Mastering Astronomy Chapters: 9-13 – Flashcards

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question
Where does an object on an elliptical orbit experience the greatest acceleration?
answer
where spacetime has the most curvature
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Imagine that the Sun could be turned into a black hole without changing its mass. How would Earth's orbit change?
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Earth's orbit would not change.
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Imagine that the Sun gained mass without changing its radius. How would the structure of spacetime change at the distance of Earth's orbit?
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Spacetime would become more curved at Earth's orbit.
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From the viewpoint of an observer in the orbiting rocket, what happens to time on the other rocket as it falls toward the event horizon of the black hole?
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Time runs increasingly slower as the rocket approaches the black hole.
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As the falling rocket plunges toward the event horizon, an observer in the orbiting rocket would see that the falling rocket __________.
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slows down as it approaches the event horizon, and never actually crosses the event horizon
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From Part B, you know that from afar we'll never see the in-falling rocket cross the event horizon, yet it will still eventually disappear from view. Why?
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Its light will become so redshifted that it will be undetectable.
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If you were inside the rocket that falls toward the event horizon, you would notice your own clock to be running __________.
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at a constant, normal rate as you approach the event horizon
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If you were inside the rocket that falls toward the event horizon, from your own viewpoint you would __________.
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accelerate as you fall and cross the event horizon completely unhindered
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All millisecond pulsars are now, or once were, members of binary-star systems.
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True
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The fact that gamma-ray bursts are so distant means that they must be very energetic events.
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True
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All things, except light, are attracted by gravity.
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False
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According to general relativity, space is warped, or curved, by matter.
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True
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Although visible light cannot escape from a black hole, high-energy radiation, like gamma rays, can escape.
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False
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A neutron star is about the same size as
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A U.S. city
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Thousands of black holes have now been identified in our Galaxy.
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False
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The most rapidly "blinking" pulsars are those that
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spin fastest
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The X-ray emission from a neutron star in a binary system comes mainly from
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heated material in an accretion disk around the neutron star.
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Gamma-ray bursts are observed to occur
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approximately uniformly over the entire sky.
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If the Sun were magically to turn into a black hole of the same mass,
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Earth's orbit would remain unchanged.
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The best place to search for black holes is in a region of space that
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has strong X-ray emission.
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In a neutron star, the core is
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made of compressed neutrons in contact with each other.
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Two important properties of young neutron stars are
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extremely rapid rotation and a strong magnetic field.
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An object more massive than the Sun, but roughly the size of a city, is a
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neutron star
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The mass range for neutron stars is
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1.4 to 3 solar masses
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Neutron stars have
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very strong bi-polar magnetic fields.
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In the Lighthouse Model,
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if the beam sweeps across us, we will detect a pulse of radiation.
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Neutron stars do not have
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rotation periods comparable to the Sun's.
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The supernova of 1054 AD produced:
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a pulsar with a period of 33 milliseconds, visible optically.
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Three terrestrial-sized planets in orbits of a fraction of an AU have been found near
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a millisecond pulsar.
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Almost half of all known millisecond pulsars are found in what type of object?
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globular clusters
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X-ray bursters occur in binary star systems. The two types of stars that must be present to make up such an object are:
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a main sequence or giant star and a neutron star in a mass transfer binary.
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Pulsars have a measured mass of
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about 1.4 solar masses.
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You would expect millisecond pulsars to be
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part of a binary system.
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A proposed explanation for gamma-ray bursters is A-coalescence of a neutron star binary. B-hypernova-making black holes and bi-polar jets. C-collisions between two white dwarfs. Both A and B are possible. All three are possible.
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Both A and B are possible.
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What would happen if more mass was added to a 1.4 solar mass neutron star?
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It could eventually become a black hole, via a hypernova explosion.
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A hypernova creates
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A black hole
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The densely packed neutrons of a neutron star cannot balance the inward pull of gravity if the total mass is
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greater than Schwartzschild's limit of 3 solar masses.
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The Schwartzschild radius for a 12 solar mass star is
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36 km
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What explanation does general relativity provide for gravity?
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Gravity is the result of curved spacetime.
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An observer on a planet sees a spaceship approaching at 0.5c. A beam of light projected by the ship would be measured by this observer to travel at
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c.
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As a spaceship's velocity gets closer to the speed of light
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its length will decrease and its clock will run more slowly.
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If light from a distant star passes close to a massive body, the light beam will
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bend towards the star due to gravity.
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What can we detect from matter that has crossed an event horizon?
