SOLAR SYSTEM EXAM 3 – Flashcards
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How can the eight major planets of our solar system can be classified on the basis of their properties and orbits?
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They divide naturally into two main groups.
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Where in the solar system would you find Kuiper belt objects?
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beyond the orbit of Neptune, extending perhaps as far as 500 AU from the Sun
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Which components of the present solar system have probably remained essentially unchanged since the solar system was formed and can therefore provide valuable clues to the manner of this formation?
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comets, asteroids, and meteoritic material
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Why do astronomers no longer consider Pluto to be a planet?
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It is a member of a system of small objects, most of which are too small to be planets and show different orbits than the eight main planets.
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An object less than a thousand kilometers across, composed of rock and iron and orbiting closer to the Sun than the planet Jupiter, would be called
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an asteroid.
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There are no impact craters on the surface of Jupiter because...
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its surface is really the top of a very deep gaseous atmosphere.
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Our planetary system is believed to have originated in a disk of gas and dust that surrounded the Sun shortly after the Sun formed. Such disks around young stars are
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an observational fact, having been observed around other stars in our Galaxy.
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What are the most abundant elements in the solar system?
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hydrogen and helium, as shown by the great mass of the giant planets
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The early universe appears to have contained only light elements, predominantly hydrogen and helium, and yet we now see significant amounts of heavier elements in stars and planets and our own bodies. Where did these heavy elements originate?
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in nuclear fusion in the deep interiors of stars and in violent explosions of massive stars (supernovae)
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The ages of lunar rocks, brought back to Earth by astronauts and robotic spacecraft, have been determined by measuring the
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relative concentrations of radioactive elements.
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What process heated the early solar nebula as it slowly condensed toward a central protosun?
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collisions of particles as they fell toward the center of the nebula due to gravity, thus converting kinetic energy into heat
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What is the fundamental law of physics that allowed the planets to form, rather than having all of the material simply fall into the Sun?
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conservation of angular momentum
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In our solar system, the inner planets are mostly rock and iron and the outer planets are mostly lighter material, such as hydrogen and ices. Why did the solar system form this way?
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The inner solar system was warm enough for the lighter material to vaporize (or never solidify), leaving rock and iron to form the inner planets.
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What is the process by which the terrestrial planets are believed to have formed?
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accretion, in which dust particles stick together to form asteroid-like objects and then collide to eventually form the planets
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What is the process by which the Jovian planets are believed to have formed?
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the accretion of dust and ice particles to form a planetary core, which then captured hydrogen and helium to form the planets that we see today
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A gas giant planet has been found in orbit around the star HD 209458. How have astronomers been able to study the atmosphere of this planet?
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The planet passes in front of the star as seen from the Earth, and its atmosphere absorbs some of the star's light at wavelengths characteristic of hydrogen and other elements in the planet's atmosphere.
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Many of the extrasolar planets that we have found have masses similar to or even greater than Jupiter, and yet they are orbiting very close to their stars—some well within Mercury's orbital distance from the Sun. Nothing like this is seen in our solar system. How did these massive extrasolar planets come to be where we find them?
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They are gas giants that formed much farther out in the protoplanetary nebula by core accretion, like our Jovian planets, and then they migrated inward to where we see them now.
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What are some properties of the large planets?
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further from sun, have rings, tend to be gaseous
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What are some properties of the small planets?
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closer to the sun, tend to be rocky
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What are some properties of the sun?
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at "center", way larger than everything else
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Do all planets orbit in the same direction?
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yes
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Which planets do not rotate on their axis in the same direction as the other planets?
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venus and uranus (and the sun)
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What are some properties of the terrestrial planets?
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rockey, inner solar system, slow rotation, few or no moons
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What are some properties of the jovian planets?
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gaseous, outer solar system, rapid rotation, rings, and many moons
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What are the properties of Mercury?
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looks a lot like moon (dry and has craters), terrstrial, very close to the sun so hard to make good observation, orbits the fastest
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What are the properties of Venus?
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Similar to earth in size and mass, has clouds, very hot and high pressure, run away green house effect, has the highest average surface tempature (greenhouse effect)
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What are the properties of the earth?
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only terrestrial planet to have a moon, has the highest density
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What are the properties of mars?
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one day is roughly 24 hours, their tilt on axis is almost the same as ours (seasons same)
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What are the properties of jupiter?
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gaseous, continuos storm, has the highest mass, most gravitational force
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What are the properties of saturn?
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rings, less dense then water
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What are the properties of uranus?
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tipped on it's side
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What are the properties of Neptune?
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Storm, "mini jupiter"
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What is a planet?
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"a planet is a body that orbits the sun, is large enough (has enough mass) to be round, and has 'cleared the neighborhood' of smaller objects"
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What is a dwarf planet?
