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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
Astronomy
579 products
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$2,899.00
高品质光学元件和高清概念
Conquest HDX 的光学卓越性基于 HD 概念:完美平衡的光学系统,结合了精选涂层、镜头和精细调整的光学设计。它可实现 90% 的透光率,从而获得最明亮的图像;色彩保真度高,从而获得逼真的图像,不会出现色边和色偏,实现完美识别;边缘到边缘的清晰度高,从而在整个视野范围内获得清晰细致的图像。
坚固耐用的设计
Conquest HDX 可在任何环境下使用,无论是极端温度、潮湿环境还是阳光直射。其耐用、防水和防震的特点归功于其坚固的机械设计和轻质镁合金外壳。此外,它覆盖有保护性橡胶装甲,在任何情况下都能提供完美的抓握力。
精心设计的人体工程学
经过精心设计的人体工程学设计,防滑手柄和平滑精确的调焦轮让长时间观察时也能舒适操作。可调节眼罩和可锁定屈光度设置确保个性化的观看体验。
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
15 ×
有效透镜直径
56 毫米
透光率
90%
出瞳直径
3.7 毫米
暮光因素
29.0
1,000 米(码)处的视野
80 分钟
主观视角
西经 69°
近对焦距离
3.5 米(11.5 英尺)
屈光度调节范围
− 4.0 | + 4.0 dpt
出瞳距离
18 毫米
瞳距
54 – 74 毫米
镜头类型
高清
棱镜系统
阿贝·柯尼希
特征
LotuTec | 充氮
是|是
防水性能
400 毫巴
方面
工作温度
− 20°C | + 63°C
瞳距为 65 毫米时的宽度
145毫米
重量
1.25公斤
长度
210毫米
推出 Fusion 系列,这是 Sky-Watcher 在天文学领域的最新创新,旨在彻底改变您的观星体验。Fusion 系列以高品质 MAK150 为首,将先进功能与用户友好型设计相结合,提供无与伦比的性能和易用性。
Fusion 120i-MAK150 主要特点:
• 轻巧耐用:Fusion 120i 支架重量仅为 8 公斤,便携且坚固,有效载荷能力为 12 公斤。
• 紧凑的尺寸:尺寸为 335 毫米 x 214 毫米 x 467 毫米,该支架非常适合家庭天文台和野外天文学观测。
• 精密工程:Fusion 120i 配备蜗轮蜗杆传动机构,确保精确运动。高度轴和方位轴各有 180 个齿,提供平稳、准确的跟踪。
• GOTO 功能:使用 GOTO 功能彻底改变您的星体导航,使定位天体变得前所未有的简单。
• 支持 Wi-Fi:通过智能手机和平板电脑上的 SynScan Pro APP 和 SynScan APP 无线控制您的望远镜。
• 双轴离合器锁定:具有高度和方位轴的离合器锁定功能,在观察期间提供更好的控制和稳定性。
• 多功能电源:选择内置可充电锂电池(9.6V 4.5Ah)和外部 DC12V-15V 3A 电源以延长使用时间。
• 兼容性:兼容具有 Losmandy 风格燕尾槽和 Vixen 风格燕尾槽的 OTA,确保广泛的可用性。
为什么选择马克苏托夫-卡塞格林(MAK150)?
• 卓越的图像质量:马克苏托夫望远镜采用全球面光学设计和弯月形校正镜头,可提供清晰、高对比度的图像。这种设计可最大限度地减少光学像差,提供更清晰、更详细的天体视图
• 长焦距和锐利的光学性能使“Maks”成为行星和月球观测的完美选择。近距离观察月球上的陨石坑和山脉、土星环、木星的卫星,甚至火星的极地冰盖!
光学规格:
| 光学设计 | 马克苏托夫一卡塞格林 |
| 光学直径 | 150毫米 |
| 焦距 | 1800毫米 |
| 寻星镜 | 8×50 |
| 调焦器直径 | 2英寸 |
| 目镜 | 28 毫米 |
$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)
$3,599.00
规格
| 放大 | 18倍 |
|---|---|
| 物镜直径 | 56 毫米 |
| 线性视场 | 194' |
| 视场角 | 3.7° |
| 眼部舒缓 | 18.0 毫米 |
| 高度 | 8.3 英寸 |
| 宽度 | 6.1 英寸 |
| 重量 | 41.6 盎司 |
| 瞳距 | 56 毫米 - 76 毫米 |
| 近距离聚焦 | 10' |
特征
|
包装内容
- GlassPak™ Pro 双筒望远镜背带
- 舒适颈带
- 测距仪袋
- 物镜盖
- 目镜盖
- 镜头布
保修单
所有 Vortex 产品均享受澳大利亚 Vortex VIP 保修
我们的保修是针对您的,而不是针对我们自己。我们的保修是针对售后您的。
VIP 是对您(我们的客户)的一项非常重要的承诺。如果您的 Vortex 产品损坏或有缺陷,我们将免费维修或更换您的产品,只需将产品寄回给我们即可。无论产品是如何发生的、是谁的错、您在哪里购买,您都可以信赖 VIP 保修,适用于所有步枪瞄准镜、红点瞄准镜、测距仪、双筒望远镜、观鸟镜和单筒望远镜。
- 无限终身保修
- 完全可转让
- 无需填写保修卡
- 无需保留收据
如果您遇到问题,无论原因如何,我们都承诺为您提供帮助。
VIP 保修不涵盖产品的丢失、误用、盗窃或故意损坏。
$1,199.00
Vortex Viper HD 12x50 HD – 顶级光学元件和坚固耐用的结构,极其紧凑、轻巧 – 您还需要什么呢?好吧,也许一条优质胸带可以让您舒适、安全。
Vortex Viper HD 12x50 HD 双筒望远镜是一款光学杰作,为猎人、射手和户外爱好者提供了无需高价的优质选择。高清光学系统提供令人惊叹的分辨率、色彩保真度和边缘清晰度。这是市场上最轻、最紧凑的全尺寸双筒望远镜之一——当装备考虑以克为单位时,这是一个值得注意的特性。包括 GlassPak 胸带,让您的双筒望远镜随时可用,同时提供舒适、安全、无压力的全天携带。
光学特性
高清镜头元件高清(高密度)超低色散玻璃提供令人印象深刻的分辨率和色彩保真度,从而产生高清图像。
XR™ 全多层镀膜专有涂层可在所有空气到玻璃表面通过多层防反射涂层来增加光透射率。
电介质棱镜涂层多层棱镜涂层可提供明亮、清晰、色彩准确的图像。
屋脊棱镜模型上的相位校正涂层可增强分辨率和对比度。
结构特点
屋脊棱镜因其更耐用和更紧凑的尺寸而受到重视。
防水 O 型圈密封可防止湿气、灰尘和碎屑进入双筒望远镜,从而确保在所有环境下提供可靠的性能。
防雾氩气吹扫可防止在很宽的温度范围内内部起雾。
ArmorTek 超硬、防刮涂层可保护外部镜片免受划痕、油污和污垢的侵害。
橡胶护套提供安全、防滑的抓握力和耐用的外部保护。
便利功能
可调节眼罩可上下旋转至精确的中间设置,以最大程度地定制贴合,无论是否戴眼镜都能舒适地观看。
中心调焦轮可同时调节两个双筒望远镜的焦距。
锁定屈光度调节器可根据用户眼睛的差异进行调节。位于右目镜上。
可适应三脚架 兼容三脚架适配器,允许在三脚架或车窗支架上使用。
规格
| 放大 | 12X |
|---|---|
| 物镜直径 | 50 毫米 |
| 线性视场 | 288 英尺/1000 码 |
| 视场角 | 5.5 度 |
| 眼部舒缓 | 16 毫米 |
| 高度 | 6.5 英寸 |
| 宽度 | 5.2 英寸 |
| 重量 | 816克 |
| 出瞳 | 4.2 毫米 |
| 瞳距 | 59-75 毫米 |
| 近距离聚焦 | 8英尺 |
特征
| ArmorTek® | 超硬、防刮涂层可保护外部镜片免受划痕、油污和污垢的侵害。 |
|---|---|
