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CGE Series Computerized Telescopes

Overview

CELESTRON CGE TELESCOPES

The CGE computerized series is Celestron’s newest line of observatory class Schmidt-Cassegrain telescopes. Offered in 8", 91/4", 11" and 14" apertures, they all come mounted on the state of the art CGE GoTo German Equatorial mount.

The German Equatorial mount has long been the favored choice of astronomy buffs and astrophotographers because of its stability and portability. More stable because the center of gravity is directly over the center of its base, more portable because it can be broken down into smaller component parts for easy storage and transportation.

For astrophotography, the German Equatorial mount offers easier balancing, unlimited space at the rear of the telescope tube to mount a camera, and whole sky access. Now you can enjoy all of the NexStar software and database features with the extra stability and portability of a German Equatorial mount.

In addition to being fully computerized with a database of over 40,000 celestial objects, the CGE German Equatorial mount offers numerous design advantages:

Portability – Set up and transportation of the CGE telescopes is made easy by separating the CGE instruments into smaller, easy-to-carry components. Unlike fork arm mounted telescopes, the CGE’s optical tubes can be quickly removed from their mounts making even the CGE 1400 easily assembled by only one person.

Stability – Recognized for superior stability, German Equatorial mounts place the center of gravity directly over the tripod legs and can be easily polar aligned without the use of an optional equatorial wedge. This proven design reduces the “tuning fork” vibration that can be associated with undersized fork mounts. An improved Super HD Tripod supports the CGE mount. This fully extendable tripod is made from the finest cold rolled carbon steel and can be raised to a height of 50". The tripod uses a dual leg support for maximum rigidity with an upper leg brace to provide an outward preload and a lower leg brace providing inward tension.

Balance – CGE equatorial mounts can easily be balanced in both axes. Simply simply sliding the counterweight for Right Ascension and moving the optical tube along its dovetail mounting for Declination accomplish balancing the weight of camera equipment and other visual accessories. This means that no additional weight needs to be added to balance the telescope when additional accessories are added.

Clearance – CGE mounts support their tubes at a single contact point allowing the tube to move freely around its polar axis without making contact with the telescope’s mount. This is particularly useful when adding photographic and CCD instruments that extend from the rear of the telescopes.

All CGE mounted telescopes are compatible with Celestron’s CN-16 GPS accessory. Combine the GPS and built-in Hibernate mode and these telescopes will keep track and remember their exact location and time without having to enter the information into the hand control.

Other CGE Capabilities Include:

Mechanical Features

  • CNC machined aluminum and stainless steel components
    Autoguide port, PC port and auxiliary ports located on the electronic pier.
  • Strain relief power cord cable protection
  • Backlit power switch
  • Drive Motors – Made in the U.S.A., Pittman® LO-COG™ brush-commutated DC motors offer smooth, quiet operation and long life. The motor armatures are skewed to minimize cogging which is required for low speed tracking. Windings are resin impregnated for greater reliability in incremental motion applications.
  • Precision Bronze Worm Gear – 32 pitch, 5.625" pitch diameter, 180 tooth bronze gear manufactured in the U.S.A. by W. M. Berg, Inc. Manufactured to AGMA Quality Class 10 standard, which minimizes total composite error and backlash.
  • Bearing and Shaft – Stainless steel worm shaft has 0.4375 pitch diameter and is preloaded with two ball bearings. The worm is made from a single piece of steel (rather than a two-piece worm-and-shaft assembly) to minimize run-out, which is a source of periodic error.
  • 4 point RA clutch system for no-slip pointing precision
  • Schmidt-Cassegrain mechanism that moves the primary mirror to adjust focus is supported by two pre-loaded ball bearings, minimizing the “mirror flop” typical of bushing focus mechanisms.
  • Latitude range: 10º to 60º northern or southern hemispheres
  • Maximum payload: 65 lb.

RA and Dec Axis

  • 1" solid ground stainless steel shaft
  • Two preloaded 0.9835" I.D. x 2.047" O.D. tapered roller bearings
  • One 3.543" I.D. x 4.724" O.D. thrust bearing (RA Axis)
  • 180 tooth, 5.625 pitch diameter enveloping bronze gear preloaded to maintain gear mesh when clutch tension varies, manufactured to AGMA 10 quality by W.M. Berg
  • 0.4375" diameter precision 303 stainless steel worm manufactured to AGMA 10 quality
  • Four point RA clutch system pre-loading a 4.65" stainless steel disk for no-slip drive and pointing precision
  • One 2.500" I.D. x 3.250" O.D. thrust bearing (Dec Axis)

Tripod

  • Adjustable height: 36" to 50"
  • Leg material: cold rolled carbon steel
  • Upper leg diameter: 2.75"; lower leg diameter: 2.375"

