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Compare and contrast stars on the upper left and lower right of the main sequence.

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Stars on the upper left are type O and B. They are hotter, more massive and luminous, have larger radii, are blue- white or white, and have relatively short lifetimes. The hottest, type O, have lines of ionized helium. Stars on the lower right are cooler, less massive and luminous, are smaller and redder, and have very long lifetimes. The coolest have molecular spectral lines.

In the H- R diagram, what are the two most important types of data plotted?


A) absolute and apparent magnitudes
B) spectral classes and absolute magnitudes
C) apparent magnitudes and temperatures
D) luminosities and masses
E) sizes and temperatures

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B

How can Betelgeuse be only half the Sun's surface temperature, yet about 10,000 times more luminous than the hotter Sun?

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It may be cooler, but it is ab...

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To find the _ velocity, we must combine proper motion and parallax data.

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A star has a parallax of 0.01 arc seconds. Its distance is


A) 10 parsecs
B) 100 parsecs.
C) 1 parsec.
D) 0.1 parsecs.
E) 0.01 parsecs.

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Two stars both have parallaxes of 0.023", but star A has apparent magnitude +2.3, while star B is magnitude +7.3. Which statement is true?


A) Star A is both 100× brighter and larger than star B.
B) Star B must be ten times more luminous.
C) Star A must be ten times closer.
D) Star A is both 100× brighter and more luminous than star B.
E) Nothing, since we do not know their absolute magnitudes.

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The ionized helium lines show up only in class stars.


A) M
B) K
C) O
D) B
E) F

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The distance to a star with a parallax angle of 0.2 arc seconds is


A) 0.2 parsec.
B) 2 parsecs.
C) 5 parsecs.
D) 12 parsecs.
E) 20 parsecs.

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C

The stars a Cygni and fi Cygni are in the constellation Cygnus. Which statement is true?


A) a Cygni appears brighter.
B) fi is hotter.
C) fi Cygni appears brighter.
D) a must be the eastern most star in the constellation.
E) fi appears redder.

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What role do molecules play in spectral classification?

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Molecules can only f...

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On the H- R diagram, white dwarfs Sirius B and Procyon B lie


A) at the top right.
B) close to the Sun, near the center.
C) at the lower left.
D) at the lower right.
E) at the top left.

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Which of these stars would be the hottest?


A) M10
B) G2
C) B0
D) A0
E) K9

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In addition to the proper motion, we also need the to find the transverse velocity of a star across our line of sight.


A) temperature
B) parallax
C) composition
D) mass
E) color

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Binary stars separated enough to be resolved in a telescope are called


A) line- of- sight binaries.
B) astrometric binaries.
C) spectroscopic binaries.
D) visual binaries.
E) orbital binaries.

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Stellar masses are measured directly by observations of the motions of


A) eclipsing binary systems.
B) visual binary systems.
C) spectroscopic binary systems.
D) All of the above can give us their masses.
E) Stellar masses cannot be measured directly by any method.

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In the M class stars, we find _ absorption lines not seen in hotter stars.

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A type B star is bluer than a type G star.

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Why is the main sequence main? Why are these stars so common?

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While their masses, luminosities, and te...

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A unique characteristic of type O stars is ionized helium lines in its spectrum.

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A star's absolute magnitude is its apparent brightness as seen from


A) Alpha Centauri.
B) 10 light- years distance.
C) Pluto.
D) 100 parsecs distance.
E) 10 parsecs distance.

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