can't stop moving to the funky, funky beat
mia - 18 - sydney - butts
can't stop moving to the funky, funky beat
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science-junkie:

What is the Multiverse, and why do we think it exists? 
[…] Our observable Universe caps out at about 92 billion light-years in diameter, less than a thousand times as large in all directions as our previous scale. It contains some 10^80 atoms, clumped together in maybe a trillion galaxies, each with typically hundreds of billions of stars. But one of the most remarkable things about the Big Bang is that all of this, some 13.8 billion years ago, was once contained in a very small region of space, a region much smaller than our Solar System is today!
The thing that you might immediately wonder is whether there’s more Universe beyond the part that’s observable to us today, and — if so — how far does it go on? And what does it look like? And what are the physical laws in that part of the Universe?
Based on our observations of everything we’ve been able to see, from stars to galaxies to the leftover glow from the Big Bang to the matter in intergalactic space, we can learn some amazing things.
Read the full article by Ethan Siegel
science-junkie:

What is the Multiverse, and why do we think it exists? 
[…] Our observable Universe caps out at about 92 billion light-years in diameter, less than a thousand times as large in all directions as our previous scale. It contains some 10^80 atoms, clumped together in maybe a trillion galaxies, each with typically hundreds of billions of stars. But one of the most remarkable things about the Big Bang is that all of this, some 13.8 billion years ago, was once contained in a very small region of space, a region much smaller than our Solar System is today!
The thing that you might immediately wonder is whether there’s more Universe beyond the part that’s observable to us today, and — if so — how far does it go on? And what does it look like? And what are the physical laws in that part of the Universe?
Based on our observations of everything we’ve been able to see, from stars to galaxies to the leftover glow from the Big Bang to the matter in intergalactic space, we can learn some amazing things.
Read the full article by Ethan Siegel
science-junkie:

What is the Multiverse, and why do we think it exists? 
[…] Our observable Universe caps out at about 92 billion light-years in diameter, less than a thousand times as large in all directions as our previous scale. It contains some 10^80 atoms, clumped together in maybe a trillion galaxies, each with typically hundreds of billions of stars. But one of the most remarkable things about the Big Bang is that all of this, some 13.8 billion years ago, was once contained in a very small region of space, a region much smaller than our Solar System is today!
The thing that you might immediately wonder is whether there’s more Universe beyond the part that’s observable to us today, and — if so — how far does it go on? And what does it look like? And what are the physical laws in that part of the Universe?
Based on our observations of everything we’ve been able to see, from stars to galaxies to the leftover glow from the Big Bang to the matter in intergalactic space, we can learn some amazing things.
Read the full article by Ethan Siegel
science-junkie:

What is the Multiverse, and why do we think it exists? 
[…] Our observable Universe caps out at about 92 billion light-years in diameter, less than a thousand times as large in all directions as our previous scale. It contains some 10^80 atoms, clumped together in maybe a trillion galaxies, each with typically hundreds of billions of stars. But one of the most remarkable things about the Big Bang is that all of this, some 13.8 billion years ago, was once contained in a very small region of space, a region much smaller than our Solar System is today!
The thing that you might immediately wonder is whether there’s more Universe beyond the part that’s observable to us today, and — if so — how far does it go on? And what does it look like? And what are the physical laws in that part of the Universe?
Based on our observations of everything we’ve been able to see, from stars to galaxies to the leftover glow from the Big Bang to the matter in intergalactic space, we can learn some amazing things.
Read the full article by Ethan Siegel
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effiearts:

more inking class homework, with digital tones
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fleurdulys:

The Blue Room - Paul Ranson
1891
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euo:

India K
euo:

India K
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gragriel:

Man Ray, Lágrimas (1930)
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radagraphic:

Sol III by Yo no me llamo Javier on Flickr.
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likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
likeafieldmouse:

Alexey Kovalev - Humble Days (2009-12)
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Wassily Kandinsky, “Tanzkurven: Zu den Tänzen der Palucca,” Das Kunstblatt, Potsdam, vol. 10, no. 3 (1926)
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