may  seem  challenging  at  first, 
but will become easier over time and with practice.
To  starhop,  only  a  minimal  amount  of  additional  equipment 
is necessary. A star chart or atlas that shows stars to at least 
magnitude 5 is required. Select one that shows the positions 
of many deep-sky objects, so you will have a lot of options to 
choose from. If you do not know the positions of the constel-
lations in the night sky, you will need to get a planisphere to 
identify them. 
Start  by  choosing  bright  objects  to  view. The  brightness  of 
an  object  is  measured  by  its  visual  magnitude;  the  brighter 
an  object,  the  lower  its  magnitude.  Choose  an  object  with 
a visual magnitude of 9 or lower. Many beginners start with 
the  Messier  objects,  which  represent  some  of  the  best  and 

Summary of Contents for SPACEPROBE 130mm EQ

Page 1: ...mer Optical Products Since 1975 Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831 763 7000 89 Hangar Way Watsonville CA 95076 instruction Manual Orion SpaceProbe 130mm EQ 9851 Equatorial Newtonian Reflector Telescope ...

Page 2: ... Tube mounting rings Tube ring clamps Primary mirror cell Collimation screws 6 R A setting circle Latitude adjustment T bolt Azimuth lock knob Leg lock knob Accessory tray Accessory tray bracket Eyepiece Focuser Dec slow motion control cable Dec setting circle R A lock knob Counterweight Counterweight lock knob Counterweight shaft R A slow motion control cable ...

Page 3: ... screws should be tightened securely to eliminate flexing and wobbling but be careful not to over tighten or the threads may strip Refer to Figure 1 during the assembly process During assembly and anytime for that matter Do not touch the surfaces of the telescope mirrors or the lenses of the finder scopes or eyepieces with your fingers The optical sur Congratulations on your purchase of a quality ...

Page 4: ... latitude lock T bolt is pointing to the mark at 40 To do this loosen the latitude lock T bolt and turn the latitude adjustment T bolt until the pointer and the 40 line up Then retighten the latitude lock T bolt The declination Dec and right ascension R A axes may need re positioning rotation as well Be sure to loosen the RA and Dec lock knobs before doing this Retighten the R A and Dec lock knobs...

Page 5: ... To place the finder scope in the finder scope bracket first unthread the two black nylon screws until the screw ends are flush with the inside diameter of the bracket Place the O ring that comes on the base of the bracket over the body of the finder scope until it seats into the slot on the middle of the finder scope Slide the eyepiece end nar row end of the finder scope into the end of the brack...

Page 6: ...g When you are actually observing with the tele scope you can adjust the eyepiece position by loosening the tube rings and rotating the optical tube 7 Retighten the tube ring clamps The telescope is now balanced on both axes Now when you loosen the lock knob on one or both axes and manually point the telescope it should move without resistance and should not drift from where you point it Focusing ...

Page 7: ...y adjustments until the two images match up NOTE The image in both the finder scope and the main telescope will appear upside down rotated 180 This is normal for finder scopes and reflector telescopes see Figure 5 The finder scope alignment needs to be checked before every observing session This can easily be done at night before viewing through the telescope Choose any bright star or planet cente...

Page 8: ...of the telescope s position to center objects within the field of view Before you can use the cables you must manually slew the mount to point the telescope in the vicinity of the desired target Do this by loosening the R A and Dec lock knobs and moving the telescope about the mount s R A and Dec axes Once the telescope is pointed somewhere close to the object to be viewed retighten the mount s R ...

Page 9: ... object Retighten the thumb screw Finding Objects With the Setting Circles Now that both setting circles are calibrated look up in a star atlas the coordinates of an object you wish to view 1 Loosen the Dec lock knob and rotate the telescope until the Dec value from the star atlas matches the reading on the Dec setting circle Retighten the Dec lock knob 2 Loosen the R A lock knob and rotate the te...

Page 10: ... other collimating devices such as Orion s LaserMate Laser Collimator obviating the need to remove the primary mirror and mark it yourself NOTE The center ring sticker need not ever be removed from the primary mirror Because it lies directly in the shadow of the secondary mirror its presence in no way adversely affects the optical performance of the telescope or the image quality That might seem c...

Page 11: ... one of the pairs of Phillips headed collimation screws one turn Look into the focuser and see if the secondary mirror reflection has moved closer to the center of the primary mirror reflection Repeat this process on the other two pairs of collimation screws if nec essary It will take a little trial and error to get a feel for how to tilt the mirror in this way to center the reflection Look into t...

Page 12: ...ing and Transparency Atmospheric conditions play a huge part in quality of view ing In conditions of good seeing star twinkling is minimal and objects appear steady in the eyepiece Seeing is best overhead worst at the horizon Also seeing generally gets better after midnight when much of the heat absorbed by the Earth during the day has radiated off into space Typically seeing conditions will be be...

Page 13: ...a magnifica tion of 36x and a 10mm which gives a magnification of 90x Other eyepieces can be used to achieve higher or lower powers It is quite common for an observer to own five or more eyepieces to access a wide range of magnifications This allows the observer to choose the best eyepiece to use depending on the object being viewed At least to begin with the two supplied eyepieces will suffice ni...

Page 14: ...ally Venus appears as a thin crescent not a full disk when at its peak brightness Because it is so close to the Sun it never wanders too far from the morning or evening horizon No surface markings can be seen on Venus which is always shrouded in dense clouds MARS The Red Planet makes its closest approach to Earth every two years During close approaches you ll see a red disk and may be able to see ...

Page 15: ...ar on the tube it will not harm the tele scope If you wish you may apply some auto touch up paint to the scratch Smudges on the tube can be wiped off with a soft cloth and a household cleaner such as Windex or Formula 409 Cleaning Lenses Any quality optical lens cleaning tissue and optical lens clean ing fluid specifically designed for multi coated optics can be used to clean the exposed lenses of...

Page 16: ...n a warm area until it is completely dry before reassembling the telescope 9 Specifications Optical tube Steel Primary mirror diameter 130mm Primary mirror coating Aluminized silicon dioxide overcoat Secondary mirror minor axis 34mm Focal length 900mm Focal ratio f 7 Eyepieces 25mm and 10mm Explorer II fully coated 1 25 Magnification 36x with 25mm 90x with 10mm Focuser Rack and pinion Finder scope...

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