Telescope captures turning point in star's death
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| This
photo, taken at different wavelengths, shows the surrounding ring-shaped
region of gas and dust cast off by the star |
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March 20, 1998
Web posted at: 10:51 a.m. EDT (1051 GMT)
WASHINGTON (Reuters) -- The Hubble Space Telescope has captured a turning
point in the death of a sun-like star: the instant when the hydrogen and
helium at the star's core are flung into interstellar space to create more
heavenly bodies.
"This is probably very much like what will happen to the sun," astronomer
William Latter said Thursday as the new Hubble images were released by
the Space Telescope Science Institute.
However, our sun is much younger than the star snapped in the new pictures,
and will not approach this phase for about 4.5 billion years, Latter said
in a telephone interview from the California Institute of Technology.
This brief period in the stellar death process actually lasts about
1,000 Earth years, a mere blink in cosmological time.
Image Gallery
When a star starts to die, Latter said, the nuclear fuel at its heart
runs out, and a very dense, cool shell of hydrogen molecules is deposited
around the star. This molecular shell cannot be seen by the naked eye,
but Hubble's infrared camera was able to snap its image.
The dying star in question, known as NGC7027 and located 3,000 light-years
from the sun in the direction of the constellation Cygnus the Swan, is
seen in the new pictures as a glowing white ball surround by red wisps
of the dissipating molecular shell.
The molecular shell is atomized and the resulting atoms are flung into
space as the most primitive building blocks for other stars, planets and
any life that may form on them, Latter said.
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| Two
planetary nebulae emerge from wrappings of gas and dust like butterflies
breaking out of their cocoons |
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"What's new about these images is we're able to see a very thin transition
between the ionized region and the formerly invisible atmosphere on the
star," he said.
Also on Thursday, the telescope institute released images of two other
dying stars that look like butterflies emerging from their cocoons.
These two -- known as the Cotton Candy nebula and the Silkworm nebula
-- show the moribund stars blowing off shells of gas that surrounded them
after their nuclear cores were exhausted.
The gaseous shells give the stars their butterfly-wing shape, astronomers
said in a statement.
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