Use LEFT and RIGHT arrow keys to navigate between flashcards;
Use UP and DOWN arrow keys to flip the card;
H to show hint;
A reads text to speech;
131 Cards in this Set
- Front
- Back
Venus and Mars are _______ planets.
|
Terrestrial
|
|
Venus is a bit ______ than Earth and has the same _____.
|
smaller
density |
|
Venus' orbit radius is _____ AU, meaning it is _____ to the sun than the Earth.
|
0.75
closer |
|
In 1962, Astronomers started using ____________ and ________ to start looking at the surface of Venus.
|
radio telescopes
radar wavelengths |
|
Retrograde Rotation (Venus demonstrates this)
|
planet is rotating backwards relative to other planets
|
|
Venus rotates extremely ____
|
slow
|
|
Venus (does/does not) have a magnetic field.
|
does not
|
|
Atmosphere of Venus:
|
96% Carbon Dioxide
3.5% Nitrogren Small amount of water, sulfuric acid, hydrochloric acid, and hydroflouric acid. |
|
Why should Venus have been "wet"?
|
As the sun aged, it got warmer and so did Venus - vaporizing the water.
|
|
Why is Venus so hot?
|
A "runaway" greenhouse effect took place, baking the carbon dioxide out of the crust and leaving the planets surface at about 900 degrees.
|
|
Clouds of Venus are made from _____ and droplets of _______.
|
sulfur
sulfuric acid |
|
The density of Venus' atmosphere is about _____ times that of Earth.
|
90
|
|
Venus (has/does not have) plate tectonics.
|
does not have
|
|
Venus' surface (is/is not) very volcanic.
|
is
|
|
Shield Volcano
|
Volcanoes are like those in Hawaii "hot spot" volcanoes.
No steep slope, more liquid lava. |
|
The surface of Venus is made from ______.
|
basalt
|
|
______ craters on Venus' surface means that the age is very _____.
|
Few (under 1000)
Young (500 million years old) |
|
Mars is relatively small; only ____ percent of Earth's volume.
|
15
|
|
Expect Mars to have ____ it's internal heat.
|
lost
|
|
Distance from the sun is about ____ AU.
|
1.5
|
|
The axis of Mars is tipped 24 degrees, leading to _____.
|
seasons
|
|
Mars (has/does not have) polar ice caps.
|
has
|
|
Best to view Mars at _______.
|
opposition
|
|
Mars (does/does not) currently have a magnetic field.
|
does not
|
|
The atmosphere of Mars is about ___ percent as dense as Earth's.
|
1
|
|
Mars' atmosphere is made of:
|
95% Carbon Dioxide
A few percent of nitrogen and argon. |
|
The atmospheric pressure of Mars is too low for _____ to exist.
|
liquid water
|
|
The oxygen in Mars' atmosphere has reacted with iron in the crust to produce ______.
|
iron oxide (rust)
|
|
Largest Volcano is on Mars. What is it's name and approximate size?
|
Olympus Mons
Size of Arizona |
|
Tharsis Rise
|
large "hot spot" volcanoes
|
|
Valles Marineris
|
Rift Valley that would stretch across the entire United States
|
|
Ice caps on Mars' North and South poles change with the seasons and are made of:
|
frozen carbon dioxide on top of water ice.
|
|
Mars has two moons named:
|
Phobos and Deimos
|
|
Phobos and Deimos are ___ moons with ____ albedos.
|
small (probably captured asteroids)
low (less than 10%, very dark) |
|
Phobos' revolves around Mars in ____ time than it takes Mars to rotate ____.
|
less
once |
|
Phobos rises in the _____, and sets in the ______.
|
West
East |
|
Since Phobos is slowly nearing Mars, it will eventually:
|
crash into it.
|
|
Jupiter and Saturn are ____ planets.
|
Jovian
|
|
Jupiter is the ____ planet.
How many earth masses? |
largest
318 2.5 times mass of all planets combined. |
|
Saturn is the ______ planet.
How many earth masses? |
second largest
95 |
|
Jupiter and Saturn (have/do not have) a surface.
|
do not have
|
|
Jupiter and Saturn rotate in about ____ hours.
|
ten
very fast |
|
Cloud belts are ____.
|
dark
E to W wind flow |
|
Cloud zones are _____.
|
light
E to W wind flow |
|
Great Red Spot
|
giant low pressure "storm" on Jupiter
|
|
Jupiter and Saturn are not spherical, they are noticeably ______.
|
oblate
|
|
Oblate shape and rotation show that Jupiter and Saturn are made of _____.
|
fluids
|
|
Differential Rotation
|
equator moves faster than poles
(Jupiter and Saturn) |
|
Jupiter and Saturn are made mostly of:
|
hydrogen and helium
|
|
Liquid metallic hydrogen creates Jupiter's:
|
large magnetic field
|
|
Clouds of Jupiter and Saturn are made of:
|
Methane
Ammonia Water Carbon Monoxide Various hydrocarbons |
|
Jupiter and Saturn give of ____ energy than they get from the sun.
|
more
|
|
Jupiter has the ________ planetary magnetic field.
|
largest and strongest
|
|
Jupiter's magnetic field is produced by:
|
liquid metallic hydrogen
|
|
Decimeter Radiation
|
0.10 m wavelength
|
|
Decameter Radiation
|
10 m wavelength
|
|
Jupiter and Saturn's magenetic fields produce _____.
|
aurorae
|
|
Big moons are broken up by ________.
|
tidal forces
|
|
Jupiter and Saturn (have/have no) rings.
|
have
|
|
Cannot see Jupiter's rings from Earth because they are _____ and made of _________.
|
tiny
micron-sized dust |
|
Larger moons are found in the _______.
