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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 Vendor
68 products
68 products
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$900.00
The Keller EZ Saddle (600182) accepts Losmandy D-style dovetail rails such as the CDK12.5, CDK14, and DeltaRho 350. This saddle comes standard with the L-350 mount and can also be attached to the outside arm of any L-series mount for dual-mounted OTA configurations.
The PlaneWave Wide Saddle (200919) comes standard with L-500, L-550, and L-600 mounts for securing CDK17, CDK 20, CDK24, and DeltaRho 500 telescopes.
$68,999.00
PlaneWave 20 英寸 CDK(校正 Dall-Kirkham)光学设计是一种创新解决方案,以实惠的价格提供无与伦比的天文成像质量。CDK 望远镜设计使用大尺寸 CCD 相机提供出色的成像效果,同时仍保持出色的视觉使用效果。CDK 设计的离轴性能远远超过大多数商用望远镜设计,包括 Ritchey-Chrétien 设计。这种不折不扣的设计独特之处在于使光学对准变得容易,准直变得非常简单。这确保了用户从望远镜中获得最佳性能。CDK 设计的图像平面的最终结果是没有离轴彗差、没有离轴散光、完全平坦的视场(没有离轴散焦)。CDK 设计将为您提供从视场中心到角落的精确恒星。有关我们的光学设计的更多信息
PlaneWave Instruments CDK20 是一款 20 英寸(0.51 米)f/6.8 校正 Dall-Kirkham 天文望远镜。CDK20 采用双碳纤维桁架设计,配有 3 个冷却风扇,从望远镜后部排出空气。CDK20 覆盖 52 毫米视野,无任何场曲、离轴彗形像差或像散。该仪器重量为 140 磅(64 千克),标配背板固定环,可随时安装您选择的调焦器。
所有 CDK20 望远镜均配备 熔融石英主镜和次镜
特征:
| 碳纤维桁架设计 | 最大限度地减少因温度变化而导致焦点偏移的热膨胀 | |
| 燕尾伸缩接头 | 考虑到碳纤维和铝之间的热膨胀差异。伸缩接头允许铝制燕尾榫膨胀和收缩,而不会对碳纤维下桁架造成压力 | |
| 冷却风扇 | 三个冷却风扇从光学管中吹出,将空气拉过望远镜并穿过主镜。这有助于望远镜快速达到热平衡。如果购买可选的电子调焦附件 (EFA 套件),风扇由计算机控制。 | |
| Delta-T 就绪 | 为了增强防露效果,CDK20 内部连接有聚酰亚胺薄膜加热垫和温度传感器,可通过可选的Delta-T 控制器进行控制。 |
光学系统
| 光圈 | 20 英寸(508 毫米) |
| 焦距 | 3454 毫米(135.98 英寸) |
| 焦距比 | 光圈/6.8 |
| 中央阻塞 | 主镜直径的 39% |
| 调焦架上的后焦 | 5.8 英寸(147 毫米) |
| 重量 | 140 磅(63.5 千克) |
| OTA 长度 | 47 英寸(1,194 毫米) |
| 上笼 | 碳纤维桁架 |
| 下笼 | 碳纤维桁架与碳纤维灯罩 |
次镜
| 直径 | 7.5 英寸(191 毫米) |
| 材料 | 熔融石英 |
| 形状 | 球形 |
| 涂层 | 增强铝 - 96% |
主镜
| 光学直径 | 20 英寸(508 毫米) |
| 外径 | 20.5 英寸(521 毫米) |
| 形状 | 长椭圆体 |
| 材料 | 熔融石英 |
| 涂层 | 增强铝 - 96% |
镜头组
| 直径 | 90 毫米(3.54 英寸) |
| 镜头数量 | 2 |
| 涂层 | 宽带增透膜(400 至 700nm 范围内反射率低于 0.5%) |
船运
| 板条箱运输重量 | 291 磅(132.0 千克) |
| 板条箱宽度 | 33 英寸(838 毫米) |
| 板条箱高度 | 40 英寸(1,016 毫米) |
| 板条箱长度 | 65 英寸(1,651 毫米) |
包含的配件
| Ronchi 垫片(200354) | 该垫片位于调焦器的位置,用于设置主镜与副镜之间的间距。其内径为 1.25 英寸,可与 1.25 英寸目镜配合使用,以进行准直。 |
| 朗奇眼科 | 该目镜是一个 Ronchi 屏幕,用于设置主镜和副镜的间距。 |
| 主镜盖 | 主镜盖保护主镜。 |
| 印刷版说明书 | 用于准直和间距 |
注意:本产品交货期较长。如需更多详细信息,请发送电子邮件至: education@bintel.com.au
From $849.00
- Piggyback dovetails for mounting accessories atop an optical tube. These dovetails accept Losmandy D-style accessories.
- Piggyback Dovetail Assemblies come with mounting brackets and a Losmandy style dovetail for mounting accessories on your CDK14, 17, 20, 24, and 700.
Please Note- For CDK17 users:
- 170990 – is for the current CDK17 design with 10.24” of backfocus
$339.00
- This adapter presents M54 x 0.75 male threads on the camera side and presents SecureFit on the telescope side.