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Nothing
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As a spaceship nears an event horizon, a clock on the spaceship will be observed
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to run slowly
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If the Sun were replaced by a one solar mass black hole
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we would still orbit it in a period of one year.
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What is Cygnus X-1?
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the leading candidate for an observable black hole binary system
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A method for identifying a black hole is to
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look for their effects on nearby companions.
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The largest known black holes
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lie in the cores of the most massive galaxies.
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Any main sequence star over 25 solar masses will probably retain enough matter in its core after its type II supernova to make a black hole.
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True
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The Schwarzschild radius of a black hole is about 3 km per solar mass; it is amazingly linear over a wide range of masses.
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True
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Special relativity says that c, the speed of light, is the maximum velocity for both matter and energy in our universe.
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True
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Who discovered the first four pulsars?
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Jocelyn Bell
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In a neutron star, the protons and electrons are fused together, leaving only neutrons.
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True
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A neutron star is what remains after a Type II supernova explosion has destroyed the rest of the star.
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True
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In a neutron star, the electrons in the core are all in contact with each other.
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False
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The "pulse" from a pulsar is due to the rapidly expanding and contracting outer shell of the star.
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False
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Pulsars are created in a Type I supernova.
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False
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The pulses from a pulsar are most likely coming from localized areas near the magnetic poles.
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True
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While most pulsars slow down over time, millisecond pulsars spin faster due to the mass transfer from a close companion.
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True
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An X-ray burster is similar to a nova.
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True
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Gamma-ray bursts are all found to be within our galaxy.
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False
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Gamma-ray bursters seem scattered randomly over the entire sky.
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True
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All the gamma-ray bursters measured to date have distances of millions or even billions of light years.
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True
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All Type II supernovae produce neutrons stars when they collapse.
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False
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Both space and time are warped near the strong gravitational fields of neutron stars and black holes.
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True
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No communication is possible across an event horizon.
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True
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The presently known laws of physics clearly describe the conditions inside a black hole's event horizon.
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False
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The radius of a white dwarf is determined by a balance between the inward force of gravity and the outward push of _________
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electron degeneracy pressure
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A(n) __________ occurs when hydrogen fusion ignites on the surface of a white dwarf in a binary system.
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nova
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A(n) _________ occurs when fusion creates iron in the core of a star.
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massive star supernova
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A white dwarf in a close binary system will explode as a supernova if it gains enough mass to exceed the ________.
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white dwarf limit (1.4 solar masses)
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A(n) _______ consists of hot, swirling gas captured by a white dwarf (or neutron star or black hole) from a binary companion star.
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accretion disk
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A(n) ________ can occur only in a binary system, and all such events are thought to have the same luminosity.
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white dwarf supernova
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All of the single red-dwarf stars that ever formed are still on the main sequence today.
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True
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The Sun will get brighter as it begins to run out of fuel in its core.
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True
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A planetary nebula is the disk of matter around a star that will eventually form a planetary system.
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False
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The various stages of stellar evolution predicted by theory can best be tested by observations of stars in clusters.
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True
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A nova is a sudden outburst of light coming from an old main-sequence star.
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False
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It takes less and less time to fuse heavier and heavier elements inside a high-mass star.
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True
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In a core-collapse supernova, the outer part of the core rebounds from the inner, high-density core, destroying the entire outer part of the star.
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True
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Because of stellar nucleosynthesis, the spectra of old stars show more heavy elements than those of young stars.
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False
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A white dwarf is supported by the pressure of tightly packed
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electrons
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A star like the Sun will end up as a
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White Dwarf
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A white dwarf can dramatically increase in brightness only if it
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Has another star nearby
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Nuclear fusion in the Sun will
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create elements up to and including oxygen.
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Most of the carbon in our bodies originated in
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the core of a red-giant star.
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If the evolutionary track in Overlay 3, showing a Sun-like star, were instead illustrating a significantly more massive star, its starting point (stage 7) would be
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up and to the left
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A star (no matter what its mass) spends most of its life:
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As a main sequence star
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When a star's inward gravity and outward pressure are balanced, the star is said to be
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in hydrostatic equilibrium.
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What temperature is needed to fuse helium into carbon?
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100 million K
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A star is on the horizontal branch of the H-R diagram. Which statement is true?
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It is burning both hydrogen and helium.
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During the hydrogen shell burning phase
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the star grows more luminous.
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A solar mass star will evolve off the main sequence when
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it builds up a core of inert helium.
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A surface explosion on a white dwarf, caused by falling matter from the atmosphere of its binary companion, creates what kind of object?
