Planets Flashcards

(16 cards)

1
Q

Mercury’s exterior

A
Uniformly Cratered
Slightly larger than moon
~600K in Day, ~100K at Night
Slow rotation
Ice deposits in permanent shadow
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2
Q

Mercury’s interior

A

Smaller size means smaller pressure
Made of heavier elements
Large iron core

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3
Q

Why is Mercury’s mag field surprising?

A

Inside should be cooled and mostly solid, plus rotational period is slow, however still has weak mag field. Large Iron core can release a lot of heat at liquid solid boundary, latent heat of crystallization is released, sending liquid iron core into convective motion

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4
Q

Venus’ exterior

A

Same size as Earth
Few craters
Surface relatively young (500mil)
Some faults and ridges

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5
Q

Venus’ interior

A

Average density, similar to Earth

Expected liquid iron core, however no mag field due slow rotation

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6
Q

Why is Venus’ surface so young?

A

Flake tectonics - Easy for magma to break through and reset due to thin crust

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7
Q

Mars’ exterior

A
24.5 hour day
normal rotation
Southern highlands heavily cratered
Northern lowlands less cratered and younger
Hotspot volcanoes
Huge canyons
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8
Q

Mars’ interior

A
Density similar to earth
cooled significantly due to smaller size
Northern lowlands could have been resurfaced due to thinner crust
residual magnetism in old highland rocks
polar caps of frozen CO2
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9
Q

Jupiter’s general properties

A
320Me, 11Re
165K
Average density low - 1300kgm-3
immense pressure in core
made of light elements
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10
Q

Jupiter’s structure

A

Rotational flattening indicate rocky core
outer core made of liquid ice(CH4, NH3, H20) from captured icy meteroids and comets
Bulk of Jupiter made up of liquid metallic H, acts as conductor for mag field
fast rotation helps
Outer layer ordinary H and He
No solid surface

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11
Q

Jupiter’s heat

A

emits twice the amount of heat energy than it absorbs
Brown dwarf style?
Still cooling from formation
Internal heat due to convection flows

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12
Q

Saturn’s properties

A

Similar to Jupiter

less massive/less pressure = less dense

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13
Q

Saturn’s ring properties

A

Thin sheet of orbiting particles

In region where tidal forces would have broken up moons

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14
Q

Uranus’ properties

A

Smaller the Jupier, similar density
Rocky core surrounded by mantle of compressed water and ammonia
rotational axis perpendicular to orbit

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15
Q

Uranus’ mag field

A

Pressure high enough for ions to dissolve in liquid
Water and ammonia
Causes a mag field with these as conductors
Aurorae seen
Mag field misaligned and off center
rotation axis off centre
large impact?

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16
Q

Neptune’s properties

A

More massive than Uranus
Larger rocky core
Internal heat source