Download Section 2 Locating Astronomical Objects in the Night Sky

Section 2 Locating Astronomical Objects in the Night Sky
Section 2
Locating Astronomical Objects in the
Night Sky What Do You See?
What Do You See?
Learning Outcomes
Think About It
In this section, you will
When you try to find your way to a new address, what tools or
methods do you use? Do you find some ways of locating new
places more useful to you than others? How do you think it
would be different to find your way to a new place in space?
• Construct a model of the night sky
to understand how star maps work.
• Describe the coordinate system used
to locate objects in the sky.
• Identify patterns in the organization
and distribution of matter in the
universe.
• How do astronomers locate objects in the sky?
Record your ideas about this question in your Geo log. Include a
sketch that demonstrates your ideas. Be prepared to discuss your
responses with your small group and the class.
Investigate
In this Investigate, you will be comparing and contrasting ways of
finding places both on the surface of Earth and in space.
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Chapter 1 Astronomy
On a globe, they form a series of circles
that decrease in size toward the poles.
Latitude lines show locations north
and south of the equator. Lines of
longitude are imaginary lines that run
from the North Pole to the South Pole.
They show locations east and west
of the prime meridian. You will now
sketch latitude lines using a compass,
protractor, and ruler.
Part A: Describing the Locations of
Places on Earth
1. With your group, discuss ways for
locating places on Earth.
a) List all the ways your
group identified.
b) Rank your list from the
most accurate to the least
accurate descriptions.
8. Use a compass to draw a circle 15 cm
in diameter.
2. Use a globe, an atlas, the Internet, or
other sources to find the most precise
location of your school as possible.
9. Draw a horizontal line through the
center of the circle (a diameter).
a) Record the location of your school.
3. Exchange your description with one
from another group.
10. Identify the longitude and latitude
coordinates for your school.
a) How does the accuracy of the other
group’s description compare to yours?
a) Record the longitude and latitude
coordinates for your school.
4. Identify the locations of two places on
Earth that have physical and historical
importance.
11. Use a protractor to draw an angle that
is equal to the latitude coordinate for
your school. Measure the angle along the
horizontal line and from the center of the
circle. Draw the angle from the center of
the circle to the edge of the circle.
a) Record each location on a separate
sheet of paper. Research and describe
in a few sentences the importance of
the physical nature and history of
each place.
5. Exchange your sheets of paper with
those from another group so that your
group has two new places.
6. Locate each new place on a map.
a) Did you have any difficulties finding
each place?
b) What information helped you or
could have helped you in finding the
places on the map?
7. You most likely used longitude and
latitude coordinates to precisely locate
your school and the places of physical
and historical importance on Earth’s
surface. Lines of latitude are imaginary
lines on Earth’s surface that run east
to west and parallel to the equator.
12. Following the same procedure as in Step
11, measure angles from 0° to 90° from the
horizontal, and mark these on the circle.
13. Obtain a globe and a world map.
Examine the lines of latitude on the
globe and map.
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Section 2 Locating Astronomical Objects in the Night Sky
3. Now imagine that you put the glass ball
into a much larger opaque ball without
any markings on it. Your model now
consists of two concentric spheres,
with the opaque sphere at a distance
from the glass sphere. In your Geo
log, sketch what a cross section of this
“sphere within a sphere” would look
like. Again, compare your sketch to
those of others in your group.
a) How do these lines compare to the
lines that you drew on your circle?
b) Describe how lines of longitude are
measured in comparison to lines
of latitude.
Part B: The Celestial Sphere
1. Imagine Earth expanding and becoming
10 times its normal diameter.
a) Could you use the longitude and
latitude coordinate system from
Part A for this larger Earth? Explain
your answer.
2. To create a coordinate system for
locating objects in the sky, you first need
to make an imaginary model of Earth.
Imagine Earth’s core as a glass ball
with two poles and an equator, just like
Earth’s. Think about this ball as having
lines of longitude and latitude just
like those on a globe. These longitude
and latitude lines are opaque, which
means light cannot pass through them.
Think of the glass between the lines as
transparent, which means light can pass
through it.
a) In your Geo log, sketch what this
glass ball might look like. Share it
with others in your group.
b) If you put a light bulb in the center
of the glass ball that radiated light
outward in all directions, and turned
out the lights in the room where the
ball was, what would you see on the
wall and ceiling? Discuss this with
your group.
a) What pattern do you think would be
projected onto the inside of the larger
sphere by the light shining out from
the glass ball? Sketch this pattern.
b) How would this pattern be similar to
the one on the glass ball?
c) How would this pattern be different
from the one on the glass ball?
d) How could you use coordinates
to find objects located on the
larger sphere?
