An analysis of the history of the sun

This allows for direct testing of materials, instead of having to take the material to a lab to figure out what the solid, liquid, or gas is made of.

This was followed a few years later by the Rydberg formulawhich described additional series of lines. Joseph von Fraunhofer made a significant experimental leap forward by replacing a prism with a diffraction grating as the source of wavelength dispersion.

Meanwhile, the substantial summary of past experiments performed by Maxwellresulted in his equations of electromagnetic waves.

August Beer then observed a relationship between light absorption and concentration and created the color comparator which was later replaced by a more accurate device called the spectrophotometer.

The laser light allowed for much higher precision experiments specifically in the uses of studying collisional effects of light as well as being able to accurately detect specific wavelengths and frequencies of light, allowing for the invention of devices such as laser atomic clocks.

Lehrer created the first fully-automated spectrometer" to help more accurately measure spectral lines. Talbot made systematic observations of salts using flame spectroscopy.

He demonstrated that the prism is not imparting or creating the colors but rather separating constituent parts of the white light.

Fraunhofer made and published systematic observations of the solar spectrum, and the dark bands he observed and specified the wavelengths of are still known as Fraunhofer lines. Infrared and Raman spectroscopy[ edit ] Many early scientists who studied the IR spectra of compounds had to develop and build their own instruments to be able to record their measurements making it very difficult to get accurate measurements.

In the process, they established the technique of analytical spectroscopy. Quantum mechanics provided an explanation of and theoretical framework for understanding spectroscopic observations.

These contracted companies started developing optical instruments and eventually created the first infrared spectrometers.

Late 19th Century - [ edit ] Johann Balmer discovered in that the four visible lines of hydrogen were part of a series that could be expressed in terms of integers. It was not until the 19th century that the quantitative measurement of dispersed light was recognized and standardized.

With the development of these commercial spectrometers Infrared Spectroscopy became a more popular method to determine the "fingerprint" for any molecule. They also used the non-relativistic Doppler shift redshift equation on the spectrum of the star Sirius in to determine its axial speed.

Subsequent experiments with prisms provided the first indications that spectra were associated uniquely with chemical constituents. A hot gas under low pressure emits a "bright-line" or emission-line spectrum. They established the linkage between chemical elements and their unique spectral patterns.

Lasers also made spectroscopy that used time methods more accurate by using speeds or decay times of photons at specific wavelengths and frequencies to keep time. In the s the husband-and-wife team of William and Margaret Huggins used spectroscopy to determine that the stars were composed of the same elements as found on earth.

He conducted his own experiments to demonstrate the effect of passing light through a single rectangular slit, two slits, and so forth, eventually developing a means of closely spacing thousands of slits to form a diffraction grating. His experiments demonstrated that white light could be split up into component colors by means of a prism and that these components could be recombined to generate white light.

One example is using laser spectroscopy to detect compounds in materials. One year later, inFrench physicist Antoine Henri Becquerel discovers radioactivity, and Dutch physicist Pieter Zeeman observes spectral lines being split by a magnetic field.

History of spectroscopy

One specific method is called Laser-induced Fluorescence Spectroscopy, and uses spectroscopic methods to be able to detect what materials are in a solid, liquid, or gas, in situ. Scientists observed the emission of distinct patterns of colour when salts were added to alcohol flames.

Foucault experimentally demonstrated that absorption and emission lines appearing at the same wavelength are both due to the same material, with the difference between the two originating from the temperature of the light source.

Historical Context of A Raisin in the Sun

The interference achieved by a diffraction grating both improves the spectral resolution over a prism and allows for the dispersed wavelengths to be quantified. Kirchhoff and Bunsen also definitively established the link between absorption and emission lines, including attributing solar absorption lines to particular elements based on their corresponding spectra.

A continuous spectrum source viewed through a cool, low-density gas produces an absorption-line spectrum. An incandescent solid, liquid or gas under high pressure emits a continuous spectrum.The history of spectroscopy began in the 17th century. New designs in optics, specifically prisms, enabled systematic observations of the solar spectrum.

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An analysis of the history of the sun
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