Close-up photos of dying star show our sun's fate (w/ Video)

Dec 15, 2009
Chi Cygni changes brightness dramatically and regularly every 408 days due to in-and-out pulsations. Using interferometry to image the star's surface at four separate times, astronomers found that the star grows to a diameter of 480 million miles -- large enough to engulf the asteroid belt -- before shrinking to a minimum diameter of 300 million miles. Chi Cygni also shows significant hotspots near minimum radius. Credit: Sylvestre Lacour, Observatoire de Paris

(PhysOrg.com) -- About 550 light-years from Earth, a star like our Sun is writhing in its death throes. Chi Cygni has swollen in size to become a red giant star so large that it would swallow every planet out to Mars in our solar system. Moreover, it has begun to pulse dramatically in and out, beating like a giant heart. New close-up photos of the surface of this distant star show its throbbing motions in unprecedented detail.

"This work opens a window onto the fate of our Sun five billion years from now, when it will near the end of its life," said lead author Sylvestre Lacour of the Observatoire de Paris.

As a sunlike star ages, it begins to run out of fuel at its core. Like a car running out of gas, its "engine" begins to splutter. On Chi Cygni, we see those splutterings as a brightening and dimming, caused by the star's contraction and expansion. Stars at this life stage are known as Mira variables after the first such example, Mira "the Wonderful," discovered by David Fabricius in 1596. As it pulses, the star is puffing off its outer layers, which in a few hundred thousand years will create a beautifully gleaming planetary nebula.

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This movie combines infrared images of the surface of Chi Cygni, obtained with IOTA, with visual brightness measurements provided by the American Association of Variable Star Observers. Chi Cygni demonstrates a 408-day-period of expanding and dimming, followed by contracting and brightening. Credit: Sylvestre Lacour, Observatoire de Paris

Chi Cygni pulses once every 408 days. At its smallest diameter of 300 million miles, it becomes mottled with brilliant spots as massive plumes of hot plasma roil its surface. (Those spots are like the granules on our Sun's surface, but much larger.) As it expands, Chi Cygni cools and dims, growing to a diameter of 480 million miles - large enough to engulf and cook our solar system's .

For the first time, astronomers have photographed these dramatic changes in detail. They reported their work in the December 10 issue of The .

"We have essentially created an animation of a pulsating star using real images," stated Lacour. "Our observations show that the pulsation is not only radial, but comes with inhomogeneities, like the giant hotspot that appeared at minimum radius."

Imaging variable stars is extremely difficult, for two main reasons. The first reason is that such stars hide within a compact and dense shell of dust and molecules. To study the stellar surface within the shell, astronomers observe the stars at a specific wavelength of infrared light. Infrared allows astronomers to see through the shell of molecules and dust, like X-rays enable physicians to see bones within the human body.

The second reason is that these stars are very far away, and thus appear very small. Even though they are huge compared to the Sun, the distance makes them appear no larger than a small house on the moon as seen from Earth. Traditional telescopes lack the proper resolution. Consequently, the team turned to a technique called interferometry, which involves combining the light coming from several telescopes to yield resolution equivalent to a telescope as large as the distance between them.

They used the Smithsonian Astrophysical Observatory's Infrared Optical Telescope Array, or IOTA, which was located at Whipple Observatory on Mount Hopkins, Arizona.

"IOTA offered unique capabilities," said co-author Marc Lacasse of the Harvard-Smithsonian Center for Astrophysics (CfA). "It allowed us to see details in the images which are about 15 times smaller than can be resolved in images from the Hubble Space Telescope."

The team also acknowledged the usefulness of the many observations contributed annually by amateur astronomers worldwide, which were provided by the American Association of Variable Star Observers (AAVSO).

In the forthcoming decade, the prospect of ultra-sharp imaging enabled by interferometry excites astronomers. Objects that, until now, appeared point-like are progressively revealing their true nature. Stellar surfaces, black hole accretion disks, and planet forming regions surrounding newborn stars all used to be understood primarily through models. Interferometry promises to reveal their true identities and, with them, some surprises.

Explore further: 'Blockbuster' science images

Provided by Harvard-Smithsonian Center for Astrophysics

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mysticshakra
Dec 15, 2009
This comment has been removed by a moderator.
LKD
3.7 / 5 (3) Dec 15, 2009
@ mystic: ?! This is a really wonderfully interesting article. I would love to know why there seems to be duel peaks in the brightness curve, one peaks higher than the other consistently through the video. It even looks like the high peek of compression is increasing brightness, slightly and progressively. I am curious what kind of process might be occurring.
acarrilho
5 / 5 (2) Dec 15, 2009
Mystic must have a problem with scientific speculation.
omatumr
2 / 5 (4) Dec 16, 2009
You are right, mysticshakra!

The world of assumption at it's best.


A dying star actually gave birth to the solar system.

See: a.) Proceedings of Robert Welch Foundation Conference on Chemical Research XII. Cosmochemistry, 263-272 (1978); b.) Nature 277, 615-620 (1979).

With kind regards,
Oliver K. Manuel

yyz
5 / 5 (1) Dec 16, 2009
Has anyone looked for a possible ultraviolet bow shock/tail emanating from CH Cygni similar to that found for Mira( http://science.na...mira.htm )? While they have similar distances, CH Cygni lies in a rich Milky Way star field, which may hamper detection of such a feature.
mysticshakra
1 / 5 (1) Dec 19, 2009
Acarrillo

When speculation becomes standard practice and speculation starts outweighing evidence then yes, I do have a problem.

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