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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
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$185.00
Specifications
|
Model
|
miniGuideScope |
|
Diameter
|
30mm |
|
Focal Length
|
130mm |
|
Aperture
|
1:4.3 |
|
Object Lens Type
|
Doublet |
|
Focus System
|
Front Side Focuser |
|
Focus Locker
|
Yes |
| Camera Interface | C/CS Mount |
| Compatible Cameras | QHY5II and QHY5III series |
| Anti-Scatter Light Matt Paint | Yes, Internal painted |
| Weight (OTA only) | 111g |
| Telescope Connector | Optional Standard ViewFinder Scope Connector with Tripod Screw Thread |
| Diameter of the OAT | 31.6mm |
| Focus Adjustable Range | Inf. to 1.5 meter |
Suggested Guide Cameras
The new CFW3 series filter wheels are available in four sizes to accommodate filters from 1.25-inch to 50 millimeters square.
For filter wheel control a custom QHY 4-pin filter wheel port is included that provides power and control signals for QHY dual control filter wheels like the series 3 filter wheels. Both the series 2 and new series 3 filter wheels can be controlled by either an independent external program using the filter wheel’s USB port or via the QHY 4-pin serial port. When connected to the QHY 4-pin port there is no need for an additional power cable or control program. All of the filter wheel functions are controlled through the camera and its operating Software.
The series 3 filter wheels utilize a new motor with direct drive and will reverse direction to take the shortest path when moving from one filter to another. For Example, in this demonstration the wheel moves from filter position 1 to position 2 to position 3 and then back to 1 again, over to position 7 and back to position 1 without ever making a complete rotation of the carousel. This saves time if you’re doing a lot of filter changes in one imaging session.
LED changes color for each filter position. The tricolor LED assigns one unique color or combination of colors to each filter position so you can tell if it’s moved to the correct position without removing it from the Telescope.
The CFW3 is also thin. This feature and the short back focus of the COLDMOS cameras means you can add one of several camera lens adapters for Canon and Nikon camera lenses for wide field imaging with the filter wheel.
In the center of the back plate is a 12-volt DC power port. This port is threaded for a short extension cable that is supplied with the camera that securely attaches such that it will not accidentally disconnect while you are imaging.
| Filter Wheel | Filter Supported | Recommended Gears | Back Focus Consumed* | Weight | Note |
| CFW3S-SR CFW3S-US |
7*1.25-inch mounted/31mm unmounted | QHY533M, QHY183M QHY5III Mono Planetary Cams (CFW1.25”Adapter needed) |
20mm (SR)+4mm (Adapter) 15.5mm (SR)+4mm (Adapter) |
About 430g | There’s no difference between S-SR and S-US expect their depth, but S-SR can be compatible with thicker 1.25” mounted filters. |
| CFW3M-SR | 5*2-inch mounted/50mm unmounted | QHY268M, QHY600M | 20.5mm+2mm (Adapter) | About 720g | |
| CFW3M-US | 7*36mm unmounted | QHY163M, QHY294M, QHY268M | 17mm+2mm (Adapter) | About 700g | |
| CFW3L | 7*2-inch mounted/50mm unmounted | QHY600M (PH/Pro) | 21.5mm | About 900g | |
| CFW3XL | 9*2-inch mounted/50mm unmounted
or 7*50mm square unmounted |
QHY461PH
QHY600M-PH SBFL |
21.5mm | About 1500g | A special adapter needed when connecting QHY600 SBFL and CFW3XL, see https://www.qhyccd.com/qhy600sbfl-cfw3xl-adapter/ |
Celestron has reinvented the Tabletop Dobsonian telescope with StarSense Explorer—the first Tabletop Dobsonian that uses your smartphone to analyze the night sky and calculate its position in real-time. This larger-aperture Celestron StarSense Explorer is ideal for beginners, thanks to the app's user-friendly interface and detailed tutorials. It's like having your own personal tour guide of the night sky.
Dock, Launch, Explore
Leave complicated star charts, imprecise planetarium apps, and computerized mounts behind. With StarSense Explorer, locating objects has never been easier, faster, or more accurate. Within minutes of setting up the telescope, you'll be navigating the sky with confidence. Simply place your phone in the unique StarSense dock and launch the StarSense Explorer app.
After aligning your phone to the telescope's optics (a quick and easy procedure), StarSense Explorer generates a list of celestial objects currently visible. Make your selection and arrows appear on-screen, guiding you as you move the telescope. When the object is ready to view in the eyepiece, the bullseye turns green. As you observe, listen to hundreds of audio descriptions and view detailed information about thousands of objects within the app’s robust database.
High-Quality Altazimuth Base
The stable Tabletop Dobsonian base provides a sturdy foundation for StarSense Explorer. The tabletop base is compact, lightweight, and easy to transport, making it perfect for travel. The base’s low-profile makes accessing the eyepiece easier for some observers (especially children). You can also place the base on a stable platform, like a table or hood of a car, to raise it to a comfortable viewing height. Consider adding the optional tripod for even more viewing options.
Teflon bearings provide smooth motion in both altitude and azimuth. The integrated altitude "brake" system allows you to adjust the tension along the altitude axis to ensure the smoothest motion, even with slight imbalances. The panning knob on the telescope tube provides an ergonomic grip so you can precisely point the telescope without introducing heat from your hands into the optical system. As celestial objects appear to drift across the night sky, you’ll be able to follow them easily.
The optical tube connects to the base via tube rings. It’s easy to adjust the tube’s position in the rings so the focuser is in the best viewing position. The base features an eyepiece rack to keep your extra eyepiece(s) close at hand.
Dazzling Views with Excellent Optics
With a large 150mm (5.9”) aperture parabolic primary mirror, this telescope has enough light gathering ability to bring out detail in celestial objects. You can expect sharp, bright views of Jupiter’s four Galilean moons, its cloud bands and Great Red Spot, the rings of Saturn, the trapezium in the Orion Nebula, and the beautiful Pleiades Open Star Cluster. You'll be able to discern subtle details while viewing the Moon and planets, as well as faint galaxies and nebulae.
This telescope features a 1.25” rack-and-pinion focuser that accepts 1.25” eyepieces and dust covers for the front of the tube and the focuser.
Perfect for the City or Dark Sky Sites
Even if you live in a light-polluted city location, the Celestron StarSense Explorer 150mm Tabletop Dobsonian is advanced enough to easily pick out Jupiter, Saturn, open star clusters like the Pleiades, double stars like Acrux (the "tail" of the Southern Cross), the Orion Nebula, Omega Centauri, and more of the best and brightest celestial objects.
But if you can take the telescope to an even slightly darker location, more objects will become visible. With this 150mm Dobsonian and relatively dark skies, hundreds of fascinating objects are well within your reach.
The StarSense Explorer Tabletop Dobsonian is equipped with carry handles, making it easy to transport to your observing site.
Smartphone Compatibility
Celestron StarSense Explorer works with most modern smartphones, including iPhone 6 and up, and most devices running Android 7.1.2 or later manufactured since 2016. For a complete compatibility list, click here.
Patented StarSense Sky Recognition Technology
StarSense Explorer uses patented technology and your smartphone to determine exactly where the telescope is pointed in the night sky. A Lost in Space Algorithm (LISA), like the ones satellites use in orbit to correctly orient themselves, helps the app match star patterns it detects overhead to its internal database.
While other astronomy apps may claim that they can help you find objects, they rely exclusively on the phone's gyros and accelerometers, which aren't as accurate as LISA technology. No other app can accurately tell you when your target is visible in the eyepiece.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design: | Newtonian Reflector |
| Aperture: | 150mm |
| Focal Length: | 750mm |
| Focal Ratio: | f/5 |
| Focal Length of Eyepiece 1: | 25mm |
| Magnification of Eyepiece 1: | 26x |
| Focal Length of Eyepiece 2: | 10mm |
| Magnification of Eyepiece 2: | 65x |
| Highest Useful Magnification: | 307x |
| Lowest Useful Magnification: | 19x |
| Limiting Stellar Magnitude: | 13.1 |
| Light Gathering Power: | 345x as compared to the human eye |
| Optical Coatings: | Aluminum with SiO2 overcoat |
| Mirror Material: | Standard optical glass for primary and secondary mirrors |
| Minor Axis of Secondary Mirror: | 38mm |
| Tube Material: | Steel |
| Focuser: | 1.25" rack-and-pinion |
| Finderscope: | StarPointer™ red-dot finderscope |
| Resolution Rayleigh: | 1.06 arcseconds |
| Resolution Dawes: | 0.89 arcseconds |
| Optical Tube Dimensions: | 615.95mm long x 165.1mm diameter |
| Optical Tube Weight: | 3.72 kg |
| MOUNT INFO: | |
| Mount Type: | Altazimuth Tabletop Dobsonian base |
| Base Material: | Particle board with melamine surfaces and edge trim, CARB compliant |
| Base Dimensions: | 482.6mm x 482.6mm x 419.1mm |
| Base Weight: | 4.99 kg |
| Slew Speeds: | Manual |
| Software: | Celestron Starry Night Basic Edition Software and StarSense Explorer App |
| Total Telescope Kit Weight: | 8.71 kg |
| Included Items: |
|
| Solar Warning |
|
Celestron has reinvented the Tabletop Dobsonian telescope with StarSense Explorer—the first Tabletop Dobsonian that uses your smartphone to analyze the night sky and calculate its position in real-time. This 130mm aperture Celestron StarSense Explorer is ideal for beginners, thanks to the app's user-friendly interface and detailed tutorials. It's like having your own personal tour guide of the night sky.
Dock, Launch, Explore
Leave complicated star charts, imprecise planetarium apps, and computerized mounts behind. With StarSense Explorer, locating objects has never been easier, faster, or more accurate. Within minutes of setting up the telescope, you'll be navigating the sky with confidence. Simply place your phone in the unique StarSense dock and launch the StarSense Explorer app.
After aligning your phone to the telescope's optics (a quick and easy procedure), StarSense Explorer generates a list of celestial objects currently visible. Make your selection and arrows appear on-screen, guiding you as you move the telescope. When the object is ready to view in the eyepiece, the bullseye turns green. As you observe, listen to hundreds of audio descriptions and view detailed information about thousands of objects within the app’s robust database.
