Image: Mira
NASA / JPL-Caltech / OCIW
A new ultraviolet mosaic from NASA's Galaxy Evolution Explorer shows a speeding star that is leaving an enormous trail of "seeds" for new solar systems. The star, named Mira (pronounced my-rah) after the Latin word for "wonderful," is shedding material that will be recycled into new stars, planets and possibly even life.
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updated 8/15/2007 11:12:08 PM ET 2007-08-16T03:12:08

A dying star hurtling through space has left a cometlike tail that reveals its history stretching back 30,000 years.

"This is an utterly new phenomenon to us, and we are still in the process of understanding the physics involved," said study team member Mark Seibert of the Carnegie Observatories in Pasadena, Calif. "We hope to be able to read Mira's tail like a ticker tape to learn about the star's life."

The red giant star, called Mira A, is streaming a cometlike tail behind it that is 13 light-years long — thousands of times the breadth of our solar system. A light-year is the distance light travels in a year, about 6 trillion miles (10 trillion kilometers).

The tail is like a glowing bread-crumb trail in the sky, showing the star's movements for the past 30 millennia, during which time it has shed large stores of carbon, oxygen and other elements.

"If Neanderthal man had ultraviolet eyes and could look above the atmosphere, he could have seen the beginning of this tail forming," study leader Chris Martin, an astronomer at the California Institute of Technology, said during a teleconference Wednesday.

The researchers think Mira's tail might have once been much longer. "It may be that the tail slowly fades with time and we just can't see it because it's below our sensitivity level," Martin said. Or, he added, "it may be that the star has moved into a region of the interstellar medium that is denser, and that makes the tail light up more."

Our own sun will one day become a red giant, so the finding, detailed in Thursday's issue of the journal Nature, could provide valuable clues about the fate of our solar system and how stars' castoff remains become seeds for new stars, planets and possibly even life.

A pulsing star
Located about 350 light-years from Earth, Mira is a so-called variable star that pulsates from dim to bright over a period of about 330 days. At its brightest, Mira A is visible to the naked eye. Traveling alongside Mira A is another star, either a white dwarf or a smaller version of our sun, called Mira B.

Video: Star with a tail The two stars are separated by about 90 astronomical units (AU), with one AU being equal to the distance between the Earth and the sun. A previous study suggested that dust shed by Mira A is accreting into a ring around Mira B and could one day become the raw material for new planets.

The stellar pair is barreling through space at a swift 291,000 mph (468,000 kilometers per hour), possibly speeded along in their journey by occasional gravity boosts from other passing stars.

"Mira is racing through space like a speeding bullet, although it's actually 300 times faster than a bullet goes on Earth," Martin said.

Scientists spotted Mira A's tail of streaming gas while using the Galaxy Evolution Explorer, an Earth-orbiting telescope, to survey the sky in ultraviolet light. Nothing of its kind has ever been observed around a star.

Visible only in UV
The streaming tail is only visible in the far ultraviolet, which might explain why it's never been seen before despite the fact that astronomers have known about Mira A for about 400 years. "We never have predicted a turbulent wake behind a star that glows only with ultraviolet light," Seibert said.

Mira A was once a star like our sun. As it aged and lost the hydrogen fuel needed to stoke its internal fires, the star swelled into a pulsating red giant. Eventually, Mira A will eject all of its remaining gas into space, forming a colorful cloud around it called a planetary nebula. This too will fade in time, and Mira A will shrivel into a burnt-out white dwarf.

The Galaxy Evolution Explorer, a project of NASA also spotted a buildup of hot gas, called a bow shock, in front of the star, as well as two thin filaments of material coming out of the star's front and back. Astronomers think the hot gas in the bow shock is heating up the gas blowing off the star, creating a trailing tail that glows in the ultraviolet.

Michael Shara, a curator in the Department of Astrophysics at the American Museum of Natural History in New York City, called the new discovery "really remarkable."

"We're seeing ourselves," Shara said. "We are seeing in a sense the process that the sun will go through in a about 4 or 5 billion years when it starts to run out of fuel and its core turns into a red giant and starts to shed material. It's also in a sense looking at where we come from. It's our origins. All the carbon in our muscles and the oxygen that we breathe everytime we take a breath comes from red giant stars."

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