Electronic and Software Features

  • GoTo system is precision accurate to 1.5 arcminutes
  • 40,000+ object database with 400 user-defined objects. Features include: Compass Calibration, Polar Alignment routine, Database Filter Limits, Hibernate, Auto North and Level, Quick Align, and user-defined slew limits.
  • Hibernate – maintains alignment even while powered down.
  • Polar alignment routines for Northern and Southern hemispheres.
  • Filter limits – displays only objects above the horizon.
  • Permanent programmable periodic error correction (PEC) – corrects for periodic tracking errors inherent to all worm drives.
  • Smooth ramping of slew motors to reduce wear on the drive train.
  • Home sensors on R.A. and Dec axes.
  • Fail-safe slew limit switches in R.A.
  • Real-time clock – maintains time even when powered down.
  • 12VDC Servo Motors with integrated optical encoders with 0.11 arcsecond resolution.
 
CGE 800 (XLT)
sku: 11058-XLT
CGE 800 (XLT)
CGE 925 (XLT)
sku: 11059-XLT
CGE 925 (XLT)
CGE 1100 (XLT)
sku: 11061-XLT
CGE 1100 (XLT)
CGE 1400 (XLT)
sku: 11063-XLT
CGE 1400 (XLT)
OPTICAL DESIGN Learn More Schmidt-Cassegrain Schmidt-Cassegrain Schmidt-Cassegrain Schmidt-Cassegrain
APERTURE Learn More 200 mm (7.87 in) 235 mm (9.25 in) 280 mm (11.02 in) 356 mm (14.02 in)
FOCAL LENGTH Learn More 2032 mm (80 in) 2350 mm (92.52 in) 2800 mm (110.24 in) 3910 mm (153.94 in)
FOCAL RATIO Learn More 10.16 10 10 10.98
FINDERSCOPE Learn More 6x30 6x30 9x50 9x50
MOUNT Learn More Computerized Equatorial Computerized Equatorial Computerized Equatorial Computerized Equatorial
OPTICAL TUBE Learn More Aluminum Aluminum Aluminum Aluminum
FASTAR COMPATIBLE Learn More Yes N/A N/A N/A
EYEPIECE 1 Learn More 25 mm (0.98 in) 25 mm (0.98 in) 40 mm (1.57 in) 40 mm (1.57 in)
MAGNIFICATION 1 Learn More 81 x 94 x 70 x 98 x
STAR DIAGONAL Learn More 1.25 1.25 1.25 1.25"
TRIPOD Learn More Adjustable, Carbon Steel Adjustable, Carbon Steel Adjustable, Carbon Steel Adjustable, Carbon Steel
CD ROM Learn More NexRemote control software with RS232 cable NexRemote control software with RS232 cable NexRemote control software with RS232 cable NexRemote control software with RS232 cable
POWER SUPPLY Learn More Car battery adapter Car battery adapter Car battery adapter Car battery adapter
HIGHEST USEFUL MAGNIFICATION Learn More 472 x 555 x 661 x 841 x
LOWEST USEFUL MAGNIFICATION Learn More 29 x 34 x 40 x 51 x
LIMITING STELLAR MAGNITUDE Learn More 14 14.4 14.7 15.3
DIAMETER Learn More 203.2 mm (8 in) N/A N/A N/A
RESOLUTION (RAYLEIGH) Learn More 0.7 arcsec 0.59 arcsec 0.5 arcsec 0.39 arcsec
RESOLUTION (DAWES) Learn More 0.58 arcsec 0.49 arcsec 0.41 arcsec 0.33 arcsec
PHOTOGRAPHIC RESOLUTION Learn More 200 line/mm 200 line/mm 200 line/mm 165 line/mm
LIGHT GATHERING POWER Learn More 816 x 1127 x 1600 x 2586 x
ANGULAR FIELD OF VIEW Learn More 0.62 ° 0.53 ° 0.71 ° 0.51 °
LINEAR FIELD OF VIEW (@1000 YDS) Learn More 32 ft (9.75 m) 28 ft (8.53 m) 38 ft (11.58 m) 27 ft (8.23 m)
OPTICAL COATINGS Learn More Starbright XLT Coating Starbright XLT Coating Starbright XLT Coating Starbright XLT Coating
