Some time ago I asked a question about gravity on a hemispherical planet.
What would gravity be like on a hemispherical planet?
Would the water all boil away at first, quickly cooling the core of the planet? Would the ocean boil for centuries?
Some time ago I asked a question about gravity on a hemispherical planet.
What would gravity be like on a hemispherical planet?
Would the water all boil away at first, quickly cooling the core of the planet? Would the ocean boil for centuries?
It's impossible to discuss what would happen to the oceans because the planet itself wouldn't be able to exist in this scenario. Planets are round for a reason: any other shape is unstable for objects of their size and mass due to their self-gravity. Unless was it was a very small borderline planet you're cutting in half, it would break up pretty cataclysmically. Given enough time and no major interference from other nearby bodies, the planet would eventually reform into a new spherical planet with half the original volume.
Well, this seems pretty easy to treat as a Fermi problem.
The heat capacity of magma (and rock in general, I suppose) is about $2\;\mathrm{kJ}/(\mathrm{kg}\cdot \mathrm{K})$.
The heat capacity of water is about $4\;\mathrm{kJ}/(\mathrm{kg}\cdot \mathrm{K})$, and it's latent heat of vaporization is about $2000\;\mathrm{kJ}/\mathrm{kg}$.
The total volume of the oceans is about $10^9\;\mathrm{km}^3$, so the total mass of water is about $10^{21}\;\mathrm{kg}$.
The total mass of magma/rock is, to a very good approximation, just the mass of the Earth, about $6\times10^{24}\;\mathrm{kg}$.
Assuming the oceans are at about $0^\circ\mathrm{C}$ (close enough), to boil them away would require:
$$\left(4\;\mathrm{kJ}/(\mathrm{kg}\cdot \mathrm{K}) \times 100\;\mathrm{K} + 2000\;\mathrm{kJ}/\mathrm{kg}\right)\times 10^{21}\;\mathrm{kg} = 2.4\times10^{24}\;\mathrm{kJ}$$
This would reduce the temperature of the magma by about:
$$\frac{2.4\times10^{24}\;\mathrm{kJ}}{2\;\mathrm{kJ}/(\mathrm{kg}\cdot \mathrm{K})\times 6\times10^{24}\;\mathrm{kg}} = \mathbf{0.2\;\mathrm{K}}$$
I'm assuming here that heat is rapidly conducted through the magma (relative to the rate of heat transfer to the ocean water). This seems more or less reasonable, and depends pretty sensitively on how water is flowing into the gap. The point is that there is plenty enough energy in the mantle to boil off the oceans.
How long it would take to boil away the oceans would depend how fast they're flowing into the gap between the hemispheres. It's also likely that the huge amounts of water vapour released into the atmosphere would wreak all kinds of havoc on the weather, and a lot of it would fall again as rain. The process of cooling the "flat" surfaces of your split planet would more or less reduce to the initial cooling of the surface of the Earth, and I guess proceed on similar timescales (though there is now significantly less heating in the mantle from the decay of radioactive isotopes, I think). What matters is how fast the vast amounts of energy stored thermally in the mantle can be transported away. You need the atmosphere to efficiently convect superheated air/steam out of the gap, and then efficiently dissipate the heat out into space (this probably works ok-ish, radiatively). It will still take a long time (geological timescales) to cool the flat sides of your hemispheres. A lot of estimation starts to break down now, because you need to know about things like pressure in the hemispheres, and because the hemispheres are not a stable structure, trying to treat them with physics breaks down at some point.