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Herschel spots comet massacre around nearby star
Researchers suggest that dust grains in a belt around Fomalhaut must be large, fluffy aggregates, similar to dust particles released from comets in our solar system.
By
ESA, Noordwijk, Netherlands —
Published:
April 12, 2012 This image shows the infrared emission from the young star Fomalhaut and the dust disk surrounding it, as recorded with ESA's Herschel Space Observatory at a wavelength of 70 micron. To explain the emission from Fomalhaut's debris disk, astronomers invoke a steady production of dust particles via comet collisions, with an average rate of 2,000 daily collisions between comets of 0.6 mile (1 kilometer) across or, alternatively, of two daily collisions between 6-mile-diameter (10km) comets.
Photo by ESA/Herschel/PACS/Bram Acke, KU Leuven, Belgium
Fomalhaut is a young star, just a few hundred million years old, and twice as massive as the Sun. Its dust belt was discovered in the 1980s by the IRAS satellite, but Herschel’s new images of the belt show it in much more detail at far-infrared wavelengths than ever before.
Bram Acke at the University of Leuven in Belgium and colleagues analyzed the Herschel observations and found that the dust temperatures in the belt are between -382° and -274° Fahrenheit (-230° and -170° Celsius). However, because Fomalhaut is slightly off-center and closer to the southern side of the belt, the southern side is warmer and brighter than the northern side.
Both the narrowness and asymmetry of the belt are thought to be due to the gravity of a possible planet in orbit around the star, as suggested by earlier Hubble Space Telescope images.
The Herschel data show that the dust in the belt has the thermal properties of small solid particles, with sizes of only a few millionths of a meter across.
But this created a paradox because the Hubble Space Telescope observations suggested solid grains more than 10 times larger.
Those observations collected starlight scattering off the grains in the belt and showed it to be very faint at Hubble’s visible wavelengths, suggesting that the dust particles are relatively large. But that appears to be incompatible with the temperature of the belt as measured by Herschel in the far-infrared.
To resolve the paradox, Acke and colleagues suggest that the dust grains must be large, fluffy aggregates, similar to dust particles released from comets in our solar system.
These would have both the correct thermal and scattering properties. However, this leads to another problem.
The bright starlight from Fomalhaut should blow small dust particles out of the belt very rapidly, yet such grains appear to remain abundant there.
The only way to overcome this contradiction is to resupply the belt through continuous collisions between larger objects in orbit around Fomalhaut, creating new dust.
To sustain the belt, the rate of collisions must be impressive: each day, the equivalent of either two 6-mile-sized (10 kilometers) comets or two thousand 0.6-mile-sized (1km) comets must be completely crushed into small, fluffy dust particles.
“I was really surprised,” said Acke. “To me, this was an extremely large number.”
To keep the collision rate so high, there must be between 260 billion and 83 trillion comets in the belt, depending on their size. Our solar system has a similar number of comets in its Oort Cloud, which formed from objects scattered from a disk surrounding the Sun when it was as young as Fomalhaut.
“These beautiful Herschel images have provided the crucial information needed to model the nature of the dust belt around Fomalhaut,” said Göran Pilbratt, ESA Herschel project scientist. |
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