Welcome to The Binocular and Telescope Shop
Main menu
-
Telescopes
- Telescopes
-
Types of Telescopes
-
Celestron Telescope
-
Smart Telescopes
-
Saxon Telescopes
-
Skywatcher Telescopes
-
TeleVue Telescopes
-
Planewave Telescopes
-
Vixen Telescopes
-
TEC Telescopes
-
BORG Telescopes
-
Founder Optics
-
Solar Astronomy
-
Binoculars
- Binoculars
-
Types of Binoculars
-
Vortex Binoculars
-
Nikon Binoculars
-
Swarovski Binoculars
-
Leica Binoculars
-
ZEISS Binoculars
-
Fujinon Binoculars
-
Gerber Binoculars
-
Vixen Binoculars
-
Pentax Binoculars
-
Olympus Binoculars
-
Kite Optics
-
Kowa Binoculars
-
GPO Binoculars
-
Zerotech Binoculars
-
Binocular Accessories
-
Spotting Scopes
- Spotting Scopes
-
ZEISS Spotting Scopes
-
Swarovski Spotting Scopes
-
Leica Spotting Scopes
-
Nikon Spotting Scopes
-
Vortex Spotting Scopes
-
Kowa Spotting Scopes
-
Pentax Spotting Scopes
-
Celestron Spotting Scopes
-
Spotting Scope Accessories
-
Microscopes
- Microscopes
-
Beaver Labs Microscopes
-
Celestron Microscopes
-
Digital Microscopes
-
Microscopes for Children
-
Biological Microscopes
-
Mounts & Tripods
- Mounts & Tripods
-
ZWO Mounts
-
Celestron EQ Mounts
-
iOptron Mounts
-
Vixen Mounts
-
Paramount EQ Mount
-
Saxon Mounts
-
PlaneWave Mounts
-
Skywatcher EQ Mounts
-
Losmandy EQ Mounts
-
Camera Tripods
-
Astro Star Tracker Mounts
-
Mount Accessories
-
Imaging
- Imaging
-
ZWO Cameras
-
QHY Cameras
-
Starlight Xpress
-
FLI Cameras
-
Atik Cameras
-
Pegasus Astro
-
Camera Lenses
-
SBIG Cameras
-
Focusing
-
Imaging Accessories
-
Filters (Imaging)
-
Autoguiding
-
Accessories
- Accessories
-
Eyepieces, Diagonals and Barlows
-
Adapters & Extensions
-
Books & Sky Guides
-
Bags, Cases & Covers
-
Cleaning and Maintanence
-
Collimation
-
Dew Control
-
Dovetail Bars & Plates
-
Filters (Visual)
-
Finderscopes
-
Tube Rings
-
Tele Vue Eyepieces
-
Bintel Eyepieces
-
Celestron Eyepieces
-
Vixen Eyepieces
-
Barlows & Powermates
-
Saxon Eyepieces
-
Eyepiece Kits
-
Diagonals
-
Tools
Your cart
Choose your Location
-
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
Telescopes Perth
Are you looking to buy a telescope in Western Australia? Look no further than Bintel!
For decades, the team here at BINTEL have been supplying telescopes and a myriad range of accessories to our customers in Perth and throughout Western Australia.
On offer are great shipping rates all over Australia and New Zealand, with telescopes and binoculars sent every week. Typically orders of items will be delivered within 3 or 4 business days for metro areas in WA, or 6 to 7 for regional areas.
We specialise in helping beginners choose high quality first telescopes and binoculars, which will last for years and years - our products have been hand-picked by expert staff, all of whom are professional astronomers or birdwatchers. Bintel has been supporting Australian optics enthusiasts for over 40 years.
169 products
169 products
Sort by:
- 特色
- 最相关
- 畅销
- 按字母顺序排序,A-Z
- 按字母顺序排序,Z-A
- 价格,从低到高
- 价格,从高到低
- 日期,从旧到新
- 日期,从新到旧
New from Sky-Watcher - the smallest member of their Esprit range of APO triplet refractors
The Sky-Watcher 70mm Esprit 70EDX Triplet APO Refractor is a professional instrument for the most demanding and exacting astrophotographers. The air spaced apochromatic triplet lenses have exceptional colour correction over the entire visible spectrum there is no chromatic aberration even on bright objects! Knife edge baffles reduce internal reflections and increase contrast, helping to bring out faint structure in deep sky objects.
Main Features:
- Air Spaced 70mm Apochromatic Triplet
- 490mm Focal Length
- Fully multi coated lenses
- Optional 0.92x Reducer Available
In The Box:
- 70/490 Apochromatic Refractor
- Retractable Dew Shield
- D Style dovetail Bar and rings w/handle
- Aluminium Foam-Lined Case
Specifications:
| Optical Design | Airspaced Apochromatic Triplet |
| Aperture | 70mm |
| Focal Length | 490mm |
| Focal Ratio | f/7 |
| Image Height | 44mm |
| Length after Lens Hood Retracted | 368mm |
| Total Length | 420mm |
| Optical Tube Weight | 3.2kg |
$6,999.00
- The Series-5 focuser is a large capacity focuser for use with Alt/Az, or equatorially mounted systems.
- The focuser is capable of lifting 40 lbs (18 kg) with a travel range of 0.6-inches (15,200 microns).
- The Series-5 focuser can be stacked with the Series-5 rotator for a complete focusing rotator solution (combined 2.78″ of occupied backfocus).
- Occupies only 1.675” of backfocus.
- 464.4283 encoder counts per micron
- Controlled via PWI4 software for autofocusing and optional field de-rotation (if using an Alt/Az mounted system).
- Requires the Series-5 Controller.
- Compatible with the DeltaRho 350 and RC700 telescopes.
$2,249.00
Saxon 8 英寸 DeepSky (203/1200)多布森望远镜是您开启天文探险之旅的完美伙伴。这款价格实惠的望远镜配有“抛物面”主镜,可消除球面像差,配有四臂副镜支架,配有精细支架(厚度为 0.5 毫米),可减少衍射尖峰和光损失。
这款望远镜的口径为 203 毫米,焦距为 1200 毫米,管径为 8 英寸。这款望远镜配有优质零件和配件 - 特殊的滚珠轴承结构、Crayford 调焦器、目镜和寻星镜都旨在帮助您获得观察体验。组装后,经过一点练习,您很快就能找到并观察月球的岩石表面、太阳系中的行星以及星团、双星、星云和星系等深空物体。
Saxon 8 英寸 DeepSky 多布森望远镜在组装过程中不需要任何额外的工具,并且使用起来非常简单,是天文学初学者的完美望远镜。
什么是多布森望远镜以及为什么要使用张力控制手柄?
