VFTS 102
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Dorado IAU.svg
Författare/Upphovsman: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg), Licens: CC BY 3.0
IAU Dorado chart
Författare/Upphovsman: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg), Licens: CC BY 3.0
IAU Dorado chart
Artist’s impression of the fastest rotating star.jpg
(c) ESA/Hubble, CC BY 4.0
This is an artist's concept of the fastest rotating star found to date. The massive, bright young star, called VFTS 102 rotates at about two million kilometres per hour. Centrifugal force from this dizzying spin rate has flattened the star into an oblate shape, and spun off a disk of hot plasma, seen edge on in this view from a hypothetical planet. The star may have "spun up" by accreting material from a binary companion star. The rapidly evolving companion later exploded as a supernova. The whirling star lies 160 000 light-years away in the Large Magellanic cloud, a satellite galaxy of the Milky Way.
(c) ESA/Hubble, CC BY 4.0
This is an artist's concept of the fastest rotating star found to date. The massive, bright young star, called VFTS 102 rotates at about two million kilometres per hour. Centrifugal force from this dizzying spin rate has flattened the star into an oblate shape, and spun off a disk of hot plasma, seen edge on in this view from a hypothetical planet. The star may have "spun up" by accreting material from a binary companion star. The rapidly evolving companion later exploded as a supernova. The whirling star lies 160 000 light-years away in the Large Magellanic cloud, a satellite galaxy of the Milky Way.
VFTS 102.jpg
Författare/Upphovsman: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit, Licens: CC BY 3.0
This view shows part of the stellar nursery called the Tarantula Nebula in the Large Magellanic Cloud, a small neighbour of the Milky Way. At the centre lies the brilliant star VFTS 102 This view includes both visible-light and infrared images from the Wide Field Imager at the MPG/ESO 2.2-metre telescope at La Silla and the 4.1-metre infrared VISTA telescope at Paranal. VFTS 102 is the most rapidly rotating star ever found.
Författare/Upphovsman: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit, Licens: CC BY 3.0
This view shows part of the stellar nursery called the Tarantula Nebula in the Large Magellanic Cloud, a small neighbour of the Milky Way. At the centre lies the brilliant star VFTS 102 This view includes both visible-light and infrared images from the Wide Field Imager at the MPG/ESO 2.2-metre telescope at La Silla and the 4.1-metre infrared VISTA telescope at Paranal. VFTS 102 is the most rapidly rotating star ever found.