Credit & Copyright: Michael Sherick
Explanation:
NGC 1333 is seen in visible light as
a reflection
nebula,
dominated by bluish hues characteristic of starlight reflected by
interstellar dust.
A mere 1,000 light-years distant toward the heroic constellation
Perseus,
it lies at the edge of a large,
star-forming
molecular cloud.
This telescopic close-up spans about two full moons on the sky or just over
15 light-years at the estimated distance of NGC 1333.
It shows details of the dusty region
along with telltale hints of contrasty red emission from
Herbig-Haro
objects, jets and shocked glowing gas
emanating from recently formed stars.
In fact, NGC 1333 contains hundreds of stars less than
a million years old, most still
hidden
from optical telescopes
by the pervasive stardust.
The chaotic environment may be similar to one in which our own Sun
formed over 4.5 billion years ago.
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A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Публикации с ключевыми словами:
reflection nebula - star formation - отражательные туманности - звездообразование
Публикации со словами: reflection nebula - star formation - отражательные туманности - звездообразование | |
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