Scorpius versus Saggitarius

Scorpius versus Saggitarius
Scorpius versus Saggitarius

Sunday, January 29, 2012

APOD 3.2

Days in the Sun
2012 January 21




The above image was taken over a six month period at University of Hertfordshire's Bayfordbury Observatory; the camera that captured the movement of the sun was composed of a tin can, photographic paper, and a tiny pinhole. What I found most remarkable was the amount of information that could be deduced from the image. From June to December, as the sun traveled across the sky it would get lower in the sky (thereby drawing lines further down the photographic paper) and trace its summer, winter, and fall routes. Also the brightness of each individual line or "day" tells us the everyday weather, a bright line would indicate a clear, sunny day where as a obscured or dim line would mean the day was cloudy. The most remarkable aspect of this article is that the cameras for solargraphy and the development of the images can all be done cheaply at home!








Tuesday, January 24, 2012

Quarter 3/ Observation #1

Jan. 24, 2012
7:30 - 8:30 P.M.
Tonight I tried to discern which star was which in the constellation Orion. The three "belt" stars are Mintaka, Alnitak, and Alnilam. I had trouble remembering which red and blue stars where Betelgeuse and Rigel; I had to double check my notes to be sure. The left, reddish star was Betelgeuse and the left, bluish star was Rigel. My way of remembering this to arrange the stars in alphabetical order/ left to right in the evening sky. Additionally I could not see the moon tonight, which actually helped me stargaze. In the northeast the Big Dipper/ Ursa Major was on the eastern horizon. The north had both the king and the queen, Cepheus and Cassiopeia. As the winter constellation rose in the east and the fall constellations fell in the west, Taurus sat almost directly overhead.

Friday, January 20, 2012

APOD 3.1

2012 January 20
The Wolf's Moon
I saw the title of this and just had to choose it for this quarter's first APOD. Apparently, this moon gained its name when hungry wolves could be heard howling outside indian villages. Luckly the photographer taking this photo was not attacked by any wolves and we are free to enjoy the full orange moon on a snowy Swedish horizon. Every month has its own named full moon; Febuaray will give us the "Snow Moon", because it was at this time that snow happened to be most abundant. Only August has two named moons; one for the first (Sturgeon) and one for the thrity-first (Corn).

Friday, January 13, 2012

APOD 2.8

Lighthouse and Meteor
2012 January 8
This picture shows a meteor from the Quadrantid meteor, named after a constellation that no longer exists. In the early 19th-century it was logged as Quadrans Muralis, when the Astronomical Union adopted the new eighty-eight constellation system it became part of Bootes. This makes the distinction between the Quadrantid and Bootes meteor showers important, since they occur in January and June respectively. Unfortunately the asteroid that gives off these meteors  (2003 EH1) mostly dim meteors in an even dimmer part of the sky. Maybe we will catch some at tomorrow's astronomy night.

Thursday, January 12, 2012

Quarter 2/ Observation #6

Jan.12,2012
7:00 P.M. - 8:00 P.M.
My initial points of reference were the Great Square of Pegasus high in the western sky, Cassiopeia in the north, Jupiter, and Orion to the southeast. I also recognized Gemini's Castor and Pollux sitting diagonally in the night sky near Auriga's genie lamp formation. Additionally, I saw the Pleiades near Perseus for the first time tonight. To conclude I used Jupiter/Aries, Orion, and the aforementioned Pleiades to find the zodiacal constellation, Taurus the Bull.

This makes all 8 hours!

Wednesday, January 11, 2012

William R. Dawes Biography Paper

Fuerst 1
Richard Fuerst
Mr. Percival
DE Astronomy
12 January 2012
William Rutter Dawes
            William R. Dawes was born in West Sussex, England on the nineteenth of March, 1799. His father William Dawes was an astronomer who would later be given the governorship of Sierra Leone for his success with the Eora people in New South Wales. This earned him the nickname of "good mouth", but caused him to miss much of his son's upbringing. William R. Dawes' mother died when he was very young; his father's absence forced him to live with relatives. Initially, the young Dawes was destined to be a clergyman in the Church of England; however , he disagreed with some of the church's tenets and began practicing medicine at Haddenham, Buckinghamshire. It was not until he found himself in Liverpool in 1826 that he became interested in astronomy as a career.

            His first observatory was one he had constructed with a refractor telescope that had an aperture of 3.8 inches, which he looked through to make micrometrical measurements of double stars. From this observatory he measured 121 double stars from the period of 1830 to 1833. Soon thereafter he took charge of George Bishop's observatory in Regent's Park, since Bishop was merely a patron of science, not an astronomer like Dawes. For 4½ years, Dawes worked at
Fuerst 2
Regent's Park with a refractor telescope that had a seven inch aperture; during that time he discovered the orbital motion of Hydrae, γ Andromedae, and Σ 3022. Additionally, he found measurements for another 250 double stars. Dawes also made several notable planetary contributions to astronomy; in 1850 he made meticulous observations of Saturn and its rings. On both the 25th and 29th of November he noticed the dark Crape ring of Saturn. These achievements earned him the Gold Medal of the Royal Astronomical Society in 1855. From 1857 till his death, Dawes lived in Haddenham with his second wife; both were in extremely poor health. In 1860 he lost his wife, but was elected a fellow of the Royal Society in 1865. He continued to observe the heavens until Feburary.15,1868, when he finally departed from this world.

