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telescopecomparison · 2-way

TEC APO140FL f/9.6 vs Takahashi TOA-150B

TEC APO140FL f/9.6
TEC

APO140FL f/9.6

Best suited for intermediate imagers building a versatile kit running a backyard imaging setup.

Takahashi TOA-150B
Takahashi

TOA-150B

Best suited for intermediate imagers building a versatile kit running a permanent observatory setup.

Key differences

+22% focal length
-7% aperture
Slower by 2.3 f-stops

Specifications

SpecificationTEC APO140FL f/9.6Takahashi TOA-150B
Optics
Typerefractorrefractor
Optical designApo triplet fluoriteApo triplet
Aperture140mm150mm
Focal length1345mm1100mm
Native f/ratiof/9.6f/7.3
Image circle88mm
Full-frame supportNoYes
Physical
Weight7.7kg13.5kg
Advantages of TEC APO140FL f/9.6
  • Tighter framing — 1345mm vs 1100mm focal length
  • Lighter (7.7kg vs 13.5kg) — easier to travel with
Advantages of Takahashi TOA-150B
  • Wider field — 1100mm vs 1345mm focal length
  • Faster optics at f/7.3 vs f/9.6
  • Larger image circle (88mm) — supports bigger sensors
Best for — TEC APO140FL f/9.6
  • Small galaxies, planetary nebulae, lunar & planetary detail
  • High-resolution long-exposure work
Best for — Takahashi TOA-150B
  • Medium-sized galaxies and planetary nebulae
  • Full-frame astro cameras and DSLRs
TEC APO140FL f/9.6 — typical FOV & scale
  • With Full-frame (36×24mm, 3.76µm)
    FOV: 1.53° × 1.02°Scale: 0.58"/px
  • With APS-C (23.5×15.7mm, 3.76µm)
    FOV: 1.00° × 0.67°Scale: 0.58"/px
  • With IMX533 square (11.3×11.3mm, 3.76µm)
    FOV: 0.48° × 0.48°Scale: 0.58"/px
Takahashi TOA-150B — typical FOV & scale
  • With Full-frame (36×24mm, 3.76µm)
    FOV: 1.88° × 1.25°Scale: 0.71"/px
  • With APS-C (23.5×15.7mm, 3.76µm)
    FOV: 1.22° × 0.82°Scale: 0.71"/px
  • With IMX533 square (11.3×11.3mm, 3.76µm)
    FOV: 0.59° × 0.59°Scale: 0.71"/px
TEC APO140FL f/9.6 — recommended user

Best suited for intermediate imagers building a versatile kit running a backyard imaging setup.

Takahashi TOA-150B — recommended user

Best suited for intermediate imagers building a versatile kit running a permanent observatory setup.

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