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IR Spectrometers01:25

IR Spectrometers

2.5K
There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
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Kepler's Third Law of Planetary Motion01:18

Kepler's Third Law of Planetary Motion

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In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
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Psychology as a Science01:13

Psychology as a Science

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Psychology, as a scientific discipline, aims to understand the mind and behavior through rigorous and systematic methods. The foundation of psychological research is evidence-based, relying heavily on the scientific method to derive and validate knowledge. This structured approach ensures that findings are reliable, valid, and applicable to broader contexts.
The scientific method in psychology involves six critical steps: making observations, formulating hypotheses, conducting tests, analyzing...
3.9K
Mass Spectrometers01:16

Mass Spectrometers

8.7K
This lesson details the instrumentation of a mass spectrometer—a physical instrument to perform mass spectrometry on analyte molecules and record the characteristic mass spectra. This is achieved via three chief functions:
8.7K
Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

5.5K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
5.5K
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

5.2K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
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Related Experiment Video

Updated: Jan 27, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

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Miniaturized ring-down spectrometer for CubeSat-based planetary science.

Bradley M Gibson

    Applied Optics
    |March 16, 2019
    PubMed
    Summary
    This summary is machine-generated.

    A compact, miniaturized spectrometer was developed for planetary science missions. This robust instrument demonstrates high sensitivity for water vapor and oxygen isotope measurements, paving the way for CubeSat deployments.

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    Area of Science:

    • Planetary Science
    • Spectroscopy
    • Astrophysics

    Background:

    • Miniaturized spectrometers are crucial for in situ analysis in space missions.
    • CubeSat platforms require compact, low-power, and low-mass instruments.
    • Cavity Ring-Down Spectroscopy (CRDS) offers high sensitivity for trace gas detection.

    Purpose of the Study:

    • To develop a robust, miniaturized CRDS for CubeSat deployment.
    • To demonstrate its capability for in situ planetary measurements.
    • To ensure flexibility for various planetary science targets across the near- and mid-infrared spectrum.

    Main Methods:

    • Development of a miniaturized CRDS laboratory demonstration model.
    • Operation at 1.39 μm for water vapor isotope measurements.
    • Demonstration of scanning performance using oxygen isotope measurements.
    • Design utilizing components with functional equivalents across the 1-5 μm range.

    Main Results:

    • Achieved a noise-equivalent absorption coefficient of 3.7×10-9 cm-1 Hz-1/2 at 1.39 μm for water vapor.
    • Successfully demonstrated scanning performance for oxygen isotope analysis.
    • Preliminary results for methane measurements at 3.27 μm were presented.

    Conclusions:

    • The developed spectrometer is compatible with CubeSat spacecraft buses.
    • Its small probed gas volume (less than 2.5 cc) meets mass, volume, and power constraints.
    • The instrument's design offers flexibility for diverse planetary science applications.