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is a planet that orbits the sun and has enough mass to be round, but doesn't clear the neighborhood of smaller objects
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What is an asteroid?
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rocky objects which orbit between mars and jupiter,
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What are comets?
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come from beyond the orbit of neptune and are chunks of very dirty ice
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Kuiper Belt
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Reigon that extends from around Neptune to about 500 AU from sun, some comets come from here, icy and rocky bodies, more massive than asteroid belt
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Oort cloud
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proposed massive sphere of cometary material from 50,000 to 100,000 AU from sun, left over material from formation of solar system, source of unbound comets
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How many dwarf planets are their in our solar system?
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5 that orbit our sun
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Which planet has the longest day?
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Venus (243 earth days) to rotate on axis
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Where did the elements come from?
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after the big band, only the lightest elements emerged (primarily hydrogen and helium), the first stars were primarily made of hydrogen with a little helium, the first stars processed the hydrogen and helium to make the heavier elements
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What are giant molecular clouds?
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cold, massive clouds of gas and a little bit of dust. 71% hydrogen 27%helium and 2% everything else, multiple stars can form one cloud
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what is a protostar?
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the greatest concentration of matter at the center. as materials fall inward it gains speed and collides with other materials and heats up. the whole nebula heats up (kelvin and helmholtz contraction)
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Roatation
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the nebula starts with some rotation, was the material collapses inward, the nebula rotates faster
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L=MVrotR conversation of angular momentum
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L=angular momentum (basically stays the same) M=mass (doesnt change) Vrot=rotational velocity (increases) R=distance from center
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what is protoplanetarydisk?
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when the nebula flattens out, it's in this disk that the planets form
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What is the result of contraction and rotation?
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a flat rapidly rotating disk forms, the matter concentrated at the centers becomes the protosun
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as the protosun was growing, what parts of the solar nebula were warmer while what parts are colder?
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the inner parts are warmer, the outer parts are colder
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what happened to the inner regions during planet formation?
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water were vaporized and other gasses were pushed away and only the heavier elements were left, terrestrial planets formed from the remaining rocky material
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What is terrestrial planet formation?
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Ionized atoms stick by sharing electrons building to dust grains, dust grains and pebbles collide sticking together, accumulate into larger planetsimals
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What is differentiation?
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Gravity tends to drag heavier objects down...planets differentiate
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What is core accreation?
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Cored build up in the same way as terrestrial planets, thanks to colder temps gas was moving slowly and was easily captured by the massive cores Uranus and Neptune probably formed closer to the sun and got flung out
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Disk instability
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Instability in the disk leads to clumps, gravitational collapse allowed planets to form,do not form from rocky cores
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Radioactive unstable nuclei
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Too many protons or neutrons
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Radioactive decay
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Change from one element to another
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Radioactive dating
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Each radioactive nucleus decays at it's own rate
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Astrometric method
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Precise measurements of a stars position in the sky relative to other stars
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Radial velocity method
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also called Doppler shift method, spectrum shifts blue to red and red to blue, yields planets orbital periods, mass and distance from star
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How do we detect extrasolar planets
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Look for wobbles in stars
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Transit method
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Planet orbits in front of star then brightness of star goes down
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Field reversal
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There is evidence that our magnetic field flips from time to time
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Solar wind
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The sun emits charged particles (mostly protons and electrons) called solar windo
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Rifts
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Where crust is breaking apart
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Subduction
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One crust may slip beneath another
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Which waves cannot make it through liquid P waves or S waves
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S waves
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Seismic waves
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Transverse
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P waves
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Longitudinal
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Earths structure
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-crust (least dense, mainly silicates) -mantle (mainly iron-magnesium, slow motion like wax) -liquid core (dense liquid material, mixture of iron, nickel and perhaps sulfur, all melted) -solid inner core (solid iron and nickel, the pressure is so high it makes it solid)
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The observation that first suggested to geologists that the Earth's core may be molten was that
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P waves from an earthquake could be observed on the diametrically opposite side of the Earth from the earthquake, but S waves could not.
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The reason the Earth has a core of almost pure iron is that
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iron is the most abundant heavy element, and it sank while the Earth was molten, by differentiation.
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The material in the innermost core of the Earth is
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hot and solid.
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The majority of earthquakes occur
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at the boundaries of tectonic plates.
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The magnetosphere is
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a cavity within the high-speed solar wind, caused by the Earth's magnetic field.
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What is the long-term behavior (over millions of years) of the Earth's magnetic field?
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The field is normally relatively stable, but the north and south magnetic poles reverse every 300,000 years or so (the north pole becomes a south pole, and vice versa).
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What is the primary function of a greenhouse gas?
