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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
Research Grade Mounts
8 products
8 products
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$31,049.00
PlaneWave L350 Direct Drive Mount
The L-Series combines versatility, simplicity and affordability by combining all the technology of our Observatory class telescopes into a compact stand-alone mount. In its Alt/Az configuration it is considerably more compact than its equatorial counterpart, allowing a larger telescope to fit in a smaller enclosure. Unlike German Equatorial mounts, there are no meridian flips to deal with, and no large protruding counterweights to create a dangerous hazard in a public observatory. Alt/Az is more intuitive to use and no polar alignment is needed. Besides, it is the way the pros do it!
L-Series Mounts Features:
- Direct-drive motors on each axis for smooth, fast, and virtually silent movement of the telescope
- Slew speeds up to 50 degrees per second
- High resolution encoders on each axis for precise positioning
- Zero backlash
- Zero periodic error
- PointXP mount modeling software
- Enclosed electronics
- Through the mount cabling
FEATURES:
| Direct drive motors and encoders | Direct Drive motors and on-axis encoders eliminate the need for gears, thereby eliminating backlash and periodic error. With high-resolution encoders providing the feedback for the direct drive motors, not only will the telescope track without periodic error and backlash, the mount will also counter wind gusts with precise servo feedback. | |
| Incredible Slew Speed | The direct drive motors can move the telescope at speeds up to 50 degrees per second for tracking satellites or just to minimize target acquisition time. | |
| Dual mounting bracket | PlaneWave style mounting bracket to hold CDK17/20 onto inside of fork arm with additional option of mounting a scope on the outside of the fork arm. Optional dovetail clamp required. | |
| Azimuth balance system | For precise center of gravity balance whether in Alt-Az or Equatorial configuration | |
| Through the mount cabling | Access panels in the fork arm and azimuth axis allow for camera equipment cabling through the inside of the mount. | |
| Proven CDK700/PW1000 Technology | The L-Series uses the same proven technology as the CDK700 and 1-Meter PW1000 which are being used in Universities round the world. |
MOUNT SYSTEM
| Type | Alt-Azimuth / Equatorial Direct Drive Mount |
| Weight | 110 lbs (50 kg) |
| Max. Load Capacity | 100 lbs (45 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
CONTROL SYSTEM
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 VAC. Supplied with 12VDC 15A Regulated Power Adapter |
MOTION CONTROL
| Motor Control | Industrial grade brushless motor control system and built in electronics |
| Motor - Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder - Azimuth and Altitude | 152mm disk built into the azimuth and altitude axes with stainless steel encoder on the circumference with reader yields 18,880,000 counts per revolution of the telescope. This translates to about 0.069 arcsecond resolution |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe All ASCOM compatible. |
SYSTEM PERFORMANCE
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcsecond |
| Tracking Accuracy | < .3 arcsecond error over 5 minute period |
| System Natural Frequency | 10 Hz or greater |
Price is ex Store
Check the PlaneWave website for Instructions and Schematics.
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
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
$72,599.00
The PlaneWave L600 Direct Drive Mount is ideal for the CDK24 and capable of holding up to 136kgs (300 lbs). Slewing at up to 50 degrees per second with pointing accuracy <10 arc seconds with Point XP and tracking accuracy of <.3 arc seconds over 5 minutes. This precision mount is a work of art.
The L-Series combines versatility, simplicity and affordability by combining all the technology of our Observatory class telescopes into a compact stand-alone mount. In its Alt/Az configuration it is considerably more compact than its equatorial counterpart, allowing a larger telescope to fit in a smaller enclosure. Unlike German Equatorial mounts, there are no meridian flips to deal with, and no large protruding counterweights to create a dangerous hazard in a public observatory. Alt/Az is more intuitive to use and no polar alignment is needed. Besides, it is the way the pros do it!
PlaneWave L600 Direct Drive Mount Features:
- Direct-drive motors on each axis for smooth, fast, and virtually silent movement of the telescope
- Slew speeds up to 50 degrees per second<
- High resolution encoders on each axis for precise positioning
- Zero backlash
- Zero periodic error
- Payload Capacity up to 136kg
- PointXP mount modeling software
- Enclosed electronics
- Weight is 153kg.
