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This four-panel graphic illustrates how the binary-star system V Hydrae is launching
balls of plasma into space. Image credit: NASA/ESA/STScI

Boasting intricate patterns and translucent colors, planetary nebulae are among the most
beautiful sights in the universe. How they got their shapes is complicated, but
astronomers think they’ve solved part of the mystery—with giant blobs of plasma
shooting through space at half a million miles per hour.
Planetary nebulae are shells of gas and dust blown off from a dying, giant star. Most
nebulae aren’t spherical, but can have multiple lobes extending from opposite sides—
possibly generated by powerful jets erupting from the star.
Using the Hubble Space Telescope, astronomers discovered blobs of plasma that could
form some of these lobes. “We’re quite excited about this,” says Raghvendra Sahai, an
astronomer at NASA’s Jet Propulsion Laboratory. “Nobody has really been able to come
up with a good argument for why we have multipolar nebulae.”
Sahai and his team discovered blobs launching from a red giant star 1,200 light years
away, called V Hydrae. The plasma is 17,000 degrees Fahrenheit and spans 40
astronomical units—roughly the distance between the sun and Pluto. The blobs don’t
erupt continuously, but once every 8.5 years.
The launching pad of these blobs, the researchers propose, is a smaller, unseen star
orbiting V Hydrae. The highly elliptical orbit brings the companion star through the outer
layers of the red giant at closest approach. The companion’s gravity pulls plasma from the
red giant. The material settles into a disk as it spirals into the companion star, whose
magnetic field channels the plasma out from its poles, hurling it into space. This happens
once per orbit—every 8.5 years—at closest approach.
When the red giant exhausts its fuel, it will shrink and get very hot, producing ultraviolet
radiation that will excite the shell of gas blown off from it in the past. This shell, with
cavities carved in it by the cannon-balls that continue to be launched every 8.5 years, will
thus become visible as a beautiful bipolar or multipolar planetary nebula.
The astronomers also discovered that the companion’s disk appears to wobble, flinging
the cannonballs in one direction during one orbit, and a slightly different one in the next.
As a result, every other orbit, the flying blobs block starlight from the red giant, which
explains why V Hydrae dims every 17 years. For decades, amateur astronomers have
been monitoring this variability, making V Hydrae one of the most well-studied stars.
Because the star fires plasma in the same few directions repeatedly, the blobs would
create multiple lobes in the nebula—and a pretty sight for future astronomers.

 

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