Astronomy Homework for Exam 2 – Flashcards
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the 8000 K star would emits more light at every wavelength and would emit photons with a higher energy
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describe 2 ways in which the thermal radiation spectrum of an 8000 K star would differ from a 4000 K star ???
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Doppler Effect
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the effect that shifts the wavelengths of spectral features in objects that are moving toward or away from the observer
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blue shifts
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shorter wavelengths. object is moving towards us
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light-collecting area and angular resolution
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two key properties of a telescope
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light-collecting area
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determines how much total light a telescope can collect at one time
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angular resolution
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the amount of detail a telescope allows us to see. best when it's small
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refracting telescope
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operates similar to the eye, using transparent lenses to collect and focus light. lenses
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reflecting telescope
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uses a precisely curved primary mirror to gather light, which reflects the gathered light to a secondary mirror that lies in front of it
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1. light pollution 2. turbulence causes twinkling 3. absorbs most of EM spectrum, including all UV and X-Ray and most infrared
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3 ways Earth's atmosphere hinders astronomical observations
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4 times
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how much greater is the light-collecting area of a 6-meter telescope than that of a 3-meter telescope?
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(I think) cooler than the Sun
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a star whose spectrum peaks in the infrared is...
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redshifted
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A spectral line that appears at a wavelength of 321 nm in the laboratory appears at a wavelength of 328 nm in the spectrum of a distant object. We say that the object's spectrum...
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(Sun) Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune (Pluto)
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order of the planets
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Sun
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contains more than 99.8% of the solar system's total mass. looks like the surface is solid, but is actually a roiling sea of hot hydrogen and helium gas
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Mercury
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made up of metal and rock. smallest of the 8 planets. days and nights here last for 3 months each. very hot and very cold
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Venus
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hottest planet in the Solar System. spins backwards on its axis. nearly identical to Earth in size
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temperature
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measuring a star's color tells us about its...
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Earth
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an oasis to life. surprisingly large moon. The only surface liquid water in the solar system
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Mars
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looks Earth-like. giant volcanoes, huge canyon, and polar caps. water flowed here in the distant past
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Jupiter
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much farther from Sun than inner planets, most H/He, no solid surface, 300 times bigger than Earth, many moons and rings
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Saturn
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Giant. mostly H and He, spectacular rings. many moons
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countless small chunks of ice and rock, each orbiting like a tiny moon. NOT SOLID
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what are Saturn's rings made out of?
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Uranus
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smaller than Jupiter and Saturn, bigger than Earth. made of H/He gas and hydrogen compounds. extreme axis tilt. moons and rings
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Neptune
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similar to Uranus (except for axis tilt). many moons
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Pluto
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much smaller than other planets. icy, comet-like composition. it's moon is similar in size to itself
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true
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(T/F) most of the solar system's planets revolve around the Sun in the same direction and rotate in the same direction as they orbit the Sun
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Mercury, Venus, Earth, and Mars
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which planets have a rocky, relatively dense composition (terrestrial)?
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Jupiter, Saturn, Uranus, and Neptune
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which planets have rings?
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patterns of motion, 2 major types of planets, asteroids and comets, exceptions to the rule
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what are the 4 major features of the solar system that provide clues to how it formed?
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patterns of motion among large bodies (feature 1 of how the solar system formed)
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the Sun, planets, and large moons generally orbit and rotate in a very organized way
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two major types of planets (feature 2 of how the solar system formed)
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the 8 planets divide clearly into 2 groups: small rocky planets that are close together and to the Sun, and the large gas-rich planets that are father apart and from the Sun
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asteroids and comets (feature 3 of how the solar system formed)
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vast numbers of these orbit the sun. the locations, orbits, and compositions of these follow a distinct pattern
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exceptions to the rule (feature 4 of how the solar system formed)
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among the inner planets only Earth has a large moon, and Uranus is tipped on its side
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terrestrial planets
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"Earth-like". Small, rocky/metal composition, closely spaced, no moons
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Jovian planets
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"Jupiter-like". Giant, hydrogen/helium composition, widely spaced, rings, lots of moons
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Jupiter, Saturn, Uranus, Neptune
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which planets are jovian?
