Credit & Copyright: Daniel López,
IAC
Explanation:
NGC 2438
is a planetary nebula,
the gaseous shroud cast off
by a dying sunlike star billions of years old whose
central reservoir of hydrogen fuel has been exhausted.
About 3,000 light-years distant it lies within the boundaries of
the nautical
constellation
Puppis.
Remarkably, NGC 2438
also seems to lie on the outskirts of bright,
relatively young open star cluster M46.
But this planetary nebula's
central
star is not only much older than the stars of M46,
it moves through space at a different speed than the cluster stars.
Distance estimates also place NGC 2438
closer than M46 and
so the nebula appears in the foreground,
only by chance along the line-of-sight to the young star cluster.
This deep image of NGC 2438
highlights a previously unseen
halo of glowing atomic gas over 4.5 light-years across, extending
beyond the nebula's brighter inner ring.
Similar haloes have been found in deep images of other
planetary nebulae,
produced during the earlier active phases of their aging
central stars.
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Publikacii s klyuchevymi slovami:
NGC 2438 - M 46 - planetary nebula - gas - Planetarnaya tumannost' - gaz - galo - halo
Publikacii so slovami: NGC 2438 - M 46 - planetary nebula - gas - Planetarnaya tumannost' - gaz - galo - halo | |
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