
science & techESA/Hubble
A dying Sun-like star has blown a glowing bubble half a light-year wide
When a Sun-like star runs out of fuel, it sheds its outer layers, and the glowing shell left behind is called a planetary nebula. The Little Gem, NGC 6818, lies about 6,000 light-years away and spans just over half a light-year. Its central star is tiny compared with the cloud, so the gas dominates the view. The shape is uneven, with knotty filaments and layers, because the ejection is not symmetrical. A fast stellar wind from the central star pushes the gas outward and carves bright blowouts where it smashes into slower material.
The star's core heats up and its outer envelope is puffed away. The fast stellar wind then catches up with the slower gas already ejected and sweeps it into a shell. Collisions between fast and slow gas create the bright, dense knots at the edges.
Planetary nebulae show how stars like the Sun end their lives, and they are a major way that material forged in stars is returned to the galaxy. Imaging at different wavelengths, as Hubble does here, reveals the chemistry and structure of the gas.
Planetary nebulae are the Sun's eventual future: in several billion years the Sun is expected to shed its outer layers in this way. Much of the carbon in living things was forged inside stars, and planetary nebulae return that material to space.
The name planetary nebula was coined by William Herschel in 1785, because the round shapes looked like planets through small telescopes.
ESA/Hubble · CC BY 4.0
Image: ESA/Hubble & NASA Acknowledgement: Judy Schmidt ( geckzilla.com )
