2005's photos by Reuters. An interesting 'around the world' tour in pictures; be aware that some photos are explicitly showing the crude reality in all its sadness while other ones just captures beauty in its simplicity. We are such strange creatures...
[ Reuters 2005 showcase ]
22 December 2005
Reuters showcase
13 December 2005
Rocketboom

Some could argue that my stance may slightly be tainted by the show’s anchorwoman: Amanda Congdon, while I certainly can’t deny that I find her charismatic, alluring and fun, this vlog is a real point of interest, from the concept to the daily content they present, it is addictive! Rocketboom covers a wide range of news every day; viewers can also suggest stories or add their comments about the show.
I applaud the well deserved success, using modest equipment and virtually no resources at all, their constant dedication and hard work finally paid off; as now, they measure up with some of the hottest comical TV shows out there!
So, if you want to keep up with the latest in an entertaining manner, save 3 minutes of your time to visit Rocketboom today, 100.001 visitors can be that wrong… everyday! ;-)
Rocketboom: [ www.Rocketboom.com ]
Amanda’s blog: Amanda unBoomed
More info on videoblogging: [ videoblogging ]
World Map of Video Blogs: [ vlogMap ]
08 December 2005
Our Sun's nuclear Nirvana

To achieve fusion on earth, scientists will use Hydrogen isotopes: deuterium and tritium. Isotopes are part of the same atomic species as their parent atom but with extra neutrons; therefore with a higher mass.
Fusion is routinely happening within the sun, thanks to the high temperatures (15 million °C) and huge pressure, hydrogen (simplest element, atomic number 1: H) atoms are transformed into Helium (atomic number 2: He, heavier element) by a proton-proton chain. Our Sun is made up of 92% hydrogen, 7.8% helium, and the remaining 0.2% is a mixture of other elements, this helps understand how it can continue to shine for another 5 billion years or so.

Now that we have a better understanding of the proportions, let's get back to our topic. Each second the sun produces 4 million tons of energy by transforming 600 million tons of H into 596 million tons of He. The produced energy is split as follows: 50% is infrared or heat energy, 40% comes out as visible light and most of the remaining is ultraviolet light.
What's even more impressive is that, due to the extreme density of the plasma core, it takes anywhere between 150.000 an a million year for that energy (mostly gamma rays, at the time, which is the highest energetic form of an electromagnetic radiation) to finally escape from the core and make its way to the outer regions of the sun (photosphere and chromosphere), the good news is that by then it has, among other things, been transformed into visible light and heat. About 8 minutes later, we can all enjoy the show on Earth!
As this is a rather complex and exciting topic, it is now clear that several posts will be required to fully appreciate the beauty of such dynamics. In later posts, I will approach, on a modest level and in a simplified way, fusion in more depth. How are the heavier elements of the periodic table forged? Which quantum principles are involved? What forces are at play?
Meanwhile, check out some stunning space-themed wallpapers: Space Wallpapers
To be continued...
India joins the nuclear fusion club
Iter will be the second largest science project in history after the International Space Station.
ITER - NUCLEAR FUSION PROJECT
Project estimated to cost 10bn euros and will run for 35 years
It will produce the first sustained fusion reactions
Final stage before full prototype of commercial reactor is built
After decades of experimentation at national and regional level, it should demonstrate once and for all whether it is possible to harness the tremendous potential of nuclear fusion in a practical and economic way.
Link: India joins Iter
More details: Step by step guide
If you missed the previous report about this kind of topic, read it here: [Focus Fusion]
Bamjan: Nepal Buddha boy

"A meditating teenage boy in south-central Nepal is drawing the attention of scientists after attracting huge crowds in the past six months and earning himself the name Buddha-reincarnate. [...] Ram Bahadur Bamjan's friends, relatives and managers say he has been meditating without drinking water for six months now and that he will carry on for another six years until he gains enlightenment." As a reminder: "Siddartha Gautam, who later attained Mahanirvana and became the Buddha, was born in 560 BC."
I fond the following quite intriguing, or is it just a mere coincidence: The name of Buddha's mother was Maya Devi exactly the same as this young boy's mother.
It is a very interesting read and a fascinating story, by BBC News: Scientists to check Nepal Buddha boy
07 December 2005
Echizen kurage
"Often the weight of the echizen kurage broke the nets or crushed the fish to death; those that survived were poisoned and beslimed by their tentacles. [...] The problem has become so serious that fishery officials from Japan, China and South Korea are to meet this month for a “jellyfish summit” to discuss strategies for dealing with the invasion."
"In some places jellyfish density is reported to be a hundred times higher than normal. Worst of all, no one yet understands why. One theory is that global warming is heating up the seawater and encouraging jellyfish breeding. " Richard Lloyd Parry
Read the complete story @ the Times: Nomura’s jellyfish
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New Year '05: One second later

This has been done many times before as Wendy Grossman from Scientific American reports: "The reason: Leap seconds are not new: 22 have been added since 1972, on June 30 or December 31. [...] Leap seconds are needed because the earth's spin is slowing down, gradually and unevenly. The rotational changes arise because of tidal forces exerted by the moon and inertial effects related to the liquid outer core sloshing around and to the cycle of evaporation, in which water at the equator gets deposited at the poles as ice that melts seasonally."
[ Wait a second! ]
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