FEATURES:
MOUNT SYSTEM
| Type | Alt-Azimuth / Equatorial Direct Drive Mount |
| Weight | 338 lbs (153 kg) |
| Max. Load Capacity | 300 lbs (136 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
CONTROL SYSTEM
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 VAC. Supplied with 12VDC 15A Regulated Power Adapter |
MOTION CONTROL
| Motor Control | Industrial grade brushless motor control system and built in electronics |
| Motor - Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder - Azimuth and Altitude | 152mm disk built into the azimuth and altitude axes with stainless steel encoder on the circumference with reader yields 18,880,000 counts per revolution of the telescope. This translates to about 0.069 arcsecond resolution |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe All ASCOM compatible. |
SYSTEM PERFORMANCE
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcsecond |
| Tracking Accuracy | < .3 arcsecond error over 5 minute period |
| System Natural Frequency | 10 Hz or greater |
PlaneWave L600 Direct Drive Schematics
NOTE: This product has a lengthy leadtime for more information email: education@bintel.com.au
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
$124,480.00
The PlaneWave T-600 Direct Drive Gimbal is engineered to meet the rigorous demands of advanced astrophotography, complex astronomical research, SSA/SDA, and FSOC applications. Leveraging cutting-edge technology, this gimbal provides a robust, precise, versatile observational platform suitable for demanding environments.
Core Features of the T-600 Gimbal
High-Torque Direct-Drive Motors
The T-600 Gimbal has high-torque, double-stacked direct-drive motors, ensuring smooth, fast, and virtually silent operation. This feature is critical for tracking celestial objects with minimal vibration and supreme accuracy, accommodating substantial payloads effectively.
High-Resolution Absolute Encoders
With high-resolution absolute encoders on each axis, it offers incredibly precise pointing and tracking capabilities, crucial for capturing sharp, detailed celestial images and conducting rigorous scientific observations.
Zero Backlash and Periodic Error
The design of the T-600 Gimbal eliminates backlash and periodic error, facilitating consistent and reliable tracking that enhances astrophotography and supports precise applications in research and space surveillance.
Advanced Customization Options
The T-600 includes optional contact gasket seals for full weatherization and supports limitless Az rotation, making it adaptable for specific research observational requirements across various environments.
Rugged and Environment-ready
Designed with rugged environments in mind, the gimbal features electronics enclosed within the mount and weatherproof cable pass-throughs, ensuring durability and reliability in light-to-moderate rain and preventing debris entry.
Application-Specific Advantages
Astrophotography
With its robust load capacity and exceptional slew speeds, it allows astrophotographers to reposition heavy equipment quickly and smoothly, capturing breathtaking images of the cosmos with ease and efficiency.
Research
Researchers will find the gimbal’s precise tracking and advanced software ideal for detailed celestial observations and data collection, particularly in demanding environments where equipment adaptability and operational reliability are paramount.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
Professionals in SSA/SDA will benefit from the T-600 Gimbal’s high-precision tracking and configurable features, which are perfect for monitoring space debris and tracking satellites, ensuring accurate surveillance and data collection in space domain awareness initiatives.
System Performance
| Acceleration (Azimuth and Altitude) | Acceleration up to 100°/second² *Depending upon installed payload-induced moment of inertia |
| Velocity | Up to 100 degrees per second *Depending upon acceleration and distance traveled |
| Pointing Accuracy | <5-arcsecond RMS* with PointXP Model *Under stable environmental conditions |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Open Loop Tracking Accuracy | 0.2 arcseconds RMS over 300 second exposure at siderial rate |
| Open Loop Axis Following Error | <0.15 arcseconds RMS at sidereal rate, <0.3 arcseconds RMS at 1 degree per second* <2 arcseconds RMS at 10 degrees per second* *Dependent on Payload |
| Internal Servo-Loop (Drive to Motor) | 10 kHz cascaded velocity/position controller, PID + Filters |
| Software Command Round-Trip | 5 – 25 msec (depending on application) |
| System Natural Frequency | 20 Hz or greater (for gimbal only) |
Mount system
| Type | Alt-Azimuth / Equatorial Direct-Drive Mount |
| Weight | 605 lbs |
| Max. Load Capacity | 600 lbs (with payload limited to 100 kg-m² moment per port with center of gravity ≤ 15 inches from mounting surface and an lowest eigenmode frequency of 20 Hz. i.e. dual mounted CDK24 telescopes are compatible) |
