Saturday, 28 March 2009

ISS Now 2nd Brightest Object in Night Sky

Screen shot from NASA TV during the solar array deployment. Credit: NASA TV


The International Space Station should now be the second brightest object in the night sky, following Friday's successful deploy of the S6 solar wings. Astronauts on board the ISS and space shuttle Discovery unfurled the arrays, successfully carrying out the main objective of the STS-119 mission. "Today was a great day," said ISS commander Mike Fincke to mission control Friday afternoon. "Today is the day the station went to full power." The length of the arrays unfurled Friday measures 73 meters (240 feet), tip to tip, with the S6 truss in between. The S6 solar array pair adds 2,926 892 square meters (9,600 square feet) to the station solar arrays, bringing the total surface area to nearly an acre. The station’s arrays now will generate as much as 120 kilowatts of usable electricity, enough to power about 42 854 260 square meter (2800-square-foot) homes.



The station should now be the second brightest object in the night sky – even brighter than Venus, and second only to the Moon.

Galaxies: Galaxy M42



Calling all astro-photo geeks! (as well as those of us that just like to look). The Royal Observatory in Greenwich, England is offering a brand new, free competition and exhibition for everyone who loves the night sky. It's open to anyone, from anywhere, including a special category for astro-photo buffs under the age of 16. There are some great prizes up for grabs and winning entries will be displayed in a special exhibition at the Royal Observatory. This competition is an International Year of Astronomy event, and from all the photos submitted, a giant, zoomable photo-collage of the Universe will be created. Even if you're not a photographer, anyone interested in astronomy can go to the gallery on Flickr and soak in the eye candy. The competition has been open for a while (and ends on July 19, 2009) and there are some awesome images taken by people from all around the world – some are absolutely breathtaking, like the image above taken by Dave Thompson.

Saturday, 14 March 2009

Infinity and the Universe


The word infinity comes from the Latin infinitas or "unboundedness." It refers to several distinct concepts which arise in philosophy, mathematics, theology and everyday life. Popular or colloquial usage of the term often does not accord with its more technical meanings.


In Greek philosophy, for example in Anaximander, 'the Boundless' is the origin of all that is. He took the beginning or first principle to be an endless, unlimited primordial mass (apeiron)


In Judeo-Christian theology, for example in the work of theologians such as Duns Scotus, the infinite nature of God invokes a sense of being without constraint, rather than a sense of being unlimited in quantity. In philosophy, infinity can be attributed to space and time, as for instance in Kant's first antinomy. In both theology and philosophy, infinity is explored in articles such as the Ultimate, the Absolute, God, and Zeno's paradoxes.


In mathematics, infinity is relevant to, or the subject matter of, limits, aleph numbers, classes in set theory, Dedekind-infinite sets, large cardinals, Russell's paradox, hyperreal numbers, projective geometry, extended real numbers and the absolute Infinite.


In popular culture, we have Buzz Lightyear's rallying cry, "To infinity - and beyond!", which may also be viewed as the rallying cry of set theorists considering large cardinals.


For a discussion about infinity and the physical universe, see Universe.


The precise origins of the infinity symbol 8 are unclear. One possibility is suggested by the name it is sometimes called - the lemniscate, from the Latin lemniscus, meaning "ribbon." One can imagine walking forever along a simple loop formed from a ribbon.



A popular explanation is that the infinity symbol is derived from the shape of a Möbius strip. Again, one can imagine walking along its surface forever. However, this explanation is improbable, since the symbol had been in use to represent infinity for over two hundred years before August Ferdinand Möbius and Johann Benedict Listing discovered the Möbius strip in 1858.



It is also possible that it is inspired by older religious/alchemical symbolism. For instance, it has been found in Tibetan rock carvings, and the ouroboros, or infinity snake, is often depicted in this shape. In the tarot, the lemniscate represents the balance of forces and is often associated with the magician card.



John Wallis is usually credited with introducing 8 as a symbol for infinity in 1655 in his De sectionibus conicis. One conjecture about why he chose this symbol is that he derived it from a Roman numeral for 1000 that was in turn derived from the Etruscan numeral for 1000, which looked somewhat like CI? and was sometimes used to mean "many." Another conjecture is that he derived it from the Greek letter (omega), the last letter in the Greek alphabet.

Saturday, 7 March 2009

Fate of the Universe


The theoretical scientific exploration of the ultimate fate of the universe became possible with Albert Einstein's 1915 theory of general relativity. General relativity can be employed to describe the universe on the largest possible scale. There are many possible solutions to the equations of general relativity, and each solution implies a possible ultimate fate of the universe. Alexander Friedmann proposed one such solution in 1921. This solution implies that the universe has been expanding from an initial singularity; this is, essentially, the Big Bang.


An important parameter in fate of the universe theory is the density parameter, Omega (O), defined as the average matter density of the universe divided by a critical value of that density. This creates three possible ultimate fates of the universe, depending on whether O is equal to, less than, or greater than 1. These are called, respectively, the Flat, Open and Closed universes. These three adjectives refer to the overall geometry of the universe, and not to the local curving of spacetime caused by smaller clumps of mass (for example, galaxies and stars).


Observational evidence was not long in coming. In 1929, Edwin Hubble published his conclusion, based on his observations of Cepheid variable stars in distant galaxies, that the universe was expanding. From then on, the beginning of the universe and its possible end have been the subjects of serious scientific investigation. In 1933, Georges-Henri Lemaître set out a theory that has since come to be called the Big Bang theory of the origin of the universe. In 1948, Fred Hoyle set out his opposing theory of a static universe, called the Steady state theory. These two theories were active contenders until the 1965 discovery, by Arno Penzias and Robert Wilson, of the cosmic microwave background radiation, a fact that is a straightforward prediction of the Big Bang theory, and one that the Steady State theory cannot account for. The Big Bang theory immediately became the most widely held view of the origin of the universe.