Friday, January 28, 2011

APOD 3.2

http://apod.nasa.gov/apod/ap110128.html


NanoSail-D (Jan. 28 2011)

               Though this photo is only an artist's illustration, it still gives a realistic portrayal of NASA's NanoSail-D. The NanoSail-D has just unraveled a very thin, ten square meter reflective sail on January 20th, becoming the first solar sail spacecraft in low Earth orbit. Though to many people this has just been considered a far off dream, sailing through space was suggested about four hundred years ago by Johannes Kepler who observed comet tails blown by the solar wind. Modern solar sail spacecraft designs, like NanoSail-D or the Japanese interplanetary spacecraft IKAROS, rely on the minute but continuous pressure from sunlight itself for thrust. Glinting in the sunlight as it circles planet Earth, the NanoSail-D solar sail will periodically be bright enough to be easily visible to the naked eye. In fact, sky gazers are being urged to participate in an ongoing contest to capture images of the reflective sail. NASA stated that the images will help monitor the satellite before it reenters the atmosphere in April or May.



Friday, January 21, 2011

APOD 3.1



The Antikythera Mechanism (Jan. 9 2011)

                     Looking at this one might ask what does this mechanism have to do with astronomy? In fact, it was found at the bottom of the sea within an ancient Greek ship. The apparent complexity of this mechanism has prompted decades of study, although some of its functions were still unknown. Recent X-ray scans of the device have now revealed the purpose of the Antikythera mechanism, and discovered several surprising functions. The Antikythera mechanism ascertains to be a mechanical computer of a level of accuracy thought impossible in 80 BC, when the ship that carried it sunk. Such sophisticated technology was not thought to be developed by humanity for another thousand years. Its wheels and gears create a portable orrery of the sky that predicted star and planet locations as well as lunar and solar eclipses in a heliocentric model. The mechanism, shown above, is thirty-three centimeters high so it is similar to the size of a text book. 

Friday, January 14, 2011

Observations 4

Astronomy Cast - Ep. 165: The Doppler Effect


                   Have you ever experience something like an ambulance driving past you and noticed that the sound changes? That’s the Doppler effect in work. It applies to both sound waves and light waves. Astronomers use the Doppler effect to study the motion of objects across the Universe, including nearby extra-solar planets to the numerous distant galaxies. Doppler shift is the change in length of a wave (light, sound, etc.) due to the relative motion of source and receiver. Things moving toward you have their wavelengths shortened. Things moving away have their emitted wavelengths lengthened. For waves that multiply in a medium, such as sound waves, the velocity of the observer and of the source are relative to the medium in which the waves are transmitted. The total Doppler effect may therefore result from motion of the source, motion of the observer, or motion of the medium. Each of these effects is analyzed separately. For waves which do not require a medium, such as light or gravity in general relativity, only the relative difference in velocity between the observer and the source needs to be considered.


APOD 2.8



A Sun Halo Beyond Stockholm (Jan 10, 2011)

                  When looking at this picture you might wonder what exactly is going on and why does the sun look like this? This image makes it seem as if there is some effect or distorted lenses. What gives it this effect is millions and millions of ice crystals which serve as a sort of lenses. When water freezes in the upper atmosphere, small, flat, six-sided, ice crystals can often be formed. When these ice crystals falling to the ground, much of the trip spent with their faces flat, parallel to the ground. An observer may pass through the same plane as many of the falling ice crystals near sunrise or sunset. Due to this alignment, each crystal can act like a natural lens, refracting sunlight into our view and creating phenomena like parhelia, which is the technical term for sundogs. The sundog is the effect you are seeing in the above image. This image was taken last year in Stockholm, Sweden and in the center of the image is the Sun, while two bright sundogs glow prominently from both the left and the right. Also visible is the bright 22 degree halo, as well as the much less common 46 degree halo, also created by sunlight reflecting off the atmospheric ice crystals.

Tuesday, January 11, 2011

Biography: Pierre Méchain

Pierre Méchain


              Pierre Méchain was born August 16, 1744 in Laon, France. He was the son of Pierre-François Méchain, who was an architect, and Marie-Marguerite Roze, and early in his life wanted to follow his father in a career in architecture. He studied mathematics and physics, but due to financial difficulties he ended up leaving college. He then became friends with Jérôme de Lalande, who allowed him to proof-read parts of the second edition of his book, L'Astronomie. In 1772, Lalande got Méchain a position as an assistant hydrographer at the Depot of Maps and Charts of the Navy in Versailles. In 1774, Méchain became the calculator with the Depot of the Navy. Then he met Charles Messier, who worked for the same department, but at the smaller observatory at the Hôtel de Clugny. Around this time they became friends and began to work together occasionally. Méchain was first involved in surveys of the French coastline. He also occasionally had to make observations at Versailles. Later in 1774, he observed an occultation of Aldebaran by the Moon, which he later presented as a memoir to the Academy of Sciences. To give one a figure of how big Aldebaran is, imagine our Sun but forty times as wide.