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nebular theory
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theory that states that our solar system formed from a giant cloud of interstellar gas
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nebula
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cloud
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asteroids
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rocky bodies that orbit the Sun like planets
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asteroid belt
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asteroids are found in this, between the orbits of Mars and Jupiter
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comets
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small objects that orbit the sun, but are made largely of ice
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solar nebula
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the particular cloud of gas from which our solar system was born
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the gas is about 98% hydrogen and helium and 2% all other elements combined
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what is the solar nebula made of?
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heating, spinning, and flattening
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what caused the solar nebula to take the form of a spinning disk?
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flattening
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collisions between particles in the cloud causes it to flatten into a disk
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heating
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the temperature of the solar nebula increased as it collapsed, which represents energy conservation
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spinning
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the solar nebula rotated faster and faster as it shrank in radius, which represents the conservation of angular momentum
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hydrogen and helium gas (98%), hydrogen compounds (1.4%), rock (0.4%), and metals (0.2%)
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what are the 4 materials in the solar nebula?
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frost line
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the boundary in the solar nebula between which ices could condense; only metals and rocks could condense within this
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rocks, metals, and hydrogen compounds
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which materials can be solid outside the frost line?
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the formation of terrestrial planets
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Small particles of rock and metal were present inside the frost line, Planetesimals of rock and metal built up as these particles collided. Gravity eventually assembled these planetesimals into these planets
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the formation of jovian planets
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Ice could also form small particles outside the frost line. Larger planetesimals and planets were able to form. The gravity of these larger planets was able to draw in surrounding H and He gases
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heavy bombardment
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the period in the first few hundred million years after the solar system formed during which the tail end of planetary accretion created most of the craters found on ancient planetary surfaces
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planetesimals
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pieces of planets
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radiometric dating
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the method by which we measure a rock's age. relies on careful measurement of the proportions of various atoms and isotopes in the rock
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half-life
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the length of time it would take for half the nuclei in the collection to decay
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accretion of planetesimals
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many smaller objects collected into just a few large ones
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inside the frost line
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where did asteroids come from?
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outside the frost line
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where did comets come from?
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TEMPERATURE
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why do we have 2 different kinds of planets in our Solar System?
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beyond Neptune's orbit, roughly in the plane of the ecliptic
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where are the Kuiper Belt comets found?
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an Oort Cloud comet
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which comet formed closest to the Sun?
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most
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how many planets orbit the Sun in the same direction as Earth does?
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fairly circular and in the same plane
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Planetary orbits in our solar system are...
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hydrogen and helium
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what is Jupiter's main ingredient?
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collapse, condensation, accretion
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list the major steps of solar system formation in the correct order
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accretion
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the process by which small "seeds" grew into planets
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comets
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leftover ice-rich plantesimals are called:
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it's surprisingly large relative to the planet it orbits
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what's unusual about our Moon?
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Venus and Uranus are exceptions (I'm pretty sure)
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are there any exceptions to the rule that planets rotate with small axis tilts and in the same direction as they orbit the Sun?
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4.5 billion years
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how old is the solar system?
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true
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(T/F) Venus has the hottest surface temperature of any planet in our solar system
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false
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(T/F) Our Moon is about the same size as moons of the other terrestrial planets
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true
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(T/F) the weather conditions on Mars today are much different than they were in the distant past
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false (I assume)
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(T/F) moons cannot have atmospheres, active volcanoes, or liquid water
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false (I think)
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(T/F) Neptune orbits the Sun in the opposite direction of all the other planets
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probably false
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(T/F) If Pluto were as large as the planet Mercury, we would classify it as a terrestrial planet
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I think it's true
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(T/F) Asteroids are made of essentially the same materials as a terrestrial planet
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Kuiper Belt
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comets formed about where they are and they're still there
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Oort Cloud
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comets formed along the present-day jovian planets and were thrown out by gravitational encounters
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core
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part of Earth's interior that has highest density; nickel and iron
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mantle
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part of Earth's interior that has moderate density, silicon, oxygen, etc.
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crust
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part of Earth's interior that has the lowest density, granite, basalt, etc.