High-Quality Altazimuth Base
The stable Tabletop Dobsonian base provides a sturdy foundation for StarSense Explorer. The tabletop base is compact, lightweight, and easy to transport, making it perfect for travel. The base’s low-profile makes accessing the eyepiece easier for some observers (especially children). You can also place the base on a stable platform, like a table or hood of a car to raise it to a comfortable viewing height. Consider adding the optional tripod for even more viewing options.
Teflon bearings provide smooth motion in both altitude and azimuth. The integrated altitude "brake" system allows you to adjust the tension along the altitude axis to ensure the smoothest motion even with slight imbalances. As celestial objects appear to drift across the night sky, you'll be able to follow them easily.
The optical tube connects to the base via tube rings and a dovetail bar. It’s easy to adjust the tube’s position in the rings so the focuser is in the most ergonomic viewing position. The base features an eyepiece rack to keep your extra eyepiece(s) close at hand.
Dazzling Views with Excellent Optics
With a 130mm (5.1”) parabolic primary mirror, this telescope has enough light gathering ability to bring out detail in celestial objects. You can expect sharp, bright views of Jupiter’s four Galilean moons, its cloud bands and Great Red Spot, the rings of Saturn, the trapezium in the Orion Nebula, and the beautiful Pleiades Open Star Cluster. You'll be able to discern subtle details while viewing the Moon and planets, as well as faint galaxies and nebulae.
This telescope features a 1.25” rack-and-pinion focuser that accepts 1.25” eyepieces and dust covers for the front of the tube and the focuser.
Perfect for the City or Dark Sky Sites
Even if you live in a light-polluted city location, the Celestron StarSense Explorer 130mm Tabletop Dobsonian is advanced enough to easily pick out Jupiter, Saturn, open star clusters like the Pleiades, double stars like Acrux (the "tail" of the Southern Cross) the Orion Nebula, Omega Centauri, and more of the best and brightest celestial objects.
But if you can take the telescope to an even slightly darker location, more objects will become visible. With this 130mm Dobsonian and relatively dark skies, hundreds of fascinating objects are well within your reach.
The StarSense Explorer Tabletop Dobsonian is lightweight and equipped with carry handles, making it easy to transport to your observing site.
Smartphone Compatibility
Celestron StarSense Explorer works with most modern smartphones, including iPhone 6 and up, and most devices running Android 7.1.2 or later manufactured since 2016. For a complete compatibility list, click here.
Patented StarSense Sky Recognition Technology
StarSense Explorer uses patented technology and your smartphone to determine exactly where the telescope is pointed in the night sky. A Lost in Space Algorithm (LISA), like the ones satellites use in orbit to correctly orient themselves, helps the app match star patterns it detects overhead to its internal database.
While other astronomy apps may claim that they can help you find objects, they rely exclusively on the phone's gyros and accelerometers, which aren't as accurate as LISA technology. No other app can accurately tell you when your target is visible in the eyepiece.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design: | Newtonian Reflector |
| Aperture: | 130mm |
| Focal Length: | 650mm |
| Focal Ratio: | f/5 |
| Focal Length of Eyepiece 1: | 25mm |
| Magnification of Eyepiece 1: | 26x |
| Focal Length of Eyepiece 2: | 10mm |
| Magnification of Eyepiece 2: | 65x |
| Highest Useful Magnification: | 307x |
| Lowest Useful Magnification: | 19x |
| Limiting Stellar Magnitude: | 13.1 |
| Light Gathering Power: | 345x as compared to the human eye |
| Optical Coatings: | Aluminum with SiO2 overcoat |
| Mirror Material: | Standard optical glass for primary and secondary mirrors |
| Minor Axis of Secondary Mirror: | 38mm |
| Tube Material: | Steel |
| Focuser: | 1.25" rack-and-pinion |
| Finderscope: | StarPointer™ red-dot finderscope |
| Resolution Rayleigh: | 1.06 arcseconds |
| Resolution Dawes: | 0.89 arcseconds |
| Optical Tube Dimensions: | 615.95mm long x 165.1mm diameter |
| Optical Tube Weight: | 3.72 kg |
| MOUNT INFO: | |
| Mount Type: | Altazimuth Tabletop Dobsonian base |
| Base Material: | Particle board with melamine surfaces and edge trim, CARB compliant |
| Base Dimensions: | 482.6mm x 482.6mm x 419.1mm |
| Base Weight: | 4.99 kg |
| Slew Speeds: | Manual |
| Software: | Celestron Starry Night Basic Edition Software and StarSense Explorer App |
| Total Telescope Kit Weight: | 8.71 kg |
| Included Items: |
|
| Solar Warning |
|
Celestron has reinvented the Tabletop Dobsonian telescope with StarSense Explorer—the first Tabletop Dobsonian that uses your smartphone to analyze the night sky and calculate its position in real-time. This 114mm aperture Celestron StarSense Explorer is ideal for beginners, thanks to the app's user-friendly interface and detailed tutorials. It's like having your own personal tour guide of the night sky.
Dock, Launch, Explore
Leave complicated star charts, imprecise planetarium apps, and computerized mounts behind. With StarSense Explorer, locating objects has never been easier, faster, or more accurate. Within minutes of setting up the telescope, you'll be navigating the sky with confidence. Simply place your phone in the unique StarSense dock and launch the StarSense Explorer app.
After aligning your phone to the telescope's optics (a quick and easy procedure), StarSense Explorer generates a list of celestial objects currently visible. Make your selection and arrows appear on-screen, guiding you as you move the telescope. When the object is ready to view in the eyepiece, the bullseye turns green. As you observe, listen to hundreds of audio descriptions and view detailed information about thousands of objects within the app’s robust database.
High-Quality Altazimuth Base
The stable Tabletop Dobsonian base provides a sturdy foundation for StarSense Explorer. The tabletop base is compact, lightweight, and easy to transport, making it perfect for travel. The base’s low profile makes accessing the eyepiece easier for some observers (especially children). You can also place the base on a stable platform, like a table or hood of a car, to raise it to a comfortable viewing height. Consider adding the optional tripod for even more viewing options.
Teflon bearings provide smooth motion in both altitude and azimuth. The integrated altitude "brake" system allows you to adjust the tension along the altitude axis to ensure the smoothest motion, even with slight imbalances. As celestial objects appear to drift across the night sky, you'll be able to follow them easily.
The optical tube connects to the base via a tube cradle. It’s easy to adjust the tube’s position in the cradle so the focuser is in the most ergonomic viewing position. The base features an eyepiece rack to keep your extra eyepiece(s) close at hand.
Dazzling Views with Excellent Optics
With a 114mm (4.5”) parabolic primary mirror, this telescope has enough light-gathering ability to bring out detail in celestial objects. You can expect sharp, bright views of Jupiter’s four Galilean moons, its cloud bands and Great Red Spot, the rings of Saturn, the trapezium in the Orion Nebula, and the beautiful Pleiades Open Star Cluster. You'll be able to discern subtle details while viewing the Moon and planets, as well as galaxies and nebulae.
This telescope features a 1.25” rack-and-pinion focuser that accepts 1.25” eyepieces and dust covers for the front of the tube and the focuser.
Perfect for the City or Dark Sky Sites
Even if you live in a light-polluted city location, the Celestron StarSense Explorer 114mm Tabletop Dobsonian is advanced enough to easily pick out Jupiter, Saturn, open star clusters like the Pleiades, double stars like Alberio, the Orion Nebula, Andromeda Galaxy, and more of the best and brightest celestial objects.
But if you can take the telescope to an even slightly darker location, more objects will become visible. With this 114mm Dobsonian and relatively dark skies, hundreds of fascinating objects are well within your reach.
The StarSense Explorer Tabletop Dobsonian is lightweight and equipped with carry handles, making it easy to transport to your observing site.
Smartphone Compatibility
Celestron StarSense Explorer works with most modern smartphones, including iPhone 6 and up, and most devices running Android 7.1.2 or later manufactured since 2016. For a complete compatibility list, click here.
Patented StarSense Sky Recognition Technology
StarSense Explorer uses patented technology and your smartphone to determine exactly where the telescope is pointed in the night sky. A Lost in Space Algorithm (LISA), like the ones satellites use in orbit to correctly orient themselves, helps the app match star patterns it detects overhead to its internal database.
While other astronomy apps may claim that they can help you find objects, they rely exclusively on the phone's gyros and accelerometers, which aren't as accurate as LISA technology. No other app can accurately tell you when your target is visible in the eyepiece.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design: | Newtonian Reflector |
| Aperture: | 114mm (4.48") |
| Focal Length: | 450mm (17.71") |
| Focal Ratio: | f/4 |
| Focal Length of Eyepiece 1: | 17mm |
| Magnification of Eyepiece 1: | 26x |
| Focal Length of Eyepiece 2: | 10mm |
| Magnification of Eyepiece 2: | 45x |
| Highest Useful Magnification: | 269x |
| Lowest Useful Magnification: | 16x |
| Limiting Stellar Magnitude: | 12.8 |
| Light Gathering Power: | 265x as compared to the human eye |
| Optical Coatings: | Aluminum with SiO2 overcoat |
| Mirror Material: | Standard optical glass for primary and secondary mirrors |
| Minor Axis of Secondary Mirror: | 34.5mm |
| Tube Material: | Steel |
| Focuser: | 1.25" rack-and-pinion |
| Finderscope: | StarPointer™ red-dot finderscope |
| Resolution Rayleigh: | 1.21 arcseconds |
| Resolution Dawes: | 1.02 arcseconds |
| Optical Tube Dimensions: | 469.9mm long x 139.7mm diameter |
| Optical Tube Weight: | 41.9 kg |
| MOUNT INFO: | |
| Mount Type: | Altazimuth Tabletop Dobsonian base |
| Base Material: | Particle board with melamine surfaces and edge trim, CARB compliant |
| Base Dimensions: | 381mm x 381mm x 393.7mm |
| Base Weight: | 3.81 kg |
| Slew Speeds: | Manual |
| Software: | Celestron Starry Night Basic Edition Software and StarSense Explorer App |
| Total Telescope Kit Weight: | 5.71 kg |
| Included Items: |
|
| Solar Warning |
|
$599.00
The Sky-Watcher 114/450 Newtonian is a fully automatic telescope ideal for beginners and those who want to get straight to observing. Aligning the mount takes mere minutes with the “Bright Object” alignment mode, and the computerised SynScan system is the ultimate upgrade that allows automatic pointing and tracking of more than 42,000 object in the sky! This means less time spent finding a faint nebula or a distant planet and more time to enjoy observing. Astronomy has never been so easy!