- Backfocus distance occupied by this adapter is 0.25″.
- Designed for use with ZWO and QHY cameras and filterwheels that accept M54.
- If using with other equipment please check the adapter PDF drawing in the download section below to confirm fitment for your specific application.
$2,149.00
- Add to the versatility of your L-350 mount with this external Right Ascension axis balance accessory.
- Balance of the mount is important for optimal direct drive motor performance and with this accessory users have the ability to fine tune the adjustments.
- The accessory includes one 2 lb and one 10 lb weights.
$6,999.00
- The Series-5 focuser is a large capacity focuser for use with Alt/Az, or equatorially mounted systems.
- The focuser is capable of lifting 40 lbs (18 kg) with a travel range of 0.6-inches (15,200 microns).
- The Series-5 focuser can be stacked with the Series-5 rotator for a complete focusing rotator solution (combined 2.78″ of occupied backfocus).
- Occupies only 1.675” of backfocus.
- 464.4283 encoder counts per micron
- Controlled via PWI4 software for autofocusing and optional field de-rotation (if using an Alt/Az mounted system).
- Requires the Series-5 Controller.
- Compatible with the DeltaRho 350 and RC700 telescopes.
$5,499.00
Add to the versatility of your L-350 direct drive mount with PlaneWave’s L-350 equatorial Wedge for precise polar alignment and tracking accuracy. Each wedge is made for your specific latitude and has an alignment range of ±3 degrees. Uses oversized fine thread adjustment screws and brass tightening nuts for a fine latitude adjustment.
$2,849.00
- Add to the versatility of your L-Series mount with this two-axis adjustable saddle to co-align two optical tubes.
- This saddle accepts Losmandy-D style dovetail plates and secures to the L-Series declination/altitude axis.
- Fits L-350, L-500, and L-600 mounts.
$1,999.00
We have designed a new 5-wire bus communication box that controls the Series-5 Focuser and Rotator, which includes M12 circular 5-wire threaded connector heads for environmental sealing.
- The Series -5 Controller has been designed for:
- Operating the Series-5 Focuser and Rotator
- Powering the fans for temperature control on DeltaRho Astrographs, as well as CDK12.5 to CDK24 telescopes
- Powering and controlling the telescope’s built-in anti-dew heating pads.
- Includes M12 circular 5-wire threaded connector heads for environmental sealing.
- Controlled via our PlaneWave Interface 4 software with ASCOM support.
$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。
From $480.00
When you need a secure way to attach a CCD camera at the image plane of a CDK telescope, the Secure Fit Spacers get you the optimal back focus spacing. These spacers attach via four screws to the PlaneWave Hedrick and IRF90 Focusers. When coupled with a PlaneWave SecureFit CCD Adapter, they practically eliminate slippage, movement, and equipment drops. The spacers come in eight different lengths: 2.1″, 3.8″, 4.5″, 5.2″, 5.9″, 6.75″, 7.5″, and 8.25″.
These spacers are made for the CDK14, 17, 20, and 24 and do not work with the CDK12.5. The CDK12.5 Secure Fit Spacers have a different bore size.
From $0.00
The PlaneWave Shroud and Mirror Cover Spacers are essential for seamlessly integrating PlaneWave fabric light shrouds with motorized primary mirror covers. These spacers ensure that the mirror covers can open and close safely without interference from the shroud, maintaining the full functionality of your telescope’s automated system.
Key Features:
- Seamless Compatibility: Designed specifically for use with PlaneWave fabric shrouds and motorized primary mirror covers.
- Reliable Operation: Allows the mirror covers to fully open and close without obstruction.
- Durable Construction: Precision-engineered for long-lasting performance in all observing conditions.
- The shroud spacers allow PlaneWave fabric shrouds to be installed in combination with PlaneWave motorized primary mirror covers.
- The spacers allow the primary mirror covers to safely open and close with the fabric shroud installed.
- Please note each order includes four spacers to install on each of the four shutter actuators.
From $0.00
Enhance your astrophotography and visual observations with the PlaneWave Fabric Light Shroud, designed specifically for PlaneWave telescopes. This high-quality light shroud effectively reduces stray light, improving contrast and ensuring clearer, sharper views of celestial objects.
Key Features:
- Superior Light Blocking: Minimizes unwanted glare and reflections for enhanced image quality.
- Durable, Breathable Fabric: Made from high-quality, stretchable material that resists sagging while allowing proper airflow to prevent dew buildup.
- Custom Fit: Designed to seamlessly wrap around your PlaneWave telescope for a secure and snug fit.
- Easy Installation & Removal: Lightweight and flexible, making it simple to attach and remove as needed.
Perfect for both amateur and professional astronomers, the PlaneWave Fabric Light Shroud is an essential accessory for maximizing the performance of your telescope under any sky conditions.
Available for the CDK14, CDK17, CDK20, CDK24, and CDK700.
