By 5.30pm local time in Prague (GMT+2), we were on version three of the planet definition. A second discussion had been scheduled, after lunchtime saw vociferous opposition to version two (which I blogged about here). A crowd gathered outside the designated room.
I was expecting to be treated to another lively exhibition of dissent – but it was not to be. Jocelyn Bell Burnell, the astronomer who discovered pulsars and a member of the IAU’s resolution committee, took formidable control of the meeting.
With only 45 minutes set aside, she said, comments were to be no more than “elevator pitches” – an idea sold in the time it takes a lift to travel one floor. “And I will cut you off if you are not brief,” she warned. The astronomers meekly followed orders.
Version three, distributed as we filed in for more drama, was a compromise that also seemed to have dissipated much of the earlier anger. It differed from version two mostly in emphasis.
That earlier definition had required first and foremost that a planet be round, then lumped planets that were not “dominant” in their local population into a subcategory of dwarf planets. The new definition required that a planet be both round and dominant, then put any round objects left over into a “dwarf-planet” category.
The details get confusing, but Bell Burnell spelled out the consequences of shuffling the priorities, “this means that Pluto is a dwarf-planet, but it is not a planet.”
Would that be acceptable to the assembled astronomers?