The Sky-Watcher 114/450 has superb Parabolic optics and provides excellent all-around performance for both the observation of the moon, planets and deep sky objects. The AZ-Go2 Mount – Wi-Fi-controllable with iOS and Android devices and compatible with the SynScan hand controller, offers smooth tracking and fast alignment. Use Wi-Fi to control the telescope wirelessly with your mobile device, either a smartphone or tablet.
Download the SynScan App from Google play or the App Store.
AZ-Go2 Mount Features:
- Wi-Fi GOTO
- DC12V Voltage
- 1.3kg Mount Weight
- DC Motor
In the Box:
- 114/450mm Newtonian
- AZ-Go2 Mount
- Smartphone Adapter
- Super Possl 25mm and 10mm Eyepieces – 1.25″ Barrel
- Red Dot Finderscope
- Power Requirement: 12v DC Power Supply (Tip Positive) or AA Batteries (not supplied)
- Stainless Steel Tripod with Accessory Tray
Specifications:
| Optical Design | Paraboloidal Newtonian Reflector |
| Optical Diameter | 114mm |
| Focal Length | 500mm |
| F/Ratio | F/4.9 |
| Highest Practical Power | 80x |
| Finder Scope | Red Dot Finder* |
| Diagonal | 1.25″ 90 degree |
| Eyepieces | 1.25″ Super 25 and 10mm |
$749.00
Sky-Watcher 127mm/1500mm Skymax 127 Maksutov-Cassegrain OTA
- Compact dimensions, ideal for transportation
- Practical main mirror focusing mechanism
- Universal accessory adaptation
- High contrast image without distracting false colour
- Quick release system for the tube
- Impressive viewing capabilities for its price range
- 5 years Sky-Watcher limited warranty
| Model Number | SWMAK127-OTA |
| Optical Design | Maksutov-Cassegrain |
| Aperture | 127mm |
| Focal Length | 1500mm |
| Eyepieces | LET28mm |
| Focuser Diameter | 2″ |
| Finder Scope | 6 x 30mm |
| Highest Practical Power | 254x |
| Recommended Usage | Advanced |
| Weight | 5.6kg |
| Recommended Usage | High Resolution Astrophotography |
Celestron has reinvented the Dobsonian telescope with StarSense Explorer—the first Dobsonian that uses your smartphone to analyze the night sky and calculate its position in real-time. This large-aperture Celestron StarSense Explorer is ideal for serious beginners and advanced observers alike, thanks to the app's user-friendly interface and detailed tutorials. It's like having your own personal tour guide of the night sky. The large aperture will ensure that you won’t outgrow the telescope as you continue on in your astronomical adventures. Advanced observers will appreciate the ease of use and spectacular views the StarSense Explorer 12” Dobsonian provides.
Dock, Launch, Explore
Leave complicated star charts, imprecise planetarium apps, and computerized mounts behind. With StarSense Explorer, locating objects has never been easier, faster, or more accurate. Within minutes of setting up the telescope, you'll be navigating the sky with confidence. Simply place your phone in the unique StarSense dock and launch the StarSense Explorer app.
After aligning your phone to the telescope's optics (a quick and easy procedure), StarSense Explorer generates a list of celestial objects currently visible. Make your selection and arrows appear on-screen, guiding you as you move the telescope. When the object is ready to view in the eyepiece, the bullseye turns green. As you observe, listen to hundreds of audio descriptions and view detailed information about thousands of objects within the app’s robust database.
High-Quality Altazimuth Base
An ultra-stable Dobsonian base provides a sturdy foundation for StarSense Explorer. It features large diameter altitude bearings with variable tensioning, Teflon azimuth bearings, and braces on the side panels for extra stability (unlike many 12” Dobsonian bases). The altitude bearings provide a smooth up-and-down motion while the integrated altitude "brake" system allows you to adjust the tension along the altitude axis for smoothest motion even with slight imbalances. The panning knob on the telescope tube provides an ergonomic grip so you can precisely point the telescope without introducing heat from your hands into the optical system. As celestial objects appear to drift across the night sky, you'll be able to easily follow them with minor adjustments to the telescope’s position.
Dazzling Views with High-Quality Optics
With a large 12" Newtonian reflector optical tube, this telescope has enough light-gathering ability to bring out impressive detail in celestial objects. You can expect sharp, bright views of Jupiter's four Galilean moons, its cloud bands and Great Red Spot, the rings of Saturn, the gaseous glow of the Orion Nebula, dust lanes in the Lagoon Nebula, and our neighbor galaxy, Andromeda. Compared to the other StarSense Explorer Dobsonian telescopes, the 12” Dobsonian has 2.25 more light gathering ability than the 8” and 2.25x more light gathering ability than the 10”, providing better views of faint objects.
All mirror surfaces are coated with our XLT optical coatings to visibly increase contrast and light throughput for brighter views. With XLT, you'll be able to discern subtle details while viewing the Moon and planets, as well as faint galaxies and nebulae. The mirrors are made of low-expansion optical glass, which helps ensure the best images under changing environmental conditions.
This telescope also comes with a high-quality 2” Crayford focuser. The Crayford design provides precise and smooth movements without focus shifting. It also includes a 2” to 1.25” adapter and a 2” extension tube, so you can use virtually any 1.25” or 2” telescope eyepiece with your StarSense Explorer Dobsonian. The focuser also features a thumbscrew so you can lock in the sharpest focus.
Perfect for the City or Dark Sky Sites
Even if you live in a light-polluted city location, the Celestron StarSense Explorer 12” Dobsonian is advanced enough to easily pick out Jupiter, Saturn, open star clusters like the Pleiades, double stars like Acrux (the "tail" of the Southern Cross, the Orion Nebula, Omega Centauri, and more of the best and brightest celestial objects.
But if you can take the telescope to an even slightly darker location, more objects will become visible. With this 12" Dobsonian and relatively dark skies, hundreds of fascinating objects are well within your reach.
Transporting your StarSense Explorer Dobsonian is easy thanks to the ergonomic carry handles located at the balance point of the tube and base. Dust covers are also included for the front of the tube and the focuser.
Smartphone Compatibility
Celestron StarSense Explorer works with most modern smartphones, including iPhone 6 and up, and most devices running Android 7.1.2 or later manufactured since 2016. For a complete compatibility list, click here.
Patented StarSense Sky Recognition Technology
StarSense Explorer uses patented technology and your smartphone to determine exactly where the telescope is pointed in the night sky. A Lost in Space Algorithm (LISA), like the ones satellites use in orbit to correctly orient themselves, helps the app match star patterns it detects overhead to its internal database.
While other astronomy apps may claim that they can help you find objects, they rely exclusively on the phone's gyros and accelerometers, which aren't as accurate as LISA technology. No other app can accurately tell you when your target is visible in the eyepiece.
Enhance Your Setup
Keep your phone charged all night while exploring with your StarSense Explorer by adding the PowerTank Glow 5000 to your must-have accessories (sold separately). This 2-in-1 accessory was made with the StarSense Explorer Dobs in mind, it has a red flashlight PLUS a USB power bank for charging mobile devices in the field. Connect the PowerTank Glow 5000 to the two posts at the front of the StarSense Explorer dock with the included bands so it is held in a convenient location for charging your smartphone while in use.
To achieve the sharpest views faster, we recommend pairing the StarSense Explorer 12” Dobsonian with the USB Cooling Fan for Dobsonian Telescopes (sold separately). The fan cools the primary mirror to the ambient outdoor temperature faster, leaving you more time to observe. It mounts directly onto the rear cell of the Dobsonian and works with any USB power source.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design: | Newtonian Reflector |
| Aperture: | 305mm (12") |
| Focal Length: | 1500mm |
| Focal Ratio: | f/4.9 |
| Focal Length of Eyepiece 1: | 32mm |
| Magnification of Eyepiece 1: | 47x |
| Highest Useful Magnification: | 720x |
| Lowest Useful Magnification: | 43x |
| Limiting Stellar Magnitude: | 14.9 |
| Light Gathering Power: | 1895x as compared to the human eye |
| Optical Coatings: | XLT reflective coatings with silicon dioxide and tantalum pentoxide protective overcoatings for primary and secondary mirrors |
| Mirror Material: | Pyrex equivalent for primary and secondary mirrors |
| Primary Mirror Thickness: | 37mm (1.45") (approx. 1:8 thickness ratio) |
| Secondary Mirror Thickness: | 11mm |
| Minor Axis of Secondary Mirror: | 70mm |
| Tube Material: | Steel |
| Focuser: | 2" Crayford focuser, includes 2" extension tube and 2"-to-1.25" adapter |
| Finderscope: | StarPointer™ red-dot finderscope |
| Resolution Rayleigh: | 0.45 arcseconds |
| Resolution Dawes: | 0.38 arcseconds |
| Optical Tube Dimensions: | 1422.4mm long x 355.6mm |
| Optical Tube Weight: | 22.58 kg |
| MOUNT INFO: | |
| Mount Type: | Altazimuth Dobsonian base |
| Base Material: | Particle board with melamine surfaces and edge trim, CARB compliant |
| Base Dimensions: | 635mm x 635mm x 736.6mm |
| Base Weight: | 15.33 kg |
| Slew Speeds: | Manual |
| Software: | Celestron Starry Night Basic Edition Software and StarSense Explorer App |
| Total Telescope Kit Weight: | 37.92 kg |
| Included Items: |
|
| Solar Warning |
|
$2,349.00
180mm/2700mm Skymax 180 Maksutov-Cassegrain OTA – High Performance Optical Tube Assembly
The Sky-Watcher Skymax 180 Maksutov-Cassegrain OTA Telescope is perfect for the seasoned enthusiast moving up to a more powerful scope. The larger aperture enables more detailed views of our close planetary neighbours and sharper images of deep space objects.