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lithosphere
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crust and RIGID part of mantle
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differentiation
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the process by which gravity separates materials according to density, with high-density materials sinking and low-density materials rising
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dense metals sank toward the center, driving less dense rocky material toward the surface
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why did the terrestrial worlds undergo differentiation?
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magnetic field
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the region surrounding a magnet in which it can affect other magnets or charged particles
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magnetosphere
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the region surrounding a planet in which charged particles are trapped by the planet's magnetic field
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impact craters
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these are created by asteroids or comets striking a planet's surface
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volcanism
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the eruption of molten rock (lava) from a planet's interior onto its surface
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tectonics
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the disruption of a planet's surface by internal stress
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erosion
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the wearing down or building up of geological features by wind, water, ice, and other phenomena of planetary weather
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outgassing
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the process of releasing gases from a planetary interior, usually through volcanic eruptions
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most of the outgassed water vapor condensed to form our oceans and much of the nitrogen remains as the dominant ingredient of our atmosphere
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how did outgassing lead to the existence of Earth's atmosphere and oceans?
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radioactive decay
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which heat source continues to contribute to Earth's internal heat?
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a small planet
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what kind of terrestrial planet would you expect to have the thickest lithosphere?
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Jovian planets would have formed closer to the Sun
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How would the solar system be different if the solar nebula had cooled everywhere with a temperature half its current value?
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there are 4 terrestrial and 4 jovian planets
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what is not explained by the nebular theory?
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metals, rocks, hydrogen compounds
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list the ingredients of the solar nebula in order of increasing abundance. (except H and He gases)
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The inner nebula was so hot that only metals and rocks were able to condense
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Why do we think the inner (terrestrial) planets became more dense than the outer planets?
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zero
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What age would radiometric dating give for a chunk of recently solidified lava from Kilauea, an active volcano in Hawaii?
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1/4 (2 half-lives)
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After two half-lives, what fraction of the original radioactive element is left?
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4.4 billion years old
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how old are the oldest moon rocks?
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4.55 billion years old
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how old are the oldest meteorites?
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4.5 billion years ago
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when did planets form?
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It must be a mix of materials of different density and material inside must be able to flow
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What is necessary for differentiation to occur in a planet?
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Yes, rock under strain may slowly deform
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do rocks stretch?
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no
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is the Earth full of lava?
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No. Planetary magnetic fields are generated by moving charges around, and if the core is cold, nothing is moving.
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If the planet core is cold, do you expect it to have magnetic fields?
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if a planet has a lot of craters, it must mean the surface has stayed untouched since the bombardment 4 billion years ago, which means it is really old
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how do craters tell us the age of a surface?
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the Moon's surface has remained untouched since the bombardment 4 billion years ago. Earth has a surface that has undergone recent change
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Explain why the Moon has more craters than Earth
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it supplies oxygen to breathe, it protects the surface from dangerous solar radiation, and makes our planet warm enough for liquid water to exist
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how does the atmosphere affect Earth?
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greenhouse effect
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Certain molecules let sunlight through but trap escaping infrared photon
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water vapor (H2O), carbon dioxide (CO2), and methane (CH4)
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what are the greenhouse gases
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greenhouse gas (NOT O2 OR N2)
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molecules with 2 or more different types of elements
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the Moon and Mercury
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which 2 planets are "geologically dead"?
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both lost their internal heat long ago, their gravity is too weak to hold gas they may have gained in the past, don't have significant atmospheres, have lots of impact craters
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describe the geological histories of the Moon and Mercury
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lunar maria
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the regions of the Moon that look smooth from Earth and actually are impact basins
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they probably formed when tectonic forces compressed the crust, causing the surface to crumple. Mercury shrank
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how are Mercury's great cliffs thought to have formed?
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one with lots of impact craters
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which kind of surface is probably older in our Solar System?
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impact cratering
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what geological process is currently active on Mars?
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some still there, but frozen under surface; some stripped by solar wind (weak magnetic field); some broken into H or O by UV light
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what happened to Mars' water?
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they cooled off faster than Earth did
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why are smaller terrestrial bodies such as Mercury or the Moon "geologically dead"?