20 世纪 70 年代末,约翰·多布森 (John Dobson) 发明了一种简单而优雅的地平式方位角支架,用于承载牛顿反射镜。多布森式支架望远镜因其结构简单而受到业余天文学家和望远镜制造商的青睐。最简单的多布森式支架由一个盒子组成,该盒子允许光学管组件在高度上旋转,而盒子本身则在底座上以方位角旋转。
多布森式支架通常依靠望远镜光学管上的侧轴承与鞍座上的摩擦材料之间的摩擦力来将光学管固定到位。如果摩擦力太大,望远镜很难移动到视野中心。如果摩擦力太小,望远镜将无法停留在原位。这使得使用多布森式支架时很难稳定望远镜的光学管,尤其是在光学管上添加了寻星镜或目镜等附件时。只要摩擦力大小合适,光学管就能稳定,望远镜就可以保持在所需位置来观察物体,即使在支架旋转时也能保持其位置。
目前可用的稳定多布森式支架上望远镜的装置包括:一个可切片的重物,以平衡望远镜的重量,一个必须调整以抑制望远镜移动的摩擦锁,以及一个连接在望远镜筒和支架之间以辅助稳定的弹簧。
这些装置使用起来很不方便,因为它们没有提供简单且用户友好的方法来调整摩擦力。saxon 张力控制手柄发明的目的是提供一种张力调节器,用户可以轻松转动它来增加或减少张力,从而增加或减少光学管和支架侧板之间的摩擦力。
通过提供这样的张力调节器,望远镜无需保持平衡即可保持在原位。张力调节器可以拧紧,这样光学管就可以保持在原位,但在需要调整光学管的位置时仍然可以移动。或者,张力调节器可以完全拧紧以将光学管锁定在原位。
ZWO FF65 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 FF65 APO 也是您进行目视观察的不错选择。它适合对角线以及各种目镜,可以实现完美对焦,甚至可以用超高倍率目镜观察行星。
望远镜的整体设计紧凑轻巧。OTA 仅重 2 公斤,包括管环和其他配件在内的全套重量为 2.8 公斤。它的光圈为 65 毫米。焦比为 f/6.4,焦距为 416 毫米。与其他 ZWO FF APO 折射镜的四片式结构不同,FF65 APO 是五片式结构,具有两个 ed 玻璃元件,可出色地控制色差和其他像差。
ZWO FF65 APO 支持全画幅成像圈,光点图精细,周边星点畸变小。2.5 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 M68、M54 和 M48 相机适配器,M48 适配器带有 2 英寸内螺纹,可用于安装滤镜。
ZWO FF65 APO主要特点
五重空气间隔 APO 设计 -无需计算后焦
小而圆的星星 -中心 RMS 半径为 2.5 微米
各种适配器 - 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
可选焦距减小器 -
-
ZWO FF65APO 0.75×全画幅减焦镜
$ 349.00
缺货
规格
| 光圈 | 65 毫米 |
| 焦距 | 416毫米 |
| 焦距比 | f/6.4 |
| 图像圈 | 44 毫米 |
| 净重 | 2公斤 |
| 毛重 | 2.8公斤 |
| 尾端螺纹类型 | M68×1-M54×0.75,M54×0.75-M54×0.75,
M54 x 0.75-M48 x 0.75 M48 x 0.75 毫米滤镜螺纹尺寸 |
| 总长度 | 328mm(含1.25英寸目镜支架,防露罩收缩) 360 毫米。(包括 dewshield 签约的 3 件式适配器) 388 毫米(包括完全展开的防露罩时的 1.25 英寸目镜支架) 420 毫米(包括防露罩完全伸展时的 3 件式适配器) |
| 三件式摄影适配器的后端 | M48 x 0.75 |
库存编号:ZWO-FF65-APO
$849.00
You expect nothing less than crystal-clear images in your scope, but what are you going to do with the mount and tripod you already have? Mount it with the saxon 200/1000 DS Astrophotography Newtonian Telescope, that's what!
Combined with the aperture of 200mm and focal length of 1000mm, this scope is great for prime-focus photography. Higher quality images can be achieved with the optional coma corrector.
This model comes in an OTA form for you to use your own mount and telescope; and customise it with your own accessories to start a great viewing sesssion immediately.
The saxon 200DS Astrophotography Newtonian Telescope features the following:
- 200mm aperture
- 1000mm focal length (F/5.0)
- 2" Dual Speed 10:1 focuser
- 9x50 finderscope
- 2" LET 28mm eyepiece.
- 2" to 1.25" adapter.
$4,299.00
New for 2026! Our most popular Smart Telescope for servious observers has been upgraded.
Highlights includes:
- New optics, with a three-group, flat-field apochromatic quadruplet.
- Light baffles to help combat stray light for urban astronomers
- 11-hour battery
- Increased internal storage
- Anti-fog system
- New, full height adjustable tripod
The most affordable premium smart telescope — built for everyone who wants more from the night sky.
Vespera 3 combines a new-generation optical design with all-night endurance and effortless automation. Whether you're under light-polluted skies or a dark rural horizon, it captures more, keeps everything, and asks nothing from you.
Eight reasons to look up.
Edge-to-edge sharpness
A new apochromatic quadruplet design eliminates chromatic aberration and field curvature across the entire frame. Every star — from centre to edge — is sharp.
Clarity even under city skies
Precision-engineered optical baffles suppress stray light before it reaches the sensor. More contrast, deeper objects — even from your backyard.
A full night. Uninterrupted.
11 hours of battery life take you from dusk to dawn without power banks or interruptions. Your session ends when you choose to stop.
Nothing gets lost
115 GB of onboard storage and USB-C transfer at 30 MB/s. Every frame from every session is saved, organised, and ready.
Fields no single shot can cover
Mosaic mode stitches multiple frames automatically — up to 24 megapixels — so you can image entire nebulae, galaxies, and clusters in a single session.
Sky colour — the integrated post-processing studio
Adjust colours, balance, and contrast directly in Singularity. From sensor to final image — no third-party software, no file juggling, no extra steps.
Your AI guide to the sky
LumENS answers your questions, explains what you're observing, and suggests your next target. Astronomy made intuitive from the very first night.
Optics that protect themselves
An integrated humidity and temperature sensor automatically activates the anti-fog system. Your optics stay clear — whatever the conditions.
From urban backyards to remote dark skies
Compact, self-contained, and fully autonomous — Vespera 3 is as comfortable at a remote dark-sky site as it is on a city rooftop.
Technical Specifications
| Aperture | 50 mm |
| Focal length | 245 mm |
| Focal ratio (F/D) | 4.9 |
| Extra feature | Refined field corrector |
| Sensor type | Sony IMX 585 (colour) |
| Resolution | 3840 × 2160 (8.3 MP) |
| Format | 1/1.2" |
| Sensor size | 11.2 × 6.3 mm |
| Pixel size | 2.9 µm |
| Native image resolution | 8.3 MP |
| Max. resolution with CovalENS | 24 MP |
| Native field of view | 2.5° × 1.4° |
| Max. FOV with CovalENS | 4.33° × 2.43° |
| Detail resolution | 2.39 arcsec/pixel |
| Internal storage | 115 GB |
| Display format | JPEG 8-bit |
| Unit images format | FITS 16-bit |
| Pre-stacked images format | TIFF 16-bit |
| Multi-night slots | 15 |
| Battery life | 11 hours |
| External connector | USB Type-C (not included) |
| Dimensions | 48 × 20 × 9 cm |
| Weight | 5 kg |
The universe doesn't wait.
Neither should you.
$1,399.00
- 25th Anniversary Edition Tabletop Dobsonian GOTO with Wi-Fi
- Controlled with SynScan Pro App for iOS and Android
- GOTO via SynScan free app
- DC12V voltage
- Freedom Find dual encoder technology
Celebrate a quarter-century of astronomical excellence with the Sky-Watcher 25th Anniversary 127 Maksutov Virtuoso GTi Tabletop Dobsonian! This special edition telescope combines the compact power of a 127mm Maksutov-Cassegrain optical system with the smart, user-friendly features of the Virtuoso GTi mount. Perfect for both newcomers and seasoned stargazers, this model offers a luxurious, precise, and enjoyable way to explore the cosmos, marking Sky-Watcher’s commitment to innovation and quality over the years.
