Friday, February 27, 2015

Henrietta Leavitt


upper-body & face of Henrietta Swan Leavitt

Henrietta Swan Leavitt was born on July 4th, 1868 in Cambridge, Massachusetts to George Roswell Leavitt and Henrietta Swan. She attended Oberlin College and graduated from the Society for Collegiate Instruction of Women, later called Radcliffe College. While in college, she studied classical Greek, fine arts, philosophy, calculus, and geometry. Leavitt did not even take an astronomy class until her fourth year of college. After graduation, she suffered a seriously dangerous disease that left her severely deaf. 
In 1895, she began to volunteer at the Harvard College Observatory. Edward Charles Pickering appointed Henriette Leavitt to a permanent position seven years later. She eventually became the head of the photography photometry department, which studied images of stars to determine their magnitude. Throughout her career, she discovered more than 2,400 variable stars, which is half of the known total in her day. Her work led to the cepheid variable period-luminosity relationship. Leavitt discovered a direct correlation between the time it took a star to go from bright to dim to how bright it actually was through the intense observation of the cepheids. This relationship helped other astronomers with their own discoveries.
Leavitt created a standard of photographic measurements that was accepted by the International Committee on Photographic Magnitudes, which became known as the Harvard Standard, in 1913. She used 299 plates from 13 telescopes and used logarithmic equations to organize stars in a range of over 17 magnitudes of brightness. 
She worked at the Harvard College Observatory until her death from cancer in 1921. 

Friday, February 20, 2015

Sources

Works Cited
Mariani, Gael. "Henrietta Leavitt – Celebrating the Forgotten Astronomer | AAVSO." AAVSO. N.p., n.d. Web. 20 Feb. 2015. <http://www.aavso.org/henrietta-leavitt-%E2%80%93-celebrating-forgotten-astronomer>.
"1912: Henrietta Leavitt Discovers the Distance Key." 1912: Henrietta Leavitt Discovers the Distance Key. Carnegie Institution for Science, n.d. Web. 20 Feb. 2015. <https://cosmology.carnegiescience.edu/timeline/1912>.
PBS. PBS, n.d. Web. 20 Feb. 2015. <http://www.pbs.org/wgbh/aso/databank/entries/baleav.html>.

APOD 3.5

An Evening Sky Conjunction: http://apod.nasa.gov/apod/ap150220.html


A pairing of the moon and Venus can be seen in this eight year old photo. Seen near the western horizon, this conjunction can be seen reflecting in the water in Bolu, Turkey. Venus has orbited the Sun at least 13 times since this photo was taken meaning that a similar conjunction can be seen tonight. The only difference is tonight the conjunction will also have a fainter Mars nearby.

Friday, February 13, 2015

APOD 3.4

M100: A Grand Design Spiral Galaxy- http://apod.nasa.gov/apod/ap150211.html


M100 is a large spiral galaxy of over 100 billion stars with well-defined spiral arms. It is comparable to our own Milky Way Galaxy. M100 is 56 million light years distant toward Berenice's Hair. Bright blue star clusters and dust lanes can be seen in this image of the galaxy from 2009. A light echo from a bright supernova can be seen in the photo too. This galaxy is truly stunning. 

Thursday, February 12, 2015

Star Formation

http://apod.nasa.gov/apod/ap040713.html

http://news.discovery.com/space/astronomy/baby-stars-are-ripping-their-stellar-nursery-to-shreds-140702.htm

http://www.cnet.com/news/swirling-spiral-galaxy-spotted-by-space-telescope/

http://www.natureworldnews.com/articles/8465/20140808/stellar-nursery-reveals-details-about-birth-of-the-sun.htm

Tuesday, February 10, 2015

Observation Feb 7th, 2015

Time: 8:30-10:30 (2 Hours) 

Place: Osprey, FL

Sky Conditions: Clear

Instruments Used: Night Sky App and Binoculars

Bright Stars noted: Polaris, Algol, Mira, Gamma Andromeda, Aldebaren, Betelgeuse, Rigel, Castor, Pollox

Constellations noted: Gemeni, Pegasus, Cepehus, Orion, Ursa Minor, Andromeda, Eridanus, Taurus, Aurigoa

Friday, February 6, 2015

APOD 3.3

M104: The Sombrero Galaxy: http://apod.nasa.gov/apod/ap150205.html


M104 is a spiral galaxy known for its nearly edge-on profile featuring a huge ring. The ring is seen because of the silhouette of cosmic dust against the bright stars. Hubble Space Telescope and ground-based Subaru data have been used to process this image to provide natural colors since the central bulge prevents the galaxy from being properly seen with ground-based instruments. The Sombrero Galaxy is thought to hold a massive black hole.