| 多层镀膜 | XR™ 全多层镀膜 |
| 高清镜头元件 | 高清 |
| 相位校正 | 屋脊棱镜模型上的涂层可增强分辨率和对比度。 |
| 橡胶装甲 | 提供安全、防滑的抓握和耐用的外部保护。 |
保修单
我们的保修是针对您的,而不是针对我们自己。我们的保修是针对售后您的。
VIP 是对您(我们的客户)的一项非常重要的承诺。如果您的 Vortex 产品损坏或有缺陷,我们将免费维修或更换您的产品,只需将产品寄回给我们即可。无论产品是如何发生的、是谁的错、您在哪里购买,您都可以信赖 VIP 保修,适用于所有步枪瞄准镜、红点瞄准镜、测距仪、双筒望远镜、观鸟镜和单筒望远镜。
- 无限终身保修
- 完全可转让
- 无需填写保修卡
- 无需保留收据
如果您遇到问题,无论原因如何,我们都承诺为您解决。
VIP 保修不涵盖产品的丢失、误用、盗窃或故意损坏。
$1,999.00
光学性能卓越,得益于佳能 Optron, Inc. 的萤石玻璃元件。精确的光学设计可产生极其清晰的图像,几乎没有色差。
推荐用于星空、星云、星团和行星的观测。
主要特点
- 模块化 BORG 设计
- 复消色差萤石玻璃元件。
- 物镜光学设计:2片2组,萤石元件,复消色差,全镀膜。
- 正立棱镜(包含在内)允许用户观察地面物体和天体。
- 包括 20 毫米和 9 毫米目镜。
- Arca-Swiss 快速释放系统三脚架环。
- 超轻重量962克。
- 物镜和主要部件均由日本制造。
| 产品代码 | 6155 |
|---|---|
| 焦距,毫米 | 250 |
| 焦距比 | f/4.5 |
| 最小长度,mm | 260 |
| 重量,克 | 962 |
| 过滤器尺寸,毫米 | 58 |
$5,925.00
BORG 107FL 望远镜套装 CR 是 BORG 高端望远镜,专为专业天文观测者设计。这款望远镜配备 600 毫米焦距物镜,并采用佳能 Optron, Inc. 的高端复消色差萤石玻璃元件。
与 90FL 相比,107FL 物镜可进一步抑制轴向色差。BORG 107FL 望远镜套装 CR 采用轻巧紧凑的碳纤维镜筒构造。随附 Arca-Swiss 快速释放底板,用于三脚架安装。BORG 107FL 望远镜套装 CR 适用于星空、星云、星团和行星观测。
您可以通过将棱镜和目镜与 BORG 相机安装适配器(单独出售)交换,将该望远镜转换为远摄镜头。
主要特点
- 光学设计中采用了佳能奥普特龙公司的萤石玻璃元件,以实现最佳分辨率和最小轴向色差。
- 物镜光学结构:2 片 2 组,萤石复消色差,全多层镀膜。
- 坚固而美观的碳纤维桶。
- BORG 80Ø 枪管系统。
- 齿条齿轮调焦系统。
- 正立棱镜(包含在内)允许用户观察地面物体和天体。
- 包括 20 毫米和 9 毫米目镜。
- 超轻,仅 3.7 公斤(包括配件)。
- Arca-Swiss 快速释放系统三脚架板。
- 物镜和主要部件均由日本制造。
“CR”代表碳纤维镜筒和齿条齿轮调焦系统。
相机安装适配器和其他相机组件单独出售。
规格
型号名称
BORG 107FL 望远镜套装 CR
产品代码
6207
焦距,毫米
600
焦距比
f/5.6
最小长度,mm
504
重量,克
3700
过滤器尺寸,毫米
82
$2,349.00
180mm/2700mm Skymax 180 Maksutov-Cassegrain OTA – 高性能光学管组件
Sky-Watcher Skymax 180 马克苏托夫-卡塞格林 OTA 望远镜非常适合那些想要升级到更强大望远镜的资深爱好者。更大的口径可以让我们更详细地观察我们的近邻行星,并更清晰地拍摄深空物体的图像。
马克苏托夫-卡塞格林的优势
这种望远镜设计具有将彗形像差降至最低的固有优势。它还呈现出更平坦和更完善的边缘清晰度。星场和星团的广角视图从未如此美丽!
带它到你最喜欢的观赏点
这些光学管组件具有明显的优势,可与不同的支架配合使用。只要有标准适配器,您就应该能够将 OTA 连接到其上。快速释放机制使您能够快速组装管子。它还允许您像在公园散步一样对管子进行细微调整。
| 光学设计 | 马克苏托夫-牛顿 |
| 型号 | SWMAK180-OTA |
| 光圈 | 180毫米 |
| 焦距 | 2700毫米 |
| 调焦器直径 | 1.25英寸 |
| 寻星镜 | 9 x 50毫米 |
| 最高实用功率 | 360x |
| 建议使用 | 先进的 |
| 建议使用 | 高分辨率天文摄影 |
$2,399.00
ZWO FF80 APO 是一款折射式天文照相仪,具有强大的平场光学设计,可为您节省昂贵的平场镜费用。它省去了计算平场镜后焦距和连接各种配件以达到该距离的麻烦。您可以连接任何所需的配件。只要目标聚焦,整个光学系统就可以完美成像。这使整个设置过程更加方便,并节省您的时间,让您更加专注于图像拍摄本身。
ZWO FF80 APO 也是您进行目视观察的不错选择。它适合对角线和各种目镜,可以实现完美对焦,甚至可以用超高倍率目镜观察行星。
该望远镜整体设计紧凑轻便,OTA重量仅为3.9kg,带筒环和其他配件的整套重量为4.7kg,口径为80mm,焦比为f/7.5,焦距为600mm。
ZWO FF80 APO采用3+1四片式镜头结构,包含两片ED玻璃,可有效降低色差,提升清晰度和锐度。支持全画幅成像圈,光点图精细,周边星点畸变小。3英寸刚性调焦器配备新型带刻度360°旋转器和取景器底座。还附带M76、M68、M54和M48相机适配器,M48适配器带有2英寸内螺纹,可安装滤镜。
ZWO FF80 APO主要特点
四重空气间隔 APO 设计 -无需计算后焦
小而圆的星星 -中心 RMS 半径为 3 微米
各种适配器 - M76/ M68/ M54/ M48
双速(1:10)调焦器 -支持细调和粗调
无需单独的场地平整器 -自平整设计
支持全画幅相机 -产生 44 毫米成像圈
焦距缩减器 -
-
FF80APO 0.76X 全画幅减焦镜
$ 449.00
缺货
规格
| 光圈 | 80毫米 |
| 焦距 | 600毫米 |
| 焦距比 | f/7.5 |
| 图像圈 | 44 毫米 |
| 净重 | 3.9公斤 |
| 毛重 | 4.7公斤 |
| 物镜 | 四片式(包括两片 ED 玻璃元件) |
| 尾端螺纹类型 | M76x1-M 68x1、M 68x1- M54x0.75、M54x0.75-M54x0.75、M54x0.74-M48x0.75、(内部有 M48 X0.75 过滤器螺纹) |
| 总长度 | 450mm(含1.25英寸目镜支架,防露罩收缩) 480mm(含防露罩收缩后的4件式适配器) 540 毫米(包括完全展开的 1.25 英寸目镜支架,防露罩) 570 毫米(包括 4 件式适配器,防露罩完全伸展) |
| 4 件式摄影适配器的后端: | M48x0.75 |
库存编号:ZWO-FF80-APO
ZWO FF130APO 是一款折射式天文照相仪,具有强大的平场光学设计,可为您节省昂贵的平场镜费用。它省去了计算平场镜后焦距和连接各种配件以达到该距离的麻烦。您可以连接任何所需的配件。只要目标聚焦,整个光学系统就可以完美成像。这使整个设置过程更加方便,并节省您的时间,让您更加专注于图像拍摄本身。
与 ZWO FF107 APO 相比,ZWO FF130 APO 尺寸更大。光圈大 23 毫米。f7/7 时的焦距也更长,这将产生更高的细节和略高的放大倍数,但视野适合所有深空物体。较长的焦距对行星和较大的深空物体尤其有效,当与更大的 130 毫米光圈结合时,将在合理的时间内提供令人惊叹的细节。
ZWO FF130 APO 采用四片式镜片结构,包含两片 ED 玻璃,可控制色差和其他像差。ZWO FF130 APO 采用自平坦设计,在天文拍摄中具有强大优势。它支持中画幅 60mm 成像圈,具有精细的光点图,外围星星畸变极小,其中心 RMS 半径小于 2 微米。
