Thermal Conductivity, Stefan Boltzmann Law, Heat Transfer, Conduction, Convecton, Radiation, Physics

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00:00:00.290
let's begin our discussion with heat
00:00:02.990 00:00:03.000 transfer there's three ways in which an
00:00:05.889 00:00:05.899 object could transfer heat energy that
00:00:10.430 00:00:10.440 is conduction convection and radiation
00:00:14.049 00:00:14.059 now let's say if we have an object that
00:00:17.900 00:00:17.910 is at a relatively high temperature of
00:00:19.760 00:00:19.770 100 degrees Celsius and let's say the
00:00:23.300 00:00:23.310 temperature of the environment is 25
00:00:25.910 00:00:25.920 degrees Celsius if you touch the object
00:00:31.550 00:00:31.560 with let's say a metal rod heat will
00:00:36.080 00:00:36.090 flow from the object directly to the
00:00:37.970 00:00:37.980 metal whenever heat transfer occurs by
00:00:42.410 00:00:42.420 contact its conduction now the object
00:00:47.330 00:00:47.340 can also transfer heat by convection air
00:00:51.700 00:00:51.710 can carry away heat energy from the hot
00:00:54.380 00:00:54.390 object so whenever heat energy is
00:00:57.680 00:00:57.690 transferred by the movement of a fluid
00:00:59.709 00:00:59.719 be it a liquid or gas that's convection
00:01:03.410 00:01:03.420 a good example of convection is let's
00:01:06.620 00:01:06.630 say if you have a hot surface this is
00:01:13.130 00:01:13.140 going to heat up the air above it so hot
00:01:16.789 00:01:16.799 air will rise
00:01:18.670 00:01:18.680 whenever you heat up an object it
00:01:21.130 00:01:21.140 expands and density is mass over volume
00:01:26.320 00:01:26.330 so when the air is heated it expands the
00:01:29.800 00:01:29.810 volume decreases until I mean the volume
00:01:33.260 00:01:33.270 increases I take that back as it expands
00:01:36.499 00:01:36.509 and the density decreases whenever you
00:01:40.370 00:01:40.380 have a light object light objects tend
00:01:42.710 00:01:42.720 to float for example if you put an
00:01:44.569 00:01:44.579 object that's less dense and water is
00:01:46.580 00:01:46.590 going to flow an object that's more
00:01:48.679 00:01:48.689 dense than water will sink so hot air
00:01:52.280 00:01:52.290 because it's light it rises up to the
00:01:55.340 00:01:55.350 top cold air will sink and so you have
00:02:00.380 00:02:00.390 this heat transfer going on and this is
00:02:02.209 00:02:02.219 an example of convection where heat is
00:02:04.789 00:02:04.799 being transferred by the movement of a
00:02:06.289 00:02:06.299 fluid now the last example
00:02:12.170 00:02:12.180 is radiation so this hot object can
00:02:20.869 00:02:20.879 radiate heat in all directions
00:02:26.470 00:02:26.480 typically heat is transferred by an
00:02:28.940 00:02:28.950 infrared radiation and there's no
00:02:32.780 00:02:32.790 contact at all so think of the Sun the
00:02:36.199 00:02:36.209 Sun emits infrared rays and visible
00:02:39.199 00:02:39.209 light waves as well but that radiation
00:02:41.750 00:02:41.760 comes to us without the need of anything
00:02:46.129 00:02:46.139 in between because space is empty so
00:02:50.030 00:02:50.040 that's the third form of energy transfer
00:02:52.009 00:02:52.019 it's radiation there's no contact for
00:02:54.860 00:02:54.870 this type of heat transfer so make sure
00:02:58.399 00:02:58.409 you know the difference between
00:02:59.319 00:02:59.329 conduction which requires contact
00:03:02.259 00:03:02.269 convection which deals with the movement
00:03:06.530 00:03:06.540 of a fluid like a liquid or gas or
00:03:08.690 00:03:08.700 radiation which doesn't require any
00:03:11.629 00:03:11.639 medium to transfer heat energy now
00:03:19.460 00:03:19.470 there's an equation that can help you to
00:03:22.099 00:03:22.109 calculate the rate of heat flow whenever
