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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
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1788 products
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From $36,350.00
推出全新派拉蒙 ME 6 系列天文台主力产品。
派拉蒙 ME 6 系列代表了最新的齿轮驱动 GEM 性能。
它的新功能包括最先进的 MKS 6000 望远镜控制系统,可让您通过 USB C、以太网和 Wi-Fi 进行连接。它的双端口 USB 2.0 集线器位于仪表板上,位置方便
Paramount ME Series 6 仍然是专业和高级业余天文学家最喜爱的天文台产品。
硬件规格
- 仪器容量 109 公斤;最大有效载荷容量 218 公斤(仪器 + 配重)
- 所有天空指向精度均等于或低于 30 角秒 RMS
- 一体式安装设计,不含配重或配重轴,重量为 38 千克
- 校正前峰峰周期误差最大为七 (7) 角秒
- 经过一次训练,周期误差为 1 角秒,峰峰值或更小
- 可选的 26 位 Renishaw 编码器可消除周期性误差和归位需要;可在低至 –40° C 的温度下运行
- 如果你现在不想使用编码器,但后来又决定要使用它们,则可以在 Paramounts ME Series 6 上进行改装
- 由于人们对编码器能做什么和不能做什么存在一些困惑,下面有一个常见问题解答,详细说明了这一点以及它们是否适合您
- 其编码器电缆位于支架内部,有助于防止障碍物。
- 所有电子设备和安装电缆均安装在安装座内,并有足够的空间容纳其他电缆
- 其最先进的 MKS 6000 望远镜控制系统 (TCS) 可让您通过 USB C、以太网和 Wi-Fi 进行连接
- 仪表板上的双端口 USB 2.0 集线器
- 随附的 Versa-Plate™ 可方便地容纳大多数望远镜
- 包含 48V DC 电源以及 PC 安装 USB 和以太网电缆
- 包含两个 14 公斤配重物。如果您的成像系统重量超过 28 公斤,您可能需要更多配重物。
- 带弹簧蜗轮的皮带传动齿轮几乎不会产生任何间隙
- 耐用且不褪色的红色粉末涂层和黑色阳极氧化表面;组件为铝制
- 无离合器设计有助于保持其 TPoint™ 辅助指向精度
- AutoHome™ 归位功能可确保支架始终知道其方向(在执行称为“归位”的初始化过程后,通常需要不到一分钟的时间)
- 校准方位角和仰角极轴对准调整速度极轴对准
软件规格
- 如果没有 TPoint™ 和 ProTrack™ 软件,派拉蒙 (Paramount) 无与伦比的指向和跟踪功能就不可能实现。
- 通过使用 TPoint 的校准和望远镜建模工具,您将享受 30 角秒 RMS 或以下的所有天空指向精度。没有什么能比它更好
- ProTrack™ 与 TPoint ™ 配合使用,不断更新支架在两个轴上的位置,以纠正系统范围的跟踪错误,包括管弯曲、大气折射、极轴失准、非中心编码器引起的谐波误差等。
- 单靠轴上绝对编码器无法纠正所有望远镜都存在的这些错误。必须正确应用望远镜模型才能实现卓越的跟踪。
- 在没有编码器的情况下,派拉蒙 ME 6 系列可以提供异常长时间的无引导曝光(一位顾客报告说是 20 分钟)。
- 有关编码器能做什么和不能做什么的更多信息,请参阅下面的常见问题解答。
- 所有包含的软件都集成到一个易于使用的应用程序中,该应用程序由 TheSky™ Professional、TPoint™、Cameras+、Domes、Multi-OS+ 和 Weather 模块组成。
- 您可以使用此应用程序控制所有与天文摄影相关的相机和设备。
- 它可以在 macOS™、Windows™、Ubuntu™ 和 Linux(x86_64 和 ARM64 架构)上运行。
- 无论您在哪种操作系统上运行它,它的外观和操作都完全相同。您甚至可以在操作系统之间切换,并且其许可证最多允许六台计算机。为什么要让自己或您的机构陷入困境呢?
- 除了派拉蒙独有的 ProTrack™ 之外,附带的软件作为 TheSky™ 通用套装单独出售,价值 1,095 美元。
库存编号:SB10616
可应要求提供可选黑色阳极氧化支架
$4,299.00
Victory® HT 高级双筒望远镜让您以全新的维度体验大自然。得益于革命性的光学概念,它们可提供 95% 以上的透射率。这一卓越价值是通过 SCHOTT HT 镜头、ZEISS T* 多层镀膜和 Abbe König 棱镜系统的完美结合实现的。即使在最深的黄昏,您也可以享受无与伦比的亮度和非凡的细节水平。人体工程学设计同样具有创新性。令人印象深刻的全新 Comfort Focus 概念在双链桥中嵌入了一个大型调焦轮。它使双筒望远镜非常坚固且非常易于使用。体验最高水平的尖端光学器件 - 拥有世界上最明亮的高级双筒望远镜。
10 倍放大倍率可提供令人难以置信的细节视图。10x54 的亮点包括极高的亮度和极高的对比度。凭借坚固而紧凑的结构,它们即使在具有挑战性的光照条件下也能为自然爱好者提供最高水平的光学效果。
95% 透光率
高透射率肖特眼镜可在弱光条件下实现最佳目标识别和分辨率。明亮、高对比度的图像为您提供狩猎所需的额外几分钟。毕竟,一天中的第一道或最后一道光往往是那些永远留在您记忆中的神奇狩猎时刻的关键。
优化的镜片直径
优化物镜直径以减轻重量。无论以何种方式握持,都能确保在任何情况下都能流畅成像。通过这种方式,设计可满足完美视觉体验的最高标准。
ComfortFocus 概念
显眼的大型对焦轮和超长的平移使您能够极其精确地对焦,以获得完美的焦点,即使戴着手套也是如此。
无论天气如何,视野都清晰
大自然中总有令人兴奋的事物值得观赏——即使在潮湿的天气。这就是蔡司开发 LotuTec® 的原因。这是一种用于双筒望远镜和观景镜镜片的涂层,可在所有天气条件下实现清晰无阻的视野。
蔡司 T* 镀膜
蔡司 T* 镀膜是您在弱光条件下和黄昏时体验到的明亮高对比度图像的保证。然而,其背后并没有构建涂层的特定配方。相反,它是一种不断调整以适应新玻璃材料和要求的技术,并且每个镜头都有所不同。
规格
放大
10 ×
有效透镜直径
54 毫米
透光率
95%
出瞳直径
5.4 毫米
暮光因素
23.2
1,000 米(码)处的视野
110 米(330 英尺)
主观视角
西经 63°
近对焦距离
3.5 米(11.5 英尺)
屈光度调节范围
− 3.0 | + 3.0 dpt
出瞳距离
16 毫米
瞳距
58 – 76 毫米
镜头类型
FL/HT型
棱镜系统
阿贝·柯尼希
特征
LotuTec | 充氮
+ | +
防水性能
500 毫巴
规格
工作温度
− 30°C | + 63°C
长度
193 毫米
瞳距为 65 毫米时的宽度
142 毫米
重量
1.05公斤
$599.00
The Sky-Watcher Black Diamond 130/650 Photo Reflector OTA is a 130mm aperture Newtonian reflector with diffraction limited optics, all the light gathering power you need for visual use or astrophotography! Newtonian reflector telescopes are among the most cost effective design on the market, reaching much larger apertures than an equivalently priced refractor. The large aperture will help resolve faint, extended objects like nebulae and galaxies, whilst the 650mm focal length will reveal fine details of lunar craters.
