Monday, May 26, 2008

Biography


Cameron Johnson

Mr. Percival

Astronomy

23 May 2008

Vera Rubin

Vera Cooper Rubin was born in Philadelphia, Pennsylvania on July 23, 1928. At a young age she found a passion for astronomy and would go on to greatly contribute in the field. In 1948, she graduated from Vassar College in New York where she got her bachelors degree in Astronomy. Vera, upon receiving her degree, applied to Princeton, but was not allowed to enroll into their graduate astronomy program, so she looked elsewhere. She was accepted to Cornell where she would go onto to earn her Master’s degree there in 1951 along side her future husband Bob Rubin, a physicist. Early in Vera’s career, she obtained a negative reputation. The Big Bang Theory was widely accepted by the astronomical community during this time, but Vera’s thesis for her masters to the American Astronomical Society would find fault in it. Her thesis suggested that all of the galaxies in the universe are rotating around a center that is not known which would disprove the theory stating that the galaxies are expanding out. This put Rubin in an unenthusiastic view because of the lack of scientific theory to help back her bold findings.

In 1954, Vera Rubin received her doctorate at Georgetown University which furthered showed her theory that that galaxies in the universe were not uniformly distributed, but were quite randomly situated. Her theory would not prove correct until fifteen years after. After receiving her doctorate, she went on to teach at Georgetown for a couple of years and during this time she would have two more children, making it a total of four. Vera received a nice offer from the Department of Terrestrial Magnetism which is associated with the Carnegie Institution, in 1956. Her work for the department would lead to some of the most important astronomical findings to date. Vera’s research disproved Newtonian laws of gravity that predicted the orbiting speeds of stars in galaxies. In the early 1970s, she examined the spectra from galaxies that should stars on the outer edge of galaxies do not orbit slower than stars in the center. It showed that stars orbiting the outer edge of spiral galaxies are going just as fast as those that are located in the center. To this day, astronomers know that there is a huge mass which is invisible that exerts a force to keep out stars in orbit in galaxies. Thus, Vera’s findings and extensive research shows that this “dark matter” comprises of at least 90% of the universe which has left astronomers struggling to identifying it.

Vera Rubin’s accomplishments did not stop with the dark matter. She is an honorary member of the U.S. National Academy of Sciences as well as the Pontifical Academy of Sciences which its purpose is to promote the progress of mathematics, physical, and natural sciences. She was also published an astounding 114 co-authored research papers. Her passion for science was also passed down to her four children. All have earned Ph. D.s in either geology, cosmic-ray physics, astronomy, or mathematics. In 1992, Vera discovered a galaxy in which half the stars were orbiting one direction in the disk and the other half were orbiting in the other direction. Most recently, her colleagues and her discovered that more than half of the galaxies in the Virgo cluster exhibit disturbances due to the closeness of their gravitational fields. Most important to her is that “My numbers mean more to me than my name. If astronomers are still using my data years from now, that’s my greatest compliment.”

Friday, May 9, 2008

4.6 Apod Entry

The photo for the week of May 6 is of Galaxies Collide in NGC 3256. This galaxy is one of the few that look likes like this. The photo contains two galaxies that are currently in the process of slowly colliding. It is estimated that the process will last 100s of millions of years in which there will only be one. The center contains two galactic nuclei with unusual tidal tails and dark dust.

Friday, May 2, 2008

4.5 Apod Entry


The photo for the week of May 2 is titled Shaping NGC 6188. This large emission nebula is located on the periphery of the constellation of Ara which is located 4,000 light-years ago. The Ara constellation is known for its star formation which emits dust and winds that have helped shape this NGC. Astronomers have speculated that the star formation is triggered by a super nova explosion. The Hubble Space Telescope captured this image with a span of 300 light years.

Friday, April 25, 2008

4.4 Apod Entry


The photo for the week of April 22 is titled The Fox Fur Nebula from CFHT. This nebula is a gigantic mass of dust and gas with hot stars constantly projecting wind and energetic light. The shape of a fox can be easily seen in this gas cloud. The dust in the lower left corner is reflecting the light from the stars in the region which gives off the color blue. The ionized hydrogen give off red emissions and with the cosmic dust creates the pink and brown areas in the image.

Friday, April 18, 2008

4.3 Apod Entry


The photo for the week of April 17 is titled Messier 63: The Sunflower Galaxy. Messier 63 is a spiral galaxy located in the northern sky in the constellation of Canes Venatici. The diameter is measured at an amazing 100k light-years which is relatively the size of our Milky Way galaxy. The core is a bright yellow core with long, blue spiral arms. Stars are forming in the area that is pink in color.

Friday, April 11, 2008

4.2 Apod Entry


The photo for the week of April 8, 2008 is titled Southern Orion: From Belt to Witch. The photo contains the all too familiar photo of the three stars that comprise Orion's Belt located in the upper left of the image. The lower left stars that forms the beginning of the belt is named Alnitak. Located to the left of the star is the giant Flame Nebula. It contains giant, bright emission clouds of dust. Below that is the popular photographic Horsehead Nebula. The giant star Rigel illuminates the the massive Witch Head Nebula.

Friday, March 28, 2008

4.1 Apod Entry


The photo for the week of March 27 is titled, The N44 Complex. The false colored photo is of an enormous emission nebula named N44. It ranges from about 1,000 light-years across in diameter and is located in the southern sky. The young stars inside this nebula create the wind and radiation from inside that eventually helped shape the nebula to what it looks like in the photo. However, these stars are not the only thing that helped shape this cloud, a nearby supernovae has drastically helped form N44's shape.