25th Anniversary Edition 127 VIRTUOSO GTi Maksutov-Cassegrain Tabletop Dobsonian
- 25th Anniversary Edition Tabletop Dobsonian GOTO with Wi-Fi
- Controlled with SynScan Pro App for iOS and Android
- GOTO via SynScan free app
- DC12V voltage
- Freedom Find dual encoder technology
The Sky-Watcher VIRTUOSO GTi 127/1500 Maksutov-Cassegrain Tabletop Dobsonian is a fully automatic telescope ideal for beginners and those who want to get straight to observing. Aligning the mount takes mere minutes with the “Bright Object” alignment mode, and the computerised SynScan system is the ultimate upgrade that allows automatic pointing and tracking of more than 42,000 object in the sky! This means less time spent finding a faint nebula or a distant planet and more time to enjoy observing. Astronomy has never been so easy!
The Maksutov-Cassegrain is a compact and powerful optical design that combines a front meniscus lens and two mirrors. The optical tube is closed by the front meniscus, keeping the mirrors protected from atmospheric agents such as humidity, dust and pollution. The tube is short but the focal length is long allowing high magnification with the standard eyepieces. With maximum practical magnification of 256x , this Sky-Watcher Telescope will reveal details in Saturn’s rings, Jupiter’s bands, the Martian polar ice caps, and the phases of Venus and the moon.
The VIRTUOSO GTi Dobsonian Mount – Wi-Fi-controllable with iOS and Android and compatible with syncs hand controller, allowing it for smooth tracking and alignment. Use Wi-Fi to control the telescope wirelessly with your mobile device; smartphone or tablet.
$2,625.00
For observation of faint nebulae and star clusters in a wide and bright field of view
The 130mm aperture Newtonian reflector with excellent light gathering power is ideal for observation of faint nebulae and star clusters, particularly for beginners who wish to start astronomical life with a large aperture excellent in light gathering power. It is equipped with a motor for tracking.
AP-SM Equatorial mount
The Advanced Polaris (AP) mount is ideal for beginners learning to use an equatorial mount, as well as experienced observers looking for a simple, grab-and-go setup. It securely supports your telescope's optical tube, providing a stable and comfortable observing experience. Thanks to its friction control system, the mount can be quickly and smoothly moved to your target object. A wide range of optional accessories is available to customize the AP mount to suit your observing needs..
R.A. Motor module and STAR BOOK ONE Set
The AP-SM equatorial mount comes equipped with the RA motor module and the STAR BOOK ONE set, which includes the main motor for celestial tracking and the STAR BOOK ONE controller. This set forms the core of the AP mount system. You can customize and expand your setup by adding additional modules to the RA motor module and STAR BOOK ONE base.
Stylish design
The new stylish and compact design helps break the stereotype of astronomical telescopes being bulky and difficult to use. Weighing just 3.6 kg (excluding the counterweight), the mount is lightweight and easy to handle—even with full-scale astronomical telescopes. The power supply, using four AA batteries, is built into the body, and the use of internal electrical contacts eliminates the need for external wiring that was previously exposed.
Friction control system
Simply point the target objects by moving the optical tube by hands. The friction control system allows you to manually point the telescope at the object without using knobs and clamps.
Simple polar alignment
The optional polar meter can be attached on the equatorial mount for simple polar alignment. Even beginners can quickly align polar axis. For precision alignment, the polar axis scope is usually used, but the polar meter can outperforms especially where Polaris is not visible.
Polar alignment scope PF-L
The PF-L polar alignment scope features a three-star alignment system and a built-in dark field illuminator, allowing you to perform polar alignment while looking directly through the scope. The illumination automatically turns off to conserve power.
To complement the PF-L, we provide a free app called "PFL Assist" for smartphones and tablets. This app supports polar alignment by visually indicating the correct star positions within the displayed constellation.
Power supply system focusing on mobility and comfort
The motor module operates with 4 pieces of the AA batteries which are commercially available anywhere easily, not only corresponding to the alkaline battery but also economical rechargeable batteries (Ni-MH, Ni-Cd). For long term use, a commercially available USB external power supply such as USB mobile battery or USB AC adapter can be used connecting to the provided USB Micro-B terminal.
R130Sf Newton reflector
The 130mm aperture newton reflector which is excellent in light gathering power is ideal for observation of faint nebulae and star clusters in a wide and bright field of view.
APP-TL130 tripod
The compact APP-TL130 tripod is adjustable from 60 cm to 130 cm, combining the portability of a photographic tripod with the strength of an astronomical telescope tripod. The tripod’s feet can be switched between rubber pads and metal spikes, preventing damage to floors when used indoors.
Optical tube
| Primary mirror | 130mm parabolic mirror, multicoated |
| Focal length | 650mm (f/5) |
| Resolving power / Limiting magnitude | 0.89 arc sec. / 12.3 |
| Light gathering power | 345x unaided eye |
| Dimensions / Weight | L: 575mm x OD 160mm, 5.3kg (Body 4.0kg) |
| Finder scope | 6x30mm, 7°actual field of view |
Drawtube
| Visual back | 43mm, 42mm for T-ring, 31.7mm push-fit |
| Eyepiece (Dia. 31.7mm) | PL20mm (33x), PL6.3mm (103x) |
Tripod
| Material, Type | Aluminium 3-section leg |
| Dimensions / Weight | L:570⇔1,296mm, H:526⇔1,159mm, closed 598.4mm, Radius: 350⇔710mm, 3.0kg |
Others
| Accessories | Counterweight 1kg x 1 pc., 1.9kg x 1 pc. |
| Photography | Eyepiece projection, prime-focus, afocal imaging. |
| Solar observation | Not possible |
| Total weight | 15.2kg without battery and eyepiece |
Included:
- Optical tube assembly
- AP-SM equatorial mount
- Eyepiece
- APP-TL130 tripod
$1,150.00
For gazing wide and bright field of view, and faint objects like nebulae and star clusters
Featuring excellent rigidity, stability, and portability, the popular PORTA II altazimuth mount with superior 130mm aperture Newtonian reflector outperforms in viewing faint celestial objects like nebulae and star clusters.
This fine optical instrument comes configured with mounting rings, a dovetail plate, and a 6x30 finder with a bracket and shoe. Two 1.25" eyepieces are also included - 1 PL 6mm, and a PL 20mm.
Specifications
| Optical Design | Newtonian reflector |
| Aperture | 130mm |
| Focal Length | 650mm |
| Focal Ratio | f/5 |
| Eyepiece Barrel Diameter | 42 mm - comes with adapter for 1.25" eyepieces |
| Resolving Power | Rayleigh - 0.89 |
| Finderscope | 6 x 30 |
| Mount Type | Porta II altazimuth |
| Optical Tube Dimensions | 16.0 x 57.2 cm |
| Weight (OTA Only) | 4.1 kg |
In The Box
- Vixen Optics R130Sf Telescope with Porta II Mount
- Porta II Mount with Tripod
- 20mm Eyepiece
- 6.0mm Eyepiece
- 6x30 Finderscope w/bracket and shoe
- 1.25" Eyepiece Adapter
- Tube Rings with 155mm Inner Diameter
- Dovetail Tube Plate
At a glance
An ideal telescope for grab and go observing.
