Wednesday, February 23, 2011

Heber Curtis

Heber Curtis was an American astronomer born June 27, 1872  in Muskegon, Michigan. The first attended the University of Michigan . However, his education at this university had very little to do with astronomy. The degrees he earned at this school was in classical languages. He then moved on to teach Latin at the Napa College. It was at this college that he discovered his penchant for astronomy by looking at the reflecting telescope that was held there. In 1895 he married Mary Raper and had four children. In 1897 Curtis switched his teaching profession over to being an astronomy and mathematics instructor. In 1902 he attended the eclipse in Georgia where he met other astronomers who encouraged him to continue his astronomical research at the University of Virginia. It was there that he recieved his PHD in astronomy. He was then easily hired at the Lick Observatory where he continued the research started by Keeler on nebulae. Heber Curtis worked at the Lick Observatory for 18 years.In 1917 Heber Curtis observed the nova S Adromadae within the Great Adromeda Nebula. It was there that he studied in depth and wrote a research paper regarding spiral nebulae. It was the presentation of this paper to the National Academy of Sciences that started the Great Debate that he is most famous for. In this debate,  Curtis argued that spiral nebulae were a seperate group of stars outside of the Milky Way galaxy. On the opposing side of the great debate was Harlow Shapley, who beleived that spiral nebulae were actually located inside of the Milky Way Galaxy. Later it would be found out that by Edwin Hubble that Curtis was in fact correct in his argument. This also proved that there are galaxies outside of our Milky Way. Shapely was correct , however in a different aspect of the argument that the Sun is not even close to being the center of the Universe. He ws also correct in his assertion that nebulae orbit the milky way much more frequently than beleived by Curtis. Other great accomplishmments of Heber Curtis in the field of stronomy included; becoming the president of the Astronomical Society of the Pacific in 1912 and in becoming the director of the Allegheny observatory in 1920. He also took part in the development of the McMath- Hulbert observatory on Lake Angelus. After a full life of mny accomplishments, Heber Curtis died in 1942 of a severe thyroid disease.

Astronomer sources

http://www.astro.virginia.edu/research/observatories/26inch/history/curtis.php

http://en.wikipedia.org/wiki/The_Great_Debate

http://www.daviddarling.info/encyclopedia/C/Curtis.html

http://en.wikipedia.org/wiki/Heber_Doust_Curtis

http://apod.nasa.gov/diamond_jubilee/debate_1920.html

http://www.astrosociety.org/pubs/mercury/30_03/seasons.html

http://incubator.rockefeller.edu/?p=266

http://www.britannica.com/EBchecked/topic/147181/Heber-D-Curtis

Tuesday, February 22, 2011

Observation

On sunday, February 20, I attended the stargaze at Pine View Scool. There I viewed the pleiades star cluster through binoculars. I also identified Orion and it's belt, along with Beteguese and Rigel. I could also see the horsehead nebula through a pair of binoculars. I  identified Sirius along with Canis Major, the contellation that it is located in. I could make out Lepus faintly below Orion, next to Canis major. I could also see Taurus, above orion, as well as Auriga and Gemini, high in the sky. Canopis could also be seen low in the horizon, shining brightly. I also viewed Jupiter and its moons through the telescope that Mr. Percival set up for us :) It was really fascinating because I could faintly make out the coloration of Jupiter and some of its swirling storms that cover its surface. It was also really cool to see the moons that I have learned about so clearly.

Friday, February 11, 2011

DOUBLE RAINBOW ALL THE WAY

When viewing a rainbow, the sun must always be always behind you. However, in this breathtaking image, composed of five different photographs, we can see the 360 degree view of the sky, in which a sunset is located on the opposite side of a rainbow. A rainbow as we all know (hopefully) is caused by the internal reflection of photons in light rays emitted from the Sun by water droplets, or water vapor in the sky. the fainter arcs seen within the primary-or brightest- arc of the rainbow. Also there is a third,dimmer arc that can be seen above the rainbow.

3.1 Crepulscular rays over Lake Michigan

Crepulscular rays are rays of sunlight that appear to pour in through a single whole in a cloud and seperate into many different rays, appearing as though heaven is pouring in through the cloud.Crepulscular rays are rays of sunlight that stream in through gaps of a cloud. The name crepulscular was derived from the time at which these rays are formed; the crepuscular hours-around sunrise and sunset. Although these lines are in fact, parallel, we perceice them as diverging because of our linear perspective from Earth. It is the diffraction, reflection, and scattering of photons by particles in the air that makes this beautiful phenomnenon visible to us .Anticrepuscular rays can not be seen in this image, but they usually appear at the same time as crespulcular rays; at the antisolar point, on the oppsite side of the sky. Anticrespuluclar rays are not as bright or prominent as crespulcular rays