Dust makes this cosmic eye look red. The eerie Spitzer Space Telescope image [
http://www.spitzer.
ssc2007-03/index.sht ml ] shows infrared [ http://coolcosmos.ip ac.caltech.edu// ] radiation from the well-studied Helix Nebula [
http://antwrp.gsfc.
] (NGC 7293) a mere 700 light-years away in the constellation Aquarius [
http://www.seds.org
]. The two light-year diameter shroud of dust and gas around a central white dwarf has long been considered an excellent example of a planetary nebula [
http://www.noao.edu
], representing the final stages in the evolution of a sun-like star. But the Spitzer data show the nebula's central star itself is immersed in a surprisingly bright infrared glow. Models [
http://arxiv.org/ab
] suggest the glow is produced by a dust debris disk [
http://antwrp.gsfc.
]. Even though the nebular material was ejected from the star many thousands of years ago, the close-in dust could be generated by collisions in a reservoir of objects analogous to our own solar system's Kuiper Belt [
http://www.ifa.hawa
] or cometary Oort cloud [
http://www.windows.
link=/comets/Oort_cl oud.html&edu=high ]. Formed in the distant planetary system, the comet-like bodies have otherwise survived even the dramatic late stages of the star's evolution [
http://en.wikipedia
].
Explanation
Dust makes this cosmic eye look red. The eerie Spitzer Space Telescope image [
http://www.spitzer.
ssc2007-03/index.sht ml ] shows infrared [ http://coolcosmos.ip ac.caltech.edu// ] radiation from the well-studied Helix Nebula [
http://antwrp.gsfc.
] (NGC 7293) a mere 700 light-years away in the constellation Aquarius [
http://www.seds.org
]. The two light-year diameter shroud of dust and gas around a central white dwarf has long been considered an excellent example of a planetary nebula [
http://www.noao.edu
], representing the final stages in the evolution of a sun-like star. But the Spitzer data show the nebula's central star itself is immersed in a surprisingly bright infrared glow. Models [
http://arxiv.org/ab
] suggest the glow is produced by a dust debris disk [
http://antwrp.gsfc.
]. Even though the nebular material was ejected from the star many thousands of years ago, the close-in dust could be generated by collisions in a reservoir of objects analogous to our own solar system's Kuiper Belt [
http://www.ifa.hawa
] or cometary Oort cloud [
http://www.windows.
link=/comets/Oort_cl oud.html&edu=high ]. Formed in the distant planetary system, the comet-like bodies have otherwise survived even the dramatic late stages of the star's evolution [
http://en.wikipedia
].
Explanation