Abstract
An analysis of hundreds of star-grazing comets in a young planetary system shows that they form two families: a group of old, dried-out comets and a younger group probably related to the break-up of a larger planetary body. See Letter p.462 The nearby star β Pictoris possesses a young planetary system that appears much like our own would have been few million years after its formation. This analysis of more a thousand archival spectra recorded between 2003 and 2011 reveals variable dust absorption signatures arising from transiting exocomets belonging to two distinct families of comets. First, an old volatile-exhausted population displaying signs of orbital evolution due to interactions with the host planet and second, a volatile-rich population presumably originating from the break-up of a few parent bodies.
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