00:03:24.409 00:03:24.419 two objects are in contact with each
00:03:26.599 00:03:26.609 other so let's say if you have something
00:03:32.479 00:03:32.489 that looks like this
00:03:37.860 00:03:37.870 on the left side let's say the
00:03:39.869 00:03:39.879 temperature is a hundred degrees Celsius
00:03:41.460 00:03:41.470 and on the right side it's only twenty
00:03:44.970 00:03:44.980 degrees Celsius you know heat is going
00:03:47.970 00:03:47.980 to flow from hot to cold
00:03:56.830 00:03:56.840 you can think of heat as being
00:03:59.320 00:03:59.330 associated with the energy of the
00:04:00.850 00:04:00.860 molecules the higher the temperature of
00:04:03.940 00:04:03.950 an object the more kinetic energy the
00:04:06.370 00:04:06.380 molecules have their vibrate and more
00:04:08.050 00:04:08.060 their collide and more and so these
00:04:10.690 00:04:10.700 molecular collisions will eventually
00:04:13.650 00:04:13.660 transfer their energy from one place to
00:04:15.790 00:04:15.800 another so heat will naturally flow from
00:04:19.720 00:04:19.730 hot to cold now there's an equation that
00:04:24.030 00:04:24.040 helps you to relate the amount of heat
00:04:26.830 00:04:26.840 that's going to flow in any given time
00:04:28.750 00:04:28.760 period so you need to know that the rate
00:04:34.360 00:04:34.370 of heat flow is proportional to the area
00:04:36.879 00:04:36.889 the cross-sectional area of the
00:04:39.659 00:04:39.669 conductor it also is dependent on the
00:04:45.040 00:04:45.050 temperature difference if these two
00:04:48.790 00:04:48.800 temperatures are the same there's going
00:04:50.740 00:04:50.750 to be no heat flow the greater the
00:04:53.740 00:04:53.750 temperature difference the greater the
00:04:55.659 00:04:55.669 amount of heat flow that will occur so
00:04:59.260 00:04:59.270 the rate of heat flow depends on the
00:05:00.520 00:05:00.530 change of temperature and also the
00:05:03.070 00:05:03.080 length between the hot and the cold
00:05:07.150 00:05:07.160 section so if you increase that distance
00:05:11.080 00:05:11.090 that should decrease the rate of the
00:05:13.480 00:05:13.490 heat flow here's the equation that you
00:05:16.990 00:05:17.000 need to know Q which represents the
00:05:19.900 00:05:19.910 amount of heat energy the change in Q
00:05:22.690 00:05:22.700 divided by T so that's the rate of heat
00:05:26.529 00:05:26.539 energy being transferred that's equal to
00:05:29.320 00:05:29.330 K which is the thermal conductivity of
00:05:31.719 00:05:31.729 the substance or the material that you
00:05:35.170 00:05:35.180 use in times the cross sectional area
00:05:38.159 00:05:38.169 times the difference in temperature
00:05:42.659 00:05:42.669 divided by L so now let's think about
00:05:47.440 00:05:47.450 what this means by the way what equation
00:05:52.330 00:05:52.340 what variable relates energy divided by
00:05:56.620 00:05:56.630 time you need to know that power is
00:05:59.920 00:05:59.930 equal to energy over time energy has
00:06:03.400 00:06:03.410 units joules time is in seconds so you
00:06:07.810 00:06:07.820 need to know that one watt which is the
00:06:09.770 00:06:09.780 of power that's equal to one Joule per
00:06:11.900 00:06:11.910 second if we increase the value of K
00:06:20.050 00:06:20.060 which is the thermal conductivity the
00:06:23.540 00:06:23.550 rate of heat flow will increase so this
00:06:27.080 00:06:27.090 which is equal to P that's going to
00:06:29.930 00:06:29.940 increase now the rate of heat flow is
00:06:33.909 00:06:33.919 also proportional to the cross sectional
00:06:36.260 00:06:36.270 area if you increase a the power or the
00:06:40.250 00:06:40.260 rate of heat flow will increase as well
00:06:43.720 00:06:43.730 basically anything in the numerator is
00:06:46.010 00:06:46.020 going to be proportional to the quantity
