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telescopecomparison · 2-way

Meade LX200 10" ACF vs Celestron C8 SCT

Meade LX200 10" ACF
Meade

LX200 10" ACF

Best suited for experienced imagers chasing detail running a permanent observatory setup.

Celestron C8 SCT
Celestron

C8 SCT

Best suited for experienced imagers chasing detail running a backyard imaging setup.

Key differences

+25% focal length
+25% aperture

Specifications

SpecificationMeade LX200 10" ACFCelestron C8 SCT
Optics
Typesctsct
Optical designAdvanced Coma-FreeSchmidt-Cassegrain
Aperture254mm203mm
Focal length2540mm2032mm
Native f/ratiof/10.0f/10.0
Image circle
Full-frame supportNoNo
Physical
Weight13.6kg5.7kg
Advantages of Meade LX200 10" ACF
  • Tighter framing — 2540mm vs 2032mm focal length
  • 25% more light-gathering aperture
Advantages of Celestron C8 SCT
  • Wider field — 2032mm vs 2540mm focal length
  • Lighter (5.7kg vs 13.6kg) — easier to travel with
Best for — Meade LX200 10" ACF
  • Small galaxies, planetary nebulae, lunar & planetary detail
  • High-resolution long-exposure work
  • Faint-object imaging under dark skies
Best for — Celestron C8 SCT
  • Small galaxies, planetary nebulae, lunar & planetary detail
  • High-resolution long-exposure work
  • Faint-object imaging under dark skies
Meade LX200 10" ACF — typical FOV & scale
  • With Full-frame (36×24mm, 3.76µm)
    FOV: 0.81° × 0.54°Scale: 0.31"/px
  • With APS-C (23.5×15.7mm, 3.76µm)
    FOV: 0.53° × 0.35°Scale: 0.31"/px
  • With IMX533 square (11.3×11.3mm, 3.76µm)
    FOV: 0.25° × 0.25°Scale: 0.31"/px
Celestron C8 SCT — typical FOV & scale
  • With Full-frame (36×24mm, 3.76µm)
    FOV: 1.02° × 0.68°Scale: 0.38"/px
  • With APS-C (23.5×15.7mm, 3.76µm)
    FOV: 0.66° × 0.44°Scale: 0.38"/px
  • With IMX533 square (11.3×11.3mm, 3.76µm)
    FOV: 0.32° × 0.32°Scale: 0.38"/px
Meade LX200 10" ACF — recommended user

Best suited for experienced imagers chasing detail running a permanent observatory setup.

Celestron C8 SCT — recommended user

Best suited for experienced imagers chasing detail running a backyard imaging setup.

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