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ES 2232G: Exploring the Planets: Sun, Earth, Planets
Laboratory 02 – Planetary Atmospheres
(Materials reproduced from the Astronomy Education at the University of Nebraska-Lincoln Web Site
(http://astro.unl.edu).
INTRODUCTION
This lab explores some of the elements that go into the retention or loss of an atmosphere by a
planet. Open a web browser and point to:
http://astro.unl.edu/naap/atmosphere/atmosphere.html
.
Work through the background sections on Escape Velocity, Projectile Simulation, and Speed
Distribution. Then complete the following questions related to the background information.
Question 1:
Imagine that asteroid A that has an escape velocity of 50 m/s. If asteroid B has twice
the mass and twice the radius, it would have an escape velocity ______________ the escape
velocity of asteroid A.
a)
4 times
b)
Twice
c)
the same as
d)
half
e)
one-fourth
Question 2:
Complete the table below by using the Projectile Simulator to determine the escape
velocities for the following objects. Since the masses and radii are given in terms of the Earth’s,
you can easily check your values by using the mathematical formula for escape velocity.
Object
Mass
(Mearth)
Radius
(Rearth)
v
esc
(km/s)
v
esc
(km/s) calculation
(optional)
Mercury
0.055
0.38
4.3
0.055
11.2
4.3
0.38
km
km
s
s
Uranus
15
4.0
21.7
√
(
15
)
(
4.0
)
(
11.2
km
s
)
=
21.1
km
s
Io
0.015
0.30
2.5
√
(
0.015
)
(
0.30
)
(
11.2
km
s
)
= 2.5
km
s
Vesta
0.00005
0.083
0.3
√
(
0.00005
)
(
0.083
)
(
11.2
km
s
)
= 0.3
Earth Sciences 2232G: Lab 02
1
km
s
Krypton
100
10
35.4
√
(
100
)
(
10
)
(
11.2
km
s
)
= 35.4
km
s
Question 3:
Experiment with the Maxwell Distribution Simulator. Then a) draw a sketch of a
typical gas curve below, b) label both the x-axis and y-axis appropriately, c) draw in the estimated
locations of the most probable velocity v
mp
and average velocity v
avg
, and d) shade in the region
corresponding to the fastest moving 3% of the gas particles.
Maxwe
ll Speed Distribution
Earth Sciences 2232G: Lab 02
Number of Particles
Average
Velocity
Most probable velocity
Particle Speeds
Fastest
3%
2
GAS RETENTION SIMULATOR
Open the
gas retention simulator
. Begin by familiarizing yourself with the capabilities of the
gas retention simulator through experimentation.
The
gas retention simulator
provides you with a
chamber
in which you can place
various gases and control the temperature. The dots moving inside this chamber should be
thought of as tracers where each represents a large number of gas particles. The walls of
the chamber can be configured to be a) impermeable so that they always rebound the gas
particles, and b) sufficiently penetrable so that particles that hit the wall with velocity over
some threshold can escape. You can also view the distributions of speeds for each gas in
relation to the escape velocity in the
Distribution Plot
panel.
The lower right panel entitled
gases
allows you to add and remove gases in the
experimental chamber. The lower left panel is entitled
chamber properties
. In its default
mode it has
allow escape from chamber
unchecked and has a
temperature
of 300 K.
Click
start simulation
to set the particles in motion in the chamber panel. Note that
stop
simulation
must be clicked to change the temperature or the gases in the simulation.
The upper right panel entitled distribution plot allows one to view the Maxwell
distribution of the gas as was possible in the background pages. Usage of the show
draggable cursor is straightforward and allows one to conveniently read off distribution
values such as the most probable velocity. The show distribution info for selected gases
requires that a gas be selected in the gas panel. This functionality anticipates a time when
more than one gas will be added to the chamber.
Exercises
Use the pull-down menu to add hydrogen to the chamber.
Question 4:
Complete the table using the draggable cursor to
measure the most probable velocity for hydrogen at each of
the given temperatures. Write a short description of the
relationship between T and v
mp
.
Temperature is a measure of
kinetic energy. Increasing the temperature, in turn increases
the kinetic energy and increases the probable velocity for
hydrogen at high temperature. Conversely, decreasing the temperature decreases the kinetic
energy and decreases the probable velocity of hydrogen. So the relationship between Temperature
and Vmp has a positive correlation.
Earth Sciences 2232G: Lab 02
3
T (K)
v
mp
(m/s)
300
1555
200
1250
100
895
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Question 5:
If the simulator allowed the temperature to be reduced to 0 K, what would you guess
would be the most probable velocity at this temperature? Why?
Absolute 0 is when a system has
little to zero thermodynamic energy and there is theoretically no atom movement.
Therefore, at
0K, the most probable velocity would be zero, due to the lack of energy emitted.
Return the temperature to 300 K. Use the gas panel to add Ammonia and Carbon Dioxide
to the chamber.
Question 6:
Complete the table using the draggable cursor
to measure the most probable velocity at a temperature of
300 K and recording the atomic mass for each gas. Write a
short description of the relationship between mass and vmp
and the width of the Maxwell distribution.
There is a
direct negative correlation between the atomic mass of the
atom and the probable velocity. As the atomic mass increases from
H
2
(2 u) to Carbon Dioxide
(44 u), the speeds of the particles at 300 K reduce. Heavier molecules tend to travel relatively
slower than lighter molecules. Looking at the width of the curves, the lower the mass, the longer
the width. Ammonia and Carbon Dioxide tend to have smaller widths and more prominent bell-
shaped curves, while Hydrogen has a very long width and less defined curve.
