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The Glowing Eye of NGC 6751
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Name: NGC 6751
Description: Planetary Nebula in the Milky Way Galaxy
Position: R.A. 19h 05m 58s   Dec. -05° 59' 20''
Constellation: Aquila

Distance: 6500 light-years (~2 kpc).
The diameter of the nebula is 24 arcseconds (about 0.8 light-years).
Instrument: WFPC2
Exposure Date: April 21, 1998
Exposure Time: 30 minutes
Filters: F502N ([O III]), F555W (V), F658N ([N II])
Image Credit: NASA and The Hubble Heritage Team (STScI/AURA)

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Astronomers using NASA's Hubble Space Telescope have obtained images of the strikingly unusual planetary nebula, NGC 6751.
Glowing in the constellation Aquila like a giant eye, the nebula is a cloud of gas ejected several thousand years ago from the hot
star visible in its center.

"Planetary nebulae" are named after their round shapes as seen visually in small telescopes, and have nothing else to do with
planets. They are shells of gas thrown off by stars of masses similar to that of our own Sun, when the stars are nearing the ends
of their lives. The loss of the outer layers of the star into space exposes the hot stellar core, whose strong ultraviolet radiation then
causes the ejected gas to fluoresce as the planetary nebula. Our own Sun is predicted to eject its planetary nebula some 6 billion
years from now.

The Hubble observations were obtained in 1998 with the Wide Field Planetary Camera 2 (WFPC2) by a team of astronomers led
by Arsen Hajian of the U.S. Naval Observatory in Washington, DC. The Hubble Heritage team, working at the Space Telescope
Science Institute in Baltimore, has prepared this color rendition by combining the Hajian team's WFPC2 images taken through
three different color filters that isolate nebular gases of different temperatures.

The nebula shows several remarkable and poorly understood features. Blue regions mark the hottest glowing gas, which forms a
roughly circular ring around the central stellar remnant. Orange and red show the locations of cooler gas. The cool gas tends to
lie in long streamers pointing away from the central star, and in a surrounding, tattered-looking ring at the outer edge of the nebula.
The origin of these cooler clouds within the nebula is still uncertain, but the streamers are clear evidence that their shapes are
affected by radiation and stellar winds from the hot star at the center. The star's surface temperature is estimated at a scorching
140,000 degrees Celsius (250,000 degrees Fahrenheit).

Hajian and his team are scheduled to reobserve NGC 6751 with Hubble's WFPC2 in 2001. Due to the expansion of the nebula,
at a speed of about 40 kilometers per second (25 miles per second), the high resolution of Hubble's camera will reveal the slight
increase in the size of the nebula since 1998. This measurement will allow the astronomers to calculate an accurate distance to
NGC 6751. In the meantime, current estimates are that NGC 6751 is roughly 6,500 light-years from Earth. The nebula's diameter
is 0.8 light-years, some 600 times the diameter of our own solar system.