SECONDARY MIRROR OBSTRUCTION Learn More 2.7 in (68.58 mm) 3.35 in (85.09 mm) 3.75 in (95.25 mm) 4.5 in (114.3 mm)
SECONDARY MIRROR OBSTRUCTION BY AREA Learn More 11.8 % 13.1 % 11.6 % 10.3 %
SECONDARY MIRROR OBSTRUCTION BY DIAMETER Learn More 34.3 % 36.2 % 34 % 32.1 %
OPTICAL TUBE LENGTH Learn More 17 in (431.8 mm) 22 in (558.8 mm) 24 in (609.6 mm) 31 in (787.4 mm)
OPTICAL TUBE WEIGHT Learn More 12.5 lb (5.67 kg) 20 lb (9.07 kg) 27.5 lb (12.47 kg) 45 lb (20.41 kg)
TRIPOD AND PIER WEIGHT Learn More 41.5 lb (18.82 kg) 41.5 lb (18.82 kg) 41.5 lb (18.82 kg) 41.5 lb (18.82 kg)
EQ MOUNT WEIGHT Learn More 42 lb (19.05 kg) 42 lb (19.05 kg) 42 lb (19.05 kg) 42 lb (19.05 kg)
COUNTERWEIGHT BAR Learn More 5 lb (2.27 kg) 5 lb (2.27 kg) 5 lb (2.27 kg) 5 lb (2.27 kg)
COUNTERWEIGHTS Learn More 1 x 11 lb 1 x 25 lb 1 x 25 lb 2 x 25 lb
MOTOR DRIVE Learn More DC Servo motors with encoders, both axes DC Servo motors with encoders, both axes DC Servo motors with encoders, both axes DC Servo motors with encoders, both axes
COMPUTER HAND CONTROL Learn More Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons
SLEW SPEEDS Learn More Nine slew speeds: 4°/sec, 2°/sec, .5°/sec, 64x, 16x, 8x, 4x, 1x, .5x Nine slew speeds: 4°/sec, 2°/sec, .5°/sec, 64x, 16x, 8x, 4x, 1x, .5x Nine slew speeds: 4°/sec, 2°/sec, .5°/sec, 64x, 16x, 8x, 4x, 1x, .5x Nine slew speeds: 4°/sec, 2°/sec, .5°/sec, 64x, 16x, 8x, 4x, 1x, .5x
TRACKING RATES Learn More Sidereal, Solar and Lunar Sidereal, Solar and Lunar Sidereal, Solar and Lunar Sidereal, Solar and Lunar
TRACKING MODES Learn More EQ North and EQ South EQ North and EQ South EQ North and EQ South EQ North and EQ South
ALIGNMENT PROCEDURES Learn More AutoAlign, 2-Star Align, Quick Align, 1-Star Align, Recall Last Alignment, 3-Star Align AutoAlign, 2-Star Align, Quick Align, 1-Star Align, Recall Last Alignment, 3-Star Align AutoAlign, 2-Star Align, Quick Align, 1-Star Align, Recall Last Alignment, 3-Star Align AutoAlign, 2-Star Align, Quick Align, 1-Star Align, Recall Last Alignment, 3-Star Align
SOFTWARE PRECISION Learn More 24bit, 0.08 calculation 24bit, 0.08 calculation 24bit, 0.08 calculation 24bit, 0.08 calculation
DATABASE Learn More 40,000+ objects, 100 user defined programmable objects. Enhanced information on over 200 objects 40,000+ objects, 100 user defined programmable objects. Enhanced information on over 200 objects 40,000+ objects, 100 user defined programmable objects. Enhanced information on over 200 objects 40,000+ objects, 100 user defined programmable objects. Enhanced information on over 200 objects
POWER REQUIREMENTS Learn More 12 VDC 2A 12 VDC 2A 12 VDC 2.0A 12 VDC 2.0A
POWER REQUIREMENTS - IDLE CURRENT Learn More 215 mA 215 mA 215 mA 215 mA
POWER REQUIREMENTS - SLEW ONE AXIS Learn More 600 mA 600 mA 600 mA 600 mA
POWER REQUIREMENTS - SLEW BOTH AXES Learn More 850 mA 850 mA 850 mA 850 mA
INTERNAL CLOCK Learn More Yes Yes Yes Yes
GPS Learn More Optional CN-16 GPS Accessory Optional CN-16 GPS Accessory Optional CN-16 GPS Accessory Optional CN-16 GPS Accessory
 