The 130/650 Photo Reflector is equipped with an excellent Crayford dual speed focuser allowing fast, coarse regulation followed by a precise 10:1 reduction adjustment knob to reach the optimal focus. A 3 element 28mm LET eyepiece is provided, allowing 23x magnification and a 56° apparent field of view with 20mm of eye relief. The aluminised primary mirror is aspheric (parabolic profile) offering an optical system free from spherical aberration. The secondary mirror is thin to allow fast cooling and it is held by extra thin spider supports for minimal diffraction spike effects on bright stars and increased contrast.
In The Box:
- SkyWatcher Black Diamond 130/650 Photo Reflector OTA
- 28mm LET Eyepiece
- 6×30 Finder Scope
- 130mm Tube Rings
- Dovetail Bar
| Optical Design | Newtonian (Parabolic) |
| Diameter/Aperure | 130mm |
| Focal Length | 650mm |
| Focal Ratio | f/5 |
| Finder Scope | 6x30mm |
| Eyepiece | LET 28mm 2" |
| Focuser | 2" Crayford 10:1 Dual Speed |
From $15,889.00
SBIG Aluma AC2020BSI
超高灵敏度背照式科学级 CMOS 相机。400 万像素传感器,像素大小为 6.5 微米,具有自适应光学功能,兼容 StarChaser Guider。
SBIG Aluma AC2020BSI 采用 1 类传感器。
熔融石英腔体窗口可配备 VIS-NIR 和 UV-VIS 光学涂层选项。
即将推出 – 可预订。
SBIG Aluma AC 系列代表了天文成像系统先进科学 CMOS 相机的最新技术。相机的先进设计允许通过 USB 3.0 连接将数据高速下载到控制计算机。SBIG Aluma AC2020BSI 使用 Gpixel GSENSE2020BSI-H CMOS 传感器,该传感器具有 400 万像素,分辨率为 6.5 微米,阵列尺寸为 2048 x 2048。传感器尺寸略大于 13.3 平方毫米。Aluma AC 系列具有强大的两级冷却功能,并支持可选的水冷。Aluma AC 相机可直接通过 12VDC 8A 电源供电。
设计特点包括:
背照式传感器
令人难以置信的灵敏度!高性能背照式传感器在制造过程中被翻转并变薄,因此入射光在到达敏感像素区域之前不会遇到任何电路。这为整个可见光谱及更远的光谱提供了最佳灵敏度。
GSENSE2020BSI-H 中的传感器峰值量子效率为 91%,可见光谱中峰值较宽。对于近紫外和红外应用,它在 200 nm 至 1000 nm 范围内具有良好的灵敏度。
腔体窗口涂层选项
GSENSE2020BSI-H 传感器是无窗的,可为整个传感器提供最佳灵敏度。对于无窗传感器,我们建议每年给干燥剂塞充电一次,以避免传感器受到湿气污染的风险。
密封传感器室上的熔融石英光学窗口有两种标准涂层可供选择,具体取决于您的应用。VIS-NIR 提供 400 nm 至 1000 nm 范围内的最佳灵敏度。UV-VIS 提供 250 nm 至 700 nm 范围内的最佳透射率。
StackPro™
SBIG Aluma AC2020BSI 科学 CMOS 相机具有StackPro™ ,这是一项在相机内部执行图像堆叠的革命性功能。
CMOS 传感器的阱深和位深度通常比其前身 CCD 传感器更有限。同时,现代 CMOS 传感器的读取噪声比同等 CCD 低得多。这种低读取噪声可以发挥优势,通过堆叠许多较短的曝光来实现相同的最终结果。然而,这会导致大量额外的磁盘使用和后期处理。
StackPro™ 可在相机内部自动执行堆叠。它会自动将您的曝光细分为最多 16 个单独的子曝光,并在下载之前将它们堆叠在相机内部。这可避免硬盘中堆积过多的数据。堆叠还可用作高动态范围 (HDR) 模式的替代方案。
H DR 模式
AC2020BSI 中的传感器能够在 HDR 模式下运行,其中高增益和低增益图像可同时读出。我们附带的 MaxIm LT 软件具有 HDR 合并功能,可大大简化生成清晰、高度线性图像的过程。
出色的冷却效果
与业界领先的 STX 系列相机共享的经过验证的针式散热器设计可散发热量,同时提供低振动。包括SmartCooling™智能热电冷却和风扇操作。
水循环准备就绪
对于高环境温度环境,液体冷却选项可提高热性能并有助于最大限度地减少暗电流。
用户可充电干燥剂
SBIG 率先采用了高科技用户可更换的滤芯,其中装有陶瓷过滤器和分子筛干燥剂。与其他竞争相机不同,当其腔体干燥剂最终饱和时,它们需要工厂维修,而用户可以轻松重新填充干燥剂。这消除了昂贵的维修需求,更不用说相关的停机时间和运输成本了。此功能在高湿度地区尤其重要。
电子和机械快门
GSENSE CMOS 传感器具有电子滚动快门。此外,Aluma AC 系列相机还配备机械快门,可方便地进行暗帧减法,以实现最佳性能和灵敏度。这对于远程/机器人操作至关重要。
可选 12 位滤光轮
SBIG Aluma AC2020BSI 与新型 12 位置 SBIG AFW-12-50R滤光轮兼容,使用 50 毫米圆形滤光片。
它还兼容 7 位置FW7-STX滤光轮,使用 50 毫米方形滤光片。
提供自导和自适应光学选项
可用的 SBIG StarChaser SC-3是在滤镜前集成自动导航的绝佳低成本选择,并且它支持我们的 SBIG AO-X自适应光学配件。
AO-X 使用倾斜窗口来快速精确地调整图像位置,以响应自动导航器的反馈。使用自适应光学系统,不会出现间隙、静摩擦或滞后,移动精确准确。这使得 AO-X 不仅可以消除周期性误差、漂移和阵风的影响,还可以减少大气视宁度的影响。与 Aluma AC 相机一起使用时,AO-X 需要 StarChaser SC-3。
更多信息请参阅AO-X 。
USB 3.0 接口
Aluma AC 包含一个 USB 3.0 接口端口,用于高速下载。对于需要较长电缆长度的安装,该端口还兼容 USB 2.0。
I2C AUX 端口
STX 相机有一个方便的辅助控制端口(也称为 I2C AUX 端口),用于控制滤光轮并提供可选的外部触发接口。与旧款 SBIG 型号不同,AUX 端口不用于 AO-X 控制,因为此功能现在由可选的 SBIG StarChaser SC-3 离轴引导相机处理。
MaxIm LT 软件
所有 SBIG 相机均配备我们的 MaxIm LT 软件 - 价值 200 美元!MaxIm LT 是我们备受推崇的 MaxIm DL 软件的一个特殊版本,可完全控制您的相机、滤光轮和自动导星器,以及高级图像处理功能。如果您愿意,可以升级到 MaxIm DL Pro,以获得完整的天文台集成以及更多的处理和分析功能。
附带配件
所有 Aluma AC 相机都配有豪华手提箱、通用电源、Aluma AC 电源延长线、USB 3.0 线和 MaxIm LT 软件。
规格
| 接触 |
0.001 至 3600 秒 |
|---|---|
| 操作系统兼容性 | Windows 7、8、10 x86/x64、MacOS 10.14 “Mojave” x86 二进制文件、Ubuntu 18.04 LTS x64、Raspbian Buster armhf、Ubuntu MATE arm64 |
| 全画幅下载 | 0.1 秒 |
| 重量 | 3.5 磅 / 1.6 千克 |
| 过滤器尺寸 | 50毫米方形 |
| 读取噪声(典型值) | 2-CMS 读出模式下为 1.2 e-,常规模式下为 1.6 e- |
| 温度调节 | 是的 |
| 计算机接口 | USB 3.0 |
| 力量 | 12 伏直流 8 安 |
| 冷却三角洲 | 典型值 ~ 40 °C,包括水冷选项 |
| 自适应光学选项 | AO-X 和 StarChaser SC-3 |
| A/D转换器 | 双 12 位,具有 HDR 功能 |
| 暗电流 e-/p/s | 0.16 e-/p/秒 @ -20C |
| 全井容量 | 55,000 电子 |
| 传感器尺寸 | 13.3 毫米 x 13.3 毫米 |
| 成像/像素阵列 | 2048 x 2048 |
| 快门 | 卷帘电子、机械暗快门 |
| 过滤器前的自我引导 | 是的,使用 StarChaser |
| 像素大小 | 6.5 微米 |
| 总像素 | 400 万 |
| 滤光轮选项 | FW7-STX |
| OAG 选项 | 追星者 |
| 影像传感器 | 长光辰芯 GSENSE2020BSI |
| 室内窗户 | 可见光-近红外光、紫外-可见光 |
$2,799.00
Optec 温度补偿聚焦器-S3i
这款型号没有偷工减料。巨大的拉管内径为 3.00 英寸,由 7075 制成,这是最坚固的商用铝合金。为了防止 Crayford 式调焦器常见的任何滑动,驱动杆以大约 500 磅的力压在拉管上。TCF-S3 可以承受这种极端压力,因为驱动杆由直径为 0.375 英寸的高速钢磨棒制成。拉管中嵌入了硬化不锈钢导轨,以接合驱动杆并承受应变。
TCF-S3 已拆下齿轮盖。所有齿轮均由 303 不锈钢制成。
