Module 4 - Follow the WaterMain MenuPhysical states of waterAnomalous properties of waterWater throughout the Solar SystemMercuryVenusMoonMarsWater in the outer Solar systemIce Giants – Uranus, NeptuneThe Icy satellitesTidal Heating - crunchy on the outside, liquid goodness on the insideIcy Geysers on EnceladusEuropa’s sub-surface oceanPlutoA final Splash - SummaryFrank Fuetendee05431475b87c68ebf15bbea4bfeac11808e9eMariek Schmidt3b678a5bd42eb8bf9a55fb761e5f17b11ce872c1
Interior of Uranus
12016-05-13T09:16:19+00:00Frank Fuetendee05431475b87c68ebf15bbea4bfeac11808e9e161The interior of both Uranus and Neptune are very similarplain2016-05-13T09:16:19+00:00Frank Fuetendee05431475b87c68ebf15bbea4bfeac11808e9e
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1media/Neptune_Uranus.jpg2016-05-09T12:46:04+00:00Ice Giants – Uranus, Neptune12image_header2020-06-30T18:45:45+00:00Uranus and Neptune are sometimes referred to as ice giants by astronomers. Both have similar internal structures. They possess a rocky core which is surrounded by liquid mantle and overlain by a gaseous atmosphere. The atmosphere contains some water vapour, but the bulk of the water in both planets is contained within the mantle. In addition to water, other ices in the mantle are methane and ammonia. Even though these mantles are often referred to as icy, their interiors are very hot. The internal core temperatures of Uranus are thought to reach 5000 K (4726.85°C) and possibly a bit higher for Neptune. Core pressures of the planets are approximately double that of the Earth 7-8 Mbar (~700-800 GPa). Under these conditions the mantles are very hot dense liquids. Why then are they referred to as ices?
Look back to the phase diagram we discussed before. At high pressures and temperatures the boundary between the ice and liquid is nearly horizontal. The core pressures of 7-8 Mbar solidly within the ice-only field and even the mantles are icy mixtures. The take-away from this is that under extreme conditions substances are forced into atomic arrangements unlike anything we experience on Earth.
The icy mantles of the ice giants exhibit unusual properties and electrically are very conductive. Both Uranus and Neptune have a layer of superionic water. Despite its name, this is not a new health drink, but a theoretical phase of water under extreme heat and pressure which has properties of both a solid and a liquid.
One question remains. If there is water vapour in the atmosphere and a strange hot, liquid water ice mixture in the mantle, is there a layer of liquid water somewhere in between? This question has been addressed in a paper entitled “Liquid water oceans in ice giants”. The conclusion is that at present Neptune only has a 15% chance of a liquid ocean. That chance will increase when the Sun becomes a cool white dwarf as it ages. So, let’s check back in a few billion years.