OTA重量仅为10.5kg,带筒环和其他配件的全套重量为12.5kg。3.4″刚性调焦器配有带刻度的新型360°旋转器和取景器底座。还附带M86、M68、M54和M48相机适配器,M48适配器带有2″内螺纹,可用于安装滤镜。与3″0.7x平场减焦镜一起使用时,望远镜可达到f/5.4的焦比和700mm的焦距,有效减少曝光时间。多功能手柄带有中央插槽,可连接带有M6螺丝孔的M6螺钉。标准KLOsmandy燕尾板,搭配坚固的双环。非常适合观看和拍摄。
ZWO FF130 APO主要特点
四重空气间隔 APO 设计 –无需计算后焦距
小而圆的恒星——中心 RMS 半径小于 2 微米
各种适配器 – M86/ M68/ M54/ M48
双速(1:10)调焦器 –支持细调和粗调
无需单独的场地平整器——自平整设计
支持中画幅相机 -可产生 60 毫米成像圈
焦距缩减器 -
-
FF107APO/FF130APO 0.7×通用减速机
$ 599.00
缺货
规格
| 光圈 | 130毫米 |
| 焦距 | 1000米 |
| 焦距比 | f/7.7 |
| 图像圈 | 60毫米 |
| 物镜 | 四片空气间隔 APO(包括两个 ED 玻璃元件) |
| 净重 | 10.5公斤 |
| 毛重 | 12.5公斤 |
| 尾端螺纹类型 | M86x1-M68x1,M68x1-M54x0.54,
M54x0.75-M54x0.54,M54x0.75-M48x0.75 (内部有 M48 x0.75 滤镜螺纹) |
| 总长度 | 842.5mm(含1.25英寸目镜支架,防露罩已收缩)
1011.5mm(含收缩防露罩的4件式适配器) 889.5 毫米(含 1.25 英寸目镜支架,带防露罩) 1061.5 毫米(包括 4 件式防露罩延长适配器) |
| 四件套摄影适配器 | M48x0.75 |
ZWO FF107 APO 是一款折射式天文照相仪,具有强大的平场光学设计,可为您节省昂贵的平场镜费用。它省去了计算平场镜后焦距和连接各种配件以达到该距离的麻烦。您可以连接任何所需的配件。只要目标聚焦,整个光学系统就可以完美成像。这使整个设置过程更加方便,并节省您的时间,让您更加专注于图像拍摄本身。
ZWO FF107 APO 也是您进行目视观察的不错选择。它适合对角线和各种目镜,可以实现完美对焦,甚至可以用超高倍率目镜观察行星。
该望远镜整体设计紧凑轻便,OTA重量仅为5.7kg,带镜筒环和其他配件的整套重量为6.9kg,口径为107mm,焦比为f/7,焦距为749mm。
ZWO FF107 APO采用3+1四片式结构,包含两片ED玻璃,可有效降低色差,提升清晰度和锐度。支持全画幅成像圈,光点图精细,周边星点畸变小。3英寸刚性调焦器配有新型带刻度的360°旋转器和取景器底座。还附带M86、M68、M54和M48相机适配器,M48适配器带有2英寸内螺纹,可安装滤镜。
ZWO FF107 APO主要特点
四重空气间隔 APO 设计 –无需计算后焦距
小而圆的恒星——中心 RMS 半径为 3 微米
各种适配器 – M86/ M68/ M54/ M48
双速(1:10)调焦器 –支持细调和粗调
无需单独的场地平整器——自平整设计
支持全画幅相机 -产生 44 毫米成像圈
焦距缩减器 -
-
FF107APO/FF130APO 0.7×通用减速机
$ 599.00
缺货
规格
| 光圈 | 107 毫米 |
| 焦距 | 749毫米 |
| 焦距比 | f/7 |
| 净重 | 5.7公斤 |
| 毛重 | 6.9公斤 |
| 图像圈 | 44 毫米 |
| 物镜 | 四重空气间隔透镜(包括两个 ED 玻璃元件) |
| 尾端螺纹类型 | M86x1-M68x1,M68x1-M54x54x0.75,
M54x0.75 - M542x0.75,M52x0.75 - M48x0.75 (带 M48x0.75 滤镜螺纹) |
| 总长度 | 602mm(含2英寸目镜支架,防露罩收缩)
655mm(含收缩防露罩的4件式适配器) 754 毫米(包括可延伸的 2 英寸目镜支架和防露罩) 806 毫米(包括 4 件式防露罩延长适配器) |
| 四件套摄影适配器 | M48x0.75 |
库存编号:ZWO-FF107-APO
$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)
$69.00
We offer secondary flat mirrors to match the complete telescope set request, our elliptic flat mirror has the same high optical quality of our parabolic primary mirrors. All mirrors have an enhance aluminum reflective coating, reflectivity is approximately 93%. The aluminum coating is protected by a properly applied protective coating (SiO2). Any custom made flat mirrors should be welcome!
Specifications:
| Item No. | Aperture | F/Ratio | Thickness | Material | PS. |
| AD041 | 28mm | Flat | 8mm | BK7 | Elliptic |
| AD012 | 31mm | Flat | 10mm | BK7 | Elliptic |
| AD046 | 46mm | Flat | 10mm | BK7 | Elliptic |
| AD007 | 50mm | Flat | 10mm | BK7 | Elliptic |
| AD047 | 62mm | Flat | 10mm | BK7 | Elliptic |
| AD091 | 68mm | Flat | 12mm | BK7 | Elliptic |
| AD009 | 70mm | Flat | 12mm | BK7 | Elliptic |
| AD092 | 74mm | Flat | 12mm | BK7 | Elliptic |
| AD091 | 80mm | Flat | 20mm | BK7 | Elliptic |
| AD037 | 88mm | Flat | 20mm | BK7 | Elliptic |
| AD018 | 104mm | Flat | 20mm | BK7 | Elliptic |
| AD077 | 120mm | Flat | 20mm | Quartz | Elliptic |
$125.00
We offer secondary flat mirrors to match the complete telescope set request, our elliptic flat mirror has the same high optical quality of our parabolic primary mirrors. All mirrors have an enhance aluminum reflective coating, reflectivity is approximately 93%. The aluminum coating is protected by a properly applied protective coating (SiO2). Any custom made flat mirrors should be welcome!
