Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19 Uranus -- God of the Sky He gives his name to Urania the Greek muse of astronomy Discovery of Uranus The other planets can only be seen with a telescope Herschel had built a very high quality telescope and was systematically observing the brighter stars when he found Uranus Observing Uranus Even with the best Earth based telescopes Uranus appears as a small featureless blue-green disk Voyager 2 is the only spacecraft to visit Uranus and Neptune Uranus Facts Size: Orbit: Description: The Rotation of Uranus Extreme tilt may be due to a large impact when Uranus was forming The large tilt produces seasons where half of the planet is in sunlight and half in darkness for long periods of time Seasons on Uranus Composition of Atmosphere The atmosphere of Uranus is similar to those of Jupiter and Saturn, with one key difference Structure of Atmosphere Uranus is too cool to have the same high altitude clouds that Jupiter and Saturn have Careful observations have determined that Uranus does not have alternating zones and bands Uranus -- True and False Color Uranus’s Rings The ring system of Uranus was first seen through stellar occultation Rings are composed of dark material The Rings of Uranus The Moons of Uranus Uranus has 5 major moons (discovered from Earth) and 10 minor moons (discovered by Voyager 2) Moons are composed of mixture of ice and rock Two of the moons shepherd the Epsilon ring Uranus’s Moons and Rings Radiation Darkening Why are the moons and rings of Uranus (and Neptune) so dark? Impacts by high energy electrons from the magnetosphere break off the carbon atoms Magnetic Fields Fields on Uranus and Neptune Voyager data indicate that Uranus and Neptune have magnetic fields The centers of the magnetic fields are offset from the center of the planet Rotation and Magnetic Axis Determining Mass How are the masses of planets determined? We can measure the period and the orbital radius of a moon or spacecraft Neptune -- God of the Sea The name is appropriate due to Neptune’s bluegreen color The Discovery of Neptune In the early 1800’s it was noticed that Uranus’s orbit differed from predictions Two scientists J. C. Adams and U. J. Le Verrier tried to calculate where such a planet should be in 1845-1846 Observing Neptune Neptune shows no detail from Earth Neptune Facts Size: ~4 Earth diameters Orbit: 30.11 AU Description: Neptune’s Atmosphere Neptune shows much more distinct cloud bands and storms than Uranus Neptune has visible storms like Jupiter, but they appear to be short lived Clouds are formed into bands which rise and fall due to convection Composition and Heating Atmosphere’s composition similar to Uranus’s Neptune has more internal heat to power cloud motions Neptune from Voyager Spots on Neptune Clouds on Neptune The Rings of Neptune Neptune’s rings were discovered via occultation Caused by the gravity of a near-by moon Inner narrow ring has shepherd moons Neptune’s Rings and Arcs The Moons of Neptune Neptune has 7 small satellites and Triton (diameter= 2700 km) Triton may be a captured Kuiper Belt object Neptune and Triton The Interiors of Uranus and Neptune We can model each planet with a similar interior The two planets have relatively more heavy elements and less hydrogen than Jupiter and Saturn The Interiors of Uranus and Neptune The Formation of Uranus and Neptune At 20-30 AU the planetesimals were fewer and more widely dispersed than at 5-10 AU By the time they formed much of the hydrogen and helium was dispersed Summary Information comes from Voyager and HST Blue-green in color with white clouds Caused by methane Radiation darkening produces dark, soot colored rings and moons Interior composed of rocky core, water and ammonia mantle and hydrogen atmosphere Offset magnetic field Formed more slowly than Jupiter and Saturn and so captured less gas Summary: Uranus Discovered by accident (1781) Faint cloud patterns Due to low internal heat Tilted on its axis Causing non-uniform solar illumination Summary: Neptune Discovered through use of Newton’s laws (1846) Most distant gas giant Has more internal heat and stronger cloud features than Uranus