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The Beer-Lambert law describes the relationship between absorbance and concentration, which combines the principles established by scientists Johann Heinrich Lambert and August Beer. Lambert's law states that when light passes through a medium, the loss in intensity is directly proportional to the original intensity and the path length of the light. Beer's law proposed that the transmittance of a solution remains constant if the product of concentration and path length is constant. The modern...
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On many occasions, physicists, other scientists, and engineers need to make estimates of a particular quantity. These are sometimes referred to as guesstimates, order-of-magnitude approximations, back-of-the-envelope calculations, or Fermi calculations. The physicist Enrico Fermi was famous for his ability to estimate various kinds of data with surprising precision. Estimating does not mean guessing a number or a formula at random. Instead, estimation means using prior experience and sound...
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Related Experiment Video

Updated: May 28, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Lunar eclipse photometry: absolute luminance measurements and modeling.

Nina Hernitschek1, Elmar Schmidt, Michael Vollmer

  • 11Starkenburg Observatory, Niemöllerstr. 9, 64646 Heppenheim, Germany.

Applied Optics
|November 28, 2008
PubMed
Summary
This summary is machine-generated.

Total lunar eclipses in 1990 and 2007 showed high minimum brightness levels, suggesting minimal stratospheric aerosol. These findings aid in understanding Earth

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Area of Science:

  • Astronomy
  • Atmospheric Science
  • Photometry

Background:

  • Total lunar eclipses offer a unique opportunity to study Earth's atmospheric conditions.
  • Previous studies have linked stratospheric aerosol content to lunar eclipse brightness.

Purpose of the Study:

  • To quantify the Moon's time-dependent luminance during total lunar eclipses.
  • To assess the presence and impact of stratospheric aerosols on eclipse brightness.

Main Methods:

  • Utilized calibrated photometers to measure lunar luminance during the 1990 and 2007 total lunar eclipses.
  • Corrected measurements to unit air mass and standard distances for Moon and Sun.
  • Performed absolute calibration using solar luminance and pre-eclipse lunar albedo (approx. 13.5%).
  • Modeled light curves using an artificial Earth shadow with atmospheric radiative transfer data.

Main Results:

  • Measured minimum brightness levels in the total phase were relatively high (-3.32 visual magnitude and -1.7 visual magnitude).
  • The high brightness suggests an absence of pronounced stratospheric aerosol during these eclipses.
  • Light curve modeling incorporated atmospheric radiative transfer calculations.

Conclusions:

  • The observed high minimum brightness during lunar eclipses indicates low stratospheric aerosol loading.
  • These findings contribute to understanding atmospheric conditions through celestial events.
  • The methodology provides a robust approach for analyzing lunar eclipse photometry.