install theme
whynotdosomestuff: Exploring the city. (at Museum Of Science)
evenaskher: Girasol

ozzyosborntodie:

i want to be a librarian when i grow up because i’ll get paid to tell people to shut up 

madgay:

how to solve every problem ever

  • ignore it 
Rape of the Sabines
Airglow, Gegenschein, and Milky Way As far as the eye could see, it was a dark night at Las Campanas Observatory in the southern Atacama desert of Chile. But near local midnight on April 11, this mosaic of 3 minute long exposures revealed a green, unusually intense, atmospheric airglow stretching over thin clouds. Image Credit & Copyright: Yuri Beletsky (Las Campanas Observatory, Carnegie Institution) Unlike aurorae powered by collisions with energetic charged particles and seen at high latitudes, the airglow is due to chemiluminescence, the production of light in a chemical reaction, and found around the globe. The chemical energy is provided by the Sun’s extreme ultraviolet radiation. Like aurorae, the greenish hue of this airglow does originate at altitudes of 100 kilometers or so dominated by emission from excited oxygen atoms. The gegenschein, sunlight reflected by dust along the solar system’s ecliptic plane was still visible on that night, a faint bluish cloud just right of picture center. At the far right, the Milky Way seems to rise from the mountain top perch of the Magellan telescopes. Left are the OGLE project and du Pont telescope domes.
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