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Ilustración artística del escenario de eyecciones de plasma de V Hydrae

This four-panel graphic illustrates how the binary-star system V Hydrae is launching balls of plasma into space.Panel 1 shows the two stars orbiting each other. One of the stars is nearing the end of its life and has swelled in size, becoming a red giant.In panel 2, the smaller s...

Fecha
Jan 1, 2016
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2016-34-3890-image
Por

This four-panel graphic illustrates how the binary-star system V Hydrae is launching balls of plasma into space.

Panel 1 shows the two stars orbiting each other. One of the stars is nearing the end of its life and has swelled in size, becoming a red giant.

In panel 2, the smaller star's orbit carries the star into the red giant's expanded atmosphere. As the star moves through the atmosphere, it gobbles up material from the red giant, which settles into a disk around the star.

The buildup of material reaches a tipping point and is eventually ejected as blobs of hot plasma along the star's spin axis, shown in panel 3.

This ejection process is repeated every eight years, the time it takes for the orbiting star to make another pass through the bloated red giant's envelope, shown in panel 4.

Credits

NASA, ESA, and R. Sahai (JPL);
Artist's Illustration Credit: NASA, ESA, and A. Feild (STScI)

Detalles de la imagen

About The Object
Object NameV Hydrae, V Hya
Object DescriptionCarbon Star, Variable Star
R.A. Position10h 51m 37.2s
Dec. Position-21° 15' 00"
ConstellationHydra
Distance1,200 light-years (roughly 400 parsecs)
About The Data
Data DescriptionData were provided through HST proposals , , , , , and : R. Sahai (JPL), C. Barnbaum (Valdosta State Univ.), G. Knapp (Princeton Univ.), M. Morris (UCLA), J. Krist (JPL), and K. Young (SAO).
InstrumentHST>STIS spectroscopy
Exposure DatesJan. 2002; Dec. 2002; Jan. 2004; July 2011; Jul. 2012; and Jul. 2013 (Exposure time: Several exposures, 1 - 914 seconds)
FiltersGratings: G430M (419 nm), G750M (658 nm)

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