Celestial spiral with a twist
Although it looks like the pattern of a shell on the beach, this intriguing spiral is in fact astronomical in nature. The Atacama Large Millimeter/submillimeter Array (ALMA) captured this remarkable image of a binary star system, where two stars — LL Pegasi and its companion — are locked in a stellar waltz, orbiting around their common centre of gravity. The old star LL Pegasi is continuously losing gaseous material as it evolves into a planetary nebula, and the distinct spiral shape is the imprint made by the stars orbiting in this gas.
The spiral spans light-years and winds around with extraordinary regularity. Based on the expansion rate of the spiralling gas, astronomers estimate that a new “layer” appears every 800 years — approximately the same time it takes for the two stars to complete one orbit around each other.
LL Pegasi was first highlighted about 10 years ago when the NASA/ESA Hubble Space Telescope obtained a picture of the almost-perfect spiral structure. This was the first time a spiral pattern had been found in material surrounding an old star. Now, ALMA’s observations, of which this image only shows one “cross-section”, have added an extra dimension to reveal the exquisitely-ordered 3D geometry of the spiral pattern. A full view of the 3D video can be seen in this video.
An additional image shows a composition of the ALMA and Hubble data.
ALMA (ESO/NAOJ/NRAO)/H. Kim et al.
|Publiseringsdato:||6. mars 2017 06:00|
|Størrelse:||996 x 997 px|
|Position (RA):||23 19 12.61|
|Position (Dec):||17° 11' 33.07"|
|Field of view:||0.32 x 0.32 arcminutes|
|Orientering:||Nord er -0.0° til venstre for vertikalen|
Farger og filtre
|Atacama Large Millimeter/submillimeter Array|