 
CGE 1400 Fastar (XLT)
sku: 11064-XLT
CGE 1400 Fastar (XLT)
CGE Computerized Mount
sku: 91524
CGE Computerized Mount
OPTICAL DESIGN Learn More Schmidt-Cassegrain N/A
APERTURE Learn More 356 mm (14.02 in) N/A
FOCAL LENGTH Learn More 3910 mm (153.94 in) N/A
FOCAL RATIO Learn More 10.98 N/A
FINDERSCOPE Learn More 9x50 N/A
MOUNT Learn More Computerized Equatorial N/A
OPTICAL TUBE Learn More Aluminum N/A
FASTAR COMPATIBLE Learn More Yes N/A
EYEPIECE 1 Learn More 40 mm (1.57 in) N/A
MAGNIFICATION 1 Learn More 98 x N/A
STAR DIAGONAL Learn More 1.25" N/A
TRIPOD Learn More Adjustable, Carbon Steel N/A
CD ROM Learn More NexRemote control software with RS232 cable N/A
POWER SUPPLY Learn More Car battery adapter N/A
HIGHEST USEFUL MAGNIFICATION Learn More 841 x N/A
LOWEST USEFUL MAGNIFICATION Learn More 51 x N/A
LIMITING STELLAR MAGNITUDE Learn More 15.3 N/A
DIAMETER Learn More N/A N/A
RESOLUTION (RAYLEIGH) Learn More 0.39 arcsec N/A
RESOLUTION (DAWES) Learn More 0.33 arcsec N/A
PHOTOGRAPHIC RESOLUTION Learn More 165 line/mm N/A
LIGHT GATHERING POWER Learn More 2586 x N/A
ANGULAR FIELD OF VIEW Learn More 0.51 ° N/A
LINEAR FIELD OF VIEW (@1000 YDS) Learn More 27 ft (8.23 m) N/A
OPTICAL COATINGS Learn More Starbright XLT Coating N/A
SECONDARY MIRROR OBSTRUCTION Learn More 4.5 in (114.3 mm) N/A
SECONDARY MIRROR OBSTRUCTION BY AREA Learn More 10.3 % N/A
SECONDARY MIRROR OBSTRUCTION BY DIAMETER Learn More 32.1 % N/A
OPTICAL TUBE LENGTH Learn More 31 in (787.4 mm) N/A
OPTICAL TUBE WEIGHT Learn More 45 lb (20.41 kg) N/A
TRIPOD AND PIER WEIGHT Learn More 41.5 lb (18.82 kg) N/A
EQ MOUNT WEIGHT Learn More 42 lb (19.05 kg) N/A
COUNTERWEIGHT BAR Learn More 5 lb (2.27 kg) N/A
COUNTERWEIGHTS Learn More 2 x 25 lb N/A
MOTOR DRIVE Learn More DC Servo motors with encoders, both axes N/A
COMPUTER HAND CONTROL Learn More Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons N/A
SLEW SPEEDS Learn More Nine slew speeds: 4°/sec, 2°/sec, .5°/sec, 64x, 16x, 8x, 4x, 1x, .5x N/A
TRACKING RATES Learn More Sidereal, Solar and Lunar N/A
TRACKING MODES Learn More EQ North and EQ South N/A
ALIGNMENT PROCEDURES Learn More AutoAlign, 2-Star Align, Quick Align, 1-Star Align, Recall Last Alignment, 3-Star Align N/A
SOFTWARE PRECISION Learn More 24bit, 0.08 calculation N/A
DATABASE Learn More 40,000+ objects, 100 user defined programmable objects. Enhanced information on over 200 objects N/A
POWER REQUIREMENTS Learn More 12 VDC 2A N/A
POWER REQUIREMENTS - IDLE CURRENT Learn More 215 mA N/A
POWER REQUIREMENTS - SLEW ONE AXIS Learn More 600 mA N/A
POWER REQUIREMENTS - SLEW BOTH AXES Learn More 850 mA N/A
INTERNAL CLOCK Learn More Yes N/A
GPS Learn More Optional CN-16 GPS Accessory N/A
 

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Images

SH2-132

SH2-132

SH2-132 22h.14m.24s +56.04.21 N
During the 1950s Stewart Sharpless cataloged many Nebulae, this object is one of Stewart's objects, Located in the Constellation of Cepheus it is often over look by astrophotographers due to the proximity of IC1396 the Elephant Trunk Nebula, it is quite a nice nebula with many dark globules and shock fronts

Camera Canon 350d Modified Baader IR/UV
Astrononmik CLS EOS Broadband Filter
Scope Carbon Fibre Celestron C8 w. 6.3 reducer
Mount Celestron CGE
4 hrs Exposure from light polluted skies
Captured 12-1-08, 12-2-08, 12-3-08
total of 40 6 Minute Subs

captured using CGE 800 (XLT)

submitted by John_Buonomo
Messier 106

Messier 106

Messier 106 (also known as NGC 4258) is a spiral galaxy about in the constellation Canes Venatici. It was discovered by Pierre M�chain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. It is also a Seyfert II galaxy, which means that due to x-rays and unusual emission lines detected, it is suspected that part of the galaxy is falling into a supermassive black hole in the center.[7] NGC 4217 is a possible companion galaxy of Messier 106.[6]

