What is the Helix Nebula?
The Helix Nebula is a planetary nebula notable for its striking resemblance to the “Eye of Sauron,” and is one of the closest radiant nebulae to Earth.
Planetary nebulae form when stars, similar to our Sun, reach the end of their lives. as these stars run out of fuel, they shed their outer layers into space, creating expanding shells of gas and plasma. The remaining core of the star becomes a white dwarf, which emits intense ultraviolet radiation that ionizes the expelled gas, causing it to glow. The Helix Nebula’s distinctive ring-like structure is a result of this process, with the central white dwarf visible at its heart.
Located approximately 655 light-years away in the constellation Aquarius, the Helix Nebula has a diameter of about 0.8 light-years. It was first discovered by Karl Ludwig Harding in 1824, and has since become a popular target for both amateur and professional astronomers.NASA’s Hubble Space Telescope has captured numerous detailed images of the nebula, revealing its intricate structure and composition.
How did the Helix nebula get its shape?
The Helix Nebula’s distinctive ring shape is highly likely due to a binary star system at its center, where a white dwarf orbits a companion star.
The interaction between the two stars influences the way the outer layers of gas are ejected, creating a complex and asymmetrical structure. The companion star’s gravity can sculpt the expanding gas shell, leading to the formation of the observed rings and filaments. Scientists believe the nebula is expanding at a rate of approximately 31 kilometers per second (19 miles per second).
In 2019, researchers using data from the Hubble Space Telescope and other observatories discovered a previously unkown structure within the Helix Nebula: a pair of faint, elongated clouds extending outward from the central star. According to Space.com, these structures are thought to be formed by material ejected during earlier phases of the star’s evolution.