The A70Lf refractor is a basic all-around telescope that gives beginners intriguing views of lunar crators and Saturn's rings.
| Feature | Description |
|---|---|
| Friction Stop Motion | Simple and intuitive operation with friction-based motion. The MOBILE PORTA allows free hand movement in vertical and horizontal directions with easy stopping. |
| Dovetail-Plate Attachment | Uses Vixen’s standard dovetail system for quick and easy attachment of different optical tubes. Supports tubes up to 3.5 kg. |
| Accessory Tray | Convenient tray for holding small items such as eyepieces—especially useful during night observations. |
| Slow Motion Control Handles | Full-circle slow motion control for both vertical and horizontal movement. Ideal for high-magnification observing. Handles can be repositioned if needed. |
| Movable Multi-Arm | Multi-arm rotates in 15° increments to prevent interference with the slow motion handles or optical tube. Vertical handle can also be moved horizontally. |
| Foldable Mount Head | Mount head folds for easy storage and transport. It is detachable from the tripod. Best stored in the Tube and Tripod Bag 100 (sold separately). Optical tube must be stored separately. |
Specificstions
| Objective lens | D=70mm, Achromatic, multi-coated |
| Focal length (Focal ratio) | F=900mm (f12.9) |
| Resolving power / Limiting magnitude | 1.66 arc seconds / 11.0 |
| Light gathering power | 100× unaided eye |
| Size / Weight | 76mm dia × 860mm / 2.5kg (Net 1.9kg) |
| Finder scope | 6x24mm, 5 degrees FoV |
Focuser
| Focusing mechanism | Rack-and-pinion type |
| Adapter threads / Visual back | 42mm for T-ring, 317mm push-fit |
| Eyepieces | NPL20mm (45X, 65' field of view), NPL6.3mm (143X, 22' field of view) |
Tripod
| Leg type, material | 2-section aluminum legs with quick-release leg clamps |
| Size | Adjustable from 720mm to 1290mm in length (from 640mm to 1140mm in height), setup radius from 410mm to 700mm |
Others
| Accessories | Erect-image prism 31.7, Allen wrenches 4mm and 3mm |
Others
| Photography | Usable with Prime focus, Eyepiece projection and Aforcal imaging |
|
Solar observation
|
Not available |
| Total weight | 4.9kg (without eyepieces) |
$1,575.00
The easy-to-maintain refractor is an excellent choice for beginners though to experts.
Vixen achromatic objective lens delivers clear images with less colour fringe.
Specifications
| Objective lens, effective aperture | 105mm achromatic, multicoated |
| Focal length | 1000mm |
| Focal ratio | F9.5 |
| Resolving power | 1.1arc seconds |
| Limiting magnitude | 11.9 |
| Light gathering power | 225×unaided eye |
| Focusing mechanism | Rack-and-pinion |
| Finder scope | XY Red dot finder (1×aiming device) |
| Adapter thread / Visual back | 60mm and 42mm for T-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
| Accessories | Tube rings, Dovetail slide bar |
| Photography | Usable with Prime focus, Eyepiece projection and Afocal imaging |
| Solar observation | Available with Sun projection screen set B |
| Dimensions / weight | 1010mm dia. and 115mm long / 4.8kg (Net 3.8kg) |
$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)
$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)
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 |
$1,199.00
Updated DX Model!
Key Features:
- Honders Advanced Catadioptric optical design
- Radiant Aluminium Quartz (RAQ)™ mirror coatings
- Wide-open 250mm focal length
- FAST f/2 focal ratio
- 125mm aperture diameter
- Lightweight 3.8kg
- 16mm image circle
- Collimatable primary mirror cell
- Rear primary mirror heliacal focuser
- Clamshell rings with a V-style dovetail
- Dual finderscope brackets
- 1.25-inch barrel
- Included accessories: 1.25-inch adapter, male and female M42x0.75
adapters, dew shield
This new HAC125DX (Honders Advanced Catadioptric) Minigraph is the smallest, fastest telescope dedicated to astrophotography available today.
This type of telescope, called an astrograph, is designed from the start to take photos of the night sky. You don't look through it, instead it connects to a dedicated astronomy camera from ZWO, QHY and others. This updated "DX" model features a rear focussing mechanism. The 16mm imaging circle well suited for IMX533 and IMX585 based cameras.
It's fast too, at just f/2.0. This means shorter exposure times and you won't even need to worry about autoguiding.
| Optical Specifications | |
|---|---|
| Optical Design | Honders Advanced Catadioptric |
| Mirror Coating | Radiant Aluminum Quartz (RAQ)™ Coatings |
| Reflectivity | 0.94% |
| Mirror Type (Monolithic/Conical/Fused conical) | Mangin |
| Corrector Coating | HTMC™ |
| Glass Type | Borosilicate |
| Primary Aperture (mm) | 125 |
| F/Ratio | 2 |
| Focal Length (mm) | 250mm |
| Image Circle | 16mm |
| Secondary Obstruction by Diameter | 53mm |
| Secondary Obstruction by Area | 0.425 |
| Primary cell supports (how many support points) | Rear Support |
| Optical Quality | Diffraction limited (1/4 wave) |
| Collimatable Cell | Primary |
| Mechanical Specifications | |
| Focuser Type | Primary focus |
| Focuser Size | Primary Mirror Helical |
| Focuser: Dual or Single Speed | Single |
| Compression Ring | No |
| Optical Tube length | 40cm |
| Optical Tube diameter | 16cm |
| Accessories | |
| Included finder | None |
| Mounting Hardware | Clamshell rings with V-style dovetail |
| Additional Accessories | 1.25" & M42x0.75 camera adapters |
| Manual | No |
| Case | No |
| Observational Info | |
| Dawes Limit | 0.93 |
| Rayleigh Limit | 1.12 |
| Limiting Magnitude | 12.96 |
$10,599.00
New Sky-Watcher 150EDX APO Telescope - redesigned body with famous Esprit optics
**Due in late September/August**
Highlights:
- Air Spaced Apochromatic Triplet
- FPL-53 extra low dispersion glass
- Zero detectable colour fringing even on bright objects
- Diffraction limited optics
- Fully multi coated lenses
- 3″ CNC machined 11:1 dual speed linear power focuser – rotatable
- Indexed focuser tube
- Knife-edge baffled system to enhance contrast
The Sky-Watcher 150mm Esprit 150ED Triplet APO Refractor is a high-end instrument for astro-photographers seeking quality images that only a telescope of this size and optical design can produce. It's also ideal for extended visual observations of deep-space objects due to its remarkable contrast and light gathering ability.
The air spaced apochromatic triplet lenses use the remarkable Ohara FPL-53 ED (extra low dispersion) glass, with exceptional colour correction over the entire visible spectrum there is no chromatic aberration even on bright objects! Knife edge baffles reduce internal reflections and increase contrast, helping to bring out faint structure in deep sky objects.
A 2-element field flattener is available separately to iron out the natural off-axis astigmatism and field curvature of the objective lens, leaving a fully corrected 42mm field of view. Designed with photography in mind, it sits on two tracks above and below the barrel to prevent flexure with a heavy camera attached, and is fully rotatable to perfectly frame a target on the sensor.
