Brainscape's Knowledge GenomeTM

Browse over 1 million classes created by top students, professors, publishers, and experts.


See full index

Astronomy Pt. 1 > chapter 12 (pt. 1), 13 & 14 > Flashcards

chapter 12 (pt. 1), 13 & 14 Flashcards

evidence for planet/star common origin comparative planetology of metallic/rock planets liquid-gas giant planets of the outer solar system

1
Q

Earth

A

home, third rock from the Sun, water planet, thin atmosphere altered by life, large terrestrial
[mantle, plate tectonics, primary atmosphere, secondary atmosphere, greenhouse effect]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Moon

A

a planet-like companion to Earth made of the Earth’s ocean crust
[albedo, anorthosite, breccia, ejecta, maria, micrometeorite, large-impact hypothesis, magma ocean, multiringed basins, late heavy bombardment]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Mercury

A

a metal planet, cooling and shrinking against the cold of space, smallest planet in solar system
[fast, very dense, inactive]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Venus

A

initially a water planet, clouding over and heating which boiled off its water so its now dry
[runaway greenhouse effect, coronae]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Mars

A

small water planet unable to hold its atmosphere which boiled away water making a cold desert
[shield volcano, outflow channel, valley network, permafrost, moons]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Jupiter

A

massive, largest planet in solar system, ball of liquid metallic hydrogen, extensive moon system, sidereal rotation period 10 hours, spins the fastest of all planets
[oblate, liquid metallic hydrogen, magnetosphere, belt-zone circulation, forward scattering, Roche limit, tidal heating]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Saturn

A

massive, visibly bright ice-particle ring, ball of liquid metallic hydrogen, extensive moon system
[ring system, shepherd satellite, gap, Titan, liquid methane/ethane, Enceladus, tiger stripe]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Uranus

A

ice giant, rich in solid and liquid water, rotation inclined to ecliptic about 98º
[trace methane, occulation, moon with ovoids]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Neptune

A

ice giant, rich in solid and liquid water, rings NOT easily detactable from Earth, satellite system, 2 discovered from Earth, 6 by Voyager 2 (1989),
Great Dark Spot (dark blue) roughly the size of Earth, circulating hurricane

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Plutino, Pluto

A

a dwarf planet (IAU defines ‘planet’ as gravitationally spherical, dominate orbit, bound to star)
[dwarf planet]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Terrestrial planets

A

Earth-like, small diameter, dense (of rock or metal), rocky, little or no atmosphere
[crater, asteroid, meteoroid (meteor, meteorite), meteor shower, carbonaceous chondrite, volatile, half-life]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Jovian Planets

A

“liquid” giants (compressed gas), worlds of the outer solar system (resemble Jupiter)
[comet, Kuiper Belt, Oort Cloud]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

solar nebula theory

A

rotating cloud of gas/dust gravitationally collapse and flatten, around forming Sun disk rotates counter clockwise, all planets revolve in the same direction, rotate as well
[uncompressed density, ice line, condensation, condensation sequence, accretion, planetesimal, protoplanet, gravitational collapse, heat of formation, differentiation, outgassing, Late Heavy Bombardment, Near Earth Objects (NEO)]

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

evolutionary theory

A

phenomenon involving slow, steady, process of sort seen happening present day

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

catastrophic theory

A

phenomenon involving special, sudden, perhaps violent events

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

comparative planetology

A

comparison of one planet with another, Earth as the template

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

active core (Earth)

A

refers to geologically mobile, as heat stirs and makes its way out of the interior

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

mantle (Earth)

A

deep layer - Earth’s dense rock, properties of solid but capable of flowing slowly (like asphalt)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

crust (Earth)

A

rocky low-density surface, radiates heat out into space

smooth surface is younger (lava flow) than cratered area (Late Heavy Bombardment)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

plate tectonics (Earth)

A

crust plates floating on mantle (Greek for “builder”)

100s M.y. movement (0.1 G.y.) 1/45 age of Earth, so sections of crust in rapid motion

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

atmosphere (Earth)

A

larger size and cooler temperature of planet important to retaining gases
gases originate from formation, space deliveries, evolution of the planet, appearance of life

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

primary atmosphere (Earth)

A

planet’s first atmosphere, gases from solar system nebula (hydrogen, methane) outgassing of carbon dioxide, nitrogen, water vapour, etc., cooked-out of hot planet rock
accreting planetesimals rich volatile materials (water, ammonia, carbon dioxide, etc.)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

secondary atmosphere (Earth)

A

replaces the primary atmosphere, e.g., outgassing, impactors, bioactivity
Earth’s relatively thin, mainly nitrogen, significant oxygen from biologucal processes

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

greenhouse effect (Earth)

A 
carbon dioxide (CO2) rich atmosphere traps heat and raises planet surface temp.
visible wavelength sunlight shines through glass roof of greenhouse, heats interior without greenhouse effect Earth would be 30ºC cooler, average temp. below freezing
human action that add CO2, water, and gases, being researched for forcing of current climate
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
Q

global warming (Earth)

