NASA’s James Webb Space Telescope’s mid-infrared image shows four coiled shells of dust around a pair of Wolf-Rayet stars known as Apep for the first time. Previous observations by other telescopes showed only one. (Watch a 3D visualization of the system.)
Webb’s data, combined with observations from the European Southern Observatory’s Very Large Telescope (VLT) in Chile, confirmed that the two Wolf-Rayet stars sail past one another approximately every 190 years. Over each orbit, they make a close pass for 25 years, producing and spewing amorphous carbon dust.
Webb’s new data also confirmed that there are three stars gravitationally bound to one another in this system. Holes are “sliced” into these shells by the third star, a massive supergiant.
About the Object
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R.A. Position16:00:50.5
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Dec. Position-51:42:45.0
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ConstellationNorma
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Distance8,000 light-years
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DimensionsImage is about 1.9 arcminutes across (4 light-years)
About the Data
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Data Description
This image was created with Webb data from proposal: 5842 (Y. Han). Image processing: Alyssa Pagan (STScI).
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InstrumentMIRI
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Exposure Dates24 July 2024
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FiltersF770W, F1500W, F2550W