Query 3

#$&*

course Phy 232

If your solution to stated problem does not match the given solution, you should self-critique per instructions athttp://vhcc2.vhcc.edu/dsmith/geninfo/labrynth_created_fall_05/levl1_22/levl2_81/file3_259.htm

Your solution, attempt at solution:

If you are unable to attempt a solution, give a phrase-by-phrase interpretation of the problem along with a statement of what you do or do not understand about it. This response should be given, based on the work you did in completing the assignment, before you look at the given solution.

*********************************************

Question: query intro set problem 14 substance, water, both temperatures and masses known, final temperature known, find spec ht

Explain how the final temperature of the system is combined with the known initial temperatures and masses of both substances to obtain the unknown specific heat

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

Mass of one substance times its specific heat capacity times the change in temperature is equal to the second mass times the second specific heat capacity times the change in temperature. The specific heat capacity of water is known, so a simple equation is set up mwater (C) (Tf-Ti)=msubstance(csubstance)(Tf-TI). Csubstance can then be solved for.

confidence rating #$&*: 5

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

** The change in the thermal energy of an isolated system is 0. So assuming that the systems are isolated the thermal energy change of one object is equal and opposite to that of the other.

For an ideal substance the change in the thermal energy of an object is directly proportional to the change in its temperature and to its mass (i.e., more mass and more change in temperature implies more change in thermal energy). The specific heat is the proportionality constant for the substance. Using `dQ for the change in the thermal energy of an object we can express this as

• `dQ = mass * specific heat * `dT.

(General College and University Physics students note that most substances do not quite behave in this ideal fashion; for most substances the specific heat is not in fact strictly constant and for most substances changes with temperature.)

For two objects combined in a closed system we have `dQ1 + `dQ2 = 0, which gives us the equation

• m1 c1 `dT1 + m2 c2 `dT2 = 0

or equivalently

• m1 c1 `dT1 = - m2 c2 `dT2.

That is, whatever energy one substance loses, the other gains.

In this situation we know the specific heat of water, the two temperature changes and the two masses. We can therefore solve this equation for specific heat c2of the unknown substance. **

Your Self-Critique:ok

Your Self-Critique Rating:

*********************************************

Question: prin phy Ch 13.26. Kelvin temperatures corresponding to 86 C, 78 F, -100 C, 5500 C and -459 F.

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

confidence rating #$&*:

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

The Kelvin temperature is 273 K higher than the Celsius temperature (actually 273.15 below, but the degree of precision in the given temperatures is not sufficient to merit consideration of tenths or hundredths of a degree).

• 86 C, -100 C and 5500 C are therefore equivalent to ( 86 + 273 ) K = 359 K, -100 + 273 K = 173 K, (5500 + 273) K = 5773 K.

The freezing point of water is 0 C or 32 F, and a Fahrenheit degree is 5/9 the size of a Celsius degree. Therefore

• 78 F is (78 F - 32 F) = 46 F above the freezing point of water.

• 46 Fahrenheit degrees is the same as (5/9 C / F ) * 46 F = 26 C above freezing.

• Since freezing is at 0 C, this means that the temperature is 26 C.

• The Kelvin temperature is therefore (26 + 273) K = 299 K.

Similar reasoning can be used to convert -459 F to Celsius

• -459 F is (459 + 32) F = 491 F below freezing, or (5/9 C / F) * (-491 F) = 273 C below freezing.

• This is -273 C or (-273 + 273) K = 0 K.

• This is absolute zero, to the nearest degree.

Your Self-Critique:

Your Self-Critique Rating:

*********************************************

Question: prin phy and gen phy Ch 13.30 air at 20 C is compressed to 1/9 of its original volume. Estimate the temperature of the compressed air assuming the pressure reaches 40 atm.

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

confidence rating #$&*:

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

First we reason this out intuitively:

If the air was compressed to 1/9 its original volume and the temperature didn’t change, it would end up with 9 times its original pressure.

However the pressure changes from 1 atm to 40 atm, which is a 40-fold increase.