00:06:48.740 00:06:48.750 on the left side in this case the power
00:06:49.940 00:06:49.950 so if we increase the change in
00:06:51.830 00:06:51.840 temperature the rate of heat flow will
00:06:54.380 00:06:54.390 increase as well but notice that it's
00:06:57.920 00:06:57.930 inversely related to L if you increase L
00:07:01.600 00:07:01.610 the energy transferred per second will
00:07:04.219 00:07:04.229 decrease let's try this problem so we
00:07:11.180 00:07:11.190 have a glass window let's see if I can
00:07:14.770 00:07:14.780 draw a nice glass window
00:07:33.260 00:07:33.270 and the glass window is 1.4 centimeters
00:07:36.470 00:07:36.480 thick it has a length of 2 meters and a
00:07:47.210 00:07:47.220 width of 3 meters and let's say the
00:07:51.340 00:07:51.350 inside temperature is 25 degrees Celsius
00:07:55.850 00:07:55.860 and the outside temperature is 22 so we
00:08:00.650 00:08:00.660 know heat is going to flow from the
00:08:02.810 00:08:02.820 inside to the outside from hot to cold
00:08:07.330 00:08:07.340 now what we want to know is what is the
00:08:09.620 00:08:09.630 rate of heat flow through a glass window
00:08:14.170 00:08:14.180 now we're given the thermal conductivity
00:08:16.250 00:08:16.260 of a typical glass window so how can we
00:08:20.780 00:08:20.790 find a rate of heat flow now let's
00:08:28.550 00:08:28.560 calculate Delta Q over T that represents
00:08:31.790 00:08:31.800 the rate of heat flow which is basically
00:08:34.390 00:08:34.400 the power in units of watts so using the
00:08:39.680 00:08:39.690 equation we know it's K times a times
00:08:42.980 00:08:42.990 the change in temperature divided by L
00:08:47.260 00:08:47.270 so let's get rid of this so K which is
00:08:54.650 00:08:54.660 the thermal conductivity
00:08:55.850 00:08:55.860 that's 0.8 for joules per second per
00:09:01.790 00:09:01.800 meter per Celsius now the area is 2 by 3
00:09:09.470 00:09:09.480 so it's 2 meters by 3 meters which is 6
00:09:13.030 00:09:13.040 square meters and the change in
00:09:16.400 00:09:16.410 temperature if you're not sure whether
00:09:18.950 00:09:18.960 the temperature should be in Celsius or
00:09:20.750 00:09:20.760 Kelvin you can go with Kelvin but
00:09:23.390 00:09:23.400 anytime you have a change in temperature
00:09:24.820 00:09:24.830 Celsius can work so the change in
00:09:27.620 00:09:27.630 temperature is 3 degrees Celsius 25
00:09:30.020 00:09:30.030 minus 22 divided by the length L is
00:09:37.970 00:09:37.980 basically the thickness of the glass
00:09:40.030 00:09:40.040 however we do need to convert it to
00:09:42.650 00:09:42.660 meters one point 100 centimeters is
00:09:46.430 00:09:46.440 basically
00:09:46.910 00:09:46.920 one meter so you need to divide 1.4
00:09:49.069 00:09:49.079 centimeters by 100 which is point zero
00:09:51.650 00:09:51.660 one four meters so notice the units
00:09:56.440 00:09:56.450 Celsius will cancel and square meters
00:10:00.170 00:10:00.180 will cancel with these two so we're left
00:10:03.740 00:10:03.750 with the unit joules per second which is
00:10:06.620 00:10:06.630 basically Watts so it's going to be
00:10:12.740 00:10:12.750 point eighty four times six times three
00:10:15.889 00:10:15.899 divided by point zero one four so the
00:10:19.250 00:10:19.260 answer is 1080 watts so basically every
00:10:27.500 00:10:27.510 second a thousand and eighty joules of
00:10:29.990 00:10:30.000 heat energy is being transferred to this
00:10:33.860 00:10:33.870 glass window let's try this problem if a
00:10:43.460 00:10:43.470 thousand eighty joules of heat energy is
00:10:45.530 00:10:45.540 transferred through the window every
00:10:46.939 00:10:46.949 second how much energy will be
00:10:48.889 00:10:48.899 transferred in a month so we know that
00:10:51.769 00:10:51.779 power is equal to energy divided by time
