Helix Nebula

5.6 lydiameter

Updated

5.60ly
Visual creditHubble 2002 / NASA, ESA, C.R. O'Dell (Vanderbilt University), M. Meixner and P. McCullough (STScI) / Public domainSource: NASA Science

Details

The Helix Nebula is one of the closest planetary nebulae to Earth, a glowing shell expelled by a dying Sun-like star. From Earth it can look like a simple doughnut, but the full structure is a layered remnant built from two nearly perpendicular gaseous disks and outflows.

The Helix Nebula is one of the nearest planetary nebulae, formed from outer layers shed by an aging low-mass star. Its apparent ring is part of a larger three-dimensional system of ionized gas, dust and thousands of dense cometary knots around the exposed stellar core.

Geometric models use intersecting disk-like structures and outflows to explain the projected shape. The quoted 5.74-light-year diameter includes faint outer material, not only the bright central ring most familiar from images.

Key facts

Category
Nebulae
Object class
Planetary nebula
Host
Milky Way
Scale fact
5.6 lydiameter
Composition
Ionized gas, dust, cometary knots
Embed

Size neighbors

Objects near Helix Nebula on the scale

On the logarithmic size axis, Helix Nebula falls between Oort Cloud and Crab Nebula. The band uses nearby Planetary nebula records.

Shared physical scale
4.28ly
NGC 70271,890 billion km
Cat's Eye Nebula3,800 billion km
Ring Nebula2.6 ly
Helix Nebula5.6 ly

Sources

References for Helix Nebula

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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