Maksutov-Cassegrain Advantage
This telescope design has the inherent advantage of minimizing coma aberrations. It also presents a flatter and a more improved edge to edge clarity. Wide angle views of star fields and clusters have never looked so good!
Bring it to Your Favorite Viewing Spot
These Optical Tube Assemblies have a distinct advantage of being designed for use with different mounts. As long as the standard adaptors are present, you should be able to attach the OTA on it. The quick release mechanism enables you to assemble the tube quickly. It also allows you to make minor adjustments to the tube like a stroll in the park.
| Optical Design | Maksutov-Newtonian |
| Model Number | SWMAK180-OTA |
| Aperture | 180mm |
| Focal Length | 2700mm |
| Focuser Diameter | 1.25″ |
| Finder Scope | 9 x 50mm |
| Highest Practical Power | 360x |
| Recommended Usage | Advanced |
| Recommended Usage | High Resolution Astrophotography |
$1,499.00
150mm/1800mm Skymax 150 Maksutov-Cassegrain OTA
| Optical Design | Maksutov-Newtonian |
| Model Number | SWMAK150-OTA |
| Aperture | 150mm |
| Focal Length | 1800mm |
| Eyepieces | LET28mm |
| Focuser Diameter | 2″ |
| Finder Scope | 9 x 50mm |
| Highest Practical Power | 300x |
| Recommended Usage | Advanced |
| Recommended Usage | High Resolution Astrophotography |
The Hummingbird spotting scope shares many qualities with its namesake bird. In the wild, hummingbirds are known for their very small size, their agility (they can fly in most any direction at will), and their ability to travel long distances. The Celestron Hummingbird is the world’s first “micro” spotting scope well suited for hikers, birder watchers, and other wildlife watchers on the go.
Go “Micro”
Standard spotting scopes tend to be large and/or heavy, making them inconvenient to carry long distances in the field. The Hummingbird will shatter your expectations for how lightweight and compact a spotting scope can be, so you’ll take it places you never thought possible. You can easily hold this spotting scope in one hand, place it in a pocket, or pack it along in your carry-on luggage without compromising space.
Crisp, clear images
Although it is small, Hummingbird does not compromise on quality. All air-to-glass surfaces are fully multi-coated with high transmission optical coatings. The result is maximum light transmission for bright, sharp and contrast images. The prism is phase-coated BaK4, which increases contrast and resolution for sharper, more detailed images.
Durable, waterproof construction
The durable body of the Hummingbird works to keep the spotting scope protected against bumps and jolts both during transport and in the field. It’s also fully waterproof and nitrogen-purged, so you can use the scope worry-free in downpours, humid conditions, and other environmental challenges.
Ready for any adventure
The Hummingbird 9-27x56 spotting scope features a close focus of 10 feet, making it perfect for viewing birds, butterflies, plants, or other nearby subjects. The magnification of the 9-27x56mm spotting scope spans the standard magnification ranges of both a binocular and a spotting scope. No matter how you choose to observe, this versatile spotting scope is an excellent all-around performer.
Ways to observe
Unlike most spotting scopes, Hummingbird is so small that you can use it handheld at the lowest magnification level for a quick view of your subject. Travelers who want to save space can replace both their binocular and their spotting scope with this one optic. But the scope is also tripod adaptable, so you can secure it to a stable platform for comfortable long-duration or long-distance viewing.
Hummingbird provides plenty of eye relief for use with or without eyeglasses. For use while wearing eyeglasses, leave the twist-up eyecup in the lowered position. For use while not wearing eyeglasses, twist the twist-up eyecup into the extended position.
| GENERAL | |
|---|---|
| Magnification: | 9-27x |
| Objective Lens Diameter: | 56mm |
| Eyepieces: | 9-27x |
| Angular Field of View: | 4.2° - 1.9° |
| Linear Field of View @1000 m: | 73 - 32 m |
| Focal Length: | 200mm |
| Exit Pupil: | 6.2mm - 2mm |
| Eye Relief: | 15mm |
| Close Focus: | 3 m |
| Twilight Factor: | 22 - 39 |
| Relative Brightness: | 38 - 4 |
| Lens Coatings: | Fully Multi-Coated |
| Prism Glass (Type): | BaK4 |
| Prism Coatings: | Phase Coated |
| Weight: | 590 g |
| Environmental Protection: | Waterproof |
| Nitrogen Filled: | Yes |
| Tripod Adaptable: | Yes |
| Carrying Case: | Padded woven nylon |
| Camera Adaptable: | Yes |
| Dimensions: | 208mm x 127mm x 68mm (8.2" x 5.0" x 2.7") |
| Included Items: |
|
| Solar Warning |
|
This remarkable tripod from BENRO is perfect for when you need a quality, lightweight tripod that also offers superb stability.
The TCBC15FS20PRO Carbon Fibre tripod kit features the new FS20PROC Hybrid head that can be used as a 3-way ball head or as a 2-way video head. In addition the FS20PROC has a dual panorama function so it can be panned both at the base or at the quick release platform. The head is Arca-plate compatible, has a pan handle that can be mounted for right or left hand use, its angle can be adjusted with the incorporated hex key and then the handle base expansion function allows you to create multiple alternative support options.
| Minimum Height | 175mm |
| Maximum Height | 1525mm |
| Folded Height | 435mm |
| Independent Leg Spread | Yes |
| Support Angle | 22° / 55° / 80° |
| Weight | 1.02kg |
| Payload | 4.5kg |
| Head Type | 2-in-1 Multi-functional Head |
| Leg Lock Type | Flip |
| Leg Sections | 5 |
| Feet Type | Rubber |
From $22,860.00
Introducing the new Paramount MX Series 6 transportable observatory.
The Paramount MX Series 6 represents the latest in gear-driven GEM performance.
Its new features include a 25% instrument capacity increase, an option for absolute digital encoders, and multiple connectivity options.
The MX German equatorial mount has always been a popular Paramount model and the new Paramount MX Series 6 offers several important improvements.
On-axis Absolute Encoders vs. Motor-based Encoders.
Paramount's equipped with on-axis absolute encoders know where they are at all times. Paramount's with incremental encoders (or motor-based encoders) know only how far they have moved since they were initialized using a nightly process called homing.
The crucial additional difference is that the on-axis absolute encoders are fitted directly to the mount axes themselves, bypassing the worm drives. Paramount's with incremental encoders are fitted to the worms instead, which means that with incremental encoders alone, periodic errors in the worm drive show up in the tracking. These mounts must be calibrated and corrected using a process called periodic error correction (PEC), which measures and records the repeatable gear train errors and removes them. (TheSky features advanced, multi-harmonic PE detection and PEC calibration that minimizes periodic error in mounts with incremental encoders.)
For mounts with incremental encoders, homing re-zeros the encoders when precise sensors on each of the axes are reached. From then on, the incremental encoders are in effect delivering absolute readings.
However, the crucial additional difference remains, namely that the incremental encoder system is behind the worm drive, and periodic error correction is still required to get the best out of the RA tracking.
High-resolution on-axis absolute encoder technology is significantly more expensive than incremental encoders.
Are on-axis absolute encoders right for me ?
The short answer is, “it depends.”
Gear-driven Paramounts equipped with on-axis absolute encoders do not have periodic error, require no mechanical initialization (or homing), and the number of TPoint pointing samples needed for precision calibration is reduced.
These advantages expedite nightly setup, negate one-time periodic error training, and shorten the calibration process require to achieve spectacular pointing and tracking performance. However, the Paramount worm gear's uncorrected periodic error is low (below 7 arc seconds peak to peak), and, after a one-time PE training, periodic error correction (PEC) generally make it negligible. The Paramount without on-axis absolute encoders requires a nightly Find Home process that usually takes a minute or less to complete.
So, at least with Paramounts, periodic error is effectively in the noise, and homing straightforward.
What about pointing and tracking?
Without on-axis absolute encoders, Paramounts routinely produce 5-to-10-minute unguided exposures; many have reported 20 minutes. Also without on-axis absolute encoders, Paramount’s produce all-sky pointing accuracies at or below 30 arcseconds RMS (usually less than 15 arcseconds on fixed mirror telescopes).
Paramount’s exceptional software makes the above performance possible. TheSky Professional edition, in conjunction with TPoint™ and ProTrack™ the mount’s position is continually updated in both axes to correct system-wide pointing and tracking errors caused by tube flexure, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders and/or worm gears, and more.
On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior pointing and tracking.
So are on-axis absolute encoders right for you? Perhaps if you want to enjoy the conveniences mentioned above. And for many, that’s enough. With that said, the optional on-axis 26-bit Renishaw absolute encoders with 0.02 arc second precision are the finest available and they operate in temperatures between +80°C and –40°C.
Hardware Specifications
- 56 kg instrument capacity; 113 kg maximum payload capacity (instruments + counterweights)
- All sky pointing accuracies at or below 30 arcseconds RMS (see Software Specifications below for details)
- Unibody mount design weighs 24 kg without counterweights or counterweight shaft
- Maximum seven (7) arcseconds peak-to-peak periodic error before correction
- After a one-time training, periodic error is 1 arcsecond, peak-to-peak or less
- Optional 26-bit Renishaw encoders eliminate periodic error and the need for homing; operates in temps as low as –40° C
- If you skip encoders now and later decide you want them, they can be retrofitted on the Paramount MX Series 6
- As there’s some confusion about what encoders can and cannot do, there’s an FAQ below that elaborates on that and whether they’re right for you
- Its encoder cables are located inside the mount to help prevent snags.
- All electronics and through-the-mount cables are housed inside the mount with ample room for additional cables
- Its state-of-the-art MKS 6000 telescope control system (TCS) lets you connect via USB C, Ethernet, and Wi-Fi
- Two-port USB 2.0 hub located on the instrument panel
- Redesigned Versa-Plate™ (included) accepts most telescopes and makes mounting them a breeze
- 48V DC power supply and PC-to-mount USB and Ethernet cables included
- Two 9 kg counterweights are included which can balance 18-22 kg. You may need more for heavier payloads.
