lecture16-1 - Jovian system Massive, gas giant planet,...

Info iconThis preview shows page 1. Sign up to view the full content.

View Full Document Right Arrow Icon
This is the end of the preview. Sign up to access the rest of the document.

Unformatted text preview: Jovian system Massive, gas giant planet, ~0.001 Solar masses Europa: radius 1560km Orbital radius: 5.2 AU - distance beyond snowline where rock and water ice dominates 4 large Galilean moons: Io (period 3.55 days) Europa Ganymede Callisto 1:2:4 resonance between the orbital periods of the inner 3 satellites Extraterrestrial Life: Spring 2008 Gradient of mean density: Io 3530 kg/m3 Europa 3018 kg/m3 Ganymede 1936 kg/m3 Callisto 1851 kg/m3 density of rock (silicates) mixture of rock plus lower density ice (~920 kg/m3) Extraterrestrial Life: Spring 2008 Surface of Europa is made of water ice Mean density would be consistent with a 6% fraction of water by mass: e.g. 1450km rocky interior with a 110km thick layer of water (liquid or ice) at the surface Evidence for an ocean on Europa (1) Global surface appearance Europa surface has very few impact craters - only 3 with diameter > 3km Young surface Cratering rate in the outer Solar System is not well determined: models suggest an age between 10 million and 1 billion years Resurfacing must involve melting at least some of the ice Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 (2) Local surface features (3) Magnetic field measurements Jupiter has a strong magnetic field, which Europa is orbiting through. Magnetic fields are generated by currents - flows of charged particles. If Europa's interior does not conduct electricity, the moon cannot generate its own magnetic field and the field measured near the surface should be that of Jupiter alone If Europa's interior conducts electricity, then the motion of the moon through Jupiter's field induces a current, which distorts the Jovian field near the moon. Galileo images of the surface show blocks of ice, km-10s km in size, separated by ridges Crust has been fractured and then refrozen in place Appearance resembles pack ice floating on the ocean at the North Pole and off the coast of Antarctica Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 1 What could the conductor be? Rock and ice are both poor conductors A salty ocean beneath the ice would be a good conductor: explains the Galileo magnetic field measurements quite well An iron core would also be a good conductor: can't exclude this possibility and if one exists, analysis is much more complicated... Galileo measurements during a close flyby Prediction based on Jupiter's magnetic field if Europa has no field of its own Conclude that Europa does possess its own magnetic field, and hence that some part of the interior of the moon must be an electrical conductor... Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 Heat source for Europa Internal heat of small bodies (Moon, Mars, Mercury) is not enough to sustain geological activity for the life of the Solar System Tidal heating Tides are raised on Europa by the different gravitational force from Jupiter on the near / far side of the moon Stress and try to crack the surface Dissipation of the tidal energy results in heat in the moon's interior Moon is distorted (very slightly) by tidal gravitational force As it rotates, tidal bulges don't quite align with the axis between the Moon and Jupiter Dissipation of the tides leads to heating tidal lag Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 Io: moon closest to Jupiter Very strong tides lead to volcanic activity on the surface Possible oceans Current data provides little constraint on the thickness of the ice layer overlying the ocean. Two models: (1) Thin ice layer (~1km), fractured by tidal forces as Europa orbits Jupiter, or local heating from volcanic events at the silicate / water boundary (2) Thick ice layer (at least 20km) fractured by convection in the ice heated by tides Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 2 If Europa indeed has an ocean, are the basic conditions for life met? Water: yes Carbon: yes - surface of the other Galilean moons show abundant impact craters... meteorites on Earth deliver organic material and the same must be true for Europa Energy: possibly... unknown whether hydrothermal vents or volcanic activity occurs at the bottom of the ocean If energy is available, conditions in Europa's ocean (T ~ 0C, probably quite salty water) fall within the range for which extremophiles survive on Earth... Europa exploration No current spacecraft in the Jovian system, and no funded mission to return by NASA or ESA High priority for "outer planets" science, but expensive and difficult to fly to Europa (distance, low Solar flux, radiation environment near Jupiter) Europa orbiter could definitively establish the presence or absence of an ocean, and measure the depth of the ice Lander could sample the ice near the surface, and conceivably drill through to the ocean Extraterrestrial Life: Spring 2008 Extraterrestrial Life: Spring 2008 3 ...
View Full Document

This note was uploaded on 08/31/2009 for the course GEOL 3300 taught by Professor Staff during the Spring '08 term at Colorado.

Ask a homework question - tutors are online