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Topic

Planetary Thermal Evolution

The modelling of how rocky planets lose the heat of their formation and how that cooling changes their interior structure, core composition and overall size.

Current clusters

science3 publishers

Roughness maps push Mercury's total contraction up by 10 to 30 percent

Mercury's lumpiest terrain carries the fewest shrinkage wrinkles, which the authors read as impact debris burying the record. Correct for that and total contraction rises to as much as 23 km, with the thermal models still to be redone.

Perspective Coverage

3 publishers
Builder
Builder 42%
Operator
Operator 33%
Investor
Investor 25%

Reality

Evidence64
Adoption18
Hype gap+22
Incentives40
Confidence66