Explanation: How much mass do flocculent spirals hide? The above true color image of flocculent spiral galaxy NGC 4414 was taken with the Hubble Space Telescope to help answer this question. Flocculent spirals -- galaxies without well defined spiral arms -- are a quite common form of galaxy, and NGC 4414 is one of the closest. Stars and gas near the visible edge of spiral galaxies orbit the center so fast that the gravity from a large amount of unseen dark matter must be present to hold them together. Pictured above is the photogenic center of NGC 4414. A bright foreground star from our Milky Way Galaxy shines in the foreground of the image. Although NGC 4414's center likely holds little dark matter, understanding its matter distribution helps calibrate the rest of the galaxy and, by deduction, flocculent spirals in general. By determining a precise distance to NGC 4414, astronomers also hope to help calibrate the scale to the more distant universe.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: spiral galaxy - NGC 4414 - flocculence - spiral'naya galaktika Publikacii so slovami: spiral galaxy - NGC 4414 - flocculence - spiral'naya galaktika
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