ZWO ASI 533MC Pro
* This product is only for bundle sale. *
The ZWO ASI533MC-Pro is a high-performance cooled color astronomy camera ideal for capturing deep-sky objects, as well as high-resolution images of the Moon, Sun, and planets. Its square-format sensor, advanced cooling system, and innovative design make it a versatile tool for astrophotographers of all levels.
Key Features
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Square 1” Sony IMX533 Sensor
Equipped with a 9-megapixel back-illuminated CMOS sensor with 3008x3008 resolution and 3.76µm pixels, the camera is perfect for framing symmetric celestial objects like star clusters and nebulae. -
Enhanced Image Quality
The back-illuminated design improves sensitivity and reduces noise, with a high quantum efficiency (QE) of 80% and low read noise of just 1.0e. The sensor’s 50,000e full well capacity ensures bright stars remain sharp without saturation. -
Zero Amp Glow
Features advanced circuitry to completely eliminate amp glow, even during long exposures at high gain, resulting in cleaner, more accurate images. -
Efficient TEC Cooling and Anti-Dew Heater
A two-stage TEC cooling system reduces sensor temperature by up to 35°C below ambient, minimizing noise. The heat generated by the cooler also prevents dew formation on the camera window. -
Fast Data Transfer
Includes a 256MB DDR3 memory buffer for stable data transfer and reduced amp glow. The USB3.0 port supports fast data rates of 20 fps at full resolution. -
Dynamic Range and Low-Noise Performance
Offers a dynamic range of up to 14 stops, with optimal performance at a gain setting of 100. This makes it well-suited for electronically assisted astronomy (EAA) and traditional astrophotography.
Compact and User-Friendly Design
The ASI533MC-Pro is ideal for both deep-sky imaging and solar-system photography. Its compact size, powerful cooling, and versatile square sensor make it a perfect choice for astrophotographers seeking excellent performance and reliability in a streamlined package.
- Sensor
- Sony IMX533 CMOS ( color )
- Resolution
- 3008 × 3008
- Pixel Size
- 2.9μm
- Sensor Size
- 1″ ( 11.31 x 11.31mm )
- Max Frame Rate
- 20 fps
- Read Noise
- 1.0e
- Cooling Temp
- △35°C
- Quantum Efficiency
- 80%
- Full Well
- 50ke
- Exposure Range
- 32μs-2000s
- DDR3 Buffer
- 256 MB
- ADC
- 14 bit
- Flange Distance
- 17.5mm
- Camera Thread
- M42
- Adapter Included
- M48 → M42 Adapters ( 0 & 16.5mm )
- M42 Extender ( 21mm )
- M28.5 → M42 Adapter
- 1.25" Nosepiece → M42 Adapter
- Interface
- USB 2.0 Type-A
- USB 3.0 Type-B
- Cable Included
- USB 2.0 Type A↔B ( 0.5m ) x2
- USB 3.0 Type A↔B ( 2m )
- Camera Weight
- 0.457 kg / 1 lbs
Choose options
What's in the box
Camera Body
Camera Bag
M48 → M42
0mm
M48 → M42
16.5mm
M42 Extender
21mm
1.25" → M42
Noisepiece
M28.5 → M42
0mm
USB 2.0 Cable x2
0.5m
USB 3.0 Cable
2m
Spacer x4
Quick Guide
Compact Camera for Deep-Sky & planetary Imaging
One Inch Square Frame
The ZWO ASI533MC-Pro cooled color astronomy camera is equipped with Sony’s CMOS IMX533 1”-format sensor with a square aspect ratio. With a resolution of 9.0 megapixels, this one-shot color camera has large pixels for high signal-to-noise ratio for imaging deep-sky objects. It’s also ideal for fast, high-resolution lunar, solar, and planetary imaging.
Two-stage TEC cooling
With a cooling fan capable of reaching -35º C below ambient temperature and a read noise as low as 0.9e, the ASI2600MC Duo keeps noise in your images very low compared to most other color cameras on the market.
Fast & Stable Data Transfer
Equipped with a high-speed USB 3.0 interface and a DDR3 buffer, designed to optimize data handling and transmission.
The DDR3 buffer temporarily stores image data, allowing for smoother and more stable data transfer between the sensor and the main control system. This ensures that high-resolution images are captured without data loss or delay.
Additionally, during long exposure sessions, the DDR3 buffer helps reduce the sensor's workload, preventing overheating and minimizing the occurrence of Amp Glow, a phenomenon where the sensor generates unwanted bright spots due to excessive heat. This combination of fast data transfer and efficient buffering enhances image quality, making it ideal for high-demand, low-light imaging situations.
Gallery
