Sometimes we view NASA Hubble Space Telescope images and see things we just don’t believe. This striking spiral is thought to be created by material spinning out of LL Pegasi.
LL Pegasi, like most stars in the galaxy, is a binary star; two stars orbiting each other. One of the stars is losing material, while another star orbits it. From our lucky vantage point on Earth, we are looking at the star from above. So we see the expanding pinwheel spiral pattern looking like a spinning water sprinkler. The regular spacing between layers in the spiral
Astronomers believe that LL Pegasi is in the first stages of forming a planetary nebula. Planetary nebulae have nothing to do with planets. Planet hunters of the 17th and 18th centuries saw many objects in their telescopes that resembled the gas giants Jupiter, Saturn and Uranus. We now know that these objects are far outside the solar system. Planetary nebulae form during the final stages of life for stars like our Sun. Once they run out of hydrogen fuel, they start to burn heavier elements, such as helium. They swell, engulfing their inner planets, and the outer layers are puffed off into space. Huge expanding bubbles and rings of material form the planetary nebulae we see. Radiation from the hot and dead core of the star causes atoms within the cloud to glow like a neon sign.
The material making up the spiral is moving away from the star at about 50,000 kilometers per hour, or 30,000 miles per hour. While we can see the material being spewed from the central star, a thick cocoon of dust blocks it from our view. Knowing the speed the material is being ejected, astronomers can measure the regular spacing between the spirals. They find that the orbital period of the companion star and the distance between the spirals is about 800 years.
LL Pegasi, or AFGL 3068, is found more than 3,000 light-years away from Earth toward the constellation of Pegasus, the Winged Horse.
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