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GEOL 3045: Planetary Geology Lysa Chizmadia Saturn’s Satellites

GEOL 3045: Planetary Geology

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GEOL 3045: Planetary Geology. Lysa Chizmadia Saturn’s Satellites. Introduction. At least 60 moons Classification of Moons: A-ring Moonlets Ring Shepherds Co-orbitals Inner Large Moons Alkyonides Trojans Outer Large Moons Irregular Moons Inuit Group Norse Group Gallic Group. - PowerPoint PPT Presentation

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Page 1: GEOL 3045: Planetary Geology

GEOL 3045: Planetary Geology

Lysa ChizmadiaSaturn’s Satellites

Page 2: GEOL 3045: Planetary Geology

Introduction At least 60 moons

Classification of Moons:– A-ring Moonlets– Ring Shepherds– Co-orbitals– Inner Large Moons

Alkyonides Trojans

– Outer Large Moons– Irregular Moons

Inuit Group Norse Group Gallic Group

Image from: http://en.wikipedia.org/wiki/Saturn

Image from: http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Moons

Page 3: GEOL 3045: Planetary Geology

A-ring Moonlets 4 discovered in 2006 by

Cassini– 8 more discovered in 2007

Tiny moons inside the A-ring– Diameters: 0.06 to 0.14 km

Probably formed due to shattering of inner satellite during impact

Discovered by propeller-shaped disturbances in ring

Image from: http://www.theregister.co.uk/2007/10/25/moonlets_a_ring/Photo Credit: NASA

Page 4: GEOL 3045: Planetary Geology

Ring Shepherds Orbit within or just outside

rings Sculpt the rings

– Giving them sharp edges & gaps

5 named & 3 unconfirmed– Pan – Daphnis – Atlas – Prometheus – Pandora– S/2004 S3, S/2004 S4, S/2004

S6Image from: http://en.wikipedia.org/wiki/Shepherd_satellite

Prometheus (left) & Pandora (right) in Saturn’s F-ring

Image from:http://en.wikipedia.org/wiki/Pan_%28moon%29

Pan in Encke Division

Ripples caused by Daphnis

Image from: http://en.wikipedia.org/wiki/Daphnis_%28moon%29

Page 5: GEOL 3045: Planetary Geology

Co-orbitals Epimetheus & Janus Orbit differs by only 50 km Inner orbits are faster so

must approach each other When inner moon catches

outer moon, gravitational attraction boosts inner’s momentum, increasing orbit

Opposite happens to outer moon

Thus, they trade places when they pass each other

Images from: http://en.wikipedia.org/wiki/Epimetheus_%28moon%29

Image from: http://en.wikipedia.org/wiki/Janus_%28moon%29

Epimetheus

Janus

Page 6: GEOL 3045: Planetary Geology

Inner Large Moons Mimas (Herschel crater) Methone Anthe Pallene Enceladus * Tethys

– Telesto (L4)– Calypso (L5)

Dione (ice cliffs)– Helene (L4)– Polydeuces (L5)

http://en.wikipedia.org/wiki/Dione_%28moon%29

Mimas

Dione

http://en.wikipedia.org/wiki/Mimas_%28moon%29

Page 7: GEOL 3045: Planetary Geology

Enceladus Ice ridges &

Cryovolcanism

Images from: http://en.wikipedia.org/wiki/Enceladus_%28moon%29

Page 8: GEOL 3045: Planetary Geology

Outer Large Moons Rhea

– Homogeneous interior– 2 adjacent large craters– Possible ring system

Titan * Hyperion

– Chaotic rotation– Sponge-like texture

Iapetus– 2 tone coloration– High inclination– Equitorial ridge

Rhea

Image from: http://en.wikipedia.org/wiki/Rhea_%28moon%29Image from: http://en.wikipedia.org/wiki/Hyperion_%28moon%29

Hyperion

Images from: http://en.wikipedia.org/wiki/Iapetus_%28moon%29

Iapetus Iapetus

Page 9: GEOL 3045: Planetary Geology

Titan Only moon w/ dense atm

– Pressure: 1.6 bars– 98.4% N2, 1.6% CH3 & H-Cs – CH3 must be produced

Not from comets b/c CO Not from nebula b/c He, Ne

Only body with liquid on surface– Other than Earth– Liquid CH3 lakes

Diameter: 5150 km– Mercury: 4879 km– Moon: 3474 km

Images from: http://en.wikipedia.org/wiki/Titan_%28moon%29

Page 10: GEOL 3045: Planetary Geology

Irregular Moons 3 main groups

– Inuit Group– Norse Group– Gallic Group

Images from: http://en.wikipedia.org/wiki/Phoebe_%28moon%29

Pheobe

Page 11: GEOL 3045: Planetary Geology

Inuit Group Prograde irregular satellites Semi-major axes: 11-18 x 106 km Inclinations: 40-50 degrees Eccentricities: 0.15-0.48 Spectral homogeneity

– Similar to Gallic Group– Break up of single object

5 members:– Kiviuq– Ijiiraq– Paaliaq– Siarnap– Tarqeq

Image from: http://en.wikipedia.org/wiki/Ijiraq_%28moon%29

Page 12: GEOL 3045: Planetary Geology

Norse Group Retrograde irregular

satellites Semi-major axes: 12-

42 x 106 km Inclinations: 136-175

degrees Eccentricities: 0.13-

0.77 Composed of > 4

subgroups– two i=174 subgroups– Skathi subgroup– Narvi subgroup

Image from: http://en.wikipedia.org/wiki/Saturn%27s_Inuit_group_of_satellites

Page 13: GEOL 3045: Planetary Geology

Gallic Group Prograde irregular satellites Semi-major axes: 16-19 x

106 km Inclinations: 35-40 degrees Eccentricities: ~0.53 Spectral homogeneity

– Similar to Inuit Group– Break up of single object

4 members:– Albiorix– Bebhionn– Erriapus– Tarvos

Image from: http://en.wikipedia.org/wiki/Ijiraq_%28moon%29

Page 14: GEOL 3045: Planetary Geology

Summary At least 60 moons At least 6 groups

– A-ring moonlets– Shepherd moons– Co-orbitals– Inner large moons

Includes Enceladus– Outer large moons

Includes Titan– Irregular Moons

Inuit group Norse group Gallic group

Mimas– Herschel Crater

Dione– Whispy ice ridges

Enceladus– Ice ridges ~ Europa– Cryovolcanism

Rhea– Homogeneous interior– Possible ring system

Titan– H-C rich atmosphere– Liquid HC on surface

Hyperion– Sponge-like surface texture

Iapetus– Two-tone surface colors– Equatorial ridge