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Circa 1000AD – The first vision aid was
invented (inventor unknown) called a
reading stone. It was a glass sphere that
magnified when laid on top of reading
materials.
Circa 1284 - Italian, Salvino D'Armate
is credited with inventing the first
wearable eye glasses.
1590 – Two Dutch eye glass
makers, Zaccharias Janssen and
son Hans Janssen experimented
with multiple lenses placed in a
tube. The Janssens observed
that viewed objects in front of
the tube appeared greatly
enlarged, creating both the
forerunner of the compound
microscope and the telescope.
1665 – English
physicist, Robert
Hooke looked at a
sliver of cork through
a microscope lens
and noticed some
"pores" or "cells" in it.
Robert Hooke's microscope
 1674 – Anton van Leeuwenhoek built
a simple microscope with only one
lens to examine blood, yeast, insects
and many other tiny objects.
Leeuwenhoek was the first person to
describe bacteria, and he invented
new methods for grinding and
polishing microscope lenses that
allowed for curvatures providing
magnifications of up to 270 diameters,
the best available lenses at that time.
18th century – Technical
innovations improved
microscopes, leading to
microscopy becoming
popular among scientists.
Lenses combining two
types of glass reduced the
"chromatic effect" the
disturbing halos
resulting from differences
in refraction of light.
1830 – Joseph Jackson
Lister reduces spherical
aberration or the
"chromatic effect" by
showing that several
weak lenses used
together at certain
distances gave good
magnification without
blurring the image. This
was the prototype for the
compound microscope.
1872 – Ernst Abbe, then
research director of the
Zeiss Optical Works, wrote
a mathematical formula
called the "Abbe Sine
Condition". His formula
provided calculations that
allowed for the maximum
resolution in microscopes
possible.
The Abbe sine condition is a condition that must
be fulfilled by a lens or other optical system in order
for it to produce sharp images of off-axis as well as
on-axis objects. It was formulated by Ernst Abbe in
the context of microscopes.
The mathematical condition is as follows:
1903 – Richard
Zsigmondy developed the
ultramicroscope that
could study objects below
the wavelength of light.
He won the Nobel Prize in
Chemistry in 1925.
Diplococcus gonorrhoeae
 1931 – Ernst Ruska co-invented
the electron microscope for
which he won the Nobel Prize in
Physics in 1986. An electron
microscope depends on electrons
rather than light to view an
object, electrons are speeded up
in a vacuum until their
wavelength is extremely short,
only one hundred-thousandth
that of white light. Electron
microscopes make it possible to
view objects as small as the
diameter of an atom.
Electron Microscope Image of a Fly Foot
1932 – Frits Zernike
invented the phase-
contrast microscope
that allowed for the
study of colorless and
transparent
biological materials
for which he won the
Nobel Prize in Physics
in 1953.
Cheek Cells
 1981 – Gerd Binnig and
Heinrich Rohrer invented
the scanning tunneling
microscope that gives three-
dimensional images of
objects down to the atomic
level. Binnig and Rohrer
won the Nobel Prize in
Physics in 1986. The
powerful scanning
tunneling microscope is the
strongest microscope to
date.
This is a scanning tunneling
microscope image of the 2-atom thick
lead film. The inset is a zoomed view
showing the atomic structure. (Image:
Dr. Ken Shih, The University of Texas
at Austin)
NUMERICAL APERTURE (N.A.)-
index of the power of the objective to
show distinctly separated, two points
close together in the objects
EQUIVALENT FOCAL LENGTH –
gives an idea as to the distance there
will be between the end of the objective
and the object when in focus

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History of the microscope

  • 1.
  • 2. Circa 1000AD – The first vision aid was invented (inventor unknown) called a reading stone. It was a glass sphere that magnified when laid on top of reading materials. Circa 1284 - Italian, Salvino D'Armate is credited with inventing the first wearable eye glasses.
  • 3. 1590 – Two Dutch eye glass makers, Zaccharias Janssen and son Hans Janssen experimented with multiple lenses placed in a tube. The Janssens observed that viewed objects in front of the tube appeared greatly enlarged, creating both the forerunner of the compound microscope and the telescope.
  • 4.
  • 5. 1665 – English physicist, Robert Hooke looked at a sliver of cork through a microscope lens and noticed some "pores" or "cells" in it.
  • 6.
  • 8.  1674 – Anton van Leeuwenhoek built a simple microscope with only one lens to examine blood, yeast, insects and many other tiny objects. Leeuwenhoek was the first person to describe bacteria, and he invented new methods for grinding and polishing microscope lenses that allowed for curvatures providing magnifications of up to 270 diameters, the best available lenses at that time.
  • 9.
  • 10.
  • 11. 18th century – Technical innovations improved microscopes, leading to microscopy becoming popular among scientists. Lenses combining two types of glass reduced the "chromatic effect" the disturbing halos resulting from differences in refraction of light.
  • 12. 1830 – Joseph Jackson Lister reduces spherical aberration or the "chromatic effect" by showing that several weak lenses used together at certain distances gave good magnification without blurring the image. This was the prototype for the compound microscope.
  • 13.
  • 14. 1872 – Ernst Abbe, then research director of the Zeiss Optical Works, wrote a mathematical formula called the "Abbe Sine Condition". His formula provided calculations that allowed for the maximum resolution in microscopes possible.
  • 15. The Abbe sine condition is a condition that must be fulfilled by a lens or other optical system in order for it to produce sharp images of off-axis as well as on-axis objects. It was formulated by Ernst Abbe in the context of microscopes. The mathematical condition is as follows:
  • 16.
  • 17. 1903 – Richard Zsigmondy developed the ultramicroscope that could study objects below the wavelength of light. He won the Nobel Prize in Chemistry in 1925.
  • 18.
  • 20.  1931 – Ernst Ruska co-invented the electron microscope for which he won the Nobel Prize in Physics in 1986. An electron microscope depends on electrons rather than light to view an object, electrons are speeded up in a vacuum until their wavelength is extremely short, only one hundred-thousandth that of white light. Electron microscopes make it possible to view objects as small as the diameter of an atom.
  • 21.
  • 22.
  • 23. Electron Microscope Image of a Fly Foot
  • 24. 1932 – Frits Zernike invented the phase- contrast microscope that allowed for the study of colorless and transparent biological materials for which he won the Nobel Prize in Physics in 1953.
  • 25.
  • 27.  1981 – Gerd Binnig and Heinrich Rohrer invented the scanning tunneling microscope that gives three- dimensional images of objects down to the atomic level. Binnig and Rohrer won the Nobel Prize in Physics in 1986. The powerful scanning tunneling microscope is the strongest microscope to date.
  • 28. This is a scanning tunneling microscope image of the 2-atom thick lead film. The inset is a zoomed view showing the atomic structure. (Image: Dr. Ken Shih, The University of Texas at Austin)
  • 29.
  • 30. NUMERICAL APERTURE (N.A.)- index of the power of the objective to show distinctly separated, two points close together in the objects EQUIVALENT FOCAL LENGTH – gives an idea as to the distance there will be between the end of the objective and the object when in focus

Editor's Notes

  1. where the variables u, U are the angles (relative to the optic axis) of any two rays as they leave the object, and u′, U′ are the angles of the same rays where they reach the image plane (say, the film plane of a camera). For example, (u,u′) might represent a paraxial ray(i.e., a ray nearly parallel with the optic axis), and (U,U′) might represent a marginal ray (i.e., a ray with the largest angle admitted by the system aperture); the condition is general, however, and does not only apply to those rays. Put in words, the sine of the output angle should be proportional to the sine of the input angle.