A 500 g bar of copper (c = 387 P/kgoC) at 20.0 oC has 10,050 J of heat removed

from it. What is its final temperature?

The final temperature is 71.94 °C

Explanation:

Step 1: Data given

Mass of the copper bar = 500 grams

The specific heat of copper = 387 J/kg°C = 0.387 J/g°C

The initial temperature = 20.0 °C

Heat removed = 10050 J

Step 2: Calculate the final temperature

Q = m*c * ΔT

⇒with Q = the heat removed = 10050 J

⇒with m = the mass of the barr of copper = 500 grams

⇒with c= the specific heat of copper = 0.387 J/g°C

⇒with ΔT = the change of temperature = T2 -T1

10050 = 500 * 0.387 * ΔT

ΔT = 10050 / (500*0.387)

ΔT = 51.94 °C

Step 3: Calculate the final temperature

ΔT = T2 - T1

⇒with ΔT = the change of temperature = 51.94 °C

⇒with T2 = the final temperature = TO BE DETERMINED

⇒with T1 = the initial temperature = 20.0 °C

51.94 °C = T2 - 20.0°C

T2 = 51.94 °C + 20.0 °C

T2 = 71.94 °C

The final temperature is 71.94 °C

most historians agree that gabriel mouton, the vicar of st. paul’s church in lyons, france, is the “founding father” of the metric system. he proposed a decimal system of measurement in 1670. mouton based it on the length of one minute of arc of a great circle of the earth (now called a nautical mile, 1852 meters). he also proposed the swing-length of a pendulum with a frequency of one beat per second as the unit of length (about 25 cm). a pendulum beating with this length would have been fairly easy to produce, thus facilitating the widespread distribution of uniform standards. over the years, his work was revised, improved, and extended by a number of french scientists.

the political sponsor of weights and measures reform in the french revolutionary national assembly was the bishop of autun, better known as talleyrand. under his auspices, the french academy appointed several committees to carry out the work of developing a usable system of weights and measures for france. one of the committees recommended a decimalized measurement system based upon a length equal to one ten-millionth of the length of a quadrant of the earth’s meridian (i.e., one ten-millionth of the distance between the equator and the north pole).