拉管的总线性行程为 1.00 英寸,分辨率为 0.0001 英寸。与 TCF-S 一样,带有 IN 和 OUT 按钮、串行计算机接口和数字显示器的控制箱可控制 TCF-S3 的所有功能。TCF-S3 的所有其他功能与 TCF-S 相似。它使用相同的电缆、温度探头和新的远程键盘。它还与当前的 Optec 控制软件 TCF-S.exe 兼容。
其他望远镜支架可在我们的商店定制。此调焦器仅适用于具有大型支架的大型望远镜。请参阅价格表以获取可用支架的列表。提供 3 英寸至 2 英寸适配器,以适合 Optec 和其他标准 2 英寸配件。
TCF-S3 配有标准配件,包括控制器、温度探头和电源(未显示)。
对于 Paramount ME 的用户,Optec 提供了一个特殊套件,可以方便地通过支架连接 TCF-S3。此外,IFW 和 Pyxis 也可通过支架进行安装和连接,以便于使用并减少电缆。
$5,899.00
One 9.0 mono 是 Atik 最新、最出色的索尼相机。它采用 9MP ICX814AL,配备极其灵敏的 EXview HAD II 技术、超低读取噪音、机械索引 5 位滤光轮和增强的冷却性能。
它还采用了全新的 CCD 腔体设计,使用高纯度氩气吹扫,并配有集成的 USB 2.0 集线器和配件电源端口。现在您只需使用两根电缆即可操作整个系统!
From $1,730.00
- The EFA kit automates focusing on the optional Hedrick Focuser, or IRF90 rotating focuser.
- Monitors temperature (primary-mirror and OTA back-plate).
- Controls the fans built into CDK telescopes.
- Ensure you have the proper EFA kit selected for your telescope below.
- 125901-Kit is for all 12.5″ OTAs (CDK/ IRDK).
- 240901-Kit is for all 14-24″ OTAs (CDK/ IRDK/ RC) and CDK700s.
*If the EFA is not purchased, the ability to automate temperature regulation for the primary mirror will be lost. This is especially significant when using a third-party focuser, as the EFA is required for full automation.
From $440.00
Adapter to feather touch focuser for CDK's.
From $1,040.00
Counterweights for 1.5″ shaft (For Paramount, ORIGINAL/MX/MX+, NOT MEII )
$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 |
$99,310.00
The CDK450 Observatory System from PlaneWave Instruments is a sophisticated solution designed for the serious astrophotographer and dedicated astronomy researcher. This high-end system combines the powerful CDK17 optical tube with the precise L-550 direct-drive mount, creating an exceptional observational platform that excels in a variety of scientific and imaging applications.
Key Features of the CDK450 Observatory System
CDK17 Optical Tube Assembly
- Advanced Optical Design: Employs a Corrected Dall-Kirkham optical design, achieving a field free of off-axis coma and astigmatism and a perfectly flat field across a 52 mm image circle, resulting in critically sharp images over the entire viewing area.
- High-Quality Construction: Constructed with robust carbon fiber, reducing thermal expansion and enabling quick thermal equilibration, which helps maintain precise optical alignment under fluctuating temperatures.
- Superior Mirrors and Coatings: Equipped with high-stability fused silica mirrors known for minimal thermal expansion, paired with high-performance coatings that maximize light throughput while minimizing stray light for optimal imaging quality.
- Thermal Management: Incorporates an advanced cooling system with strategically placed fans that ensure rapid thermal stabilization, essential for maintaining consistent, high-quality imaging and minimizing focus shifts caused by temperature changes.
CDK17 f/6.8 OTA
- Aperture and Focal Length: Features a 17-inch aperture, a shorter 3454 mm focal length at a faster f/6.8 focal ratio, and a shorter back focus of 262 mm.
L-550 Direct Drive Mount
- Direct Drive Motors: Features state-of-the-art direct-drive motors on each axis, providing smooth, fast, and virtually silent movement of the telescope with zero backlash and zero periodic error, perfect for precise tracking and rapid repositioning of celestial objects.
- High-Resolution Encoders: Outfitted with high-resolution optical encoders on both axes, offering precise positioning and movement, which is crucial for elite astrophotography and detailed astronomical studies.
- 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, essential for prolonged accurate tracking and reducing stress on the mount during extended observations.
- Rapid Target Acquisition: Capable of impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial bodies and satellites, vital for dynamic observations and responsive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK450 is a formidable system for astrophotographers, offering unmatched tracking accuracy and image stability, which facilitate capturing spectacular celestial images with detailed resolution and vibrant colors. The L-550 carries a greater payload capacity – perfect for holding a second telescope on the outside hub.
Astronomy Research
Researchers will find the CDK450 invaluable for its consistent performance and precise data collection capabilities. It serves as a robust platform for sophisticated photometry, spectroscopy, and minor planet tracking, offering a solid foundation for scientific discovery and exploration.