Specifications:
| Item No. | Aperture | F/Ratio | Thickness | Material | PS. |
| AD041 | 28mm | Flat | 8mm | BK7 | Elliptic |
| AD012 | 31mm | Flat | 10mm | BK7 | Elliptic |
| AD046 | 46mm | Flat | 10mm | BK7 | Elliptic |
| AD007 | 50mm | Flat | 10mm | BK7 | Elliptic |
| AD047 | 62mm | Flat | 10mm | BK7 | Elliptic |
| AD091 | 68mm | Flat | 12mm | BK7 | Elliptic |
| AD009 | 70mm | Flat | 12mm | BK7 | Elliptic |
| AD092 | 74mm | Flat | 12mm | BK7 | Elliptic |
| AD091 | 80mm | Flat | 20mm | BK7 | Elliptic |
| AD037 | 88mm | Flat | 20mm | BK7 | Elliptic |
| AD018 | 104mm | Flat | 20mm | BK7 | Elliptic |
| AD077 | 120mm | Flat | 20mm | Quartz | Elliptic |
Celestron 照明 RACI 寻星镜
Celestron 照明 RACI 寻星镜是对大多数施密特-卡塞格林望远镜的常规寻星镜的重大升级。50 毫米光学元件可产生明亮、清晰的图像,放大倍数为 9 倍,视场角为 5º。同时,直角、正确图像设计可使物体保持正面朝上,左右正确。您将享受能够在宽阔的视野中定位和跟踪物体的不同之处。目镜模块可向左或向右旋转,以便您找到完美的视角。
与单十字线目镜不同,双十字线标线不会遮挡视野中心的目标。无论您是校准电脑望远镜还是自行寻找深空物体,双十字线标线都可以独立对焦,不受取景器本身的影响。电池供电的照明器会以柔和的红光照亮十字线,并且可以通过转动开/关旋钮轻松调节照明。
Celestron 9x50 RACI 寻星镜配有坚固的支架,由两个环和一个集成燕尾槽组成。使用超大号翼形螺钉可以轻松调整寻星镜的对准度。燕尾槽可以轻松安装和拆卸大多数施密特-卡塞格林和 EdgeHD 光学镜筒组件(包括 NexStar 和 Evolution 系列),而不会影响寻星镜的对准度。
| 光圈 | 50毫米(1.97英寸) |
| 放大 | 9倍 |
| 最高有用放大倍数 | 118x |
| 最低有用放大倍数 | 7.14x |
| 限制恒星星等 | 11 |
| 分辨率(瑞利) | 2.79 角秒 |
| 解析度(道斯) | 2.32 角秒 |
| 聚光能力(与人眼相比) | 51x |
| 视场 | 5° |
| 重量 | 24 盎司(680 克) |
| 外部长度 | 191毫米(7.5英寸) |
| 外部高度 | 140毫米(5.5英寸) |
From $249.00
Shroud
Crafted from premium Nylon/Lycra blended materials, the Hubble Shroud is a must-have for any Dobsonian. It keeps stray light out, reduces thermal currents around the tube, and helps protect your optics during transport or storage. Free shipping is included when purchased with your telescope.
Mirror Cover
Protect your primary mirror with this durable, high-quality plastic cover. It fits snugly over the mirror cell to shield the optics from dust, debris, and accidental contact when the telescope is not in use.
Light Baffle
The Hubble Light Baffle reduces stray and scattered light, improving contrast and detail in your night sky views. Designed to integrate seamlessly with the telescope tube, it is an essential addition for observing faint deep-sky objects or working under bright skies.
Note: Telescope not included.
$59.00
The TMB Super Plossl Series
The TMB Super Plossl series is a clear upgrade over the basic eyepieces supplied with most telescopes, offering sharper images, better contrast, and improved build quality at an accessible price point.
Using a classic 4 element Plossl optical design and a 50 degree apparent field of view, these eyepieces deliver bright, well corrected views across the field. Fully multi coated optics enhance light transmission and reduce internal reflections, helping planetary detail stand out more clearly and deep sky objects appear cleaner and more defined compared to standard kit eyepieces.
Each eyepiece features a standard 1.25 inch barrel with filter threads, solid metal construction, and protective caps, making them a dependable addition to any observing kit.
The TMB 40mm Super Plossl
The 40mm TMB Super Plossl provides the lowest magnification in the range, producing bright, relaxed views that are well suited to large extended objects and longer focal length telescopes.
Eye relief is very generous, offering a comfortable viewing experience.
This focal length is particularly useful when a softer, lower power view is preferred or when maximising brightness for faint, diffuse targets.
$49.00
The TMB Super Plossl Series
The TMB Super Plossl series is a clear upgrade over the basic eyepieces supplied with most telescopes, offering sharper images, better contrast, and improved build quality at an accessible price point.
Using a classic 4 element Plossl optical design and a 50 degree apparent field of view, these eyepieces deliver bright, well corrected views across the field. Fully multi coated optics enhance light transmission and reduce internal reflections, helping planetary detail stand out more clearly and deep sky objects appear cleaner and more defined compared to standard kit eyepieces.
Each eyepiece features a standard 1.25 inch barrel with filter threads, solid metal construction, and protective caps, making them a dependable addition to any observing kit.
The TMB 12mm Super Plossl
The 12mm TMB Super Plossl offers an excellent balance between magnification and comfort. It performs well on the Moon, planets, and smaller deep sky targets while remaining easy to use.
Eye relief is noticeably more comfortable than shorter focal lengths, making it well suited for extended viewing sessions.
For many telescope setups, the 12mm represents a very useful medium high power that will see regular use across a wide range of targets.
$99.00
TMB PlanetView Planetary Eyepieces:
The TMB PlanetView Planetary Eyepiece series is designed for high-magnification planetary and lunar observing, delivering sharp, high-contrast views with excellent eye comfort. Choosing the right focal length for your telescope typically provides a significant upgrade in magnification and fine detail compared to the stock eyepieces supplied with most telescopes, making planetary features clearer and easier to observe. Featuring a 5-element optical design and a wide 58° apparent field of view, these eyepieces offer a more immersive experience than traditional narrow-field planetary designs while maintaining the crisp detail needed for serious observing.
Fully multi-coated optics and internal baffling maximise light transmission and suppress stray reflections, improving contrast on subtle planetary features and fine lunar detail. The large eye lens and generous eye relief make these eyepieces comfortable to use, especially during long observing sessions or when wearing glasses.
Built with an all-metal housing and a fold-down rubber eyecup, TMB PlanetView eyepieces are robust, practical, and compatible with all standard 1.25" focusers and filters. They are also Bintel’s number one recommended first upgrade for most telescopes, offering one of the simplest and most noticeable improvements you can make to planetary and lunar performance.
The 3.2mm TMB PlanetView:
The TMB PlanetView 3.2mm Planetary Eyepiece is ideal for high-power planetary observing with short to medium focal length telescopes.
Works particularly well with:
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Celestron StarSense Explorer DX 130AZ Newtonian Telescope
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Celestron StarSense Explorer 130mm Tabletop Dobsonian Telescope
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Specs:
| Specification | Details |
|---|---|
| Optical design | 5 elements |
| Apparent field of view | 58° |
| Focal length | 3.2mm |
| Barrel size | 1.25" (31.75mm) |
| Eye relief | 16mm |
| Eye lens diameter | 21mm |
| Lens coatings | Fully multi-coated |
| Internal baffling | Yes |
| Eyecup | Fold-down rubber |
| Filter thread | Standard 1.25" |
| Body material | Metal |
| Included accessories | Front and rear lens caps |
From $4,890.00
Hubble UL12 – 12" Lightweight Reflector Telescope
Hubble UP12 – An Ultra-Portable 12" Dobsonian Telescope
The Hubble UP12 is a premium 12-inch Dobsonian designed for observers who want serious optical performance in an exceptionally compact and travel-friendly form. Weighing just 14.5 kg) fully assembled, the UP12 delivers true large-aperture performance in a package that can be transported, stored, and deployed with ease.
Once disassembled, the UP12 can be packed into airline-approved luggage, making it one of the most portable 12-inch telescopes available. This is a genuine “take anywhere” instrument for dark-sky trips, remote expeditions, and observers who value performance without bulk.
Light, Compact and Truly Portable
The UP12 is less than half the weight of a traditional 12-inch Dobsonian. Its modular construction allows the entire system to be assembled in just a few minutes, with no heavy components and no complex setup.
All major structural elements are made from precision-machined aluminium alloy, providing excellent rigidity while keeping weight to an absolute minimum. The result is a telescope that feels effortless to transport, yet remains mechanically stable at high magnifications.
Optical Performance
The UP12 uses a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, delivering high contrast and sharp stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput and reducing scatter. From a dark sky site, the UP12 is capable of revealing most NGC objects, subtle structure in bright nebulae, fine planetary detail on Jupiter and Saturn, and even challenging targets such as the Horsehead Nebula when used with appropriate filters.
A Perfect Balance of Power and Portability
The UP12 gathers around 44% more light than a 10-inch telescope, yet remains dramatically smaller and lighter than traditional 12-inch designs. Its full 12-inch optical surface (with a generous 12.4-inch overall diameter) provides slightly more true light-gathering area than many mass-produced 12-inch mirrors.
This balance makes the UP12 a telescope that actually gets used. It is large enough to deliver meaningful deep-sky performance, yet portable enough to be taken out frequently without hesitation.
