Presentation is loading. Please wait.

Presentation is loading. Please wait.

Uranus, Neptune and Beyond

Similar presentations


Presentation on theme: "Uranus, Neptune and Beyond"— Presentation transcript:

1 Uranus, Neptune and Beyond
Physics 112 Star Systems Lecture 17 Uranus, Neptune and Beyond Kevin H Knuth University at Albany Fall 2012

2 The heavens are now seen to resemble a luxuriant garden, which contains the greatest variety of productions, in different flourishing beds William Herschel Discoverer of Uranus, Mimas, Enceladus, Titania, and Oberon

3 Comparison of Planetary Sizes

4 Comparison of Planetary Interiors

5 Uranus Mass: 8.68 x 1025 kg Diameter: 31,690 km Density: 1.29 gm/cm3
19.2 AU from the Sun Rotation: hours Revolution: 84 years “Surface” gravity: 7.77 m/s2 “Surface” Temp: -315° F Atmospheric Composition: 83% H2 15% Helium 2% Methane

6 Uranus

7 Uranus’ Rings

8 Uranus System

9

10 Uranus’ Moons Oberon Ophelia Portia Prospero Puck Rosalind Setebos
Stephano Sycorax S/1986 U10 S/2001 U2 S/2001 U3 S/2003 U1 S/2003 U2 S/2003 U3 Titania Trinculo Umbriel Ariel Belinda Bianca Caliban Cordelia Cressida Desdemona Juliet Miranda

11 Uranus’ Moons Miranda Ariel Umbriel Titania Oberon

12 Neptune Mass: 1.02 x 1026 kg Diameter: 61,400 km Density: 1.64 gm/cm3
30.1 AU from the Sun Rotation: hours Revolution: years “Surface” Temp: -243° to ° F Atmospheric Composition: 85% H2 13% Helium 2% Methane

13

14 Neptune vs. Earth

15 Neptune

16 High-Altitude Clouds

17 Cirrus Clouds on Neptune

18 Great Dark Spot

19 Small Dark Spot

20 Neptune’s Rings Neptune’s rings are almost broken into what we call ring arcs.

21 Neptune’s Moons Larissa Proteus Naiad Thalassa Triton Nereid
S/2002 N1 S/2002 N2 S/2002 N3 S/2002 N4 S/2003 N1 Naiad Thalassa Despina Galatea

22 Triton Mass: 2.14 x 1022 kg Diameter: 3,354 km Density: 1.29 gm/cm3
“Surface” Temp: -391° F Atmospheric Composition: Nitrogen (tenuous) Coldest known object in the Solar System. Triton is in a retrograde orbit. Due to its orbit and warped shape scientist’s believe that it once was a double planet and was captured by Neptune. Where its partner is is anyone’s guess!

23 Neptune and Triton

24 Ice Plain

25 Cantaloupe Terrain Such terrain has only been seen on Triton.
It is probably due to tectonic activity with liquid coming up through the cracks and refreezing.

26 A Closeup of Triton

27 Liquid Nitrogen Geysers!!!

28 Artist’s Conception

29

30 Detection of Triton’s Atmosphere

31

32 The Icy Worlds of the Kuiper Belt

33 Kuiper Belt

34

35 Kuiper Belt and Oort Cloud
While there are many Kuiper Belt Objects, there collective mass is estimated to be about 1/10 Earth’s mass.

36

37

38 Pluto, Charon and Nix and Hydra

39 Pluto from HST

40 Best Image of Pluto

41 Pluto Comparison

42 New Horizon’s Mission to Pluto
The New Horizons mission is on its way to Pluto. It will make Pluto closest approach on 14 July 2015

43 View from Eris (formerly Xena) and Dysnomia

44 View from Sedna


Download ppt "Uranus, Neptune and Beyond"

Similar presentations


Ads by Google