00:10:54.350 00:10:54.360 so the energy is the power multiplied by
00:10:57.079 00:10:57.089 the time the time is one month but we
00:11:00.769 00:11:00.779 need to convert answer seconds on
00:11:06.230 00:11:06.240 average there's 30 days per month and
00:11:10.840 00:11:10.850 it's 24 hours in a day and there's about
00:11:17.139 00:11:17.149 60 minutes in an hour and 60 seconds in
00:11:20.120 00:11:20.130 a minute
00:11:20.480 00:11:20.490 so there's 3,600 seconds in a single
00:11:23.689 00:11:23.699 hour so if we multiply 30 times 24 times
00:11:29.410 00:11:29.420 3600 you should get a time value of 2
00:11:34.100 00:11:34.110 million 592 seconds in a single month so
00:11:39.889 00:11:39.899 now let's calculate the energy so we
00:11:43.280 00:11:43.290 have a thousand 80 joules of energy
00:11:47.720 00:11:47.730 being transferred every second so if we
00:11:50.210 00:11:50.220 multiply by this many seconds we should
00:11:54.319 00:11:54.329 get the total energy transferred in a
00:11:57.620 00:11:57.630 single month
00:11:59.990 00:12:00.000 so the final answer is about two point
00:12:03.990 00:12:04.000 seven nine nine times 10 to the ninth
00:12:10.920 00:12:10.930 power so that's how many joules is being
00:12:15.630 00:12:15.640 transferred through this window in a
00:12:17.040 00:12:17.050 single month now let's move on to
00:12:19.920 00:12:19.930 another topic sometimes you might have
00:12:27.780 00:12:27.790 to deal with our values the r-value
00:12:32.240 00:12:32.250 basically describes the thermal
00:12:34.560 00:12:34.570 resistance of an insulator it's equal to
00:12:39.900 00:12:39.910 L divided by K where L is the thickness
00:12:47.730 00:12:47.740 of the material which is the distance
00:12:52.260 00:12:52.270 between the hot and cold section of the
00:12:55.050 00:12:55.060 material so notice that K and R are
00:12:59.790 00:12:59.800 inversely related
00:13:00.860 00:13:00.870 whenever K goes up R goes down and R and
00:13:07.890 00:13:07.900 L are directly related if L goes up R
00:13:11.880 00:13:11.890 goes up so whenever you increase the
00:13:14.850 00:13:14.860 thickness of material you increase its
00:13:17.970 00:13:17.980 insulation its thermal resistance if you
00:13:22.770 00:13:22.780 increase the conductivity while the
00:13:25.320 00:13:25.330 insulation decreases so can are are
00:13:28.530 00:13:28.540 inversely related so for example let's
00:13:36.990 00:13:37.000 consider a metal such as silver metals
00:13:44.070 00:13:44.080 are excellent conductors of heat and so
00:13:48.660 00:13:48.670 for silver the thermal conductivity is
00:13:51.150 00:13:51.160 very high it's 420 joules per second per
00:13:55.290 00:13:55.300 meter per Celsius in the case of glass
00:14:00.710 00:14:00.720 glass has a thermal conductivity of 0.8
00:14:05.400 00:14:05.410 for
00:14:11.340 00:14:11.350 fiberglass has a thermal conductivity
00:14:15.280 00:14:15.290 value of point zero four eight now we
00:14:21.820 00:14:21.830 can see why silver which is a metal is
00:14:25.140 00:14:25.150 an excellent conductor of heat metals
00:14:29.620 00:14:29.630 conduct heat very well due to the free
00:14:32.470 00:14:32.480 flowing electrons that are found in
00:14:33.910 00:14:33.920 metals so it has the highest K value
00:14:36.390 00:14:36.400 therefore silver should have a very low
00:14:39.360 00:14:39.370 r-value now glass is an insulator that
00:14:45.280 00:14:45.290 doesn't really conduct heat very well
00:14:46.890 00:14:46.900 but fiberglass is a better insulator
00:14:49.720 00:14:49.730 because it has a lower kVAL which means
00:14:52.360 00:14:52.370 fiberglass has a relatively high r-value
00:14:56.820 00:14:56.830 so just keep this in mind k describes
00:14:59.530 00:14:59.540 the thermal conductivity of a material
00:15:01.740 00:15:01.750 so if it has a high K value it's a heat