Specs:
| Specification | Details |
|---|---|
| Optical design | Reflector |
| Optical diameter | 12" (304.8 mm) |
| Focal length | 1372 mm |
| Focal ratio | f/4.5 |
| Eyepiece height at zenith | ~1320 mm |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | Lightweight low-profile 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 60 mm |
| Secondary mirror obstruction by diameter | 19.7% |
| Secondary mirror obstruction by area | 3.9% |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws all aluminium alloy structure |
| Weight, fully assembled | ~14.5 kg |
| Dawes Limit | 0.38″ |
| Rayleigh Limit | 0.44″ |
| Limiting Magnitude | 14.9 |
| Maximum Magnification | 600× |
| Additional / optional accessories | Red-dot finder 8×50 Finder Tube Shroud Vinyl foam cushioned grips |
| Other features | Stainless steel cable sling lateral support and deluxe push-pull brass knob collimation screws |
$48,290.00
Hubble UL32 – 32" Lightweight Reflector Telescope
The Hubble UL32sg is a flagship 32-inch Dobsonian telescope designed for serious deep-sky observers, research-grade visual work, and advanced EAA applications. With a massive 32-inch primary mirror, the UL32sg delivers 16 times the light grasp of an 8-inch telescope and four times that of a 16-inch, revealing galaxies, nebulae, and fine structure at a level few instruments on Earth can match.
Despite its extraordinary aperture, the UL32sg is engineered to remain as compact and transportable as possible for its class. Fully assembled, the telescope weighs around 150 kg and features a modular, all-metal construction with sectional truss tubes and a folding altitude bearing structure. A real mirror box provides safe protection for the primary mirror during transport and storage.
Light, Strong, Compact and Still Portable
The UL32sg is built using precision-machined aluminium alloy components, extensively modelled with CAD and FEA to optimise structural rigidity while minimising weight. Eight rigid sectional truss tubes ensure excellent stiffness and collimation stability, even at extreme elevations.
While the UL32sg is not a casual backyard instrument, it remains one of the most compact and practical 32-inch class telescopes available, capable of being transported and assembled by a small team for dark-sky expeditions, observatories, and research installations.
Revolutionary Smart Go-To System
The UL32sg is supplied exclusively in a Smart Go-To configuration, built around the state-of-the-art OnStep control system. This advanced platform combines fully motorised Go-To, high-resolution encoders, and a revolutionary plate-solving smart finder for unmatched pointing accuracy.
Using the system is simple: select a target via the smart hand controller or third-party software such as SkySafari or Stellarium, then with a single button press the telescope captures an image, plate-solves its position, and automatically refines its pointing until the target is perfectly centred.
The system supports automated star alignment, automated “Star Shows” such as Messier Marathons, intelligent routing to reduce slewing time by 30–50%, and full EAA live stacking for electronically assisted observing.
Connectivity includes built-in WiFi and Bluetooth, INDI and ASCOM drivers, real-time clock, spiral search, park/unpark, and full sidereal, lunar, and solar tracking rates. Control is available via smart hand controller, desktop software, or mobile apps on Windows, macOS, Linux, iOS, and Android.
Exclusive Sandwich Mirror Technology
The UL32sg uses a lightweight sandwich primary mirror designed to reach thermal equilibrium far faster than traditional solid mirrors. Rapid cooling dramatically reduces mirror seeing and internal turbulence, allowing the telescope to achieve its full optical potential much sooner in real-world conditions.
Unlike thick solid mirrors that may never stabilise during changing temperatures, the sandwich design delivers sharp, stable images without the need for active cooling systems, avoiding vibration and mechanical complexity.
Enhanced Optical Coatings
Both primary and secondary mirrors receive 96% enhanced dielectric coatings with multiple precision-controlled layers. These coatings maximise reflectivity, reduce scatter, and provide excellent chemical and mechanical durability, delivering bright, high-contrast images even at extreme magnifications.
Real Mirror Cell in a Real Mirror Box
The UL32sg features a fully engineered 27-point flotation mirror cell with sling and 90-degree pivoting lateral supports. This system prevents mirror deformation and eliminates astigmatism commonly caused by simpler collimation designs.
The independent three-point rod-end collimation system allows precise adjustment without stressing the mirror edge, maintaining optical integrity under all observing orientations.
Dual-Speed 2" Linear Bearing Crayford Focuser
The UL32sg is fitted with a precision 2-inch dual-speed linear bearing Crayford focuser, capable of handling heavy modern eyepieces and imaging equipment. The fine focus control provides ten times finer adjustment for critical focusing at high power or during EAA use, with approximately 50 mm of travel.
Specifications (UL16)
| Optical design | Reflector |
|---|---|
| Optical diameter | 32" (812.8 mm) |
| Focal length | ~2683 mm |
| Focal ratio | f/3.3 |
| Eyepiece height at zenith | ~2570 mm |
| Optics type | Parabolic |
| Control system | State-of-the-art OnStep Smart Go-To |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 180 mm |
| Secondary mirror obstruction by diameter | 22.1% |
| Secondary mirror obstruction by area | 4.9% |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~2600 mm |
| Weight, optical tube | ~120 kg |
| Weight, fully assembled | ~150 kg |
| Connectivity | Built-in WiFi and Bluetooth |
| Power supply | Control: 12 VDC 2A Motors: 24 VDC 5A |
| Dawes Limit | 0.14″ |
| Rayleigh Limit | 0.17″ |
| Limiting Magnitude | 17.3 |
| Maximum Magnification | 1600× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | 27-point flotation mirror cell sling lateral support deluxe push-pull brass knob collimation screws |
From $21,190.00
Hubble UL24 – A Lightweight 24" Dobsonian Telescope
The Hubble UL24 is a made-to-order 24-inch Dobsonian telescope, designed for experienced observers who want truly extreme aperture without sacrificing transportability.
With a huge 24-inch primary mirror, the UL24 delivers around nine times the light grasp of an 8-inch telescope and four times that of a 12-inch, revealing ultra-faint galaxies, subtle nebular structure, and fine detail in planetary nebulae that smaller instruments simply cannot reach.
Light, Strong, and Surprisingly Portable
The UL24 features a precision-machined all-metal construction with eight rigid aluminium truss tubes and an extremely strong folding altitude bearing structure. Despite its massive aperture, the complete telescope weighs only around 70 kg, making it dramatically lighter than traditional 24-inch Dobsonians.
A real mirror box protects the primary mirror during transport, while the modular design allows the telescope to be broken down into manageable components for storage and travel. The heaviest single component is the primary mirror at around 30 kg, allowing one person to realistically transport the system to dark-sky locations.
Optical Performance
At the heart of the UL24 is a premium parabolic primary mirror with a full 24-inch optical surface and an overall diameter of 24.4 inches. This provides around 4% more true optical area than many other 24-inch designs that use undersized optical surfaces.
Each mirror is individually tested and finished to achieve diffraction-limited performance, with a Strehl ratio of 0.95+ for the primary and 1/10 wave or better for the secondary. Both mirrors receive 96% enhanced reflective coatings, maximising light throughput and contrast while reducing scatter.
The fast f/3.3 focal ratio keeps the eyepiece height to just 1955 mm at zenith, allowing most observers to use the telescope without a ladder while still enjoying extreme aperture.
Choose Your Telescope Control
The UL24 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL24 remains a highly refined Dobsonian with smooth, stable motion and precise balance. Manual observing delivers the classic deep-sky experience at a scale few observers ever reach.
Guided Push-To Version
The Guided Push-To version uses the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution encoders on both axes feed live position data into compatible planetarium software.
Alignment is quick and intuitive using one- or two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices.
Power consumption is extremely low, allowing up to 100 hours of operation from a standard USB power bank. Both WiFi and Bluetooth are supported.
Automatic Go-To Version
The Go-To version adds fully motorised pointing and tracking for hands-free observing. A smart hand controller with a 30,000-object database supports multi-star alignment for highly accurate pointing.
Built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking. The system can be controlled via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android.
