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Advanced Microscopy Simplified
Designed with modularity in mind, the BX3M series provide versatility for a wide variety of materials science and industrial applications. With improved integration with OLYMPUS Stream software, the BX53M provides a seamless workflow for standard microscopy and digital imaging users from observation to report creation.
Choose the Best Model
Comfortable and Easy to Use
Functional
The BX53M maintains the traditional contrast methods of conventional microscopy, such as brightfield, darkfield, polarized light, and differential interference contrast. As new materials are developed, many of the difficulties associated with detecting defects using standard contrast methods can be solved using advanced microscopy techniques for more accurate and reliable inspections. New illumination techniques and options for image acquisition within OLYMPUS Stream image analysis software give users more choices of how to evaluate their samples and document findings.
Leading-Edge Optics
Olympus’ history of developing high-quality optics has resulted in a record of proven optical quality and microscopes that offer excellent measurement accuracy.
Wave Front Aberration Control
Bad wavefront |
Good wavefront (UIS2 objective) |
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BX53MTRF-S |
BX53MRF-S |
BXFM |
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Optical system |
UIS2 optical system (infinity-corrected) |
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Microscope frame |
Illumination |
Reflected/transmitted |
Reflected |
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Focus |
Stroke: 25 mm |
Stroke: 30 mm |
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Fine stroke per rotation: 100 μm |
Fine stroke per rotation: 200 μm |
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Minimum graduation: 1 μm |
Minimum graduation: 2 μm |
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With upper limit stopper, torque adjustment for coarse handle |
With torque adjustment for coarse handle |
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Max. specimen height |
35 mm (w/o spacer) |
65 mm (w/o spacer) |
Depends on the mounting configuration |
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75 mm (with BX3M-ARMAD) |
105 mm (with BX3M-ARMAD) |
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Observation tube |
Wide-field FN 22 |
Inverted: binocular, trinocular, tilting binocular |
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Erect: trinocular, tilting binocular |
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Super-wide-field FN 26.5 |
Inverted: trinocular |
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Erect: trinocular, tilting trinocular |
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Reflected light illumination |
Traditional observation technique |
BX3M-RLAS-S |
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Coded, white LED, BF/DF/DIC/POL/MIX FS, AS (with centering mechanism) |
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BX3M-KMA-S |
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White LED, BF/DIC/POL/MIX FS, AS (with centering mechanism) |
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BX3M-RLA-S |
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100W halogen lamp, white LED, BF/DF/DIC/POL/MIX/ FS, AS (with centering mechanism), |
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BF/DF interlocking, ND filter |
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U-KMAS |
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White LED, 100W halogen |
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Fiber illumination, BF/DIC/POL/MIX |
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Fluorescence |
BX3M-URAS-S |
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Coded, 100W mercury lamp, 4 position mirror unit turret, (standard: WB, WG, WU+BF etc) |
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With FS, AS (with centering mechanism), with shutter mechanism |
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Transmitted light |
White LED |
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Abbe/long working distance condensers |
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Revolving nosepiece |
For BF |
Sextuple, centering sextuple, septuple, coded quintuple (optional motorized revolving nosepieces) |
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For BF/DF |
Sextuple, quintuple, centering quintuple, coded quintuple (optional motorized revolving nosepieces) |
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Stage |
Coaxial left (right) handle stage: |
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76 mm × 52 mm, with torque adjustment |
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Large-size coaxial left (right) handle stage: |
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105 mm × 100 mm, with locking mechanism in Y-axis |
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Large-size coaxial right handle stage: |
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150 mm × 100 mm, with torque adjustment and locking mechanism in Y-axis |
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Weight |
Approx. 18.3 kg |
Approx. 15.8 kg |
Approx. 11.1 kg |
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(Microscope frame 7.6 kg) |
(Microscope frame 7.4 kg) |
(Microscope frame 1.9 kg) |