In Class:
Question to Ponder
Occasionally, parts of the outer bits of the Sun can explode and
substantially increase the number of particles in the solar wind for a
short time. The particles released by these "coronal mass ejections"
are generally fast movers, with speeds of 700 km/s or more (typical
solar wind particles move at about 400 km/s). Based on this
information, how long after a "coronal mass ejection" is seen on the
Sun will the particles released reach the Earth?
(1 A.U. = 1.5 x 108 km)
- a) About eight minutes
- b) About an hour
- c) About a day
- d) About two days
- e) About a week
Why Isn't the Moon More Like Earth?
- Same distance from the Sun.
- (Roughly) the same composition.
- The big difference is size.
Why Does Size Matter?
- Size determines interior temperature.
- Small planets cool faster, and have less radioactive heating.
- So no plate tectonics, and no atmosphere production.
- Doesn't really matter anyway, since because the Moon's small,
it's gravity is weak -- too weak, in fact, to retain any gaseous atmosphere.
- With no atmosphere, liquid surface water isn't possible. The water
will boil away even at low temperatures with no surrounding air pressure.
So What Happens on The Moon?
- Not much.
- It's an airless, waterless, barren place.
- Only real surface evolution comes from meteorite impacts.
- Impacts create craters and pulverize the surface into a fine dust layer.
Formation of the Moon
- Two reasonable possibilities: capture and Earth impact.
- Capture isn't likely because it's hard and typically would result
in a moon with a highly eccentric orbit.
- Earth impact involves a glancing blow onto the early Earth by a
Mars-sized object.
- Most of the impactor's mass becomes a part of the Earth, but a small
amount could be ejected by the impact into orbit around the Earth.
- Explains why the moon has so little iron (e..g, material that made the
Moon was blasted off the outer layers of the Earth, where there's little iron).
- Detailed calculations show that such a scenario is plausible.
The Moon Since Formation
- Evolution via impacts.
- About 3.5-3.9 billion years ago, the Moon was pretty much fully formed.
- At that time, it's core was probably stll hot enough to be molten.
- The Moon was gravitationally differentiated, and the crust was rocky
material, seen today as the bright highlands region.
- A few massive impactors hit the Moon --- not quite big enough to
destroy it, but big enough to crack its crust and allow the molten
interior to seep out.
- Interior stuff seeps out, forms big lava lakes, and cools to form the
flat maria.
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