Journal article Open Access

Interior Structure of Neptune: Comparison with Uranus

Hubbard, W. B.; Nellis, W. J.; Mitchell, A. C.; Holmes, N. C.; Limaye, S. S.; McCandless, P. C.

Measurements of rotation rates and gravitational harmonics of Neptune made with the Voyager 2 spacecraft allow tighter constraints on models of the planet's interior. Shock measurements of material that may match the composition of Neptune, the so-calied planetary ;;ice,'' have been carried out to pressures exceeding 200 gigapascals (2 megabars). Comparison of shock data with inferred pressure-density profiles for both Uranus and Neptune shows substantial similarity through most of the mass of both planets. Analysis of the effect of Neptune's strong differential rotation on its gravitational harmonics indicates that differential rotation involves only the outermost few percent of Neptune's mass.

Files (239.5 kB)
Name Size
239.5 kB Download
Views 25
Downloads 4
Data volume 957.9 kB
Unique views 25
Unique downloads 4


Cite as