like seriously
complaints
umadson [1] |
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Because breaking wind or belching releases part of the life force you are given upon your birth into the world |
Nosferatu [1] <Solo Act>
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It's gas, from your colon. The same place shit comes from. Seriously, you need an explanation..... |
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Farts are like the best thing in the world. They make a trumpet sound, smell like poo, and come out of your ass!! |
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Imagine if they came from somewhere else, like your nose o_O |
<Apex>
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Methane, probably because of other chemicals too though. |
12ed12um [43] |
because you touch yourself at night. |
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the only way you will really know for sure is if you calculate the mass of the sun and when it will burn out. |
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Both google-able pieces of information. |
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fuck that |
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Bots4 is the new Google. |
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How does google feel about being replaced? |
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That's kind of ironic. Without "google" none of this would be possible. |
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yes it would. what does google provide for bots4? (apart from analytics and forum search) |
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they pay for enders stuff. all of it. |
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Not all of it, I'm pretty sure my stars bought Ender two or three sandiwiches at least. |
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We know that the sun shines via nuclear reactions in the core that transform four hyrogen atoms into one helium atom. If you look at a periodic table, you will see that one helium atom has a little less mass than four hydrogen atoms combined; about 0.7% of the original mass has "disappeared". This "missing mass" gets transformed into energy, and this is the energy that causes the sun to shine. Therefore, using Einstein's famous formula E=mc^2 for the conversion between mass and energy we have that the available energy in the sun is: E = 0.007 x M c^2 where c is the speed of light and M is the amount of mass in the sun that is capable of undergoing the above nuclear reactions. Now, it turns out that only the central part of the sun is at a high enough temperature to actually undergo these reactions. You would need to use a detailed model of the sun's structure to figure out exactly how much of the sun is at a high enough temperature, but if we're just estimating things we can say that on the order of 10% of the sun's mass is in the central part of the sun where it is hot enough to undergo nuclear reactions. We then have: E = 0.007 x 0.1 x Msun c^2 where Msun is the total mass of the sun, 2 x 1030 kilograms. We therefore can calculate that the total energy the sun has to burn is around 1.3 x 1044 Joules. Dividing 3.8 x 1026 Watts (the rate at which the sun is giving off energy) into this number gives an approximate value of 10 billion years for the sun's lifetime. -thanks Google. |
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How ignorant.. we all know god created everything.. therefore god also is responsible for the creation of google and all of mans knowledge. THANK GOD. |
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Amen brother |
Nosferatu [1] <Solo Act>
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Gods* Just like men, it always takes more than one. |