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it must have lost most of its carbon dioxide gas, which would have weakened the greenhouse effect until the planet essentially froze over
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how did Mars lose its atmosphere?
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it was too small to maintain the internal heat needed to keep water and gas
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How did Mars's size affect the loss of its atmosphere?
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it has cratering, many volcanoes, tectonic stresses, and erosion
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describe the basic geology of Venus
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Venus does not appear to have plate tectonics, but its entire surface seems to have been "repaved" 750 million years ago
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why is it surprising Venus lacks tectonic plates?
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runaway greenhouse effect
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a positive feedback cycle in which heating caused by the greenhouse effect causes more greenhouse gases to enter the atmosphere, which further enhances the greenhouse effect
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the runaway process would cause Earth to heat up until the oceans completely evaporated and the carbonate rocks released all their carbon dioxide back into the atmosphere
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why does the runaway greenhouse effect occur on Venus but not Earth?
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surface liquid water, atmospheric oxygen, plate tectonics, and climate stability
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How is Earth unique among the terrestrial planets?
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plate tectonics
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move at average speeds of a few cm's per year, but over millions of years their motions act like a giant conveyor belt for Earth's lithosphere, creating new crust and recycling old crust back into the mantle
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carbon dioxide cycle
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the process that cycles carbon dioxide between Earth's atmosphere and surface rocks
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it acts as a long-term thermostat
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why is the carbon dioxide cycle so important to Earth?
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the greenhouse effect is much stronger on Venus than on Earth
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what is the main reason Venus is so hot?
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located at optimal distance from the Sun for liquid water to exist and large enough for geological activity to release and retain water and atmosphere
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what makes a planet habitable?
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size
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which of a planet's fundamental properties has the greatest effect on its level of volcanic and tectonic activity?
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Venus
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which terrestrial world has the most atmospheric gas?
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carbon dioxide
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what is a strong greenhouse gas?
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life
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the oxygen in Earth's atmosphere was released by...
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locked up in rocks
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where is most of the CO2 that has outgassed from Earth's volcanoes?
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once important but no longer is
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describe our understanding of flowing water on Mars
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beyond the frost line, planetesimals could accumulate ice. Hydrogen compounds are more abundant than rock/metal so jovian planets got bigger and acquired H/He atmospheres. TIMING AND LOCATION
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Briefly describe how differences in composition among the jovian planets can be traced to their formation
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The extra mass of Jupiter compresses its underlying gas layers to a much higher density
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Why is Jupiter so much more dense than Saturn?
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The planet that forms earliest captures the most hydrogen and helium gas. Capture ceases after the first solar wind blows the leftover gas away.
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why is timing important in jovian planet formation?
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yes
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could a planet be smaller in size than Jupiter but greater in mass?
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Core: rock, metal & hydrogen compounds. Hydrogen gaseous form in surface. In deeper high pressure compress hydrogen into liquid form. Below, the temperatures and pressure hydrogen is formed into compact, liquid metallic form. Because the gravity compresses it into layers.
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Briefly describe the interior structure of Jupiter
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Saturn has the same layering as Jupiter but weighs less. Uranus and Neptune have different layering b/c their internal pressures never became high enough to form liquid or metallic hydrogen
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How do the interiors of the other jovian planets compare to that of Jupiter?
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The planet that forms in a denser part of the nebula forms its core first
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why is location important in forming the jovian planets?
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Earth's mass wasn't large enough to hold onto a H and He atmosphere
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Why didn't Earth accrete H and He gas from the solar nebula?
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it was generated by Jupiter's thick layer of metallic hydrogen
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why does Jupiter have such a strong magnetic field?
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Jupiter's atmosphere has 3 major types of clouds, each of which form at different altitudes. H compounds in Jupiter form clouds. Different cloud layers correspond to freezing points of different H compounds
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describe Jupiter's cloud layers
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the highest, coldest layer reflects white. Some clouds produce brown and red
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how do the cloud layers help explain Jupiter's colors?
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less light penetrates to the depths at which Saturn's clouds are found, and the light they reflect is more obscured by the atmosphere above them. deeper in and farther from the Sun
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Why are Saturn's colors more subdued?