00:15:05.170 00:15:05.180 conductor if it has a low K value it's
00:15:07.090 00:15:07.100 an insulator the r-value describes
00:15:10.450 00:15:10.460 insulation a substance with a low
00:15:13.960 00:15:13.970 r-value is a good heat conductor and the
00:15:17.350 00:15:17.360 substance with a high r-value is a good
00:15:20.110 00:15:20.120 insulator now let's work on this problem
00:15:25.630 00:15:25.640 the r-value for a certain building
00:15:27.910 00:15:27.920 material that is two point four
00:15:29.500 00:15:29.510 millimeters thick is one point five what
00:15:32.020 00:15:32.030 is the R value if the thickness is
00:15:33.640 00:15:33.650 increased to four point eight
00:15:35.050 00:15:35.060 millimeters we know that R is directly
00:15:40.600 00:15:40.610 related to Al but inversely related to K
00:15:43.500 00:15:43.510 so if we increase out R is going to
00:15:46.210 00:15:46.220 increase now let's say if we double the
00:15:49.720 00:15:49.730 value of L because it increased from two
00:15:52.480 00:15:52.490 point four to four point eight and
00:15:54.910 00:15:54.920 increase by a factor of two what should
00:15:58.870 00:15:58.880 happen to the r-value because R is
00:16:02.860 00:16:02.870 proportional to L to the first power the
00:16:05.280 00:16:05.290 r-value should double as well so it
00:16:08.440 00:16:08.450 should equal three point oh now we can
00:16:12.760 00:16:12.770 come up with an equation that relates R
00:16:14.530 00:16:14.540 now let's write the ratio between r2 and
00:16:19.150 00:16:19.160 r1
00:16:20.600 00:16:20.610 artoo is going to be l 2 divided by K
00:16:23.280 00:16:23.290 and R 1 is L 1 divided by K for the same
00:16:27.480 00:16:27.490 substance K is the same so we don't need
00:16:29.700 00:16:29.710 to write a subscript for it which means
00:16:31.950 00:16:31.960 we can cancel K and then we're going to
00:16:34.860 00:16:34.870 get this equation r2 divided by r1 is
00:16:37.290 00:16:37.300 equal to L 2 divided by L 1 so R 1 is
00:16:46.520 00:16:46.530 1.5 we're looking for r2 l1 is two point
00:16:51.060 00:16:51.070 four millimeters l2 is four point eight
00:16:54.260 00:16:54.270 so if we cross multiply this is going to
00:16:57.480 00:16:57.490 be two point four times r2 and that's
00:17:00.630 00:17:00.640 equal to one point five times four point
00:17:05.610 00:17:05.620 eight which is seven point two and to
00:17:09.540 00:17:09.550 find our two is to divide both sides by
00:17:11.310 00:17:11.320 two point four seven point two divided
00:17:13.260 00:17:13.270 by two point four is three so now we can
00:17:18.600 00:17:18.610 answer the second part of the problem
00:17:24.410 00:17:24.420 let's use the same equation so if we
00:17:27.600 00:17:27.610 decrease the thickness the R value
00:17:29.850 00:17:29.860 should be less than one point five so R
00:17:33.570 00:17:33.580 1 is still 1 point five we're looking
00:17:35.130 00:17:35.140 for are two again l1 is two point four
00:17:38.310 00:17:38.320 but l2 is one point seven so let's cross
00:17:41.490 00:17:41.500 multiply one point five times one point
00:17:44.400 00:17:44.410 seven is about two point 55 and that's
00:17:49.320 00:17:49.330 equal to two point four r2 so now two
00:17:53.340 00:17:53.350 point 55 divided by two point four will
00:17:55.860 00:17:55.870 give us an r2 value of one point zero
00:17:58.500 00:17:58.510 six so as you can see it's the less than
00:18:03.630 00:18:03.640 one point five now the next thing that
00:18:08.400 00:18:08.410 we need to quantify is the amount of
00:18:10.890 00:18:10.900 heat energy that flows by means of
00:18:14.400 00:18:14.410 radiation so let's say if we have an
00:18:16.890 00:18:16.900 object
00:18:21.409 00:18:21.419 every object emits thermal radiation as
00:18:25.180 00:18:25.190 you increase the temperature of the