A

gradual increase in surface temperature of Earth caused by human modifications, a concept no longer used by science which claims to link all climate change directly to human action

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
26
Q

surface evolution (Earth)

A

report of changes that destroys traces of earlier formation processes

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
27
Q

albedo (Moon)

A

ratio of the amount of light reflected from an object to the amount received
perfectly black = 0, perfectly white (full reflection) = 1
Moon albedo is not that high (0.06) only reflects about 6% of light that hits it, a dark grey world

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
28
Q

anorthosite (Moon)

A

light coloured, aliminum and calcium-rich silicate rock, first solidified, float to top
most rock is hardened lava and breccia (fragments of older broken bound together)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
29
Q

maria (mare, Latin “seas) (Moon)

A

smooth lunar lowlands of successive flows of dark lava

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
30
Q

micrometeorites (Moon)

A

meteorites of microscopic size

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
31
Q

large impact hypothesis (Moon)

A

1970s, Moon formed when Mars size planetesimal smashed into Earth

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
32
Q

magma ocean exterior (Moon)

A

newborn Moon, shell of molten rock hundreds of km thick

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
33
Q

late heavy bombardment (Moon)

A

impacts from possible final accretion and migration of Uranus and Neptune

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
34
Q

multiringed basin (Moon)

A

large impact feature, +/- 2 concentric rims, fracture of planet crust, 100skm diameter

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
35
Q

fast (Mercury)

A

orbital period of 88 days

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
36
Q

very dense (Mercury)

A

sugggests a large metallic core about 70% of planet radius (metal planet, thin rock mantle)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
37
Q

inactive (Mercury)

A

due to lost internal heat, core contracted, crust compressed and broke in long shrink ridges

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
38
Q

runaway greenhouse effect (Venus)

A

greenhouse effect so dramatic it amplifies itself

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
39
Q

hot (Venus)

A

the surface can melt lead
it is corrosive and has great pressure
no spacesuit is protective

40
Q

coronae (Venus)

A

large round geological faults in the crust caused by intrusion of magma below the crust

41
Q

iron oxide (Mars)

A

reddish orange mineral caused by oxidation of iron in the presence of free O2 molecules

42
Q

outflow channels (Mars)

A

geological surface feature flow of vast amount of water released suddenly

43
Q

valley networks (Mars)

A

system of drainage channels, resemble beds of rivers and tributary systems on Earth but some water may still be present at permafrost

44
Q

permafrost (Mars)

A

permanently frozen soil that seasonally thaws

45
Q

satellite system [moons] (Mars)

A

very tiny so cold, irregular (potato) in shape, likely captured asteroids

46
Q

oblateness (Jupiter)

A

flattening of spherical body caused by rotation, fraction equatorial diameter exceeds polar

47
Q

heavy element core (Jupiter)

A

“rocky core” refers to chemical composition (iron, nickel,silicon, …), NOT properties this matter 4x hotter than the surface of the Sun, pressure 50 million times Earth’s at sea level

48
Q

liquid metallic hydrogen (Jupiter)

A

liquid hydrogen under very high pressure, good conductor electricity stirred by convection currents and spun by planet’s rapid rotation drives dynamo effect

49
Q

magnetosphere (Jupiter)

A

magnetic field volume of space around planet, traps solar wind charged particles

50
Q

aurora (Jupiter)

A

charged solar particles follow polar magnetic fields, imaged by UV for Jupiter

51
Q

belt-zone circulation (Jupiter)

A

cloud belts and zones form stripes that circle the planet parallel to equator ammonia (NH3), ammonia hydrosulphide (NH4SH), water (H2O) can condense into droplets
belt - darker descending gas lower in atmosphere
zone - brighter, rising gas cloud high in atmosphere, reflects stronger sunlight near surface to viewer embedded circulating storms

52
Q

forward scattering (Jupiter)

A

optical property, finely divided particles, direct light in direction light is traveling
diameters approximately equal to wavelength of visible light, cigarette smoke size within Roche limit

53
Q

Roche limit (Jupiter)

A

minimum distance planet to a satellite that can hold itself together by own gravity
satellite within Roche limit is pulled apart by tidal forces (where raw material cannot coalesce)
about 2.4x the planets radius, depending somewhat on the relative densities of planet and moon

54
Q

tidal heating (Jupiter)

A

heating of a planet or a satellite because of internal friction due to (gravitational) tides

55
Q

satellite system (Jupiter)

A

4 large Galilean moons
related to eachother and probably formed with Jupiter
[Io, Europa]

56
Q

Io

A

slightly larger than Earth’s moon (looks like a pizza)
density 3.6g/cm^3, rock and metal
intense warming (tidal heating) could have driven off much internal ice

57
Q

Europa

A

slightly smaller than Earth’s moon (looks like cracked ice ball) density 3g/cm^3, mostly rock with thin ice crust, visible surface very clean, few craters, long cracks

