Astrophotoguru · Compare

cameracomparison · 2-way

ZWO ASI6200MM Pro vs ZWO ASI2400MM Pro

ZWO ASI6200MM Pro
ZWO

ASI6200MM Pro

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

ZWO ASI2400MM Pro
ZWO

ASI2400MM Pro

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

Key differences

Finer pixels (3.76µm vs 5.94µm)
153% more resolution

Specifications

SpecificationZWO ASI6200MM ProZWO ASI2400MM Pro
Sensor
TypeDedicated CooledDedicated Cooled
SensorSony IMX455Sony IMX410
Sensor techCMOSCMOS
FormatFull FrameFull Frame
Sensor size36.0×24.0mm36.0×24.0mm
Diagonal43.3mm43.3mm
Pixel size3.76µm5.94µm
Resolution9576×63886072×4042
Megapixels62.0MP24.5MP
ColorNoNo
Cooling
CooledYesYes
Performance
Full well51400e⁻100000e⁻
Peak QE91%80%
Advantages of ZWO ASI6200MM Pro
  • Finer sampling at 3.76µm pixels
  • Higher resolution (62MP vs 24.5MP)
Advantages of ZWO ASI2400MM Pro
  • Larger pixels — better low-light per-pixel sensitivity
Best for — ZWO ASI6200MM Pro
  • Wide-field mosaics and full-frame telescopes
  • Well-sampled deep-sky at medium focal lengths
  • Long-exposure deep-sky under any sky
  • Narrowband and LRGB workflows
Best for — ZWO ASI2400MM Pro
  • Wide-field mosaics and full-frame telescopes
  • Fast, low-noise deep-sky at short focal lengths
  • Long-exposure deep-sky under any sky
  • Narrowband and LRGB workflows
ZWO ASI6200MM Pro — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 8.25° × 5.50°Scale: 3.10"/px
  • On 800mm SCT reducer
    FOV: 2.58° × 1.72°Scale: 0.97"/px
  • On 2000mm SCT native
    FOV: 1.03° × 0.69°Scale: 0.39"/px
ZWO ASI2400MM Pro — typical FOV & scale
  • On 250mm refractor (wide)
    FOV: 8.25° × 5.50°Scale: 4.90"/px
  • On 800mm SCT reducer
    FOV: 2.58° × 1.72°Scale: 1.53"/px
  • On 2000mm SCT native
    FOV: 1.03° × 0.69°Scale: 0.61"/px
ZWO ASI6200MM Pro — recommended user

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

ZWO ASI2400MM Pro — recommended user

A strong fit for dedicated deep-sky imagers pairing with wide-field refractors.

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