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Exam 2 Review Astronomy 101 Jeopardy The Interstellar Medium Measurement Techniques The Lives of Stars The Deaths of Stars The H-R Diagram 10 20 30 40 50
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An astronomer studying newborn stars should search for these star- forming regions of the ISM.
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10 points Giant molecular clouds
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This type of light is the most easily scattered.
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20 points Blue Light
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Thermal energy causes clumps in giant molecular clouds to increase their temperature; this form of energy causes the clumps to contract in size.
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30 points Gravitational potential energy
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OB Associations produce UV radiation which can excite or ionize hydrogen atoms, producing a reddish glow from these types of nebulae.
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40 points Emission nebulae
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Young stars eject mass into space, creating a solar wind that blows away any remaining parts of the nebula, during this stage of star formation.
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50 points T Tauri stage
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The color index B-V measures a star's apparent magnitude in these two filters.
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10 points B = Blue V = Visible or Yellow
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The distance between Earth and a nearby star can be calculated by measuring this.
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20 points Parallax angle
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We can use apparent magnitudes when determining the age of a star cluster because we assume all the stars have this in common.
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30 points Distance from Earth
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A parsec is a unit of distance, and is equivalent to this many light years.
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40 points 3.26 light years
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If we measure a parallax angle of 1 arcsec for a star that we know is 1 pc away, then we know the baseline for our measurement must be this.
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50 points 1 AU (astronomical unit)
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Stars spend about 90% of their lifetimes in this region of the H-R diagram.
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10 points Main Sequence
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While on the main sequence, the core of a star is undergoing nuclear fusion which turns hydrogen into this element.
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Helium 20 points
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This spectral type of star (OBAFGKM) spends the longest amount of time on the main sequence.
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30 points M Stars
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This balance is reached when the inward pull of gravity is exactly balanced by a source of outward pressure.
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40 points Hydrostatic Equilibrium
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The stellar classifications scheme (OBAFGKM) was originally based on the strength of absorption lines produced by this element.
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50 points Hydrogen
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Stars leave the main sequence when this process stops in their cores.
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10 points Hydrogen fusion
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Very heavy elements, such as gold, are made when very massive stars become one of these.
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20 points Supernova explosion
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When a star like the Sun dies and becomes a white dwarf, it will be composed mostly of this element.
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30 points Carbon
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This strange form of pressure prevents a white dwarf from collapsing into a neutron star or black hole.
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40 points Electron degeneracy pressure
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The cores of very massive stars never reach a degenerate stage between fusion cycles; thus, massive stars never experience this (which is common in low mass stars).
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50 points Helium Flash
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The H-R diagram is used to show the relationship between the temperature of a star and this.
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10 points Luminosity
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Astronomers use these to trace out a star's evolution on the HR diagram.
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20 points Evolutionary tracks
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These types of diagrams, which plot apparent magnitudes as a function of color indices, are really H-R diagrams in disguise.
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30 points Color Magnitude Diagrams
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Main sequence stars form (approximately) a diagonal line across an H-R diagram. These types of objects occupy the lower left region of an H-R diagram (high temperature, low luminosity).
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40 points White dwarfs
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The H-R diagram is named after these two astronomers who developed it.
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50 points Hertzsprung and Russell
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Astronomy Jeopardy Rules Get into groups of 4-5 people and select one person to be the team “buzzer.” After a question is asked, everyone on a team must agree on the answer. When you have the answer, the team “buzzer” who puts his/her hand up fastest will be called on first. You must answer in the form of a question! No shouting out answers! Play Jeopardy!
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