In The Box:
- 150/1050 Apochromatic Refractor
- Fixed Dew Shield
- 2″ Dielectric Star Diagonal
- 9×50 Right Angled Erect Image Diagonal
- D Style dovetail Bar
- 2″ to 1.25″ Eyepiece Adaptor
- Aluminium Foam-Lined Case
SPECIFICATIONS
| Model | SWESPRIT150 |
| Optical Design | Air spaced Apochromatic Triplet |
| Aperture | 150mm |
| Focal Length | 1050mm |
| Focal Ratio | f/7 |
| Diameter of the corrected field | 40mm |
| Visual Back Focus | 170mm |
| Resolving Power | 0.80″ |
| Stellar Limit Magnitude | 12.9 |
| Highest Practical Magnification | 300X |
| Light gathering power (compared to the unaided eye) | 459 |
| Focuser | 3″ Crayford dual speed with 2″ and 1.25″ adaptor |
| Optical Tube Length | 920mm |
| Optical Tube Weight | 15kg |
$61,199.00
The CDK350 Observatory System from PlaneWave Instruments is a premium setup designed for the astrophotography aficionado and the dedicated astronomy researcher. This system marries the high-performing CDK14 optical tube assembly with the robust L-350 direct-drive mount, creating an unmatched observational platform that excels across a spectrum of applications, from deep celestial studies to sophisticated astrophotography
Key Features of the CDK350 Observatory System
CDK14 Optical Tube Assembly
- Aperture and Focal Length: Boasts a 14-inch aperture and a 2563 mm focal length at an f/7.2 focal ratio, ideal for capturing wide-field views of the cosmos with incredible depth and clarity.
- Advanced Optical Design: Features a Corrected Dall-Kirkham optical design, providing a field free of off-axis coma and astigmatism while achieving a perfectly flat field across a 70 mm image circle, ensuring critically sharp images throughout the entire field.
- High-Quality Construction: Constructed from lightweight yet durable carbon fiber, minimizing thermal expansion and allowing for rapid thermal equilibration, which helps maintain optical precision in fluctuating temperatures.
- Superior Mirrors and Coatings: Fitted with rock-solid fused silica mirrors known for their minimal thermal expansion, paired with premium coatings that enhance light throughput while minimizing stray light for optimal image quality.
- Thermal Management: Integrates an advanced cooling system with multiple fans that promote rapid thermal stabilization, essential for maintaining consistent high-quality imaging during lengthy exposures and minimizing focus shifts caused by temperature variations.
L-350 Direct Drive Mount
- Direct Drive Motors: Features sophisticated direct-drive motors on each axis, ensuring smooth, swift, and near-silent movement of the telescope with zero backlash and zero periodic error, perfect for both tracking celestial objects and quick repositioning.
- High-Resolution Encoders: Comes equipped with high-resolution optical encoders on both axes, delivering precise positioning and movement, which is critical for high-quality astrophotography and detailed celestial research.
- Azimuth Dovetail Balance System: Includes a finely adjustable balance system that enhances the stability and performance of the setup in both alt-azimuth and equatorial configurations, critical for sustained accurate tracking and easing the strain on the mount during prolonged observations.
- Rapid Target Acquisition: Boasts direct-drive motors capable of impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial objects and satellites, vital for dynamic observations and responsive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK350 is a powerhouse for astrophotographers, offering exceptional tracking accuracy and image stability which facilitate capturing breathtaking celestial images with intricate details and vibrant colors.
Astronomy Research
Researchers will find the CDK350 invaluable for its consistent performance and precise data collection capabilities. It serves as a reliable platform for photometry, spectroscopy, and minor planet tracking, providing a robust foundation for scientific exploration and discovery.
Visual Observations
For enthusiasts of visual astronomy, the CDK350 delivers vibrant and detailed views of the universe. Its substantial aperture and high-quality optical components ensure superb viewing of planetary, lunar, and deep-sky objects, enhancing every observational session.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-350 mount in the CDK350 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount System
| Mount Weight | 50kg (110 lbs) |
| Max. Load Capacity | 45 kg (100 lbs) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
Control system
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount to find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter |
Optical Systems
| Aperture | 356mm (14") |
| Focal Length | 2563 mm (101") |
| Focal Ratio | f/7.2 |
| Central Obstruction | 23.5% by surface area; 48.5% of the Primary Mirror Diameter |
| Back Focus | 282 mm (11.09") |
| Weight | 22 kg (48 lbs) |
| Optimal Field of View | 52 mm Image Circle |
Mechanical Structure
| Fork Assembly | L-350 Mount |
| Fork Base | Welded stainless steel torsion box |
| Optical Tube | Carbon fiber truss and light shroud |
| Instrument Payload | 45 kg (100 lbs) |
Motion control
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe. Provides HTTP and ASCOM control interfaces. MaxIm DL is required for camera control when building a pointing model within our PWI4 software. |
Included items
| Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube |
| Flash drive -Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror |
| Hardware - Six 3/8-16 x 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 3/8-16 x 1/4″ washers; One extended length shoulder bolt for RA axis to EQ wedge alignment |
| One 16′ USB cable - To connect the mount to the observatory control computer |
| One 120VAC power cable - To provide power to the mount |
| Standard Allen Key set - For tightening bolts used on the mount |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
| Keller EZ-Saddle (600182) - The Keller EZ saddle comes standard with the L-350 mount |
$53,499.00
The CDK300 Observatory System from PlaneWave Instruments, an elite configuration designed specifically for the astrophotography enthusiast and serious astronomy researcher. This system combines the precision-engineered CDK12.5 optical tube assembly with the robust L-350 direct-drive mount, offering an unparalleled observational experience that excels in a wide array of applications from detailed celestial studies to advanced astrophotography.
Key Features of the CDK300 Observatory System
CDK12.5 Optical Tube Assembly
- Aperture and Focal Length: Features a 12.5-inch aperture and a 2541 mm focal length at an f/8 focal ratio, perfect for capturing deep-sky objects with exceptional depth of field and clarity.
- Advanced Optical Design: Utilizes a Corrected Dall-Kirkham optical design, eliminating off-axis coma and astigmatism while achieving a perfectly flat field across a 52 mm image circle, ensuring sharp and detailed images across the entire field.
- High-Quality Construction: The optical tube is constructed from lightweight and sturdy carbon fiber, reducing thermal expansion and allowing rapid cooling, which maintains optical alignment in varying temperatures.
- Superior Mirrors and Coatings: Equipped with rock-solid fused silica mirrors known for their low thermal expansion, along with high-quality coatings that maximize light transmission and minimize stray light.
- Thermal Management: Incorporates a sophisticated cooling system featuring three rear cooling fans and four boundary layer fans. This setup rapidly achieves thermal equilibrium, essential for maintaining consistent imaging quality during long exposure astrophotography and reducing thermal-induced focus shifts.
L-350 Direct Drive Mount
- Direct Drive Motors: Employs state-of-the-art direct-drive motors on each axis, providing smooth, fast, and ultra-quiet movement of the telescope with zero backlash and zero periodic error.
- High-Resolution Encoders: Integrated high-resolution encoders offer precise positioning, essential for capturing high-quality astrophotography and conducting detailed astronomical research.
