Planetary nebulae do [
http://antwrp.gsfc.
] look simple, round, and planet-like in small telescopes. But images from the orbiting Hubble Space Telescope [
http://hubble.stsci
] have become well known for showing these fluorescent gas shrouds [
http://antwrp.gsfc.
] of dying Sun-like stars to possess a staggering variety [
http://oposite.stsc
] of detailed symmetries and shapes. This composite color Hubble image of NGC 6751 [
http://oposite.stsc
] is a beautiful example of a classic planetary nebula with complex features and was selected to commemorate the tenth anniversary [
http://pao.gsfc.nas
] of Hubble in orbit. The colors were chosen to represent the relative temperature of the gas - blue, orange, and red indicating the hottest to coolest gas. Winds and radiation from the intensely hot central star [
http://antwrp.gsfc.
] (140,000 degrees [
http://www.unidata.
blynds/tmp.html ] Celsius [
http://www.cchem.be
temperature.html ]) have apparently created the nebula's streamer-like features. The nebula's [
http://heritage.sts
ngc6751table.html ] actual diameter is approximately 0.8 light-years or about 600 times the size [
http://antwrp.gsfc.
] of our solar system. NGC 6751 is 6,500 light-years distant in the constellation Aquila [
http://www.astro.wi
constellations/Aquil a.html ].
Explanation
Planetary nebulae do [
http://antwrp.gsfc.
] look simple, round, and planet-like in small telescopes. But images from the orbiting Hubble Space Telescope [
http://hubble.stsci
] have become well known for showing these fluorescent gas shrouds [
http://antwrp.gsfc.
] of dying Sun-like stars to possess a staggering variety [
http://oposite.stsc
] of detailed symmetries and shapes. This composite color Hubble image of NGC 6751 [
http://oposite.stsc
] is a beautiful example of a classic planetary nebula with complex features and was selected to commemorate the tenth anniversary [
http://pao.gsfc.nas
] of Hubble in orbit. The colors were chosen to represent the relative temperature of the gas - blue, orange, and red indicating the hottest to coolest gas. Winds and radiation from the intensely hot central star [
http://antwrp.gsfc.
] (140,000 degrees [
http://www.unidata.
blynds/tmp.html ] Celsius [
http://www.cchem.be
temperature.html ]) have apparently created the nebula's streamer-like features. The nebula's [
http://heritage.sts
ngc6751table.html ] actual diameter is approximately 0.8 light-years or about 600 times the size [
http://antwrp.gsfc.
] of our solar system. NGC 6751 is 6,500 light-years distant in the constellation Aquila [
http://www.astro.wi
constellations/Aquil a.html ].
Explanation