  • geologically active crust breaks as moon is flexed by gravitational tides from Jupiter and other moons
  • liquid water ocean 20km deep suggested by the gravitational influence on Galileo spacecraft
58
Q

ring system (Saturn)

A 
multiple rings (e.g., Saturn's three main rings, A, B, C)
golf ball size chunks of ice mainly, sometimes rock, down to dust from broken satellites and geysers
59
Q

shepherd satallite (Saturn)

A

body that confine rings, gravitationally usher stray particles back into the rings

60
Q

gap (Saturn)

A

space in rings that is not empty, small moon orbits inside

61
Q

Titan (Saturn)

A

the largest moon of Saturn (bit larger than Mercury), surface fluid circulation system and erosion

62
Q

liquid methane/ethane (Saturn)

A

hydrocarbon at very cold temperatures (180ºC)

63
Q

Enceladus (Saturn)

A

moon of Saturn, signs of recent geological activity, some parts 1000 fewer craters

64
Q

tiger stripe (Saturn)

A

tidal force fissure or crustal crack where liquid water erupts as geyser

65
Q

trace methane (Uranus)

A

small quantity causes a teal, or green-blue, or green colour in planetary atmosphere
rings NOT easily detectable from Earth, dark, faint, contain little dust, confined by shepherd satellites

66
Q

occulations (Uranus)

A

passage of a larger body in front of a smaller one, planet in front of a star

67
Q

Miranda (Uranus)

A

innermost moon of the 5, 14% the diameter of Moon

68
Q

Ovoid (Uranus)

A

surface marks groves, oval features may have been caused by internal heat, convection

69
Q

dwarf planet (Pluto/Plutino)

A

body orbiting Sun, not satellite of planet, round but not massive enough to clear its orbit

70
Q

Plutino

A

one of the icy Kuiper belt objects caught in a 3:2 orbital resonance with Neptune (like Pluto)

71
Q

crater (Terrestrial planet)

A

impact size, nearly every firm surface in the solar system peppered by meteorite impacts

72
Q

asteroids (Terrestrial planet)

A

small rocky world, most orbit the Sub between Mars and Jupiter in the Asteroid Belt

73
Q

meteoroid (Terrestrial planet)

A

small bit of matter (dust, sand, pebble, most less than 1 gram) in space

74
Q

meteor (Terrestrial planet)

A

meteoroid falling into Earth’s atmosphere, friction heats it/surface into incandescent vapour

75
Q

meteorite (Terrestrial planet)

A

meteor large enough that a portion survives fall through atmosphere, strikes ground

76
Q

carbonaceous chondrite (Terrestrial planet)

A

contains small glassy spheres called chondrules and volatiles

77
Q

volatile (Terrestrial planet)

A

easily vaporized compounds, carbon dioxide, carbon monoxide, methane, ammonia

78
Q

meteor shower (Terrestrial planet)

A

meteor display appear to originate from one region of the night sky, cometary debris

79
Q

half-life (Terrestrial planet)

A

time required for half of radioactive atoms in a sample to decay

80
Q

Comet (Jovian planet)

A

small ice body orbit the Sun, produce tails of gas and dust when they approach the Sun (tail always points away from the Sun)

81
Q

Kuiper belt (Jovian planet)

A

collection of icy planetesimals orbiting just beyond Neptune to +50 AU, ~1000 discovered

82
Q

Oort Cloud (Jovian planet)

A

hypothetical source of distant comets, icy bodies, spherical shell to 100000 AU from Sun

83
Q

uncompressed density

A

density a planet would have if its gravity were not compressing it

84
Q

ice line

A

boundary beyond which water vapour could freeze to form ice grains

85
Q

condensation

A

growth of a particle by addition of material from surrounding gas, atom by atom

86
Q

condensation sequence

A

distance from proto-Sun that different materials condense in the solar nebula

87
Q

accretion

A

sticking together of solid particles to produce larger particle (e.g., snowflakes stuck together)

88
Q

planetesimals

A

small body formed of dust grains (not gas) in the solar nebula, eventually protoplanet

89
Q

protoplanet

A

coalescence of planetesimals in solar nebula, massive object, destined to become planet

90
Q

gravitaional collapse

A

forming body, gravitationally captures gas rapidly from the nebula

91
Q

heat of formation (in planetology)

A

heat released by infalling matter during planet body formation

92
Q

differentiation

A

melting of most of a planet permitting separation of material according to density

93
Q

outgassing

A

release of gasses from a planet’s interior (seen in modern-day volcanoes)

94
Q

impact

A

meteor or comet body that reaches the surface of another Solar System object, usually violent

95
Q

late heavy bombardment

A

crater evidence intense comet and asteroid hits in first 0.5by of solar system

96
Q

near Earth objects (NEOs)

A

small solar system body (comet, asteroid) orbit that poses threat, collision

Astronomy Pt. 1 (11 decks)

Brainscape helps you reach your goals faster, through stronger study habits.
© 2025 Bold Learning Solutions. Terms and Conditions