            Now why was he known as William "Eagle-eyed" Dawes, and why are certain craters named after him? His fantastic observations with his reflector telescopes were simply astounding. When William Lassell looked at Saturn with his twenty-four inch he missed Saturn's Crepe ring, Dawes did not. In fact Dawes managed to discern the ring with his 6.5 aperture telescope. Other difficult accomplishments by Dawes include: markings on Jupiter's satellites III and IV, a white spot on Saturn (S. lat. 40-45 degrees), the satellite of Neptune, Saturn's inner satellite Mimas, white spots on Jupiter's southern hemisphere, the great Ellipse of Jupiter, and the companion of Sirius. Ironically, Dawes was notoriously near-sighted. His name is also used to describe an optical phenomena that he discovered; the Dawes limit is a formula to express the maximum resolving power in a microscope/telephone. Where R (in arc seconds)  is the
Fuerst 3
resolving power of the instrument and D is the diameter of the main lens (aperture), the formula is R = 4.56/D (in inches).

Monday, January 9, 2012

Quarter 2/ Observations #6

Jan.9,2012
7:00 P.M. - 8:00 P.M.
This morning's moon was full in the western horizon, meaning that at 7 P.M. the moon rising in the east was waning gibbous. Cancer sat below the moon and Gemini sat above it. Gemini is adjacent to Auriga so I saw that too. To the southwest I saw Jupiter, and since Jupiter currently rests in Aries I was able to find that as well. In the south/southeast I spent a great deal of time looking for Eridanus. I used Orion's belt to point out Taurus and find Eridanus right next to it. Finally in the west I saw Cepheus, Andromeda, and Triangulum.

Sunday, January 8, 2012

Quarter 2/ Observation #5

December. 31, 2011
Jan. 1, 2012
10:30-12:30 P.M.
The Moon was first quarter tonight. I spent most of the night trying to discern constellations that I have not covered previously. My starting points in the sky where Andromeda, Perseus, and Aries. I had to use my winter chart to find out that Auriga sits next to Perseus, which helped me locate Gemini and Cancer. Additionally, I used Orion's belt to find Taurus, thereby getting a better understanding of the winter sky. Finally I observed Lacerta in the northwestern sky, Camelopardalis in the north, and in the south/southwest was Cetus, Pieces, Pegasus, and Aquarius.

Friday, January 6, 2012

APOD 2.7

Starburst Galaxy IC 10
2012 January 4
Located in the northern part of Cassiopeia and "lurking" behind some of the interstellar dust of the Milky Way, the galaxy, IC 10, produces a impressive amount of red light. It was discovered by Lewis Swift on October 8, 1887; he also found the comet, Swift-Tuttle, that produces the Perseids meteor shower! Now what makes this galaxy significant? The fact that it is a starburst galaxy tells us that the galaxy is undergoing a period of intense star forming activity. A starburst can yield ten to a hundred times the amount of stars a normal galaxy would produce and do so in 10 million years (which is like a month in the life of a galaxy)! Starbursts result from colliding galaxies that condense gases to form new stars. These new stars quickly expend their energy and go supernova, thereby creating more instability when they generate shock waves. The resulting chain reaction leads to an explosion of new stars in galaxies like IC 10, that blew my mind!

Wednesday, January 4, 2012

William R. Dawes Biography Sources

Source 1
Gillispie, Charles. "Dawes, William Rutter." Dictionary of Scientific Biography. Vol. 3. Detriot: Charles Scribner's Sons, 2008. P.605-.606. Gale Virtual Library. 4 Jan. 2012. Web. 4 Jan. 2012. <http://go.galegroup.com/ps/retrieve.do?sgHitCountType=None&sort=RELEVANCE&inPS=true&prodId=GVRL&userGroupName=fl_sarhs&tabID=T003&searchId=R4&resultListType=RESULT_LIST&contentSegment=&searchType=BasicSearchForm¤tPosition=1&contentSet=GALE%7CCX2830901096&&docId=GALE|CX2830901096&docType=GALE>
Source 2
Hall, Jeff. "William Rutter Dawes (1799 - 1868)." The Home of Amateur Astronomy in the UK. University of Liverpool, 30 Nov. 2009. Web. 05 Jan. 2012. <http://www.mikeoates.org/astro-history/dawes.htm>
Source 3
Anonymous. "The Observatory." SAO/NASA Astrophysics Data System (ADS). Harvard Edu, 14 Apr. 2011. Web. 11 Jan. 2012. <http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1913Obs....36..419D&db_key=AST&page_ind=0&data_type=GIF&type=SCREEN_VIEW&classic=YES>..