- Azimuth Dovetail Balance System: Provides precise center of gravity adjustments, enhancing the stability and performance of the system in both alt-azimuth and equatorial configurations, crucial for maintaining accurate tracking and reducing strain on the mount during extended observations.
- Azimuth Dovetail Balance System: Provides precise center of gravity adjustments, enhancing the stability and performance of the system in both alt-azimuth and equatorial configurations, crucial for maintaining accurate tracking and reducing strain on the mount during extended observations.
- Rapid Target Acquisition: Equipped with direct-drive motors capable of slew speeds up to 50 degrees per second, enabling quick and efficient targeting of celestial objects and satellites, crucial for dynamic observations and time-sensitive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK300 system is a powerhouse for astrophotographers, providing exceptional tracking accuracy and image stability which allow for capturing breathtaking celestial images with intricate details and vibrant colors.
Astronomy Research
Researchers will find the CDK300 invaluable for its consistent performance and precise data collection capabilities. Ideal for photometry, spectroscopy, and minor planet tracking, it serves as a reliable platform for scientific exploration and discovery.
Visual Observations
For those who enjoy visual astronomy, the CDK300 offers vibrant and detailed views of the cosmos. Its large aperture and high-quality optical components make it perfect for viewing planetary, lunar, and deep-sky objects, enriching every observational session.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-350 mount in the CDK300 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount System
| Mount Weight | 50kg (110 lbs) |
| Max. Load Capacity | 45 kg (100 lbs) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
Control System
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount to find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter |
Optical Systems
| Aperture | 318 mm (12.5 inch) |
| Focal Length | 100.04 inch (2541 mm) |
| Focal Ratio | f/8 |
| Central Obstruction | 42% of the primary mirror diameter |
| Backfocus from Mounting Surface | 265 mm (10.445 inch) |
| Backfocus from Racked in Focuser | 183 mm (7.2 inch) |
| Weight | 19 kg (42 lbs) |
| Optimal Field of View | 52 mm image circle |
Mechanical Structure
| Fork Assembly | L-350 Mount |
| Fork Base | Welded stainless steel torsion box |
| Optical Tube | Carbon fiber |
| Instrument Payload | 45 kg (101 lbs) |
Motion Control
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom-designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe. Provides HTTP and ASCOM control interfaces. MaxIm DL is required for camera control when building a pointing model within our PWI4 software. |
Included Items
| Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube |
| Flash drive - Contains PWI4 software for mount control, instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror |
| Hardware - Six 3/8-16 x 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 3/8-16 x 1/4″ washers; One extended length shoulder bolt for RA axis to EQ wedge alignment |
| One 16′ USB cable - To connect the mount to the observatory control computer |
| One 120VAC power cable - To provide power to the mount |
| Standard Allen Key set - For tightening bolts used on the mount |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
| Keller EZ-Saddle (600182) - The Keller EZ saddle comes standard with the L-350 mount |
| One 16′ USB cable - To connect the mount to the observatory control computer |
$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
$4,790.00
Tele Vue 85 OTA 象牙白
Tele Vue-85 兼具口径和小尺寸,是一款出色的“随身携带、无所不能”的跨界仪器 — 当然,它还具有 Tele Vue 品质。凭借 APO 性能和航空便携性,Tele Vue-85 一直让天文学和观鸟爱好者以及评论家们感到欣喜。“令人瞠目结舌的性能提高了高度便携仪器的卓越标准。”《天空与望远镜》杂志对双星、月球细节、深空和摄影的评价为:“真是太棒了!……难以置信!……这景色几乎让我从椅子上跳了下来!……”结论是:“……这是一款极其强大、紧凑的仪器,能够提供令人惊叹的宇宙图像。”
Better View Desired 网站的评论员在总结 Tele Vue 的“体验”时表示,他会选择 Tele Vue-85,“……真正享受活着的鸟类的令人难以置信的美丽……而且,即使是现在,每次我通过一种特殊的传统观鸟镜观察一只鸟时,我都会想:‘我想知道通过 Tele Vue-85 会是什么样子?我想知道这只鸟到底长什么样?’”是的,纯粹享受大自然的美丽,而没有意识到中间的东西。
含软壳
库存编号:WXO-3372
购买 Tele Vue TVP-3373 TV 85 配件套件,可节省 20% 的单独价格
Tele Vue 的新配件套件包括以下物品
EDE-18.2 18.2mm Tele Vue DeLite 目镜
RS3-8003 3 英寸环形安装座
DSF-8002 2" 90° Tele Vue Everbrite - 缎面
ASF-8125 2 英寸 - 1.25 英寸适配器 - 缎面高音镲
| 类型: | APO(双合)折射镜 |
| 元素/组: | 2 / 1 |
| 物镜直径: | 85毫米 |
| 焦距: | 600毫米 |
| 焦距比 (f/): | f/7 |
| 拉管/调焦器 | 2 英寸,Focusmate 双速齿条和小齿轮 |
| 长度 OTA | 484毫米 |
| 对角线长度 | 556 毫米(对角线 2 英寸) |
| OTA 重量/标准配置 (kg) | 2.77公斤 / 3.63公斤 |
| 最大视野(度) | 4.4 度(使用 2 英寸 55 毫米普罗索尔) |
| 建议最大放大倍数 | 225X |
$9,420.00
Tele Vue-NP101is
我们决心让 NP 系列在光学、机械和功能上尽可能完美,以便对最大 50 毫米对角线芯片进行成像,而不会影响其近乎理想的视觉操作。 (审稿人注。)怎么做?通过将为 Tele Vue-60is 开发的成果应用到新的 NP101is 和 NP127is 上,然后继续超越。
NP101(540mm、f/5.4、4”)保留了其光学规格,但采用了重新设计的 4 元件光学系统。更大的后镜头组绝对可以最大程度地减少对角线长度达 50mm 的格式中的晕影。针对这些大型芯片,开发了可选的场校正器,因此新照亮的边缘的角落几乎与场中心一样完美。
接下来,为了充分利用更大的镜头,我们开发了更大的调焦器和拉管,其前孔径为 3 英寸,后孔径为 2.4 英寸。这消除了更大直径会聚光锥的任何限制。我们制造并测试了齿条齿轮调焦器,使其能够承受超过 5 公斤的重量,但仍可通过 10:1 双速小齿轮组件实现极其精细的聚焦控制。这种新的拉管还允许从视觉操作快速切换到成像操作,并允许相机完全旋转而无需改变焦点。此外,它能够校正任何残余焦平面倾斜,并接受我们的数字千分尺的“位置停止”,以实现可重复的焦点测量,精度为 0.0001”。
为了在改变相机方向时保持与光轴的垂直度,拉管上有四个锁定螺钉,可拧紧“成像插入”环上的锥形部分。此插入件带有螺纹,可容纳 Tele Vue 的新型成像系统配件,包括大直径延长管、光学配件以及相机和 CCD 附件,所有附件均带有配合螺纹。
Focusmate 10:1 行星球型缩焦器提供极其灵敏的调焦功能,使用可选的数字测微计套件可以测量到优于 1/10,000" 的精度。此外,可选的 Focusmate 驱动器允许电子马达控制调焦过程。Focusmate 驱动器具有方向按钮和可调速度。轻按按钮可以实现无振动调焦,步长最小约为 0.0005"。Focusmate 驱动器可以通过 Focusmaster 计算机接口进行远程计算机控制。
Tele Vue 以生产“比您想象的还要好”的视觉仪器而闻名。我们的目标是通过我们的成像设备实现同样的目标。我们敬业的当地机械师和内部员工一如既往地致力于实现这些质量和性能目标。
库存编号:NPI-4057
| 类型 | APO(Nagler-Petzval)折射镜(元件/组:4/2) |
| 物镜(毫米) | 101 |
| 焦距(毫米) | 540 |
| 焦距比 (f/#) | 5.4 |
| 镜筒/调焦器 | 2.4 英寸 Focusmate 双速齿条/小齿轮 |
| 长度OTA(毫米) | 648 |
| 重量(OTA) (kg) | 4.8 |
| 最大视野(度) | 5.1(带 2 英寸 41 毫米全景声) |
| 最大建议功率 (x) | 250 |
**Special Price on the BINTEL Display Model! One only available**
Highlights:
- Ideal for visual observation and astrophotography.
