Models of the internal structure of Neptune with a rotation period determined from Voyager-2 data

Details Models of the internal structure of Neptune with a rotation period determined from Voyager-2 data Models of the internal structure of Neptune with a rotation period determined from Voyager-2 data

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..174g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Feb. 1990, p. 174-177. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Neptune (Planet), Planetary Rotation, Planetary Structure, Astronomical Models, Planetary Magnetic Fields, Voyager 2 Spacecraft

Scientific paper

New models of the Neptune internal structure are calculated, using the value of the magnetic-field rotation period of the planet (tauH = 16 h 3 min) determined from Voyager-2 data. The old value of tau = 18 h characterizes the rotation of the planet's equatorial zone and is evidence of its significant differential rotation. The new models for Neptune are similar to those for Uranus.

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