lab2

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2232

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Dec 6, 2023

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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