| Dimensions | 34” x 20” x 23.5” (H/D/W) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Motor Torque (Azimuth and Altitude) | 127 ft-lbs (peak) |
| Azimuth Axis Range of Motion (Optional) | |
| Cable Management | Through-the-mount cabling |
| Coudé Path (Optional) | Limits elevation axis range of motion to 180º |
| Power Requirement | 100 to 240 VAC (50-60 Hz), 20 amp service at 120 VAC, 10 amp service at 240 VAC |
| Operating Temperature Range | -30 C to +50 C |
| Storage Temperature Range | -50 C to +70 C |
Mechanical structure
| Gimbal Assembly | Fully CNC machined construction (Surface finish treated with UV resistant coating on all exposed metal surfaces) |
| Default Weatherization | 2-Layer non-contact labrynth sealing at each motion-surface to prevent water (light-to-moderate rain) and debris entry. *Optional rubber seals may be added for further ruggedization. |
| Azimuth Bearing | 4-way loaded radial ball bearings |
| Altitude Bearing | 4-way loaded radial ball bearings |
| Instrument Mounting | Breadboard plate on both mounting surfaces (see interface document for complete mounting information) |
| Lifting Points | Present for lifting in “any orientation” |
Motion control
| Drive Electronics (Azimuth and Altitude) | Elmo Motion Control Systems industrial grade off-the-shelf brushless motor drives |
| Motors (Azimuth and Altitude) | Each axis includes a double stacked direct-drive 3 phase axial-flux torque motor |
| Encoders (Azimuth and Altitude) | 26-bit absolute encoder ring with readhead |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software by Dave Rowe. Includes ASCOM driver. |
| Advanced Timing Features (Optional) | Timestamped using GPS Reciever, or PTP/NPT Server <100-microseconds accuracy |
Included items
| Included Items | Hardware- Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment |
| One 16' USB cable - Too connect the mount to the observatory control computer | |
| One 120VAC power cable- to provide power to the mount | |
| Flashdrive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror | |
| 3/8 Socket - Used for operating the RA balance leadscrew on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
$62,999.00
State-of-the-Art Direct-Drive Motors
Equipped with PlaneWave's proprietary direct-drive motors on each axis, the L-550 ensures the telescopes' smooth, fast, and whisper-quiet movement. This capability is crucial for swiftly tracking celestial objects and satellites across the sky with minimal vibration and maximum accuracy.
High-Resolution Encoders
With high-resolution encoders on each axis, the L-550 delivers exact positioning, essential for capturing crisp, detailed night sky images. These encoders are vital for scientific applications demanding precise data collection.
Zero Backlash and Periodic Error
The L-550's design eliminates backlash and periodic error, facilitating steady tracking vital for top-notch astrophotography and dependable, long-term observational research.
Flexible Installation Options
The L-550 is available in both Alt/Az and equatorial configurations to meet a variety of observational needs. This versatility makes it suitable for fixed installations in educational observatories and adaptable setups for amateur astronomers.
Through-the-Mount Cabling
The innovative through-the-mount cabling system enhances setup cleanliness and safety, preventing cable snagging and reducing setup time.
Azimuth Dovetail Balance System
Provides precise center of gravity adjustments, enhancing the stability and performance of the system in both alt-azimuth and equatorial configurations, crucial for maintaining accurate tracking and reducing strain on the mount during extended observations.
Optional Dual Mounting Bracket
Allows for the attachment of additional telescopes or accessories on the mount, enhancing versatility and enabling simultaneous multi-instrument use, ideal for complex observational setups or educational demonstrations.
Rapid Target Acquisition
Equipped with direct-drive motors capable of slew speeds up to 50 degrees per second, enabling quick and efficient targeting of celestial objects and satellites, crucial for dynamic observations and time-sensitive astrophotography.
PointXP Mount Modeling Software
Included with the mount, PointXP software precisely models the mount's tracking behavior, enhancing its accuracy for critical applications. This software is invaluable for projects that require exact positioning and consistent tracking over extended periods.
Application-Specific Advantages
Astrophotography
The L-550's rapid slew speeds and silent operation allow astrophotographers to reposition swiftly and quietly between shots, capturing stunning celestial images without disrupting the observational setting.
