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twinkling
starlight
nuclear reactions inside a
star heat the star up from
the center, causing it to
emit light and heat from its
surface. a star appears to
flicker or twinkle because
its light passes through
Earth’s atmosphere, which
is a constantly shifting
blanket of gases. seen from
a traveling spacecraft, stars
shine steadily because
there is no surrounding
atmosphere to disturb
the path of the light.
Constellations
Modern astronomers group stars into
88 constellations. Each has a latin
name, such as Ursa Major (the
great Bear), or Corona australis
(the southern Crown). the “sun
signs” of astrology have the same
names as the 12 constellations of
the zodiac—the band of sky along
which the sun and planets appear to
pass during the course of a year.
VariaBlE stars
Many stars, called variable stars, appear to vary in
brightness. some stars constantly swell and shrink,
becoming alternately fainter and brighter. Other variables
are really two stars that circle each other and block off
each other’s light from time to time.
Double stars circle around each other.
When one star is in front of the other, the
brightness dims. When both stars can be
seen, the brightness increases.
Some variable stars are produced
by exploding stars. The
explosion makes the star
appear much brighter than
usual for a period that can last
from a few days, to a few years.
star qUalitiEs
the color of a star’s light corresponds to the surface
temperature of the star: red stars are the coolest, blue stars
are the hottest. a star’s brightness (the amount of energy
it gives out) is linked to its mass (the amount of material it
contains): heavier stars are brighter than lighter stars.
astronomers can use the color and brightness of the
light emitted from a star to help calculate its size and
distance from Earth.
Parallax
astronomers use a
technique called parallax
to measure the distance of
a star from Earth. as Earth
moves around the sun, the
closest stars seem to move
very slightly compared
with stars farther away.
astronomers measure the
position of a star once, and
then again six months later.
From their measurements
they can then calculate the
distance of a star.
star BrightnEss
a star’s brightness is called its
magnitude. the brightest
magnitudes are the smallest
numbers, so magnitude 1 stars
are brighter than magnitude 2
stars. how bright a star looks
depends on its distance and
how much light it emits.
Neutron stars
(pulsars) are the
smallest stars. They
have about the same
mass as the sun, but
are only about
10 miles (16 km)
in diameter.
White dwarfs are
small stars at the
end of their life;
some are smaller
than Earth.
Giants have
diameters between
100 and 1,000
times larger than
that of the sun.
Supergiants are the largest
stars, with diameters up to
1,000 times that of the sun.
Yellow dwarfs, or
medium-sized stars,
are about the same
size as the sun.
astronomy
Black holes
gravity
navigation
Planets
sun
telescopes
Universe
When the constellation of Orion (above) is in the
night sky, it can be seen from anywhere on Earth.
Apparent position of nearby star when viewed from B Distant star
Apparent position of
nearby star when
viewed from A
Angle of parallax
gives distance
of star.
Earth in position
for second
measurement, six
months later (B)
Sun
Earth in position for
first measurement (A)
stars
Find out more
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