The only way the pressure could end up at 40 times the original pressure, as opposed to 9 times the original, would be to heat up. Its absolute temperaturewould therefore have to rise by a factor of 40 / 9.

Its original temperature was 20 C = 293 K, so the final temperature would be 293 K * 40/9, or over 1300 K.

Now we reason in terms of the ideal gas law.

P V = n R T.

In this situation the number of moles n of the gas remains constant. Thus P V / T = n R, which is constant, and thus P1 V1 / T1 = P2 V2 /T2.

The final temperature T2 is therefore

• T2 = (P2 / P1) * (V2 / V1) * T1.

From the given information P2 / P1 = 40 and V2 / V1 = 1/9 so

• T2 = 40 * 1/9 * T1.

The original temperature is 20 C = 293 K so that T1 = 293 K, and we get

• T2 = 40 * 1/9 * 293 K,

the same result as before.

Your Self-Critique:

Your Self-Critique Rating:

*********************************************

Question: query gen phy ch 13.38 fraction of air released after tire temp increases from 15 to 38 C at 220 kPa gauge

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

confidence rating #$&*:

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

(Note that the given 220 kPa initial gauge pressure implies an absolute pressure of 311 k Pa; assuming atmospheric pressure of about 101 k Pa, we add this to the gauge pressure to get absolute pressure).

Remember that the gas laws are stated in terms of absolute temperature and pressure.

The gas goes through three states. The temperature and pressure change between the first and second states, leaving the volume and the number n of molesconstant. Between the second and third states pressure returns to its original value while volume remains constant and the number n of moles decreases.

From the first state to the second:

T1 = 288 K, T2 = 311 K so T2 / T1 = 311 / 288 = 1.08, approx.

This is approx. an 8% increase in temperature. The pressure must therefore rise to

P2 = 3ll / 288 * 321 kPa = 346 kPa, approx

(note that we have to use actual rather than gauge pressure so init pressure is 220 kPa + 101 kPa = 321 kPa, approx. )

From the second state to the third, pressure is then released by releasing some gas, changing the number n of moles of gas in order to get pressure back to 331 kPa. Thus

n3 / n2 = P3 / P2 = 321 kPa / 346 kPa or approximately .93, which would be about a 7% decrease. So we have to release about 7% of the air.

Note that these calculations have been done mentally, and they might not be particularly accurate. Work out the process to botain the accurate numerical results.

Note also that temperature changes from the second to third state were not mentioned in the problem. We would in fact expect a temperature change to accompany the release of the air, but this applies only to the air that escapes. The air left in the tire would probably change temperature for one reason or another, but it wouldn't do so as a direct result of releasing the air.

STUDENT QUESTION

It seems that the air goes from 288 to 311 K, so the ratio should be n2 / n1 = 288 / 311 and the proportional loss should be about (1 - 288 / 311)

INSTRUCTOR RESPONSE

The Kelvin temperature goes from 288 K to 311 K.

If the air is released at constant pressure, then volume and pressure remain constant while temperature and number of moles vary according to

n T = P V / R

so that

n1 T1 = n2 T2, and

n2 = n1 * (T1 / T2) = n1 * (288 / 311)

and the change in amount of gas is n1 - n2 = n1 - 288/311 n1 = n1( 1 - 288 / 311), or about 7.4% of n1.

If the temperature is first raised to 311 K, then the gas is released, it is the pressure and amount of gas that change. In that case the change in the amount of the gas is n1 - n3 = n1 - (321 kPa / 346 kPa) * n1 = n1 ( 1 - 321 / 346), or about 7.2% of n1.

The fractions 288/311 and 321 / 346 don't differ by much, not do the percents, but they do differ.

Your Self-Critique:

Your Self-Critique Rating:

*********************************************

Question: query univ phy 17.114 / 17.116 (15.106 10th edition) 1.5 * 10^11 m, 1.5 kW/m^2, sun rad 6.96 * 10^8 m.

How did you calculate the total radiation of the Sun and how did you use this result to get the radiation per unit area?