$61,199.00
The CDK350 Observatory System from PlaneWave Instruments is a premium setup designed for the astrophotography aficionado and the dedicated astronomy researcher. This system marries the high-performing CDK14 optical tube assembly with the robust L-350 direct-drive mount, creating an unmatched observational platform that excels across a spectrum of applications, from deep celestial studies to sophisticated astrophotography
Key Features of the CDK350 Observatory System
CDK14 Optical Tube Assembly
- Aperture and Focal Length: Boasts a 14-inch aperture and a 2563 mm focal length at an f/7.2 focal ratio, ideal for capturing wide-field views of the cosmos with incredible depth and clarity.
- Advanced Optical Design: Features a Corrected Dall-Kirkham optical design, providing a field free of off-axis coma and astigmatism while achieving a perfectly flat field across a 70 mm image circle, ensuring critically sharp images throughout the entire field.
- High-Quality Construction: Constructed from lightweight yet durable carbon fiber, minimizing thermal expansion and allowing for rapid thermal equilibration, which helps maintain optical precision in fluctuating temperatures.
- Superior Mirrors and Coatings: Fitted with rock-solid fused silica mirrors known for their minimal thermal expansion, paired with premium coatings that enhance light throughput while minimizing stray light for optimal image quality.
- Thermal Management: Integrates an advanced cooling system with multiple fans that promote rapid thermal stabilization, essential for maintaining consistent high-quality imaging during lengthy exposures and minimizing focus shifts caused by temperature variations.
L-350 Direct Drive Mount
- Direct Drive Motors: Features sophisticated direct-drive motors on each axis, ensuring smooth, swift, and near-silent movement of the telescope with zero backlash and zero periodic error, perfect for both tracking celestial objects and quick repositioning.
- High-Resolution Encoders: Comes equipped with high-resolution optical encoders on both axes, delivering precise positioning and movement, which is critical for high-quality astrophotography and detailed celestial research.
- Azimuth Dovetail Balance System: Includes a finely adjustable balance system that enhances the stability and performance of the setup in both alt-azimuth and equatorial configurations, critical for sustained accurate tracking and easing the strain on the mount during prolonged observations.
- Rapid Target Acquisition: Boasts direct-drive motors capable of impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial objects and satellites, vital for dynamic observations and responsive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK350 is a powerhouse for astrophotographers, offering exceptional tracking accuracy and image stability which facilitate capturing breathtaking celestial images with intricate details and vibrant colors.
Astronomy Research
Researchers will find the CDK350 invaluable for its consistent performance and precise data collection capabilities. It serves as a reliable platform for photometry, spectroscopy, and minor planet tracking, providing a robust foundation for scientific exploration and discovery.
Visual Observations
For enthusiasts of visual astronomy, the CDK350 delivers vibrant and detailed views of the universe. Its substantial aperture and high-quality optical components ensure superb viewing of planetary, lunar, and deep-sky objects, enhancing every observational session.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-350 mount in the CDK350 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount System
| Mount Weight | 50kg (110 lbs) |
| Max. Load Capacity | 45 kg (100 lbs) |
| 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 to 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 |
Optical Systems
| Aperture | 356mm (14") |
| Focal Length | 2563 mm (101") |
| Focal Ratio | f/7.2 |
| Central Obstruction | 23.5% by surface area; 48.5% of the Primary Mirror Diameter |
| Back Focus | 282 mm (11.09") |
| Weight | 22 kg (48 lbs) |
| Optimal Field of View | 52 mm Image Circle |
Mechanical Structure
| Fork Assembly | L-350 Mount |
| Fork Base | Welded stainless steel torsion box |
| Optical Tube | Carbon fiber truss and light shroud |
| Instrument Payload | 45 kg (100 lbs) |
Motion control
| 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 | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe. Provides HTTP and ASCOM control interfaces. MaxIm DL is required for camera control when building a pointing model within our PWI4 software. |
Included items
| Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube |
| Flash drive -Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror |
| Hardware - Six 3/8-16 x 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 3/8-16 x 1/4″ 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 |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
| Keller EZ-Saddle (600182) - The Keller EZ saddle comes standard with the L-350 mount |
$53,499.00
The CDK300 Observatory System from PlaneWave Instruments, an elite configuration designed specifically for the astrophotography enthusiast and serious astronomy researcher. This system combines the precision-engineered CDK12.5 optical tube assembly with the robust L-350 direct-drive mount, offering an unparalleled observational experience that excels in a wide array of applications from detailed celestial studies to advanced astrophotography.
Key Features of the CDK300 Observatory System
CDK12.5 Optical Tube Assembly
- Aperture and Focal Length: Features a 12.5-inch aperture and a 2541 mm focal length at an f/8 focal ratio, perfect for capturing deep-sky objects with exceptional depth of field and clarity.
- Advanced Optical Design: Utilizes a Corrected Dall-Kirkham optical design, eliminating off-axis coma and astigmatism while achieving a perfectly flat field across a 52 mm image circle, ensuring sharp and detailed images across the entire field.
- High-Quality Construction: The optical tube is constructed from lightweight and sturdy carbon fiber, reducing thermal expansion and allowing rapid cooling, which maintains optical alignment in varying temperatures.