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methane gas absorbs red light and transmits blue light. blue light reflects off methane clouds
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Why are Uranus and Neptune blue?
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Strong winds and powerful storms. Stripes on Jupiter- Bands of rising air are white because the rising air condenses and forms white ammonia clouds at high altitudes.
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Briefly describe Jupiter's weather patterns
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Great Red Spot
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a large, high-pressure storm on Jupiter
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small (1500 km)
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describe how we categorize jovian moons by size
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They actually contain very little material in a gaseous state
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The Jovian planets are sometimes called "gas giants". In what way is this term misleading?
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Gaseous on the outside, then liquid hydrogen, more dense metallic hydrogen, "rocky" core
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What is the structure of Jupiter like?
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It has metallic hydrogen inside, which circulates and makes a magnetic field
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Jupiter does not have a large metal core like Earth. How can it have a magnetic field?
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Most formed by accretion within the disks of gas surrounding individual jovian planets
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what is the origin of most of the medium and large size moons?
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Most are captured asteroids or comets
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what is the origin of most of the small moons?
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Io, Europa, Ganymede, Callisto
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name the order of Jupiter's Galilean moons (inside-outside)
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Io
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most volcanically active moon. Hot because of tidal heating
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Europa
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surface covered by water ice. few impact craters. clear signs of water activity. Like Io, it has tidal heating but weaker
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Ganymede
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surface of water ice. Largest moon in the solar system. Clear evidence of geological activity. Tidal heating plus heat from radioactive decay
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Callisto
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outermost Galilean moon, heavily cratered iceball. no tidal heating or orbital resonances. has magnetic field
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Saturn's Enceladus
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Shows clear evidence of ongoing geological activity, few impact craters because of that (erased). Could potentially have an ocean. Internal heat comes from tidal heating through an orbital resonance.
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Jupiter pulls harder on one side than the other
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how does Io get heated by Jupiter?
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Titan (Saturn)
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only moon in the solar system that has a thick atmosphere. It consists mostly of nitrogen with some argon, methane, and ethane.
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it had liquid methane and "rocks" made of ice. could have lakes of liquid methane
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describe Titan's (Saturn) surface
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It orbits Neptune "backward" and at a high inclination to Neptune's equator. Triton may have been a member of a Kuiper belt object that passed so close to Neptune that Triton lost energy & was captured while its companion gained energy and was flung away at high speed.
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why do we think Triton (Neptune) is a captured moon?
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they contain large proportions of ice -ice can melt or deform at lower temperature than rock. Tidal heating
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Briefly explain why icy moons can have active geology at much smaller sizes than rocky worlds.
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Particles moving slowly relative to one another and occasionally colliding and at times being forced out at others
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What are planetary rings made of?
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gap moons
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small moons within the rings that nudge the orbits of ring particles in a certain way
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New particles must replenish what has been destroyed. We think they must come from a source that lies in each planet's equatorial plane. Source is numerous small "moonlets" moons the size of gap moon that formed in the disks of material orbiting the young jovian planets
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Explain why ring particles must be replenished over time, and where we think ring particles come from
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its higher mass and gravity compress its interior
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why is Jupiter denser than Saturn?
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ongoing contraction or differentiation
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some jovian planets give off more energy than they receive because of...
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frozen hydrogen compounds
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The main ingredients of most moons of the Jovian planets are...
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Io has a different internal heat source
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Why is Io more volcanically active than our moon?
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it orbits Neptune (its planet) backwards
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what is unusual about Triton?
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Titan
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which moon shows evidence of rainfall and erosion by some liquid substance?
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orbital resonances
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Saturn's many moons affect its rings through...
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Are continually supplied with new particles by impacts with small moons.
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Saturn's rings...
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at least 1 km across. the largest is about 1000 km (Ceres)
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how large are asteroids?
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All the asteroids in the solar system wouldn't add up to even a small terrestrial planet
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how does the total mass of all asteroids compare to the mass of a terrestrial world?
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between the orbits of Mars and Jupiter
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where is the asteroid belt located?
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Jupiter's gravity, through influence of orbital resonances, stirred up asteroid orbits and prevented their accretion into a planet
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how have orbital resonances with Jupiter affected the asteroid belt?