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

The total radiation of the sun is equal to the rate of radiation times the surface area of the sun. The surface area of the sun is 4pi*6.96*10^8m*6.96*10^8m=6.09*10^18m^2

This times the rate of radiation is 6.09*10^18m^2(1.5kw/m^2)=9.135*10^18kw

The radiation per unit area is found by taking the value for total radiation and dividing by the surface area of radiation which is equal to 4pi(1.5*10^11m)^2=2.82*10^23m^2 (surface area of radiation)

So the final value would be 9.135*10^18kw/2.82*10^23m^2=0.0323w/m^2

confidence rating #$&*:4

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

Outline of solution strategy:

If we multiply the number of watts per unit of area by the surface area of the Sun we get the number of watts radiated from the Sun.

The energy flows outward in a spherically symmetric manner; at any distance the entire power is distributed over the radius of a sphere concentric with the Sun and of radius equal to the distance.

So if we divide that number of watts by the area of a sphere whose radius is equal to that of the Earth’s orbit, we get the number of watts per unit of area at that distance.

This strategy is followed in the student solution given below:

Good student solution:

Surface area of sphere of radius r is 4 pi r^2; if flux intensity is I then flux = 4 pi r^2 I.

When r = 1.5 * 10^11 m, I = 1500 W / m^2, so the flux is 4 pi r^2 I = 4 pi * (1.5 * 10^11 m)^2 * 1500 W / m^2 = 4.28 * 10^26 watts.

4.28055 x 10 ^ 26 W / (4*`pi * (6.96 x 10 ^ 8 m)^2) = 4.28055 x 10 ^ 26 W / 6.08735 x 10 ^ 18 m^2 = 70318775.82 J/s/m^2 = 7.03 x 10 ^ 7 J/s/m^2

If the sun is radiating as an ideal blackbody, e = 1, then T would be found as follows:

H = `dQ/`dt = 4.28055 x 10 ^ 26 W = (4*`pi * (6.96 x 10 ^ 8 m)^2) * (1) * (5.67051 x 10^-8 W/m^2*K) * T^4

So T^ 4 = 4.28055 x 10 ^ 26 W / 6.087351 x 10 ^ 18 m^2) * 1 * (5.67051 x 10^-8 W/m^2*K)

T^4 = 1.240 * 10 ^ 15 K ^4

T = 5934.10766 K on surface of sun. **

Your Self-Critique: I didn’t really know how to start this problem, so I looked at the instructor’s response initially to start this problem, but I think that there are some discrepancies between the instructor solution and the student solution.

Your Self-Critique Rating: 4

@&

My outline might be ambiguous. In any case it could be clearer.

The energy radiated from the Sun passes through concentric spheres centered at the Sun. Whatever intensity occurs on Earth occurs over a sphere whose radius is equal to that of the Earth's orbit. This result is the power flux of the Sun's radiant energy.

That power emanates from the surface of the Sun. So if we divide our result by the area of the Sun we get the radiant intensity at its surface.

From this we can determine the temperature of the surface.

*@

???? The student solution does not follow the layout set up by the instructor. It would appear that the student used the radius from the earth to the sun for the initial surface area that is multiplied by the watts per unit area of 1.5 kW. The instructor, however, says that the way to do this problem is to multiply the surface area of the sun by the watts per unit area of 1.5 Kw to get the total watts radiated by the sun. I followed the way that the instructor laid out to do the problem, so I don’t know whether the instructor’s solution is wrong or whether or not the student’s solution is wrong. The student found the total watts radiated by multiplying the sphere of radius 1.5 *10^11 instead of the radius of the sun. In this case, it means that his/her final answer for watts per unit area was found by dividing by the surface area of the sun. This is not what should have been done as stated by the instructor. Could you please clarify this for me?????

*********************************************

Question: univ phy (omitted from 12th edition, but should be worked now) was 17.115 Solar radiation of intensity 600 watts / m^2 is incident on an ice sheet. The temperature above and below the ice sheet is 0 Celsius. Assuming that 70% of the radiation is absorbed at the surface of the ice, how long take to melt a layer of ice 1.2 cm thick?

