Henrietta Swan Leavitt, born in Lancaster, Massachusetts July 4, 1868, was born to a congressional church minister and house wife. Her early education is less known about but it is known that she went Oberlin College for some time but then moved to Radcliffe College and graduated from that institution. While at Radcliffe, Leavitt attended an astronomy class in her senior year, sparking her interests. After graduation in 1892 she went to work at the Harvard college observatory under Edward Charles Pickering, another famous astronomer, and became part of the team of women who calculated the brightness of variable stars, thousands by the end of the observing time. While documenting these stars she noted that the brighter stars had a longer period. After 4 years of further study she found that those with a higher luminosity almost always had a larger period. This discovery leads to the period-luminosity relationship, specifically Cepheid Variables. With this new relationship in hand, astronomers were eventually able to calculate distance beyond parallax, meaning, a new yard stick had been made to measure the universe with!!!!! The work done by Leavitt would allow Hubble, the man and not the telescoped named after him, to do his most famous works and eventually, kids in high school would use her method of determining distance. Sadly, she was never a very healthy person and in 1921 she succumbed to cancer. Oddly enough, she was almost nominated for a Noble Prize in 1926 in physics because the nominator was unaware of her death. Now, the asteroid 5383 Leavitt and the lunar crater Leavitt are named in her honor.
Monday, March 5, 2012
Bibliography
"SJSU Virtual Museum." Powering Silicon Valley. Web. 05 Mar. 2012. <http://www.sjsu.edu/depts/Museum/lea.html>.
"Henrietta Leavitt." Welcome to "She Is an Astronomer" Web. 05 Mar. 2012. <http://sheisanastronomer.org/index.php/history/henrietta-leavitt>.
"CWP at Physics.UCLA.edu // Leavitt." Henrietta Swan Leavitt. UCLA.edu. Web. 05 Mar. 2012. <http://www.physics.ucla.edu/~cwp/Phase2/Leavitt,_Henrietta_Swan@871234567.html>.
"Henrietta Swan Leavitt." Wikipedia. Wikimedia Foundation, 03 Apr. 2012. Web. 05 Mar. 2012. <http://en.wikipedia.org/wiki/Henrietta_Swan_Leavitt>.
Byers, Nina, and Gary A. Williams. "Biographical Info." Out of the Shadows: Contributions of Twentieth-century Women to Physics. Cambridge, UK: Cambridge UP, 2006. Print.
3.8 Mar 5
Today's blog entry is about a video of the ISS orbiting earth. In this video things like cities become mere shining dots on the surface of the earth while lighting and can be seen striking down on the earth below. Oceans and continents seem to be equal in size but not in depth, the oceans seeming like they have no bottom. We are also treated to seeing the auroras from above, appearing to be moving like strands in the breeze. We can also observe on top of the auroras a band of red that lightly dances on top of the bright green. The final notable thing in this video is the view of the atmosphere, almost always present in the video as the band on the horizon that lights up slowly as the ISS approaches day light.
http://apod.nasa.gov/apod/astropix.html
http://apod.nasa.gov/apod/astropix.html
3.7 Feb. 27
This weeks image is actually a gif of supernova going off and lighting a ring of debris around it on fire. Supernova 1987A was the brightest supernova ever recorded in modern times and has been watched closely, especially from 1994 to 2009, which is when these photos were taken. We can see the ring of debris, only slightly orange in the beginning of the gif, turn a bright yellow indicating a collision with the blast wave sent out in 1987. This ring was a light year wide before the explosion but now expands rapidly and at temperatures at millions of degrees kelvin. We are lucky because all of this is occurring right in our Milky Way's backyard in the large Large Magellanic cloud.
http://apod.nasa.gov/apod/ap120227.html
http://apod.nasa.gov/apod/ap120227.html
3.6 Feb 25
This week's picture features Stephan's Quintet. These galaxies appeared to be locked gravitationally and doomed to go crashing into each other, and this is the case for most of these galaxies. the three in the upper part of the picture, the ones that appear more warped and closer to each other, are the ones that are locked together. the fourth galaxy, that is more blue and closer to the bottom of the picture, is only 40 million light years away while the others are a good 300 million light years away. Overall this picture tells a cosmic story that could be rare or common occurrence, but no matter what, very interesting and majestic to see unfold. With luck our great generations millions of years from now will look back at this picture and be able to compare it to their own pictures, and see just how much everything changed.
http://apod.nasa.gov/apod/ap120225.html
http://apod.nasa.gov/apod/ap120225.html
3.5 Feb. 18
In this week's picture we can view the very beautiful and very large Carina Nebula. Taken in Chile and with a slightly specialized camera, this picture captures non-polluted light from the galaxy and one of its largest star forming region, and main subject matter, the Carina Nebula. Being 7500 light years away and a mere 300 light years across, the gemstone of the southern sky is a not just a star forming region but a supernova factory. the stars made here are so massive that scientist predict that supernovas go off regularly, causing even more star formation. Soon, the European Extremely Large Telescope will have a first class view of this Nebula and all it has to offer.
http://apod.nasa.gov/apod/ap120218.html
http://apod.nasa.gov/apod/ap120218.html
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