00:18:27.259 00:18:27.269 object the more thermal radiation it's
00:18:30.829 00:18:30.839 going to emit and the equation that you
00:18:33.109 00:18:33.119 need it's called the Stefan Boltzmann
00:18:35.509 00:18:35.519 equation the rate of heat flow is equal
00:18:41.419 00:18:41.429 to the emissive the emissivity there we
00:18:45.469 00:18:45.479 go
00:18:45.799 00:18:45.809 almost pronounce that wrong times the
00:18:50.089 00:18:50.099 Stefan Boltzmann constant times the area
00:18:53.719 00:18:53.729 of the object times the temperature
00:18:57.949 00:18:57.959 raised to the fourth power so this is
00:19:00.829 00:19:00.839 how much energy that is being emitted by
00:19:03.529 00:19:03.539 this particular object the emissivity
00:19:07.369 00:19:07.379 factor varies between 0 to 1 an object
00:19:14.539 00:19:14.549 with an emissivity of 1 is an object
00:19:18.289 00:19:18.299 that is a good absorber of heat and also
00:19:21.349 00:19:21.359 it can emit heat very efficiently if the
00:19:25.369 00:19:25.379 emissivity factor is close to zero that
00:19:28.039 00:19:28.049 means that it really is not good in
00:19:30.319 00:19:30.329 emitting heat energy now this particular
00:19:35.119 00:19:35.129 value is 5.67
00:19:39.909 00:19:39.919 times 10 to the minus 8 watts per square
00:19:45.709 00:19:45.719 meter per Kelvin to the fourth power so
00:19:50.989 00:19:50.999 that's the Stefan Boltzmann constant and
00:19:52.879 00:19:52.889 a is the area in square meters and
00:19:55.959 00:19:55.969 temperature notice that we don't have a
00:19:58.310 00:19:58.320 change in temperature temperature has to
00:20:00.949 00:20:00.959 be in Kelvin not Celsius for this to
00:20:02.629 00:20:02.639 work in this problem we have a sphere
00:20:11.440 00:20:11.450 with a radius of 25 centimeters which is
00:20:17.799 00:20:17.809 0.25 meters
00:20:22.980 00:20:22.990 and this fear is at a temperature of 27
00:20:27.210 00:20:27.220 degrees Celsius the temperature of the
00:20:30.480 00:20:30.490 surroundings is positive two degrees
00:20:33.540 00:20:33.550 Celsius so heat is going to flow out of
00:20:36.960 00:20:36.970 the sphere into the surroundings
00:20:42.150 00:20:42.160 however this heat flow is the net heat
00:20:45.630 00:20:45.640 flow in this problem we need to
00:20:47.460 00:20:47.470 understand that he not only leaves the
00:20:50.430 00:20:50.440 sphere but also enters this view however
00:20:55.530 00:20:55.540 the amount of heat that's emitted by the
00:20:58.080 00:20:58.090 sphere is greater than the amount of
00:21:00.419 00:21:00.429 heat that is absorbed by the sphere from
00:21:03.900 00:21:03.910 the surroundings so that there's a net
00:21:06.000 00:21:06.010 heat flow of heat leaving the sphere so
00:21:10.080 00:21:10.090 generally speaking heat will flow from
00:21:11.610 00:21:11.620 hot to cold even though goes both ways
00:21:14.430 00:21:14.440 the net heat flow is from hot to cold
00:21:18.049 00:21:18.059 now let's work on part a so let's move
00:21:21.870 00:21:21.880 this somewhere else so what is the rate
00:21:26.490 00:21:26.500 of heat energy leaving the sphere so
00:21:28.680 00:21:28.690 let's use the equation Delta Q divided
00:21:31.350 00:21:31.360 by delta T is equal to e theta times a
00:21:36.299 00:21:36.309 times the change or just times T raised
00:21:39.600 00:21:39.610 to the fourth power so the emissivity
00:21:43.290 00:21:43.300 factor in this problem is 0.42
00:21:47.930 00:21:47.940 the constant is always going to be the
00:21:50.580 00:21:50.590 same and that is five point six seven
00:21:57.140 00:21:57.150 times ten to the minus eight now what
00:22:03.270 00:22:03.280 about the area of the sphere the area is
00:22:06.180 00:22:06.190 equal to four pi times R squared so
00:22:11.240 00:22:11.250 point twenty five squared
