Compare Model Drawings, CAD & Specs Availability Price
50102-01
Microscope Objective Lens, Reflective, 36x, 160 mm BFL
$2,992
In Stock
 50102-01 Microscope Objective Lens, Reflective, 36x, 160 mm BFL
In Stock
 $2,992
50102-02
Microscope Objective Lens, Reflective, 36x, Infinite BFL
$2,992
In Stock
 50102-02 Microscope Objective Lens, Reflective, 36x, Infinite BFL
In Stock
 $2,992
50105-01
Microscope Objective Lens, Reflective, 15x, 160 mm BFL
$2,743
In Stock
 50105-01 Microscope Objective Lens, Reflective, 15x, 160 mm BFL
In Stock
 $2,743
50105-02
Microscope Objective Lens, Reflective, 15x, Infinite BFL
$2,743
In Stock
 50105-02 Microscope Objective Lens, Reflective, 15x, Infinite BFL
In Stock
 $2,743

Specifications

Features

Broad Bandwidth

Reflective optics do not experience chromatic effects associated with refractive optics, where refractive index varies with wavelength. Consequently reflective objectives can have excellent optical performance across an extremely broad wavelength range limited only by mirror reflectance. The reflective surfaces are broadband coated with aluminum and over-coated with magnesium fluoride (MgF2). They are usable from 200 nm to 20 µm. Average reflection per surface of each mirror is 85% in the UV-VIS, and 90% in the IR (with a dip to 76% near 820nm). Special coatings are available upon request including Gold for the visible to IR region.

Typical reflectance curves of metallic reflective coatings

Reflective Objective Construction

Our reflective microscope objectives are fabricated from a single material providing a uniform thermal coefficient of expansion. Each objective contains two highly polished nickel spherical mirrors coated with aluminum and magnesium fluoride. The primary mirror has a spherical concave surface with a center hole. The secondary mirror is a small convex spherical mirror that is machined into the spider assembly. The objectives are hand assembled in interferometric alignment fixtures allowing each pair of mirrors to be optimized as a set to achieve maximum resolution. Spot sizes of 2 µm for the 15X objective and 1 µm for the 36X objective are typical.

Reverse Cassegrain Design

In a typical focusing application, collimated light passes through the aperture hole in the primary mirror to the secondary mirror. The secondary mirror then reflects and diverges the beam to fill the primary mirror. Finally, the primary mirror focuses the beam to a small spot called the Object Plane or Focal Point. This dual mirror configuration is known as a reverse Cassegrain (primary mirror collects or focuses light from or to a point, and the secondary mirror interacts with collimated light, the opposite of a traditional Cassegrain telescope). These objectives follow the Schwarzschild design. Accordingly, they have zero chromatic aberration, and negligible coma, spherical, and astigmatic aberrations.

Infinite or Finite Back Focal Lengths

Newport Reflective Microscope Objectives are available with either an infinite back focal length (BFL) or finite BFL of 160 mm, a typical tube length of a microscope. Objectives with an infinite BFL – also known as infinity corrected reflective objectives – are useful for focusing applications as collimated light enters through the aperture hole in the primary mirror to be focused at the specified working distance. Objectives with a finite BFL – also known as finite conjugate reflective objectives – are ideal for imaging applications that do not require an additional lens for focusing.

A) Diagram of a typical focusing application of a reflective microscope objective. B) Illustration of the rear focal plane of a 160 mm back focal length objective

Fourier Transform IR (FTIR) Spectroscopy Applications

In Fourier Transform Infrared (FTIR) spectroscopy, light from a broad spectrum point-like source is collimated and input into a split beam interferometer, such as a Michelson. Displacing one of the mirrors sinusoidally using a motorized mount creates a time dependent optical path difference (OPD) between the two interferometer arms. This OPD corresponds to a different number of wave cycles for each spectral component in the source. Wavelengths that undergo constructive interference will output the system and be focused onto a detector. Spectral composition of the source may be calculated by taking the Fourier transform of the detected light intensity vs time. In FTIR, the maximum spectral resolution depends on system étendue, which is often limited by the size and collection angle of the detector. Reflective microscope objectives allow large collection angles without chromatic aberrations, which helps FTIR systems achieve high spectral resolution over wide spectral ranges.

Applications

  • UV Metrology and Microscopy
  • Spatial Filtering
  • Photomicroscopy
  • Laser Energy Delivery Systems
  • FT-IR Spectroscopy

Resources

Selection Guides