Landsat 7 Education Activity
Finding Impact Craters with Landsat
Student Name: ____________________________________
Class Period: _____________________________________
Date: ___________________________________________
Student
Worksheet for Step 1:
When an Extraterrestrial Object Hits the Earth
You wouldn't hear it coming. A 100-ton extraterrestrial object
hits the Earth at hypervelocity, more than 11 kilometers per second,
and sometimes as fast as 20-25 km/sec. (Smaller objects slow down
or are destroyed because of air resistance.) That's faster than sound
(about 300 m/sec).
The object comes to a stop in about one hundredth of a second.
1. There is a rapid release of a tremendous amount of kinetic energy.
What would be the effect of that rapid release of energy on the solid
earth, the air, and living things? What forms might that energy take,
and where might it go? Respond here:
Effects on rocks and soil: ________________________________________________________
____________________________________________________________________________
____________________________________________________________________________
Effects on the shape of
the land (topography): ________________________________________
____________________________________________________________________________
____________________________________________________________________________
Effects on the air: ________________________________________________________
____________________________________________________________________________
____________________________________________________________________________
Effects on living things:
________________________________________________________
____________________________________________________________________________
____________________________________________________________________________
2. The energy release creates
a shockwave stronger than any material it hits. What could be the
effects of that shockwave on the rocks and soil, and on large bodies
of water? Respond here:
____________________________________________________________________________
____________________________________________________________________________
3. What would be the effects
of impact on the object itself? Would it remain intact (in one piece)?
Respond here:
____________________________________________________________________________
____________________________________________________________________________
Download PDF
of this worksheet.
Landsat 7 Educational Activity
Finding Impact Craters with Landsat
Student Name: _______________________________
Class Period: ________________________________
Date: _______________________________________
Student
Reading for Step 2:
Known Effects of Impact Events
When an object from space hits the Earth
- There's a huge explosion.
- The impact makes a big
hole or crater with a raised rim and sometimes a central peak.
The hole is many times larger than the impacting object.
- There is a rapid release
of a tremendous amount of kinetic energy as the object comes to a
stop in about one hundredth of a second.
- The impact releases extreme
heat. Usually, the object itself is vaporized. Sometimes it melts
completely and mixes with melted rocks at the site.
- If the impact occurs in
water, a whole column of water is vaporized.
- The impact also produces
a super-hot blastwave a shockwave that radiates rapidly
outward from the impact point through the target rocks at velocities
of a few kilometers per second.
The shockwave is stronger than any material on Earth. It deforms rock
in ways that are characteristic of an impact event. No other event
on Earth deforms rock in these ways.
- Tiny glass droplets can
form during the rapid cooling of molten rock that splashes into the
atmosphere.
- Large impacts also crush,
shatter, and/or fracture the target rocks extensively beneath and
around the crater. See diagram at: http://craters.gsfc.nasa.gov/crater_diagram.html
- Hot debris is ejected
from the target area, and falls in the area surrounding the crater.
Close to the crater, the ejecta typically form a thick, continuous
layer. At larger distances, the ejecta may occur as discontinuous
lumps of material.
- Large impact events can
blow out a hole in the atmosphere above the impact site, permitting
some impact materials to be dispersed globally by the impact fireball,
which rises above the atmosphere. The resulting extensive dusk and
smoke clouds can cause darkness lasting for a year.
- Special carbon molecules
called Buckminsterfullerene
or (Bucky-balls, after Buckminster Fuller) can travel to the Earth
in the impactor. They can hold special gases called "noble"
gases that are indicators of extraterrestrial origin.
- Large impacts can trigger
earthquakes and initiate volcanic eruptions.
- The heat ignites fires,
and they may rage across a large region.
- Impact events can alter
the chemical composition of the atmosphere. The extreme heat can generate
large amounts of nitrogen oxides (NOx). NOx is easily transformed
into nitric acid, resulting in acid rain.
More About
...
More About Impact Events
in General
Impact craters
are geologic structures formed when a large meteoroid, asteroid or
comet smashes into a planet or a satellite.
A very large number of
meteoroids enter the Earth's atmosphere each day, amounting to more
than a hundred tons of material. They are almost all very small, just
a few milligrams each. Only the largest ones ever reach the surface.
The average meteoroid enters the atmosphere at between 10 and 70 km/sec.
All but the very largest are quickly decelerated to a few hundred
km/hour by atmospheric friction, and they hit the Earth's surface
with very little fanfare. However meteoroids larger than a few hundred
tons are slowed very little; only these large (and fortunately rare)
ones make craters.
All the inner bodies in
our solar system have been heavily bombarded by meteoroids throughout
their history. The surfaces of the Moon, Mars and Mercury, where other
geologic processes stopped millions of years ago, record this bombardment
clearly. On the Earth, however, which has been even more heavily impacted
than the Moon, craters are continually erased by erosion and redeposition
as well as by volcanic resurfacing and tectonic activity. Thus only
about 120 terrestrial impact craters have been recognized, the majority
in geologically stable areas of North America, Europe and Australia.
Spacecraft imagery has helped to identify structures in more remote
locations that can be explored for positive identification.
More About the Energy
Released by Impact
Energies of impact
are almost incomprehensibly large. They come chiefly from the kinetic
energy of the impacting object. An object only a few meters across
carries the kinetic energy of an atomic bomb as it strikes another
object at high velocity. The impact of an object only a few kilometers
across (smaller than many known asteroids and comets) can release
more energy in seconds than the whole Earth releases (through volcanism,
earthquakes, tectonic processes, and heat flow) in hundreds or thousands
of years.
