Planet Building More Chaotic Than Expected

by | Oct 19, 2004 | Exoplanetary Science

If planets form the way we used to think — in a relatively smooth condensation out of material surrounding young stars — then the dust discs from which they form should gradually fade from view. Planetary formation, in other words, should scour a solar system, leaving it relatively free of dust; other than their planets, older stars would show little signs of the material from which their systems were made.

But NASA’s Spitzer Space Telescope, working in the infrared, is telling a different tale. Studying the dusty discs around 266 nearby stars — all similar in size but varying in age — George Rieke of the University of Arizona, Tucson and colleagues have found 71 discs, presumably containing planets. And there goes the old theory, because within the first two hundred million years of a star’s life, there is no necessary correlation between the density of the disc and the star’s age.

Spitzer diagram of planetary formation

Image: The graph above shows the Spitzer findings. Along the vertical axis is the brightness (or size) of the disc), plotted against the age of the stars on the horizontal. You can see that huge amounts of debris persist around stars that are 100 to 200 million years old. Yet even among some of the youngest stars, no debris appears. The upshot: the collision rate between rocky objects in these systems varies widely from star to star. Credit: Credit: NASA/JPL-Caltech/G. Rieke (Univ. of Arizona).

“We thought young stars, about one million years old, would have larger, brighter discs, and older stars from 10 to 100 million years old would have fainter ones,” Rieke said. “But we found some young stars missing discs and some old stars with massive discs.”

Collisions between large objects may continue to infuse planetary discs with dust, up to hundreds of millions of years after the host star was formed. And planetary formation may be chaotic indeed, taking far longer than the 10 million years previously assumed by some theories. “It’s a mess out there,” adds Rieke. “We are seeing that planets have a long, rocky road to go down before they become full grown.”

More about these findings at the Spitzer telescope’s Web site. And here’s a San Francisco Chronicle story on the subject.

0 Comments

Now Reading

Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

Recent Posts

On Comments

If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. Human comments only, please -- cut and paste from AI will not be acceptable. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.


Advanced Propulsion Research

Beginning and End

Archives