3D View: The Dragon's Egg Nebula & HD 148937 Binary Star System | ESO
This 3D animation of the beautiful nebula NGC 6164/6165, also known as the Dragon’s Egg, imagines what it might feel like to fly close to these swirling clouds of gas and dust and approach the star pair HD 148937 at its heart. This video is based on a real image from the VLT Survey Telescope, hosted at ESO’s Paranal site, but the 3D view is not real—the location of the stars shown here is only indicative.
Nebula NGC 6164/6165 surrounding the HD 148937 star system as seen in visible light. Most of the image is taken up by a cloud-like structure shaped like an egg, slightly tilted to the right. It is colored in shades of orange and pink, with certain areas brighter than others. In a gap at its center, a white sphere shines brightly, with white, blue and green rays coming out of it. Surrounding the cloud are stars of different sizes and colors over a dark background. Distance: 4,000 light years
This image, taken with the VLT Survey Telescope hosted at the European Southern Observatory’s Paranal Observatory, shows the beautiful nebula NGC 6164/6165, also known as the Dragon’s Egg. The nebula is a cloud of gas and dust surrounding a pair of stars called HD 148937.
In a new study using ESO data, astronomers have shown that the two stars are unusually different from each other—one appears much younger and, unlike the other, is magnetic. Moreover, the nebula is significantly younger than either star at its heart, and is made up of gases normally found deep within a star and not on the outside. These clues together helped solve the mystery of the HD 148937 system—there were most likely three stars in the system until two of them clashed and merged, creating a new, larger and magnetic star. This violent event also created the spectacular nebula that now surrounds the remaining stars.
Credits: European Southern Observatory (ESO)/M. Kornmesser, VPHAS+ team
Acknowledgement: Cambridge Astronomical Survey Unit (CASU)
Duration: 16 seconds
Release Date: April 4, 2024
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