Test Flashcards

(37 cards)

1
Q

what are the atmospheres of the terrestrial planets like?

A
  • made of rocky substances
  • metallic core composed of mostly iron with a surrounding silicate mantle (mercury venus earth mars)
  • have common surface features like canyons, creaters, mountains, volcanoes
  • have secondary atmospheres which are gnereated through volcano or comet impact
  • more dense than jovian
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2
Q

where did the water for earths oceans come from

A

-water came from comets and icy objects bombarding the earth

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3
Q

why dont venus and mars have oceans

A
  • mars is too cold, low temperatures water wouldnt be stable in liquid phase
  • venus is too hot to sustain water
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4
Q

how do the jovian planets differ from earth? why are they so different?

A
  • made of gas
  • jupiter and saturn contain almost entirely hydrogen and helium
  • different because of formation of solar system: formed behind frost line where hydrogen could condense into ice - formed farther from sun
  • jovian planerts are larger than earth & terrestrial planets - less dense
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5
Q

how do we know that earth formed from the accretion of smaller rocky objects

A
  • craters on earths surface
  • iron meteorite and stony meteorite
  • moon and mercury show evidence through meteorites
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6
Q

where are most comets located? how do we explain the origin of comets

A
  • comets are located in the oort cloud - 10,000x farther away from sun then earth
  • they originate from the oort cloud and Kupier belt
  • oort cloud - has icy bodies and a star can pull one out letting it fall to earth as a comet
  • kupier belt - composed of icy bodies (short period comets)
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7
Q

why is the solar system flat?

A
  • based on current obsevations, we can see solar systems beyond our own
  • the solar system is flat because of angular momentum
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8
Q

what is the nebular hypothesis?

A
  • the nebular hypothesis ocurred when the gravity contracted the solar nebula na dmost of the material collected in the center to from the protosun
  • remaining materials formed a thick, flattened, rotating disk within which matter gradually cooled and condensed into grain of clumps and icy, rocky material
  • repeated collisions resulted in the material clumping together into planets
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9
Q

what seven wanderers did the ancient greek astronomers identify in geocentrism

A
  • moon
  • mercury
  • venus
  • sun
  • mars
  • jupiter
  • saturn
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10
Q

what did the Ptolemaic (geocentric) model include and why ?

A
  • earth was the center of the solar system - motionless
  • believed all celestial objects orbited erath
  • assumed each planet moved on a small sphere of circle called an epicycle
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11
Q

what discover made by galileo led to the downfall of geo-centrism? why?

A
  • the discovery of the phases of venus
  • ptolemaic system argues that the crescent phases of venus should never be seen from earth
  • we are able to see phases, therefore copernican view of sun centered universe is more accurate
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12
Q

what is retrograde motion?

A
  • the westward motion of planets. Since Earth moves much faster than the other planets, the slower moving planets appear as if theyre going in reverse
  • earth moves faster than mars so when it passes mars it looks like mars is moving backwards
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13
Q

How was retrograde motion explained in both the Ptolemaic (geocentric) and Copernican (heliocentric) models?

A
  • geocentric: used epicycles to explain the retrograde motion - the center of the epicycle moves in large circl called a deferent
  • heliocentric: planets further from sun move more slowly. As earth laps mars, mars appears to go bakcward as seen by observer on earth
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14
Q

what is keplers three laws of planetary motion?

A

a. Elliptical orbits (all planets move about sun in elliptical orbits) - planets are sometimes closer to sun and go fast. further away and go slow
b. equal areas in equal times - describes the speed of a planet traveling in an elliptical orbit around the sun. Line between sun and planet sweeps equal areas in equal times
c. period squared = distance cubed - planets in solar sytem have no linear relationship between planets orbit and distance around sun

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15
Q

what discovery by newton verified keplers laws?

A

when he proposed the law of univeral gravitation. Gravitational force was the cause of Kepler’s laws

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16
Q

what are the phases of the moon? Is the moon ever visible during the day? Start with new moon

A

New moon: The moon is between sun and earth - back lit
waxing crescent: sunlit portion is increasing but still less than half (right side lit)
first quarter: half of the moon is lit. right side
waxing gibbous: more than half is lit (left side is unlit)
full moon: earth sun and moon are in approximate alignment - entire sunlit part is facing us
waning gibbous: light decreases, more than half lit (right side unlit
third quarter: half moon is lit - left side is lit
waning crescent: more is dark lit, only part of left side is lit

  • the moon can be seen during the day when it is in New moon as it moves away from the sun
17
Q

what are the differences between the crescent moon visible after sunset and the one visible before sunrise?

A

After sunset: moon appears very low in western sky, has low surface brightness, ddrawn curved to the right
before sunrise: points eastward - drawn curved to the left

18
Q

what is the connection between lunar phases? why don’t eclipses happen every month?