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meteor
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the bright trail left by a meteorite
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meteorite
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A rock from space that falls through Earth's atmosphere
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primitive meteorite
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meteorites unchanged in composition since they first formed 4.6 billion years ago. stony, carbon-rich, rocky
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processed meteorites
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meteorites that are younger, have experienced processes such as volcanism or differentiation. metal-rich
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The inner part of a large asteroid that was shattered in a collision
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You find a meteorite that is made of metal. What is its origin?
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the comet is completely frozen and looks like a "dirty snowball"
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what does a comet look like when it is far from the Sun?
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coma
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atmosphere that comes from heated nucleus (comet)
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plasma tail
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gas escaping from coma, pushed by solar wind
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dust tail
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tail that is pushed by photons
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nucleus of a comet
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a chunk of ice mixed with rocky dust and some more complex chemicals
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the solar wind blows on them
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why do the comet tails point away from the Sun?
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a meteor shower would occur
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If Earth passed through the tail of a comet, what would happen?
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a Kuiper belt comet
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what do scientists think Pluto is?
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near the current orbits of the Jovian planets
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where did Oort Cloud comets form?
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because the orbiting Earth passes through a particular comet's orbit at the same time each year
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why do meteor showers recur at about the same time each year?
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in the Kuiper belt
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where did Kuiper belt comets form?
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tilted and significantly elliptical
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what is Pluto's orbit like?
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very cold. thin nitrogen atmosphere that refreezes on the surface. it's largest moon is as big as Pluto
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describe Pluto
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orbital resonances prevent it
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why won't Pluto collide with Neptune?
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the gravity can redirect a comet
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how do Jovian planets influence comets?
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Meteor showers are caused by the passage of Earth through the debris left by a comet in its orbit
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what produces meteor showers?
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yes, it must have been the core of a shattered asteroid
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can an asteroid be pure metal?
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no because Jupiter prevented one from accreting
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Did a large terrestrial planet ever form in the region of the asteroid belt?
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a comet
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what does Pluto most resemble?
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a grain of sand or a small pebble
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How big an object causes a typical shooting star?
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Oort cloud comets
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Which have the most elliptical and tilted orbits?
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Kuiper belt comets
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Which are thought to have formed farthest from the Sun?
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every million years
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About how often does a 1-kilometer object strike Earth?
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It would cause widespread devastation and climate change
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What would happen if a 1-kilometer object struck Earth?
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they formed in the Kuiper belt
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where do Kuiper belt comets come from?
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there would be more impacts from comets and fewer from asteroids
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how would the impact history on Earth have been different if Jupiter did not exist?
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a Sun-like star is about a billion times brighter than the light reflected from its planets. Planets are close to their stars, relative to the distance from us to the star.
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why are extrasolar planets difficult to detect?
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extrasolar planet
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a planet orbiting a star other than our Sun
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direct planet detection
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pictures or spectra of the planets themselves
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indirect planet detection
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measurements of stellar properties revealing the effects of orbiting planets
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observing the motion of a star to detect the subtle gravitational tugs or orbiting planets and observing changes to a star's brightness that occur when one of its planets passes in front of the star as viewed from Earth
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what are the 2 current major approaches to detecting extrasolar planets indirectly?
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The Sun's motion around the solar system's center of mass depends on tugs from all the planets
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how can gravitational tugs from orbiting planets affect the motion of a star?
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astrometric method
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the detection of extrasolar planets through the side-to-side motion of a star caused by gravitational tugs from the planet. difficult to measure
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GAIA Mission
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has the ambitious goal of performing astrometric observations of a billion stars in our galaxy with an accuracy of 10 microarcseconds, which should enable it to detect thousands of extrasolar planets
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Doppler Method
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searches for a star's orbital movement around the center of mass by looking for changing Doppler shifts in its spectrum
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hot Jupiter planet
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a planet that has a Jupiter-like mass but a much higher surface temperature
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transit method
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searches for transits and eclipses by carefully monitoring a star system's brightness over an extended period of time
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transit
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when a planet crosses in front of a star
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a transit reduces the star's apparent brightness and tells us the planet's radius
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what does a transit tell us?
