While exploring the inner edge of the Helix Nebula [
http://antwrp.gsfc.
] with the Hubble Space Telescope [
http://antwrp.gsfc.
]'s Wide Field Planetary Camera 2 [
http://www.stsci.ed
], astronomers were able to produce this striking image [
http://oposite.stsc
] - rich in details of an exotic environment. This planetary nebula [
http://www.noao.edu
], created near the final phase of a sun-like [
http://instruct1.ci
] star's life [
http://antwrp.gsfc.
], is composed of tenuous shells of gas ejected by the hot central star. The atoms [
http://education.jl
] of gas, stripped of electrons [
http://www.aip.org/
] by ultraviolet radiation [
http://liftoff.msfc
] from the central star, radiate light at characteristic energies allowing specific chemical elements [
http://pearl1.lanl.
] to be identified. In this image [
http://oposite.stsc
], emission from nitrogen [
http://pearl1.lanl.
] is represented as red, hydrogen [
http://pearl1.lanl.
] emission as green, and oxygen [
http://pearl1.lanl.
] as blue. The inner edge of the Helix Nebula [
http://www.seds.org
], also known as NGC 7293, is in the direction toward the central star, which is toward the upper right. Clearly visible near the inner edge are finger shaped cometary knots [
http://antwrp.gsfc.
].
Explanation
While exploring the inner edge of the Helix Nebula [
http://antwrp.gsfc.
] with the Hubble Space Telescope [
http://antwrp.gsfc.
]'s Wide Field Planetary Camera 2 [
http://www.stsci.ed
], astronomers were able to produce this striking image [
http://oposite.stsc
] - rich in details of an exotic environment. This planetary nebula [
http://www.noao.edu
], created near the final phase of a sun-like [
http://instruct1.ci
] star's life [
http://antwrp.gsfc.
], is composed of tenuous shells of gas ejected by the hot central star. The atoms [
http://education.jl
] of gas, stripped of electrons [
http://www.aip.org/
] by ultraviolet radiation [
http://liftoff.msfc
] from the central star, radiate light at characteristic energies allowing specific chemical elements [
http://pearl1.lanl.
] to be identified. In this image [
http://oposite.stsc
], emission from nitrogen [
http://pearl1.lanl.
] is represented as red, hydrogen [
http://pearl1.lanl.
] emission as green, and oxygen [
http://pearl1.lanl.
] as blue. The inner edge of the Helix Nebula [
http://www.seds.org
], also known as NGC 7293, is in the direction toward the central star, which is toward the upper right. Clearly visible near the inner edge are finger shaped cometary knots [
http://antwrp.gsfc.
].
Explanation