- Designed for the amateur astronomer or photographer who wants to view and photograph the moon, planets, and deep sky objects.
- Features FPL53 "super" extra-low dispersion (ED) glass in a fully multicoated apochromatic lens system that corrects for both spherical and chromatic aberrations, astigmatism, and off-axis comas.
- This correction creates a wide flat field of view without distortion and removes the blue-tinted halo effect for true high-contrast color transmission.
- Can accept both 2" and 1.25" eyepieces and accessories for visual use.
- Threads on the drawtube allow direct connection of T-rings and other camera mounts.
A ring spacer placed around the objective lens refines star images beautifully in astrophotography.
In the previous SD81S model, a set of three tiny tin foils are placed around the objective lens as a spacer between the doublet lens. The end of the tin foils protruding over the objective lens obstruct the incoming light. As a result, the protruding tin foils make the light of diffraction of stars chipped radially. Exchanging the tin foils for the spacer ring makes the diffraction of the stars' light equal. It allows you to create more refined and beautiful star images in your astrophotography.
The SD lens suppresses residual chromatic aberration far below the threshold of visibility.
A lens of refracting telescopes has chromatic aberration which is caused by different wavelength of visible light (colors) focusing at different distances. The Vixen SD lenses, made of FPL53 super extra-low dispersion glass, allow for correcting the chromatic aberration over a wide spectrum of light. The SD81SII delivers outstandingly sharp images with high contrast for both visual and photographic applications. Moderately bright F7.7 images will satisfy the most demanding visual astronomer or astrophotographer.
A short optical tube in length is handy for not only visual observation but also astrophotography.
The ED81SII optical tube has a moderate short length to enable you to carry and set it up readily. Also, a lightweight optical tube allows you to balance it with fewer counterweights. The ED81S comes equipped with a metal carry handle and the Vixen standard dovetail slide bar M for quick attaching and detaching. The provided Flip mirror diagonal switches incoming light to allow for using two eyepieces of different magnifications alternately. Also, you can install a camera on the straight side and view an image through an eyepiece on the right-angled side of the flip mirror diagonal.
Full-frame imaging with a DSLR camera.
Using an SD reducer HD kit or an SD Flattener SD kit, which are available optionally, the SD80SII provides an image circle of 44mm, adequate for taking photos with a DSLR camera. (Photo) M8, M20 nebulae taken with Vixen SD81SII with SD reducer HD kit (compound focus 496mm) and Pentax K-1 at ISO1600, 49 minutes exposure.
Optional accessories to expand your pleasure of taking astrophotography.
SD Reducer HD Kit: This kit includes a flattener lens to be combined with a reducer lens for a flat and wide imaging field when you use them with the SD81SII, SD103SII, or SD115SII optical tube. The reducer lens reduces a focal length by 0.7X. Direct Wide Photo Adapter 60DX: It is available for Canon EOS or Nikon DSLR cameras. It is possible to change the orientation of a camera for a framing of the photographic field.
Wide Photo Adapter 60DX
High precision camera adapters for prime focus astrophotography are optionally available for Canon EOS and Nikon. The Wide Photo Adapter 60DX is designed to be an integrated camera mount reducing vignetting to the maximum. They are highly effective with full-frame DSLR cameras, and can be used with SD series refractors (in combination with the SD Reducer HD Kit or SD Flattener HD Kit).
Specifications
| Optical Tube | |
|---|---|
| Objective Lens / Effective Aperture | 81mm SD Apochromat Multi-Coated |
| Focal Length (Focal Ratio) | 625mm (F7.7) |
| Resolution / Limiting Magnitude | 1.43 arc sec., 11.3 mag., 134× unaided eye |
| Dimensions / Weight | Length 585mm, outer diameter 90mm, 3.6kg (main body 2.3kg) |
| Finder Scope | XY Red Dot Finder II (one-power aiming device) |
| Eyepiece / Focuser | |
| Focusing System | Rack and Pinion |
| Threads / Visual Back | Screw-in: 60mm, 42mm T-ring Push-fit: 50.8mm, 31.7mm (with Flip Mirror Diagonal) |
| Eyepiece — SLV20mm | 31×, 97′ actual field of view |
| Eyepiece — SLV5mm | 125×, 24′ actual field of view |
| Tripod | |
| Material / Form | Large hexagonal aluminium two-stage extension legs (one-touch type) |
| Leg Length / Height | 570–1,296mm leg length; 526–1,159mm height (from ground) |
| Overall Length / Setting Radius / Weight | 598.4mm overall; setting radius 350–710mm; 3.0kg |
| General | |
| Main Accessories | Parts case, counterweight 1kg ×1, 1.9kg ×1 |
| Solar Observation | Compatible with Sun Projection Screen Set B (sold separately) — short-term observation only |
| Total Weight | 13.1kg (excluding eyepiece) |
| Set Contents | |
| Included Items | SD81SII OTA, AP Mount, APP-TL130 Tripod, Eyepiece SLV20mm, Eyepiece SLV5mm, Parts Case, Counterweight 1kg ×1, Counterweight 1.9kg ×1 |
$15,049.00
f/2.75.
What used to take a week now takes a night.
The DeltaRho 280 Argus is PlaneWave’s observatory-class wide-field astrograph for serious imagers and sky-survey programmes. Fused silica quartz mirrors, a carbon fibre OTA, and a 55 mm image circle at f/2.75 — 280 mm of aperture that turns nights of integration into a few productive hours.
f/2.75 is not just fast. It is the difference between finishing a target tonight and coming back next month.
13× faster than f/10. Every photon counts more.
At f/2.75, the DeltaRho 280 gathers light 13 times faster than an f/10 instrument of identical aperture. That is not an incremental advantage — it is the difference between a productive one-hour session and a week of cloud-interrupted integration. Research programmes and sky surveys that would otherwise take months become achievable in a single season.
mm image circle — large enough to cover full-frame sensors and beyond, with sharp stars from centre to corner at 4.5 μm RMS or better at 27.5 mm off-axis.
Focus stays locked. All night.
Primary and secondary mirrors are optical-grade fused silica quartz — near-zero thermal expansion, the same material used in premier research observatories. As temperature drops through the night, conventional glass mirrors shift focus. The DR280’s quartz mirrors do not.
Stiff where it matters. Light where it counts.