Desc- Wiki.org

captured using CGE 800 (XLT)

submitted by John_Buonomo
Messier 42,43 and NGC1977

Messier 42,43 and NGC1977

The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated south[b] of Orion's Belt. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,270�76 light years[2] and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light years across. Older texts frequently referred to the Orion Nebula as the Great Nebula in Orion or the Great Orion Nebula. Yet older, astrological texts refer to it as Ensis (Latin for "sword"), which was also the name given to the star Eta Orionis, which can be seen close to the nebula from Earth.[5]

The Orion Nebula is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely studied celestial features.[6] The nebula has revealed much about the process of how stars and planetary systems are formed from collapsing clouds of gas and dust. Astronomers have directly observed protoplanetary disks, brown dwarfs, intense and turbulent motions of the gas, and the photo-ionizing effects of massive nearby stars in the nebula.There are also supersonic bullets of gas piercing through the dense hydrogen clouds of the Orion Nebula. Each bullet is ten times the diameter of Pluto's orbit and are tipped with iron atoms glowing bright blue.They were probably formed one thousand years ago from an unkown violent event.

-Desc -Wiki.org

captured using CGE 800 (XLT)

submitted by John_Buonomo
The Horsehead and Flame Nebula

The Horsehead and Flame Nebula

The Horsehead Nebula (also known as Barnard 33 in bright nebula IC 434) is a dark nebula in the Orion constellation. The nebula is located just below Alnitak, the star furthest left on Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. It is approximately 1500 light years from Earth. It is one of the most identifiable nebulae because of the shape of its swirling cloud of dark dust and gases, which is similar to that of a horse's head. The shape was first noticed in 1888 by Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory.


The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming.



Desc- Wiki.org

captured using CGE 800 (XLT)

submitted by John_Buonomo
Orion's Sword

Orion's Sword

The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated south[b] of Orion's Belt. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,270�76 light years[2] and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light years across. Older texts frequently referred to the Orion Nebula as the Great Nebula in Orion or the Great Orion Nebula. Yet older, astrological texts refer to it as Ensis (Latin for "sword"), which was also the name given to the star Eta Orionis, which can be seen close to the nebula from Earth.[5]

The Orion Nebula is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely studied celestial features.[6] The nebula has revealed much about the process of how stars and planetary systems are formed from collapsing clouds of gas and dust. Astronomers have directly observed protoplanetary disks, brown dwarfs, intense and turbulent motions of the gas, and the photo-ionizing effects of massive nearby stars in the nebula. There are also supersonic bullets of gas piercing through the dense hydrogen clouds of the Orion Nebula. Each bullet is ten times the diameter of Pluto's orbit and are tipped with iron atoms glowing bright blue. They were probably formed one thousand years ago from an unknown violent event.



-Wiki Desc

captured using CGE 800 (XLT)

submitted by John_Buonomo
IC443 The JellyFish Nebula

IC443 The JellyFish Nebula

IC 443 (also known as the Jellyfish Nebula) is a Galactic supernova remnant (SNR) in the constellation Gemini. On the plan of the sky, it is located near the star Eta Geminorum. Its distance is roughly 5,000 light years (~5�1016 km) from Earth.
IC 443 is thought to be the remains of a supernova occurred 3,000 - 30,000 years ago. The same supernova event likely created the neutron star CXOU J061705.3+222127, the collapsed remnant of the stellar core.
IC 443 is one of the best-studied case of supernova remnant interacting with surrounding molecular clouds.

captured using CGE 800 (XLT)

submitted by John_Buonomo
The Xmas Tree Cluster

The Xmas Tree Cluster

NGC 2264 is sometimes referred to as the Christmas Tree Cluster and the Cone Nebula. However, the designation of NGC 2264 in the New General Catalogue refers to both objects and not the cluster alone.

captured using CGE 800 (XLT)

submitted by John_Buonomo
The Rosette Nebula

The Rosette Nebula

The Rosette Nebula is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter.

captured using CGE 800 (XLT)

submitted by John_Buonomo
Section of Aurigae

Section of Aurigae

Section of the Constellation Auriga which Includes a few Intresting Objects
At the Top are the Tadpoles of IC410, In the Middle is IC417 and the Clusters at the bottom are Messier 38 and NGC1907

captured using CGE 800 (XLT)

submitted by John_Buonomo
NGC2174 the Monkey Head Nebula

NGC2174 the Monkey Head Nebula

NGC 2174 is an H II emission nebula located in the constellation Orion and is associated with the open star cluster NGC 2175 It is thought to be located about 6400 light-years away from earth. The nebula may have formed through hierarchical collapse, To the lower part of the image is a SuperNova Remenant cataloged by Stewart Sharpless in the 1950s as catalog entry, sh2-247

captured using CGE 800 (XLT)

submitted by John_Buonomo
moon

moon


captured using CGE 925 (XLT)

submitted by Tibi
M13

M13


captured using CGE 925 (XLT)

submitted by Tibi
dumbbellnebula (m27)

dumbbellnebula (m27)