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

Only 70% of the radiation is absorbed which is .7*600watts/m^2=420W/m^2

The volume of a 1.2cm thick square meter of ice would be 0.012m(1)(1)=0.012m^3

The density of ice is 916.17 Kg/m^3

D=m/v

916.17kg/m^3(0.012m^3)=10.99kg

The heat needed to melt 10.99Kg is equal to the heat of fusion times the mass which is 333.55Kj/Kg(10.99Kg)=3665.17 KJ=3665714.5J

At the rate of 420J/s it would take 3665714.5J/420J/2=8727 seconds.

confidence rating #$&*:5

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

** Thermal energy is not radiating in significant quantities from the ice, so only the incoming radiation needs to be considered, and as stated only 70% of that energyis absorbed by the ice..

• 70% of the incoming 600 watts/m^2 is 420 watts / m^2, or 420 Joules/second for every square meter if ice.

• Melting takes place at 0 C so there is no thermal exchange with the environment. Thus each square meter absorbs 420 Joules of energy per second.

We need to consider the volume of ice corresponding to a square meter. Having found that we can determine the energy required to melt the given thickness:

• A 1.2 cm thickness of ice will have a volume of .012 m^3 for every square meter of surface area; the mass will be close to 1000 kg/m^3, so there are about12 kg of ice for every m^2 of surface (you can obtain a more accurate result by using the a more accurate density; the density of ice (which floats in water) is actually somewhat less than that of water).

• It takes about 330,000 Joules to melt a kg of ice at 0 C, so to melt 12 kg requires around 4,000,000 J. At 420 Joules/sec this will require roughly10,000 seconds, or around 3 hours.

All these calculations were done mentally and are therefore approximate. You should check them yourself, using appropriately precise values of the constants, etc. **

"

Self-critique (if necessary):

------------------------------------------------

Self-critique rating:

???? The student solution does not follow the layout set up by the instructor. It would appear that the student used the radius from the earth to the sun for the initial surface area that is multiplied by the watts per unit area of 1.5 kW. The instructor, however, says that the way to do this problem is to multiply the surface area of the sun by the watts per unit area of 1.5 Kw to get the total watts radiated by the sun. I followed the way that the instructor laid out to do the problem, so I don’t know whether the instructor’s solution is wrong or whether or not the student’s solution is wrong. The student found the total watts radiated by multiplying the sphere of radius 1.5 *10^11 instead of the radius of the sun. In this case, it means that his/her final answer for watts per unit area was found by dividing by the surface area of the sun. This is not what should have been done as stated by the instructor. Could you please clarify this for me?????

*********************************************

Question: univ phy (omitted from 12th edition, but should be worked now) was 17.115 Solar radiation of intensity 600 watts / m^2 is incident on an ice sheet. The temperature above and below the ice sheet is 0 Celsius. Assuming that 70% of the radiation is absorbed at the surface of the ice, how long take to melt a layer of ice 1.2 cm thick?

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

Only 70% of the radiation is absorbed which is .7*600watts/m^2=420W/m^2

The volume of a 1.2cm thick square meter of ice would be 0.012m(1)(1)=0.012m^3

The density of ice is 916.17 Kg/m^3

D=m/v

916.17kg/m^3(0.012m^3)=10.99kg

The heat needed to melt 10.99Kg is equal to the heat of fusion times the mass which is 333.55Kj/Kg(10.99Kg)=3665.17 KJ=3665714.5J

At the rate of 420J/s it would take 3665714.5J/420J/2=8727 seconds.

confidence rating #$&*:5

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

** Thermal energy is not radiating in significant quantities from the ice, so only the incoming radiation needs to be considered, and as stated only 70% of that energyis absorbed by the ice..

• 70% of the incoming 600 watts/m^2 is 420 watts / m^2, or 420 Joules/second for every square meter if ice.