A
  • solar eclipses only happen when moon is in new moon phase: plane of moons orbit is aligned with earth’s orbit around sun - only happens once or twice a year
  • lunar eclipses only occur when moon in in full phase - planes have to align
  • They dont happen every month because the moon does not orbit in the same plane as earths orbital plane
  • more likely to see lunar eclipse
19
Q

what do we know about the suns visible surface and outer atmosphere & how do we know it

A

outer atmosphere: photosphere, chromosphere, and corone
Photosphere: very active, gives off visible light strongly, has sunspotss which emerge when suns magentic field breaks through the surface
Chromosphere: emits a reddish glow as hydrogen burns off. Plays a role in heat from interior to corona
Corona: thrid layer of suns atmosphere. hotter than photosphere. only visible during a solar eclipse.

-studied through solar exlipses and satellite devices

20
Q

what do we know about the suns interior and how do we know it

A

-suns interior is opaque
-core: pure helium
-radiation zone: hydrogen
Convection zone: doesnt transmit light
-observed throug hhelioseismology which studies suns movement/swinging. these movements are caused by sound waves

21
Q

how big is the sun and how does it compare to other stars

A
  • the suns circumference is about 2,700,000 miles - you could line up 109 earths across the face of the sun
  • suns diameter is 100 times wider than earth, gaseous, not very dense
  • stars are 700 times bigger than our sun - our sun is ver y average
22
Q

what are the two most abundant chemical elements in the sun? How are they related to the source of the suns energy

A

-hyrdogen and helium - hydrogen nuclei crash together and form helium in nuclear fusion - releases gamma waves which turn into visible light

23
Q

what are the seven regions of the electromagnetic spectrum? what are their similarities and differences

A

highest energy - lowest (shortest - longest wavelength)

a. gamma rays
b. x ray
c. ultraviolet
d. visible
e. infared
f. microwave
g. radio wave

24
Q

why are radio telescopes placed in desert valleys? why are optical telescopes placed on mountain tops? why are some telescopes put into orbit?

A

Desert valleys: humans dont emit radio waves in deserts & can get away from human interference, possible to do day or night
Mountain tops: less atmosphere pollution, easier to see, less light interference from cities
orbital telescopes: study visible light from space and ultraviolet telescopes study very hot stars, these lights can only be studied from space bc theyre . blocked from our atmosphere

25
why do some stars appear reddish, and others blue white in color?
- the coolest stars appear red (long wavelength, high energy) - hotter stars become blue (short wavelength, low energy)
26
what is a bright line spectrum? why does it contain only a few specific colors?
- sample of low pressure gas, heat excites it and emits photons, gas glows at color corresponding with electrons coming down from excited state - carbon glows magenta - chemical fingerprint
27
what is a dark line spectrum? what can be learned about a star from studying it?
- a pattern of light produced by continous spectrum through cool gas - some light filtered out - violet (high energy) - can learn about a stars total energy output, surface temp, radius, chemical composition, rotation period
28
how is the doppler effect used in astronomy?
- used to tell if objects are coming towards or away from us - waves get shorter when star approaches - blue light - waves get longer when leaving (more spread out) - red light
29
how do massive stars end their lives? what does this have to do with earths composition?
- stars end their life by collapsing on themselves. When all the nuclear fuel in a star is used up, gravity will win over pressure and the star will die. - high mass stars die first, in a gigantic explosion called the supernova. Supernova explosion brought about nuclear fusion in core which produces iron, iron forms causing a collapse - iron in core shown by spectroscopy
30
where do you fin the empty spaces in the structures of our universe? th
between galaxies and stars, and enormous empty space between the electron's atoms
31
how big is the solar system? what is an astronomical unit?
the solar system is 100 AU across which is equal to 93 million miles. An astronomical unit is a convenient yard stick for measuring things in space
32
The sun is a star. how far away are the next nearest stars? What is a light year?
the next nearest stars are 4.3 light years away. (nearest star is proxima centauri). A light year is the measure of distance at which light travels. One light year is 6 trillion miles.
33
what is the average distance between stars?
10 light years
34
What are the properties of the milky way? what holds it together?
- is is a spiral galaxy -it is made of dust, stars, gas, and dark matter - their is a dark hole held together by gravity in the center consists of 200 billion stars -it is 75, 000 light years across - its overall shape is a disk
35
how far apart are the galaxies?
the galaxies are 3 million light years apart
36
how do we know the universe is expanding?
- hubble found that almost all galaxies are moving away from us through recession velocity - we know the universe is expanding because of the doppler effect. when things are moving away, shifts to red spectrum. red shift was moving faster at farther away galaxies.
37
describe the origin of the universe. what evidence do we have of this
- the origin of the universe started when the earth was a hot dense state and began to expand and cool becoming less dense. Everything we can see was only energy and was seen through gamma waves. - evidence of this is cosmic background radiation. radiation from very early phase of unidverse should still be detectable today. saw microwaves instead of gamma bc its extremely red shifted