- Superior Mirrors and Coatings: Equipped with rock-solid fused silica mirrors known for their low thermal expansion, along with high-quality coatings that maximize light transmission and minimize stray light.
- Thermal Management: Incorporates a sophisticated cooling system featuring three rear cooling fans and four boundary layer fans. This setup rapidly achieves thermal equilibrium, essential for maintaining consistent imaging quality during long exposure astrophotography and reducing thermal-induced focus shifts.
L-350 Direct Drive Mount
- Direct Drive Motors: Employs state-of-the-art direct-drive motors on each axis, providing smooth, fast, and ultra-quiet movement of the telescope with zero backlash and zero periodic error.
- High-Resolution Encoders: Integrated high-resolution encoders offer precise positioning, essential for capturing high-quality astrophotography and conducting detailed astronomical research.
- 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.
- 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.
- 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.
Application-Specific Advantages
Astrophotography
The CDK300 system is a powerhouse for astrophotographers, providing exceptional tracking accuracy and image stability which allow for capturing breathtaking celestial images with intricate details and vibrant colors.
Astronomy Research
Researchers will find the CDK300 invaluable for its consistent performance and precise data collection capabilities. Ideal for photometry, spectroscopy, and minor planet tracking, it serves as a reliable platform for scientific exploration and discovery.
Visual Observations
For those who enjoy visual astronomy, the CDK300 offers vibrant and detailed views of the cosmos. Its large aperture and high-quality optical components make it perfect for viewing planetary, lunar, and deep-sky objects, enriching every observational session.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-350 mount in the CDK300 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount System
| Mount Weight | 50kg (110 lbs) |
| Max. Load Capacity | 45 kg (100 lbs) |
| 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 to 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 |
Optical Systems
| Aperture | 318 mm (12.5 inch) |
| Focal Length | 100.04 inch (2541 mm) |
| Focal Ratio | f/8 |
| Central Obstruction | 42% of the primary mirror diameter |
| Backfocus from Mounting Surface | 265 mm (10.445 inch) |
| Backfocus from Racked in Focuser | 183 mm (7.2 inch) |
| Weight | 19 kg (42 lbs) |
| Optimal Field of View | 52 mm image circle |
Mechanical Structure
| Fork Assembly | L-350 Mount |
| Fork Base | Welded stainless steel torsion box |
| Optical Tube | Carbon fiber |
| Instrument Payload | 45 kg (101 lbs) |
Motion Control
| 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 | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe. Provides HTTP and ASCOM control interfaces. MaxIm DL is required for camera control when building a pointing model within our PWI4 software. |
Included Items
| Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube |
| Flash drive - Contains PWI4 software for mount control, instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror |
