query 3

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course Phy 232

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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.

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Question:

query problem 15 introductory problem sets temperature and volume information find final temperature.

When temperature and volume remain constant what ratio remains constant?

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Your Solution:

Pv=nRT

So if volume and temperature remain constant, then V/T=(nR)/P, which means the ratio (nR)/P is a constant ratio.

Since R is constant anyways, if volume and temperature remain constant then n/P is the constant ration.""

confidence rating #$&*:

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Given Solution:

** PV = n R T so n R / P = V / T

Since T and V remain constant, V / T remains constant.

· Therefore n R / P remain constant.

· Since R is constant it follows that n / P remains constant. **

STUDENT QUESTION:

I don’t understand why P is in the denominator when nR was moved to the left side of the equation

INSTRUCTOR RESPONSE:

The given equation was obtained by dividing both sides by P and by T, then reversing the sides.

We could equally well have divided both sides by v and by n R to obtain

P / (n R) = T / V,

and would have concluded that P / n is constant.

To say that P / n is constant is equivalent to saying the n / P is constant.

Your Self-Critique: OK

Your Self-Critique Rating:OK

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Question: why, in terms of the ideal gas law, is T / V constant when only temperature and volume change?

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Your Solution:

PV=nRT

V/T=nR/P

so when nothing else changes, n P and R are all constant so nR/P is constant, therefore T/V is also constant

confidence rating #$&*:

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Given Solution:

** STUDENT ANSWER AND INSTRUCTOR RESPONSE:

They are inversely proportional. They must change together to maintain that proportion.

INSTRUCTOR RESPONSE:

You haven't justified your answer in terms of the ideal gas law:

PV = n R T so V / T = n R / P.

If only T and V change, n and P don't change so n R / P is constant.

Therefore V / T is constant, and so therefore is T / V.

You need to be able to justify any of the less general relationships (Boyle's Law, Charles' Law, etc.) in terms of the general gas law, using a similar strategy. **

Your Self-Critique: OK

Your Self-Critique Rating: OK

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

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Your Solution:

N/A university phys 232

confidence rating #$&*:

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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:

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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.

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Your Solution:

N/A university phy

confidence rating #$&*:

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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 temperature would 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:

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

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Your Solution:

N/A university

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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 moles constant. 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:

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Question: `q001. The temperature of a certain object increases from 50 Celsius to 150 Celsius. What is its change in temperature in Celsius?

Convert 50 Celsius and 150 Celsius to Kelvin.

What is the change in temperature in Kelvin?

What is the change in temperature in Fahrenheit?

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Your Solution:

150 - 50 = 50 C

50 +273 =323 K

9/5*150 +32 -9/5*50 +32=180 F

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Self-Critique Rating: OK

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Question: `q002. A sample of gas originally at 0 Celsius and pressure 1 atmosphere is compressed from volume 450 milliliters to volume 50 milliliters, in which state its pressure is 16 atmospheres. What is its temperature in the new state?

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Your Solution:

P1V1/T1=P2V2/T2

1*450/273=16*50/T2

t2=485 K or 212 C

confidence rating #$&*:

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Self-Critique Rating: OK

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Question: `q003. What product or ratio involving P, V, n and T would remain constant if V and T were held constant?

Why does this make sense?

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Your Solution:

PV=nRT

V/T=nR/P

so nR/P would also be constant. This makes sense mathematically and logically through solving the equationl.

@&

Good.

However note that R is already constant, so it contributes nothing to include it.

All the necessary information is included if you just say that n / P is constant.

*@

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Self-Critique Rating: OK

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Question: query univ phy 17.112/ 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?

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Your Solution:

Surface area=4*pi*r^2

surface area=6.1 x 10 ^ 18 m^2

I dont know how to find total radiation, but you would divide total radiation by 6.1 x 10 ^ 18 to fine radiation

per unit area.

confidence rating #$&*:1

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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:

That makes much more sense. I was confused as to how to find radiation, but by multiplying watts per unit by the

surface area, you could get the total number of watts radiated. Then by dividing the number of watts by the area of

the sphere equal to Earth's orbit, you could get watts per unit area of that distance, not by dividing them by the

sun's surface area like I did in the problem.

Your Self-Critique Rating: 2

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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?

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Your Solution:

70% of the incoming radiation is 420 J/second for every m^2 of ice.

.012 m^3 of thickness for every square meter, the mass is a little less than 1000 kg/m^3 so there's about

12 kg of ice in every m^2

To melt 12 kg, it takes 12,000 g * 333.55 =4002600 J to melt the ice. At 420 J/sec, 4002600/420=9530 seconds or

2.65 hours.

confidence rating #$&*: 3

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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 energy is 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 about 12 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 roughly 10,000 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:OK

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Self-Critique Rating:

OK

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Question: `q004. A body with a 1/2 m^2 surface area, at temperature 25 Celsius, has an emissivity of approximately 1. It exchanges energy by radiation with a large surface at temperature -20 Celsius. At what net rate does it lose energy?

By what percent would the rate of energy loss change if the large surface was at temperature -270 Celsius?

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Your Solution:

P=1*5.67x10^-8*.5*(298^4-253^4)

P=107.4

P=1*5.67x10^-8*.5*(298^4-3^4)

P=223.6

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Self-Critique Rating:"

Self-critique (if necessary):

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Self-critique rating:

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