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Nova
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Virtually all the carbon-rich dust in the plane of the galaxy originated in
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Low mass stars
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An iron core cannot support a star because
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iron cannot fuse with other nuclei to produce energy.
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A 20 solar mass star will stay on the main sequence for 10 million years, yet its iron core can exist for only a
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day
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As a star's evolution approaches the Type II supernova, we find A.) helium to carbon fusion takes at least 100 million K to start. B.) the heavier the element, the higher the temperature to fuse it. C.) photo disintegration of iron nuclei begins at 10 billion K to ignite the supernova. D.) the heavier the element, the less time it takes to make it. E.) All of the above
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All of the above
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As a 4-10 solar mass star leaves the main sequence on its way to becoming a red supergiant, its luminosity
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remains roughly constant.
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Which of the following best describes the evolutionary track of the most massive stars?
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Horizontal right
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If it gains sufficient mass, a white dwarf can become a
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type I supernova.
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For a white dwarf to explode entirely as a Type I supernova, it's mass must be
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1.4 solar masses, the Chandrasekhar Limit
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The heaviest nuclei of all are formed
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in the core collapse that set the stage of Type II supernovae.
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The Chandrasekhar limit is
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the upper mass limit for a white dwarf.
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Where was supernova 1987a located?
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in our companion galaxy, the Large Magellanic Cloud
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Which of these events is not possible?
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white dwarfs and companion stars producing recurrent Type I supernova events
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Which of these does not depend on a close binary system to occur?
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a Type II supernova
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What can you conclude about a Type I supernova?
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It was originally a low-mass star.
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A recurrent nova could eventually build up to a
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Type I supernova
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The brightest stars of a young open cluster will be
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massive blue main sequence stars.
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Noting the turnoff mass in a star cluster allows you to determine its
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age
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Compared to a cluster containing type O and B stars, a cluster with only type F and cooler stars will be
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older
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Which stars in globular clusters are believed to be examples of mergers?
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blue stragglers
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What made supernova 1987a so useful to study? A. We saw direct evidence of nickel to iron decay in its light curve. B. Its progenitor had been observed previously. C. In the Large Magellanic Cloud, we already knew its distance. D. It occurred after new telescopes, such as Hubble, could observe it very closely. E. All of these are correct.
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All of these are correct.
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While more massive than most of its neighbors, the Sun is still technically a low mass star.
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true
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A massive star can fuse only up to the element silicon in its core.
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False
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Because they all involve formation of iron in cores of massive stars, all type II supernovae are equally luminous.
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False
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Because they all involve the detonation of a carbon-rich white dwarf at Chandrasekhar's limit, all type I supernovae are equally luminous.
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True
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Novae are more closely related to type II than to type I supernovae.
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False
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A carbon-detonation supernova starts out as a white dwarf in a close binary system.
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True
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Most of the energy released during a supernova is emitted as neutrinos.
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True
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Which of these is true of planetary nebulae?
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They are ejected envelopes surrounding a highly evolved low-mass star.
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Compared to our Sun, a typical white dwarf has
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about the same mass and a million times higher density.
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Which of these evolutionary paths is the fate of our Sun?
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Planetary Nebula
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Black dwarfs are
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not found yet; the oldest, coldest white dwarf in the Galaxy has not cooled enough yet.
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About 90% of the star's total life is spent on the main sequence.
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True
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Paradoxically, while the core of the red giant is contracting and heating up, its radiation pressure causes its photosphere to swell up and cool off.
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True
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A star may undergo two or more red giant expansion stages.
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True
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A star system may undergo two or more nova outbursts.
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True
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Our Sun will eventually become a nova.
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False
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Today the majority of the mass of the universe is already in the form of black dwarfs, the solution to the "dark matter" problem.
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False
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White dwarfs were once the cores of stars that produced planetary nebulae.
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True
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It is the formation of iron in an evolved giant's core that triggers the Type II supernova event.
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True
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In the cores of the most massive stars, the electrons and protons fuse together and form neutrons.
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False
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Elements heavier than iron are formed mainly in supernovae.
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True
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Supergiants are burning different fuels in several shells around the core.
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True
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A star system can become a Type I supernova several times.
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False
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Neutrinos can move faster than c, the speed of light, as was discovered in SN1987A in 1987.
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False
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The spectra of the oldest stars show the most heavy elements.
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False
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As a clump of interstellar gas contracts to become a main-sequence star, its changing position on the H-R diagram tells us __________.