• Melting takes place at 0 C so there is no thermal exchange with the environment. Thus each square meter absorbs 420 Joules of energy per second.

We need to consider the volume of ice corresponding to a square meter. Having found that we can determine the energy required to melt the given thickness:

• A 1.2 cm thickness of ice will have a volume of .012 m^3 for every square meter of surface area; the mass will be close to 1000 kg/m^3, so there are about12 kg of ice for every m^2 of surface (you can obtain a more accurate result by using the a more accurate density; the density of ice (which floats in water) is actually somewhat less than that of water).

• It takes about 330,000 Joules to melt a kg of ice at 0 C, so to melt 12 kg requires around 4,000,000 J. At 420 Joules/sec this will require roughly10,000 seconds, or around 3 hours.

All these calculations were done mentally and are therefore approximate. You should check them yourself, using appropriately precise values of the constants, etc. **

"

Self-critique (if necessary):

------------------------------------------------

Self-critique rating:

#*&!

???? The student solution does not follow the layout set up by the instructor. It would appear that the student used the radius from the earth to the sun for the initial surface area that is multiplied by the watts per unit area of 1.5 kW. The instructor, however, says that the way to do this problem is to multiply the surface area of the sun by the watts per unit area of 1.5 Kw to get the total watts radiated by the sun. I followed the way that the instructor laid out to do the problem, so I don’t know whether the instructor’s solution is wrong or whether or not the student’s solution is wrong. The student found the total watts radiated by multiplying the sphere of radius 1.5 *10^11 instead of the radius of the sun. In this case, it means that his/her final answer for watts per unit area was found by dividing by the surface area of the sun. This is not what should have been done as stated by the instructor. Could you please clarify this for me?????

*********************************************

Question: univ phy (omitted from 12th edition, but should be worked now) was 17.115 Solar radiation of intensity 600 watts / m^2 is incident on an ice sheet. The temperature above and below the ice sheet is 0 Celsius. Assuming that 70% of the radiation is absorbed at the surface of the ice, how long take to melt a layer of ice 1.2 cm thick?

YYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYYY

Your Solution:

Only 70% of the radiation is absorbed which is .7*600watts/m^2=420W/m^2

The volume of a 1.2cm thick square meter of ice would be 0.012m(1)(1)=0.012m^3

The density of ice is 916.17 Kg/m^3

D=m/v

916.17kg/m^3(0.012m^3)=10.99kg

The heat needed to melt 10.99Kg is equal to the heat of fusion times the mass which is 333.55Kj/Kg(10.99Kg)=3665.17 KJ=3665714.5J

At the rate of 420J/s it would take 3665714.5J/420J/2=8727 seconds.

confidence rating #$&*:5

^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

.............................................

Given Solution:

** Thermal energy is not radiating in significant quantities from the ice, so only the incoming radiation needs to be considered, and as stated only 70% of that energyis absorbed by the ice..

• 70% of the incoming 600 watts/m^2 is 420 watts / m^2, or 420 Joules/second for every square meter if ice.

• Melting takes place at 0 C so there is no thermal exchange with the environment. Thus each square meter absorbs 420 Joules of energy per second.

We need to consider the volume of ice corresponding to a square meter. Having found that we can determine the energy required to melt the given thickness:

• A 1.2 cm thickness of ice will have a volume of .012 m^3 for every square meter of surface area; the mass will be close to 1000 kg/m^3, so there are about12 kg of ice for every m^2 of surface (you can obtain a more accurate result by using the a more accurate density; the density of ice (which floats in water) is actually somewhat less than that of water).

• It takes about 330,000 Joules to melt a kg of ice at 0 C, so to melt 12 kg requires around 4,000,000 J. At 420 Joules/sec this will require roughly10,000 seconds, or around 3 hours.

All these calculations were done mentally and are therefore approximate. You should check them yourself, using appropriately precise values of the constants, etc. **

"

Self-critique (if necessary):

------------------------------------------------

Self-critique rating:

#*&!#*&!

&#This looks good. See my notes. Let me know if you have any questions. &#