Skip to main content

A 10,000-year-old conflict between two stars formed the Necklace Nebula

The interaction of two doomed stars has created this spectacular ring adorned with bright clumps of gas ­– a diamond necklace of cosmic proportions. Fittingly known as the “Necklace Nebula,” this planetary nebula is located 15,000 light-years away from Earth in the small, dim constellation of Sagitta (the Arrow).
The interaction of two doomed stars has created this spectacular ring adorned with bright clumps of gas ­– a diamond necklace of cosmic proportions. Fittingly known as the “Necklace Nebula,” this planetary nebula is located 15,000 light-years away from Earth in the small, dim constellation of Sagitta (the Arrow). ESA/Hubble & NASA, K. Noll

Around 10,000 years ago, two stars that had been orbited each other peacefully came into a sticky conflict when the larger of the two came too close to its companion and ballooned outward, engulfing the other. The resulting mess of a bloated star spun so quickly that it threw off its outer layers, forming a bubble of gas which expanded out into space, eventually stretching over two light-years wide.

This dramatic event formed the beautiful Necklace Nebula, also known as PN G054.2-03.4, located 15,000 light-years away in the constellation Sagitta (the Arrow). This nebula was recently captured by the Hubble Space Telescope in the image shown above. The ring of gas is dotted with clumps of gas that shine brightly like jewelry, for which the nebula was given its name. The gas glows as it is illuminated with ultraviolet light produced by nearby stars, giving the nebula its distinctive appearance.

Recommended Videos

Even after their dramatic conflict, the two stars at the heart of the nebula continue to orbit each other closely. They are just a few million miles apart and orbit each other in just over a day. They are so close together that they appear as a single dot in the image.

This is not the first time that Hubble has imaged this particular nebula. It also captured the image below in 2011, when the nebula had only recently been discovered. Hubble used its Wide Field Camera 3, installed in 2009, to take this image.

A previous image of the Necklace Nebula, taken by Hubble in 2011.
A previous image of the Necklace Nebula, taken by Hubble in 2011. NASA , ESA , and the Hubble Heritage Team (STScI /AURA )

Since 2011, Hubble’s hardware has remained largely the same, but software has improved, such as image processing technology. This allowed the creation of a crisper image of the target which shows more detail than the version from 10 years prior. The latest image is a composite, including images taken by the same Wide Field Camera 3.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
See Hubble’s take on the famous and beautiful Carina Nebula
This sparkling new image depicts a small section of the Carina Nebula, one of the NASA Hubble Space Telescope’s most-imaged objects. The Carina Nebula, NGC 3372, is an enormous cloud of gas and dust home to several massive and bright stars, including at least a dozen that are 50 to 100 times the mass of our Sun.

The Hubble Space Telescope recently captured a scene made famous by its sibling, the James Webb Space Telescope. One of the first images released from Webb showed the Carina Nebula, a particularly striking structure of dust and gas located in an area of the Milky Way called the Carina-Sagittarius arm. Recently, Hubble has imaged Carina as well, snapping an image of a small section of this famous nebula.

Compared to Webb's image of Carina, which was taken in the infrared wavelength, Hubble's image is more pastel. Although Hubble operates primarily in the visible light wavelength and Webb operates in the infrared, in this case, Hubble used its infrared capabilities to peer through the dust of the nebula and see its structure.

Read more
Hubble captures an open star cluster in a nearby satellite galaxy
Against a backdrop littered with tiny pinpricks of light glint a few, brighter stars. This whole collection is NGC 1858, an open star cluster in the northwest region of the Large Magellanic Cloud, a satellite galaxy of our Milky Way that boasts an abundance of star-forming regions. NGC 1858 is estimated to be around 10 million years old.clock

The Hubble Space Telescope recently captured an image of a beautiful star cluster called NGC 1858, located in an area full of star-forming regions. This area is part of the Large Magellanic Cloud, one of the Milky Way's satellite galaxies, and is located 160,000 light-years away and is thought to be around 10 million years old.

The Large Magellanic Cloud is one of several satellite galaxies to the Milky Way, which are smaller galaxies that are gravitationally bound to our galaxy. Along with its companion, the Small Magellanic Cloud, it orbits around the Milky Way and will eventually collide with our galaxy in billions of years' time.

Read more
Astronomers find remnants of planets around 10 billion-year-old stars
Artist’s impression of the old white dwarfs WDJ2147-4035 and WDJ1922+0233 surrounded by orbiting planetary debris, which will accrete onto the stars and pollute their atmospheres. WDJ2147-4035 is extremely red and dim, while WDJ1922+0233 is unusually blue.

Far away in the depths of the Milky Way lie two small, dim stars that are in the final stage of their life. At over 10 billion years old, white dwarfs WDJ2147-4035 and WDJ1922+0233 are among the oldest stars in our galaxy, and recently, astronomers discovered something special orbiting around them: the remains of planets, making this one of the oldest known rocky planetary systems.

Astronomers used data from GAIA, the Dark Energy Survey, and the X-Shooter instrument at the European Southern Observatory to peer at this system. They identified debris from orbiting planetesimals, which are globs of dust and rock which are created during planetary formation. The researchers used spectroscopy to look at the light coming from the two white dwarf stars and break it down into different wavelengths, which can show what materials the stars and the surrounding matter are made of.

Read more