Suppose you have a #25xx45xx2.5# #"cm"# steel bar whose density is #"7.8 g/cm"^3# at #22^@ "C"#. If #"3.8 kJ"# was imparted into it by solar energy, and the bar's specific heat capacity is #"0.49 J/g"^@ "C"#, to what temperature does it rise?
1 Answer
I get
This illustrates that heat capacity (
This overall will be using the equation for heat flow
#q = mC_PDeltaT# ,where:
#m# is the mass in#"g"# .#C_P# is the specific heat capacity in#"0.49 J/g"^@ "C"# at constant pressure, the amount of heat required to increase the temperature of one gram of substance by#1^@ "C"# .#DeltaT = T_2 - T_1# is the change in temperature in#""^@ "C"# .
The extra step here is to find the mass using the steel bar's volume
#D = m/V#
You gave the volume as
#"25 cm" xx "45 cm" xx "2.5 cm" = "2812.5 cm"^3#
So, the mass is given by
#m = DV = "7.8 g"/cancel("cm"^3) xx 2812.5 cancel("cm"^3)#
#=# #"21937.5 g"#
You also gave that the heat that went in was
#q = +"3.8 kJ" = +"38000 J"# (which you should remember to make sure is in the same energy unit,
#"J"# , as in#C_P# , and not#"kJ"# !)
and the specific heat capacity as
#C_P = "0.49 J/g"^@ "C"# .
As a result, we now have enough information to determine the final temperature,
#q = mC_PDeltaT#
#"38000 J" = (21937.5 cancel"g")("0.49 J/"cancel"g"^@ "C")(T_2 - 22^@ "C")#
#"38000 J" = overbrace(("10749.375 J/"^@ "C"))^("Heat Capacity, " mC_P)(T_2 - 22^@ "C")#
Divide over the heat capacity
#38000/10749.375 ""^@ "C" = 3.535^@ "C" = T_2 - 22^@ "C"#
Therefore, the new temperature is:
#color(blue)(T_2) = 22 + 3.535 = 25.535^@ "C"#
#= color(blue)(26^@ "C")# to two sig figs.