More About Extraterrestrial
Objects in the Solar System
Thousands, possibly
millions, of objects move throughout the solar system, orbiting the
Sun. They range from microscopic dust particles to objects tens of
kilometers across. Each object moves in its own orbit. We don't know
how often they have hit the Earth in the past.
More About Impact Velocity
The minimum impact velocity for collisions with Earth is 11.2 km/s.
This is equal to the escape velocity for an object launched into space
from Earth's surface.
More About the Sizes of Craters
Objects of less than half a kilometer in diameter can make craters
10 km in diameter.
More About Crater Shapes
Nearly all impact events result in circular craters. In rare cases
where the angle of impact was very low (0-10 degrees from the plane
of the horizon), craters can be ovoid in shape.
More About Finding Impact Craters on the Ground
When looking for impact craters in satellite images, first pay attention
to circular features in topography or bedrock geology. Look for lakes,
rings of hills, or isolated circular areas.
On the ground, look for
changes in the physical properties of the rocks in and around impact
structures. Fractured rock is less dense than unaltered target rock
around the structure. Also look ejecta and shocked rock fragments
on the original ground surface outside the crater, and for fragments
of the meteorite.
Download PDF of
this worksheet.
Landsat 7 Educational
Activity
Finding Impact Craters with Landsat
Student Name: __________________________________
Class Period: ___________________________________
Date:_________________________________________
Student
Worksheet for Step 4:
Describing Satellite Images of Possible Impact Craters
Part I. Consider what effects an impact event might have, and
describe those effects below. Though you are working in groups for
this step of the activity, each student must complete this worksheet.
A. The object itself: Would you expect to see any evidence
of the object itself in a satellite image? What evidence might you
find?
_________________________________________________________________________________________
_______________________________________________________________________________________
B. Shape of the land: What kinds of changes would that impact make
to the shape of the land where it hit, and all around?
_________________________________________________________________________________________
_________________________________________________________________________________________
C. Effects of Time: What kinds of changes will occur to the impact
site over time? Remember that some changes are fast, and some are
slow.
_________________________________________________________________________________________
_________________________________________________________________________________________
D. What else might you see in these satellite images that could help
you learn about an impact crater?
________________________________________________________________________________________
_________________________________________________________________________________________
_________________________________________________________________________________________
Part II. As a group,
study all of the satellite images. Below are their fake names
(to use until you've identified them yourselves as impact craters
or something else):
AOR
Latitude: N 19° 6'
Longitude: E 19° 15'
Size: 12.6 km in diameter
ELG
Latitude: N 67° 30'
Longitude: E 172° 5'
Size: 18 km in diameter
HGH
Latitude: N 75° 22'
Longitude: W 89° 41'
Size: 20 km in diameter
MAN
Latitude: N 51° 23'
Longitude: W 68° 42'
Size: 72 km in diameter
MSH
Latitude: N 46° 16'
Longitude: W 122° 12'
Size: several km in diameter
RCH
Latitude: 21°04'N
Longitude: 11°22'W
Size: 38 km in diameter
SCH
Latitude: N 37° 20' 36.1"
Longitude: W 116° 33' 59.9"
Size: About 300 m in diameter
You need to know
that
All of these satellite
images show the Earth's land surface, not another planet's surface,
and not the Earth's atmosphere. No hurricanes or tornadoes appear
in these images.
The colors in
these images are false colors. White isn't always snow; lakes often
appear black; vegetation is sometimes red.
All of these landforms
are large. One is 300 m in diameter, and the others are 1 km in
diameter or larger. Most of them 10-90 km in diameter.
Aliens from other
parts of the universe had nothing to do with creating the landforms
in these images.
If you see a letter
or a face, it's just an accident of nature.
People sometimes
make large craters with explosives or large mining equipment.
Multiple Impacts:
Sometimes impacts come in twos or threes. It's rare, but it can
happen when a comet or asteroid breaks into a couple of large pieces
just before it strikes the Earth.
Part III. As a group,
now choose two of the images you find most interesting, and prepare
to describe them to the class as directed by your teacher.
A. Circle the name or names of the one or two landform(s) your group
has chosen to describe for the class. Write next to it if you think
it is an impact crater or some other kind of landform.
AOR ELG HGH MAN MSH
RCH SCH
B. What evidence
do you see in the satellite image that your landform is or is not
an impact crater? Describe it here:
_______________________________________________________________________________________
_________________________________________________________________________________________
_________________________________________________________________________________________
Come to agreement as a
group about whether or not the image you've chosen is or is not an
impact crater, and why.
Download PDF
of this worksheet.
Landsat 7 Educational Activity
Finding Impact Craters with Landsat
Student Name: _______________________________
Class Period: ______________________________________
Date: _______________________________________
Student
Worksheet for Step 6:
Questions You Would Ask
on a Field Expedition to a Possible Impact Crater
Identifying what might be an impact crater in a satellite image is
only the first step in identifying it with 100 percent certainty.
That requires people making a field expedition to gather and study
evidence at the site itself.
Field expeditions cost money. Getting money nearly always requires
writing excellent grant proposals. You have to prove you understand
the science and know what you're doing before people will give you
the money to do it.
Your task
is to write a series of questions you would use to guide a field expedition
to determine whether or not a given landform was an impact crater.
You will do well on this learning assessment if you:
Show evidence
that you have a full and complete understanding of how an impact
event can shape the land, soil, and surrounding rocks, as well as
the atmosphere and living things;
Use terminology accurately;
Explain your ideas in ways that makes sense;
Use complete sentences.
Download PDF of
this worksheet.
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