Geometry of the Blue Ring Nebula (Animation)
The Blue Ring Nebula is thought to be the product of two stars merging into one. The collision of the bodies ejected a cloud of hot debris into space. A disk of gas orbiting the larger star cut the cloud in half, creating two cones that are moving away from the star in opposite directions. The base of one cone is moving almost directly toward Earth, while the other is moving almost directly away. Magenta represents optical light from the shockwave at the front of the expanding debris cones, outlining the two cone bases at their widest points. Blue represents far-ultraviolet light (not visible to the human eye) and comes from gas behind the shockwave. As the gas expands and cools, it forms hydrogen molecules that interact with the interstellar medium and emit only far-ultraviolet light. These emissions are visible only where the cones overlap (as seen from Earth), forming the blue ring around the central star. Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA23868
- Date
- 2020-11-18
- Photographer / author
- NASA/JPL-Caltech/R. Hurt
- Collection
- JPL
- Archive
- NASA Image and Video Library
- Type
- illustration (NASA artwork)
Public domainsafest
Reason: a NASA work: not copyrighted in the United States.
Read from: NASA media usage guidelines: NASA material is not copyrighted in the US unless noted; no third-party credit or mark found.
Credit line
"Geometry of the Blue Ring Nebula (Animation)" (2020-11-18). NASA/JPL/NASA/JPL-Caltech/R. Hurt. Public domain. https://images.nasa.gov/details/PIA23868Need photos for a whole script? Add Find Any Photo to Claude and ask for this one by its id: 16581.
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