- Belt-driven gears with spring loaded worm gears produce virtually zero backlash
- Durable and fade-resistant red powder coating and black anodized finish; components are aluminum
- Clutch-free design helps maintain its TPoint™ assisted pointing accuracy
- AutoHome™ homing capability ensures the mount always knows its orientation (after performing an initializing process called “homing” that typically takes less than a minute)
- Calibrated azimuth and elevation polar alignment adjustments speed polar alignment
Software Specifications
- Paramount’s unequaled pointing and tracking wouldn’t be possible without its TPoint™ and ProTrack™ software.
- By employing TPoint’s calibration and telescope modeling tools, you’ll enjoy all sky pointing accuracies at or below 30 arcseconds RMS.
- Operating in conjunction with TPoint ™, ProTrack™ continuously updates the mount’s position across both axes to correct system-wide tracking errors including tube flexures, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders, and more.
- On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior tracking.
- Without encoders, Paramounts can deliver uncommonly long unguided exposures (one customer reported 20 minutes).
- For more information about what encoders can and cannot do, please see the FAQ below.
- All the included software is integrated into a single, easy-to-use, application consisting of TheSky™ Professional, TPoint™, Cameras+, Domes, Multi-OS+, and Weather modules.
- You can control all your astrophotography-related cameras and devices with this one app.
- It runs on macOS™, Windows™, Ubuntu™, and Linux (x86_64 and ARM64 architectures).
- Regardless of the operating system you run it on, it appears and operates identically. You can even switch between operating systems and its license allows up to six computers. Why paint yourself or your institution into a corner?
- Absent ProTrack™ which is unique to Paramounts, the included software is sold separately as TheSky™ Universal Bundle and represents a US$1,095 value.
SKU: SB-10613
Optional Black Anodised available on request
$45.00
This 3-D printed bracket from BINTEL connects a QHY PoleMaster electronic polar assistance tool to a ZWO AM5 to eliminate polar alignment hassles.
(Please note this is the bracket only. QHY PoleMaster and ZWO AM5 mount not included.)
Itmes included:
- Bintel QHY Polemaster Adapter
- AM5 adapter (2 pieces)
From $36,350.00
Introducing the new Paramount ME Series 6 observatory workhorse.
The Paramount ME Series 6 represents the latest in gear-driven GEM performance.
Its new features include a state-of-the-art MKS 6000 telescope control system that lets you connect via USB C, Ethernet, and Wi-Fi. Its two-port USB 2.0 hub is conveniently located on the instrument panel
The Paramount ME Series 6 remains an observatory favorite among professional and advanced-amateur astronomers.
On-axis Absolute Encoders vs. Motor-based Encoders.
Paramount's equipped with on-axis absolute encoders know where they are at all times. Paramount's with incremental encoders (or motor-based encoders) know only how far they have moved since they were initialized using a nightly process called homing.
The crucial additional difference is that the on-axis absolute encoders are fitted directly to the mount axes themselves, bypassing the worm drives. Paramount's with incremental encoders are fitted to the worms instead, which means that with incremental encoders alone, periodic errors in the worm drive show up in the tracking. These mounts must be calibrated and corrected using a process called periodic error correction (PEC), which measures and records the repeatable gear train errors and removes them. (TheSky features advanced, multi-harmonic PE detection and PEC calibration that minimizes periodic error in mounts with incremental encoders.)
For mounts with incremental encoders, homing re-zeros the encoders when precise sensors on each of the axes are reached. From then on, the incremental encoders are in effect delivering absolute readings.
However, the crucial additional difference remains, namely that the incremental encoder system is behind the worm drive, and periodic error correction is still required to get the best out of the RA tracking.
High-resolution on-axis absolute encoder technology is significantly more expensive than incremental encoders.
Are on-axis absolute encoders right for me ?
The short answer is, “it depends.”
Gear-driven Paramounts equipped with on-axis absolute encoders do not have periodic error, require no mechanical initialization (or homing), and the number of TPoint pointing samples needed for precision calibration is reduced.
These advantages expedite nightly setup, negate one-time periodic error training, and shorten the calibration process require to achieve spectacular pointing and tracking performance. However, the Paramount worm gear's uncorrected periodic error is low (below 7 arc seconds peak to peak), and, after a one-time PE training, periodic error correction (PEC) generally make it negligible. The Paramount without on-axis absolute encoders requires a nightly Find Home process that usually takes a minute or less to complete.
So, at least with Paramounts, periodic error is effectively in the noise, and homing straightforward.
What about pointing and tracking?
Without on-axis absolute encoders, Paramounts routinely produce 5-to-10-minute unguided exposures; many have reported 20 minutes. Also without on-axis absolute encoders, Paramount’s produce all-sky pointing accuracies at or below 30 arcseconds RMS (usually less than 15 arcseconds on fixed mirror telescopes).
Paramount’s exceptional software makes the above performance possible. TheSky Professional edition, in conjunction with TPoint™ and ProTrack™ the mount’s position is continually updated in both axes to correct system-wide pointing and tracking errors caused by tube flexure, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders and/or worm gears, and more.
On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior pointing and tracking.
So are on-axis absolute encoders right for you? Perhaps if you want to enjoy the conveniences mentioned above. And for many, that’s enough. With that said, the optional on-axis 26-bit Renishaw absolute encoders with 0.02 arc second precision are the finest available and they operate in temperatures between +80°C and –40°C.
Hardware Specifications
- 109 kg instrument capacity; 218 kg maximum payload capacity (instruments + counterweights)
- All sky pointing accuracies at or below 30 arcseconds RMS
- Unibody mount design weighs 38 kg without counterweights or counterweight shaft
- Maximum seven (7) arcseconds peak-to-peak periodic error before correction
- After a one-time training, periodic error is 1 arcsecond, peak-to-peak or less
- Optional 26-bit Renishaw encoders eliminate periodic error and the need for homing; operates in temps as low as –40° C
- If you skip encoders now and later decide you want them, they can be retrofitted on the Paramounts ME Series 6
- As there’s some confusion about what encoders can and cannot do, there’s an FAQ below that elaborates on that and whether they’re right for you
- Its encoder cables are located inside the mount to help prevent snags.
- All electronics and through-the-mount cables are housed inside the mount with ample room for additional cables
- Its state-of-the-art MKS 6000 telescope control system (TCS) lets you connect via USB C, Ethernet, and Wi-Fi
- Two-port USB 2.0 hub located on instrument panel
- Included Versa-Plate™ conveniently accepts most telescopes
- 48V DC power supply and PC-to-mount USB and Ethernet cables included
- Two 14 kg counterweights included. You may need more if your imaging system weighs more than 28 kg.
- Belt-driven gears with spring loaded worm gears produce virtually zero backlash
- Durable and fade-resistant red powder coating and black anodized finish; components are aluminum
- Clutch-free design helps maintain its TPoint™ assisted pointing accuracy
- AutoHome™ homing capability ensures the mount always knows its orientation (after performing an initializing process called “homing” that typically takes less than a minute)
- Calibrated azimuth and elevation polar alignment adjustments speed polar alignment
Software Specifications
- Paramount’s unequaled pointing and tracking wouldn’t be possible without its TPoint™ and ProTrack™ software.
- By employing TPoint’s calibration and telescope modeling tools, you’ll enjoy all sky pointing accuracies at or below 30 arcseconds RMS. Nothing outperforms that
- Operating in conjunction with TPoint ™, ProTrack™ continuously updates the mount’s position across both axes to correct system-wide tracking errors including tube flexures, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders, and more.
- On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior tracking.
- Without encoders, the Paramount ME Series 6 can deliver uncommonly long unguided exposures (one customer reported 20 minutes).
- For more information about what encoders can and cannot do, please see the FAQ below.
- All the included software is integrated into a single, easy-to-use, application consisting of TheSky™ Professional, TPoint™, Cameras+, Domes, Multi-OS+, and Weather modules.
- You can control all your astrophotography-related cameras and devices with this one app.
- It runs on macOS™, Windows™, Ubuntu™, and Linux (x86_64 and ARM64 architectures).
- Regardless of the operating system you run it on, it appears and operates identically. You can even switch between operating systems and its license allows up to six computers. Why paint yourself or your institution into a corner?
- Absent ProTrack™ which is unique to Paramount, the included software is sold separately as TheSky™ Universal Bundle and represents a US$1,095 value.
SKU: SB10616
Optional Black Anodised mounts available on request
From $16,370.00
The Paramount MYT Series 6 delivers exceptional performance made possible through its artful integration of precision mechanics, advanced control system electronics, and the uniquely capable Paramount Software Suite (included).
Skillfully carrying up to 32 kg of telescopes, cameras, and accessories, the Paramount MYT can help you create your next astrophoto masterpiece, at home, or on the go.
New features include:
- All new MKS 6000 offers built-in Ethernet, USB-C and Wi-Fi communication options and more.
- Optional Power On and Observe™ on-axis absolute encoder technology. No homing required and no periodic error.
- High-amperage XT60 connectors can supply continuous 12V DC power up to 60A.
- Improved Versa-Plate dovetail features drop-in telescope installation.
- Increased capacity: up to 32 kg of instrumentation, 64 kg with counterweights.
- Streamlined Instrument Panel provides pass through Ethernet connection and 3 XT60 power ports.
- Red components are powder coated aluminium for fade-resistant durability, black components anodized aluminium.
Introducing the new Paramount MYT Series 6 portable observatory.
Its new features include a 40% instrument capacity increase, an option for absolute digital encoders, and multiple connectivity options.
Being the lightest of all the Paramounts, the Paramount MYT Series 6 is the ultimate grab-and-go observatory.
On-axis Absolute Encoders vs. Motor-based Encoders.
Paramount's equipped with on-axis absolute encoders know where they are at all times. Paramount's with incremental encoders (or motor-based encoders) know only how far they have moved since they were initialized using a nightly process called homing.
The crucial additional difference is that the on-axis absolute encoders are fitted directly to the mount axes themselves, bypassing the worm drives. Paramount's with incremental encoders are fitted to the worms instead, which means that with incremental encoders alone, periodic errors in the worm drive show up in the tracking. These mounts must be calibrated and corrected using a process called periodic error correction (PEC), which measures and records the repeatable gear train errors and removes them. (TheSky features advanced, multi-harmonic PE detection and PEC calibration that minimizes periodic error in mounts with incremental encoders.)
