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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
PlaneWave 支架
5 products
5 products
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$31,049.00
PlaneWave L350 直接驱动支架
L 系列将我们天文台级望远镜的所有技术整合到一个紧凑的独立支架中,集多功能性、简单性和经济性于一身。在 Alt/Az 配置中,它比赤道仪更加紧凑,可以将更大的望远镜装入更小的外壳中。与德国赤道仪不同,它无需处理子午线翻转问题,也无需在公共天文台中安装大型突出配重物,以免造成危险。Alt/Az 使用起来更直观,无需极轴校准。此外,这是专业人士使用的方式!
L系列支架特点:
- 每个轴上均采用直驱电机,使望远镜平稳、快速且几乎无声地移动
- 旋转速度高达每秒 50 度
- 每个轴上都有高分辨率编码器,可实现精确定位
- 零间隙
- 零周期误差
- PointXP 安装建模软件
- 封闭式电子设备
- 通过安装布线
特征:
| 直驱电机和编码器 | 直接驱动电机和轴上编码器无需齿轮,从而消除了间隙和周期性误差。高分辨率编码器为直接驱动电机提供反馈,不仅望远镜可以无周期性误差和间隙跟踪,而且支架还可以通过精确的伺服反馈抵消阵风。 | |
| 令人难以置信的回转速度 | 直接驱动电机可以使望远镜以每秒高达 50 度的速度移动,以跟踪卫星或只是最大限度地缩短目标获取时间。 | |
| 双安装支架 | PlaneWave 型安装支架可将 CDK17/20 固定在叉臂内侧,还可选择在叉臂外侧安装瞄准镜。需要选配燕尾夹。 | |
| 方位平衡系统 | 无论是在地轴还是赤道配置下,都能实现精确的重心平衡 | |
| 通过安装布线 | 叉臂和方位轴上的检修面板允许摄像设备电缆穿过支架内部。 | |
| 成熟的 CDK700/PW1000 技术 | L 系列采用与世界各地的大学正在使用的 CDK700 和 1 米 PW1000 相同的成熟技术。 |
安装系统
| 类型 | 高度方位角/赤道仪直接驱动支架 |
| 重量 | 110 磅(50 千克) |
| 最大负载能力 | 100磅(45千克) |
| 纬度范围 | 0 至 90 度,北半球和南半球 |
| 电缆管理 | 设备电缆可以通过安装座进行连接 |
控制系统
| 控制电子元件 | PlaneWave 接口双轴望远镜控制 |
| 用户界面 | PlaneWave Interface 4 (PWI4) 控制软件,集成 PointXP 安装建模软件 |
| 导航传感器 | 包含原位传感器,允许安装座在通电时找到其原位。 |
| 转换速率 | 每秒 20 度(标准);每秒 50 度(最大),双轴 |
| 电源要求 | 接受 120 VAC。配备 12VDC 15A 稳压电源适配器 |
运动控制
| 电机控制 | 工业级无刷电机控制系统和内置电子设备 |
| 电机 - 方位角和高度 | 直接驱动三相轴向磁通力矩电机 |
| 编码器 - 方位角和高度 | 152 毫米圆盘内置于方位角和高度轴中,圆周上装有不锈钢编码器,读取器每转一圈可产生 18,880,000 次计数。这相当于约 0.069 角秒的分辨率 |
| 电机扭矩 | 持续约 20 英尺磅;峰值 50 英尺磅 |
| 驱动电子 | 每个轴均采用工业级现成的无刷电机驱动器,并配有定制设计的接口卡 |
| 望远镜控制软件 | PlaneWave 接口 (PWI4)。集成 Dave Rowe 开发的 PointXP 安装建模软件,与所有 ASCOM 兼容。 |
系统性能
| 指向精度 | <10 角秒 RMS,采用 PointXP 模型 |
| 指向精度 | 2 角秒 |
| 追踪精度 | 5 分钟内误差小于 .3 角秒 |
| 系统固有频率 | 10 Hz 或更高 |
价格为出厂价
请查看PlaneWave网站上的说明和示意图。
$72,599.00
PlaneWave L600 直接驱动支架是 CDK24 的理想选择,可承受高达 136 公斤(300 磅)的重量。使用 Point XP 时,旋转速度高达每秒 50 度,指向精度小于 10 弧秒,跟踪精度在 5 分钟内小于 0.3 弧秒。这款精密支架堪称艺术品。
L 系列将我们天文台级望远镜的所有技术整合到一个紧凑的独立支架中,集多功能性、简单性和经济性于一身。在 Alt/Az 配置中,它比赤道仪更加紧凑,可以将更大的望远镜装入更小的外壳中。与德国赤道仪不同,它无需处理子午线翻转问题,也无需在公共天文台中安装大型突出配重物,以免造成危险。Alt/Az 使用起来更直观,无需极轴校准。此外,这是专业人士使用的方式!