Adjustable slew and guide speeds, spiral search, and park/unpark functionality ensure smooth, precise operation during long observing sessions.
| Optical design | Reflector |
|---|---|
| Optical diameter | 24" |
| Focal length | ~2012 mm |
| Focal ratio | f/3.3 |
| Eyepiece height at zenith | ~1955 mm |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality |
Diffraction limited++ (Strehl 0.95+ for primary, 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford |
| Secondary mirror | 127 mm |
| Secondary obstruction (diameter) | 20.80% |
| Secondary obstruction (area) | 4.30% |
| Mirror coatings |
96% Enhanced coating on primary and secondary mirrors |
| Tube material |
6063-T6 aluminium alloy tubes Aluminium alloy OTA & mount Steel mirror cell |
| Weight (optical tube) | ~61 kg |
| Weight (fully assembled) | ~70 kg |
| Dawes Limit | 0.19" |
| Rayleigh Limit | 0.23" |
| Limiting magnitude | 16.4 |
| Maximum magnification | 1200× |
| Optional accessories |
8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features |
Sling lateral support Deluxe push-pull brass knob collimation screws |
From $10,690.00
Hubble UL20 – A Lightweight 20" Dobsonian Telescope
The Hubble UL20 is a made-to-order 20-inch Dobsonian telescope designed for observers who want truly extreme aperture without the bulk and weight of traditional large Dobsonians.
With its enormous 20-inch primary mirror, the UL20 gathers over six times more light than an 8-inch telescope, and almost three times the light grasp of a 12-inch, revealing galaxies, nebulae, and fine structure at a level normally reserved for permanent observatory installations.
A Premium, Light, Compact and Portable Design
Despite its size, the UL20 is engineered to remain practical and transportable. The precision-machined all-metal truss construction delivers exceptional rigidity while keeping overall weight to around half that of traditional 20-inch Dobsonians.
The modular truss design allows the telescope to be broken down for transport, while the reinforced mirror box protects the primary mirror during storage and travel. This makes the UL20 a genuine “portable observatory” for dedicated deep-sky observers.
Optical Performance
At the heart of the UL20 is a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, ensuring excellent contrast and pinpoint stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput while reducing scatter. This results in breathtaking deep-sky views, extremely faint object detection, and exceptional planetary performance even at very high magnifications.
Choose Your Telescope Control
The UL20 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL20 remains a precision Dobsonian with smooth, stable bearings and a well-balanced truss structure. This allows for classic hands-on observing with direct control and intuitive sky navigation.
Guided Push-To Version
The UL20 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time telescope positioning without motorised tracking. High-resolution 8192 PPR encoders on both axes continuously update your telescope’s position in compatible planetarium software.
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Fast one-star alignment, with optional two-star alignment for higher accuracy
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Compatible with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM software
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Works on Windows, macOS, Android, and iOS devices
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Extremely low power consumption, up to 100 hours from a 15,000 mAh USB power bank
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WiFi and Bluetooth supported (WiFi only for iOS devices)
Automatic Go-To Version
The UL20 Go-To version adds fully motorised pointing and tracking for a hands-free observing experience. It includes a smart hand controller with a 30,000-object database and supports advanced 1–9 star alignment for high pointing accuracy.
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Built-in encoders and real-time clock maintain accurate sidereal, lunar, and solar tracking rates
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Control via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI software
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Compatible with Windows, macOS, Linux, iOS, and Android
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Adjustable slew and guide speeds, spiral search, and park/unpark functionality
Choosing Your Focal Ratio: f/3.3, f/3.7 or f/4.2
The UL20 is available in three focal ratios, allowing you to balance comfort, optical performance, and field of view.
Why choose f/4.2?
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Sharper images with almost 50% less coma than f/3.7
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Smaller central obstruction (3.5" secondary vs 4.0" on f/3.7)
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Easier to achieve perfect collimation
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Better suited for high-magnification lunar and planetary observing
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A coma corrector is helpful but not essential for many users
Why choose f/3.3 or f/3.7?
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No ladder required at all for f/3.3; only a small step may be needed for f/4.2 near zenith
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Extremely wide true field of view, especially with f/3.3
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Ideal for sweeping large nebulae and rich Milky Way fields
All three versions deliver extraordinary performance. A coma corrector is strongly recommended for the UL20 f/3.3, while the f/4.2 prioritises optical cleanliness and ease of use.
Thanks to Hubble’s two-section truss design for f/4.2 (single-section for f/3.3 and f/3.7), all versions remain equally rigid and transportable. Please note that counterweights may be required for balance, depending on configuration, and are not included.
Specifications (UL20)
| Optical design | Reflector |
|---|---|
| Optical diameter | 20" (508 mm) |
| Focal length | ~1676 mm (f/3.3) ~1880 mm (f/3.7) ~2134 mm (f/4.2) |
| Focal ratio | f/3.3, f/3.7, f/4.2 |
| Eyepiece height at zenith | ~1490 mm (f/3.3) ~1745 mm (f/3.7) ~2000 mm (f/4.2) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 100 mm (f/3.3 f/3.7) 90 mm (f/4.2) |
| Secondary mirror obstruction by diameter | 19.7% (f/3.3 f/3.7) 17.7% (f/4.2) |
| Secondary mirror obstruction by area | 3.9% (f/3.3 f/3.7) 3.1% (f/4.2) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~1850 mm (f/3.3 f/3.7) ~2110 mm (f/4.2) |
| Weight, optical tube | ~34.5 kg (f/3.3 f/3.7) ~35 kg (f/4.2) |
| Weight, fully assembled | ~40 kg (f/3.3 f/3.7) ~40.5 kg (f/4.2) |
| Dawes Limit | 0.19″ |
| Rayleigh Limit | 0.23″ |
| Limiting Magnitude | 16.4 |
| Maximum Magnification | 1200× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
From $8,090.00
Hubble UL18 – A Lightweight 18" Dobsonian Telescope
The Hubble UL18 is a made-to-order 18-inch Dobsonian telescope, built specifically for serious visual observers who want true observatory-class performance in a portable, transportable design.
With a massive 18-inch primary mirror, the UL18 gathers over five times more light than an 8-inch telescope, and more than twice the light grasp of a 12-inch, unlocking faint galaxies, delicate nebular structure, and extreme planetary detail that simply isn’t possible with smaller apertures.
Light, Strong, and Surprisingly Portable
Each UL18 is custom built to order using precision-machined all-metal components. The truss construction uses eight rigid aluminium truss tubes and a folding altitude bearing structure to provide exceptional stiffness while keeping overall weight under control.
The large mirror box design protects the primary mirror during transport, while the modular layout allows the telescope to be broken down quickly for storage or travel. Fully assembled, the UL18 weighs just ~33 kg, making it one of the most portable 18-inch class Dobsonians available.
Optical Performance
At the heart of the UL18 is a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, ensuring excellent contrast and pinpoint stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput while reducing scatter. This results in brighter deep-sky views, improved low-contrast detail, and excellent planetary performance even at extreme magnifications.
Choose Your Telescope Control
The UL18 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL18 is a precision Dobsonian with smooth, stable bearings and an easy-to-use truss design. You can enjoy the classic hands-on experience, exploring the night sky exactly as the great visual observers have for decades.
Guided Push-To Version
The UL18 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time telescope positioning without motorised tracking. High-resolution 8192 PPR encoders on both axes continuously update your telescope’s position in compatible planetarium software.
-
Alignment is fast and intuitive using a simple one-star alignment, with optional two-star alignment for increased accuracy.
-
Works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices.
-
Extremely low power consumption: up to 100 hours from a 15,000 mAh USB power bank.
-
WiFi and Bluetooth supported (WiFi only for iOS devices).
Automatic Go-To Version
The UL18 Go-To version adds fully motorised pointing and tracking for a completely hands-free observing experience. It includes a smart hand controller with a 30,000-object database and supports advanced 1–9 star alignment for precise pointing accuracy.
-
Built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
-
Control via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android.
-
Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise movement for extended observing sessions.
Choosing Your Focal Ratio: f/4.0 or f/4.5
The UL18 is available in f/4.0 or f/4.5, allowing you to prioritise either maximum comfort or maximum optical refinement.
Why choose f/4.0?
-
Lower eyepiece height – no ladder required for most users
-
More compact overall system
-
Wider true field of view
-
Ideal for observers who value comfort and portability
Why choose f/4.5?
-
Reduced coma across the field
-
Slightly smaller secondary obstruction
-
Better suited to high-power planetary and lunar observing
-
Preferred by observers seeking ultimate optical purity
Both versions deliver extraordinary performance. The f/4.0 favours ergonomic comfort and wide-field observing, while the f/4.5 favours optical cleanliness and contrast. The choice ultimately comes down to observing style and personal preference.