| Hardware - Six 3/8-16 x 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 3/8-16 x 1/4″ 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 |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
| Keller EZ-Saddle (600182) - The Keller EZ saddle comes standard with the L-350 mount |
| One 16′ USB cable - To connect the mount to the observatory control computer |
$117,999.00
成功推出 DeltaRho 350 后,DeltaRho 500 现已推出,可克服超广角成像的挑战。主镜固定到位,只需简单调整副镜的倾斜度和倾斜度,即可快速实现准直。由于 PlaneWave 追求完美的望远镜,其聚光能力是 DeltaRho 350 的两倍多,最大限度地提高天文照相仪的性能从未如此简单!
- 修正卡塞格林焦点光学设计
- 孔径 – 508 毫米 (20″)
- 焦距 – 1537 毫米
- 焦距比 – f /3.03
- 70mm 像圈 > 2.6 度
- 固定主镜
- 通过副镜上的 3 个倾斜螺钉进行准直
- 距安装表面 9.166 英寸(232.8 毫米)(不含调焦器和旋转器)。
- 安装 Series-5XL 调焦器和 Series-5 旋转器后,后焦距为 5.81 英寸 (147.6 毫米)(调焦器位于行程范围的中间点)。
- 内置主、辅除露加热器,配有温度传感器
- 与 L-500 或 600 系列直接驱动支架兼容。
PlaneWave 团队热衷于设计卓越的望远镜,以便世界各地的用户能够捕捉到最令人惊叹的天文图像。从设计到制造,DeltaRho 500 的目标都是围绕创造革命性的广角望远镜。DeltaRho 500 采用卡塞格林光学设计,成像列车位于望远镜后部,以防止仪器受阻。与主焦点设计相比,这具有真正的优势,主焦点设计会严重限制用户使用滤光轮或大型相机的能力。DeltaRho 500 以 f/3 和 1537 毫米焦距运行,见证望远镜技术的惊人突破,这必将彻底改变您的天文摄影。
最后,但并非最不重要的一点是,DeltaRho 500 提供了平坦的视野,可确保从角落到角落的图像都具有令人惊叹的清晰度,而不会降低场曲率。DeltaRho 500 提供单镜准直的简便性、先进 3D 打印挡板的杂散光控制以及通过有限元分析 (FEA) 创建的结构性能。使用大型 16803/4040 (52mm) 尺寸的相机传感器时,DeltaRho 500 用户可以从边缘到边缘体验精确的星星和 2 度视野。这个视野是我们 CDK 20 的两倍多!这种设备让用户体验到全新水平的广角成像,可以让他们比以往任何时候都更接近深空。DeltaRho 500 让用户和令人惊叹的天文图像之间没有任何障碍。
碳纤维管设计
最大限度地减少热膨胀,避免成像过程中温度变化导致焦点偏移。碳纤维还能快速达到环境温度,而且重量极轻且坚硬,有助于确保生成出色的成像数据。
准直软件
与附带的准直掩模一起,PlaneWave 准直软件可以快速轻松地进行准直,从而最大程度地提高快速 f 比光学系统的性能。
3D 打印挡板
PlaneWave 的数字 3D 打印技术在我们的挡板系统中添加了连续的材料层,从而实现了轻量、精确定位的内部杂散光控制,从而最大限度地减少渐晕并最大限度地提高图像对比度。
冷却风扇
三个风扇巧妙地安装在光学管的背板上,以便通过望远镜和主镜通风。光学管侧面的四个附加风扇为主镜提供气流,有效地实现热平衡,以防止因温度变化而导致图像失真。
风扇通过 PWI 4 软件进行控制,PlaneWave 5 系列控制器单独出售。
防露控制
为了增强防露效果,DR500 内部连接有聚酰亚胺薄膜加热垫和温度传感器,可通过 PWI 4 软件使用 5 系列控制器进行控制。
光学系统
| 光学设计 | 修正卡塞格林 |
| 光圈 | 508 毫米(20 英寸) |
| 焦距 | 1537 毫米(60.5 英寸) |
| 焦距比 | f/3 |
| 中央阻塞 | 59%(按直径) |
| 安装表面的后焦距(未安装调焦器/旋转器) | 距安装表面 9.166 英寸 (232.8 毫米);距镜头盒 7.271 英寸 (184.7 毫米) |
| 重量 | 165 磅(75 千克) |
| OTA 长度 | 35.1 英寸(892 毫米) |
| 光学设计性能(光斑直径) | 轴上 3.86 微米 RMS、轴外 22 毫米处 4.04 微米 RMS、轴外 35 毫米处 6.04 微米 RMS(光斑直径) |
| 望远镜笼 | 碳纤维桁架杆,带碳纤维罩 |
| 最佳视野 | 70mm 像圈 |
主镜
| 光学直径 | 20 英寸(508 毫米) |
| 外径 | 20.8 英寸(528 毫米) |
| 形状 | 长椭圆体 |
| 材料 | 熔融石英(石英) |
| 涂层 | 增强铝 – 96% |
次镜
| 直径 | 286 毫米(11.26 英寸) |
| 材料 | 熔融石英(石英) |
| 形状 | 球形 |
| 涂层 | 增强铝 – 96% |
镜头组
| 直径 | 最大镜头:160 毫米(6.3 英寸) |
| 镜头数量 | 三 |
| 涂层 | 宽带增透膜(400 至 700 nm 范围内平均反射率小于 0.5%) |
包含物品
| 防结露加热元件 | 主镜和副镜上的加热垫需要 5 系列控制器(单独出售)。 |
| OTA封面 | 它可以保护主镜和光学管内部。 |
| 闪存盘 | 包含用于准直和间隔主镜和次镜的软件和说明。 |
| 扳手套装 (5812A35) | 标准六角扳手(仅限欧洲订单) |
配置
对于 DeltaRho 500 和 Series-5XL 调焦器:
为了获得适当的机械间隙,需要使用0.5 英寸垫片 (#6003165)。
如果用户计划使用我们的调焦器和旋转器,则将 0.5 英寸垫片放置在调焦器和旋转器之间,然后放置倾斜适配器。
如果用户计划仅使用调焦器,则 0.5 英寸垫片的组装方式如下:OTA、调焦器、垫片,然后是倾斜适配器。
倾斜适配器与 Series-5XL 调焦器兼容,因为调焦器和倾斜配件均使用 7.125 英寸法兰接口。
推荐配件
安装配件
- L-500 直接驱动安装座 (600550)
影像配件
- 适用于 5 系列调焦器或旋转器的倾斜适配器,可连接至 SecureFit (6061006)
OTA 配件
- 适用于 7.125 英寸法兰接口的 0.5 英寸延伸垫片 (6003165)
- 背驮式燕尾杆 (201990)
- 系列-5XL 调焦器 (6071001)
- 5 系列旋转器 (6021001)
- 5系列控制器(600199)
$38,000.00
多年来,我们一直梦想着打造出一款完美的广角成像望远镜,而 PlaneWave 革命性的 DeltaRho 350 f /3 望远镜终于实现了我们对创新的追求。DeltaRho 350 专为无与伦比的广角成像和现场易用性而设计。由于主镜固定到位,因此只需调整副镜的倾斜度和倾斜度即可快速实现准直。有了 Delta Rho 350,您的天文摄影体验将无与伦比!
