telescopecomparison · 2-way
Meade LX200 8" ACF vs Takahashi Mewlon-210
Meade
LX200 8" ACF
Best suited for experienced imagers chasing detail running a backyard imaging setup.
Takahashi
Mewlon-210
Best suited for experienced imagers chasing detail running a permanent observatory setup.
Key differences
-16% focal length
Faster by 1.5 f-stops
Specifications
| Specification | Meade LX200 8" ACF | Takahashi Mewlon-210 |
|---|---|---|
| Optics | ||
| Type | sct | cassegrain |
| Optical design | Advanced Coma-Free | Dall-Kirkham |
| Aperture | 203mm | 210mm |
| Focal length | 2032mm | 2415mm |
| Native f/ratio | f/10.0 | f/11.5 |
| Image circle | — | — |
| Full-frame support | No | No |
| Physical | ||
| Weight | 10.0kg | 15.5kg |
Advantages of Meade LX200 8" ACF
- Wider field — 2032mm vs 2415mm focal length
- Faster optics at f/10 vs f/11.5
- Lighter (10kg vs 15.5kg) — easier to travel with
Advantages of Takahashi Mewlon-210
- Tighter framing — 2415mm vs 2032mm focal length
Best for — Meade LX200 8" ACF
- Small galaxies, planetary nebulae, lunar & planetary detail
- High-resolution long-exposure work
- Faint-object imaging under dark skies
Best for — Takahashi Mewlon-210
- Small galaxies, planetary nebulae, lunar & planetary detail
- High-resolution long-exposure work
- Faint-object imaging under dark skies
Meade LX200 8" ACF — 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
Takahashi Mewlon-210 — typical FOV & scale
- With Full-frame (36×24mm, 3.76µm)FOV: 0.85° × 0.57°Scale: 0.32"/px
- With APS-C (23.5×15.7mm, 3.76µm)FOV: 0.56° × 0.37°Scale: 0.32"/px
- With IMX533 square (11.3×11.3mm, 3.76µm)FOV: 0.27° × 0.27°Scale: 0.32"/px
Meade LX200 8" ACF — recommended user
Best suited for experienced imagers chasing detail running a backyard imaging setup.
Takahashi Mewlon-210 — recommended user
Best suited for experienced imagers chasing detail running a permanent observatory setup.