The Jovian Planets, Part III Uranus and Neptune URANUS The God of the Heavens Physical Data Discovered by William Herschel in 1781 Diameter: 51,118 km (4.01 Dearth) Mass: 8.69x1025 kg (14.54 Mearth) Density: 1.24 g/cm3 Rotation Period: 17.24 hours o Tilt of Axis: 98 (retrograde rotation!) o Surface Temperature: 52 K (-366 F) Physical Data Orbital Semi-Major Axis: 19.18 AU Orbital Period: 84.01 years o Orbital Inclination: 0.8 Orbital Eccentricity: 0.047 Surface Gravity: 0.919 Earth gravity Satellites: 27 as of 2011 Magnetic Field: yes Uranus’ Interior MOLECULAR HYDROGEN ATMOSPHERE ICE ROCK The Discovery of Uranus First discovered planet even though at its closest to earth it can be seen with the naked eye Was recorded 22 times as a star on star charts before W. Herschel discovered it as a planet in 1781 m Uranus’ Motions N S N SUN N S S N S Uranus rotates on its side, producing strange seasons and day-night patterns Uranus’ Atmosphere COMPOSITION: 85% Hydrogen 15% Helium Traces of Methane CLOUDS: Mostly made of methane ice Featureless cloudtops (inconspicous bands) Uranus’ Magnetic Field Magnetic dipole is offset 31% from the center of the planet o Tilted -59 from rotational axis Comparable in strength to Earth’s (0.74 Earth’s) Uranus has aurora and radio emissions Uranus’ Rings Found from star occultations in 1977 Thought to be made of stone Uranus also has partial rings called “ring arcs” Also has sheperd satellites Uranus’ Moons All are named after William Shakespeare and Alexander Pope characters There are 15 known moons Uranus’ Moons MIRANDA: Surface is a weird mix of old and new terrain It has been proposed than it was shattered and reassembled in this way There was not enough heat to fuse it smoothly together m Uranus’ Moons ARIEL: Youngest surface of the Uranian Satellites There is evidence of tectonic activity It has faults over 10 km deep Uranus’ Moons TITANIA: Largest of Uranus’ moons Has faults up to 100 km across Has a heavily cratered surface NEPTUNE GOD OF THE SEA Physical Data First observed in 1846 by Johann Galle Diameter: 49,500 km (3.89 Dearth) Mass: 1.030x1026 kg (17.23 Mearth) Density: 1.61 g/cm3 Rotation Period: 16.11 hours o Tilt of Axis: 28.76 o Surface Temperature: 57 K (-357 F) Physical Data Orbital Semi-Major Axis: 30.06 AU Orbital Period: 164.79 years o Orbital Inclination: 1.8 Orbital Eccentricity: 0.009 Surface Gravity: 1.19 Earth’s gravity Satellites: 13 as of 2011 Magnetic Field: yes The Discovery of Neptune It’s existence was calculated before it was observed from variations of Uranus’ orbit from what was predicted Calculations were made by U.J. Leverrier, sent to Johann Galle at Berlin Observatory, and he found Neptune after searching for 30 minutes Galileo actually recorded Neptune twice in 1612 and 1613 in his notebooks as a background star in his drawings of Jupiter Neptune’s Interior ATMOSPHERE MOLECULAR HYDROGEN ICE ROCK Similar to Uranus Neptune’s Atmosphere 75% Hydrogen 25% Helium Small amounts of: Methane, Ammonia & Acetylene There are three majors cloud-top features: The Great Dark Spot Dark Spot 2 Scooter Neptune’s Atmosphere The Great Dark Spot: Anti-cyclone with a circulation period of 16 days About the size of Earth In southern hemisphere Neptune’s Atmosphere Great Dark Spot Scooter Dark Spot 2 Dark Spot 2: Smaller cyclone in S. hemispere Scooter: Fast rotating Rapidly changes shape Neptune’s Magnetic Field Magnetic dipole is offset 55% from center of Neptune o Tilted -47 with respect to rotational axis Has a field strength of 0.4x Earth’s at the equator Has aurora and radio emissions Neptune’s Rings Discovered in 1981 Brighter areas are ring arcs There is a total of 5 rings, all very thin Neptune’s Moons TRITON: Has thin atmosphere, geysers, and strange “cantaloupe terrain” Diameter: 3000km Neptune’s Moons Proteus: Second largest moon of Neptune discovered by Voyager Surprisingly, Neried, Neptune’s third largest moon was discovered from the ground before Proteus