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eclipse
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the planet passing behind the star
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the Kepler mission
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launched in 2008 to begin looking for transiting planets. It is designed to measure the 0.008% decline in brightness when an Earth-mass planet eclipses a Sun-like star.
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gravitational lensing
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Mass bends light in a special way when a star with planets passes in front of another star
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features in dust disks
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Gaps, waves, or ripples in disks of dusty gas around stars can indicate presence of planets
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orbital period and distance, orbital eccentricity, mass, size, density, and planet's atmospheric composition and temperature
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what properties of extrasolar planets can we measure?
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direct starlight is billions of times brighter than the starlight reflected from planets
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what makes imaging extremely difficult?
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about its planets
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what does a star's periodic motion tell us?
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through Doppler shifts or by measuring its motion across the sky
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how is a star's periodic motion detected?
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transiting planets
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what reduces a star's brightness?
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lower limits on masses
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what does Doppler data give us?
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It has a planet orbiting at greater than 1 AU
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Suppose you found a star with the same mass as the Sun moving back and forth with a period of 16 months. What could you conclude?
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ones that are closer to their star, are big, and have large masses
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what type of extrasolar planets are easier to find?
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they have wide variety of masses and sizes and many are orbiting close to their stars with large masses
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How do extrasolar planets compare with planets in our solar system?
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planetary migration
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A young planet's motion can create waves in a planet-forming disk. matter in these waves can tug on a planet, causing its orbit to migrate inward.
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they can eject one planet while flinging the other into a highly elliptical orbit
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what happens when there are close gravitational encounters between two massive planets?
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Multiple close encounters with smaller planetesimals
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what can cause inward migration?
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It transfers energy and angular momentum to another object.
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What happens in a gravitational encounter that allows a planet's orbit to move inward?
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incomplete
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is the nebular theory complete or incomplete?
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we don't know yet
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are planetary systems like ours common?
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Yes; Original nebular theory cannot account for the existence of hot Jupiters. Planetary migration or gravitational encounters may explain how Jupiter-like planets moved inward
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Do we need to modify our theory of solar system formation?
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no
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is the Sun on fire?
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no way
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is the Sun contracting?
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yes
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is the Sun powered by nuclear energy?
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the transit method
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what method has detected the most extrasolar planets so far?
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less than about 1%
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What fraction of extrasolar planets could in principle be detected by the transit method?
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its size
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Which one of the following can the transit method tell us about a planet?
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astrometric method
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Which method could detect a planet in an orbit that is face-on to the Earth?
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the transit method
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Which detection method was used by the Kepler mission?
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the transit and Doppler methods together
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To determine a planet's average density, we can use:
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"water world"
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Based on the model types shown in Figure 10.12, a planet made almost entirely of hydrogen compounds would be considered a
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They formed farther out like Jupiter but then migrated inward
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What's the best explanation for the location of hot Jupiters?
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present around at least 99% of all stars
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Based on current data, planetary systems appear to be
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gravitational equilibrium
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Gravity pulling in balances pressure pushing out
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energy balance
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Thermal energy released by fusion in core balances radiative energy lost from surface
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gravitational contraction
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provided energy that heated the core as the Sun was forming
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when fusion started replacing the energy radiated into space
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when does gravitational contraction stop?
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10 billion years
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How long will the Sun shine powered by nuclear fusion?
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the outward force of pressure is equal to the inward force of gravity everywhere in the Sun
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When we say the Sun is in gravitational equilibrium, we mean that...
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6.9 x 10⁸ m (109 times Earth)
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the Sun's radius
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2 x 10³⁰ kg (300,000 Earths)
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the Sun's mass
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3.8 x 10²⁶ watts
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the Sun's luminosity
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solar wind
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A flow of charged particles from the surface of the Sun
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corona (Sun)
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outermost layer of solar atmosphere (~1 million K)
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chromosphere (Sun)
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middle layer of solar atmosphere (~ 10⁴-10⁵ K)
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photosphere
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visible surface of the Sun (~6000 K)
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convection zone (Sun)
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energy transported upward by rising hot gas
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radiation zone (Sun)
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energy transported upward by photons
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core (Sun)
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energy generated by nuclear fusion (~15 million K)
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Core, Radiation zone, Convection zone, Photosphere, Chromosphere, Corona
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From inside out, what are the layers of the Sun?
