February 29, 2008

Willem De Sitter

Willem De Sitter was born in Sneek on May 6, 1872. He was a Dutch astronomer and mathematician. In his early years, he had done experimental work for physics at the astronomical laboratory of Jacobus C. Kapteyn. He was also involved in measuring photographic plates from the Cape Observatory in South Africa to chart the southern skies.

In 1897, De Sitter began working on celestial mechanics and stellar photometry. He worked with others to measure the four Galilean satellites of Jupiter. He calculated the mass of the satellites from perturbations in its orbit. Then, he published the results in his New Mathematical Theory of Jupiter's Satellites in 1925.

In 1908, he was professor of theoretic astronomy of the University of Leiden. Then, he was appointed the chair of astronomy at the university. From 1919 up until his death, he was also the director of their Observatory.

In 1932, he and Einstein co-authored a paper where they argued the existence of dark matter, where there's a large amount of matter but they do not emit light. Afterwards, De Sitter proposed the de Sitter universe which was in contrast to the Einstein universe. Einstein had came up with a static universe from solving equations of his general relativity theory. But De Sitter came across another solution to the equation. He was able to solve it even if no matter were present. De Sitter concluded that space can't be in a stable equilibrium. So, Einstein's universe had matter but no motion while de Sitter's had motion but no matter. A few years after, two Russian mathematicians indepently came up with the idea of an expanding universe with moving matter. De Sitter's universe could now be transformed into an expanding universe. Ultimately, it combined with Einstein's universe to form the Einstein-de Sitter universe which contained normal Euclidean space and a simple curved space. It formulated the idea that the universe is expanding at a decreasing rate that gets closer and closer to zero.

In 1919, he was operated for gallstones. But the overdose of ether that was given caused his health to degenerate. He also had tuberculosis which made him spend two years in Switzerland. But, he still continued his research and carried out observational studies. In his lifetime, he received the Gold medal of the Royal Astronomical Society and the Bruce Medal of the Astronomical Society of the Pacific. From 1925 to 1928, he was the president of the International Astronomical Union. Then on November 19, 1934, he passed away from illness.

3.8 APOD

Dawn of the Large Hadron Collider
Wow there's so much going on in this picture. At first glance, I thought it was a view from above some tall structure looking down. But then, I saw the little guy standing in the middle. Apparently you're looking straight through the tunnel. This is the most powerful particle accelerator called the Large Hadron Collider. This operation will start going into effect this May, exploring the many wonders surrounding the property of mass.

February 14, 2008

3.6 APOD

Long Stem Rosette
This is a nice picture for Valentine's Day...a nebula that looks like a rose! The petals of the "rose" were shaped by the winds and radiation from its central cluster of hot young stars. While the stars in the cluster is only a few million years old, the central cavity of this Rosette Nebula is about 50 light years in diameter. I like how they colored this pink too so it looks so nice.

February 7, 2008

3.5 APOD

Light Echoes from V838 Mon
Wow! This looks like a big furball dispersed in the night sky. Apparently, this V838 Mon's outer surface expanded so much that it suddenly became the brightest star in the entire Milky Way Galaxy. While there are material being expelled into space, the light echo is being reflected by distant rings around the star. This just looks so unreal!

February 1, 2008

3.4 APOD

Young Star Cluster Westerlund 2
That looks so cool, especially the way they colored it and made it look more mysterious. The central part is so full of hot stars that you can see the bright orange glow coming from it. Westerlund 2 has some of our galaxy's mostluminous, massive, and short lived stars. That little square area is actually 50 light years wide.