Carbon fibre delivers exceptional torsional rigidity with minimal mass. At 14.5 kg for a 451 mm OTA, the DR280 is a 280 mm instrument that mounts on observatory-class and high-end portable mounts alike — without needing a counterweight upgrade.
Sensor alignment without shimming or guesswork.
The integrated tip-tilt focal plane adjuster lets you dial in perfect sensor tilt with precision — no shims, no trial-and-error. It is consistent, repeatable, and done in minutes at the start of any session.
The Heart Nebula. In one frame.
The 770.6 mm focal length paired with the 55 mm image circle delivers over 4 degrees of field of view. Large nebula complexes, galaxy groups, and wide-field targets that require mosaics on narrow-field systems fit comfortably into a single frame — or anchor a multi-panel survey.
Dew control built in. Session-ending fog, ruled out.
Integrated dew control heater technology keeps the optical path clear on humid Australian nights. One less cable to run, one less failure point — the DR280 keeps imaging when lesser rigs fog out and call it a night.
Collimation solved. From first session to thousandth.
The DeltaRho 280 ships with PlaneWave’s collimation software that walks you through mirror alignment step by step — no iterative star-testing, no guesswork. Set it once: the rigid carbon fibre structure holds alignment through the night. The low-profile focuser delivers 0.5 inches of travel from a 163 mm back focus distance, giving your imaging train room to breathe.
M51. The Whirlpool Galaxy.
Galaxy arms, tidal bridges, and foreground stars resolved in a single short session. At f/2.75, integration time that would fill a week on a slower system compresses to a few productive hours.
IC 1805. The Heart Nebula.
H-alpha, RGB narrowband composite. The 4-degree–plus field captures the Heart Nebula’s full complex and surrounding star-forming regions in a single pointing — a target that demands a mosaic from slower, narrower systems.
Built for imagers who treat every clear night as a resource. Nothing wasted.
280 mm (11″) aperture with fused silica (quartz) primary and secondary mirrors for temperature-stable performance
f/2.75 focal ratio — 13 times faster than f/10, reducing required integration time dramatically
55 mm image circle at 4.0 μm RMS on-axis and 4.5 μm RMS at the full 27.5 mm off-axis radius
Integrated tip-tilt focal plane adjuster for precise sensor alignment without physical shimming
Carbon fibre optical tube — 451 mm OTA, 14.5 kg total weight for use on observatory-class mounts
Built-in dew control heater and broadband AR coatings (<1% reflection, 400–800 nm) for consistent all-weather performance
4°+ field of view capability with a 55 mm sensor — ideal for large nebula complexes and sky surveys
Compatible with PlaneWave L350 Direct Drive Mount — designed as an integrated professional imaging system
Every number that matters.
Professional imaging. Backed by Australia’s telescope authority.
$9,869.00
The fast SCT, reinvented.
8 inches. f/2.8. Carry-on weight.
The Observable Space FSCT8 is the first native f/2.8 Schmidt-Cassegrain ever built in an 8-inch form factor. A 42 mm image circle, fused silica quartz mirrors, and a 267 mm carbon-fibre OTA under 9 kg — designed from the optical axis out for astrophotographers who demand observatory results without the observatory.
Every clear night is too short. The FSCT8 makes sure you get the most out of every hour of it.
f/2.8 native. The SCT form factor finally fast.
A conventional 8-inch SCT runs at f/10. The FSCT8 runs at f/2.8 natively — no reducer stacks, no optical compromises. That is a 13-fold increase in photon-gathering speed. A four-hour integration target becomes roughly 20 minutes of effective exposure. For imagers working under Australian skies with limited clear nights, this is the most impactful single step up possible.
mm fully illuminated image circle. Sharp stars across the entire field at under 6.2 μm RMS — covering APS-C and most medium-format sensors with no vignetting.
Quartz mirrors. Focus doesn’t move.
Primary (210 mm) and secondary (114 mm) mirrors are both fused silica quartz — the same glass used in research-grade observatories. Near-zero thermal expansion means the focus point does not drift as temperature drops. Your collimation is still correct at 3 am.
267 mm OTA. Fits where full-size SCTs don’t.
The carbon-fibre upper cage is rigid, thermally stable, and keeps total OTA length at just 267 mm. That is shorter than many refractors. It mounts on mid-range equatorial platforms and travels as carry-on — without sacrificing the optical performance of a full 8-inch system.
Flat field. Corner to corner. No caveats.
The 88 mm broadband AR-coated corrector lens flattens the focal plane and holds sub-6.2 μm RMS optical performance across the full 42 mm image circle — from dead-centre to the corner of a full APS-C sensor.
Your full imaging train. No extensions required.
A 100 mm back focus from the mounting surface accommodates camera, filter wheel, electronic focuser, and off-axis guider without extension tubes. The 2.75 μm per arcsecond image scale is matched to modern small-pixel CMOS sensors — making the most of every pixel in the frame.
Purpose-built for imaging. Not retrofitted for it.
Observable Space — the PlaneWave and OurSky collaboration — built the FSCT8 as an imaging instrument from the ground up. Mirror material, corrector geometry, tube construction, back focus distance: every decision serves the astrophotographer. This is not a visual SCT with a reducer bolted on. It is a dedicated astrograph that fits in a carry-on bag.
8-inch aperture. Mid-range mount. Dark-sky remote site. All viable.
At under 9 kg and just 267 mm OTA length, the FSCT8 is mountable on equatorial platforms that a conventional 8-inch SCT with reducer stack would overload. It travels as carry-on, sets up in minutes, and puts professional-grade optical performance within reach of any dark-sky site — no permanent observatory required.
NGC 6992. The Eastern Veil Nebula.
Supernova remnant in Cygnus. Delicate filamentary emission structure that demands long exposures from slower systems resolves here in a fraction of the integration time — f/2.8 working exactly as intended.
M97. The Owl Nebula.
Planetary nebula in Ursa Major, approximately 2,600 light years distant. Extended shell structure and the characteristic owl-eye cavities resolved in a single night — a target that a slow system would need multiple sessions to match.
More signal per hour. Every clear night finally worth the effort.
Native f/2.8 focal ratio — the first fast SCT in an 8-inch system, designed for wide-field deep-sky imaging from the optical axis out
42 mm fully illuminated image circle with optical performance under 6.2 μm RMS across the full field — sharp stars edge to edge
Fused silica (optical-grade quartz) primary (210 mm) and secondary (114 mm) mirrors with enhanced aluminium coatings for temperature stability
Carbon-fibre upper cage construction — 267 mm OTA, under 9 kg total weight for use on mid-range to high-end imaging mounts
88 mm broadband AR-coated corrector lens delivers a flat focal plane and 2.75 μm per arcsecond image scale suited to modern CMOS sensors
100 mm back focus from mounting surface — accommodates cameras, filter wheels, and electronic focusers in a standard imaging train
4°+ field of view with a 42 mm sensor — ideal for large emission nebulae, galaxy groups, and all-sky survey programmes
An Observable Space instrument — the merger of PlaneWave precision optics engineering and OurSky imaging systems expertise, purpose-built for the astrophotographer
Every number that matters.
The fast SCT, reimagined. Backed by Australia’s telescope authority.
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.
Showing 120/169
Explore Related Collections
- Choosing a selection results in a full page refresh.
- Opens in a new window.