Question 7:
Check the box entitled allow
escape from chamber
in the chamber properties panel.
You should still have an evenly balanced mixture of hydrogen, ammonia, and carbon dioxide.
Run each of the simulations specified in the table below for the mixture. Click
reset proportions
to restore the original gas levels. Write a description below of the results similar to the example
completed for you (max 5 lines).
Earth Sciences 2232G: Lab 02
4
Gas
Mass (u)
v
mp
(m/s)
H
2
2
1555
NH
3
17
538
CO
2
44
325
Run
T (K)
v
esc
(m/s)
Description of Simulation
1
500
1500
H
2
is very quickly lost since it only has a mass of 2u and its
most probable velocity is greater than the escape velocity,
NH
3
is slowly lost since it is a medium mass gas (18u) and
a significant fraction of its velocity distribution is greater
than 1500 m/s, CO
2
is unaffected since its most probable
velocity is far less than the escape velocity.
2
500
1000
H
2
is lost very quickly since it has a relatively low mass and
since its most probable velocity is much higher than the
escape velocity for this stimulation.
NH
3
escapes at a
medium speed, faster than at 1500 m/s escape velocity, as a
more significant fraction of the distribution is greater than
1000m/s. CO
2
is lost very slowly, but faster than 1500m/s.
3
500
500
All three gases are lost relatively fast because large
fractions of all three of the velocity distributions are greater
than the escape speed of 500. However, H
2
is still lost the
fastest, NH
3
the second fastest and CO
2
the third fastest.
4
100
1500
H
2
is the only gas that is escapes from the chamber,
reducing relatively fast. Both NH
3
and CO
2
are unaffected
since the most probable velocity is far less than the escape
velocity and large fractions of their distribution curves are
less than 1500m/s.
5
100
1000
Once again, H
2
is the only gas that is escapes from the
chamber, reducing relatively fast. Both NH
3
and CO
2
are
unaffected since the most probable velocity is far less than
the escape velocity and majority of their distribution curves
are less than 1000m/s.
6
100
500
H
2
leaves very quickly, as a large fraction of its distribution
is greater than 500m/s. A quarter of the NH
3
distribution is
greater than the escape velocity, hence it escapes at a
medium speed. CO
2
is lost, but very slowly.
Question 8:
Write a summary of the results contained in the table above. Under what
circumstances was a gas likely to be retained? Under what circumstances is a gas likely to escape
the chamber?
The gas is likely to be retained in the chamber if the most probable velocity and a
large fraction of the velocity distribution is less than escape velocity, as it does not have the
velocity to escape the chamber. It is likely to escape when the most probable velocity and a large
portion of the curve is greater than the escape velocity, as it has the velocity to escape the
chamber.
A general trend was H
2
would always escape first and fastest and majority
of the
time CO
2
would escape very slowly, if not at all.
Earth Sciences 2232G: Lab 02
5
GAS RETENTION PLOT
This simulator presents an interactive plot summarizing the interplay between escape velocities
of large bodies in our solar system and the Maxwell distribution for common gases. The plot has
velocity on the y-axis and temperature on the x-axis. Two types of plotting are possible:
A point on the graph represents a large body with that particular escape velocity and outer
atmosphere temperature. An active (red) point can be dragged or controlled with sliders.
Realize that the escape velocity of a body depends on both the density (or mass) and the
radius of an object.
A line on the graph represents 10 times the average velocity (10×v
avg
) for a particular gas
and its variation with temperature. This region is shaded with a unique color for each gas.
o
If a body has an escape velocity v
esc
over 10×v
avg
of a gas, it will certainly retain
that gas over time intervals on the order of the age of our solar system.
o
If v
esc
is roughly 5 to 9 times v
avg
, the gas will be partially retained and the color
fades into white over this parameter range.
o
If v
esc
< 5 v
avg
, the gas will escape into space quickly.
Exercises
Begin experimenting with all boxes unchecked in both the gasses and plot options.
Question 9:
Plot the retention curves for the gases hydrogen, helium, ammonia, nitrogen, carbon
dioxide, and xenon. Explain the appearance of these curves on the retention plot.
The retention
curves for all 6 gases appear to be positively linear, with speed increases directly correlated with
increases in temperature. The difference is, gases such as hydrogen are lighter and start speeds
are higher on the graph, while xenon the heaviest gas is lower on the graph, with lower start
speeds. Differences in the B intercept for all 6 gases.
Check show gas giants in the plot options panel.
Question 10:
Discuss the capability of our solar system’s gas giants to retain particular gases
among those shown.
Gas giants in our solar system naturally have really high escape
velocities, which allows them to retain certain gasses better. Gas giants have average speeds
around 10-100 times higher than Mercury.
Question 11:
Drag the active point to the location (comparable with the escape speed and
temperature) of Mercury. The gases hydrogen, helium, methane, ammonia, nitrogen, and carbon
dioxide were common in the early solar system. Which of these gases would Mercury be able to
retain?
Looking at the graph, Mercury would not be able to retain anything, as it is under
all the retention lines. However, theoretically it will be better at retaining heavier gases, such as
Nitrogen and Carbon dioxide, because its speeds are relatively close to Mercury’s speeds as well.
Earth Sciences 2232G: Lab 02
6
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This is why Mercury is not a gas giant, but a large metal/rock body.
THINGS TO SUBMIT:
Submit this document via OWL to complete this lab.
Earth Sciences 2232G: Lab 02
7