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nuclear fusion in the core maintains both gravitational equilibrium between pressure and gravity and energy balance between thermal energy released in core and radiative energy lost from the Sun's surface
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why does the Sun shine?
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4 individual protons
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which of these groups of particles has the greatest mass?
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the photosphere
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Which of these layers of the sun is coolest?
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corona
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X-Ray images of the Sun generally show the...
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The mass of the product of the reaction is less than the mass of the hydrogen atoms that enter the reaction
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How do the nuclear reactions in the Sun's core produce energy?
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nuclear fission
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big nucleus splits into smaller pieces (nuclear power plants)
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nuclear fusion
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small nuclei stick together to make a bigger one (Sun, stars)
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High temperatures enable nuclear fusion to happen in the core. the higher the temperature, the more energetic the collisions
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why does nuclear fusion require high temperatures and pressures?
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fusion converts about 600 million tons of hydrogen into 596 million tons of helium every second, which means that 4 million tons of matter is turned into energy every second
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what is the overall nuclear fusion reaction in the Sun?
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by fusing 4 hydrogen nuclei into 1 helium nucleus
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how does the Sun release energy?
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proton-proton chain
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this is how hydrogen fuses into helium in the Sun
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step 1 of the proton-proton chain
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2 protons fuse to make a deuterium nucleus (1 proton and 1 neutron). this step occurs twice in the overall reaction
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step 2 of the proton-proton chain
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the deuterium nucleus and a proton fuse to make a nucleus of helium-3 (2 protons, 1 neutron). this step occurs twice in the overall reaction
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step 3 of the proton-proton chain
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2 helium-3 nuclei fuse to form helium-4 (2 protons, 2 neutrons), releasing 2 excess protons in the process
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4He nucleus, 2 gamma rays, 2 positrons, 2 neutrinos. total mass is 0.7% lower
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what is the overall reaction of the proton-proton chain?
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4 protons
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what goes IN in the proton-proton chain?
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4He nucleus, 2 gamma rays, 2 positrons, and 2 neutrinos
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what goes OUT in the proton-proton chain?
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the core would expand and cool
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What would happen inside the Sun if a slight rise in core temperature led to a rapid rise in fusion energy?
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solar thermostat
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keeps the rate of fusion steady
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neutrinos
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a type of fundamental particle that has extremely low mass and responds only to the weak force
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solar neutrino problem
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the disagreement between the predicted and observed number of neutrinos coming from the Sun
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solar activity
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short-lived phenomena on the Sun, including the emergence and disappearance of individual sunspots, prominences, and flares
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sunspots
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blotches on the surface of the Sun that appear darker than surrounding regions. cooler than other parts of the Sun's surface. STRONG magnetic fields
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solar prominences
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vaulted loops of hot gas that rise above the Sun's surface and follow magnetic field lines
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solar flares
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huge and sudden releases of energy on the solar surface, probably caused when energy stored in magnetic fields is suddenly released
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coronal mass ejections
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bursts of charged particles from the Sun's corona that travel outward into space
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helium, energy, and neutrinos
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At the center of the Sun, fusion converts hydrogen into
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photons
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Solar energy leaves the core of the Sun in the form of
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about the same
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How does the number of neutrinos passing through your body at night compare with the number passing through your body during the day?
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they are proportional. Increasing the temperature increases the pressure and vice versa. Decreasing the temperature decreases the pressure and vice versa
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how are temperature and pressure related?
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they are inversely proportional. P is proportional to 1/V. Decreasing the volume will increase the pressure. (compress the gas). Increasing the volume will decrease the pressure. (decompress)
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how are pressure and volume related?
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a couple hundred thousand years
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How long does it take for energy produced in the Sun's core to reach the photosphere?
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a few days
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How long does convection take to bring energy to the surface of the Sun?
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convection
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rising hot gas
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Zeeman Effect
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We can measure magnetic fields in sunspots by observing the splitting of spectral lines. lines get twisted