Magnitude: 7.30
Luminosit� surfacique: 11.20
Description: !!vB,vL,bi-N,IE,Dumbbell Neb
PK60-3.1;Lord Rosse drew 18* invl

captured using CGE 925 (XLT)

submitted by satlocenr
Polaris

Polaris

image was taken in prime focus

captured using CGE 925 (XLT)

submitted by travd
NGC 2841

NGC 2841

NGC 2841, a nice galaxy and a difficult target.

captured using CGE 925 (XLT)

submitted by hgg
M51

M51

alaxie M 101 (NGC 5457)
Constellation: Grande Ourse
Dimension: 28.5'x 28.3' / Magnitude: 7.90
Luminosit� surfacique: 14.90

J2000 RA: 14h03m12.00s DE:+54�20'60.0"
Date RA: 14h03m31.80s DE:+54�18'19.3"
D�PART DE LA S�ANCE : Azimut : +65�49' / Altitude :+69�45'
FIN DE LA S�ANCE : Azimut : +255�13' / Altitude : +80�59'
Culmination : 23h45m

captured using CGE 925 (XLT)

submitted by satlocenr
NGC4631 - The Whale Galaxy

NGC4631 - The Whale Galaxy

NGC4631, The Whale Galaxy

captured using CGE 925 (XLT)

submitted by hgg
M13 - Hercules Cluster

M13 - Hercules Cluster

One of the most beautiful star clusters of the nothern hemisphere!

captured using CGE 925 (XLT)

submitted by hgg
andromeda-wide

andromeda-wide

This was shot with 300mm zoom piggybaked. One 5 min. shot before dew invaded my lenses.

captured using CGE 925 (XLT)

submitted by Ed_Malm
The Galactic Kiwi!

The Galactic Kiwi!

The Galactic Centre, Just an update to my last image.

captured using CGE 1100 (XLT)

submitted by Terry_nz
M16 Narrowband

M16 Narrowband


captured using CGE 1100 (XLT)

submitted by drpdmartin
B33

B33

This is a combination of 3 Different images with 3 different cameras and focal lenghs combined in Registar

captured using CGE 1100 (XLT)

submitted by Les T
CGE1100 Field Equipment

CGE1100 Field Equipment

This is my standard Star Party portable equipment. I've built a computer hutch which folds flat for transport, and all the equipment fits into my Chevy Blazer. The computer is a home built 2.4 GHz Athlon tower with MaximDL, Celestron's NexRemote and PEC (both fantastic), TheSky6, Maxpoint, and Photoshop CS3.

captured using CGE 1100 (XLT)

submitted by drpdmartin
Saturn

Saturn

Saturn captured at f/20 with C11, Neximage

captured using CGE 1100 (XLT)

submitted by tbone44011
M42

M42

See the comments for Markarian's chain

captured using CGE 1100 (XLT)

submitted by drpdmartin
Markarian's Chain

Markarian's Chain

Texas Star Party 2009
Fantastic seeing
Hyperstar 3/QHY8:
FOV=2.4 X 1.6 arc min
Inset is M88 enlarged to show the detail present in the image

captured using CGE 1100 (XLT)

submitted by drpdmartin
North American Nebula

North American Nebula


captured using CGE 1100 (XLT)

submitted by drpdmartin
Trifid Lagoon Nebulas

Trifid Lagoon Nebulas


captured using CGE 1100 (XLT)

submitted by drpdmartin
M13 - The Great Hercules Cluster

M13 - The Great Hercules Cluster

I was testing what ISO 3200 can do.

captured using CGE 1400 (XLT)

submitted by Fred_Caron
Jupiter and Io

Jupiter and Io

Io can be seen clearly above the NEB. The GRS, red Junior and the new red spot all grace this image. A wonderful night.

captured using CGE 1400 (XLT)

submitted by Paul_Haese
Saturn

Saturn

This image was taken from 35 degrees South at a time when Saturn was near its most northern declination. Saturn was at 44 degrees from the horizon.

captured using CGE 1400 (XLT)

submitted by Paul_Haese
Jupiter and Callisto

Jupiter and Callisto

Callisto can be seen here with detail showing as it moves onto the limb of Jupiter. The new spots near the GRS can also be seen well too.

