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Into the Eye of the Helix
Helix Nebula, NGC 7293, Caldwell 63
RA 22h 29m 48.20s Dec. -20° 49' 26.0"
About 700 light years
February 25, 2009
Other images: N0311 N0432 N0601 N0703 N0907 N1205 N1211
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ABOUT THIS IMAGE:
A deep new image of the magnificent Helix planetary nebula has been obtained using the Wide Field Imager at ESO's La Silla Observatory. The image shows a rich background of distant galaxies, usually not seen in other images of this object.
The Helix Nebula, NGC 7293, lies about 700 light-years away in the constellation of Aquarius (the Water Bearer). It is one of the closest and most spectacular examples of a planetary nebula. These exotic objects have nothing to do with planets, but are the final blooming of Sun-like stars before their retirement as white dwarfs. Shells of gas are blown off from a star's surface, often in intricate and beautiful patterns, and shine under the harsh ultraviolet radiation from the faint, but very hot, central star. The main ring of the Helix Nebula is about two light-years across or half the distance between the Sun and its closest stellar neighbor.
Despite being photographically very spectacular the Helix is hard to see visually as its light is thinly spread over a large area of sky and the history of its discovery is rather obscure. It first appears in a list of new objects compiled by the German astronomer Karl Ludwig Harding in 1824. The name Helix comes from the rough corkscrew shape seen in the earlier photographs.
Although the Helix looks very much like a doughnut, studies have shown that it possibly consists of at least two separate discs with outer rings and filaments. The brighter inner disc seems to be expanding at about 100 000 km/h and to have taken about 12 000 years to have formed.
the Helix is relatively close - it covers an area of the sky about a quarter
of the full Moon - it can be studied in much greater detail than most
other planetary nebulae and has been found to have an unexpected and complex
structure. All around the inside of the ring are small blobs, known as
"cometary knots", with faint tails extending away from the central
star. They look remarkably like droplets of liquid running down a sheet
of glass. Although they look tiny, each knot is about as large as our
Solar System. These knots have been extensively studied, both with the
ESO Very Large Telescope and with the NASA/ESA Hubble Space Telescope,
but remain only partially understood. A careful look at the central part
of this object reveals not only the knots, but also many remote galaxies
seen right through the thinly spread glowing gas. Some of these seem to
be gathered in separate galaxy groups scattered over various parts of