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Uranus and Neptune Overview

Jul 23, 2025

Overview

This lecture compares the planets Uranus and Neptune, focusing on their similarities, internal structures, atmospheres, magnetic fields, weather, and unique features.

Similarities Between Uranus and Neptune

  • Uranus and Neptune are similar in size and both appear bluish.
  • Their atmospheres are primarily hydrogen and helium, with about 5% methane giving them their blue color.
  • Both planets have three main layers: a solid rocky core, a water-ammonia ocean, and a gaseous atmosphere.
  • Both planets have magnetic fields generated by their conductive water-ammonia oceans.

Internal Structure

  • The innermost layer is a solid, rocky core composed mainly of iron and silicates under high pressure.
  • The middle layer is an ocean of water with ammonia (and some methane), similar to industrial cleaning fluid.
  • The outer layer is an atmosphere mostly made of hydrogen, helium, and some methane.

Magnetic Fields

  • Magnetic fields on Uranus and Neptune are generated by the motion of their water-ammonia oceans.
  • Their magnetic fields are significantly tilted, almost 90 degrees off from the planetary rotation axis.
  • Possible explanations for this tilt include magnetic field flipping or the presence of a theorized “liquid diamond” layer.

Atmospheric Appearance and Weather

  • Uranus and Neptune show little atmospheric detail compared to Jupiter and Saturn due to lower gravity spreading out cloud layers.
  • Despite plain appearances, both planets have active storms and turbulence deep in their atmospheres.
  • Infrared imaging reveals hidden atmospheric bands and storms, especially on Uranus.

Axial Tilt and Rotation

  • Uranus is highly tilted, rotating almost completely on its side (most tilted planet).
  • Neptune is not significantly tilted compared to Uranus.

Clouds and Storms

  • Visible clouds on Uranus and Neptune are made of methane ice due to extremely cold temperatures.
  • Methane ice clouds appear white because frozen particles reflect sunlight.
  • Neptune formerly had a large storm called the "Great Dark Spot," similar to Jupiter’s Great Red Spot, which has since disappeared.
  • Uranus has its own storms, mostly visible in infrared wavelengths.

Key Terms & Definitions

  • Methane — a colorless, odorless gas; present in the atmospheres of Uranus and Neptune, causing their blue color.
  • Water-ammonia ocean — liquid layer under the atmosphere, composed of water and ammonia.
  • Rocky core — dense inner center made of rock and metal.
  • Magnetic field — invisible field generated by moving, electrically conductive materials inside a planet.
  • Axial tilt — the angle between a planet's rotational axis and its orbital axis.
  • Methane ice clouds — frozen methane particles forming cloud layers in the upper atmospheres.

Action Items / Next Steps

  • Review planetary layers and magnetic field concepts for Uranus and Neptune.
  • Read assigned textbook section on outer planets’ atmospheres and internal structures.