captured using CGE 1400 (XLT)

submitted by Paul_Haese
Mars

Mars

Mars, with IR + Blue, synth. G Chanal;

captured using CGE 1400 (XLT)

submitted by Christoph_Kaltseis
Cat's eye nebula, ngc 6543

Cat's eye nebula, ngc 6543

Planetary nebula in Draco. The angular size is about 20" (about 1/2 of Jupiters diameter)

captured using CGE 1400 (XLT)

submitted by erlend_langsrud@hotmail.com
Vega

Vega


captured using CGE 1400 (XLT)

submitted by omegaequalsone
NGC 6934

NGC 6934

GLobular cluster NGC 6934

captured using CGE 1400 (XLT)

submitted by al@kellysky.net
Saturn

Saturn

Saturn as seen from my backyard

captured using CGE 1400 (XLT)

submitted by jrstegeman
moon at the telephone

moon at the telephone

A piece of Moon just take with the phone camera
(1 frame)

captured using CGE 1400 Fastar (XLT)

submitted by marcdica
Moon at the phone II

Moon at the phone II

A new photo putting only the phone camera on a new eyepiece, testing to wiew a full moon image without focal reducer

captured using CGE 1400 Fastar (XLT)

submitted by marcdica
Maris Crisium

Maris Crisium


captured using CGE 1400 Fastar (XLT)

submitted by marcdica
Half Moon with phone camera

Half Moon with phone camera

Half Moon, low resolution and free hand shot in eyepiece projection

captured using CGE 1400 Fastar (XLT)

submitted by marcdica
Messier 82 the Cigar

Messier 82 the Cigar

Messier 82 (also known as NGC 3034 or the Cigar Galaxy) is the prototype[3] nearby starburst galaxy about 12 million light-years away in the constellation Ursa Major. The starburst galaxy is five times as bright as the whole Milky Way and one hundred times as bright as our galaxy's center.[3]

In 2005, the Hubble revealed 197 young massive clusters in the starburst core.[3] The average mass of these clusters is around 2�105 M⊙, hence the starburst core is a very energetic and high-density environment.[3] Throughout the galaxy's center, young stars are being born 10 times faster than they are inside our entire Milky Way Galaxy.[4]

captured using CGE Computerized Mount

submitted by John_Buonomo
NGC2903 Galaxy in Leo

NGC2903 Galaxy in Leo

NGC 2903 is a barred spiral galaxy about 20.5 million light-years away in the constellation Leo. It was discovered by William Herschel who cataloged it as on November 16, 1784. NGC 2905 is a bright knot (star cloud) within this galaxy.

captured using CGE Computerized Mount

submitted by John_Buonomo
Messier 46 Ngc 2438

Messier 46 Ngc 2438

Messier 46 (also known as M 46 or NGC 2437) is an open cluster in the constellation of Puppis. It was discovered by Charles Messier in 1771. Dreyer described it as "very bright, very rich, very large." M46 is about 5,500 light-years away with an estimated age on the order of several 100 million years.[1]

The planetary nebula NGC 2438 appears to lie within the cluster near its northern edge (the faint smudge at the top center of the image), but it is most likely unrelated since it does not share the cluster's radial velocity.[1][2] The case is yet another example of a superposed pair, joining the famed case of NGC 2818. [3][1]

M46 is about a degree east of M47 in the sky, so the two fit well in a binocular or wide-angle telescope field.

- Wiki

captured using CGE Computerized Mount

submitted by John_Buonomo
Eskimo Nebula (NGC 2392)

Eskimo Nebula (NGC 2392)

The Eskimo Nebula (NGC 2392), also known as the Clownface Nebula,[4] is a bipolar[2] double-shell[5] planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. From the ground, it resembles a person's head surrounded by a parka hood. In 2000, the Hubble Space Telescope produced an image of it. From space, the nebula displays gas clouds so complex that they are not fully understood.

Its inner shell measures 18″ � 15″ and is bright and elliptical and marked on its south rim by two blister-like protrusions. Its outer shell is nearly circular measuring 24″ radius and contains a set of complex low-ionization features. It is observed to have high-dispersion spectra of optical nebular lines which indicate a fast collimated outflow with a velocity along our line of sight of nearly 200 km/s producing dynamic interaction with nebular material. As of 2003, it is estimated to be only ≥1060 years old. The earth's perspective is almost along its axis of symmetry. Its knots have a highly developed symmetry along a radius vector from the PN's central star, except their tails are somewhat irregular. The tails are well developed and frequently of a discernible optical thickness in the visual spectrum. The knots are bright rimmed and have low ionization (as compared to those found in NGC 7293) which indicates their location being inside the ionized zone yet close to the boundary. The knots' heads have local photoionization fronts which appear as bright cusps. At the cusps, the knots become optically thick to Lyc photons from the central star.

It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by strong wind of particles from the central star. The outer disk contains unusual light-year long orange filaments.

NGC 2392 lies about 3000 light-years away and is visible with a small telescope in the constellation of Gemini.

- Wiki

captured using CGE Computerized Mount

submitted by John_Buonomo
Messier 1 The Crab Nebula

Messier 1 The Crab Nebula

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The nebula was first observed by John Bevis, and corresponds to a bright supernova recorded by Chinese and Arab astronomers in 1054. Located at a distance of about 6,500 light-years (2 kpc) from Earth, the nebula has a diameter of 11 ly (3.4 pc) and expands at a rate of about 1,500 kilometers per second.

