Astronomers using the Atacama Large Millimeter/submillimeter Array
(ALMA) in Chile have discovered that planets orbiting the star Fomalhaut
must be much smaller than originally thought.
The discovery was made possible by exceptionally sharp ALMA images of a disc, or ring, of dust orbiting Fomalhaut, which lies about 25 light-years from Eart
The discovery was made possible by exceptionally sharp ALMA images of a disc, or ring, of dust orbiting Fomalhaut, which lies about 25 light-years from Eart
h.
It helps resolve a controversy among earlier observers of the system.
The ALMA images show that both the inner and outer edges of the thin,
dusty disc have very sharp edges. That fact, combined with computer
simulations, led the scientists to conclude that the dust particles in
the disc are kept within the disc by the gravitational effect of two
planets — one closer to the star than the disc and one more distant.
Their calculations also indicated the probable size of the planets — larger than Mars but no larger than a few times the size of the Earth. This is much smaller than astronomers had previously thought. In 2008, a NASA/ESA Hubble Space Telescope image had revealed the inner planet, then thought to be larger than Saturn, the second largest planet in our Solar System. However, later observations with infrared telescopes failed to detect the planet
Their calculations also indicated the probable size of the planets — larger than Mars but no larger than a few times the size of the Earth. This is much smaller than astronomers had previously thought. In 2008, a NASA/ESA Hubble Space Telescope image had revealed the inner planet, then thought to be larger than Saturn, the second largest planet in our Solar System. However, later observations with infrared telescopes failed to detect the planet
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