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how its outward appearance is changing
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Watch the red dot representing the protostar in the animation. After it reaches its highest point on the diagram, how do the protostar's surface temperature and luminosity change as it approaches the main sequence?
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Its surface temperature increases, but its luminosity decreases.
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When does a newly forming star have the greatest luminosity?
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when it is a shrinking protostar with no internal fusion
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When a newly forming star is at its greatest luminosity, what is its energy source?
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gravitational contraction
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How do the properties of long-lived stars compare to those of short-lived stars?
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Long-lived stars begin their lives with less mass and a smaller amount of hydrogen fuel. Long-lived stars are less luminous during their main-sequence lives.
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A main-sequence star twice as massive as the Sun would last __________.
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much less than half as long as the Sun
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If stars A and B are both main-sequence stars and star A has a greater fusion rate than star B, which of the following statements hold(s)?
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Star A must be more luminous than star B. Star A must be more massive than star B.
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The formation of the first high-mass stars in a collapsing cloud tends to inhibit further star formation within that cloud.
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True
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A protostar that will eventually turn into a star like the Sun is significantly
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More luminous
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Interstellar matter is quite evenly distributed throughout the Milky Way Galaxy.
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False
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Twenty-one-centimeter radiation observations can be used to probe the interiors of molecular clouds.
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False
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More massive stars form more rapidly.
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True
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Brown dwarfs take a long time to form, but will eventually become visible as stars on the lower main sequence.
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False
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Most stars form as members of groups or clusters.
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True
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A dark interstellar globule is about the same size as
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The Oort Cloud
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Of the following telescopes, the one best suited to observing dark dust clouds is
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A radio telescope
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Interstellar gas is composed of
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90% hydrogen, 9% helium by weight.
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What effect does even thin clouds of dust have on light passing through them?
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It dims and reddens the light of all more distant stars.
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Which statement about the dark nebulae is true?
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They can be penetrated only with longer wavelengths such as radio and infrared.
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Some regions along the plane of the Milky Way appear dark because
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stars in that region are hidden by dark dust particles.
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Due to absorption of shorter wavelengths by interstellar dust clouds, distant stars appear
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redder
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Which statement is true about the interstellar medium?
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We know more about the gas than the dust.
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The spectra of interstellar gas clouds show that they have the same basic composition as
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Stars
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Emission nebulae like M42 occur only near stars that emit large amounts of
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Ultraviolet Radiation
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What is the primary visible color of an emission nebula?
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red due to ionized hydrogen atoms
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The density of interstellar dust is very low, yet it still blocks starlight because
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the dust particles are about the same size as the light waves they absorb.
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The gas density in an emission nebula is typically about how many particles per cc?
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Hundred
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What two things are needed to create an emission nebulae?
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hot stars and interstellar gas, particularly hydrogen
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A large gas cloud in the interstellar medium that contains several type O and B stars would appear to us as
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an emission nebula.
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Which of these is not a consequence of dust in the interstellar medium?
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red light from the emission nebulae
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Why are dark dust clouds largely misnamed?
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They contain much more gas than dust.
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Complex molecules in the interstellar medium are found
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primarily in the dense dust clouds.
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Interstellar dust clouds are best observed at what wavelength?
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Radio and infrared
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When an electron in H changes its spin from the same to the opposite direction as the proton, it
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emits a radio wave photon.
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A newly formed protostar will radiate primarily at which wavelength?
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infrared
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During a protostar's T Tauri phase, it
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may develop very strong winds.
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Which statement about the stages of starbirth is false?
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nuclear reactions begin in the core by stage 4.
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On an H-R diagram, a protostar would be
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above and to the right of the main sequence.
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A cloud fragment too small to collapse into a main sequence star becomes a
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Brown dwarf
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How long does it take an M class star to reach the main sequence, compared to a solar type star?
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about twenty times longer
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All globular clusters in our Milky Way are about how old?
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Around ten billion years old
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What are the characteristics of an open cluster of stars?
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a few hundred, mainly main sequence stars
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Which is characteristic of globular star clusters?
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old age and hundreds of thousands of stars, only about 30 ly wide
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Most stars in our part of the Galaxy are formed
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in open clusters of a few dozen.
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There is as much mass in the voids between the stars as in the stars themselves.
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True
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Interstellar matter is distributed very evenly through the galaxy.
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False
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The gas in the interstellar medium consists of mostly heavy elements.
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False
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Molecular clouds are much warmer than typical interstellar gas clouds.
