Friday, November 22, 2013

Comet Ison's core














This picture of Comet Ison was taken by the Chinese Space Radar on September 03, 2013. This picture is impressive because not only can we see the comet's core but we can observe two objects travelling alongside the comet. These two objects were probably released from the comet by the escaping gasses and a weak gravitational field.

Friday, November 8, 2013

Solar Eclipse as seen from Uganda


This picture is from the most recient solar eclipse taken from Uganda. Since we are currently studying the solar system I thought this picture would be fitting. Around the moon, you can see the solar corona and the many solar flares which can extend more than a few Earth lengths off the surface of the sun.

Friday, November 1, 2013

Andromeda Galaxy in Infrared

















This is a picture of the Andromeda Galaxy as seen in infrared. This shot was taken by the Spitzer telescope in 2005. The Andromeda Galaxy is the closest galaxy in the local group and is about twice the size of ours. The bright red lines are caused by excess gas withing the arms of the galaxy.

Sunday, October 20, 2013

Johannes Helvelius Biography - Matthew Lawlor

Johannes Hevelius

Early Life:
               Born on January 28, 1611, Johannes Hevelius was one of the leading astronomers of his time. He studied at the University of Leiden where he studied jurisprudence, the theory of law, and spent his free time studying Astronomy. After his studies, Hevelius spent many years traveling around Europe, specifically to France and England, to consult many astronomers of the time. After he returned to his native town of Danzig, he took over the family business of brewing and began to study municipal administration with which he became town councilor in 1651. Hevelius dedicated his life to astronomy until his death on his seventy sixth birthday, 1687.

Career:
               After he returned to his hometown, Hevelius used some of his family’s wealth to buy two houses adjacent to his own and he begun construction of his instruments. In the prime of his career, Hevelius built a keplerian telescope that had a focal length of 150 feet. Made from just wood and wire, this telescope’s performance was impacted by the wind and sometimes even by the heat of the day. On the twenty sixth of September, 1679, while Johannes was out of town, a fire broke out in one of his three adjacent houses. Unfortunately the fire destroyed all three houses including all of his instruments and his almost completed book. Hevelius later rebuilt his instruments but they were never as accurate as his earlier instruments. Despite the setback, he continued his research and eventually finished his book.  Hevelius is most known for his lunar topography, the mapping of the moon’s surface, which he made about sixty precise drawings. He is also well known for his mapping of sunspots and his discovery of many comets and messier objects. In one of his last published books, Hevelius created new constellations, eleven of which are still used today.

Legacy:

               Hevelius’s instruments were some of the most extensive, most accurate of the time period. His one hundred fifty foot home made telescope was a feat of engineering. Despite the resources and time Hevelius spent building the telescope, he didn’t believe telescopes made observations more accurate. As seen with his discussions with another leading astronomer, Robert Hooke. Hevelius proved mathematically that his observations we marginally more accurate than one made with a telescope. Many historians today believe this was because of the quality of Hevelius’s personal instruments and his skills as an observer rather than the accuracy of the telescope.

Friday, September 27, 2013

M31 versus M33





This is a picture of the galaxies M31 and M33. They are two members of our local group. M31 is the well known Andromeda Galaxy, our closest neighboring galaxy, and M33 is the lesser known Triangulum Galaxy. These two galaxies will merge with ours in a few billion years. The star in the center of the picture is Mirach and is part of the Milky Way.   

Friday, September 20, 2013

M2-9 The Wings of a Butterfly Nebula


M2-9  The Wings of a Butterfly Nebula

This is a high definition picture of a planetary nebula. This one was formed by a pair of quickly rotating stars on their way to become white dwarfs. When a star becomes a white dwarf, it sheds its outer layers of gas, this results in the impressive structures that we can see. This nebula will fade in about two thousand years.

Friday, September 13, 2013

This as a high quality picture of the Andromeda Galaxy. This galaxy is the closest one to ours at an outstanding 2.5 million light years away.  When I saw this I said to my home-dawg, "yo bro, check this out!" then my boy was like "You should totes post this on your blog!" The deep shades of blue are caused by hot, massive, and young stars which were created when a smaller gallexy merged.