For mounts with incremental encoders, homing re-zeros the encoders when precise sensors on each of the axes are reached. From then on, the incremental encoders are in effect delivering absolute readings.
However, the crucial additional difference remains, namely that the incremental encoder system is behind the worm drive, and periodic error correction is still required to get the best out of the RA tracking.
High-resolution on-axis absolute encoder technology is significantly more expensive than incremental encoders.
Are on-axis absolute encoders right for me ?
The short answer is, “it depends.”
Gear-driven Paramounts equipped with on-axis absolute encoders do not have periodic error, require no mechanical initialization (or homing), and the number of TPoint pointing samples needed for precision calibration is reduced.
These advantages expedite nightly setup, negate one-time periodic error training, and shorten the calibration process require to achieve spectacular pointing and tracking performance. However, the Paramount worm gear's uncorrected periodic error is low (below 7 arc seconds peak to peak), and, after a one-time PE training, periodic error correction (PEC) generally make it negligible. The Paramount without on-axis absolute encoders requires a nightly Find Home process that usually takes a minute or less to complete.
So, at least with Paramounts, periodic error is effectively in the noise, and homing straightforward.
What about pointing and tracking?
Without on-axis absolute encoders, Paramounts routinely produce 5-to-10-minute unguided exposures; many have reported 20 minutes. Also without on-axis absolute encoders, Paramount’s produce all-sky pointing accuracies at or below 30 arcseconds RMS (usually less than 15 arcseconds on fixed mirror telescopes).
Paramount’s exceptional software makes the above performance possible. TheSky Professional edition, in conjunction with TPoint™ and ProTrack™ the mount’s position is continually updated in both axes to correct system-wide pointing and tracking errors caused by tube flexure, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders and/or worm gears, and more.
On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior pointing and tracking.
So are on-axis absolute encoders right for you? Perhaps if you want to enjoy the conveniences mentioned above. And for many, that’s enough. With that said, the optional on-axis 26-bit Renishaw absolute encoders with 0.02 arc second precision are the finest available and they operate in temperatures between +80°C and –40°C.
Hardware Specifications
- 32 kg instrument capacity; 64 kg maximum payload capacity (instruments + counterweights)
- All sky pointing accuracies at or below 30 arcseconds RMS (see Software Specifications below for details)
- Unibody mount design weighs 16 kg without counterweights or counterweight shaft
- Maximum seven (7) arcseconds peak-to-peak periodic error before correction
- After a one-time training, periodic error is 1 arcsecond, peak-to-peak or less
- Optional 26-bit Renishaw encoders eliminate periodic error and the need for homing; operates in temps as low as –40° C
- If you skip encoders now and later decide you want them, they can be retrofitted on Series 6 Paramounts
- As there’s some confusion about what encoders can and cannot do, there’s an FAQ below that elaborates on that and whether they’re right for you
- Its encoder cables are located inside the mount to help prevent snags.
- All electronics and through-the-mount cables are housed inside the mount with ample room for additional cables
- Its state-of-the-art MKS 6000 telescope control system (TCS) lets you connect via USB C, Ethernet, and Wi-Fi
- Two-port USB 2.0 hub located on the instrument panel
- Redesigned Versa-Plate™ (included) accepts most telescopes and makes mounting them a breeze
- 48V DC power supply and PC-to-mount USB and Ethernet cables included
- 9 kg counterweight included and can balance 9 kg. You may need to purchase more for heavier payloads.
- Belt-driven gears with spring-loaded worm gears produce virtually zero backlash
- Durable and fade-resistant red powder coating and black anodized finish; components are aluminium
- Clutch-free design helps maintain its TPoint™ assisted pointing accuracy
- AutoHome™ homing capability ensures the mount always knows its orientation (after performing an initializing process called “homing” that typically takes less a minute or less)
- Calibrated azimuth and elevation polar alignment adjustments speed polar alignment
Software Specifications
- Paramount’s unequaled pointing and tracking wouldn’t be possible without its TPoint™ and ProTrack™ software.
- By employing TPoint’s calibration and telescope modeling tools, you’ll enjoy all-sky pointing accuracies at or below 30 arcseconds RMS. Nothing outperforms that.
- Operating in conjunction with TPoint ™, ProTrack™ continuously updates the mount’s position across both axes to correct system-wide tracking errors including tube flexures, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders, and more.
- On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior tracking.
- Without encoders, Paramounts can deliver uncommonly long unguided exposures (one customer reported 20 minutes).
- For more information about what encoders can and cannot do, please see the FAQ below.
- All the included software is integrated into a single, easy-to-use, application consisting of TheSky™ Professional, TPoint™, Cameras+, Domes, Multi-OS+, and Weather modules.
- You can control all your astrophotography-related cameras and devices with this one app.
- It runs on macOS™, Windows™, Ubuntu™, and Linux (x86_64 and ARM64 architectures.
- Regardless of the operating system you run it on, it appears and operates identically. You can even switch between operating systems and its license allows up to six computers. Why paint yourself or your institution into a corner?
- Absent ProTrack™ which is unique to Paramount, the included software is sold separately as TheSky™ Universal Bundle and represents a $1,095 value.
SKU: SB-10610
Optional Black Annodised mount available on request
$5,910.00
The Helium ME400 Red Tripod is ideal for portable Paramount use and is available for the Paramount MEII and ME6 models:
- Provides a stable platform for all your equipment
- Helium ME400 has a maximum payload capacity of 180 kg when the legs are fully extended, or up to 227 kg capacity when the legs are fully retracted
- Allows eyepiece placement at a convenient height with an adjustable height range Helium ME400 from 61cm to 100 cm.
- The ultra-portable and lightweight design weighs in at 14kg
Helium MX400 Features
- Simple and intelligent mechanics permit the legs to be expanded or collapsed in seconds and produce exceptional stability at all heights
- The top plate rotates 360 degrees for hassle-free polar alignment in azimuth.
- A wide range of coarse leveling adjustments can accommodate gently sloping surfaces.
- Fine-level adjustments help achieve the optimal level
- Swiveling feet can be fit with spikes or other third-party commercial tripod feet based on your observing site (grass, wood, concrete, gravel, etc.)
- Built-in bubble level helps quickly get the top plate horizontal.
- The 6061 aluminum tripod legs are red anodized with black anodized aluminum structural components (top plate, feet, etc.)
- Large tray between the legs conveniently stows your eyepieces and other equipment
- Legs accept many off-the-shelf tripod feet (including spikes, and wide rubber pads) to optimize coupling to the observing surface
The result of these innovative features is an exceptionally stable and readily portable imaging platform that can be quickly set up on any surface, leveled and aligned with the celestial pole, and easily taken down each night.
$1,299.00
Most SBIG filter wheels require a direct connection to an SBIG camera to be operated. Some specialized imaging configurations either require additional filter wheels, or a direct SBIG camera connection is not possible. In this case, the SBIG USB to Filter Wheel Adapter (USB-FW) can be used to control the wheel.
Note: The USB-FW does not include mechanical adapters. If the wheel is not directly coupled to an SBIG camera then custom mechanical adapters may be required.
Features
- USB Mini B interface, 15 foot (4.5 m) USB A to Mini B cable included
- DB-9 style I2C connector for filter wheel – connects to original filter wheel cable
- Universal AC power supply with 9 foot (2.7 m) extension cable and locking power connector included
- Uses ASCOM driver for control from most astronomical imaging software or via custom scripts
- Works with SBIG AFW series filter wheels, FW8S-STXL, FW8S-STT, FW8-8300, and FW7-STX.
- Supports dual wheel operation for the SBIG AFW series wheels
Note: Older SBIG wheels with a DB-9 style I2C connector may also be compatible, but have not been tested with the USB-FW adapter and correct operation is not guaranteed.
$2,599.00
Rediscover the world of birdwatching with the ZEISS Victory® SF. You can experience every spectacle nature has to offer with brilliant optics and an unparalleled wide-angle field of view. Thanks to its light weight, unique ergonomic design and dynamic fast-focus feature, the Victory SF allows for hours of relaxing birding without fatigue. The Victory SF is the new benchmark for birding and wildlife observation in the 125-year development of ZEISS binoculars.
With a field of view of 148m / 1000m, the 8x magnification offers the widest, most natural view and leaves nothing hidden. The seven-lens eyepiece delivers extremely sharp focus all the way to the edges. The moderate magnification, balanced weight distribution and ergonomic grip make these binoculars easy to hold for hours of relaxing viewing. A transmission rate of 92% and large exit pupil measuring over 5 mm reveal the details in dark shadows or the dim light of dusk.
92% Light Transmission
The Ultra-FL Concept is containing several SCHOTT fluoride glasses for absolute color fidelity, brightness, clarity and the finest resolution of details, even in the harshest conditions and most challenging environment.
Extremely wide field of view
With birds often hiding in dense cover, it’s essential that you have a wide field of view to allow you to spot any slight movements. The wide field of view of the ZEISS Victory SF binoculars increases the observable area of interest by up to 20% in comparison with other binoculars. Depending on the model, the field of view is between 120 m and 155 m, giving the user an impressive overview.
True-to-life image quality
Compromises cannot be made when it comes to bird identification – fine details have to be recognised within seconds for an accurate and reliable identification. The ZEISS Victory SF family was developed to master the most demanding situations encountered in birdwatching. The optical performance was maximised with a UFL Concept. This allows the user to master the most demanding of bird-watching scenarios, ensuring every precious moment is captured with absolute clarity.
SmartFocus Concept
The outstanding SmartFocus concept allows you to respond as quickly and intuitively thanks to the improved focusing speed. The focusing wheel is positioned in the triple-link bridge to allow for a comfortable, natural hand position. The anti-slip surface allows for easier, more precise operation and ideal focusing.
ZEISS T* Coating
ZEISS T* coating is a guarantee of the brilliant, high-contrast images which you will experience above all in adverse light conditions and in the twilight. Behind it, however, there is no specific formula for building up the layers. Instead, it is a technology that is constantly adjusted to suit new glass materials and requirements, which varies from lens to lens.
