Friday, February 25, 2011

APOD 3.6-NGC 1999: South of Orion

1,500 light years away, on the edge of the constellation of Orion, lies the reflection nebula called NGC 1999. The nebula appears to have a large sideways T-shape at its center. The entire NGC 1999 is about 10 light years wide.The dark T-shape is believed to be a hole that was formed through the nebula by the energy of young stars. Young stars within the nebula produce their luminosity from the powerful outflows of shock waves. V380 Orionis is a star within the nebula that provides NGC with its illumination. The red objects in the photo are shock waves named HH1 and HH2. Infrared images show that stellar jets of shock waves push through interstellar materials at hundreds of kilometers per second, forming large dark spots, along with the shock waves, like the ones seen in NGC 1999.

Thursday, February 24, 2011

Annie Jump Cannon Biography



Annie Jump Cannon was born in Dover, Delaware on December 11, 1863. Annie’s passion for astronomy and the stars was inspired by her mother, who taught her about constellations when Annie was a child. She attended Wellesley and majored in the fields of astronomy and physics, where she learned many of the astronomical skills she later used in her studies. She later returned to Wellesley to teach as a junior physics teacher as well as being a student at Radcliffe. Later, Cannon was hired by Edward Pickering and became a member of “Pickering’s Women” and did her astronomical calculations while working for Harvard College Observatory.

Annie Jump Cannon’s significant contributions to astronomy began when she was put in charge of a project for classifying stars. She developed the system in which stars would be classified in spectral classes using the letters O, B, A, F, K, M (which can be remembered with the acronym Oh Be A Fine Girl Kiss Me). She studied spectroscopy, in which light is broken up into component colors, which form the colors in the spectrum of light. By studying the spectra of stars scientists can learn an enormous amount of information about them. Annie Cannon discovered a total of over three hundred stars and classified over a quarter of a million stars into the Henry Draper Catalog before her retirement in 1940. She was also voted one of the top twelve greatest American women. She was named Curator of Astronomical Photographs at Harvard. Annie Jump Cannon contributed significantly to the fields of astronomy and physics and laid a foundation for future astronomers and women in her field of study through her discoveries and developments. Annie Jump Cannon died on April 13, 1941.

Wednesday, February 23, 2011

Observation 3- Stargaze: Sunday, February 21

 Place: Pine View School
Time: 8:30-10:00 P.M.

On Sunday night, the skies were extremely clear. Ten first magnitude stars could be seen above the horizon, some of which being, Sirius, Rigel, Betelgeuse, Algol and Polaris. Through the telescope I was able to see emission nebulae, such as the Orion nebula, several binary stars, and M35 and M41. I also identified the location of the ecliptic, along which I could see the winter zodiacal constellations. The constellation of Orion served as a starting place from which I could identify various other stars, constellations, and M objects in the night sky. Around ten o'clock the moon began to rise and a few clouds covered up the stars.

Friday, February 18, 2011

APOD 3.5- Stars Versus Mountains

6,400 light years away, in the head of the constellation of the Hunter, Orion, NGC 2174 appears to be mountains of dust speckled with stars. These mounds of dust are actually dark stellar nurseries being dispersed by the formation of large nearby stars. The nurseries are made of small amounts of opaque interstellar dust. Sulfur and red hydrogen emissions are apparent and give the dust clouds their glowing color. As more stars are formed in the nurseries, more of the clouds dissipate and eventually it will completely disperse.

APOD 3.4- Rosette Nebula

The Rosette Nebula, NGC 2237, is an enormous emission nebula located in the constellation Monoceros, nearly 5,000 light years away and 100 light years in width. An open cluster of stars about 4 million years old  is inside the nebula is home to many bright young stars, NGC 2244. The nebula appears to glow because of ultraviolet light being emitted from the star cluster. The center of the Rosette Nebula appears to be darker because it is a hole, surrounded by hot gas and gas, being created by stellar winds.

Sunday, February 13, 2011

Annie Jump Cannon Biography Bibliography


"ACannon." Home Page. The Woman Astronomer, 1 Jan. 2008. Web. 13 Feb. 2011. <http://www.womanastronomer.com/acannon.htm>.
"Annie Jump Cannon Biography." Biography.com. 1994-2010 Encyclopædia Britannica, Inc. Web. 13 Feb. 2011. <http://www.biography.com/articles/Annie-Jump-Cannon-9236960>.
"Annie Jump Cannon." Novelguide: Free Study Guides, Free Book Summaries, Free Book Notes, & More. Novelguide.com. Web. 13 Feb. 2011. <http://www.novelguide.com/a/discover/ewb_03/ewb_03_01102.html>.
"Annie Jump Cannon: Theorist of Star Spectra." San Diego Supercomputer Center. Web. 13 Feb. 2011. <http://www.sdsc.edu/ScienceWomen/cannon.html>.

Thursday, February 10, 2011

Observation 2

Time: February 8. 10:30 P.M.
Place: Casey Key

Around 10:30 the moon was relatively bright as about one third of it was illuminated. The brightness of the waxing crescent moon, along with cloudy weather, makes it difficult to view the skies. However, I was able to see Venus appear nearly ten degrees below the moon as the sky became darker but I could not see Uranus due to cloud cover.

Observation 1

Time: February 1, 2011. 7:30-8 P.M.
Place: Casey Key beach

On the night of February 1st an iridium flare was predicted to be seen at about 7:45 P.M. and 20 degrees above the horizon. At 7:40 I began to look for the flare and just before 7:45 I looked above the horizon due  south, and saw the beginning of the flare. The flare only lasted for approximately 25 seconds, however, it did not seem to reach the maximum predicted magnitude of -8.

Friday, February 4, 2011

APOD 3.3- Zeta Oph: Runaway Star

Zeta Oph is an enormous runaway star made of compressed interstellar material nearly 460 light years away. It is believed that the star was at one time a member of an binary star system, however, it outlived its companion and is now moving through the universe. The star itself is approximately twenty times larger than our Sun and 65,000 times more luminous, however because of the high speed at which the star is traveling (24 kiliometres per second), Zeta Oph creates a trailing interstellar bow. The high speed winds in front of the star compress and heat the materials within the star. Zeta Oph, if it were not obstructed by interstellar dust, would be the brightest star in the night sky.