Respuesta :

Mercury's

Surface features

Quite a range of temperatures

Up to 400 deg. C at 'noon'

Proximity to sun supplies the daytime heat

Drops to -175 deg. C just before dawn

Lack of atmosphere allows the heat to escape at night

This would give your heat pump a real workout

Heavily cratered like the moon

With areas that have been flooded by basalt

Volcanic s very early in planets history (4 b.y.)

No evidence of plate tectonics

Isolated 'scarps' indicate shrinkage during cooling (fig. 13.25, pg. 232)

General tectonic history indicates:

Early expansion while hot

Releasing basaltic flows

Later shrinkage during cooling

Causing scarps due to compression/contraction

Venus's

Extremely harsh surface conditions

Temperature well above 400 deg. C

Atmospheric pressure 90X that of earth (we would implode!)

Both the result of the extremely dense atmosphere (96% CO2)

Thick cloud cover is the result of H2SO4 droplets in the atmosphere

Probably derived from extensive volcanic activity

Greenhouse effect

DIGRESS TO: runaway greenhouse effect

Venus used to be more like Earth

Almost certainly had large amounts of surface water

Initial slow surface heating due to small increase in atmospheric CO2

Leads to increased evaporation and H2O content in air

Leads to more heat retention, and the "Runaway Greenhouse Effect" cycle

Carried to its logical conclusion...

Leads to evaporation of any surface waters and a "hot water" atmosphere

Water vapor is not stable in UV light and breaks down into atomic form

Hydrogen escapes into space

Oxygen combines with iron, etc. at the surface

Therefore, the loss of surface water is permanent  

Marses

The "red planet" named for the God of War

Much smaller than the earth

Approx. 11% earth's mass

Atmosphere similar to Venus in composition (95% CO2)

But not in density - .006 bar (Mars) to 1 bar (Earth) to 90 bar (Venus)

Surface similar to earth 200 mya when Pangea was complete

Southern highland (continent) which is heavily cratered (probably older)

Surrounded by younger volcanic plains (not covered by water)

Several kilometers lower in elevation than the "continent"

Extensive tectonic and volcanic activity

No direct evidence of plate tectonic activity

Several features indicating tectonic/volcanic activity

Most 1-3 billion years old

Tharsis Bulge - active region the size of North America

Concentration of "recent" volcanic activity

Olympus Mons (fig. 14.8, pg. 241)

Probably largest volcano in solar system (fig. 15.14, pg. 268)

Possibly still intermittently active!

Valles Marineris (fig. 14.10, pg. 243)

A tectonic feature so not really a "valley"

Basically tension cracks on the edge of the Tharsis Bulge

Similar to tensional features in Africa

Big! 5000 km X 100 km X 7 km deep

Possibly plate-style activity may have started long ago

Did not develop like on earth due to smaller mass, quicker overall cooling

Much evidence for surface water (See: photo pg. 234; fig. 14.8b, pg. 241)

Most drainage features limited to older cratered highland areas

Two kinds of drainage patterns

Normal dendritic patterns (fig. 14.12, pg. 244)

Developed on the older cratered upland areas

Evidence for catastrophic floods (fig. 14.21, pg. 250)

From the upland onto the lava plains

Like the Channeled Scablands of Eastern Washington

Evidence for glacial ice ages in the Martian past?

Supports theory that surface water was present during 2 periods in the past

The first 4 billion years ago related to "normal" rainfall/runoff

Then later a sudden release of frozen water by volcanic heating, or?

All surface water now frozen into polar ice caps

Jupiter  

In orbit: 16 moons, faint ring

Has an extensive cloud cover

Vivid colors (white, orange, red, brown)

Essentially condensed ammonia (anyone for a walk in the rain?)

Great Red Spot (fig. 16.2, pg. 276) and (fig. 16.12, pg. 284)

A large "storm" in the atmosphere - almost 30,000 km across!

Has been "stable" for at least 300 years

How can it last for so long?

Nothing solid to interfere with the circulation of the gas

Saturn

In orbit: 19 moons. extensive rings

Uranus

In orbit: 15 moons, intricate system of dark ringsNeptune

In orbit: 8 moons, faint rings

Great Dark Spot: similar to GRS on Jupiter

Atmospheric storm 10,000 km acrossPluto

Discovered after a systematic search

Its presence was indicated by "wobbles" in Neptune's orbit

In orbit: a single large moon (Charon)

Essentially a binary system

if u need more information just go hear http://www.seds.org/nineplanets/nineplanets/

really hope this information helps and have a nice day