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R Aquarii - A Nearby Exploding Star

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dc.creator NASA
dc.date 1990
dc.date.accessioned 2019-10-03T18:54:25Z
dc.date.available 2019-10-03T18:54:25Z
dc.identifier.uri http://hdl.handle.net/20.500.11925/2567613
dc.description *Description*: This is the first picture taken by HST of a recent nova, the star system R-Aquarii. The two dark knots at the center of the image probably contain the binary star system itself, which consists of a red giant and white dwarf star. The knots are dark due to saturation effects produced by the FOC detector when it observes very bright objects. The filamentary features emanating from the core are hot gas (plasma) that has been ejected at high speeds from the binary pair. The plasma emerges as a 400 billion kilometer-long geyser which is twisted by the force of the explosion and channeled upwards and outwards by strong magnetic fields. The flowing material appears to bend back on itself in a spiral pattern, perhaps due to obstruction in the path. Technical facts about this news release: Back to entire collection [ http://hubblesite.org/newscenter/archive/releases/index/660/ ] Next release [ http://hubblesite.org/newscenter/archive/releases/1990/13/ ] Previous release [ http://hubblesite.org/newscenter/archive/releases/1990/19/ ] *News Release Number:*: STScI-1990-15a
dc.rights pd
dc.source http://hubblesite.org/newscenter/archive/releases/1990/15/image/a/
dc.title R Aquarii - A Nearby Exploding Star
dc.type Изображение
dc.date.updated 2016-05-26T03:50:22Z
dc.rightsholder NASA
dc.identifier.url https://archive.org/download/SPD-HUBBLE-STScI-1990-15a/full_tif.jpg
dc.identifier.ianasa SPD-HUBBLE-STScI-1990-15a

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