Scientists have speculated that what appeared to be a warp in the main disk of dust was in fact a second disk. Confirmation of its existence has sparked new speculation that there is at least one gas giant in the stellar system. To see the second ring of dust, astronomers had to block the direct light from Beta Pictoris using the (currently offline) Advanced Camera’s coronagraph. The secondary disk, which is inclined at about four degrees from the main disk, is visible as far as 24bn miles from the star, despite being much fainter than the main dust belt. The...