- 修正卡塞格林焦点光学设计
- 孔径 – 350 毫米
- 焦距 – 1050 毫米
- 焦距比 – f /3
- 60mm 像圈 > 3 度
- 固定主镜
- 通过副镜上的 3 个倾斜螺钉进行准直
- 距安装表面(不含调焦器和旋转器)的后焦距为 5.651 英寸(143.535 毫米)。此距离包括来自滤光片的折射。
- 安装 5 系列调焦器和 5 系列旋转器后,后焦距为 2.525 英寸 (64.135 毫米)(调焦器位于行程范围的中间点)。
- 内置主、辅除露加热器,配有温度传感器
- *产品照片中的 L-350 支架单独出售
拍摄最令人惊叹的天文照片是我们团队所热衷的事情。从设计到制造,我们对 DeltaRho 350 的目标都是打造一款改变游戏规则的广角望远镜。DeltaRho 350 采用卡塞格林光学设计,这意味着成像列车固定在望远镜的背面,不会阻挡光路,而主焦点设计会严重限制用户使用滤光轮或大型相机的能力。
DeltaRho 350 是望远镜技术和易用性方面的一项惊人突破。DeltaRho 以 f/3 和 1050 毫米焦距运行,是一款广角望远镜,必将彻底改变您的天文摄影!
此外,DeltaRho 350 提供了完美的平坦视野,因此您的天文照片从图像的角落到角落都将具有惊人的清晰度,而场曲率不会降低照片的质量。DeltaRho 350 是一款出色的望远镜,它具有单镜准直的简便性、高级挡板的杂散光控制、通过有限元分析 (FEA) 创建的结构性能以及数十年的望远镜设计经验。使用大型 16803/4040 尺寸相机传感器时,DeltaRho 350 用户可以从边到边体验精确的星星和 170 x 170 弧分的视野。这个视野几乎是我们 CDK14 的 3 倍!当设备淡入背景并简单地运行时,天文摄影体验变得更加有趣和有益!
光学系统
| 光学设计 | 修正的 Dall-Kirkham (CDK) |
| 光圈 | 350 毫米 |
| 焦距 | 1050毫米(41.34英寸) |
| 焦距比 | f / 3 |
次镜
| 直径 | 7.48 英寸(190 毫米) |
| 材料 | 熔融石英(石英) |
| 形状 | 球形 |
| 涂层 | 增强铝 – 96% |
主镜
| 光学直径 | 13.78 英寸(350 毫米) |
| 外径 | 14.5 英寸(468.3 毫米) |
| 形状 | 长椭圆体 |
| 材料 | 熔融石英(石英) |
镜头组
| 直径 | 110 毫米(4.33 英寸) |
| 镜头数量 | 三 |
| 涂层 | 宽带增透膜(400 至 700nm 范围内反射率低于 0.5%) |
标准功能
| 修正卡塞格林 | 校正后的设计可产生没有离轴像散、彗形像差和场曲的平坦场。 |
| 碳纤维桁架设计 | 最大限度地减少因温度变化而引起的焦点偏移的热膨胀。 |
| 燕尾伸缩接头 | 考虑到碳纤维和铝之间的热膨胀差异。伸缩接头允许铝制燕尾榫膨胀和收缩,而不会对碳纤维下桁架造成压力 |
| 冷却风扇 | 三个冷却风扇将空气吹入望远镜后部。这有助于望远镜快速达到热平衡。如果购买可选的电子调焦附件 (EFA 套件),风扇将由计算机控制。 |
| Delta-T 就绪 | 为了增强防露效果,DR350 内部连接有聚酰亚胺薄膜加热垫和温度传感器,可通过可选的 Delta-T 控制器进行控制。 |
船运
| 板条箱运输重量 | 225磅 | 102 公斤 |
| 板条箱宽度 | 31英寸 | 787.4 毫米 |
| 板条箱高度 | 26英寸 | 660.4 毫米 |
| 板条箱长度 | 53英寸 | 1346.2 毫米 |
包含物品
| 防结露加热元件 | 主镜和副镜上的加热垫需要单独出售的 5 系列控制器 |
| OTA封面 | 保护主镜和光学管内部 |
| 闪存盘 | 包含主镜与次镜准直和间隔的软件和说明 |
| 扳手套装 (5812A35) | 标准六角扳手(仅限欧洲订单) |
推荐配件
OTA 配件
- 5 系列调焦器 (6011001)
- 5 系列旋转器 (6021001)
- 5系列控制器(600199)
安装配件
- L-350 直接驱动安装座 (600549)
- DeltaRho 350 背驮式燕尾槽 (140990)
影像配件
- 适用于 5 系列调焦器或旋转器的倾斜适配器,可连接至 SecureFit (6061006)
$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
$15,049.00
f/2.75.
What used to take a week now takes a night.
The DeltaRho 280 Argus is PlaneWave’s observatory-class wide-field astrograph for serious imagers and sky-survey programmes. Fused silica quartz mirrors, a carbon fibre OTA, and a 55 mm image circle at f/2.75 — 280 mm of aperture that turns nights of integration into a few productive hours.
f/2.75 is not just fast. It is the difference between finishing a target tonight and coming back next month.
13× faster than f/10. Every photon counts more.
