The Fibonacci Sequence As Seen in Flowers gallery by Environmental Graffiti is a math and history lesson wrapped in a pretty...
NGC 3372: The Great Carina Nebula
One of our galaxy’s largest star-forming regions.
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[noun]
1. a fluid or viscous substance used for writing or printing.
2 .a dark, protective fluid ejected by the...
BigBlast_small.mov (by SDOmission2009)
cwnl:
Comet colliding with the Sun coincides with a coronal mass ejection. Image from the NASA SOHO Observatory.
(via ikenbot)
NASA SDO - Solar Eclipse May 3, 2011 (Moon Transit) (by LittleSDOHMI)
(via ikenbot)
Green flashes and green rays are optical phenomena that occur shortly after sunset or before sunrise, when a green spot is visible, usually for no more than a second or two, above the sun, or a green ray shoots up from the sunset point. […]
The reason for a green flash lies in refraction of light (as in a prism) in the atmosphere: light moves more slowly in the lower, denser air than in the thinner air above, so sunlight rays follow paths that curve slightly, in the same direction as the curvature of the Earth. Higher frequency light (green/blue) curves more than lower frequency light (red/orange), so green/blue rays from the upper limb of the setting sun remain visible after the red rays are obstructed by the curvature of the earth.
Green flashes are enhanced by mirage, which increase the density gradient in the atmosphere, and therefore increase refraction. A green flash is more likely to be seen in clear air, when more of the light from the setting sun reaches the observer without being scattered. We might expect to see a blue flash, but the blue is preferentially scattered out of our line of sight and remaining light ends up looking green.
With slight magnification a green rim on the top limb of the solar disk can be seen on most clear-day sunsets. However the flash or ray effects require a stronger layering of the atmosphere and a mirage which serves to magnify the green for a fraction of a second to a couple of seconds.
There are problems with the explanation of the cause of the green flash. The refractive index of air is 1.0003 compared with about 1.5 for glass, which means that a ray of light will suffer little refraction in the atmosphere, i.e. the ray will continue in almost the same direction as that before encountering the atmosphere. Further, there is the question of why the flash is of such a small area considering the size of the sun’s image. There are many unanswered questions relating to this phenomenon. […] (via wikipedia- green flash)
Monster Prominence Erupts from the Sun
When a rather large M 3.6 class flare occurred near the edge of the Sun on Feb. 24, 2011, it blew out a gorgeous, waving mass of erupting magnetic plasma that swirled and twisted for 90 minutes. NASA’s SDO captured the event in extreme ultraviolet light.
Because SDO images are high definition, the team was able to zoom in on the flare and still see exquisite details. And using a cadence of a frame taken every 24 seconds, the sense of motion is, by all appearances, seamless.
(via fuckyeahspace)