ZWO ASI294MC Color
- 11.7 Megapixel 4/3" Sony IMX294 Color CMOS Sensor
- 4.63µm Pixels and 63,700e Full Well Capacity
- 19 FPS at Full 4144 x 2822 Resolution
- Ultra-Low 1.2e Read Noise
- USB 3.0 and ST-4 Guiding Ports
The ZWO ASI294MC combines the 11.7 MP Sony IMX294 sensor with high-speed USB 3.0 electronics, capturing full-resolution 4144 x 2822 frames at up to 19 FPS. Its 4.63µm pixels are ideal for sampling planetary detail on a wide range of telescopes, while the back-illuminated sensor's deep 63,700e full well and exceptionally low 1.2e read noise extract subtle color variations on Jupiter's cloud bands and Saturn's rings. This uncooled camera delivers its full 14-bit ADC data stream over a 5Gbps USB 3.0 interface, making it a dedicated tool for high-framerate solar system imaging.
At the core of the ASI294MC is a large 4/3" Sony CMOS sensor with a 21.63mm diagonal, providing a generous field of view for framing the entire lunar disc or large solar prominences. The back-illuminated (BSI) architecture maximizes sensitivity by placing the sensor's wiring layer behind the photodiodes. This design, combined with a massive 63,700e- full well capacity and 1.2e read noise, yields a high dynamic range essential for capturing bright planetary limbs and faint atmospheric details in the same exposure without clipping highlights.
The ASI294MC is engineered for lucky imaging, a technique that freezes moments of steady atmospheric seeing. It streams full 11.7 MP frames at 19 FPS over its USB 3.0 port, allowing you to capture thousands of frames in a short period. This high-speed capture is critical for imaging targets like Jupiter, which rotates quickly, and ensures you have enough data to stack only the sharpest frames for a final, detail-rich image.
As an uncooled camera, the ASI294MC has a significant advantage in weight, power simplicity, and cost. Weighing only 0.25 lbs and requiring no external 12V power supply for cooling, it runs entirely off the USB 3.0 port. This makes it an ideal grab-and-go planetary camera that minimizes cable clutter and power management at the telescope, getting you imaging faster. The trade-off is higher thermal noise on exposures longer than a few seconds, which firmly establishes its role as a specialist for short-exposure planetary, lunar, and solar work rather than long-exposure deep-sky imaging.
The primary distinction between this camera and its sibling, the ASI294MC Pro, is thermoelectric cooling. The Pro version is built for long-exposure deep-sky astrophotography, while this uncooled model is optimized for high-speed planetary work.
This is an excellent pairing. For planetary imaging, the optimal focal ratio is typically 5 to 7 times the camera's pixel size. With the ASI294MC's 4.63µm pixels, your target focal ratio is between f/23 and f/32. On an f/10 SCT, you would use a 2.5x or 3x Barlow lens to achieve this magnification, which will give you a well-resolved image of Jupiter's cloud bands and Great Red Spot under good seeing conditions.
Yes, but with a specific technique. As an uncooled camera, the ASI294MC is susceptible to thermal noise on long exposures. However, its high sensitivity and low read noise make it excellent for Electronically-Assisted Astronomy (EAA) or "live stacking." By taking many short exposures (e.g., 5-15 seconds) and stacking them in real-time, you can view bright deep-sky objects like the Orion Nebula (M42) or the Hercules Cluster (M13) without needing active cooling.
An uncooled camera like the ASI294MC does not have a thermoelectric cooling (TEC) system. This means the sensor's temperature will fluctuate with the ambient air temperature, generating thermal noise (a random electronic signal) during longer exposures. This makes it ideal for short-exposure "lucky imaging" of bright solar system objects where exposure times are fractions of a second, but less suitable for traditional long-exposure deep-sky astrophotography where exposures can last several minutes.
The ZWO ASI294MC is compatible with a wide range of free and paid software on Windows, Mac, and Linux. For planetary imaging, popular choices include FireCapture and SharpCap for capturing video data. For post-processing and stacking the resulting video files, imagers commonly use AutoStakkert!, RegiStax, and WinJUPOS.
No. The ZWO ASI294MC is powered entirely through the included USB 3.0 cable. It does not have a port for an external 12V power supply, which simplifies its setup and makes it more portable compared to cooled cameras that require a separate power source for the TEC cooler.
A Back-Illuminated Sensor (BSI) has its metal wiring layer moved behind the light-sensitive photodiode area. In traditional front-illuminated sensors, this wiring can obstruct some of the incoming light. By moving it out of the way, a BSI sensor achieves higher quantum efficiency (QE), meaning it converts a higher percentage of photons into a usable electronic signal. This results in cleaner, more sensitive images, especially in low-light conditions.
| Sensor | 4/3" Sony IMX294 Color CMOS (BSI) |
| Resolution | 4144 x 2822 (11.7 MP) |
| Pixel Size | 4.63 µm |
| Sensor Dimensions | 19.1 mm x 13.0 mm |
| Sensor Diagonal | 21.63 mm |
| Max Frame Rate | 19 FPS at 4144 x 2822 |
| Full Well Capacity | 63,700e- |
| Read Noise | 1.2e |
| Native Bit Depth | 14-bit |
| Shutter Type | Electronic Rolling Shutter |
| Exposure Range | 32 µs to 2000 s |
| ROI Support | Yes |
| Back Focus | 17.5 mm |
| Camera Series | ZWO ASI294 |
| Cooling | Uncooled |
| Guide Port | ST-4 |
| Computer Interface | USB 3.0 / USB 2.0 |
| Telescope Connection | 1.25", 2", M42x0.75 |
| Camera Window | AR Coated |
| On-Camera Memory | 192K byte user-accessible space |
| Working Temperature | -5°C to 45°C |
| Storage Temperature | -20°C to 60°C |
| Working Humidity | 20% to 80% |
| Dimensions | 62 mm x 36 mm |
| Weight | 0.25 lbs |
| OS Compatibility | Mac, Windows, Linux |
ZWO ASI294MC Camera Body
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1.25" Nosepiece
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2m USB 3.0 Cable
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2m ST-4 Autoguider Cable
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T2 to 1.25" Adapter
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11 mm T2 Spacer
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2" Dust Cap
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1.25" Dust Cap
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Quick Guide
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