What, him too?
!@$!@$!@%!@%$
I just read the paper...
Great stuff! Mike Brown - thanks for the open publication of such interesting information. It's good to know when a piece is peer reviewed, but that's always slow and sometimes imperfect. Some at least of the reading public is ready to do it's own reviewing.
From the last paragraph of section 5:
On Titan, the solar insolation is so small that evaporative cooling dominates over any heating, so the lakes are never warmer than the overlying air, thus, on Titan an extra lifting mechanism - presumably mechanical lifting over topography - is required (to initiate convection).
I note there is no mention of the fact that because Titan's air can hold so much methane the mean molecular weight can decrease by 1% or more when the humidity is raised. Would this not also provide an extra lifting mechanism? Since it isn't mentioned in the paper I assume it's less significant than I thought, but I don't understand why. Can anyone enlighten me?
The final sentence is an exciting weather forecast:
With Titan's extensive north polar lakes, northern summer should be a time of dramatic northern cloud events.
In other words we ain't seen nothin yet! Let's hope we're still there watching.
Maybe we'll see some in the next few days - this is from Ciclops 'looking ahead':
On September 20 and 21, as Cassini approaches apoapsis, ISS will perform two observations of Titan’s trailing hemisphere. These observations will be acquired from a distance of 1.55-1.81 million km (0.97-1.12 million mi). The observations are designed to look for cloud motions over an 18-hour period, as well as to look for changes at Kraken Mare (one of the large lakes in the northern polar region).
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