Gas Adsorption

When a gas or vapor is brought into contact with a solid, part of it is taken up by the solid. The molecules that dissappear from the gas either enter the inside of the solid, or remain on the outside attached to the surface. The former phenomenon is termed absorption (or dissolution) and the latter adsorption. When the phenomena occur simultaneously, the process is termed sorption. The phenomenon of adsorption was disovered over two centuries ago. The uptake of gases by charcoal was studied by C. W. Scheele in 1773 and by the F. Fontana in 1777. In 1785, charcoal was found to decolorize' solutions by a surface adsorption mechanism. Since these processes have such a long history, we will make little attempt to be fair to the early pathfinders in this field nor to the historical development of the science.

The solid that takes up the gas is called the adsorbent, and the gas or vapor taken up on the surface is called the adsorbate. It is not always easy to tell whether the gas is inside the solid or merely at the surface because most practical' absorbents are very porous bodies with large internal' surfaces. It is not possible to determine the surface areas of such materials by optical or electron microscopy because of the size and complexity of the pores and channels of the material. The gas adsorption itself, however, can be used to determine the accesible surface area of most absorbents.

Gas adsorption is of practical consequence to engineers and chemists in many ways. It can provide a convenient, cheap and reusable method for fluid purification and purification. Gas masks used in WWI (and even in present day) are an example of the utility of charcoal as an absorbent. More significantly, perhaps, the phenomenon of surface adsorption has been used to modify the rates of product yields of chemical reactions through heterogeneous catalysis. For a catalyst to be useful, it must have a large surface area, bind the reactants quickly and effectively, stabilize the activated complex, and release the products of the reaction. Thus the attraction of various molecules on the surface, as well as the total surface area of the catalyst, are extremely important properties of potential catalytic materials.

Gas adsorption has been studied theoretically for most of this century and the simplist of the resulting theories provide the insight needed for most applications. We will investigate two such treatments, one attributed to Langmuir and one to Brunauer, Emmett and Teller (BET) and apply their equations to our experimental data. We will investigate the adsorption of N2 at cryogenic temperatures on common high area supports such as alumina. We will use this information to test simple adsorption theory, determine the specific area of the absorbent, and estimate the heat of adsorption of N2.

Additional information on experiments of this type may be obtained from many sources including:

  • S. Brunauer, "Physical Adsorption" (Princeton University Press, Princeton, N. J., 1945)
  • P. Atkins, "Physical Chemistry" (Freeman, New York, 1978)
  • G. A. Somorjai, "Principles of Surface Chemistry (Prentice-Hall, Englewood Cliffs, N. J. 1972)

    Theory of Adsorption

    Molecules and atoms can attach themselves onto surfaces in two ways. In physisorption (physical adsorption), there is a weak van der Waals attraction of the adsorbate to the surface. The attraction to the surface is weak but long ranged and the energy released upon accommodation to the surface is of the same order of magnitude as an enthalpy of condensation (on the order of 20 kJ/mol). During the process of physisorption, the chemical identity of the adsorbate remains intact, i.e. no breakage of the covalent structure of the adsorbate takes place. Physisorption, to be a spontaneous thermodynamic process, must have a negative DELTA G. Because translational degrees of freedom of the gas phase adsorbate are lost upon deposition onto the substrate DELTA S is negative for the process. Since DELTA G = DELTA H - TDELTA S , DELTA H for physisorption must be exothermic.

    In chemisorption (chemical adsorption), the adsorbate sticks to the solid by the formation of a chemical bond with the surface. This interaction is much stronger than physisorption, and, in general, chemisorption has more stringent requirements for the compatibility of adsorbate and surface site than physisorption. The chemisorption may be stronger than the bonds internal to the free adsorbate which can result in the dissociation of the adsorbate upon adsorption (dissociative adsorption). In some cases DELTA S for dissociative adsorption can be greater than zero, which means endothermic chemisorption, although uncommon, is possible.