|
Roche Limit
|
|
Saturn's rings are _____ and _____ visible from Earth. They are made of _____.
|
large
easily small water ice particles |
|
Ringlets
|
about 1000 make up larger rings
|
|
F-Ring of Saturn
|
Shepherd Moons hold it in place. Inside moon puts energy in, outside moon takes energy out.
|
|
Jupiter's rings are _____ and _____ than Saturn's. Made of _____.
|
smaller
thinner water ice |
|
Saturn's rings are ____ in color than Jupiter's because they are made of _____.
|
darker
small bits of rock and dust |
|
Saturn gets about _____ as much sunlight as Earth.
|
1/100
Ices are common. |
|
Jupiter gets about ____ as much sunlight as Earth.
|
1/25
Ices are common. |
|
Galilean Moons (names)
|
Io
Europa Ganymede Callisto |
|
Rocky Galilean Moons
|
Io
Europa |
|
Icy Galilean Moons
|
Ganymede
Callisto |
|
Callisto
|
heavily cratered
old surface surface is mostly water ice surface is very dark (low albedo) |
|
Ganymede
|
largest moon in the solar system
|
|
Europa
|
surface is bright white
new surface very few craters presumably the water ice is redone by liquid water |
|
How is Europa's water ice redone?
|
The water ice is redone by liquid water. Tidal forces due to resonance effect and friction produces heat.
|
|
Io
|
No craters
Has many active volcanoes Produce many compunds of sulfur Color is yellow, red, and black Most geologically active place in the solar system |
|
Sulfur on Io does what?
|
conducts current and makes decameter radiation
|
|
Io is the most geologically active place in the solar system because of:
|
heat produced by tidal effects
|
|
Saturn's largest moon:
|
Titan
|
|
Titan
|
has substantial atmosphere
85% Nitrogen Ammonnia Organic "smog" covers it Density is about 1.5 times Earth's atmosphere |
|
Titan can retain an atmopshere because:
|
the surface is cold
|
|
Uranus and Neptune are _____ planets.
|
Jovian
|
|
Uranus and Neptune's solar winds are in _____ and _____.
|
belts
zones |
|
Uranus is essentially tipped on it's _____, so seasons are _____.
|
side
extreme |
|
Uranus and Neptune are blue colored due to:
|
methane absorbing red light
|
|
Neptune was the first _____ planet discovered.
|
predicted
|
|
Uranus' magnetic field is:
|
shifted off to the side in the mantle
|
|
The source of Uranus' magenetic field is:
|
liquid water mantle with dissolved ammonia and methane
|
|
Uranus' rings are:
|
pieces of frozen methane
|
|
Uranus has a ____ surface.
|
dark
|
|
Uranus' dark surface is from:
|
carbon produced by UV light interacting with methane.
|
|
Occultation
|
planet and rings cover up stars
|
|
Neptune's rings are ___ shaped.
|
arc
Don't go all the way around. |
|
Moons of Neptune (names)
|
Triton
Nereid |
|
Triton
|
Retrograde Rotation
Has a thin nitrogen atmosphere. Is moving toward Neptune. |
|
Triton is similar to _____.
|
Pluto
|
|
Nereid's orbit is:
|
extremely elliptical.
|
|
Pluto was discovered ______.
|
accidentally in 1930.
|
|
Pluto's moons:
|
Charon
+ two more tiny moons Made of methane ice |
|
Asteroid belt is found:
|
between Mars and Jupiter
|
|
Largest asteroid
|
Ceres
|
|
_______ gaps show effects of Jupiter through resonances.
|
Kirkwood
|
|
Asteroids are similar in composition to _______ planets.
|
terrestrial
|
|
Asteroids are ______ left over from the formation of the solar system.
|
planetesimals
|
|
Asteroids ______ frequently.
|
collide
|
|
Asteroid Classes
|
S-type
M-type C-type |
|
S-type Asteroids
|
"stony"; made from silicate rocks
|
|
M-type Asteroids
|
"metal"; made from iron and nickel
|
|
C-type Asteroids
|
"carbon"; have a large concentration of carbon
|
|
Leftovers from the outer solar system make up the _______ belt and ______ cloud.
|
Kuiper
Oort |
|
Kuiper Belt is approximately in the plane of the Solar System in orbits just outside _______.
|
Neptune
|
|
Oort Cloud is a ________ distribution located thousands of AU from the sun.
|
spherical
|
|
Two types of comet tails
|
Ion Tail
Dust Tail |
|
Comet tails always point _____ the sun.
|
away from
|
|
Comet dust tails are pushed back by ______.
|
light pressure
|
|
Comet ion tails are pushed back by _____.
|
solar wind
|
|
Body of comet is called ____.
|
coma
|
|
Dust particles from comets produce:
|
meteor showers
|
|
Meteoroid
|
small body still in space that's approaching the Earth
|
|
Meteor
|
an object vaporizing in the Earth's atmosphere (dust from comets)
|
|
Meteorite
|
meteor that lands on earth (come from asteroids)
|
|
Easiest to find meteorites in:
|
Antarctica
|
|
Meteorite "finds"
|
didn't see it fall
|
|
Meteorite "falls"
|
did see it fall
|
|
Iron Meteorites:
|
cooled from a molten state very slowly, a few degrees every million years
|
|
Most meteorite "finds" are:
|
Iron meteorites
|
|
Most meteorite "falls" are:
|
Stony meteorites
|
|
Two types of stony meteorites:
|
Chondrites
Achondrites |
|
Carbonaceous Condrites
|
similar to carbon asteroids
have not been heated - come from a cold part of the solar system still have volatile compounds |
|
Achondrites
|
heated
lava |
|
Widmanstatten Pattern
|
crosshatch pattern found in iron meteroites
due to slow cooling process |