00:22:13.490 00:22:13.500 make sure R is in meters times four pi
00:22:16.260 00:22:16.270 is about 0.785 now we need to multiply
00:22:24.510 00:22:24.520 it by the temperature of the sphere
00:22:26.310 00:22:26.320 which is 27 degrees Celsius but we need
00:22:28.799 00:22:28.809 to convert it to Kelvin to find the
00:22:31.049 00:22:31.059 temperature in Kelvin add the Celsius
00:22:33.150 00:22:33.160 temperature plus 273
00:22:36.240 00:22:36.250 so this is going to be 300 Kelvin raised
00:22:38.970 00:22:38.980 to the fourth power 300 raised to the
00:22:42.600 00:22:42.610 fourth power is a big number
00:22:43.890 00:22:43.900 it's about 8.1 billion if we multiply
00:22:50.820 00:22:50.830 that by point seven eight five and point
00:22:56.310 00:22:56.320 four two and the other number you should
00:23:02.310 00:23:02.320 get a value of 150 one point four watts
00:23:08.340 00:23:08.350 so every second the sphere is emitting
00:23:15.590 00:23:15.600 150 one point four joules of energy so
00:23:20.190 00:23:20.200 that's how much energy its emitting by
00:23:22.440 00:23:22.450 radiation
00:23:23.220 00:23:23.230 now how much energy is going into it by
00:23:26.340 00:23:26.350 radiation we need to use the same
00:23:29.430 00:23:29.440 equation by the way let's put a negative
00:23:31.919 00:23:31.929 sign since this is how much energy to
00:23:36.029 00:23:36.039 lose in every second now Part B to find
00:23:40.470 00:23:40.480 the energy that's entering into the
00:23:42.570 00:23:42.580 sphere we need to use the temperature of
00:23:44.669 00:23:44.679 the surroundings so everything is going
00:23:46.590 00:23:46.600 to be the same the 0.35 the constant and
00:23:50.299 00:23:50.309 the area is going to stay the same
00:23:59.830 00:23:59.840 the only difference is the Kelvin
00:24:01.389 00:24:01.399 temperature so we need to add 273 to 2
00:24:05.049 00:24:05.059 degrees Celsius to get a Kelvin
00:24:06.459 00:24:06.469 temperature of 275 raised to the 4th
00:24:09.849 00:24:09.859 power so if we multiply everything
00:24:20.270 00:24:20.280 I do need to fix something I don't know
00:24:22.010 00:24:22.020 why I have point three five that should
00:24:24.680 00:24:24.690 be a point for tune
00:24:36.090 00:24:36.100 so this is equal to a hundred and 6.9
00:24:40.920 00:24:40.930 watts so that's the answer to Part B so
00:24:49.590 00:24:49.600 in Part A the amount of energy that the
00:24:52.380 00:24:52.390 sphere is losing is 150 1.4 watts Part B
00:24:59.880 00:24:59.890 the amount of energy that the sphere
00:25:03.300 00:25:03.310 gains per second is positive 106 point 9
00:25:08.970 00:25:08.980 watts which means that there's a net
00:25:13.140 00:25:13.150 loss if we combine these two
00:25:24.380 00:25:24.390 of 44.5 watts so what this means is that
00:25:31.280 00:25:31.290 every second the sphere loses 44.5
00:25:35.510 00:25:35.520 joules of energy every second and we
00:25:39.170 00:25:39.180 could see why is losing energy the
00:25:41.090 00:25:41.100 temperature of the sphere is greater
00:25:43.490 00:25:43.500 than the temperature of the surroundings
00:25:45.470 00:25:45.480 so that means that the sphere emits more
00:25:48.710 00:25:48.720 radiant energy than the amount of energy
00:25:52.040 00:25:52.050 it absorbs from the environment but when
00:25:54.920 00:25:54.930 the temperature of the environment is
00:25:56.270 00:25:56.280 greater than the temperature of the
00:25:57.440 00:25:57.450 sphere the environment will emit more
00:25:59.930 00:25:59.940 radiation into the sphere than the
00:26:02.030 00:26:02.040 amount that the sphere will already into
00:26:04.100 00:26:04.110 the environment so whichever object has
00:26:08.180 00:26:08.190 the higher temperature it's going to
00:26:09.800 00:26:09.810 emit a greater amount of heat then the
00:26:13.550 00:26:13.560 amount of heat that is absorbed by the