PlaneWave L600 直接驱动安装座特点:
- 每个轴上均采用直驱电机,使望远镜平稳、快速且几乎无声地移动
- 旋转速度高达每秒 50 度<
- 每个轴上都有高分辨率编码器,可实现精确定位
- 零间隙
- 零周期误差
- 有效载荷能力高达 136 公斤
- PointXP 安装建模软件
- 封闭式电子设备
- 重量是153公斤。
特征:
安装系统
| 类型 | 高度方位角/赤道仪直接驱动支架 |
| 重量 | 338 磅(153 千克) |
| 最大负载能力 | 300 磅(136 千克) |
| 纬度范围 | 0 至 90 度,北半球和南半球 |
| 电缆管理 | 设备电缆可以通过安装座进行连接 |
控制系统
| 控制电子元件 | PlaneWave 接口双轴望远镜控制 |
| 用户界面 | PlaneWave 接口 4 (PWI4) 控制软件,集成 PointXP 安装建模软件 |
| 导航传感器 | 包含原位传感器,允许安装座在通电时找到其原位。 |
| 转换速率 | 每秒 20 度(标准);每秒 50 度(最大),双轴 |
| 电源要求 | 接受 120 VAC。配备 12VDC 15A 稳压电源适配器 |
运动控制
| 电机控制 | 工业级无刷电机控制系统和内置电子设备 |
| 电机 - 方位角和高度 | 直接驱动三相轴向磁通力矩电机 |
| 编码器 - 方位角和高度 | 152 毫米圆盘内置于方位角和高度轴中,圆周上装有不锈钢编码器,读取器每旋转一圈可产生 18,880,000 次计数。这相当于约 0.069 角秒的分辨率 |
| 电机扭矩 | 持续约 20 英尺磅;峰值 50 英尺磅 |
| 驱动电子 | 每个轴均采用工业级现成的无刷电机驱动器,并配有定制设计的接口卡 |
| 望远镜控制软件 | PlaneWave 接口 (PWI4)。集成 Dave Rowe 开发的 PointXP 安装建模软件,与所有 ASCOM 兼容。 |
系统性能
| 指向精度 | <10 角秒 RMS,采用 PointXP 模型 |
| 指向精度 | 2 角秒 |
| 追踪精度 | 5 分钟内误差小于 .3 角秒 |
| 系统固有频率 | 10 Hz 或更高 |
注意:本产品的交货期较长,如需更多信息,请发送电子邮件至: education@bintel.com.au
$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
PlaneWave L500 将我们天文台级望远镜的所有技术整合到一个紧凑的独立支架中,集多功能性、简单性和经济性于一身。在 Alt/Az 配置中,它比赤道仪更加紧凑,可以将更大的望远镜装入更小的外壳中。制造刚性 alt/az 支架所需的质量要小得多,从而节省了成本。与德国赤道仪支架不同,它无需处理子午线翻转问题,也无需在公共天文台中制造危险的突出配重。Alt/Az 使用起来更直观,无需极轴校准。此外,这是专业人士使用的方式!
Planewave L500 安装架特点:
- 每个轴上均采用直驱电机,使望远镜平稳、快速且几乎无声地移动
- 旋转速度高达每秒 50 度
- 每个轴上都有高分辨率编码器,可实现精确定位
- 零间隙
- 零周期误差
- PointXP 安装建模软件
- 封闭式电子设备
- 通过安装布线
特征:
| 直驱电机和编码器 | 直接驱动电机和轴上编码器无需齿轮,从而消除了间隙和周期性误差。高分辨率编码器为直接驱动电机提供反馈,不仅望远镜可以无周期性误差和间隙跟踪,而且支架还可以通过精确的伺服反馈抵消阵风。 |
|
| 令人难以置信的回转速度 | 直接驱动电机可以使望远镜以每秒高达 50 度的速度移动,以跟踪卫星或只是最大限度地缩短目标获取时间。 |
|
| 双安装支架 | PlaneWave 型安装支架可将 CDK17/20 固定在叉臂内侧,还可选择在叉臂外侧安装瞄准镜。需要选配燕尾夹。 |
|
| 方位燕尾平衡系统 | 无论是在地轴还是赤道配置下,都能实现精确的重心平衡 |
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| 通过安装布线 | 叉臂和方位轴上的检修面板允许摄像设备电缆穿过支架内部。 |
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安装系统
| 类型 | 高度方位角/赤道仪直接驱动支架 |
| 重量 | 257 磅(100 千克) |
| 组件重量 | 方位底座 - 121 磅,叉臂 - 136 磅 |
| 最大负载能力 | 200 磅(91 千克) |
| 纬度范围 | 0 至 90 度,北半球和南半球 |
| 电缆管理 | 设备电缆可以通过安装座进行连接 |
控制系统
| 控制电子元件 | PlaneWave 接口双轴望远镜控制 |
| 用户界面 | PlaneWave Interface 4 (PWI4) 控制软件,集成 PointXP 安装建模软件 |
| 导航传感器 | 包含原位传感器,允许安装座在通电时找到其原位。 |
| 转换速率 | 每秒 20 度(标准);每秒 50 度(最大),双轴 |
| 电源要求 | 接受 120 VAC。配备 12VDC 15A 稳压电源适配器 |
运动控制
| 电机控制 | 工业级无刷电机控制系统和内置电子设备 |
| 电机 - 方位角和高度 | 直接驱动三相轴向磁通力矩电机 |
| 编码器 - 方位角和高度 | 152 毫米圆盘内置于方位角和高度轴中,圆周上装有不锈钢编码器,读取器每转一圈可产生 18,880,000 次计数。这相当于约 0.069 角秒的分辨率 |
| 电机扭矩 | 持续约 20 英尺磅;峰值 50 英尺磅 |
| 驱动电子 | 每个轴均采用工业级现成的无刷电机驱动器,并配有定制设计的接口卡 |
| 望远镜控制软件 | PlaneWave 接口 (PWI4)。集成 Dave Rowe 开发的 PointXP 安装建模软件,与所有 ASCOM 兼容。 |
系统性能
| 指向精度 | <10 角秒 RMS,采用 PointXP 模型 |
| 指向精度 | 2 角秒 |
| 追踪精度 | 5 分钟内误差小于 .3 角秒 |
| 系统固有频率 | 10 Hz 或更高 |
请查看PlaneWave网站上的说明和示意图。
注意:本产品交货时间较长。如需更多信息,请发送电子邮件至education@bintel.com.au
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