The first hint of what will become of our Sun [
http://www.nineplan
] was discovered inadvertently in 1764 [
http://en.wikipedia
]. At that time, Charles Messier [
http://www.seds.org
] was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier's list [
http://antwrp.gsfc.
], now known as M27 [
http://www.seds.org
] or the Dumbbell Nebula, is a planetary nebula [
http://antwrp.gsfc.
], the type of nebula our Sun [
http://antwrp.gsfc.
] will produce when nuclear fusion [
http://fusedweb.ppp
] stops in its core. M27 [
http://antwrp.gsfc.
] is one of the brightest planetary nebulae [
http://www.seds.org
] on the sky, and can be seen in the constellation [
http://www.astro.wi
] Vulpecula [
http://www.astronom
] with binoculars. It takes light about 1000 years to reach us from M27, shown above [
http://www.noao.edu
], digitally sharpened, in three standard colors. Understanding the physics and significance of M27 [
http://astro.ninepl
] was well beyond 18th century science. Even today, many things remain mysterious about bipolar planetary nebula [
http://antwrp.gsfc.
] like M27, including the physical mechanism that expels a low-mass star's gaseous outer-envelope, leaving an X-ray [
http://www.treasure
] hot white dwarf [
http://imagine.gsfc
].
Explanation
The first hint of what will become of our Sun [
http://www.nineplan
] was discovered inadvertently in 1764 [
http://en.wikipedia
]. At that time, Charles Messier [
http://www.seds.org
] was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier's list [
http://antwrp.gsfc.
], now known as M27 [
http://www.seds.org
] or the Dumbbell Nebula, is a planetary nebula [
http://antwrp.gsfc.
], the type of nebula our Sun [
http://antwrp.gsfc.
] will produce when nuclear fusion [
http://fusedweb.ppp
] stops in its core. M27 [
http://antwrp.gsfc.
] is one of the brightest planetary nebulae [
http://www.seds.org
] on the sky, and can be seen in the constellation [
http://www.astro.wi
] Vulpecula [
http://www.astronom
] with binoculars. It takes light about 1000 years to reach us from M27, shown above [
http://www.noao.edu
], digitally sharpened, in three standard colors. Understanding the physics and significance of M27 [
http://astro.ninepl
] was well beyond 18th century science. Even today, many things remain mysterious about bipolar planetary nebula [
http://antwrp.gsfc.
] like M27, including the physical mechanism that expels a low-mass star's gaseous outer-envelope, leaving an X-ray [
http://www.treasure
] hot white dwarf [
http://imagine.gsfc
].
Explanation