wow can’t believe jupiter is actually trans <3
taylor price
todays bird
macklin celebrini has autism

roma★

blake kathryn
NASA
The Bowery Presents
Sweet Seals For You, Always

@theartofmadeline
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PUT YOUR BEARD IN MY MOUTH
Interview Vampire Daily
tumblr dot com
Xuebing Du
$LAYYYTER
official daine visual archive

izzy's playlists!

if i look back, i am lost
Fai_Ryy
EXPECTATIONS
seen from United States
seen from Germany
seen from Bangladesh

seen from United States
seen from United States
seen from Colombia
seen from Germany

seen from China
seen from Malaysia
seen from Malaysia
seen from Germany

seen from United States
seen from United States
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seen from United Kingdom

seen from Malaysia
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seen from Venezuela

seen from Germany
@techlime
wow can’t believe jupiter is actually trans <3
@grimes: There were Humans and Gods and nothing but Angels in between
my name is dark g r i m e s
Claire Against the Machine
Lana Del Rey photographed by Glen Luchford for Gucci Guilty campaign.
Outtakes for NFR album shoot.
Off to the races
American actress Jean Harlow (1911 - 1937) leans on a La Salle, 15th June 1932. (Photo via John Kobal Foundation Getty Images)
Ghost in the Shell (1995) Directed by Mamoru Oshii
Inside the Flame Nebula : The Flame Nebula stands out in this optical image of the dusty, crowded star forming regions toward Orion’s belt, a mere 1,400 light-years away. X-ray data from the Chandra Observatory and infrared images from the Spitzer Space Telescope can take you inside the glowing gas and obscuring dust clouds though. Swiping your cursor (or clicking the image) will reveal many stars of the recently formed, embedded cluster NGC 2024, ranging in age from 200,000 years to 1.5 million years young. The X-ray/infrared composite image overlay spans about 15 light-years across the Flame’s center. The X-ray/infrared data also indicate that the youngest stars are concentrated near the middle of the Flame Nebula cluster. That’s the opposite of the simplest models of star formation for the stellar nursery that predict star formation begins in the denser center of a molecular cloud core. The result requires a more complex model; perhaps star formation continues longer in the center, or older stars are ejected from the center due to subcluster mergers. via NASA
irene bedard in siege at wounded knee (1994)