At the center of the nebula lies the Crab Pulsar, a rotating neutron star, which emits pulses of radiation from gamma rays to radio waves with a spin rate of 30.2 times per second. The nebula was the first astronomical object identified with a historical supernova explosion.

The nebula acts as a source of radiation for studying celestial bodies that occult it. In the 1950s and 1960s, the Sun's corona was mapped from observations of the Crab's radio waves passing through it, and more recently, the thickness of the atmosphere of Saturn's moon Titan was measured as it blocked out X-rays from the nebula.


- WIKI

captured using CGE Computerized Mount

submitted by John_Buonomo
NGC 4244 the Splinter Galaxy

NGC 4244 the Splinter Galaxy

NGC 4244, also Caldwell 26, is an edge-on loose Spiral galaxy and Caldwell object in the constellation Canes Venatici. It shines at magnitude +10.2/+10.6. Its celestial cooridinates are RA 12h 17.5m, dec +37� 49′. It is located near a naked-eye G-class star Beta Canum Venaticorum, barred spiral galaxy NGC 4151, and irregular galaxy NGC 4214. The galaxy lies approximately 6.5 million[1]/14 million[2] light years away, with a redshift of +243/493[1] km/s. A nuclear star cluster and halo is located at the centre of this galaxy.[2][3]

- Wiki

captured using CGE Computerized Mount

submitted by John_Buonomo
Messier 3

Messier 3

Messier 3 (also known as M3 or NGC 5272) is a globular cluster in the constellation Canes Venatici. It was discovered by Charles Messier in 1764, and resolved into stars by William Herschel around 1784. This cluster is one of the largest and brightest, and is made up of around 500,000 stars. It is located at a distance of about 33,900 light-years away from Earth. M3 has an apparent magnitude of 6.2, making it visible to the naked eye under dark conditions. From a moderate-sized telescope, the cluster is fully defined.



- Wiki

captured using CGE Computerized Mount

submitted by John_Buonomo
Messier 67 Cluster In Cancer

Messier 67 Cluster In Cancer

Messier 67 (also known as M67 or NGC 2682) is an open cluster, or galactic cluster, in the constellation Cancer. M67's Trumpler class is variously given as II 2 r, II 2 m, or II 3 r. It was discovered by Johann Gottfried Koehler in 1779. Its age is estimated at between 3.2 and 5 billion years. The most recently estimated age of four billion years appears to be the most reliable[citation needed]; thus the stars of M67 are most likely slightly younger than the Sun.

M67 is not the oldest known open cluster, but there are very few in the galaxy known to be older. M67 is an important laboratory for studying stellar evolution, since all its stars are at the same distance and age, except for approximately 30 anomalous blue stragglers[1], whose origins are not fully understood.

M67 is one of the most-studied open clusters, yet estimates of its physical parameters such as age, mass, and number of stars of a given type, vary substantially. Richer et al. [2] estimate its age to be 4 Gyr, its mass to be 1080 solar masses, and the number of white dwarfs to be 150. Hurley et al. [3] estimate its current mass to be 1400 solar masses and its initial mass to be approximately 10 times as great.

M67 has more than 100 stars similar to the Sun, and many red giants. The total star count has been estimated at over 500[citation needed]. The cluster contains no main sequence stars bluer than spectral type F, other than perhaps some of the blue stragglers, since the brighter stars of that age have already left the main sequence. In fact, when the stars of the cluster are plotted on the Hertzsprung-Russell diagram, there is a distinct "turn-off" representing the stars which are just about to leave the main sequence and become red giants. As the cluster ages, the turn-off will move down the main sequence.

It appears that M67 does not contain an unbiased sample of stars. One cause of this is mass segregation, the process by which lighter stars (actually, systems) gain speed at the expense of more massive stars during close encounters, which causes the lighter stars to be at a greater average distance from the center of the cluster or to escape altogether[4


- WIKI

captured using CGE Computerized Mount

submitted by John_Buonomo
M101 Galaxy with Edge HD8 on CGE and 20d

M101 Galaxy with Edge HD8 on CGE and 20d

M101 Galaxy with Edge HD8 on cge guided with MetaGuide and OAG. Canon 20d, un-mod.

captured using CGE Computerized Mount

submitted by FrankMG
M65 M66 Edge HD8

M65 M66 Edge HD8

M65 and M66 galaxies with Edge HD8 on CGE guided with MetaGuide OAG. Un-Mod Canon 20d. Capture and processing with ImagesPlus

captured using CGE Computerized Mount

submitted by FrankMG

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