Okay so here is the next part. Yup. I'm just going to nonchalantly shove it down your throat with some milk and barbecue sauce. Why that combination you ask? You don't get to ask, you have duct tape on your mouth. You have just now noticed the duct tape on your mouth. look down. look back up. nope still duct tape on your mouth. I lied. There was never duct tape on your mouth. It was masking tape. DUN DUN DUN. Except it wasn't. There was nothing. You've been in the drugs again haven't you. What? Don't give me that look. We both know you like dat Fun Dip. MMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMM Eucalyptus Okay, I got the real masking tape now. Here you go person's mouth, hope you are nice and cozy now. You will be even more cozy if you rip it off violently. Yup, blood circulation is nice, and so is water. I'm really fucking bored. This is occupying me a bit though. Rules of Nature another bit. Melting ice too. You know that this part was the worst when it came to exporting. This time my computer had TWO guns to its monitor. Luckily for me it doesn't have hands, the monitor isn't what it should be aiming at, and the guns are just imaginary. Seriously though, took forever for my computer to run at normal speed despite the exporting finishing. It's like I was watching a movie, but with no popcorn and a drastically reduced screen. 100/10 Michael bay doesn't have shit on my suicidal computer. You know, I have come to a realization that a description should be describing things, like the video. So I'm going to provide a description for a part of the video. A star is a massive, luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Other stars, mostly in the Milky Way, are visible from Earth during the night, appearing as a multitude of fixed luminous points due to their immense distance. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime and, for some stars, by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, luminosity, and spectrum respectively. The total mass of a star is the principal determinant of its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung–Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined. - Taken from Wikipedia, Thank you Wikipedia!!! I would provide some MLA Citation but this isn't school, this is a description. Not as hardcore. Btw from reading this you should now know that our characters are gods. We are holding hundreds of stars on us like freaking skittles. Taste the radiation! I have one last message for you guys: PARTY HARD! PARTY HARD! PARTY HARD! PARTY HARD! PARTY HARD! PARTY HARD! PARTY HARD! I'm Kawaii bitch OAO

• published: 14 Jan 2015
• views: 2