    The energetics of adsorption depend on the extent to which the available surface is covered with adsorbate molecules. This is because the adsorbates can interact with each other when they lie upon the surface (in general they would be expected to repel each other). The fractional coverage of a surface is defined by the quantity THETA:

    At any temperature, the adsorbate and the surface come to a dynamic equilibrium, that is, the chemical potentials of the free adsorbate and the surface bound adsorbate are equal. The chemical potential of the free adsorbate depends on the pressure of the gas, and the chemical potential of the bound adsorbate depends on the coverage THETA. Thus the coverage at a given temperature is a function of the applied adsorbate pressure. The variation of THETA with p at a given T is called an adsorption isotherm.

    Several adsorption isotherms have proven useful in understanding the process of adsorption. The simplest isotherm is attributed to a pioneer in the study of surface processes, Langmuir, and is called the Langmuir isotherm. If one assumes:

  • Adsorption cannot proceed beyond the point at which the adsorbates are one layer thick' on the surface (monolayer)
  • All adsorption sites are equivalent.
  • The adsorption and desorption rate is independent of the population of neighboring sites.

    then one can derive a simple formula for an adsorption isotherm [I. Langmuir, J. Amer. Chem. Soc., 40, 1361 (1918); I. Langmuir, J. Amer. Chem. Soc., 54, 2798 (1932); I. Langmuir, Nobel Lecture, 1932]. Consider the equilibrium

    eq. 2

    where A is the free adsorbate, S is the free surface, and A.S is the substrate bound to the surface. The rate of adsorption will be proportional to the pressure of the gas and the number of vacant sites for adsorption. If the total number of sites on the surface is N, then the rate of change of the surface coverage due to adsorption is:

    eq. 3

    The rate of change of the coverage due to the adsorbate leaving the surface (desorption) is proportional to the number of adsorbed species:

    eq. 4

    In these equations, ka and kd are the rate constants for adsorption and desorption respectively and p is the pressure of the adsorbate gas. At equilibrium, the coverage is independent of time and thus the adsorption and desorption rates are equal. The solution to this condition gives us a relation for THETA:

    eq. 5

    where K = ka / kd. Note that because K is an equilibrium constant, the value of K at various temperatures determined from the Langmuir isotherm allows for the evaluation of the enthalpy of adsorption, DELTA Hads, through the van't Hoff equation:

    eq. 6

    Complications, complications...

    The Langmuir isotherm gives us a wonderfully simple picture of adsorption at low coverage and is applicable in some situations. At high adsorbate pressures and thus high coverage, this simple isotherm fails to predict experimental results and thus cannot provide a correct explanation of adsorption in these conditions. What is missing in the Langmuir treatment is the possibility of the initial overlayer of adsorbate acting as a substrate surface itself, allowing for more adsorption beyond a saturated (monolayer) coverage. This possibility has been treated by Brunauer, Emmett, and Teller [J. Amer. Chem. Soc., 60, 309 (1938)] and the result is named the BET isotherm. This isotherm is useful in cases where multilayer adsorption must be considered. The form of this isotherm is:

    eq. 7

    where n/nmono is the ratio of the moles adsorbed to the moles adsorbed in a single monolayer, and z = p/p0, where p0 is the vapor pressure of the pure condensed adsorbate. The n/nmono ratio represents a generalized coverage' because its value can exceed unity. The constant c represents the relative strengths of adsorption to the surface and condensation of the pure adsorbate. Simple theory predicts an approximate value of this constant as:

    eq. 8

    The BET isotherm predicts that the amount of adsorption increases indefinitely as the pressure is increased since there is no limit to the amount of condensation of the adsorbate. In the limit that adsorption to the surface is much 'stronger' than the condensation to a liquid (such as for the adsorption of unreactive gases onto polar substrates) the BET isotherm simplifies to the form (c=INFINITY):

    eq. 9

    The Langmuir isotherm is found to be useful only at very small coverages (sub-monolayer) but is generally applied to all cases involving chemisorption. This would correspond to the limiting case of c approaching infinity in the BET formalism, and no insight is provided by BET below one monolayer in this limit.

    The BET isotherm is found to describe adequately the physisorption at intermediate coverage (THETA = 0.8 - 2.0) but fails to represent observations at low or high coverage. The BET isotherm is reasonably valid around THETA =1.0, however, and this is useful in characterizing the area of the absorbent. If one can determine experimentally the number of moles of adsorbate required to give THETA = 1.0 (i.e. a monolayer), one can determine the specific area of the absorbent:

    eq. 10

    Practically, one measures the number of moles adsorbed as a function of equilibrium pressure, i.e. one does not directly measure THETA. Algebraic rearrangement of the BET isotherm to produce a linear equation is usually applied to experimental data.

