December 10, 2004
Spitzer, Hubble Get Planet-Building ‘Snapshots’
JPL -- Two of NASA's Great Observatories, the Spitzer Space Telescope and the Hubble Space Telescope, have provided astronomers an unprecedented look at dusty planetary debris around stars the size of our Sun.
Spitzer has discovered for the first time dusty discs around mature, Sun-like stars known to have planets. Hubble captured the most detailed image ever of a brighter disc circling a much younger Sun- like star. The findings offer "snapshots" of the process by which our own solar system evolved, from its dusty and chaotic beginnings to its more settled present-day state.
"Young stars have huge reservoirs of planet-building materials, while older ones have only leftover piles of rubble. Hubble saw the reservoirs and Spitzer, the rubble," said Dr. Charles Beichman of NASA's Jet Propulsion Laboratory, Pasadena, Calif. He is lead author of the Spitzer study. "This demonstrates how the two telescopes complement each other," he added.
The young star observed by Hubble is 50 million to 250 million years old. This is old enough to theoretically have gas planets, but young enough that rocky planets like Earth may still be forming. The six older stars studied by Spitzer average 4 billion years old, nearly the same age as the Sun. They are known to have gas planets, and rocky planets may also be present.
"The new Hubble image gives us the best look so far at reflected light from a disc around a star the mass of the Sun," said Hubble study lead author, Dr. David Ardila of the Johns Hopkins University, Baltimore. "Basically, it shows one of the possible pasts of our own solar system," he said.
Debris discs around older stars the same size and age as our Sun, including those hosting known planets, are even harder to detect. These discs are 10 to 100 times thinner than the ones around young stars. Spitzer's highly sensitive infrared detectors were able to sense their warm glow for the first time.
"Spitzer has established the first direct link between planets and discs," Beichman said. "Now, we can study the relationship between the two." These studies will help future planet-hunting missions, including NASA's Terrestrial Planet Finder and the Space Interferometry Mission, predict which stars have planets. Finding and studying planets around other stars is a key goal of NASA's exploration mission.
Rocky planets arise out of large clouds of dust that envelop young stars. Dust particles collide and stick together until a planet eventually forms. Sometimes the accumulating bodies crash together and shatter.
Debris from these collisions collects into giant doughnut-shaped discs, the centers of which may be carved out by orbiting planets. With time, the discs fade and a smaller, stable debris disc, like the comet-filled Kuiper Belt in our own solar system, is all that is left.
The debris disc imaged by Hubble surrounds the Sun-like star called HD 107146, located 88 light-years away. John Krist, a JPL astronomer, also used Hubble to capture another disc around a smaller star, a red dwarf called AU Microscopii, located 32 light-years away and only 12 million years old.
The Hubble view reveals a gap in the disc, where planets may have swept up dust and cleared a path. The disc around HD 107146 also has an inner gap.
Beichman and his colleagues at JPL and the University of Arizona, Tucson, used Spitzer to scan 26 older Sun-like stars with known planets, and found six with Kuiper Belt-like debris discs.
The stars range from 50 to 160 light-years away. Their discs are about 100 times fainter than those recently imaged by Hubble, and about 100 times brighter than the debris disc around the Sun. These discs are also punctuated by holes at their centers.
Both Hubble images were taken with the advanced camera for surveys. They will be published in the Astronomical Journal and the Astrophysical Journal Letters. The Spitzer observations are from the multiband imaging photometer and will appear in the Astrophysical Journal.
Videos and Animations
A Distant Solar System (Artist's Concept Animation) -- This animation portrays an artist's concept of a distant hypothetical solar system, about the same age as our own. It begins close to the star, and then moves out past a number of planets. Though "extrasolar" planets are too small to be seen with telescopes, astronomers have detected more than 100 gas giants like Jupiter via their gravitational tug on their parent stars.
The view pulls back to reveal the outer fringes of the system and a ring of dusty debris that circles the star. This debris is all that remains of the planet-forming disk from which the planets evolved.
Planets are formed when dusty material in a large disk surrounding a young star clumps together. Leftover material is eventually blown out by solar wind or pushed out by gravitational interactions with planets. Billions of years later, only an outer disk of debris remains.
These outer debris disks are too faint to be imaged directly by visible-light telescopes. They are washed out by the glare of the Sun. However, NASAÃ•s Spitzer Space Telescope can detect their heat, or excess thermal emission, in infrared light. This allows astronomers to study the aftermath of planet building in distant solar systems like our own.
Slow Connections (160x120): Windows Media (72 KB) | QuickTime 4.0 (52 KB)
Fast Connections (320x240): Windows Media (448 KB) | QuickTime 4.0 (832 KB) | QuickTime 6.0 (820 KB) | MPEG 1 (1 MB) | MPEG 4 (592 KB)
Full-Size (640x480): Windows Media (469 KB) | QuickTime 6.0 (1.5 MB) | MPEG 4 (1.5 MB)
The Evolution of a Planet-Forming Disk (Artist's Concept Animation) -- This animation shows the evolution of a planet-forming disk around a star. Initially, the young disk is bright and thick with dust, providing raw materials for building planets. In the first 10 million years or so, gaps appear within the disk as newborn planets coalesce out of the dust, clearing out a path.
In time, this planetary "debris disk" thins out as gravitational interactions with numerous planets slowly sweep away the dust. Steady pressure from the starlight and solar winds also blows out the dust. After a few billion years, only a thin ring remains in the outermost reaches of the system, a faint echo of the once-brilliant disk.
Our own solar system has a similar debris disk a ring of comets called the Kuiper Belt. Leftover dust in the inner portion of the solar system is known as "zodiacal dust."
Bright, young disks can be imaged directly by visible-light telescopes, such as NASA's Hubble Space Telescope. Older, fainter debris disks can be detected only by infrared telescopes like NASA's Spitzer Space Telescope, which sense the disks' dim heat.
Slow Connections (160x120): Windows Media (84 KB) | QuickTime 4.0 (60 KB)
Fast Connections (320x240): Windows Media (544 KB) | QuickTime 4.0 (1 MB) | QuickTime 6.0 (1 MB) | MPEG 1 (1.1 MB) | MPEG 4 (720 KB)
Full-Size (640x480): Windows Media (544 KB) | QuickTime 6.0 (1.9 MB) | MPEG 4 (1.9 MB)
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