– Hot stellar core glowing light blue.
– Gas and dust appearing as dark orange material following pockets of dark blue areas.
– Evidence of inner fast winds affecting outer halos over thousands of years.
– Concentric rings likely carved by the secondary star orbiting the main star during earlier mass-shedding stages.
– Cool molecular gas traced as red (NIRCam) and blue (MIRI), while ionized hot gas concentrates toward the center.
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The discovery deepens our understanding of planetary nebulae formation and thier diverse structures influenced by binary interactions between stars. For India-as it continues to expand its contributions to space exploration-the findings highlight how cutting-edge technologies like NASA’s James Webb telescope advance our knowledge about stellar evolution beyond conventional expectations.This provides valuable insights for Indian researchers developing instruments or missions aimed at studying distant cosmic phenomena under specialized conditions.
India may find opportunities to collaborate internationally on such astronomical studies, given its increasing aspirations in space science reflected through ISRO projects like Aditya-L1 solar observatory mission or Chandrayaan series. Understanding complex celestial dynamics involving planetary nebulae could inspire similar endeavors locally or globally promoting scientific innovation for all humanity.