Visual Observations
For enthusiasts of visual astronomy, the CDK450 provides vibrant and detailed views of the universe. Its significant aperture and high-quality optical components ensure exceptional viewing of planetary, lunar, and deep-sky objects, enriching every observational experience.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-550 mount in the CDK450 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 | 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 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Optical systems
| Aperture | 17 inch (432 mm) |
| Focal Length | 2939 mm (115.71 inch) |
| Focal Ratio | f/6.8 |
| Central Obstruction | 23.7% by surface area; 48.6% of the primary mirror diameter |
| Backfocus from Mounting Surface | 10.32 inch (262.33 mm) |
| Backfocus from Racked in Focuser | 7.24 inch (184 mm) |
| Weight | 106 lbs (48 kg) |
| Optimal Field of View | 70mm image circle |
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 | 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
| 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 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 | |
| Gamepad - Used for control of the mount tracking speeds for visual observing | |
| Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-550 mount |
$63,800.00
The DeltaRho 350 Telescope System from PlaneWave Instruments is crafted for elite astronomers and astrophotographers who demand the best. Created with a passion for excellence, the DeltaRho 350 Telescope System brings groundbreaking features to advanced imaging, offering unmatched versatility across a spectrum of scientific and communicative applications. The DeltaRho 350 Telescope System from PlaneWave Instruments features a 350mm wide-field, f/3 aperture. This premium CDK optical tube combines a DeltaRho 350 with a L-350 direct drive mount.
DeltaRho 350 Telescope System’s Key Features
Large Aperture and Fast Focal Ratio
The DeltRho 350 has a 350 mm aperture and an impressively fast f/3 focal ratio. This combination allows significant light-gathering capability and rapid image capture, perfect for detailed SSA/SDA object capture and deep-sky photography.
Advanced Optical Design
Featuring a corrected Cassegrain focus optical system, the DeltaRho 350 ensures top-tier image clarity. Achieve sharp, flat fields across the entire field of view with no curvature, capturing stellar images that require minimal post-processing.
Mechanical Structure
Constructed with a lightweight yet sturdy carbon fiber tube. This Offers enhanced durability and stability while minimizing thermal expansion and maintaining optimal image quality under various environmental conditions.
High-Performance Coatings
Equipped with high-quality mirror coatings that can be customized to meet specific observational requirements. It enhances light transmission and reduces stray light, optimizing the telescope for specialized applications such as SSA/SDA and FSO.
Collimation Software
The DeltaRho 350 is equipped with user-friendly collimation software designed to ensure optimal alignment of optical elements quickly and accurately. This feature is crucial for maintaining the high resolution and sharpness needed for professional-level imaging and research, allowing users to adjust collimation on the fly easily.
Dew Control
Integrated dew control systems in the DeltaRho 350 utilize advanced heater technology to prevent condensation on optical surfaces. This system ensures that dew does not interrupt observations and imaging sessions, providing consistent clarity and performance in various environmental conditions.
Application-Specific Benefits
Astrophotography
The DeltaRho 350’s fast exposures and expansive field view allow astrophotographers to capture breathtaking night sky images with exceptional detail and clarity.
Astronomy Research
With its robust build and advanced optics, the DeltaRho 350 is an excellent tool for universities and research institutions engaged in long-term astronomical studies.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
The Delta Rho's fast focal ratio and large image circle allow you to take shorter exposures and use larger Sensors. Making it perfect for surveying larger areas of the sky for quicker monitoring and cataloging of space debris and satellites.
Mount Systems
| 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 systems
| 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 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Optical Systems
| Aperture | 350 mm |
| Focal Length | 1050 mm (41.34 in.) |
| Focal Ratio | f/3 |
| Central Obstruction | 56 % by diameter |
| Backfocus from Mounting Surface | 5.6 in. (142.24 mm). This distance includes refraction from filters. |
| Weight | 46 lbs (21 kg) |
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 | 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
| 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 | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror |
$142.00
Made from a special high-buoyancy material, the floating shoulder strap prevents binoculars from sinking should they fall into water.
$5,299.00
介绍 iOptron 应变波齿轮安装系列的新成员 - AZ/EQ 双安装 HAE29 和 HAE29EC!这些重量轻、有效载荷高的小型巨人将带来前所未有的天文体验。想象一下,安装头重 8 磅,有效载荷能力 29.7 磅,无需笨重的配重或轴。HAE29 运用 iOptron 数十年打造精密安装的经验,将这一愿景变为现实。
HAE29 采用最先进的应变波齿轮技术,用于 RA 和 DEC 机芯,提供无与伦比的重量与有效载荷效率。其黑色阳极氧化全金属 CNC 加工机身不仅外观漂亮,而且坚固耐用,在未来许多年内都能保持最高水平的性能。电子摩擦制动器和断电记忆等独特功能使支架能够安全停止和恢复 GoTo 旋转,或者在突然断电后继续跟踪(无需重新调整并从头开始)。
HAE29 支架可由计算机控制,可通过 Windows PC 的 ASCOM/Commander 或 MacOS 软件的第三方 INDI 驱动程序进行控制;可通过 iOptron Commander Lite 或 SkySafari 等应用程序通过智能手机/平板电脑进行控制;或通过 INDI 驱动程序通过 Raspberry Pi 设备进行控制。
HAE29EC 具有高精度 RA 轴编码器,可提供令人难以置信的跟踪精度,足以让许多人选择“无”引导的图像。
特征
- 先进的谐波齿轮系统技术
- 有效载荷能力为 13.5 千克(29.7 磅),安装重量为 3.7 千克(8.15 磅,包括燕尾鞍座)
- CNC加工
- RA 和 DEC 上均采用独特的摩擦制动器,可在计划内或计划外断电期间安全停止运动
- 360秒档位周期
- 带实时 PEC (RPEC) 的高精度编码器
- Go2Nova® 手动控制器,带有 ~212,000 个对象数据库
- iPolar 电子极轴镜,可轻松、准确地进行极轴校准
- 客户电缆管理系统已准备就绪
- 双鞍座(Vixen 和 Losmandy-D 款式)
- 内置零位搜索和定位器
- 断电位置和位置记忆
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi(通过手动控制器)
- USB 端口用于固件升级和计算机控制
- 携带箱
- 两年保修
规格
| 山 | 应变波地平仪/赤道仪 |
| RA 齿轮系统 | 谐波齿轮 |
| DEC齿轮系统 | 谐波齿轮 |
| 减速比 | 红移 480:1,赤经 360:1 |
| 不含 CW 的有效载荷 * | 29.7 磅(13.5 千克) |
| 安装重量 | 8.15 磅(3.7 千克),含燕尾鞍座 |
| 有效载荷/安装重量 | 3.65 |
| 带 CW 的有效载荷* | 40磅(18公斤) |
| 高精度编码器 | 是 (RA) |
| 聚乙烯醇 | 实时 PEC (RPEC) |
| 时期 | 360 秒 |
| 驱动电机 | 步进电机 |
| 结构材料 | 全金属,CNC加工 |
| 外饰 | 阳极氧化黑色 |
| 极地观测镜 | iPolar 电子极轴镜(外置) |
| 液位指示器 | 水准气泡 |
| 控制系统 | GOTONOVA/指挥官 |
| 手持控制器 | Go2Nova® 8409 拥有约 212,000 个对象的数据库 |
| 追踪 | 自动的 |
| 最大回转速度 | 6度/秒 |
| 功耗 | 0.6A(跟踪),1A(GOTO) |
| 力量 | DC12V-5A(5.5/2.5mm DC插头) |
| 交流适配器 | 100V ~ 240V (含,仅限室内使用) |
| 电缆管理 | 准备 DIY |
| 断电刹车 | 电子摩擦制动器 |
| 掉电记忆 | 是的 |
| 无线上网 | 内置 |
| 通信端口 | 是(Wi-Fi 和 USB,通过 HC) |
| 自动导航端口 | 是(兼容 ST-4) |
| 固件升级 | 是的 |
| 燕尾鞍座 | 泼妇与洛斯曼迪 |
| 三脚架 | 选修的 |
| 配重轴 | SS Φ20X200mm, 3/8"-16 螺纹 (可选) |
| 配重 | 10 磅(4.5 千克)(可选) |
| 操作温度 | -20℃~40℃ (手动控制器-10℃~40℃) |
| 保修单 | 两年有限 |
* 200 毫米,有效载荷重心位于 RA 旋转轴。或者 OTA 尺寸约为 220 毫米。
$899.00
Pixfra Mile 2 Thermal Monocular: creating new pathways for birding and conservation
Thermal imaging is changing the way we observe and count birds in their natural environment - at all times of the day or night, without intrusive lighting or disturbance.
