Henrietta Leavitt veritably revolutionized astronomy. She is one of the most influential astronomers in history, yet she is not remembered like Newton, Hubble, or Galileo, because she was lucky enough to be born female. Leavitt was born on July 4, 1868 in Lancaster, Massachusetts. She attended Oberlin College and Radcliffe College. She never took an astronomy course until her final year of college, but she was thoroughly intrigued. Following her graduation, Leavitt began working at the Harvard College Observatory. She was one of the many women hired as "computers" to catalog the brightness of stars as they appeared in the observatory's collection. At this time, women were not allowed to operate telescopes. She was instructed by her supervisor to begin cataloging variable stars, whose brightness would change over time.
She worked hard, but was not expected to find anything, instead just hired to do work that the men didn't want. In fact, Leavitt would make a discovery that would change astronomy. In one study published in the Annals of the Astronomical Observatory of Harvard College, Leavitt noted that variable stars with greater luminosity had longer periods. She confirmed this by studying the Cepheid variables intensely, and realized that the relationship between period and luminosity was very concrete. The discovery is known as the "period-luminosity relationship" which says that the logarithm of the period s linearly related to the star's intrinsic luminosity. This finally allowed scientists to measure the distance to galaxies which were too far away to be computed through stellar parallax. Thanks to Leavitt's discovery, the distances to any Cepheid in the Milky Way could be determined with great accuracy. Later, Edwin Hubble used Leavitt's discovery to measure distances to Cepheids in the Andromeda Galaxy. Thus, Leavitt's discovery led to the realization that the universe is much larger than our Milky Way, and other spiral galaxies exist independently outside of our Milky Way. This discovery was one of the most revolutionary in history.
In 1921, Leavitt was made director of stellar photometry at Harvard. However, by the end of that year, illnesses which plagued her since graduating from college finally took their toll, causing Leavitt to die from cancer. She was buried in the Cambridge Cemetery. Other than making the most influential discovery in astronomy, she received many honors. She was a member of Phi Beta Kappa, the American Association of University Women, the American Astronomical
and Astrophysical Society, the American Association for the Advancement
of Science, and an honorary member of the American Association of
Variable Star Observers.
Monday, February 25, 2013
APOD 3.6
Mercury on the Horizon
This image showcases a beautiful sky and the trail of mercury as it follows the sun, rising above the horizon and quickly disappearing. Mercury orbits very closely to the sun and therefore is only visible shortly after sunset or before sunrise for a short while. It takes careful planning and finesse to follow Mercury during certain times of the year. Currently it will be visible in the western sky right after sunset, for the northern hemisphere.
Henrietta Leavitt Biography: Sources
"Henrietta Leavitt." PBS. PBS, n.d. Web. 25 Feb. 2013. <http://www.pbs.org/wgbh/aso/databank/entries/baleav.html>.
Johnson, George (2005). Miss Leavitt's Stars: The Untold Story of the Woman Who Discovered How to Measure the Universe. New York: W.W. Norton & Company.
"Leavitt." CWP at Physics.UCLA.edu. N.p., n.d. Web. 25 Feb. 2013. <http://www.physics.ucla.edu/~cwp/Phase2/Leavitt,_Henrietta_Swan@871234567.html>.
Friday, February 15, 2013
APOD 3.5
This image shows a subvisual red aurora which was only detected after an extended photographic exposure. The skyscape also shows clearly Jupiter near the horizon, the bright Pleiades cluster, and Auriga, Taurus, and Gemini. These auroras showed up over Anchorage, Alaska, due to energetic solar particles affecting our own magnetosphere. Red and green aurora are caused by excited oxygen atoms.
Friday, February 8, 2013
APOD 3.4
This image shows the Andromeda Galaxy, the closest spiral galaxy to our own, in Infrared from the Herschel Space Observatory. Andromeda is 200,000 light-years across, double the size of the Milky Way. The red light in the outskirts of the galaxy shows dust heated and glowing from starlight. The blue core shows hotter dust. Andromeda contains a huge capacity for future star development, shown by the amount of molecular gas present.
APOD 3.3
This photograph shows a clear dark sky, crescent moon, and city lights in Santiago. In that sky is Comet McNaught, one of the most photogenic comets which was beautiful when it passed over the northern hemisphere and even more magnificent when it reached around the southern hemisphere. By that time it had developed a long dust tail. McNaught has been the brightest comet in decades. This photo is resurfacing because 2013 is expected to bring even more brilliant comets. Comet ISON, at the end of the year, may become one of the brightest comets in history.
Monday, February 4, 2013
Subscribe to:
Posts (Atom)