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False
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Dark nebulae are opaque to all wavelengths of electromagnetic radiation.
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False
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The 21 cm line of hydrogen is strongly absorbed by interstellar dust.
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False
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What information does 21-cm radiation provide about the gas clouds?
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their motion; their distribution; their density; their temperature
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Light from distant stars that must pass through dust arrives bluer than when it left its star.
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False
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The predominant color of emission nebula is blue.
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False
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Emission nebulae get their red color from the red supergiants forming in them.
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False
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Dark dust clouds are optically invisible, but give off radio energy.
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True
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Dark dust clouds are cooler than their surroundings.
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True
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Globular clusters are typically much older than open clusters.
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True
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Globular clusters contain mostly blue stars.
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False
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Compared to a main-sequence star with a short lifetime, a main-sequence star with a long lifetime is __________.
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less luminous, cooler, smaller, and less massive
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Compared to a high-luminosity main-sequence star, stars in the upper right of the H-R diagram are
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Cooler and larger in radius
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Compared to a low-luminosity main-sequence star, stars in the lower left of the H-R diagram are
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Hotter and smaller in radius
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Red giants are very bright because they are extremely hot.
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False
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Star A appears brighter than star B, as seen from Earth. Therefore, star A must be closer to Earth than star B.
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False
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The radius of a star can be indirectly determined if the star's distance and luminosity are known.
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False
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Astronomers can distinguish between main-sequence and giant stars purely by spectroscopic means.
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True
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In a spectroscopic binary, the orbital motion of the component stars appears as variations in the overall apparent brightness of the system.
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False
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From a distance of 1 parsec, the angular size of Earth's orbit would be
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2 arc seconds
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Compared with a star of absolute magnitude -2 at a distance of 100 pc, a star of absolute magnitude 5 at a distance of 10 pc will appear
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Fainter
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Stars of spectral class M do not show strong lines of hydrogen in their spectra because
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their surfaces are so cool that most hydrogen is in the ground state.
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Cool stars can be very luminous if they are very
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Large
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The mass of a star may be determined
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by studying its orbit around a binary companion.
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If a star has a parallax of 0.05", then its distance in light years is about:
answer
65 light years
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Which statement about stellar motion is incorrect?
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Like parallax, proper motion is measured over intervals of exactly six months.
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What physical property of a star does the spectral type measure?
answer
Temperature
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The star's color index is a quick way of determining its:
answer
Temperature
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On the H-R diagram, the Sun lies
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about the middle of the main sequence.
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On the H-R diagram, white dwarfs lie Sirius B and Procyon B lie
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at lower left
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On the H-R diagram, red supergiants like Betelguese lie
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at top right
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Which type of binary can have their sizes measured directly by photometry?
answer
eclipsing
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In what range of masses are most stars found?
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0.1 to 2 solar masses
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The nearest star to our Sun, Alpha Centauri, is still over a parsec distant.
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True
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A type B9 star is hotter than a type A0.
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True
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The vast majority of stars near us would fall to the bottom right on the H-R diagram.
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True
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A star's absolute magnitude is its apparent brightness as seen from
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33 light years distant
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What can be said with certainty about a red star and a blue star?
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The blue star is hotter than the red star
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The H-R diagram can plot
answer
temperature vs luminosity
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On the H-R diagram, the bright blue stars that dominate the naked-eye sky lie
answer
at the top left.
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A star near the lower right of the H-R diagram is likely to be
answer
red with low luminosity
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Binary stars separated enough to be resolved in a telescope are called
answer
visual binaries
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A parsec is about 3.3 light years.
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True
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Less than 100 stars lie within 5 parsecs of the Sun.
answer
True
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Our nearest stellar neighbor is a little less than 1 parsec away.
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False
question
A type B star is bluer than a type G star.
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True
question
Only A type stars show hydrogen lines in their spectra.
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False
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White dwarfs lies on the lower left portion of the H-R diagram.
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True
question
Our Sun lies about the middle of the main sequence and the H-R diagram.
answer
True
question
Main sequence stars are fusing hydrogen into helium in their cores.
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True
question
The mass of a newly formed star will determine its position on the main sequence.
answer
True
question
Most stars are single stars like our own.