Specifications (UL18)
| Optical design | Reflector |
|---|---|
| Optical diameter | 18" (457.2 mm) |
| Focal length | ~1860 mm (f/4.0) ~2058 mm (f/4.5) |
| Focal ratio | f/4.0, f/4.5 |
| Eyepiece height at zenith | ~1730 mm (f/4.0) ~1930 mm (f/4.5) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 90 mm (f/4.0), 80 mm (f/4.5) |
| Secondary mirror obstruction by diameter | 19.7% (f/4.0), 17.2% (f/4.5) |
| Secondary mirror obstruction by area | 3.9% (f/4.0), 3.0% (f/4.5) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~1830 mm (f/4.0) ~2010 mm (f/4.5) |
| Weight, optical tube | ~28 kg |
| Weight, fully assembled | ~33 kg |
| Dawes Limit | 0.25″ |
| Rayleigh Limit | 0.30″ |
| Limiting Magnitude | 15.8 |
| Maximum Magnification | 900× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
$3,499.95
A new modern large Maksutov telescope for superb viewing and imaging
- 200 mm Maksutov Cassegrain flat field optics Edge to edge sharpness and contrast
- 2000 mm focal length at F10 Large 44 mm image height support
- Optional 0.7x focal reducer compatibility
- Compact well balanced OTA design
Overview
Available May 2026!
Discover why "Maks" are renowned for their sharp imaging and visual observation with the new Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope
The Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope is a premium 200 mm optical system built for astronomers and astrophotographers who want exceptional sharpness, strong contrast, and consistent field flatness across a large image circle.
Designed around an optimised flat field Maksutov Cassegrain layout, the Skymax 200DX delivers clean, accurate performance for detailed visual observation and high resolution imaging.
With an effective aperture of 200 mm and a focal length of 2000 mm at F10, this telescope excels at revealing fine surface detail on the Moon and planets while also delivering strong results on compact deep sky targets. Its advanced optical design helps suppress off axis coma and other aberrations, producing consistent star images from the centre of the field right through to the edge.
For imaging applications, the Skymax 200DX includes a generous 44 mm image height, making it well suited for modern large sensor cameras and full frame astrophotography workflows. For users wanting wider fields and faster exposure times, an optional 0.7x focal reducer is available, expanding flexibility without taking away from the telescope’s refined optical purpose.
Despite its high performance optical profile, the Skymax 200DX remains compact and well balanced, making it a practical option for permanent observatory setups or portable imaging rigs when paired with a suitably rated equatorial mount.
Specifications
| Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope | |
|---|---|
| Optical Design | Maksutov Cassegrain |
| Effective Aperture | 200 mm |
| Focal Length | 2000 mm |
| Focal Ratio | F10 |
| Image Height | 44 mm |
| Optional Focal Reducer | 0.7x |
| OTA Length | 665 mm |
| OTA Diameter | 235 mm |
| OTA Net Weight | 12kg |
From $5,290.00
Hubble UL16 – 16" Lightweight Reflector Telescope
The Hubble UL16 is a made-to-order 16-inch Dobsonian telescope built for serious visual observers who want maximum aperture without sacrificing portability. Combining advanced mirror technology with precision engineering, the UL16 delivers exceptional deep-sky and planetary performance in a surprisingly manageable package.
Optical Performance
At the heart of the UL16 is a full 16-inch parabolic primary mirror featuring Hubble’s exclusive Sandwich Mirror Technology. This lightweight yet rigid design achieves diffraction-limited performance (Strehl 0.95+) while reaching thermal equilibrium up to ten times faster than traditional solid mirrors. Faster cooldown means reduced mirror seeing and sharper, steadier views sooner after setup.
Both primary and secondary mirrors feature 96% enhanced reflective coatings, maximising light throughput and contrast while minimising scatter. The result is brighter galaxies, improved nebular detail, and high-contrast planetary views even at high magnification.
Engineered for Precision
A carefully designed flotation mirror support system combined with independent collimation ensures the primary mirror is evenly supported, minimising astigmatism and maintaining optical accuracy across the sky. The UL16’s robust construction uses CNC-machined aluminium structural components and a steel mirror cell, providing excellent rigidity without unnecessary mass.
Smooth, Accurate Focusing
The UL16 is equipped with a 2-inch dual-speed Crayford focuser featuring linear bearings for smooth, backlash-free operation. Fine focus control allows precise adjustment at high magnifications and works seamlessly with heavy eyepieces or imaging accessories.
Big Aperture, Thoughtful Portability
Despite its impressive aperture, the UL16 is designed with transport in mind. The truss-tube construction breaks down easily for travel, while the fast focal ratios keep eyepiece height within a comfortable range. Whether observing from your backyard or transporting to dark skies, the UL16 balances power with practicality.
Unmatched Observing Potential
With significantly more light-gathering power than a 14-inch telescope, the UL16 reveals faint galaxies, subtle nebular structure, and fine planetary detail that smaller instruments simply cannot match. From resolving globular clusters to tracking delicate dust lanes in distant galaxies, the UL16 is built for observers who want to go deeper.
Push-To and Go-To Options
Guided Push-To Version
The UL16 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution (8192 PPR) encoders on both axes continuously update your telescope’s position in compatible planetarium software.
Alignment is quick and intuitive using a one-star or optional two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices. Power consumption is extremely low, allowing up to 100 hours of operation from a 15,000 mAh USB power bank. WiFi and Bluetooth are supported (WiFi only for iOS).
Automatic Go-To Version
The UL16 Go-To version adds fully motorised pointing and tracking with a smart hand controller featuring a 30,000-object database. Multi-star alignment (1–9 stars) ensures precise pointing accuracy, while built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
Control the system via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android. Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise operation for extended observing sessions.
Choosing Your Focal Ratio: f/5 or f/4.5
The UL16 is available in f/5.0 or f/4.5, allowing you to tailor the telescope to your observing style.
Why choose f/5?
-
Approximately 30% less coma than the f/4.5 version
-
No coma corrector required for most observers
-
Lower cost, saving around $500
-
Smaller central obstruction (2.76" secondary vs 3.1" on f/4.5)
-
Optimised for observers seeking the cleanest possible visual performance
Why choose f/4.5?
-
Lower eyepiece height, no ladder required for most users
-
Wider true field of view, ideal for large nebulae and star fields
-
Slightly more compact overall system
-
Coma is mild and often unnoticed by most observers without a corrector
Both focal ratios deliver outstanding views. The f/5 prioritises ultimate optical cleanliness, while the f/4.5 emphasises comfort and wide-field observing. Thanks to Hubble’s two-section truss design for f/5 (single-section for f/4.5), both versions remain equally portable and rigid.
Please note that counterweights are required for the f/5 configuration and are not included.
Specifications (UL16)
| Optical design | Reflector |
|---|---|
| Optical diameter | 16" (406.4 mm) |
| Focal length | 1829 mm (f/4.5) 2032 mm (f/5) |
| Focal ratio | f/4.5, f/5 |
| Eyepiece height at zenith | ~1690 mm (f/4.5) ~1890 mm (f/5) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 80 mm (f/4.5), 70 mm (f/5) |
| Secondary mirror obstruction by diameter | 19.7% (f/4.5), 17.3% (f/5) |
| Secondary mirror obstruction by area | 3.9% (f/4.5), 3.0% (f/5) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Weight, optical tube | ~25 kg |
| Weight, fully assembled | ~29.5 kg |
| Dawes Limit | 0.29″ |
| Rayleigh Limit | 0.33″ |
| Limiting Magnitude | 15.5 |
| Maximum Magnification | 800× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
$59.99
NBM – Challenger/DX:
nanoblock is a micro sized building block from Japan. Start building on a scale never seen before! This amazingly small micro sized block makes it possible to create detailed masterpieces from tiny animals and miniature musical instruments to architectural landmarks from around the globe. With exciting models to appeal to every personality, nanoblock is sure to captivate builders of all ages.
Features:
- With between 450-800 blocks, each nanoblock Challenger set takes between 90-180 minutes to complete
- Includes detailed colour instructions
- Popular with boys and girls 12+ years
- Loved by the young and young at heart
- Collect them all!
