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Oct28_planetary_science.pptx

Planets of the solar system- a closer look

Three types:

Rocky (like Earth)

Smaller, close to sun

Terrestrial planets

Mercury

Venus

Earth

Mars

2. Big and gassy like Jupiter

Jovian planets

(Jove is synonym for Jupiter)

Jupiter

Saturn

Uranus

Neptune

And a third type is the dwarf planets which are small, cold, icy and similar to many satellites: Example: Pluto and the Galilean satellites of Jupiter

Goal today

Lay out differences  emphasis on earth’s uniqueness

Main causes of variations  size and distance from sun

(a minor cause of variations may be presence of a large moon

… more complicated, we’ll discuss over several lectures)

Main types of variations  temperature of planet,

its atmosphere (or lack)

surface features/geology

presence of water or ice

We’ve already discussed this

Venus is too close to the sun  too hot, oceans boiled away

Mars is too far  too cold, water and dry ice  no liquid

Earth is just right for liquid water  the “Goldilocks Zone”

Size considerations

Bigger planets have more gravity  can capture and keep a

thicker atmosphere. Its why the Jovian planets are gas giants.

Today, we focus on the smaller ones terrestrial and dwarf planets/icy moons

(and Earth’s moon)

Mercury

Moon

Start with some pictures- differences emerge

Earth

Mars

Venus

Whats the difference?

Earth photo

Mars photo

Google Earth

Google Mars

Clouds in the photo

Photo is hazier

Mercury

Moon

Atmospheres: Earth, Venus, and Mars have them

Mercury and Moon do not  too small (gravity too weak)

Earth

Mars

Venus

Venus: Our Evil Twin

Almost exactly the same size as Earth,

but choked in poisonous clouds of

sulfuric acid. Hellish conditions.

Atmosphere much thicker than earth-

acts as blanket (extreme greenhouse

effect- future lecture topic)

Surface temp = that of a self cleaning

Oven

The Russians landed a spacecraft on its

surface and it got fried after a couple of

minutes! We don’t know too much about

Its geology; there are probably volcanoes

Astronauts will never visit.

Note: Venus once might have been more habitable, but being

too close to the sun- the oceans evaporated away

Right now, Mars is more similar to Earth

even though its only 1/2 the diameter

Because Mars is significantly smaller, it has weaker gravity and

can’t keep as thick an atmosphere as the earth.

But still, some photos from the surface look strangly

familiar……….

What does this look like?

And This

Mars has sedimentary rock and sand like Earth. How did it get sand?

Weathering and erosion can occur on Mars (but very slowly since its air

pressure is so low (air is thin)).

Which is which planet? (Mars or Earth?)

PSC 121 Prince George's Community College

Did Mars have liquid water?

What are these?

Whats the similarity?

Whats the difference?

Yes! Mars has evidence for dried up rivers

and sedimentary rock

14

An old stream and delta

Fun facts: rotation of Mars is 25 hours (almost identical to Earth)

seasons/weather are somewhat similar (except no rain)

Mars has water, probably all frozen

Frost on Martian surface

Impact Craters: Whats the difference?

Mars Moon

Mars fewer than the moon. They aren’t as “sharp”- more eroded

Cratering: an important tool to study surfaces of planets and satellites

Surface of Callisto

Surface of Europa

Mars

Mercury

Craters do exist on Earth (rare)

Manicougan crater- Canada

(view from earth orbit)

Meteor Crater, Arizona, ¾ miles across

Crater Lake, OR: from a volcano

Ring-lake is 45 miles across

The meteor was 3 miles wide

215 million years ago (early Mesozoic)

The meteor was 160 feet across, 50,000 years ago

Panoramic view of Meteor Crater

What’s happening to this crater?

Its being weathered and eroded away  in a few 100 thousand

years, it will be gone

Cratering and surface changes

Misconception: Earths atmosphere protects us.

No! (ask the dinosaurs)

Reality: How fast craters disappear tells you about

weathering/erosion

Longer term: plate tectonics/volcanoes completely

change the surface

All planets get craters. They all get hit by meteors

Surface age

No weathering/erosion.

