Download Stars, Galaxies, and the Universe Section 1

Stars, Galaxies, and the Universe
Section 1: Characteristics of Stars
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• Objectives
• Analyzing Starlight
• The Compositions of Stars
• The Temperatures of Stars
• The Sizes and Masses of Stars
• Stellar Motion
• Distances to Stars
• Light-Year
• Stellar Brightness
• Absolute and Apparent Motion
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Stars, Galaxies, and the Universe
Section 1
Objectives
• Describe how astronomers determine the compositions
and temperature of stars.
• Explain why stars appear to move in the sky.
• Describe one way astronomers measure the distances
to stars.
• Explain the difference between absolute magnitude and
apparent magnitude.
Stars, Galaxies, and the Universe
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Analyzing Starlight
• star a large celestial body that is composed of gas and
that emits light.
• Nuclear fusion is the combination of light atomic nuclei to
form heavier atomic nuclei
• Astronomers learn about stars by analyzing the light that
the stars emit.
• Starlight passing through a spectrograph produces a
display of colors and lines called a spectrum.
Stars, Galaxies, and the Universe
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Analyzing Starlight, continued
• All stars have dark-line spectra, which are bands of color
crossed by dark lines where the color is diminished.
• A star’s dark-line spectrum reveals the star’s composition
and temperature.
• Stars are made up of different elements in the form of
gases.
• Because different elements absorb different wavelengths
of light, scientists can determine the elements that make
up a star by studying its spectrum.
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The Compositions of Stars
• Scientists have learned that stars are made up of the
same elements that compose Earth.
• The most common element in stars is hydrogen.
• Helium is the second most common element in stars.
• Small quantities of carbon, oxygen, and nitrogen are also
found in stars.
Stars, Galaxies, and the Universe
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The Temperatures of Stars
• The temperature of most stars ranges from 2,800˚C to
24,000˚C.
• Blue stars have average surface temperatures of
35,000˚C.
• Yellow stars, such as the sun, have surface
temperatures of about 5,500˚C.
• Red stars have average surface temperatures of
3,000˚C.
Stars, Galaxies, and the Universe
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The Sizes and Masses of Stars
• Stars vary in size and mass.
• Stars such as the sun are considered medium-sized
stars. The sun has a diameter of 1,390,000 km.
• Most stars visible from Earth are medium-sized stars.
• Many stars have about the same mass as the sun,
however, some stars may be more or less massive.
Stars, Galaxies, and the Universe
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Stellar Motion
Apparent Motion
• The apparent motion of stars is the motion visible to the
unaided eye. Apparent motion is caused by the
movement of Earth.
• The rotation of Earth causes the apparent motion of
stars to be as though the stars are moving counterclockwise around the North Star.
• Earth’s revolution around the sun causes the stars to
appear to shift slightly to the west every night.
Stars, Galaxies, and the Universe
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Stellar Motion, continued
Reading Check
Why does Polaris appear to remain stationary in the night
sky?
Polaris is almost exactly above the pole of Earth’s
rotational axis, so Polaris moves only slightly around the
pole during one rotation of Earth.
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Stellar Motion, continued
Circumpolar Stars
• Some stars are always visible in the night sky. These
stars never pass below the horizon.
• In the Northern Hemisphere, the movement of these
stars makes them appear to circle the North Star.
• These circling stars are called circumpolar stars.
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Stellar Motion, continued
Actual Motion of Stars
• Most stars have several types of actual motion.
• Stars rotate on an axis.
• Some stars may revolve around another star.
• Stars either move away from or toward our solar system.
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Stellar Motion, continued
Actual Motion of Stars
• Doppler effect an observed change in the frequency of
a wave when the source or observer is moving
• The spectrum of a star that is moving toward or away
from Earth appears to shift, due to the Doppler effect.
• Stars moving toward Earth are shifted slightly toward
blue, which is called blue shift.
• Stars moving away from Earth are shifted slightly toward
red, which is called red shift.
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Stellar Motion, continued
The spectrum of a star that is moving toward or away from
Earth appears to shift, as shown in the diagram below.
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Distances to Stars
• light-year the distance that light travels in one year.
• Distances between the stars and Earth are measured in
light-years.
• parallax an apparent shift in the position of an object
when viewed from different locations.
• For relatively close stars, scientists determine a star’s
distance by measuring parallax.
Stars, Galaxies, and the Universe
Light-Year
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Stars, Galaxies, and the Universe
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Stellar Brightness
• Apparent magnitude the brightness of a star as seen
from the Earth.
• The apparent magnitude of a star depends on both how
much light the star emits and how far the star is from
Earth.
• Absolute magnitude the brightness that a star would
have at a distance of 32.6 light-years from Earth
• The brighter a star is, the lower the number of its
absolute magnitude.
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Stellar Brightness
The lower the number of the star on the scale shown on the
diagram below, the brighter the star appears to observers.
Stars, Galaxies, and the Universe
Absolute and Apparent Motion
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