VLT images the Saturn Nebula

A glowing cloud of cosmic dust and gas known as the Saturn Nebula, or NGC 7009, has been imaged by the Very Large Telescope (VLT) in a bid to help astronomers understand how these kinds of nebulae form.

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Planetary nebula NGC 7009, or the Saturn Nebula, glows pink and blue. These observations with the Very Large Telescope have been used to create the first detailed optical maps of gas and dust distributed throughout a planetary nebula.
Credit: ESO/J. Walsh

 

The Saturn Nebula is a planetary nebula, although it has nothing to do with planetary bodies. The name of these nebulae derives from the fact that they appear mostly round and symmetrical, like planets.

The Saturn Nebula is so-called because it resembles the most iconic ringed planet in our Solar System.

In order to better understand how planetary nebulae form, astronomers used the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s VLT to observe NGC 7009.

These observations produced the first ever detailed optical maps of the gas and dust distributed throughout a planetary nebula.

The resulting image of the Saturn Nebula shows an elliptical inner shell, an outer shell and a halo.

But the astronomers behind the study also found a wave-like feature in the dust of the nebula, which is not yet understood.

 

Perhaps the most famous planetary nebula: the Dumbbell Nebula. This image was also captured by the VLT, in 1998. From its shape, it is easy to see how these nebulae got their 'planetary' name.
Credit: ESO

 

Planetary nebulae are incredibly dusty places, as they are formed when a star begins to expand and shed its outer layers towards the end of its life. This results in a blowout of material that glows with ultraviolet radiation from the remaining stellar core.

Dust is distributed throughout the Saturn Nebula, but there is an absence of dust at the rim of the inner shell, as though it was being destroyed. 

Perhaps the expanding shock wave of the inner shell is smashing into the grains of dust and destroying them.

Or, perhaps the heat from this shock wave is simply evaporating the dust.

Studies like these provide incredible images of these cosmic structures, but also enable astronomers to get closer to the mysteries of how planetary nebulae form and evolve.


 

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