In 1777, Méchain married Barbe-Thérèse Marjou whom he met while working in Versailles. They had two sons: Jérôme, and Augustin, and one daughter who's name I did not find.
Like Messier, Méchain became extremely devoted to comet observing and discovering new ones. He also started to stumble upon nebulous objects, and between 1779 and 1782, discovered a considerable number of thirty deep sky objects, twenty six of which were first discovered by him. He almost instantly discussed his observations with Charles Messier, who usually checked their positions and added them to his catalog. Both astronomers undertook a vigorous effort to find more nebulae between late August 1780 and March 1781, when the manuscript for the final version of the Messier catalog was sent out to print. Méchain's last two contributions, M102 and M103, went into the publication unchecked and without positions. Four other findings missed the publication; these are now known as M104, M105, M106, and M107. He sent them to Bernoulli, the editor of the Berliner Astronomisches Jahrbuch at the time. Since these four objects were not contained in the original Messier catalog, they were attributed separately to Pierre Méchain, John Herschel, and J.L.E. Dreyer. In this same letter, Méchain disclaimed his discovery of M102 as an erroneous re-observation of M101, thereby initiating a still open discussion on the true founder of this object.
In this letter he also mentioned the objects listed in Messier's catalog with M97 which are now recognized as M108 and M109 after their addition proposed by Owen Gingerich. Moreover, Pierre Méchain stated to have observed some more nebulae in the region of the Virgo Cluster which Messier had not included in his catalog, but unfortunately he did not give any credit to Méchain for this discovery.


Méchain discovered his first two comets in 1781, and because of his mathematical skills, he was able to calculate their orbits. In particular, he investigated the orbits of the comets of 1532 and 1661, and disproved the common hypothesis at the time that these were the same object. This work won the Grand Prix of 1782 of the Academy of Sciences, and was the main reason that he became a member of the Academy of Sciences in 1782. During the 1780s, Méchain began numerous surveys to produce maps of Germany and Northern Italy. In 1785, Pierre Méchain became editor of the Connoissance des Temps, the journal which had published the Messier Catalog. Méchain was principle editor of the Connoissance des Temps from 1788 to 1794. In 1787, Méchain collaborated with J.D. Cassini and Legendre on measuring the accurate longitude difference between Paris and Greenwich. At this time all three visited William Herschel at his observatory in Slough, England.


In 1791, Méchain undertook the southern part of a new survey of the meridian from Dunkirk to Barcelona, together with an assistant, Tranchot. The operation began in June 25, 1792, suffering from various obstacles from the French revolution: For example, Méchain and Tranchot got arrested by revolutioneers in Essone, who first mistook their telescopes as weapons, but eventually freed them. Shortly after this, war broke out between France and Spain, and he unfortunately was drafted into the war. Nevertheless, he discovered another comet, his 7th, from Barcelona on January 10, 1793. During the terror regime in Paris, while he was away, all of his property was confiscated, and his family suffered immensely. Once he returned, he became a member of the new Academy of Sciences, and the Bureau of Longitudes. Moreover, he was made director of the Paris Observatory, where he discovered his 8th and last comet on December 26, 1799; he also received help from Messier to find its orbit. Unfortunately shortly after this discovery, Pierre Méchain caught yellow fever and died in Castillion de la Plana in Spain on September 20, 1804.

Friday, January 7, 2011

APOD 2.7


Light Everywhere (7 Jan. 2011)

             What is being shown in this photograph is the hundreds of billions of stars within the vast Milky Way. What I found most interesting about this photo was actually the process of taking the photo and making it as you see now. This is because along with many other things, photography is a large part of astronomy because what can't be explained through words and facts can be more easily explained through a photograph. This photograph is a panorama made with eight sets of five photos at eight seconds each. Much exposure was required for the galaxy so the foreground of course is a bit overexposed. Also the shooting star that you see required about fifty different shots. I believe it is important not only to praise the astronomers for all they have discovered about our vast universe but also the photographers and artists who are able to put the astronomer's vision into a sort of reality.

Biography Sources - Pierre Méchain

  • Connor, J.J. O' "Mechain Biography." MacTutor History of Mathematics. Web. 6 Jan. 2011.       <http://www-history.mcs.st-and.ac.uk/Biographies/Mechain.html>.
  •  Frommert, Hartmut. "Pierre Méchain (1744-1804)." SEDS. 19 May 2009. Web. 6 Jan. 2011. <http://seds.org/messier/xtra/history/pmechain.html>.
  • Kenneth Glyn Jones, 1991. Messier's Nebulae and Star Clusters. 2nd ed, Cambridge University Press, p. 335-6. 6 Jan. 2011
  • OPTCorp. "Méchain, Pierre François André - OPT Telescopes." Meade Telescopes, Celestron Telescopes and Telescope Accessories - OPT Telescopes. Web. 6 Jan. 2011. <http://www.optcorp.com/edu/articleDetailEDU.aspx?aid=2446>.