At f/2.75, the DeltaRho 280 gathers light 13 times faster than an f/10 instrument of identical aperture. That is not an incremental advantage — it is the difference between a productive one-hour session and a week of cloud-interrupted integration. Research programmes and sky surveys that would otherwise take months become achievable in a single season.
mm image circle — large enough to cover full-frame sensors and beyond, with sharp stars from centre to corner at 4.5 μm RMS or better at 27.5 mm off-axis.
Focus stays locked. All night.
Primary and secondary mirrors are optical-grade fused silica quartz — near-zero thermal expansion, the same material used in premier research observatories. As temperature drops through the night, conventional glass mirrors shift focus. The DR280’s quartz mirrors do not.
Stiff where it matters. Light where it counts.
Carbon fibre delivers exceptional torsional rigidity with minimal mass. At 14.5 kg for a 451 mm OTA, the DR280 is a 280 mm instrument that mounts on observatory-class and high-end portable mounts alike — without needing a counterweight upgrade.
Sensor alignment without shimming or guesswork.
The integrated tip-tilt focal plane adjuster lets you dial in perfect sensor tilt with precision — no shims, no trial-and-error. It is consistent, repeatable, and done in minutes at the start of any session.
The Heart Nebula. In one frame.
The 770.6 mm focal length paired with the 55 mm image circle delivers over 4 degrees of field of view. Large nebula complexes, galaxy groups, and wide-field targets that require mosaics on narrow-field systems fit comfortably into a single frame — or anchor a multi-panel survey.
Dew control built in. Session-ending fog, ruled out.
Integrated dew control heater technology keeps the optical path clear on humid Australian nights. One less cable to run, one less failure point — the DR280 keeps imaging when lesser rigs fog out and call it a night.
Collimation solved. From first session to thousandth.
The DeltaRho 280 ships with PlaneWave’s collimation software that walks you through mirror alignment step by step — no iterative star-testing, no guesswork. Set it once: the rigid carbon fibre structure holds alignment through the night. The low-profile focuser delivers 0.5 inches of travel from a 163 mm back focus distance, giving your imaging train room to breathe.
M51. The Whirlpool Galaxy.
Galaxy arms, tidal bridges, and foreground stars resolved in a single short session. At f/2.75, integration time that would fill a week on a slower system compresses to a few productive hours.
IC 1805. The Heart Nebula.
H-alpha, RGB narrowband composite. The 4-degree–plus field captures the Heart Nebula’s full complex and surrounding star-forming regions in a single pointing — a target that demands a mosaic from slower, narrower systems.
Built for imagers who treat every clear night as a resource. Nothing wasted.
280 mm (11″) aperture with fused silica (quartz) primary and secondary mirrors for temperature-stable performance
f/2.75 focal ratio — 13 times faster than f/10, reducing required integration time dramatically
55 mm image circle at 4.0 μm RMS on-axis and 4.5 μm RMS at the full 27.5 mm off-axis radius
Integrated tip-tilt focal plane adjuster for precise sensor alignment without physical shimming
Carbon fibre optical tube — 451 mm OTA, 14.5 kg total weight for use on observatory-class mounts
Built-in dew control heater and broadband AR coatings (<1% reflection, 400–800 nm) for consistent all-weather performance
4°+ field of view capability with a 55 mm sensor — ideal for large nebula complexes and sky surveys
Compatible with PlaneWave L350 Direct Drive Mount — designed as an integrated professional imaging system
Every number that matters.
Professional imaging. Backed by Australia’s telescope authority.
$9,869.00
The fast SCT, reinvented.
8 inches. f/2.8. Carry-on weight.
The Observable Space FSCT8 is the first native f/2.8 Schmidt-Cassegrain ever built in an 8-inch form factor. A 42 mm image circle, fused silica quartz mirrors, and a 267 mm carbon-fibre OTA under 9 kg — designed from the optical axis out for astrophotographers who demand observatory results without the observatory.
Every clear night is too short. The FSCT8 makes sure you get the most out of every hour of it.
f/2.8 native. The SCT form factor finally fast.
A conventional 8-inch SCT runs at f/10. The FSCT8 runs at f/2.8 natively — no reducer stacks, no optical compromises. That is a 13-fold increase in photon-gathering speed. A four-hour integration target becomes roughly 20 minutes of effective exposure. For imagers working under Australian skies with limited clear nights, this is the most impactful single step up possible.
mm fully illuminated image circle. Sharp stars across the entire field at under 6.2 μm RMS — covering APS-C and most medium-format sensors with no vignetting.
Quartz mirrors. Focus doesn’t move.
Primary (210 mm) and secondary (114 mm) mirrors are both fused silica quartz — the same glass used in research-grade observatories. Near-zero thermal expansion means the focus point does not drift as temperature drops. Your collimation is still correct at 3 am.
267 mm OTA. Fits where full-size SCTs don’t.
The carbon-fibre upper cage is rigid, thermally stable, and keeps total OTA length at just 267 mm. That is shorter than many refractors. It mounts on mid-range equatorial platforms and travels as carry-on — without sacrificing the optical performance of a full 8-inch system.