Research
Researchers benefit from the L-550's robust construction and precise tracking to conduct detailed celestial observations and night-long monitoring with minimal interruption and consistent data quality.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its ability to swiftly and accurately reposition, the L-550 has ben been used for tracking satellites and space debris. However, our L-series mounts work best for astrophotography and research applications. To exceed the ideal performance requirements for SSA/SDA applications, we created the T-600 Direct-Drive Gimbal.
Mount Systems
| Type | Alt-Azimuth / Equatorial Direct Drive Mount |
| Weight | 153kg (338 lbs) |
| Max Load Capacity | 136kg (300 lbs) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
| Swing-Through Length (From Altitude Axis) | 650.748 mm (25.62") |
Control Systems
| Control Electronics | PlaneWave Interface dual axis telescope control |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Motion control
| Motor Control | Industrial grade brushless motor control system and built in electronics |
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible. |
System Performance
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Tracking Accuracy | 0.3 arcseconds over a 5-minute period at sidereal velocity |
| System Natural Frequency | 10 Hz or greater |
| Included Items | Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-550 mount |
| Hardware - Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment | |
| One 16' USB Cable - To connect the mount to the observatory control computer | |
| One 120VAC power cable- To provide power to the mount | |
| Standard Allen Key Set- For tightening bolts used on the mount | |
| Flash drive- Contains PWI4 software for mount control and instructions for installation | |
| 3/8 Socket - Used for operating the RA balance leadscrew on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing | |
| Standard Allen Key Set- For tightening bolts used on the mount |
$47,599.00
The PlaneWave L500 combines versatility, simplicity and affordability by combining all the technology of our Observatory class telescopes into a compact stand-alone mount. In its Alt/Az configuration it is considerably more compact than its equatorial counterpart, allowing a larger telescope to fit in a smaller enclosure. The mass it takes to make a rigid alt/az mount is substantially less, leading to cost savings. Unlike German Equatorial mounts, there are no meridian flips to deal with, and no large protruding counterweights to create a dangerous hazard in a public observatory. Alt/Az is more intuitive to use and no polar alignment is needed. Besides, it is the way the pros do it!
Planewave L500 Mount Features:
- Direct-drive motors on each axis for smooth, fast, and virtually silent movement of the telescope
- Slew speeds up to 50 degrees per second
- High resolution encoders on each axis for precise positioning
- Zero backlash
- Zero periodic error
- PointXP mount modeling software
- Enclosed electronics
- Through the mount cabling
FEATURES:
| Direct drive motors and encoders | Direct Drive motors and on-axis encoders eliminate the need for gears, thereby eliminating backlash and periodic error. With high-resolution encoders providing the feedback for the direct drive motors, not only will the telescope track without periodic error and backlash, the mount will also counter wind gusts with precise servo feedback. | |
| Incredible Slew Speed | The direct drive motors can move the telescope at speeds up to 50 degrees per second for tracking satellites or just to minimize target acquisition time. | |
| Dual mounting bracket | PlaneWave style mounting bracket to hold CDK17/20 onto inside of fork arm with additional option of mounting a scope on the outside of the fork arm. Optional dovetail clamp required. | |
| Azimuth dovetail balance system | For precise center of gravity balance whether in Alt-Az or Equatorial configuration | |
| Through the mount cabling | Access panels in the fork arm and azimuth axis allow for camera equipment cabling through the inside of the mount. |
MOUNT SYSTEM
| Type | Alt-Azimuth / Equatorial Direct Drive Mount |
| Weight | 257 lbs (100 kg) |
| Component Weights | Azimuth Base - 121 lbs, Fork Arm - 136 lbs |
| Max. Load Capacity | 200 lbs (91 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
CONTROL SYSTEM
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 VAC. Supplied with 12VDC 15A Regulated Power Adapter |
MOTION CONTROL
| Motor Control | Industrial grade brushless motor control system and built in electronics |
| Motor - Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder - Azimuth and Altitude | 152mm disk built into the azimuth and altitude axes with stainless steel encoder on the circumference with reader yields 18,880,000 counts per revolution of the telescope. This translates to about 0.069 arcsecond resolution |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe All ASCOM compatible. |
SYSTEM PERFORMANCE
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcsecond |
| Tracking Accuracy | < .3 arcsecond error over 5 minute period |
| System Natural Frequency | 10 Hz or greater |
Check the PlaneWave website for Instructions and Schematics.
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