Performance
| Magnification | 10 × |
| Effective lens diameter | 30 mm |
| Light transmission | 90% |
| Exit pupil diameter | 3.0 mm |
| Twilight factor | 17.3 |
| Field of view at 1,000 m (yds) | 120 m (360 ft) |
| Subjective viewing angle | 65° Ww |
| Close focusing distance | 1.5 m (4.9 ft) |
| Diopter adjustment range | − 4.0 | + 4.0 dpt |
| Exit pupil distance | 18 mm |
| Pupil distance | 54 – 74 mm |
| Lens type | UHD |
| Prism system | Schmidt-Pechan |
Features
| LotuTec | Nitrogen filled | + | + |
| Water resistance | 400 mbar |
Physical
| Operating temperature | − 20°C | + 55°C (− 4°F | + 131°F) |
| Length | 120 mm (4.7 ") |
| Width at an interpupillary distance of 65 mm | 107 mm (4.6 ") |
| Weight | 460 g (16.2 oz) |
ErgoBalance Concept
Thanks to the ErgoBalance Concept, the binoculars are ideally balanced in the hands and enable prolonged and steady observation with minimum fatigue by reducing stresses on the muscles of the upper and lower arms.
A clear view, whatever the weather
There are always exciting things to be seen in the world of nature – even in wet weather. This is why ZEISS developed LotuTec®. A coating for the lenses of binoculars and spotting scopes that enables a clear and unhindered view in all weather conditions.
| Magnification | 8 × |
| Effective lens diameter | 30 mm |
| Light transmission | 92% |
| Exit pupil diameter | 3.75 mm |
| Twilight factor | 15.5 |
| Field of view at 1,000 m (yds) | 142 m (444 ft) |
| Subjective viewing angle | 63° Ww |
| Close focusing distance | 1.5 m (4.9 ft) |
| Diopter adjustment range | − 4.0 | + 4.0 dpt |
| Exit pupil distance | 18 mm |
| Pupil distance | 54 – 74 mm |
| Lens type | Ultra-FL |
| Prism system | Schmidt-Pechan |
Features
| LotuTec | Nitrogen filled | + | + |
| Water resistance | 400 mbar |
Physical
| Operating temperature | − 20°C | + 55°C (− 4°F | + 131°F) |
| Length | 120 mm (6.8 ") |
| Width at an interpupillary distance of 65 mm | 107 mm (4.9 ") |
| Weight | 460 g (27.8 oz) |
The Sky-Watcher HelioFind solar tracking mount is lightweight and ridiculously easy to use. No need to worry about aligning your equipment the night before or early in the morning. Using its patented HelioFind solar finder and built-in GPS, HelioFind automatically levels and calculates the azimuth and altitude of the Sun, all with the single push of a button. Once self-aligned, the mount locates and tracks the Sun for hours at a time. HelioFind is perfect for eclipse chasers, educators who teach science and astronomy during the day, or anyone fascinated with our nearest star.
Tired of wasting half the day not staring into space? Can’t wait until the Sun goes down to start your observing sessions? Need to fulfill those science curriculum standards for your classroom? Already planning your next total solar eclipse road trip? Nothing makes observing our home star as easy and engaging as HelioFind from Sky-Watcher!
You will need a small, dedicated Solar Telescope or small telescope with suitable Solar Filters attached.
Take the Sky-Watcher HelioFind outside on a sunny day, switch it on and it will automatically locate and point towards the Sun and then track it throughout the rest nest of the day. You don't need to align it or carry out any more adjustments
Ideal for observing sunspots, planetary transits, transits of the International or Chinese Space Stations, and solar eclipses with a white light solar filter. Or, attach an H-Alpha solar filter and observe the surface detail of the Sun directly along with tracking the daily changes in stormy prominences, filaments, plages, and even solar flares and coronal mass ejections.
Can be used with any standard photographic tripod (not included)
Perfect platform for Meade Corondo PST or Lunt 40mm, Lunt 50mm H-Alpha scopes.
Sky-Watcher HelioFind Mount is designed for solar observation only.
$5,910.00
The Helium MX400 Red Tripod is ideal for portable Paramount use and is available for the Paramount MX+ and MX6 models:
- Provides a stable platform for all your equipment
- Helium MX400 has a maximum payload capacity of 180 kg when the legs are fully extended, or up to 227 kg capacity when the legs are fully retracted
- Allows eyepiece placement at a convenient height with an adjustable height range Helium MX400 from 61cm to 100 cm.
- The ultra-portable and lightweight design weighs in at 14kg
Helium MX400 Features
- Simple and intelligent mechanics permit the legs to be expanded or collapsed in seconds and produce exceptional stability at all heights
- The top plate rotates 360 degrees for hassle-free polar alignment in azimuth.
- A wide range of coarse leveling adjustments can accommodate gently sloping surfaces.
- Fine-level adjustments help achieve the optimal level
- Swiveling feet can be fit with spikes or other third-party commercial tripod feet based on your observing site (grass, wood, concrete, gravel, etc.)
- Built-in bubble level helps quickly get the top plate horizontal.
- The 6061 aluminum tripod legs are red anodized with black anodized aluminum structural components (top plate, feet, etc.)
- Large tray between the legs conveniently stows your eyepieces and other equipment
- Legs accept many off-the-shelf tripod feet (including spikes, and wide rubber pads) to optimize coupling to the observing surface
The result of these innovative features is an exceptionally stable and readily portable imaging platform that can be quickly set up on any surface, leveled and aligned with the celestial pole, and easily taken down each night.
QHY5III200M is a new generation of QHY5III V2 series planetary guide camera, using domestic CMOS, with excellent quality, and near-infrared high sensitivity similar to 5III462C. QHY5III200 is also the first mono CMOS planetary camera with near-infrared enhancement characteristics QHY developed. In addition, the 4um large picture elements make it easier to use for guiding.
The QHY5III (Ver. 2) series planetary and guiding cameras are all equipped with a 512MB DDR3 image buffer which can effectively reduce the pressure on computer transmission, a great help for planetary photography which often requires writing a large amount of data in a short period of time. Some deep-sky astrophotography cameras on the market today only have 256MB, for example.
Tips: It is recommended to use the official standard Type-C data cable of QHYCCD. As the market is flooded with a large number of poor-quality Type-C cables, casual use may lead to the camera malfunctioning. If you use your own spare cable, please make sure it is a high-quality cable.
The custom interfaces of the previous generation of planetary cameras and guiders has been replaced in the QHY5III (Ver.2) cameras with a more universal ST-4 compatible guiding interface. Now, even if the guiding cable is lost or damaged, you will be able to easily get a replacement on the market at a low cost.
Specifications
| Model | QHY5III200M |
| CMOS Sensor | SC2210 |
| Pixel Size | 4um*4um |
| Effective Pixel Area | 1920*1080 |
| Effective Pixels | 2 Mega Pixel |
| Fullwell | 8000e |
| Readout Noise | 0.75e – 3e |
| AD Sample Depth | 12bit (output as 16bit and 8bit) |
| Built-in Image Buffer | 512MB DDR3 Memory |
| ROI Frame Rate | Full Resolution 96.5FPS @8BIT 60FPS @16BIT
960Lines 187FPS @8BIT 116FPS @16BIT 480Lines 209FPS @8BIT 130FPS @16BIT |
| Exposure Time Range | 15us-900sec |
| Shutter Type | Electric Rolling Shutter |
| Computer Interface | USB3.2 Gen1 Type-C |
| Guide Port | st4 |
| Telescope Interface | 1.25-inch, compatible with CS-port and C-port lenses by replacing the front-end connector (An IR AR glass and an IR850nm filter are included in the standard version.) |
| Back Focal Length | 17mm(with adapter); 8±0.5mm(without adapter) |
| Weight | 90g |
Camera Curves
$129.00
Sky-Watcher 9x50mm Finder Scope with Brackets
The Sky-Watcher 9×50 Finder Scope with Brackets is a vital accessory for accurate aiming. With its large 50mm aperture, wide 45° field of view and a simple cross-hair reticle, you are certain to gain almost perfect navigation sight with this excellent accessory for your astroviewing purposes. Besides, the finderscope also comes with a mounting bracket for easy setup and will fix to almost all standard finder shoes from Skywatcher.
- Achromatic 9x50mm Finderscope
- Large 50mm Aperture
- Wide 45° Field of View
- Cross-Hair Reticle
- Comes with a Mounting Bracket
This will fit all telescopes with a standard finderscope dovetail shoe. If you want to attach this to a Celestron SCT tube, you can use this BINTEL accessory:
$1,549.00
Specifications
- CCD type: ICX267AL Sony SuperHAD interline CCD with low dark current and vertical anti-blooming.
- CCD Full resolution pixel data: Pixel size: 4.65uM x 4.65uM, Image format: 1392 x 1040 pixels
- CCD Image area: 6.4mm (Horizontal) x 4.75mm (Vertical).
- CCD quality: Grade 1
- Spectral Response: QE max at 520nM (~50%), 30% at 420nM and 670nM.
- Readout Noise: Less than 10 electrons RMS – typically only 7 electrons.
- Full-well capacity: Greater than 15,000 e- (unbinned)
- Anti-blooming: Overload margin greater than 1000x.
- Dark current: Less than 0.1 electrons/second @ + 10C ambient.
- Data format: 16 bits.
- System gain: 0.3 electrons per ADU
- Lens details: 2.5mm f/1.2 150 degree ‘Fish Eye’
$980.00
A reducer has the optical property of decreasing the effective focal length of a telescope. This results in a wider-field and faster imaging time on nebulae and galaxies. Model NPR-2073 0.8x Reducer for NP Scopes is specifically designed to be used with the NP127is and NP101is. While it can also be used to enlarge the field of other Tele Vue Petzval type telescopes, it will not provide additional correction for those models.
This reducer was designed to minimize vignetting with camera sensors up to 43mm diagonal (Full Frame) and is a replacement for the previous 0.8x reducer, the NPR-1073, which worked best up to APS-C sensors. When combined with a Tele Vue Petzval type telescope, it reduces the focal length of the telescope by 20% and makes it that much faster. This increases the telescope's field of view by 25%.