Learning Through Technology
To use online resources to
practice finding objects in
space, go to the EarthComm
Web site at http://www
.agiweb.org/education/earthcomm2/.
There you will be able to explore the ways
in which astronomers locate stars, planets,
and other celestial objects.
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Chapter 1 Astronomy
Digging Deeper
THE CELESTIAL SPHERE
In the Investigate, you explored different ways of locating places on
Earth. You then investigated how you could find objects in space. Locating
objects in space has been a challenge for people for a very long time. For
thousands of years, people from all parts of the planet recognized groups
of stars in the night sky. The Greeks, Egyptians, Babylonians, and others
gave names to the groups of stars. They told stories about them that
allowed for their positions to be learned without needing instruments.
Some scientists think that caves in France may contain drawings of the
night sky from 17,300 years ago.
Figure 1 An ancient star chart showing animals and objects that
represent the constellations.
Geo Words
constellation: a
grouping of stars in
the night sky that
forms a recognizable
pattern.
celestial sphere: an
imaginary sphere
of infinite radius
that projects around
Earth, and whose
interior is inscribed
with a grid system
for taking celestial
coordinates.
There are 88 groupings of stars in the sky. Astronomers call a grouping
of stars a constellation. Each constellation has a Latin name. The name is
given a three-letter abbreviation. For example, Cassiopeia is abbreviated
as Cas. Draco is abbreviated as Dra. Constellations are important reference
points for locating planets and other astronomical objects in the night sky.
Many ancient astronomers thought that the stars were attached to a
giant hollow sphere that surrounded Earth. Astronomers now know
that such a sphere does not exist. Stars are located throughout space at
different distances from Earth. However, the idea of a giant sphere, called
the celestial sphere, is useful. It provides a model on which to place and
locate stars, planets, and other objects in space. The word celestial means
pertaining to the sky. The difference between astronomical objects and
celestial objects is that celestial objects do not include Earth.
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Section 2 Locating Astronomical Objects in the Night Sky
Figure 2 View of the celestial sphere looking toward
the north celestial pole.
To describe the location of an object in the sky, astronomers use a special
reference system. It is known as the celestial coordinate system. This
system is similar to the one used for locating objects on Earth’s surface. It
uses measurements from known reference points or lines. These lines are
similar to lines of longitude and latitude. The main reference line in the
celestial sphere is the celestial equator. It is an imaginary circle created by
extending Earth’s equator into space.
Geo Words
celestial coordinate
system: a coordinate
system for mapping
positions on the
celestial sphere.
longitude: an eastwest measurement of
position on Earth.
latitude: a northsouth measurement
of position on Earth.
celestial equator:
an imaginary circle
created by extending
Earth’s equator into
space; the main
reference line in the
celestial sphere.
Figure 3 Locations on Earth’s surface can be precisely located
using longitude and latitude.
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Chapter 1 Astronomy
Geo Words
declination (dec): a
coordinate used on
the celestial sphere,
just as latitude is used
on Earth.
right ascension (R.A.):
a coordinate used on
the celestial sphere,
just as longitude is
used on Earth.
vernal equinox: the
position of the Sun as
it crosses the celestial
equator into the
Northern Hemisphere
each spring.
The celestial coordinate system uses declination (dec) to measure how far
north or south an object is from the celestial equator. Declination is similar
to latitude. It is measured in degrees. The celestial equator has a declination
of zero degrees. Objects north of the celestial equator have a positive
value. Those south of the celestial equator have a negative value.
On Earth, longitude is measured east or west of the prime meridian. The
prime meridian is located at 0°. It runs through Greenwich, England. Like all
other lines of longitude, it runs north to south. It converges with all other
lines of longitude at the poles. If you look down onto a globe at the North
Pole, you can see the 360° through which Earth rotates every 24 h (hours).
It rotates through an angle of 15° every hour. According to these different
measurements for longitude, the city of Miami, Florida lies 80°, or 5 hours
and 20 minutes, west of the prime meridian. Los Angeles, California lies
118°, or 7 hours and 52 minutes, west of the prime meridian.