Any birder knows there's often times when birds are hidden from view, either by foliage or the time of day. It becomes even more frustrating when bird counts are needed to estimate population or species locations for conservation efforts and protection and they simply can't be properly seen.
In situations like this, no matter how powerful the binoculars you're using, the birds will remain hidden.
Thermal imaging devices lets you "see" birds via the heat their bodies produce - revealing them in bushes and trees or when there's simply not enough natural light otherwise.
Have a chat to the experts at BINTEL about how new generation devices like the Pixfra Mile 2 can help how you discover new ways to view nature.
Includes:
- 15mm lens
- 2.33x-18.64x magnification
- View wildlife up to 800m away
- 8 Hours Battery Life
- Share your live views with up to up 4 people nearby
- Vanadium oxide uncooled focal plane detector.
- Ultra-low power consumption.
- Connects to the mobile app through Wi-Fi.
- Six colour palettes.
- Built-in EMMC (16 GB).
- Electronic compass for quick direction identification.
- Lightweight and portable.
- IP67 rated.
A design wonder
Hidden Power Switch, Non-Slip Silicone Texture, and a Smooth, Continuous Exterior for Unmatched Ergonomics.
Compact size that sits easily in your hand
Truly pocked sized, the PixFra Mile 2 Series monoculars fit the palm of your hand and can be used for extended periods of time without fatigue.
Despite the compact design, the Mile 2 also produces 640x512 resolution images on your devices.
Logical, Easy to Use Button Layout
Perfect for night-time use or low light conditions, the control button layout is thoughtfully laid out and can be easily used one-handed without a second thought .
Main Features
| Thermal | |
| Thermal Detector Type | Vanadium oxide uncooled focal plane detector |
| Effective Pixels | 256 (H) × 192 (V) |
| Pixel Pitch | 12 μm |
| Spectral Range | 8 μm–14 μm |
| Sensitivity (NETD) | ≤35 mK@f/1.0, 25 °C |
| Focal Length | 15mm |
| Aperture | 2.6m |
| Detection Distance | 800m |
| Magnification | 2.33x |
| Frame Rate | 50 Hz |
| Display | |
| Screen | 800 × 600, 0.32 inch, OLED |
| Colour Palettes | 6 (white hot/black hot/iron red/alarm/emerald/amber) |
| Video Compression | –3 D to +1 D |
| Eye Relief | 13mm |
| Exit Pupil | 5mm |
| Functions | |
| Digital Zoom | 1×, 2×, 4×, 8× |
| Video Recorder | Yes |
| Snapshot | Yes |
| Wi-Fi Hotspot | Yes |
| Hot Spot Track | Yes |
| Video Distance Measurement | Yes |
| FFC Calibration | Auto, Manual, External Correction |
| Standby Mode | Yes |
| DPC (Defective Pixel Correction) | Yes |
| Storage Built-in | 16 Gb |
| Power | |
| Battery Type | Rechargeable Lithium battery |
| Battery Life | Battery Life 8.5 hrs @25 °C |
| Power Supply | 5 VDC/2A |
| Port | USB Type-C |
| Overvoltage Protection |
Yes |
| General | |
| Operating Temperature |
–30 °C to +55 °C |
| Operating Humidity |
≤95% |
| Packaging Dimensions |
180.0 mm × 123.0 mm × 96.0 mm |
| Product Dimensions |
149.0 mm × 56.6 mm × 50.3 mm ( |
| Gross Weight |
760g |
| Net Weight |
270g |
$2,550.00
LEICA GEOVID R SE 8x42
The binoculars with rangefinder.
The new Geovid R SE 8x42 is a daylight glass with good twilight performance, making it a popular choice for hunters. With its compact dimensions and low weight, this model sits comfortably in the hand, offers a large field of view, and enables fatigue-free observation of stable images. The Geovid R SE models are classics among the Leica rangefinder binoculars, now winning users over with essential product features based on the proven Geovid family. All models are rugged and precise, equipped with must-have functions to meet the demands of modern, ethical hunters. For example, the laser of the Geovid R SE 8x42 measures distances of up to 1500 m, into early twilight.
The essentials:
- Best-in-class optical performance
- Absolutely precise laser rangefinding up to 1500 meters, for a safe shot
- Very steady image and large field of view
- Easy handling
- Particularly light, compact construction
IN THE BOX
- Geovid R SE 8x42, Carrying Case, Carrying Strap, Lens Cleaning Cloth, Quick Start Guide.
$8,999.00
Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope
The Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope is a high-performance imaging solution designed for advanced applications in life sciences, cell culture, and research. Its robust design, advanced optical features, and user-friendly operation make it an essential tool for professionals in clinical and laboratory settings.
Key Features:
- Optical Excellence: Equipped with high-quality infinity-corrected optical systems, including phase contrast objectives, the NIB620 ensures sharp, clear images with enhanced contrast.
- Magnification Range: Offers a magnification range of 40x to 400x with 10x eyepieces and Plan Phase objectives (10x, 20x, 40x) and an infinity Plan 4x objective.
- Eyepieces: Widefield 10x/22mm eyepieces for a broad and comfortable field of view.
- Illumination: Powerful LED illumination with adjustable brightness for even lighting and reduced eye strain.
- Stage: Spacious 250mm x 170mm mechanical stage with smooth X/Y control and a 110mm x 74mm movement range.
- Condenser: Long working distance condenser with phase sliders for optimized light control during observation.
- Ergonomic Design: Features a comfortable viewing angle and intuitive controls for prolonged use in lab settings.
- Camera Compatibility: Includes a trinocular port for digital imaging, making it ideal for documentation and image analysis.
Applications:
- Cell Culture Studies: Perfect for analyzing live cells and monitoring cell cultures in life science research.
- Clinical Diagnostics: Ideal for laboratory research in microbiology, pathology, and cytology.
- Educational Use: Suitable for teaching advanced microscopy techniques in universities and research institutions.
The Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope combines high-quality optics, ergonomic design, and advanced features to deliver precision and reliability for demanding applications.
| Warranty Information | 3-Years Limited Warranty |
|---|---|
| Eyepiece | Extra Wide Field 10x/ 22mm |
| Magnification Range | 10x, 40x, 200x, 400x |
| Objectives | Infinity Plan 4x, Phrase Contrast 10x, 20x, 40x |
| Field of View | 22mm |
| Working Distance | 75mm |
| Illumination | LED |
| Head Type | Inverted Binoculars |
| Focus | Coarse and Fine, Coaxial |
| Condenser | NA 0.3, WD 75 |
| Stage Type | Fixed with Attached Mechnical Slide Holder (250 x 170mm) |
| Stand | Inverted |
| Power Supply | 250v 10A Power cord |
$3,899.00
Nexcope NE620 Trinocular Professional Microscope 40x-1000x
The Nexcope NE620 Trinocular Professional Microscope is a premium optical instrument designed for advanced research and professional applications. Combining precision engineering with user-friendly features, the NE620 delivers exceptional image clarity and versatility, making it an excellent choice for a variety of fields, including biology, materials science, and industrial research.
Key Features:
- Optics: High-contrast NIS infinity plan objectives for outstanding resolution and image quality.
- Magnification: Wide range of magnifications for detailed observation.
- Viewing Comfort: Ergonomically designed viewing head for prolonged usage without discomfort.
- Condenser: Multifunctional condensers support bright field, dark field, and phase contrast observation methods. (Dark field, and phase contrast slider to be purchased separately)
- Illumination: Intelligent brightness control with even, bright illumination to ensure optimal viewing conditions.
Applications:
- Biological Research: Ideal for cellular studies, tissue examination, and live cell imaging.
- Industrial Inspection: Suitable for material analysis, quality control, and failure diagnostics.
- Educational Use: Perfect for advanced teaching in universities and research institutions.
The Nexcope NE620 microscope combines innovative design, superior optics, and versatility, making it a reliable and high-performing solution for professionals and researchers.
| Warranty Information | 3-Years Limited Warranty |
|---|---|
| Eyepiece | Extra Wide Field 10x/ 22mm |
| Magnification Range | 40x, 100x, 400x, 1000x |
| Objectives | NIS Inifnite Plan Achromatic 4x, 10x, 40x, 100x (Oil) |
| Field of View | 22mm |
| Working Distance | 28mm |
| Illumination | 3W LED |
| Head Type | Trinocular |
| Focus | Coarse and Fine, Coaxial |
| Condenser | NA 1.25 |
| Stage Type | Fixed with Attached Mechnical Slide Holder (185 x 142mm) |
| Stand | Curved Arm |
| Power Supply | 250v 10A Power cord |
$649.00
saxon SmartOne Biological Microscope 40x-1600x
The SmartOne Biological Microscope is a reliable and versatile equipment for educational, home schooling, and hobby applications. With its impressive magnification range and precision engineering, this microscope offers exceptional clarity and functionality for various biological studies.
Key Features:
- Magnification: 40x, 64x, 100x, 160x, 400x, 640x, 1000x,1600x
- Binocular Viewing Head: Provides a comfortable, ergonomic experience during prolonged use.
- Eyepieces: Includes 10x and 16x wide-field eyepieces for enhanced viewing flexibility.
- Quadruple Nosepiece: Smoothly rotating nosepiece to easily switch between objectives.
- Achromatic Objectives: 4x, 10x, 40x, and 100x oil immersion for sharp, high-contrast images.
- Stage: Precision mechanical stage measuring 110x125mm for smooth sample positioning.
- Condenser: NA 1.25 Abbe condenser with an iris diaphragm for optimal light control.
- Coarse & Fine Focusing: Ensures detailed observation.
- Illumination: Bright and even LED illumination for detailed observation.
Applications:
- Education: Ideal for home schooling, schools, and universities for teaching cellular biology and microbiology.
- Research: Suitable for biological, medical, and environmental studies requiring high precision.
The saxon SmartOne Biological Microscope combines quality optics, a robust design, and ease of use, making it an excellent choice for both professionals and enthusiasts.
| Warranty Information | 3-Years Limited Warranty |
|---|---|
| Eyepiece | WF 10x/18mm, WF 16x |
| Magnification Range | 40x, 64x, 100x, 160x, 400x, 640x, 1000x, 1600x |
| Objectives | 4x, 10x, 40xR, 100xR |
| Field of View | 18mm |
| Working Distance | 4x @ 37.5mm, 10x @ 6.5mm, 40x @ 0.63mm, 100x @ 0.195mm |
| Illumination | LED |
| Head Type | Binoculars |
| Focus | Coarse and Fine, Coaxial |
| Condenser | 1.25 Abbe |
| Stage Type | Fixed with Attached Mechanical Slide Holder (115 x 125mm) |
| Stand | Arm |
| Power Supply | 250v 10A Power cord |
| Weight | 4kgs |
| Shipping Dimensions | 41 x 34 x 26 cm3 |
| Shipping Weight | 5.2kgs |
$39,000.00
The IRDK14 from PlaneWave Instruments is a precisely engineered optical system designed for high performance in infrared wavelengths. It is an excellent tool for advanced astronomical research and remote sensing applications, offering superior performance for infrared imaging.
IRDK14’s Key Features
Large Aperture and Optimized Focal Ratio
The IRDK14 features a 356 mm aperture and an f/7.2 focal ratio, enhancing its capacity to gather infrared light effectively. This setup is ideal for detailed infrared observations and long-exposure imaging, providing exceptional light-gathering capabilities.
Specialized Optical Design for Infrared
The Dall-Kirkham optical design of the IRDK14 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. The reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), making it well-suited for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, and potential customers are encouraged to contact our technical sales team to discuss UV optimization.
Robust Mechanical Structure
Constructed using carbon fiber, the optical tube of the IRDK14 offers durability and stability with minimal thermal expansion. This design ensures consistent performance under various environmental conditions, making it suitable for intensive scientific applications.
Advanced Thermal Management
The IRDK14 includes cooling fans and a system prepared for Delta-T applications, promoting rapid thermal equilibrium. This feature is critical for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.
Integrated Dew Control
Infrared observations are prone to condensation, but the IRDK14 tackles this with advanced dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces stay clear from dew, maintaining consistent and clear imaging performance.
Application-Specific Benefits
Infrared Astronomy
The IRDK14 excels in infrared astronomy, where its significant aperture and infrared-optimized optics allow for precise observation of celestial objects in infrared light. This capability is essential for studying astrophysical phenomena invisible to the naked eye or standard optical wavelengths.
Advanced Research and LIDAR Applications
With its specialized design and infrared optimization, the IRDK14 is a robust platform for advanced scientific research, including LIDAR and other remote sensing applications.
