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Earth
& Mars
Using Math
to Compare
Planets
By Bob Albrecht and Paul Davis
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Bob and Paul present questions and
investigations
to help compare Earth and Mars in terms of mass, size,
shape, volume,
density, rotation speeds, gravity, and so on.
Web Resources
Note. These Web sites were
valid when
this issue of L&L went to press. We have
no control
over these sites, though, and the Web is very volatile.
Please let
us know if you find a broken link, and well do our
best to
update it.
National
Space Sciences Data Center: http://nssdc.gsfc.nasa.gov
The
Mars Fact Sheet: http://nssdc.gsfc.nasa.gov/planetary/factsheet/marsfact.html
Starship
Gaia E-Mail Newsletter
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subscribe to Starship Gaia, send an e-mail request to DragonFun@aol.com.
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newsletter.
Problems
- Calculate
the ratio of Marss mass to Earths and
compare your
answer to the ratio shown in Table 1.
- What
is the equatorial diameter of Mars? of
Earth?
- What
is the polar diameter of Mars? of Earth?
- Investigation.
Why are the equatorial diameters of Mars and Earth
greater than
their polar diameters?
- In
circumnavigating Earth along the equator, how far do
you walk
and swim?
- In
circling Earth along a meridian, how far do you
snowshoe, walk,
and swim?
- Investigation.
In circumnavigating Earth, what countries do you pass
through?
What oceans, lakes, and rivers do you cross? What
mountains
do you climb? What towns and cities do you travel
through?
- You
go to Mars and lope around its equator. How far do you
travel?
- Still
fresh as a daisy, you circumnavigate Mars along a
meridian.
This takes you across both the north and south polar
caps. How
far do you walk and snowshoe?
- Investigation.
In circumnavigating Mars, what mountains do you climb?
What
craters do you cross? What valles (sinuous valleys;
singular:
vallis) do you cross? Do you cross any oceans, lakes,
or rivers?
- There
are 360 degrees in a circle. As you circumnavigate a
planet
along its equator or a meridian, you turn through 360
degrees
relative to the planets center. How far (in km)
do you
travel per degree along Earths equator? along an
Earth
meridian?
- How
far (in km) do you travel per degree along Marss
equator?
along a Mars meridian?
- Extra
for the trigonometrically unchallenged: In Shuhaw Hall
at Santa
Rosa Junior College in California, a benchmark is
located at
122ƒ 43' 10" west longitude, 38ƒ 27' 20" north
latitude. If
you go around the meridian, how far do you travel? If
you follow
the latitude until you return to your starting point,
how far
do you travel?
- Make
a table showing:
a.
latitude from 0ƒ to 90ƒ in 10ƒ increments,
b.
radius of each circle of latitude in km,
c.
circumference of each circle of latitude in km, and
d.
distance in km/degree in traveling around each circle
of latitude.
- Do
#14 for Mars.
- The
volumetric mean radius of Mars is 3,390 km. Calculate
the volume
of Mars and compare your answer with the value in Table
1.
- Use
the mass and volume of Mars to calculate its density.
Compare
your answer to the value given in Table
1.
- Convert
1,674 kilometers per hour to meters per second.
(Answer: 465
m/s)
- Suppose
you are standing on Marss equator. How fast are
you traveling
because of the rotation of Mars in kilometers per
hour? in meters
per second?
- Circles
of latitude get smaller as you go from the equator
toward either
pole, but the rotational angular velocity is the same
at every
latitude (well, its zero at a pole). For Earth
or Mars
or both, make a table showing:
a.
latitude from 0ƒ to 90ƒ in 10ƒ increments, and
b.
the speed at which you are traveling at that latitude
in kilometers
per hour and meters per second.
- Using
the mass and polar radius given in Table
1, calculate Earths gravity at its
poles.
- Calculate
Marss gravity at its equator and at its
poles.
- Using
Earths solar irradiance, the Mars-to-Earth
distance from
the Sun ratio (1.5), and the inverse square
relationship, calculate
the solar irradiance on Mars and compare your answer
with the
value given in Table
1.
- If
a solar cell array can convert 15% of the solar
irradiance to
electricity, how many watts per square meter will it
produce
on Earth? on Mars?
- Investigation.
Where on Mars is water likely to be found and how can
it be
obtained?
- Investigation.
How can water (H2O) be split into hydrogen
(H) and
oxygen (O)?
- Investigation.
How much oxygen does an average human adult consume
per Martian
solar day (24h 39m 35s)? How much water? How can this
oxygen
and water be recycled?
- Investigation.
In a habitat supplied with air that is 20% oxygen, 78%
nitrogen,
1% argon, and 1% water vapor at a pressure of 1,014
millibars,
what is the density of the air in kilograms per cubic
meter?
What is the total mass of the air in a habitat that
has a volume
of 1,000 cubic meters?
- Investigation.
Humans inhale oxygen and exhale carbon dioxide. How
much carbon
dioxide does one human produce per hour? In a closed
environment,
excess carbon dioxide must be removed from the air.
How can
this be done?
- Investigation.
Martians will grow plants for food. Plants consume
carbon dioxide
and give off oxygen. How much carbon dioxide does a
bunch of
plants consume per hour? How much oxygen does it
produce per
hour? Please quantify bunch (e.g., romaine lettuce
with a total
leafy surface area of one meter).
- Investigation.
How can atmospheric carbon dioxide (CO2) be
split
into carbon (C) and oxygen (O)?
- Investigation.
How can methane (CH4) be made from carbon
(C) and
hydrogen (H)? To burn methane as a fuel, what else is
needed?
When methane is burned, what are the exhaust products?
Do they
pollute the atmosphere of Mars?
Table 1. Mars and Earth data adapted
from
the Mars Fact Sheet of the National Space Sciences Data
Center
|
Planetary
Characteristic
|
Mars
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Earth
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Ratio
(Mars/Earth)
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Mass
(1024 kg)
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0.6419
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5.9736
|
0.107
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Volume
(1010 km3)
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16.318
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108.321
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0.151
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|
Equatorial
radius (km)
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3,397
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6,378
|
0.533
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|
Polar
radius (km)
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3,375
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6,356
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0.531
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|
Volumetric
mean radius (km)
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3,390
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6,371
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0.532
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Mean
density (kg/m3)
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3,933
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5,515
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0.713
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Surface
gravity (m/s2)
|
3.69
|
9.78
|
0.377
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Sidereal
rotation period (h)
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24.6229
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23.9345
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1.029
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Synodic
rotation period (h)
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24.6597
|
24.0000
|
1.029
|
|
Solar
irradiance (W/m2)
|
595
|
1,368
|
0.431
|
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Bob Albrecht (dragonfun@aol.com)
is a writer and developer of science, math, and
technology
curricula. George Firedrake is his alter ego and
takes the
form of a dragon. Laran Stardrake, whose quotes
sometimes
lead off this column, is another of Bobs
accomplices.
Shes half-dragon and half-human. As Laran is
fond of
saying, Reality expands to fill the available
fantasies.
The DragonFun image is from an original painting by
Marcy
Kier-Hawthorne.
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Paul Davis (ctec1@mchs.srcs.k12.ca.us)
is a mathematics teacher at Maria Carrillo High
School in
Santa Rosa, California. He was a happy, normal
teacher until
he met Bob Albrecht and George Firedrake in 1992 and
became
another one of their accomplices. Since then, Paul
has been
intertwingling math, science, and technology in his
classroom
with the help of Bob and George.
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Copyright © 2000, ISTE (International
Society for Technology in Education).
All rights reserved.
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