LL Pegasi (AFGL 3068) is a Mira variable star surrounded by a pinwheel-shaped nebula, IRAS 23166+1655, thought to be a preplanetary nebula. It is a binary system that includes an extreme carbon star. The pair is hidden by the dust cloud ejected from the carbon star and is only visible in infrared light.
Variability
LL Pegasi is obscured at visual wavelengths, but is strongly variable in brightness at infrared wavelengths. It is classified as a Mira variable and has a period of about 696 days.
Nebula The nebula displays an unusual Archimedean spiral shape. The shape is thought to be formed through the interaction between the stellar companion and the carbon star, as has been seen in other binary systems, although not with such a precise geometric form. The distance between the spiral arms and their rate of expansion is consistent with estimates of the pair's 810 year orbital period based on their apparent angular separation.
Gallery
Notes
See also List of largest stars
References
External links 3D view of LL Pegasi Celestial spiral with a twist An Extraordinary Celestial Spiral Celestial spiral goes viral Hubble Spots Ghostly Space Spiral — discovery.com Archived 2010-09-09 at the Wayback Machine An Extraordinary Spiral from LL Pegasi, APOD


![LL Pegasi: A near-infrared (L- band) light curve for LL Pegasi, plotted from data published by Le Bertre (1992)[9]](https://upload.wikimedia.org/wikipedia/commons/thumb/7/7d/LLPegLightCurve.png/1280px-LLPegLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)