From $4,890.00
Hubble UL14g – 14" Lightweight Reflector Telescope
The Hubble UL14g is a premium 14-inch Dobsonian telescope designed for serious visual observers who want substantial aperture in a system that remains genuinely portable. Combining advanced mirror technology with precision-machined construction, the UL14g delivers impressive deep-sky and planetary performance in a compact, travel-friendly design.
Optical Performance
At the heart of the UL14g is a full 14-inch parabolic primary mirror featuring Hubble’s exclusive Sandwich Mirror Technology. This lightweight yet rigid design achieves diffraction-limited performance (Strehl 0.95+) while reaching thermal equilibrium up to ten times faster than traditional solid mirrors. Faster cooldown means reduced mirror seeing and sharper, more stable views shortly after setup.
Both primary and secondary mirrors feature 96% enhanced reflective coatings, maximising light throughput and contrast while minimising scatter. This results in brighter galaxies, improved nebular structure, and high-contrast planetary detail even at high magnifications.
Engineered for Precision
The UL14g uses a real mirror box and precision flotation mirror support system to evenly distribute load across the primary mirror, minimising deformation and preserving optical accuracy across the sky. The structure is built from CNC-machined aluminium components with a steel mirror cell, providing excellent rigidity while remaining exceptionally lightweight.
Eight rigid truss tubes ensure stable collimation, while the large altitude bearings provide smooth and predictable motion during tracking.
Smooth, Accurate Focusing
The UL14g is equipped with a 2-inch dual-speed Crayford focuser with linear bearings, delivering smooth, backlash-free focusing. Fine focus control makes it easy to achieve critical focus at high power and supports heavy wide-field eyepieces without flex or slippage.
Big Aperture, Exceptional Portability
Despite its 14-inch aperture, the UL14g is remarkably easy to transport and set up. The modular truss-tube design breaks down into compact components that can be assembled in just a few minutes without tools. The heaviest single component is the primary mirror, weighing around 7 kg, making solo transport realistic for most observers.
With its fast f/4.6 focal ratio, the eyepiece height remains accessible at all times — just 60 inches at zenith — allowing comfortable observing with both feet on the ground.
Unmatched Observing Potential
The UL14g collects approximately 36% more light than a 12-inch telescope and nearly double that of a 10-inch, allowing significantly fainter objects and finer details to be resolved. From dense globular clusters to delicate dust lanes in distant galaxies, the UL14g reveals a level of structure that smaller instruments simply cannot match.
From dark-sky sites, most NGC objects are within reach. Bright emission nebulae show subtle hints of colour, planetary nebulae display internal structure, and Jupiter reveals fine banding and atmospheric detail. With an H-beta filter, even challenging targets like the Horsehead Nebula become achievable under good conditions.
The UL14g strikes a rare balance between serious aperture and true portability, making it a telescope that gets used often, not one that stays in storage.
Push-To and Go-To Options
Guided Push-To Version
The UL16 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution (8192 PPR) encoders on both axes continuously update your telescope’s position in compatible planetarium software.
Alignment is quick and intuitive using a one-star or optional two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices. Power consumption is extremely low, allowing up to 100 hours of operation from a 15,000 mAh USB power bank. WiFi and Bluetooth are supported (WiFi only for iOS).
Automatic Go-To Version
The UL16 Go-To version adds fully motorised pointing and tracking with a smart hand controller featuring a 30,000-object database. Multi-star alignment (1–9 stars) ensures precise pointing accuracy, while built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
Control the system via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android. Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise operation for extended observing sessions.
Specifications (UL14)
| Optical design | Reflector |
|---|---|
| Optical diameter | 355.6 mm (14") |
| Focal length | 1635 mm |
| Focal ratio | f/4.6 |
| Eyepiece height at zenith | 1525 mm (60") |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford |
| Secondary mirror size | 70 mm |
| Secondary mirror obstruction by diameter | 19.7% |
| Secondary mirror obstruction by area | 3.9% |
| Mirror coatings / over-coatings | 96% enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 aluminium alloy tubes aluminium alloy structure steel mirror cell |
| Length of optical tube | 1525 mm (60") |
| Weight, optical tube | 18.1 kg (40 lb) |
| Weight, fully assembled | 26.8 kg (59 lb) |
| Built-in WiFi | Yes |
| Power supply | 12–15 V DC 2A centre positive |
| Dawes limit | 0.33″ |
| Rayleigh limit | 0.38″ |
| Limiting magnitude | 15.2 |
| Maximum magnification | 700× |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
$12,499.00
Celestron C14-AF XLT 光学管组件
- 14" 施密特-卡塞格伦光管组件
- 铝光学管
- 兼容 Fastar
- Celestron 的优质 StarBright XLT 涂层
- 焦距 3910 毫米 (f/11)
- 附赠 40 毫米 1.25 英寸目镜 (98x)
- 可视背面允许使用 2 英寸配件
- 9x50 寻星镜帮助准确找到物体
- 2 英寸的镜子对角线可在观察高空物体时提供更舒适的观看位置
- 包括与 CGE 安装座兼容的燕尾导轨
规格
| 光学设计 | 施密特一卡塞格林 |
|---|---|
| 孔径(毫米) | 355.6 毫米(14 英寸) |
| 焦距 | 3910 毫米 |
| 焦距比 | 11 |
| 目镜焦距 | 40 毫米 |
| 目镜放大倍数 | 98 x |
| 寻星镜 | 9x50 |
| 星对角线 | 1.25 |
| 光学筒 | 铝 |
| 兼容 Fastar | 是的 |
| 最高有用放大倍数 | 840 x |
| 最低有用放大倍数 | 51 x |
| 限制恒星星等 | 15.3 |
| 分辨率(瑞利) | 0.39 角秒 |
| 解析度(道斯) | 0.33 角秒 |
| 聚光能力(与人眼相比) | 2581 x |
| 次镜遮挡 | 114 毫米 |
| 次镜直径遮挡 | 32% |
| 次镜遮挡面积 | 10% |
| 光学涂层 | 星光闪耀 XLT |
| 光学管长度 | 787 毫米 |
| 光学筒重量 | 21公斤 |
| 燕尾兼容性 | CGE 安装 |
$1,399.00
借助专为 RASA 设计的这款光污染成像滤镜,即使在光污染的天空下,也能充分利用 Celestron Rowe-Ackermann Schmidt Astrograph 11。无论您使用哪种相机,这款滤镜的宽大 68 毫米通光孔径都使其能够轻松容纳当今最大的传感器。这款滤镜采用机加工铝制外壳和 Schott B270 玻璃,取代了 RASA 的透明光学窗口,因此 RASA 的光学性能不会受到影响。
消除光污染,同时保持图像明亮
光污染限制了我们能够看到和拍摄的夜空范围。在光污染区域使用彩色相机拍摄时,天空辉光会降低图像质量。光污染滤镜有助于选择性地阻挡普通路灯和其他环境照明发出的光线。但大多数光污染滤镜会严重影响总光通量,导致图像暗淡,并对色彩平衡产生负面影响,导致图像显得太绿或太蓝。
RASA 的光污染成像滤镜“精准”地去除了不需要的光污染,同时尽可能多地保留有用的光谱。这意味着您仍将保留望远镜在许多波长下捕获的 90% 以上的光线。
与其他光污染抑制滤镜不同,Celestron LP RASA 成像滤镜保持相对中性的色彩平衡,因此您可以呈现星系和其他暗淡深空物体的微妙色彩。多层特殊配方的介电涂层可提供所需的透射率,而防反射涂层可最大限度地减少星晕和内部反射。
还包括一个透明塑料盒,用于在不使用时保护过滤器
单独质量测试
每个 RASA 11 光污染成像滤镜都经过单独透光测试。包装盒内有一张图表,详细说明了特定滤镜的实际透射光谱。
| 玻璃厚度 | 2.1 毫米 |
| 过滤器直径 | 72 毫米 |
| 通光孔径 | 68 毫米 |
| 涂料 | 硬涂层介电体和多层抗反射涂层 |
| 滤光玻璃 | 肖特B270 |
| 住房 | 阳极氧化铝 |
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