    This implies that over the range where the BET isotherm is valid a plot of z/n(1-z) vs z will be linear. The slope and intercept of this line will allow the determination of nmono and c. The specific area of the sample is simply:

    In our studies, SIGMA, the molecular area of the absorbate N2 is taken to be 15.8 Angstoms2, NA is Avogadro's number, and m is the mass of the sample.

    The adsorption process is generally taken as completely reversible, but, under some conditions the isotherm may exhibit a different shape upon desorption as compared to absorption. This is called hysteresis. Sometimes hysteresis data can be used to determine the structure and size of pores in the absorbent. We will therefore need to generate an isotherm for both absorption and desorption.

    Experimental Procedure

    Figure 3

    We will perform the adsorption measurements in a commercial vacuum manifold called the Omnisorb 360, manufactured by Omnicron. A schematic diagram of the relevant portion of the vacuum system is shown in Figure 4.

    Although this system is designed for semi-automated use, we will use the equipment manually. The numbers on the above schematic represent some of the numbered valves on the system and the diagram above is similar to the layout of the valve controls on the machine itself. Each valve is pneumatically controlled by a numbered push button switch. Simply push the button to open any valve; an open valve is indicated by the switch lamp on. To close, hit the button again.

    Several portions of the system require some discussion. The adsorbtive gases enter the system through valves 10(N2),13(CO2, not used in this experiment), and 12(He). The inlet is the portion of the system between these valves, valve 11, the flow controller, and valve 8. The manifold is the portion of the system between valves 7,8, and the sample port valves 3,4,5 and 6. The manifold is evacuated by a vacuum pump when valves 9 and 7 are open. The vaccum pump pressure is monitored by a Pirani gauge on the upper left of the console. The manifold pressure is monitored by two (0-1000 torr, 0-10 torr) capacitance manometers (Baratrons). (Please note where the pressure measurement is made on the manifold in Figure 3. Since there is a slight change in the manifold volume depending on the state of valves 3 - 8, all pressure readings should be made with these valves closed whenever possible).


    Figure 4


    Sample preparation (this may be performed for you)

    Weigh (tare) a sample bulb with valve. Introduce less than one gram of sample into the bulb. Degas the sample (Degassing is accomplished in the furnace at the left bottom of the instrument). Determine as accurately as possible the degassed weight of the sample plus bulb and thus the sample mass. Attach the bulb to sample port #3 or #6 and fill the Dewar with LN2 to a level about 2" above the bulb. Record the atmospheric pressure (barometer) and manifold temperature (displayed on the upper center of the control panel in oC).

    System Setup

    You will find the system with the mechanical and diffusion pumps already on. Evacuate the inlet and manifold by opening valves 9,7,8. Close the Flow controller by setting the flow rate to 0.00. Evacuate the sample and known volume by opening the appropriate sample port valves. Note the base pressure indications on all three pressure gauges (One Pirani, and the two Baratrons) and record these in your notebook. As the system will base at a lower pressure than the manometers can indicate, the Baratron readings you take now will be used as a zero offset and will be used to correct all subsequent readings.

    Close the sample port valves and flush the inlet and manifold with the gas to be used (initially He). Gas is introduced into the manifold by the following procedure: Close valve 8 and momentarily open (open, then close) the inlet valve for the desired gas. The inlet is now charged. Now open and close valve 8. A slug of gas has been introduced into the manifold and you should see the pressure rise (to about 300 torr at this point). Now pump out the manifold and inlet by opening the appropriate valves. Repeat this procedure a couple of times each time you change gases.

    Volume Determinations

    Only one volume in the system is known at the onset, Vk, the volume of the bulb on port #5. We will use it to determine the manifold volume, Vm, as well as the free volume in our sample bulb, Vs.

    Manifold Volume

    Fill the manifold and known volume bulb to about 700 torr with He and record the pressure. This may take two 'charges' from the inlet. Evacuate the inlet and manifold but leave the known volume pressurized, and record the value. Now fill the manifold with gas from the known volume bulb. Record the pressure again. The reduction in pressure will allow you to calculate the ratio of the manifold volume to the known volume through the ideal gas relation. Close valve #5, evacuate the manifold, and refill from the known volume again. This will give you another determination of the manifold volume. Repeat this procedure several times to obtain an average value of Vm.