00:26:15.200 00:26:15.210 surroundings so with these problems you
00:26:18.680 00:26:18.690 have to think of the like how much
00:26:20.810 00:26:20.820 energy is going in how much is going out
00:26:22.730 00:26:22.740 and what's the net flow of the energy so
00:26:25.820 00:26:25.830 this is the answer for Part C now what
00:26:28.730 00:26:28.740 about Part D so we know the change in
00:26:31.880 00:26:31.890 power is forty four point five watts how
00:26:38.450 00:26:38.460 long will it take for the sphere to lose
00:26:41.440 00:26:41.450 1 million joules of energy so remember
00:26:47.930 00:26:47.940 one why is one Joule per second so the
00:26:51.320 00:26:51.330 sphere it loses forty five point forty
00:26:54.680 00:26:54.690 four point five joules per second you
00:26:59.390 00:26:59.400 know that power is equal to energy
00:27:01.130 00:27:01.140 divided by time and energy is power
00:27:04.220 00:27:04.230 multiplied by time in this problem we're
00:27:06.770 00:27:06.780 looking for the time the time is the
00:27:09.740 00:27:09.750 energy divided by the power so let's
00:27:13.280 00:27:13.290 start with the energy which is 1 times
00:27:14.810 00:27:14.820 10 to the six joules and we're going to
00:27:17.630 00:27:17.640 divide it by the power which is forty
00:27:21.950 00:27:21.960 four point five joules per second notice
00:27:26.720 00:27:26.730 that the unit joules cancel so we simply
00:27:30.470 00:27:30.480 have to divide these two numbers one
00:27:32.270 00:27:32.280 times ten to the six divided by forty
00:27:34.820 00:27:34.830 four point five is about
00:27:37.920 00:27:37.930 twenty two thousand four hundred and
00:27:40.320 00:27:40.330 seventy two seconds now how many hours
00:27:45.990 00:27:46.000 is that because that's a long time in
00:27:47.820 00:27:47.830 seconds whenever you have a time value
00:27:52.920 00:27:52.930 that's very high in seconds converted to
00:27:55.050 00:27:55.060 a more practical unit so let's convert
00:27:57.780 00:27:57.790 it to hours we know that there's 3,600
00:28:02.760 00:28:02.770 seconds in a single hour so this is
00:28:11.490 00:28:11.500 about 6.2 hours so that's how long it's
00:28:16.260 00:28:16.270 going to take for the sphere to lose 1
00:28:19.710 00:28:19.720 million joules of energy assuming of
00:28:21.300 00:28:21.310 course if the rate of heat flow is
00:28:23.490 00:28:23.500 constant that is if the temperature of
00:28:25.740 00:28:25.750 the sphere and the temperature of the
00:28:27.660 00:28:27.670 surroundings if it stays at that level
00:28:31.010 00:28:31.020 now we know in reality the temperature
00:28:33.480 00:28:33.490 of the sphere is going to decrease and
00:28:35.130 00:28:35.140 as that happens the rate of the rate of
00:28:38.730 00:28:38.740 heat flow will decrease as well because
00:28:40.410 00:28:40.420 it's depend on temperature so as the
00:28:43.440 00:28:43.450 temperature decreases the rate of heat
00:28:46.860 00:28:46.870 flow will decrease as well so it's not
00:28:48.480 00:28:48.490 really constant but we're going to
00:28:51.720 00:28:51.730 assume as if it's constant if it is it's
00:28:54.960 00:28:54.970 about 6.2 hours but in reality since the
00:28:59.310 00:28:59.320 temperature is decreasing over time the
00:29:01.740 00:29:01.750 rate of heat energy that's leaving the
00:29:03.480 00:29:03.490 sphere will decrease and so it's going
00:29:05.880 00:29:05.890 to take longer for the spheres to lose a
00:29:09.390 00:29:09.400 million joules of energy so it's really
00:29:11.940 00:29:11.950 longer or greater than 6.2 hours but
00:29:16.230 00:29:16.240 we're going to keep this problem simple
00:29:17.430 00:29:17.440 we're going to assume that the rate of
00:29:19.470 00:29:19.480 heat flow stays constant
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