Most Detailed Observations Ever of the Ring Nebula

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Ring Nebula

Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula. It is both relatively close to Earth and fairly bright, and so was first recorded in the late 18th century.

As is common with astronomical objects, its precise distance is not known, but it is thought to lie just over 2,000 light-years from Earth.

From Earth's perspective, the nebula looks roughly elliptical. However, astronomers have combined ground-based data with new observations using the NASA/ESA Hubble Space Telescope to observe the nebula again, hunting for clues about its structure, evolution, physical conditions and motion.

It turns out that the nebula is shaped like a distorted doughnut. We are gazing almost directly down one of the poles of this structure, with a brightly colored barrel of material stretching away from us. Although the center of this doughnut may look empty, it is actually full of lower density material that stretches both towards and away from us, creating a shape similar to a rugby ball slotted into the doughnut's central gap.

The brightest part of this nebula is what we see as the colorful main ring. This is composed of gas thrown off by a dying star at the center of the nebula. This star is on its way to becoming a white dwarf -- a very small, dense, and hot body that is the final evolutionary stage for a star like the Sun.

The Ring Nebula is one of the most notable objects in our skies. It was discovered in 1779 by astronomer Antoine Darquier de Pellepoix, and also observed later that same month by Charles Messier, and added to the Messier Catalogue. Both astronomers stumbled upon the nebula when trying to follow the path of a comet through the constellation of Lyra, passing very close to the Ring Nebula [2].

Notes

[1] Planetary nebulae take their name from their roughly circular appearance through low-magnification telescopes. The phenomenon has nothing to do with planets.

[2] Messier 57 was not the only object to be discovered during the tracking of this comet, named C/1779 A1. Messier and other astronomers added a handful of other nebulae to the catalogue during this observing period -- Messiers 56, 58, 59, 60, and 61.

PIO Contact:
Nicky Guttridge
ESA/Hubble, Garching bei Muenchen, Germany
+49-89-3200-6855
nguttrid@partner.eso.org

Science Contact:
C. Robert O'Dell
Vanderbilt University, Tennessee, USA
+1 615-343-1779
cr.odell@vanderbilt.edu

Image credit: NASA, ESA, and C. Robert O'Dell

The research on Messier 57 is described in a set of three papers, two published and one accepted for publication in The Astronomical Journal:

* "Studies of NGC 6720 with Calibrated HST WFC3 Emission Line Filter Images -- I: Structure and Evolution" [http://www.spacetelescope.org/static/archives/releases/science_papers/heic1310a.pdf]

* "Studies of NGC 6720 with Calibrated HST WFC3 Emission Line Filter Images -- II: Physical Conditions" [http://www.spacetelescope.org/static/archives/releases/science_papers/heic1310b.pdf]

* "Studies of NGC 6720 with Calibrated HST WFC3 Emission Line Filter Images -- III: Tangential Motions using AstroDrizzle Images" [http://www.spacetelescope.org/static/archives/releases/science_papers/heic1310c.pdf]

The NASA/ESA Hubble Space Telescope observations used in this image were led by C. R. O'Dell (Vanderbilt University, USA), G. J. Ferland (University of Kentucky, USA), W. J. Henney (Universidad Nacional Autonoma de Mexico, Mexico), and M. Peimbert (Universidad Nacional Autonoma de Mexico, Mexico).

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

Text, images, and video: http://www.spacetelescope.org/news/heic1310/

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