Flat field. Corner to corner. No caveats.
The 88 mm broadband AR-coated corrector lens flattens the focal plane and holds sub-6.2 μm RMS optical performance across the full 42 mm image circle — from dead-centre to the corner of a full APS-C sensor.
Your full imaging train. No extensions required.
A 100 mm back focus from the mounting surface accommodates camera, filter wheel, electronic focuser, and off-axis guider without extension tubes. The 2.75 μm per arcsecond image scale is matched to modern small-pixel CMOS sensors — making the most of every pixel in the frame.
Purpose-built for imaging. Not retrofitted for it.
Observable Space — the PlaneWave and OurSky collaboration — built the FSCT8 as an imaging instrument from the ground up. Mirror material, corrector geometry, tube construction, back focus distance: every decision serves the astrophotographer. This is not a visual SCT with a reducer bolted on. It is a dedicated astrograph that fits in a carry-on bag.
8-inch aperture. Mid-range mount. Dark-sky remote site. All viable.
At under 9 kg and just 267 mm OTA length, the FSCT8 is mountable on equatorial platforms that a conventional 8-inch SCT with reducer stack would overload. It travels as carry-on, sets up in minutes, and puts professional-grade optical performance within reach of any dark-sky site — no permanent observatory required.
NGC 6992. The Eastern Veil Nebula.
Supernova remnant in Cygnus. Delicate filamentary emission structure that demands long exposures from slower systems resolves here in a fraction of the integration time — f/2.8 working exactly as intended.
M97. The Owl Nebula.
Planetary nebula in Ursa Major, approximately 2,600 light years distant. Extended shell structure and the characteristic owl-eye cavities resolved in a single night — a target that a slow system would need multiple sessions to match.
More signal per hour. Every clear night finally worth the effort.
Native f/2.8 focal ratio — the first fast SCT in an 8-inch system, designed for wide-field deep-sky imaging from the optical axis out
42 mm fully illuminated image circle with optical performance under 6.2 μm RMS across the full field — sharp stars edge to edge
Fused silica (optical-grade quartz) primary (210 mm) and secondary (114 mm) mirrors with enhanced aluminium coatings for temperature stability
Carbon-fibre upper cage construction — 267 mm OTA, under 9 kg total weight for use on mid-range to high-end imaging mounts
88 mm broadband AR-coated corrector lens delivers a flat focal plane and 2.75 μm per arcsecond image scale suited to modern CMOS sensors
100 mm back focus from mounting surface — accommodates cameras, filter wheels, and electronic focusers in a standard imaging train
4°+ field of view with a 42 mm sensor — ideal for large emission nebulae, galaxy groups, and all-sky survey programmes
An Observable Space instrument — the merger of PlaneWave precision optics engineering and OurSky imaging systems expertise, purpose-built for the astrophotographer
Every number that matters.
The fast SCT, reimagined. Backed by Australia’s telescope authority.
$950.00
The back plate on all of the CDK models has four mounting positions for a finder mounting plate.
- The finder mounting plate attaches to the back plate of the telescope and the quick-release finder bracket attaches to the mounting plate.
- If the telescope is used on a German Equatorial mount it may be convenient to purchase two finder scopes, one for the east and one for the west side of the telescope.
- The finder scope is a Baader 10×60 Varios with mounting rings and L- bracket.
$160.00
- This is an L-shaped bracket that attaches in four different places on the back of any of the CDK models.
- This is used to mount a finderscope or some other accessory.
- Two 1/4-20 screws provided attach the bracket to the backplate of the telescope and two 10-32 threaded holes spaced at 1.450″ can be used to mount accessories too.
$1,210.00
Sliding counterweight system, counterweights not included.
From $600.00
Allows multiple 4.5 or 9 lbs weights that can have their distance to the optical axis adjusted, in and out, and slide up and down, on the lower piggyback dovetail of a fork-mounted CDK14, 17, 20, 24, or 700.
$320.00
Dovetail counterweight adapter.
$230.00
Counterweight bracket for CDK14, CDK17 and CDK20.
$520.00
The counterweight kit comes with a mounting bracket and three 0.5 lb weights.
Additional weights can be purchased separately.
$620.00
Counterweight kit for CDK12.5 attaches to the dovetail bar for critical balance in Declination.
$200.00
The EFA PC Port Kit allows connecting the PWI Software to the PC port on the EFA Box. Each kit contains:
- a USB to Serial Converter
- an Ethernet to 9-pin Adapter and
- a short Ethernet cable
$720.00
The EFA (Electronic Focusing Accessory) control box can be mounted to the back plate of any PlaneWave telescope OTA (12.5 through 24 inches). The EFA Kit reads the primary mirror and ambient temperature sensors.The EFA controls the fan systems that are built into each telescope.
A Hand Controller is provided to control an optional Focuser or Rotator when standing at the eyepiece. The EFA kit comes with PlaneWave Interface (PWI4), a software package that controls all EFA functions from a PC. Cables and adapters are provided to attach the EFA kit to a PC. The EFA kit is ASCOM compatible.
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