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False
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In describing other stellar properties, almost everything is relative to our Sun.
answer
True
question
In which of the following layers of the Sun does nuclear fusion occur?
answer
Core
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Which of the following layers of the Sun can be seen with some type of telescope? Consider all forms of light, but do not consider neutrinos or other particles.
answer
Corona, Photosphere, Chromosphere
question
Nuclear fusion of hydrogen into helium occurs in the ____
answer
Core
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Energy moves through the sun's ______________ by means of the rising of hot gas and falling of cooler gas.
answer
Convection Zone
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Nearly all the visible light we see from the Sun is emitted from the ___________.
answer
Photosphere
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Most of the Sun's ultraviolet light is emitted from the narrow layer called the ____________ where temperature increases with altitude.
answer
Chromosphere
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We can see the Sun's _________ most easily during total solar eclipses
answer
Corona
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The ______________ is the layer of the Sun between its core and convection zone
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Radiation Zone
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The most abundant element in the Sun is hydrogen.
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True
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The density and temperature in the solar corona are much higher than in the photosphere.
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False
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Sunspots appear dark because they are hotter than the surrounding gas of the photosphere.
answer
False
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Flares are caused by magnetic disturbances in the lower atmosphere of the Sun.
answer
True
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The proton-proton chain releases energy because mass is created in the process.
answer
False
question
Neutrinos have never been detected experimentally.
answer
False
question
Compared with Earth's diameter, the Sun's diameter is about
answer
100 times larger
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The Sun spins on its axis roughly once each
answer
month
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If astronomers lived on Venus instead of on Earth, the solar constant they measure would be
answer
Larger
question
A typical solar granule is about the size of
answer
Large U.S. State
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The time between successive sunspot maxima is about
answer
Decade
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The primary source of the Sun's energy is
answer
fusion of light nuclei to make heavier ones
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From inside out, which is in the correct order for the structure of the Sun?
answer
radiative zone, convective zone, chromosphere
question
How long does the sunspot cycle last, on average?
answer
11 years
question
Visible sunspots lie in the
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granulation in the photosphere.
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As the Sun rotates, an individual sunspot can be tracked across its face. From eastern to western limb, this takes about
answer
2 weeks
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The most striking example of solar variability was the
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Maunder Minimum from 1645-1715.
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Sunspots
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come in pairs, representing the north and south magnetic fields.
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During a period of high solar activity, the corona
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Is more irregular
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Sunspots are dark splotches on the Sun. Which statement is true?
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They are extremely hot, but cooler than the surrounding areas of the Sun.
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Suppose a large flare is detected optically. How long until radio interference arrives?
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Simultaneously
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While observing the Sun, you note a large number of sunspots. What can you conclude?
answer
There are likely to be an above average number of flares and prominences.
question
What natural barrier tries to prevent two protons from combining?
answer
electromagnetic repulsion
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The critical temperature to initiate the proton-proton cycle in the cores of stars is:
answer
10 Million K
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In the proton-proton cycle, the helium atom and neutrino have less mass than the original hydrogen. What happens to the "lost" mass?
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It's converted to energy
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The primary source of the Sun's energy is
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the strong force fusing hydrogen into helium.
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In the proton-proton cycle, the positron is
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An anti-electron
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Which is the net result of the proton-proton chain?
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4 protons = 1 helium 4 + 2 neutrinos + gamma rays
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The photosphere is about 100 times the diameter of the Earth, and large sunspots are larger than our whole planet.
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True
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Granulation is the most obvious proof of solar convective energy transport.
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True
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The solar corona is much cooler than the Sun's surface, hence we must wait for a total solar eclipse to glimpse it with the naked eye.
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False
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What is the meaning of the solar constant?
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the amount of energy the Earth receives per unit area and unit time
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The density of the Sun is most similar to which object?
answer
Jupiter
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Which of these are not associated with the active Sun? aurora flares sunspots prominences granulation
answer
Granulation
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The outward pressure of hot gas in the Sun
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is balanced by the inward gravitational pressure.
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The Sun's radius is one astronomical unit by definition.
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False
question
The Sun's structure is uniform throughout its interior, with no evidence of different layers.
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False
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The Sun's magnetic field is very weak compared to Earth's.
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False
question
Sunspots usually come in pairs, each a magnetic pole.
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True
question
The sunspot cycle averages about 11 months.
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False
question
Although sunspots are cooler areas in the photosphere, an increase in their number tells us the Sun is becoming more active.
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True
question
The solar corona is best studied using X-ray telescopes.
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True
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The solar neutrinos observed on Earth come from the hot spots in the corona.
answer
False
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The Sun produces energy by fusing hydrogen into helium.
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True
question
During the fusion process, mass is converted into energy.
answer
True
question
The Solar Neutrino Problem is that we observe more neutrinos than predicted.
answer
False
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