Altho there were some

Lava flows at one point

 The grey basalt

Some weathering

And erosion

Earth’s surface is

Very young

Zoomed in shot of horizon. Including haze in the atmosphere

Three possibilities for lack of craters on Pluto

 one hypothesis- in the outer solar system, things move

more slowly. They don’t crash with the same impact.

 2nd hypothesis. Ice can slowly flow (like glaciers)-erodes

the craters

 3rd hypothesis. Pluto does have a thin atmosphere. Some weathering?

The ices of Pluto: how many of the magnificent 7 elements do we have? What’s missing?

Fe (iron) and silicon- those are for rocks (Pluto is an ice world)

And Helium- mostly on the sun or Jupiter/Saturn

Carbon monoxide

On earth (and Venus and

Mars, we also have

CO2: carbon dioxide

Landforms of the Solar System

Both planets have mountains/volcanos

Olympus Mons on Mars. Largest

volcano in the solar system (25 km)

Mt. Everest: Highest mountain

on Earth (9 km)

Surface of Mars: Elevation changes

Rift Valley?

volcanos

Martian mountains come in bunches, not ridges like the earth. Why?

What you don’t see on Mars (or anywhere else in the solar system)

Plates!

Rock Formation: Earth, Moon and Mars

Why is igneous rock present on all three objects?

Why is metamorphic rock not likely to exist in great

amounts on Mars? (if at all)

Earth Mars Moon
Igneous Y Y Y
Sedimentary Y Y N
Metamorphic Y N N

If Mars doesn’t have metamorphic rock, and doesn’t have

Plate tectonics, what other rock should it not have

(hint: it’s a type of igneous rock)

Granite on Mars? (maybe)

The specific chemical varieties include things not found on Mars before. But apart from rounding out Mars’ rock collection, they have some pretty interesting things to tell us about Mars’ early history. The granite-like rocks are similar to some of the rocks that make up Earth’s earliest truly continental crust, which differs from the basalt that makes up the seafloor. That could have come about by partly melting pre-existing basalts that began to sink back into Mars’ still-soft interior, for example.

Regardless of how it happened, the idea that there was continental crust being manufactured on Mars makes that planet’s early history look more like the Earth’s than we thought. The researchers also note that the existence of some of these rocks “challenge[s] the simple idea of continuous cooling of the Martian mantle over geologic time, pointing to more complex global or local variation in mantle temperature”.

Curiosity finds continent-building rocks on Mars

Early Mars may have been a bit more like early Earth.

SCOTT K. JOHNSON - 7/13/2015, 6:35 PM

What makes Earth unique:

1. Only planet currently in the Habitable zone

 present day surface liquid water

2. Only planet with plate tectonics. Earth’s surface

gets recycled more than any other planet

Consequence for types of rocks found

3. Largest moon compared with the planet (to be

discussed next week)

Obviously: abundant life (but that’s biology,

and this is not a biology class! So the

three characteristics above are what really

counts in this class)

One unknown: do other planets have a liquid in their cores and

a mantle like the earth? Not sure. Recent evidence for

Mercury says it might have liquid in its core

Little Differences

Craters on earth are rare because weathering and erosion is more rapid

Moon has no atmosphere  most craters (actually Mercury because no lava flows)

Mars has a thin atmosphere  a lot of craters, more weathered and eroded than the moon

Summary of Earth Compared to other solar system objects

Similarities

Cratering and volcanism on Earth, moon and Mars

Sediments on both Earth and Mars (moon is all igneous rock)

River features on both Earth and Mars

Some atmospheric weathering (sand), ice,

and evidence of past liquid water on Mars but not the moon

Some other moons around other planets are totally covered in ice

Big Differences

Earth is the only object in the solar system with plate tectonics

 probably only object with lots of metamorphic rocks

 probably only object with long mountain ridges (and folds/faults)

 probably the only object with significant amounts of granite

Earth is the only object in the solar system with liquid surface water