In the celestial coordinate system, the lines that correspond to longitude on
Earth are called right ascension (R.A.). Right ascension is measured in hours,
minutes, and seconds, much like lines of longitude can be measured. Right
ascension is slightly more complicated to understand than longitude. Due to
Earth’s counterclockwise rotation, objects appear to move across the sky at
night. Earth’s eastward rotation causes stars to appear to move west. Thinking
about the rising Moon might help you understand how this works. The Moon
appears to rise above the horizon from a given point on Earth’s surface. As
Earth rotates, that point moves away from the Moon, which appears to rise
upward and to the right. Similarly, Earth’s rotation causes the positions of the
stars in the sky to appear to change gradually throughout the night.
Figure 4 The trail of the rising Moon over Seattle.
In order to properly measure right ascension, a fixed point is needed. The
sky lacks a fixed point. Even the stars are moving as they slowly orbit the
center of the galaxy. As a result, astronomers have chosen the point on the
celestial equator where the Sun crosses into the Northern Hemisphere in
spring. This is a point in time known as the vernal equinox. Notice that this
point does not coincide with the point where the prime meridian intersects
the equator.
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Section 2 Locating Astronomical Objects in the Night Sky
The stars seem to travel across the sky at night and the Sun seems to travel
across the sky during the day. While it may appear that these objects are
moving, they are not. The reason for this motion is because Earth rotates
360° about its axis every 24 hours. The points about which the sky seems
to rotate are called celestial poles. One is located above the North Pole
and the other is located above the South Pole. Over time, stars located
near the celestial poles make small circles in the sky. Currently, the star
called Polaris lies very close to the northern celestial pole. It therefore
appears to be almost stationary in the night sky. As a result, this star has
become known as the North Star or Pole Star. It has been of great use
in navigation. The nearest star to the Sun is Proxima Centauri, located at
right ascension 14 hours 38 minutes and declination –60° 46’.
Geo Words
celestial pole: the
point about which the
sky seems to rotate.
Checking Up
Figure 5 Polaris is the Pole Star seen at the center of the concentric rings in this
photograph. The rings are the apparent paths of stars produced by Earth’s rotation
about its axis.
Not all of the stars in the sky can be seen from a single location. A person
viewing stars in the Northern Hemisphere cannot see all the stars visible
in the Southern Hemisphere. Some are located below the horizon. The
stars that can be observed from any given place also vary throughout the
year. As Earth moves around its orbit, the North and South Poles point
toward different parts of the universe. As a result, different constellations
and other celestial objects come into view at different times.
1. What is the main
difference between
a point on Earth’s
grid system
and one on the
celestial system?
2. What is special
about Polaris, the
Pole Star?
3. Why do the
objects you see in
the sky at night
change throughout
the year?
Think About It Again
At the beginning of this section, you were asked the following:
• How do astronomers locate objects in the sky?
Record your ideas about this question now. Be sure that you describe the
celestial coordinate system in your answer.
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Chapter 1 Astronomy
Reflecting on the Section and the Challenge
You used longitude and latitude coordinates to locate your school and two places of
physical and historical importance on Earth’s surface. Drawing your own latitude lines
using a compass, protractor, and ruler helped you to understand how lines of latitude are
drawn on globes and world maps. You then transferred your understanding of coordinate
systems on Earth to developing a coordinate system for locating objects in the sky. You
applied this new system to a model of the night sky. This will help you to describe Earth
and its place in the universe for the Chapter Challenge.
Understanding and Applying
1. Describe the objects in the night sky above your community.
2. How do the objects you can see in the sky at night change during the year?
3. Why is it important for astronomers to make observations of the night sky from
many locations?
4. Explain why you can see above and below the celestial equator.
5. Why is it that new constellations gradually enter our field of view from the east and
the old ones disappear to the west?
6. Preparing for the Chapter Challenge
Continue developing your radio or podcast script for the Chapter Challenge. Explain
the use of the celestial coordinate system in plotting positions in the sky. Use examples
of astronomical objects to illustrate your explanation. Help your audience to understand
how precisely locating objects in the sky helps to identify Earth’s place in the universe.
Inquiring Further
1. Earth’s axial tilt
Over a period of 13,000 years, Earth’s axis wobbles like a spinning top. How does
this affect the relative position of Polaris? Find out more about Earth’s wobble, the
position of Polaris, and stars that have marked the south celestial pole.
2. Using star charts
Get to know your community’s night sky and its movements. The constellations
above the horizon change with time and with the seasons. Use monthly star charts to
examine the evening sky. Hold the chart overhead and turn it to match the direction
you are facing. Which way do the constellations appear to move during an evening?
3. The stories of the stars
Different cultures give the various constellations different names and stories.
Choose three constellations and recount the different cultural stories that have
developed about them.
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