Credit & Copyright: Denis Priou
Explanation:
Galactic or
open star clusters
are young.
These swarms of stars are born together near the plane of the Milky Way,
but their numbers steadily dwindle as cluster members are
ejected by galactic tides and gravitational interactions.
In fact,
this
bright open cluster, known as M46, is around 300 million years
young.
It still contains a few hundred stars within a span of
30 light-years or so.
Located about 5,000 light-years away toward the
constellation
Puppis, M46
also seems to contain contradictions to its youthful status.
In this pretty starscape,
the colorful, circular patch above and right of the center of M46
is the planetary nebula NGC 2438.
Fainter still, a second planetary nebula, PK231+4.1,
is identified
by the box at the right and enlarged in the inset.
Planetary nebulae are a brief, final phase in the life of a sun-like
star a billion
years old or more,
whose central reservoir of hydrogen fuel has been exhausted.
NGC 2438
is estimated to be only 3,000 light-years distant, though, and
moves at a different speed than M46 cluster members.
Along with its fainter cohort, planetary nebula NGC 2438 is likely
only by chance
appearing near our line-of-sight to the young stars of M46.
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Публикации с ключевыми словами:
open cluster - planetary nebula - M 46 - Рассеянное скопление - Планетарная туманность
Публикации со словами: open cluster - planetary nebula - M 46 - Рассеянное скопление - Планетарная туманность | |
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