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A laboratory technician drops a 0.0850-kg sample of unknown solid material, at 100.0\(^\circ\)C, into a calorimeter. The calorimeter can, initially at 19.0\(^\circ\)C, is made of 0.150 kg of copper and contains 0.200 kg of water. The final temperature of the calorimeter can and contents is 26.1\(^\circ\)C. Compute the specific heat of the sample.

Short Answer

Expert verified
The specific heat of the sample is approximately 1.0 J/g°C.

Step by step solution

01

Understand the Problem

We are dealing with a calorimetry problem where an unknown solid is placed in a calorimeter, reaching thermal equilibrium. We are to find the specific heat of the solid sample using the given initial and final temperatures.
02

Write the Heat Exchange Equation

Since no heat is lost to the surroundings, we apply the conservation of heat principle: the heat lost by the sample is equal to the heat gained by the copper and water in the calorimeter.\[ m_s c_s (T_{s,i} - T_f) = m_c c_c (T_f - T_{c,i}) + m_w c_w (T_f - T_{w,i}) \]where:- \(m_s = 0.0850\,\text{kg}\)- \(T_{s,i} = 100.0\, ^\circ\text{C}\)- \(T_f = 26.1\, ^\circ\text{C}\)- \(m_c = 0.150\,\text{kg}\)- \(c_c = 0.385\, \text{J/g} ^\circ\text{C}\)- \(T_{c,i} = 19.0\, ^\circ\text{C}\)- \(m_w = 0.200\,\text{kg}\)- \(c_w = 4.186\, \text{J/g} ^\circ\text{C}\)- \(T_{w,i} = 19.0\, ^\circ\text{C}\)
03

Substitute Known Values

Substituting the known values into the equation:\[0.085 \cdot c_s \cdot (100.0 - 26.1) = 0.150 \cdot 0.385 \cdot (26.1 - 19.0) + 0.200 \cdot 4.186 \cdot (26.1 - 19.0)\]
04

Simplify and Solve for Specific Heat

Calculate each term separately:- Heat lost by the sample: \(0.085 \cdot c_s \cdot 73.9\)- Heat gained by the copper: \(0.150 \cdot 0.385 \cdot 7.1 = 0.410025\, \text{J}\)- Heat gained by the water: \(0.200 \cdot 4.186 \cdot 7.1 = 5.94352\, \text{J}\)Combine the heat gained by the copper and water:\[0.410025 + 5.94352 = 6.353545 \, \text{J}\]Set up the equation for the specific heat:\[0.085 \cdot c_s \cdot 73.9 = 6.353545\]Solve for \(c_s\):\[c_s = \frac{6.353545}{0.085 \times 73.9} \approx 1.0 \, \text{J/g} ^\circ\text{C}\]
05

Conclusion

The specific heat of the unknown solid is calculated to be approximately \(1.0 \, \text{J/g} ^\circ\text{C}\). This is a reasonable result compared to familiar substances.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Specific Heat Capacity
Specific heat capacity refers to the amount of heat required to raise the temperature of 1 gram of a substance by 1 degree Celsius. Different materials require different amounts of heat to achieve the same temperature change. Metals, like copper, generally have low specific heats, meaning they warm up and cool down quickly. Water, on the other hand, has a high specific heat capacity, which allows it to absorb more heat before its temperature changes significantly.

Understanding the specific heat capacity is crucial when dealing with calorimetry problems—experiments designed to measure heat transfer. When a substance is introduced into a calorimeter, the specific heat capacity helps determine how much heat the substance will absorb or release to reach thermal equilibrium.
Heat Exchange Equation
The heat exchange equation is a mathematical representation of the heat transfer between substances involved in a calorimetry experiment. It is based on the principle that the total heat lost by hot objects must equal the total heat gained by cold objects, provided no heat is lost to the surroundings.

The equation used in the problem is expressed as:
  • \( m_s c_s (T_{s,i} - T_f) = m_c c_c (T_f - T_{c,i}) + m_w c_w (T_f - T_{w,i}) \)
This equation is set up to calculate how much heat is gained or lost based on the specific heat capacities, masses, and temperature changes of the substances involved.
Thermal Equilibrium
Thermal equilibrium occurs when two or more substances reach the same temperature and no further heat transfer occurs between them. In the context of the calorimetry problem, reaching thermal equilibrium means that the heat lost by the hotter substance (unknown sample) is equal to the heat gained by the colder substances (calorimeter can and water).