    Sample Void Volume

    Now that the manifold volume is known, determine the sample void volume by the same procedure as above but fill the manifold from the sample bulb instead of the bulb on port #5. Helium is used for volume determinations because it does not adsorb to anything at 77K.

    Adsorption Studies

    Evacuate the sample and close the valve connecting it to the manifold. Close valve #5 and isolate the known volume from the manifold for the remainder of the experiment. Flush the inlet and manifold with N2. Fill the manifold with N2 to about 40 torr and record the pressure. Since one 'charge' from the inlet will produce more pressure than this, you will have to reduce the pressure by closing #8, evacuating the manifold, momentarily opening #8, and repeating until the manifold pressure is about the desired value. With all valves closed open the sample port valve and expose the sample to the sealed off manifold. The pressure will drop when the sample bulb is opened to the manifold filled with nitrogen but it will drop significantly more more than would occur if the gas in the manifold were He. This is because some of the nitrogen gas is adsorbing to the sample surface. Allow the sample and adsorbate to equilibrate at 77K.

    NOTE: The approach to equilibrium is perceptably slow, especially at high coverage. It would in principle take an infinite time for equilibrium to be exactly established. The nature of the isotherm and the required precision of the measurement suggests that equilibrium pressures need be known only to a few percent. Take a few point allowing a long time for equilibrium to be achieved and plot the approach to equilibrium as a function of time. Is this a first order process in adsorbate? Estimate the time it takes to get to within 5% of the equilibrium pressure and us this as a cutoff time for data taken at similar coverage. Correct for the incomplete equilibration in working up the data. In summary, use your judgement as to how long to wait at each pressure. Analyse and exploit kinetic information about the approach to equilibrium. Don't get old waiting and not thinking.

    Record the equilibrium pressure. This procedure generates the data you need to allow you to determine the number of moles adsorbed on the solid as a function of (equilibrium) pressure.

    Close the valve to the sample tube and refill the manifold. 'Dose' the sample again and record the pressures. You now have the next point on the isotherm.

    Repeat the above with ca. 50 torr in the manifold until the equilibrium pressure reaches ca. 20 torr. Then increase the initial manifold pressure to 300 torr and repeat until the equilibrium pressure reaches about 200 torr. Then increase the initial manifold pressure to ca. 700 torr until the equilibrium pressure reaches ca. 500 torr. This completes the data acquisition needed to generate the adsorption isotherm.

    Desorption Studies

    The desorption measurement is performed to see if there is any hysterisis or non-equilibrium effects in the adsorption/desorption cycle. This is basically performed in reverse of the procedure above. You should already have the sample and manifold in equilibrium at some pressure ca. 450 torr from the adsorption run. Close the sample off from the manifold and evacuate the manifold. Open the sample to the manifold and allow equilibrium to be achieved. Record this pressure. You now know how many moles of gas have been removed from the sample and the new equilibrium pressure --- so this is the first point on the desorption isotherm. Repeat this procedure until the equilibrium pressure reaches ca. 5 torr.

    If time permits, perform adsorption and desorption studies for all three solids: alumina, silica, and charcoal.

    Data Analysis


    Experimental Data taken on the Omnisorp 360 for a ca. 0.3 g sample of silica

    Additional Food for thought

    How does the BET theory fail in comparison to the actual data at low and high coverage? Why does this behaviour occur? Does the Langmuir Theory work for your physisorption data at low (sub monolayer) coverage?

    REFERENCES

  • S. Brunauer, "Physical Adsorption" (Princeton University Press, Princeton, N. J., 1945)
  • P. Atkins, "Physical Chemistry" (Freeman, New York, 1978)
  • G. A. Somorjai, "Principles of Surface Chemistry (Prentice-Hall, Englewood Cliffs, N. J. 1972)
  • R.S. Drago, C.E. Webster, and J.M. McGilvray, J. Am. Chem. Soc., 1998, 120, 538
    This experiment is dedicated to the memory of Russ Drago

    Have a look at a sample papers on this experiment
    Andrew Knight 15.11.1996


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