Helix Nebula

Stars like our Sun end their lives by casting off their outer layers, briefly forming a spectacular "planetary nebula" like the Helix Nebula. In visible light, we see the glow of hot gases illuminated by a hot, compact core, known as a "white dwarf." Shifting into the near-infrared reveals the glow of more complex molecules formed in the outer shell. The mid-infrared glow highlights the warm (bright red) dust surrounding the white dwarf.

Visible: Hot gas ejected from a dying star glows.

Near-infrared: Near-infrared light reveals cooler material.

Mid-infrared: Warm dust is identified in mid-infrared light.

CREDITS: Visible: NASA, NOAO, ESA, the Hubble Helix Nebula Team, M. Meixner (STScI), and T.A. Rector (NRAO). Near-infrared: ESO/VISTA/J. Emerson. Acknowledgment: Cambridge Astronomical Survey Unit. Mid-infrared: NASA/JPL-Caltech/K. Su (Univ. of Arizona).
Default View
image of Visible Helix Nebula
image of Near-infrared Helix Nebula
image of Mid-infrared Helix Nebula