Thermal equilibrium is important because it signifies the end point of the heat exchange process. Once thermal equilibrium is achieved, we know that all possible heat transfer has occurred and the temperatures will stabilize. In the exercise provided, thermal equilibrium was reached at 26.1\(^\circ\)C.
Conservation of Heat
Conservation of heat is a fundamental concept in thermodynamics, stating that energy cannot be created or destroyed, only transferred. In the context of calorimetry, this means that the total amount of heat exchanged in an isolated system remains constant.

The problem highlights the conservation of heat through the heat exchange equation, where the sum of the heat lost must equal the sum of the heat gained.

By assuming no heat is lost to the environment, we ensure that all heat accounted for is used in calculating the specific heat capacity, as seen in the example where total heat lost by the unknown solid is equal to total heat gained by the calorimeter's contents.

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Most popular questions from this chapter

You have probably seen people jogging in extremely hot weather. There are good reasons not to do this! When jogging strenuously, an average runner of mass 68 kg and surface area 1.85 m\(^2\) produces energy at a rate of up to 1300 W, 80% of which is converted to heat. The jogger radiates heat but actually absorbs more from the hot air than he radiates away. At such high levels of activity, the skin's temperature can be elevated to around 33\(^\circ\)C instead of the usual 30\(^\circ\)C. (Ignore conduction, which would bring even more heat into his body.) The only way for the body to get rid of this extra heat is by evaporating water (sweating). (a) How much heat per second is produced just by the act of jogging? (b) How much net heat per second does the runner gain just from radiation if the air temperature is 40.0\(^\circ\)C (104\(^\circ\)F)? (Remember: He radiates out, but the environment radiates back in.) (c) What is the total amount of excess heat this runner's body must get rid of per second? (d) How much water must his body evaporate every minute due to his activity? The heat of vaporization of water at body temperature is \(2.42 \times 10{^6} J/kg\). (e) How many 750-mL bottles of water must he drink after (or preferably before!) jogging for a half hour? Recall that a liter of water has a mass of 1.0 kg.

In a container of negligible mass, 0.0400 kg of steam at 100\(^\circ\)C and atmospheric pressure is added to 0.200 kg of water at 50.0\(^\circ\)C. (a) If no heat is lost to the surroundings, what is the final temperature of the system? (b) At the final temperature, how many kilograms are there of steam and how many of liquid water?

A metal sphere with radius 3.20 cm is suspended in a large metal box with interior walls that are maintained at 30.0\(^\circ\)C. A small electric heater is embedded in the sphere. Heat energy must be supplied to the sphere at the rate of 0.660 J/s to maintain the sphere at a constant temperature of 41.0\(^\circ\)C. (a) What is the emissivity of the metal sphere? (b) What power input to the sphere is required to maintain it at 82.0\(^\circ\)C? What is the ratio of the power required for 82.0\(^\circ\)C to the power required for 41.0\(^\circ\)C? How does this ratio compare with 2\(^4\)? Explain.

A 4.00-kg silver ingot is taken from a furnace, where its temperature is 750.0\(^\circ\)C, and placed on a large block of ice at 0.0\(^\circ\)C. Assuming that all the heat given up by the silver is used to melt the ice, how much ice is melted?

The hot glowing surfaces of stars emit energy in the form of electromagnetic radiation. It is a good approximation to assume e = 1 for these surfaces. Find the radii of the following stars (assumed to be spherical): (a) Rigel, the bright blue star in the constellation Orion, which radiates energy at a rate of \(2.7 \times 10{^3}{^2} W\) and has surface temperature 11,000 K; (b) Procyon B (visible only using a telescope), which radiates energy at a rate of \(2.1 \times 10{^2}{^3} W\) and has surface temperature 10,000 K. (c) Compare your answers to the radius of the earth, the radius of the sun, and the distance between the earth and the sun. (Rigel is an example of a supergiant star, and Procyon B is an example of a white dwarf star.)

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