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It absorbs infrared radiation emitted by the ground.
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How many different layers are there in the Earth's atmosphere?
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4
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What are the four layers of the Earth's atmosphere?
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1.) Troposphere 2.) Stratosphere 3.) Mesosphere 4.) thermosphere/lonosphere
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What happens in the troposphere?
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sunlight heats earth's surface, causes convection (warm on bottom, cold on top), contains half of the earth's atmosphere, weather occurs in this layer
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What happens in the stratosphere?
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ozone absorbs harmful rays from the sun and UV here and heats up, temperature increases with height, very stable
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What happens in the mesosphere?
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temperature decreases with height, meteors and rock fragments burn up
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What happens in the thermosphere / lonosphere?
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layer with auroras, oxygen and nitrogen atoms absorb, short UV radiation
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What is half life?
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time in which one-half of the nuclei decays, comparing the ratio of elements determines the age
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Gravitational lensing method
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planet passes in front of different star (a star thats behind it), gravitational lensing makes background star look brighter, very rare method
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What happens as you go from the outter layers of the earth to the inner?
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the pressure and temperature increase
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What is the difference between small and large bodies when it comes to internal heating?
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smaller bodies radiate heat quicker, larger bodies should have hot interiors radioactive decay radiates heat
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Do geographic poles and magnetic poles line up?
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No, a geographic north pole is a magnetic south pole and geographic south pole is magnetic north pole
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What can generate magnetic fields?
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electric currents
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For planets, where is the electric current generated from?
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molten outter core in rotation, need a charged material (hot liquid) and needs to be in rotation
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is the magnetic field static?
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No, it is moving all the time and the pole location is changing, north and south poles move independently
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What is field reversal?
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there is evidence that our magnetic field flips from time to time, not clear why it does
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What is the aurora?
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particle overload, a leak through the magnetic field, an interaction with upper atmosphere, when charged particle collide with atoms, northern lights come from here as a result of light being emited
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What is the internal structure of the earth?
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low density crust, crust mantle, liquid outer core (process of differentiation), solid inner core
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Earths atmosphere
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78% N, 21% O, 0.03% Co2, and 0-2% H2O atmosphere shields us from harmful UV radiation help keeps surface warm and spreads heat around gases mostly released through volcanic activity
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What is the coriolis effect?
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on a non-rotating body (object), objects travel in a straight line the earth rotates causing the path of the object to change causes rotation seen in weather systems
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Greenhouse effect
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greenhouse gases (CO2 and H2O) are transparent to visible light, but not to infrared light
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What does a lot of craters on the moons surface mean?
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means the surface is old and has no weathering
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Does the moon have plate tectonics?
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no, or no magnetic field, or no atmosphere has cooler interior
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What is maria?
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remains of huge lava flows, less craters than highlands, is younger, circular in shape (implies large impacts), explains mountains: materials being thrust up from the impact
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What are lunar highlands?
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older, light-colored terrain, far side of the moon is predominately lunar highlands, presume crust is thicker
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maira vs highlands
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maria made of basalt and rich in iron, magnesium, and titanium highlands are rich in calcium and aluminum silicates highland material is generally less dense and older
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Lunar structure
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Magnetometers: no magnetic field seismometers: found moonquakes, but way more earthquakes per year Crust: varies in structure Mantle: too cold and rigid Small molten core containing little iron *compared to earth
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Lunar rocks
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all lunar rocks are igneous rocks (were molten at one time), similar to terrestrial volcanic rocks, are totally dry
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What is the primary reason for tides?
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the moon, but the sun also plays a roll
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What are spring tides?
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when the moon and sun line up their tidal forces line up giving a larger shift in the water level moon is in new or full phase
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What are neap tides?
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when the sun and moon are at right angels the tidal forces partially cancel each other out yielding smaller tidal shifts
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What is tidal recession?
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our moon has even a long term effect on our earth and itself, the earths rotation is faster than the moons orbit around the earth
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What is synchronous rotation?
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the earth exerts tidal forces on the moon, the moon would buldge towards earth due to tidal forces (when moon was molten rock), earths gravitational pull would try and force an alignment, slowing down the moons rotation, moon cooled and locked in this rotation rate and shape
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What is the fission theory?
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spin of earth threw off material from earth onto the moon, can't explain the differing properties of the rocks (missing some elements)
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What is the capture theory?
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the moon was captured by earth's gravity, this is very unlikely
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What is the co creation theory?
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the moon formed debris, similar to the planets. but why only around the earth did a moon form?
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What is the collisional ejection theory?
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collision of large body with young earth > ejected debris from the collision forms the moon > moons interior is molten > moon's surface cools and crust forms: smaller impacts create craters > large impacts create basins > basins flood with lava to form maria