РефератыИностранный языкThThe Stars And Galaxies Essay Research Paper

The Stars And Galaxies Essay Research Paper

The Stars And Galaxies Essay, Research Paper


MEGAN JACKSON


MS. KEYS


SCIENCE


DECEMBER 5,2000


THE STARS AND GALAXIES


Have you ever looked up at the sky and wondered what


are those bright and shiny things up there.


Stars: a natural luminious body visible in the sky


especially at night. A self-luminious gaseous celestial body


ofgreat mass which produces energy by means of nuclear


fusion reactions, whose shape is usually spheroidal, and


whose size may be as small as the earth or larger than the


earth?s orbit.


Galaxies: Any of the very large groups of stars and


associated matter that are found throughout the universe.


In 1802, William Wollaston noted that the spectrum of


sunlight did not appear to be a continious band of colors,


but rather had a series of dark lines superimposed on it.


Wollaston attributed the lines to natural boundaries between


colors. Joseph Fraunhofer made a more careful set of


observations of the solar spectrum in 1814 and found some


600 dark lines, and he specifically measured the wavelenght


of 324 of them. Many of the Fraunhofer lines in the solar


spectrum retain the notations he created to designate them.


In 1864, Sir William Huggins matched some of these dark


lines in the spectra from other stars with terrestrial


substances, demonstrating that the stars are made of the


>

same materials of everyday material rather than exotic


substances. This paved the way for modern spectroscopy.


Since even before the discovery of the spectra,


scientists had tried to find ways to catergorize stars. By


observing spectra , astronomers realized that the large


numbers of stars exhibit a small number of distinct patterns


in their spectral lines. Classification by the spectral


features quickly proved to be a powerful tool for


understanding stars.


The current spectral classification scheme was


developed at Harvard Observatory in the early 20th


century. Work was begun by Henry Draper who


photographed the first spectrum of Vega in 1872.


After his death, his wife donated the equipment and


a sum of money to the Observatory to continue his


work. The bulk of classification work was done by


Annie Jump Cannon from 1918 to 1924. The original


scheme used capital letters running alphabetically,


but the subsequent revisions have reduced this as


stellar evolution and typing has become better


understood. The work was published in the Henry


Draper Catalog and Henry Draper Extension which


contained spectra of 225,000 stars down to ninth


magnitude.


The scheme is based on lines which are mainly sensitiveto


stellar surface tempertures rather than actual composition


differences,gravity, or luminosity. Inportant lines

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