Date: 14 Aug 1997
Satellite: ISO
Depicts: Helix Nebula
Copyright: ESA/ISO, ISOCAM, and P. Cox et al

Pierre Cox of the Institut d'Astrophysique Spatiale in Orsay, France, leads the ISO investigation of this object by a team of French, American, Dutch and Spanish astronomers. They expected to find dust, because it is commonplace in the outer layers of dying stars. Nevertheless ISO, using its special ability to identify dusty materials by their characteristic infrared emission, has established that the Helix Nebula contains no small dust grains. Cox and his colleagues believe that during the lifetime of the nebula (a few thousand years) the grains have been destroyed by powerful ultraviolet rays emitted by the very hot white dwarf at the center of the nebula.

As a result, in this image of the Helix Nebula obtained by ISO's camera ISOCAM at a wavelength of 7 microns, the infrared emission comes not from dust but from molecular hydrogen gas. At first glance the image looks like pictures of the nebula in visible-light. The shells appear as rings because more of the emitting material is concentrated along tangential lines of sight. Other stars are seen as bright dots, through the nebula.

Details revealed with special clarity in the ISO image include an outer shell, blown off from the star before its final death throes. The radial streaks are also remarkable. Notably absent is the white dwarf star at the center of the nebula. This is seen in visible light, but it is so hot that it emits very little of its radiation in the infrared.

Planetary nebulae are so called because they looked round, like planets, to early astronomers using small telescopes. The Helix Nebula (alias NGC 7293) is the closest example, at a distance of 500 light-years.