Credit & Copyright: Infrared:
NASA,
ESA, M. Regan & B. Whitmore
(STScI), & R. Chandar
(U. Toledo);
Optical: NASA, ESA, S. Beckwith (STScI), & the Hubble Heritage Team (STScI/AURA)
Explanation:
How do spiral galaxies form stars?
To help find out, the
Hubble Space Telescope
imaged the nearby photogenic spiral
M51 in
infrared light to highlight the dust that traces the dense gas that best forms
stars.
To further isolate the
dust, much of the
optical light from stars has also been
digitally removed.
The resulting unique image shows swirling and intricate patterns on the longest
scales, while numerous bright clumps of previously hidden
open star clusters
appear on the smaller scales.
To see the
detailed optical light image
for comparison, run your cursor over the above image.
Anyone with a good pair of
binoculars can see the
Whirlpool toward the constellation
of the
Hunting Dogs
(Canes Venatici).
M51 lies about 30 million light years away, while the above imaged area spans about
15,000 light years from top to bottom.
Astronomers speculate that M51's
spiral structure is primarily due to its gravitational interaction with
a neighboring smaller galaxy.
Optical: NASA, ESA, S. Beckwith (STScI), & the Hubble Heritage Team (STScI/AURA)
Browse:
See the latest images submitted to APOD
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Publikacii s klyuchevymi slovami:
M 51 - Whirlpool galaxy - dust - infrared - galaktika Vodovorot - pyl' - infrakrasnoe izluchenie
Publikacii so slovami: M 51 - Whirlpool galaxy - dust - infrared - galaktika Vodovorot - pyl' - infrakrasnoe izluchenie | |
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