Of the three ways in which energy is transferred in nature (radiation, conduction, and convection) which two are important to the sun? |
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Radiation and Convection |
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Parallax is the |
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Apparent shift in the position of a nearby object as we move. |
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What process provides the power for the sun? |
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Fusion of hydrogen into helium. |
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Granulation on the surface of the Sun in caused by |
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Convective currents carrying heat from beneath the surface. |
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The nuetrino is |
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An elusive, subatomic particle having little or no mass and very difficult to detect. |
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What is the characteristic color of an emission nebula? |
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Red. |
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Astronomers measure the masses of stars by |
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Observing the motion of two stars in a binary star system. |
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A brown dwarf is |
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An object intermediate between a planet and a star, with not enough mass to begin nuclear reaction in its core. |
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The evolution of a star is controlled mostly by its |
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initial mass |
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The spectral sequence of star surface temperature as determined by relative spectral line strengths has been given which sequence of letters, in order of decreasing temperature? |
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OBAFGKM |
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If stellar parallax can be measured to a precision of about 0.01 arcsec using a telescope on Earth to observe stars, to what distance does this correspond in space? |
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100 pc |
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What is a positron? |
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A positive electron. |
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The phrase "hydrostatic equilibrium" in the sun refers to: |
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the balance of gravity inward and gas pressure outward. |
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The Hertzsprung-Russell diagram is a statistical plot of which stellar parameters? |
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Luminosity and Surface temperature |
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An arching column of gas suspended over a sunspot group is called |
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A prominence |
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The star Hadar has a spectral classification of B1 III. This tells us that Hadar is a |
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Hot Giant |
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Sunspots are |
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Cooler, darker regions on the suns surface |
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Stars that have ejected a planetary nebula go on to become |
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white dwarfs |
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The temperature of the center of the sun where thermonuclear processes take place is approximately |
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1.5 x 107 K |
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The spectral class of the sun in G2 and the star Enif in K2. From this information, we know that Enif is |
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Cooler than the sun. |
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Where do we find the most massive stars on the main sequence in a HR diagram? |
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Upper left |
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What fraction of the stars in the night sky are main sequence stars? |
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Almost all, 90% |
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The temperature of the sun's photosphere is |
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5800 K |
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How can we characterize the rotation of the Sun? |
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Differential rotation with the equator rotating faster than the poles |
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What occurance defines the end of the protostar phase of a star's life and the start of the main sequence phase? |
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Nuclear reactions begin in its core |
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What name is given to the visible "surface" of the Sun? |
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Photosphere |
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There is a mass limit for a star in the white dwarf phase, the Chandrasekhar limit, beyond which the star can no longer support it's own weight. This mass limit, in terms of solar mass, is |
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1.4 |
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The Zeeman effect refers to |
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the splitting of spectral lines when magnetic fields are applied to atoms |
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What is a red giant? |
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A star burning hydrogen into helium in a shell around the core |
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What is the last nuclear burning stage in the life of a low mass star like the sun? |
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Fusion of helium nuclei to form carbon and oxygen |
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Degeneracy occurs when |
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electrons inside a star resist being pushed closer together than a certain limit. |
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What proportion of visible stars in the night sky are multiple star systems? |
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About 50% or __ |
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A corona hole shows up most prominently in photographs taken at what wavelength? |
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X-ray |
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The majority of the elements heavier than hydrogen and helium in the universe are believed to have originated in |
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The central cores of stars |
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The effect of interstellar dust on starlight is |
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to dim and redden distant stars by preferentially scattering their blue light |
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The corona of the Sun has a temperature of |
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1-2 million K |
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Apparent Magnitude is a measure of the |
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Brightness of a star as seen from Earth |
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From the center outwards, the order of the layers or parts of the Sun is |
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Radiative, convective, photosphere, chromosphere, corona |
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The extremely high gas temperatures in the solar corona mean that this region is best observed at a wavelength of |
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X-rays |
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The termperature at which thermonuclear reactions begin to convert helium into carbon (helium burning) is |
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100 million K |
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Sunspots are caused by |
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Differential rotation and its effect on weak magnetic fields |
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A planetary nebula is |
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An expanding gas shell surrounding a hot, white dwarf |
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What is the most abundant element in the universe? |
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Hydrogen |
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The total time that the Sun will spend as a main sequence star is |
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About 10 billion years (1010 years) |
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At what distance are stars assumed to be from the Earth when they are represented by their absolute magnitude? |
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10 years |
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What happens to the helium rich core of a star after the core runs out of hydrogen? |
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It contracts and heats |
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On the HR diagram, in which direction does the position occupied by a star move after hydrogen burning ends in the star's core? |
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Towards the upper right |
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The age of a cluster can be found by |
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Determining the turnoff point on the main sequence of its HR diagram |
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The Orion Nebula is |
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A large interstellar gas and dust cloud containing many young stars |
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The spectral type of a star is most directly related to (and determines uniquely) its |
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surface temperature |
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