Key Features Overview
The IRDK14 comes with impressive specifications tailored for infrared optimization:
- Gold-coated mirrors optimized for high reflectivity in infrared wavelengths (ultraviolet optimization available)
- 14-inch (356 mm) aperture
- 2563 mm focal length
- f/7.2 focal ratio
- 282mm back focus from mounting surface
- 70mm image circle
- Rock-solid fused silica mirrors with low thermal expansion
- Lightweight and rigid carbon fiber optical tube assembly
Optical Systems
| Aperture | 356mm (14 in) |
| Focal Length | 2563mm (101 in) |
| Focal Ratio | F/7.2 |
| Central Obstruction | 23.5% by Surface Area: 48.5% by Diameter |
| Back Focus From Mounting Surface | 282mm (11.09 in) |
| Weight | 22kg (48lbs) |
| OTA Length | 889mm (35 in) |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss And Light Shroud |
Secondary Mirror
| Diameter | 165mm (6.5 in) |
| Material | Fused Silica (Quartz) |
| Shape | Spherical |
| Coating | Protected Gold |
Primary Mirror
| Optical Diameter | 355.6mm (14 in) |
| Outer Diameter | 468.3mm (14.5 in) |
| Shape | Prolated Ellipsoid |
| Material | Fused Silica (Quartz) |
| 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 | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror | |
| Wrench Set (5812A35) - Standard hex wrenches (European orders only) |
$7,930.00
Clarity right up to the edge - SWAROVISION Field Flattener
This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.
The result: every detail is instantly captured, producing a perfect image without any distortions.
Maximum contrast - Including HD optics
A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.
The result: an even more lifelike, contrast-rich image.
A complete view - Large field of view and high zoom range
Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.
In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.
Eye relief plus - Large field of view even for spectacle wearers
SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.
The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.
Maximum colour fidelity - Optimised coatings
The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.
The result: even more impressive observing experiences, even in low light.
Ingenious System
The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.
Perfectly designed down to the smallest detail making you equipped for any situation.
Just one hand
When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other.
This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus.
Easy to transport
Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past.
The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.
$6,650.00
Clarity right up to the edge - SWAROVISION Field Flattener
This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.
The result: every detail is instantly captured, producing a perfect image without any distortions.
Maximum contrast - Including HD optics
A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.
The result: an even more lifelike, contrast-rich image.
A complete view - Large field of view and high zoom range
Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.
In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.
Eye relief plus - Large field of view even for spectacle wearers
SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.
The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.
Maximum colour fidelity - Optimised coatings
The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.
The result: even more impressive observing experiences, even in low light.
Ingenious System
The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.
Perfectly designed down to the smallest detail making you equipped for any situation.
Just one hand
When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other.
This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus.
Easy to transport
Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past.
The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.
$4,950.00
Clarity right up to the edge - SWAROVISION Field Flattener
This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.
The result: every detail is instantly captured, producing a perfect image without any distortions.
Maximum contrast - Including HD optics
A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.
The result: an even more lifelike, contrast-rich image.
A complete view - Large field of view and high zoom range
Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.
In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.
Eye relief plus - Large field of view even for spectacle wearers
SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.
The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.
Maximum colour fidelity - Optimised coatings
The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.
The result: even more impressive observing experiences, even in low light.
Ingenious System
The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.
Perfectly designed down to the smallest detail making you equipped for any situation.
Just one hand
When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other. This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus. Easy to transport
Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past. The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.
From $520.00
The Chroma Technology 8nm SII filter is a high-performance narrowband filter designed for astrophotography and scientific imaging. It isolates the Sulfur II (SII) emission line at 672.4nm with an 8nm bandwidth, offering excellent contrast and detail for capturing deep-sky objects, especially emission nebulae.
Crafted with precision, this filter incorporates advanced multi-layer dielectric coatings for outstanding light transmission and durability. Its 8nm design balances light collection and selectivity, effectively reducing light pollution and moonlight interference while allowing more signal for fainter objects. Whether you're imaging in urban environments or under pristine dark skies, the Chroma 8nm SII filter delivers sharp, halo-free results with minimal reflections, making it an essential tool for astrophotographers striving for stunning and detailed imagery.
From $840.00
The Chroma Technology 5nm SII filter is a high-performance narrowband filter designed for astrophotography and scientific imaging. It isolates the Sulfur II (SII) emission line at 672.4nm with a narrow 5nm bandwidth, offering excellent contrast and detail for capturing deep-sky objects, especially emission nebulae.
Crafted with precision, this filter incorporates advanced multi-layer dielectric coatings for outstanding light transmission and durability. Its 5nm design effectively minimizes light pollution and moonlight interference, making it suitable for imaging under a variety of conditions. Whether you're capturing images in urban settings or beneath dark skies, the Chroma 5nm SII filter delivers sharp, halo-free results with minimal reflections, making it a must-have for astrophotographers seeking stunning and detailed imagery.
From $840.00
The 5nm Chroma H-BETA Filter is a high-performance astrophotography tool crafted to capture stunning details in hydrogen-beta emission nebulae. With its precise 5nm bandwidth, this filter isolates the H-Beta spectral line (486.1nm), boosting contrast and revealing intricate structures in faint nebulae like the Horsehead Nebula and the California Nebula.
Built with premium optical coatings, the Chroma H-BETA filter ensures excellent transmission, maximizing light throughput while effectively blocking unwanted wavelengths such as light pollution and moonlight. Its robust design provides exceptional durability, scratch resistance, and consistent performance across a variety of imaging systems.
Whether you’re using a DSLR, CCD, or CMOS camera, the 5nm Chroma H-BETA filter is an ideal choice for astrophotographers aiming to enhance the depth and detail in their deep-sky images. Discover the cosmos with clarity and precision, as only Chroma can provide.
From $1,040.00
The 3nm Chroma H-BETA Filter is a premium astrophotography tool designed for capturing breathtaking details in hydrogen-beta emission nebulae. With a precise 3nm bandwidth, this filter isolates the H-Beta spectral line (486.1nm), enhancing contrast and revealing subtle features in faint nebulae like the Horsehead Nebula and the California Nebula.
Engineered with superior optical coatings, the Chroma H-BETA filter offers exceptional transmission, ensuring maximum light throughput while effectively blocking unwanted wavelengths such as light pollution and moonlight. Its advanced construction guarantees durability, scratch resistance, and unparalleled performance across a wide range of imaging systems.
Whether you're imaging with a DSLR, CCD, or CMOS camera, the 3nm Chroma H-BETA filter is the perfect choice for astrophotographers seeking to unlock new levels of detail in their deep-sky images. Experience the universe with clarity and precision, as only Chroma can deliver.
