Posted 16 hours ago
hey tav are you and catfox doing it
Anonymous asked

O-Oh my~ Anon-kun…you’re being so direct…I-I don’t know what to say~

Posted 16 hours ago
rarityfox:

tav you think this is a game?


(ノ╥ω╥)ノ♥ n-nyo?

rarityfox:

tav you think this is a game?

(ノ╥ω╥)ノ♥ n-nyo?

Posted 16 hours ago
[Flash 10 is required to watch video]

rarityfox:

tav

rarity

Posted 16 hours ago

rarityfox:

tavangel:

rarityfox:

mfw tav

LOL NO JUST KIDDING

mfw rarity

LOL NOT KIDDING

get me another vanilla coke and i’ll touch yer hand for a second

I think you mean, you get to give me a coke for touching my hand~

Posted 17 hours ago

rarityfox:

mfw tav

LOL NO JUST KIDDING

mfw rarity

LOL NOT KIDDING

Posted 17 hours ago

d00dle b4 bed~

Posted 18 hours ago

catfoxrage:

laurangeblossom:

simple commission for Tav of Catfox’s character~

ORGYMFJDFJKDFNHJGFOMGOMGOGMI CQN I CQNCANt AAAAGSGFKJF

WHAT A CUTIEFOX ~<3

Posted 22 hours ago
It is not the strongest or the most intelligent who will survive but those who can best manage change.
Charles Darwin (via sushi-cupcake)
Posted 1 day ago
lespritmodeste:

A coronary angiogram is a procedure that uses X-ray imaging to see the inside of the heart’s blood vessels.

lespritmodeste:

A coronary angiogram is a procedure that uses X-ray imaging to see the inside of the heart’s blood vessels.

Posted 2 days ago

ikenbot:

How Did Galaxies Form?

Image: M81 Spiral galaxy Credit: NASA Spitzer Space Telescope

This is one of the questions we still don’t have a conclusive answer to, but as scientists search the cosmos for clues, the mystery becomes clearer.

Galaxies probably began to form less than a billion years after the Big Bang, which occurred around 13.7 billion years ago. The primordial Universe consisted almost entirely of hydrogen and helium gas, as well as dark matter, and was, for a time, almost completely homogeneous. It is believed that hypothetical dark matter played a major role in the formation of galaxies and the advent of a heterogeneous Universe. Clouds of gas first began clumping together due to the accumulation of primordial fluctuations, which were small changes of the density in certain parts of the early Universe. Through gravity, gas and dark matter were drawn towards the denser regions of the Universe.

There are two main hypotheses on how galaxies began to form, both of which are based on the gravitational effects of collapsing gas. One is called the “bottom-up” theory, in which giant clouds of gas came together in small clumps, which then merged to form larger galaxies. The second theory is the “top-down” one, in which clouds of gas the size of multiple galaxies broke down into individual clumps. This theory would explain why galaxies occur in clusters, and is the most widely accepted model.

Hydrogen and helium gas were then drawn towards the inner part of protogalaxies while dark matter formed a halo surrounding the outer part. The gas within these infant galaxies also began to clump together and heat up, forming the first stars. In the beginning, matter in the Universe was composed almost exclusively of hydrogen and helium. Nuclear fusion within stars (and during supernovae) would help make the rest of the heavier elements.