For use on other Tele Vue Petzval model telescopes with 2-inch focusers, use the RAD-1074 Imaging System Nosepiece for 2" Focuser instead of the I.S. Imaging Adapter. Note that when used with 2" focusers there will be increased vignetting for full frame sensors because of the inner diameter of the 2-inch barrel.
This reducer requires the Imaging System insert to attach to the drawtube and Imaging System rings to attach to your accessories and camera.
SKU: NPR-2073
$1,999.00
Specifications
The guide camera images a star through an off-axis guider (OAG), either supplied with the AO Unit as an optional extra, or through an OAG built into a filter wheel such as the MIDI or MAXI filter wheels from SX. The software calculates the centroid of the guide star rapidly and accurately, and if the guide star moves, the optical window can be adjusted to compensate for the movement of the guide star. As the guide camera and imaging camera are looking through the same optical system, any corrections made for the guide star are automatically translated through to the main imaging camera.
The optical corrections are controlled by 4 stepper motors, so the small amount of movement, combined with the lightweight mass of the optical window, allows the corrections to be implemented very quickly and much more accurately than the mount drive system is capable of achieving.
Ideally suited to longer focal lengths optical systems, the benefits of the Active Optics on the final image can also be seen with shorter focal length systems on less accurate mounts.
-
- Image tracking and stabilisation using a high speed tip-tilt optical window.
- Fast tracking speed of 5mS per increment.
- Overcomes rapid gear errors to stabilise even difficult mounts.
- Mount control output for correcting large drive errors while maintaining AO stabilisation.
- Image shift factor independent of optical system or camera back-focus spacing.
- May be used to image stabilise many other makes and types of camera, given suitable control software.
- Clear aperture of 60mm for up to 35mm full-frame size chips.
- Short optical length – 74mm with OAG, 44mm without (add 6mm if front end adaptor is used).
- Very low light loss (~2%) from the multicoated optics.
- Filter threads for adding 48mm narrow band. IR blocking or pollution rejection filters without affecting the guide camera sensitivity.
- USB or Serial RS232 control via the computer.
- Low power consumption. Less than 600 mA at 12v DC when moving – 50mA quiescent current.
- Compact and lightweight – only 132mm in diameter x 44mm long – less than 700 grams load on the ‘scope.
The SXV-AO-USB should be used with the off-axis guider assembly for the best results with most optical systems.
This non-OAG (off-axis guider) version of the SXV-AO-USB is designed to work with either a filter wheel with a built in OAG such as the MIDI filter wheel or MAXI filter wheel or a main imaging camera that has a built in OAG.
Combine this with the incredibly sensitive Lodestar PRO or Ultrastar PRO auto guide cameras, finding a guide star and tracking through the Active Optics system works absolutely seamlessly.
PRODUCT MANUAL Handbook-for-the-Starlight-Xpress-SX-AO-USB
Examples
Some examples of the AO in use.
No processing was applied, other than cropping, so that the images are essentially ‘raw’. The mount used was a Celestron CI700 with a C11 SCT at F10
A 2x enlarged clip from an SXV-H9 image. Ten minutes with a C11 at F10 using mount guiding only.
Another clip taken a few minutes later with the AO switched on and operating at 3 updates per second.
Here are some ‘extreme’ images from an Ultima 2000 on a fork mount with poor polar alignment and rapid gear errors. The camera was an SXV-M8C and the images have been resampled to 50% of full size for display.
Without AO correction.
With the AO switched on. (The short coloured spikes on the bright stars were produced when the AO switched off for image download)
$2,399.00
Specifications
The guide camera images a star through an off-axis guider (OAG), either supplied with the AO Unit as an optional extra, or through an OAG built into a filter wheel such as the MIDI or MAXI filter wheels from SX. The software calculates the centroid of the guide star rapidly and accurately, and if the guide star moves, the optical window can be adjusted to compensate for the movement of the guide star. As the guide camera and imaging camera are looking through the same optical system, any corrections made for the guide star are automatically translated through to the main imaging camera.
The optical corrections are controlled by 4 stepper motors, so the small amount of movement, combined with the lightweight mass of the optical window, allows the corrections to be implemented very quickly and much more accurately than the mount drive system is capable of achieving.
Ideally suited to longer focal lengths optical systems, the benefits of the Active Optics on the final image can also be seen with shorter focal length systems on less accurate mounts.
- Image tracking and stabilisation using a high speed tip-tilt optical window.
- Fast tracking speed of 5mS per increment.
- Overcomes rapid gear errors to stabilise even difficult mounts.
- Mount control output for correcting large drive errors while maintaining AO stabilisation.
- Image shift factor independent of optical system or camera back-focus spacing.
- Off-axis guider assembly for use with a Lodestar Pro/Ultrastar Pro guide camera.
- May be used to image stabilise many other makes and types of camera, given suitable control software.
- Clear aperture of 60mm for up to 35mm full-frame size chips.
- Short optical length – 74mm with OAG, 44mm without (add 6mm if front end adaptor is used).
- Very low light loss (~2%) from the multicoated optics.
- Filter threads for adding 48mm narrow band. IR blocking or pollution rejection filters without affecting the guide camera sensitivity.
- USB or Serial RS232 control via the computer.
- Low power consumption. Less than 600 mA at 12v DC when moving – 50mA quiescent current.
- Compact and lightweight – only 132mm in diameter x 44mm long – less than 750 grams load on the ‘scope.
The SXV-AO-USB should be used with the off-axis guider assembly for the best results with most optical systems.
This combination uses ideally suited to using the LodestarPRO or Ultrastar PRO to view the edge of the telescope field via a 10mm square prism and provides accurate positional feedback to the control software. Unlike cameras with an integrated guider chip, the OAG puts the guide camera ahead of any filters that the user fits into the camera ring recess and so its sensitivity is always at maximum. The guide camera mounting is designed to be parfocal with a SX camera when used in this combination – fine focus adjustment is provided by moving the threaded guider mount along the prism tube. If you do not need the OAG barrel (e.g. when using a filter wheel such as the MIDI or MAXI filter wheel by SX which has a built in OAG or a camera with a built-in OAG or guide chip), you can fit the 72mm or T adaptor directly onto the rear of the AO assembly.
$1,999.00
Specifications
- CCD type: ICX825AL Sony ExView II interline CCD with ultra low dark current and vertical anti-blooming.
- CCD Full resolution pixel data: Pixel size: 6.45uM x 6.45uM, Image format: 1392 x 1040 pixels
- CCD Image area: 8.98mm (Horizontal) x 6.71mm (Vertical).
- CCD quality: Grade 1
- Spectral Response: QE max at 580nM (~75%), 50% at 400nM and 770nM.
- Readout Noise: Typically ONLY 3.5 electrons.
- Full-well capacity: Greater than 23,000 e- (unbinned)
- Anti-blooming: Overload margin greater than 1000x.
- Dark current: Less than 0.1 electrons/second @ + 10C ambient.
- Data format: 16 bits.
- System gain: 0.3 electrons per ADU
- Lens details: 1.55mm FL F/2 180 degree ‘Fish Eye’
- Computer Interface: Built-in USB 2.0 compatible interface.
- Image download time: Typically 0.6 seconds at full resolution using USB 2.0.
- Power requirements: Camera & Dew Heater requires 12v at 1.5 amp max.
- Input connection: ‘Mini B’ USB socket for USB2.0 and a 2.1mm jack for +12v heater supply. Cooling system: Ambient air cooling.
- Viewing dome: High quality polycarbonate hemisphere (replaceable)
- Overall size: 150mm tall x 95mm diameter
PRODUCT MANUAL Handbook-for-the-Oculus-PRO_Iss3
$899.00
The Lodestar utilises a very sensitive Sony ‘ExView’ CCD (the ICX829AK) with an array of 752 x 580 pixels in a ‘half-inch’ format. Although the chip is not cooled, it has a very low dark signal and very little readout noise, so it can be used to guide on faint stars that are beyond the reach of webcams and CMOS chip based guide cameras.
Specification
-
- CCD type: ICX829AK Sony Exview interline CCD with low dark current and vertical anti-blooming.
- CCD Full resolution Pixel data: Pixel size: 8.6uM x 8.3uM, Image format: 752 x 580 pixels
- CCD Image area: 6.4mm (Horizontal) x 4.75mm (Vertical).
- Colour filter grid array: YMCG secondary colour filters.
- CCD quality: Grade 1
- Spectral Response: QE max at 620nM (~65%), 35% at 400nM and 770nM.
- Readout Noise: Less than 15 electrons RMS – typically only 10 electrons.
- Full-well capacity: Greater than 50,000 e- (unbinned)
- Anti-blooming: Overload margin greater than 1000x.
- Dark current: Dark frame saturation time greater than 1 hour. Less than 0.1 electrons/second @ + 10C ambient.
- Data format: 16 bits.
- System gain: 0.9 electrons per ADU
- Computer Interface: Built-in USB 2.0 compatible interface.
- Image download time: Typically 0.2 seconds at full resolution using USB 2.0.
- Power requirements: USB powered.
- Cooling system: Ambient air cooling.
- Size: 32 x 72mm black anodised aluminium barrel with 25 x 0.75mm ‘C mount’ thread at the CCD window end & input/output plugs at rear.
- Weight: approx. 50g.
Here is a rear view of the guider:
$1,549.00
Specifications
- CCD: Sony ICX825AL ExView2 monochrome CCD
- Pixel count: 1392(H) x 1040(V)
- Pixel size: 6.45 x 6.45uM
- Optical size: 8.98 x 6.71 mm
- Read noise: Typically 5.0 electrons
- QE: Peak QE 75% (yellow light)
- Gain: 0.3 e/ADU
- Barrel size: 31.75mm dia. x 85mm long (1.25 inch eyepiece push fit size)
- Barrel thread: 25.4mm x 0.75mm ‘CS’ mount lens thread
- Input connection: ‘Mini B’ USB socket for USB2.0
- Output connection: Standard RJ12 autoguider socket
- Output type: Opto-isolated 4 lines (N,S,E & W) pull down with common return line
- Download rate: Approx. 2 frames per second in binned 1×1 mode
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