$1,799.00
Paramount ME II 大型燕尾槽是一款可选配件,它使 Paramount ME II 的 Versa-Plate 能够容纳使用平面波仪器燕尾槽的光学管组件(包括平面波仪器和 Officina Stellare 望远镜)。
大型燕尾榫的额定承载重量为 108 公斤。
总附加重量为 1.5 公斤
该装置包含在多 OTA 安装套件中
$3,670.00
介绍 iOptron 应变波齿轮安装系列的新成员 - AZ/EQ 双安装 HAE29 和 HAE29EC!这些重量轻、有效载荷高的小型巨人将带来前所未有的天文体验。想象一下,安装头重 8 磅,有效载荷能力 29.7 磅,无需笨重的配重或轴。HAE29 运用 iOptron 数十年打造精密安装的经验,将这一愿景变为现实。
HAE29 采用最先进的应变波齿轮技术,用于 RA 和 DEC 机芯,提供无与伦比的重量与有效载荷效率。其黑色阳极氧化全金属 CNC 加工机身不仅外观漂亮,而且坚固耐用,在未来许多年内都能保持最高水平的性能。电子摩擦制动器和断电记忆等独特功能使支架能够安全停止和恢复 GoTo 旋转,或者在突然断电后继续跟踪(无需重新调整并从头开始)。
HAE29 支架可由计算机控制,可通过 Windows PC 的 ASCOM/Commander 或 MacOS 软件的第三方 INDI 驱动程序进行控制;可通过 iOptron Commander Lite 或 SkySafari 等应用程序通过智能手机/平板电脑进行控制;或通过 INDI 驱动程序通过 Raspberry Pi 设备进行控制。
特征
- 先进的谐波齿轮系统技术
- 有效载荷能力为 13.5 千克(29.7 磅),安装重量为 3.7 千克(8.15 磅,包括燕尾鞍座)
- CNC加工
- RA 和 DEC 上均采用独特的摩擦制动器,可在计划内或计划外断电期间安全停止运动
- 360秒档位周期
- Go2Nova® 手动控制器,带有 ~212,000 个对象数据库
- iPolar 电子极轴镜,可轻松、准确地进行极轴校准
- 客户电缆管理系统已准备就绪
- 双鞍座(Vixen 和 Losmandy-D 款式)
- 内置零位搜索和定位器
- 断电位置和位置记忆
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi(通过手动控制器)
- USB 端口用于固件升级和计算机控制
- 便携包
- 两年保修
规格
| 山 | 应变波经纬仪/赤道仪 |
| RA 齿轮系统 | 谐波齿轮 |
| DEC齿轮系统 | 谐波齿轮 |
| 减速比 | 红移 480:1,赤经 360:1 |
| 不含 CW 的有效载荷 * | 29.7 磅(13.5 千克) |
| 安装重量 | 8.15 磅(3.7 千克),含燕尾鞍座 |
| 有效载荷/安装重量 | 3.65 |
| 带 CW 的有效载荷* | 40磅(18公斤) |
| 时期 | 360 秒 |
| 驱动电机 | 步进电机 |
| 结构材料 | 全金属,CNC加工 |
| 外饰 | 阳极氧化黑色 |
| 极地望远镜 | iPolar 电子极轴镜(外置) |
| 液位指示器 | 水准气泡 |
| 控制系统 | GOTONOVA/指挥官 |
| 手持控制器 | Go2Nova® 8409 拥有约 212,000 个对象的数据库 |
| 追踪 | 自动的 |
| 最大回转速度 | 6度/秒 |
| 功耗 | 0.6A(跟踪),1A(GOTO) |
| 力量 | DC12V-5A(5.5/2.5mm DC插头) |
| 交流适配器 | 100V ~ 240V (含,仅限室内使用) |
| 电缆管理 | 准备 DIY |
| 断电刹车 | 电子摩擦制动器 |
| 掉电记忆 | 是的 |
| 无线上网 | 内置 |
| 通信端口 | 是(Wi-Fi 和 USB,通过 HC) |
| 自动导航端口 | 是(兼容 ST-4) |
| 固件升级 | 是的 |
| 燕尾鞍座 | 泼妇与洛斯曼迪 |
| 三脚架 | 选修的 |
| 配重轴 | SS Φ20X200mm, 3/8"-16 螺纹 (可选) |
| 配重 | 10 磅(4.5 千克)(可选) |
| 操作温度 | -20℃~40℃ (手动控制器-10℃~40℃) |
| 保修单 | 两年有限 |
$5,020.00
介绍 iOptron 应变波齿轮安装系列的新成员 - AZ/EQ 双安装 HAE43 和 HAE43EC!这些重量轻、结构紧凑、中等有效载荷的巨无霸将带来前所未有的天文体验。想象一下,安装头重量不到 13 磅,有效载荷能力为 44 磅,无需笨重的配重或轴。利用 iOptron 数十年打造精密安装的经验,HAE43 将这一愿景变为现实。
HAE43 采用最先进的应变波齿轮技术,用于 RA 和 DEC 机芯,提供无与伦比的重量与有效载荷效率。其黑色阳极氧化全金属 CNC 加工机身不仅外观漂亮,而且坚固耐用,在未来许多年内都能保持最高水平的性能。电子摩擦制动器和断电记忆等独特功能使支架能够安全停止和恢复 GoTo 旋转,或者在突然断电后继续跟踪(无需重新调整并从头开始)。
HAE43 支架可由计算机控制,可通过 Windows PC 的 ASCOM/Commander 或 MacOS 软件的第三方 INDI 驱动程序进行控制;可通过 iOptron Commander Lite 或 SkySafari 等应用程序通过智能手机/平板电脑进行控制;或通过 INDI 驱动程序通过 Raspberry Pi 设备进行控制。
特征
- 先进的谐波齿轮系统技术
- 有效载荷能力为 20 公斤(44 磅),支架重量为 5.8 公斤(12.8 磅,包括燕尾鞍座)
- CNC加工
- RA 和 DEC 上均采用独特的摩擦制动器,可在计划内或计划外断电期间安全停止运动
- 270 第二档周期
- Go2Nova® 手动控制器,带有 ~212,000 个对象数据库
- iPolar 电子极轴镜,可轻松、准确地进行极轴校准
- 客户电缆管理系统已准备就绪
- 双鞍座(Vixen 和 Losmandy-D 款式)
- 内置零位搜索和定位器
- 断电位置和位置记忆
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi(通过手动控制器)
- USB 端口用于固件升级和计算机控制
- 铝制手提箱
- 两年保修
| 山 | 应变波经纬仪/赤道仪 |
| RA 齿轮系统 | 谐波齿轮 |
| DEC齿轮系统 | 谐波齿轮 |
| 减速比 | 赤道几内亚 640:1,赤道几内亚 480:1 |
| 不含 CW 的有效载荷 * | 44磅(20公斤) |
| 安装重量 | 12.8 磅(5.8 千克),带燕尾鞍座 |
| 有效载荷/安装重量 | 3.45 |
| 带 CW 的有效载荷* | 55磅(25公斤) |
| 时期 | 270 秒 |
| 驱动电机 | 步进电机 |
| 结构材料 | 全金属,CNC加工 |
| 外饰 | 阳极氧化黑色 |
| 极地观测镜 | iPolar 电子极轴镜(外置) |
| 液位指示器 | 水准气泡 |
| 控制系统 | GOTONOVA/指挥官 |
| 手持控制器 | Go2Nova® 8409 拥有约 212,000 个对象的数据库 |
| 追踪 | 自动的 |
| 最大回转速度 | 6度/秒 |
| 功耗 | 0.7A(跟踪),1.2A(GOTO) |
| 力量 | DC12V-5A(5.5/2.5mm DC插头) |
| 交流适配器 | 100V ~ 240V (含,仅限室内使用) |
| 电缆管理 | 准备 DIY |
| 断电刹车 | 电子摩擦制动器 |
| 掉电记忆 | 是的 |
| 无线上网 | 内置 |
| 通信端口 | 是(Wi-Fi 和 USB,通过 HC) |
| 自动导航端口 | 是(兼容 ST-4) |
| 固件升级 | 是的 |
| 燕尾鞍座 | 泼妇与洛斯曼迪 |
| 三脚架 | 选修的 |
| 配重轴 | SS Φ20X200mm, 3/8"-16 螺纹 (可选) |
| 配重 | 10 磅(4.5 千克)(可选) |
| 操作温度 | -20℃~40℃ (手动控制器-10℃~40℃) |
| 保修单 | 两年有限 |
* 200 毫米,有效载荷重心位于 RA 旋转轴。或者 OTA 尺寸约为 220 毫米。
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