Schol SPACE Flashcards
What gives a planet a magnetic field?
Mobile conductive fluids.
Eg. Earth’s outer core of molten iron and nickel
What is implied if a planet has a strong magnetic field?
It has a large liquid core
The core is rich in metals
High rotation rate
What does earth’s magnetic field do?
protects the earth from high levels of radiation 
Prevents erosion of the atmosphere
How does the magnetic field affect solar wind?
Solar wind = stream of energetic charged particles from the sun
Mag field deflects the charged particles. Channels some charged particles into the Van Allen radiation belts.
Solar winds cause the magnetic field to be compressed on the side closest to the sun, and extend far out away from it.
Lack of magnetic field results in…
Eg Mars
Solar winds not deflected, strips away atmosphere so it is very thin. Low surface pressure
Why does venus and Mercury have a weak magnetic field
Both rotate slowly (compared to earth)
No evidence of tectonic activity on Venus
Weak mag field on Mars suggests circulation of a molten iron core (due to eccentric orbit and large tidal forces)
Define ‘locking’
Give an example
An object has the same rotational period as it’s orbital period
Eg moons generally have synchronous rotation with the planet (1:1 tidal locking)
Tidally locked planets in the solar system
Generally only planets within close proximity of a star can be tidally locked
Mercury 3:2, as orbit is eccentric
(Rotates 3 times for every 2 orbits)
Define habitable zone
Area around a star where the temp allows LIQUID water to exist on the surface of a planet
Depends on the type of star (eg red dwarf zone is closer to the star, likely to be tidally locked)
Define tidal flexing
Occurs when interior of orbiting body subjected to FRICTIONAL FORCES because of the gravity of the thing it’s orbiting.
Effects of tidal flexing on moons around gas giants (Jupiter)
Huge planet, large grav forces.
Cold, but friction creates heat… perhaps some moons are habitable
Effects of tidal flexing are amplified if orbit is eccentric.
Eg tidal bulges on Io (Jupiter’s closest moon). Close to planet, large bulge.
Tidal locking and Io
Elliptical orbit and huge tidal forces. Variation of orbit causes variation in flexing, causes further friction.
Causes frictional heating of rocks into magma and VOLCANISM on the surface.
The most volcanically active body in the solar system due to huge tidal forces from Jupiter AND other large moons (Europa, Ganymede)
Tidal locking and Enceladus
Icy, high albedo. BUT may have ocean under ice because of heating by tidal flexing, keeps water under the surface in liquid form.
Evidenced by plumes of water vapour and salty ice.
Possibility of geothermal vents due to flexing
—> extremophiles: potential for Chemotropic (and halotrophic) life forms… similar to those around geothermic vents. Plumes of water contain CO2, source of carbon.
Tidal flexing and Europa
Thick ice on surface.
May be liquid water ocean under ice
Possibility of underwater volcanoes as a result of tidal flexing
Requirements for life
Conditions that allow liquid water to be present
(warmth from sun/geothermal activity/tidal flexing)
A carbon source (C compounds for catabolism/anabolism)
Energy source to ‘fix’ inorganic C to organic. (Photosynthesis / chemosynthesis)
Protection from harmful radiation, and TIME for life to evolve (4 billion years for earth)