Destrokk

Can we bring yesterday back around? ´cause I know how I feel about you now. :blank:

congratulations on this

xyloto comes from xylophone and they just made it rhyme with mylo does this answer your question?

In my country its to be a good Mexican :surprised:

After reading this thread, you guys need to chill out man. I regret so much showing everybody I know that i liked Coldplay. Every moment I mentioned them, I don´t even know why I have friends now.. and you might think now, ¨whatevs i´ll be a fan forevah¨ But really this could just be a long fad and then you´ll regret all of you crazy fandom because you know what people are telling you behind your back? Things like, ¨you need a life¨ ¨you need a boyfriend¨ ¨..you´re too obsessed..¨ and then what? You could ignore but just save all of that regret :blank: DO IT NOW. And also, if people don´t like a band then thats their opinion, ok? Thats like asking, Why do people hate Justin Bieber? Why do people think his voice sounds like a girl? Why to people call him fag and want to kill him? Its just opinion, I wont say, oh fuck them! because its their opinion. Not everyone in the world has to love them :blank:

omfjhuyrhug

:heart: yahoo answers :heart:

Electron Degeneracy Electron degeneracy is a stellar application of the Pauli Exclusion Principle, as is neutron degeneracy. No two electrons can occupy identical states, even under the pressure of a collapsing star of several solar masses. For stellar masses less than about 1.44 solar masses, the energy from the gravitational collapse is not sufficient to produce the neutrons of a neutron star, so the collapse is halted by electron degeneracy to form white dwarfs. This maximum mass for a white dwarf is called the Chandrasekhar limit. As the star contracts, all the lowest electron energy levels are filled and the electrons are forced into higher and higher energy levels, filling the lowest unoccupied energy levels. This creates an effective pressure which prevents further gravitational collapse. Neutron Degeneracy Neutron degeneracy is a stellar application of the Pauli Exclusion Principle, as is electron degeneracy. No two neutrons can occupy identical states, even under the pressure of a collapsing star of several solar masses. For stellar masses less than about 1.44 solar masses (the Chandrasekhar limit), the energy from the gravitational collapse is not sufficient to produce the neutrons of a neutron star, so the collapse is halted by electron degeneracy to form white dwarfs. Above 1.44 solar masses, enough energy is available from the gravitational collapse to force the combination of electrons and protons to form neutrons. As the star contracts further, all the lowest neutron energy levels are filled and the neutrons are forced into higher and higher energy levels, filling the lowest unoccupied energy levels. This creates an effective pressure which prevents further gravitational collapse, forming a neutron star. However, for masses greater than 2 to 3 solar masses, even neutron degeneracy can't prevent further collapse and it continues toward the black hole state.

Okay goodnight kat :heart: Anette*

DSITRACTIONS i love cats

Viri :heart: I know it´s damn hard, Its like you want to just move on so badly but UGH he just stays in your mind and this is probably making it worse :disappointed:

that smiley makes me laugh like lol that heart has a face

K A T Chris did a skit on SNL... :heart:

Kind of sounds all the same to me, I think in mexico it´s a little more pop rock or dreamy but still kind of crappy.

:hug:

korean pop? :surprised: what is this?

you´re 13 and i have a problem with that

pew pew pew

THE MATRIX

Why don´t you :elephant: yourself.

:blank:

can we ask you for advice?

it´s a quincianera that was waited for 3 years and then OOPS WOOPS no one is going AWESOME

damn it i was going to this party and no one i know is going WRuyfurrwefFR

lol jonas bjerre