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The energy emitted by the Sun is produced in a very small region at:
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Tremendous pressure is created at the Sun’s center due to its own gravity. The Sun is kept from collapsing by thermal pressure generated by:
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The existence in the Sun’s atmosphere of elements such as calcium is inferred from absorption lines in
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the photosphere and chromosphere |
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The photosphere (visible surface) of the Sun is like:
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a cloud. You would notice very little changes of its apparent surface changes as you went through it |
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The ________ is the outermost, hottest part of the Sun’s atmosphere:
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The temperature in and around the sun drops as you move from the core to the
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chromosphere then rises again |
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The ______-year solar cycle is characterized by a variation in the number of sunspots AND reversal of the Sun’s magnetic field.
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Sunspots appear dark because they are
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a bit cooler and thus dimmer than the rest of the photosphere |
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How would sunspots appear if you could magically seperate them from the Sun?
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They would shine brightly with and orange color |
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The seen visible interaction of the solar wind with Earth’s magnetic field is
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The sun is a stable as a star because
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gravity blances forces from pressure. |
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The proton-proton cycles involves what kind of fusion process?
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What is responsible for the increase in temperature of the corona?
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The number of sunspots and solar activity in general peaks
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The temperature of the layer of atmpsphere that produces the visible surface of the sun is
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By what mechanism does solar energy reach the sun’s photosphere from the layer just underneath it
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What is the meaning of solar constant?
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The amount of solar energy reaching the earth per unit area |
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Loops of glowing solar material seen sticking out from the solar limb during eclipses totality are called
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The solar nuetrino problem refers to the fact that astronomers can only |
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dectect about 1/3 of neutrinos expected by this theory |
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You can best model the size and distance of our sun and the next nearest star using |
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two golf balls a few hundred km apart |
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The angle of stellar parallax for a star gets larger as the length of the |
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A star’s proper motion is |
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its annual apparent motion in the sky. |
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A star’s apparent magnitude is
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a number used to describe how our eyes measure its perceived brightness. |
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The absolute magnitude of a star is its brightness as seen from a distance of
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Wien’s law (related to the black body curve) tells us that the
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hotter an object the shorter peak wavelength of its emitted light. |
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We can estimate the surface temperature of a star by using its |
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color, the pattern of absorption lines, Wiens’ law differences in brightness as measures through blue and red filters. |
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If the sun had the diameter of a tennis ball then the red supergiant Betelgeuse would have a diameter of
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23 m (larger than the scaled size of Mars’ orbit.) |
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Two stars have the same surface temp, but the radius of one is 100 times that of the other.
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The larger star is 10,000 times more luminous (100^2). |
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What are the two most important intrinsic properties for classifying stars?.
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Luminosity and surface temp |
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Which property of a star would not change if we could observe it from twice as far away |
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Astronomers can estimate the size of a star using |
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apparent brightness, direct observation of diameter, and temperature. |
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Stellar parallax is used to measure |
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In the stellar magnitude system, invented by Hipparchus, a smaller magnitude indicates a
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Which of the following quantities do you need in order to calculate a star’s luminosity? |
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Apparent brightness and distance to the star |
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Which spectral classification type corresponds to a star like the sun?
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Eclipsing binary stars are very useful for determining
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What is the single most important characteristic in determining the course of a star’s evolution? |
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When a star’s visible light passes through interstellar dust, the light we see is
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The _________ of light passing through thin dust clouds lets us map the milky way galaxy’s magnetic field:
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Emission nebulae like M42 in Orion occur only near stars that emit |
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large amounts of UV radiation. |
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An emission nebula appears primarily ________ in color, due to ionized hydrogen:
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What do “forbidden” lines reveal about interstellar space?
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The density and pressure of interstellar gas is much lower than can be produced in a lab on Earth |
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If one region of the sky shows nearby stars, but no distant stars or galaxies, our view is
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probably blocked by interstellar dark cloud of gas and dust |
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The Local Bubble was probably created by a nearby supernova perhaps
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300,000 years ago brighter than the full moon. |
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What information does 21-c radiation provide about the gas cloud that emitted it?
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Radial velocity, density, temperature. |
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21-C radiation is important and useful because its radio waves
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pass unaffected through interstellar dust |
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Interstellar gas is composed of |
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90 percent hydrogen, 9 percent helium, and 1 percent heavier elements |
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Some regions of the Milky Way's disk appear dark because |
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stars in that direction are obscured by interstellar dust |
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When a star's visible light passes through interstellar dust, the light we see |
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Of the given forms of radiation, visible radiation gives us the least accss
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• Most of the hydrogen molecules (2 hydrogen molecules) in the universe are found in ➢ |
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Cold, dense, interstellar clouds |
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• The reddish color of emission nebulae indicates that ➢ |
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• Complex molecules in a space are found ➢ |
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Primarily inside dense, cold dust clouds |
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