Date | May 2022 | Marks available | 1 | Reference code | 22M.1.SL.TZ1.29 |
Level | Standard level | Paper | Paper 1 | Time zone | 1 |
Command term | Question number | 29 | Adapted from | N/A |
Question
Three mechanisms that affect the composition of the atmosphere of the Earth are:
I. Loss of forests that would otherwise store carbon dioxide – CO2
II. Release of methane – CH4 by the digestive system of grazing animals
III. Increase of nitrous oxide – N2O due to extensive use of fertilizer
Which of these statements describe a process that contributes to global warming?
A. I and II only
B. I and III only
C. II and III only
D. I, II and III
Markscheme
D
Examiners report
This question was well answered by candidates, although option A was a frequent distractor suggesting candidates may be less clear about the role of nitrous oxide in global warming.
Syllabus sections
- 17N.2.SL.TZ0.5b.ii: Suggest how the difference between λS and λE helps to account for the greenhouse effect.
-
18M.2.SL.TZ1.6c.iii:
Calculate the peak wavelength in the intensity of the radiation emitted by the ice sample.
-
18M.1.SL.TZ2.29:
Three gases in the atmosphere are
I. carbon dioxide (CO2)
II. dinitrogen monoxide (N2O)
III. oxygen (O2).
Which of these are considered to be greenhouse gases?
A. I and II only
B. I and III only
C. II and III only
D. I, II and III
- 17N.1.SL.TZ0.29: The three statements give possible reasons why an average value should be used for the solar...
- 17M.1.SL.TZ1.29: Planet X and planet Y both emit radiation as black bodies. Planet X has a surface temperature...
- 16N.1.HL.TZ0.24: The solar constant is the intensity of the Sun’s radiation at A. the surface of the...
-
22M.1.SL.TZ1.30:
The diagram shows, for a region on the Earth’s surface, the incident, radiated and reflected intensities of the solar radiation.
What is the albedo of the region?
A.
B.
C.
D.
-
16N.1.HL.TZ0.25:
X and Y are two spherical black-body radiators that emit the same total power. The absolute temperature of X is half that of Y.
What is ?
A. 4
B. 8
C. 16
D. 32
-
18M.2.HL.TZ1.6c.i:
State what is meant by thermal radiation.
- 17M.1.SL.TZ1.15: Two pulses are travelling towards each other. What is a possible pulse shape when the...
- 18N.1.SL.TZ0.30: Light of intensity I0 is incident on a snow-covered area of Earth. In a model of this...
- 18N.2.SL.TZ0.6c: The atmosphere of Mars is composed mainly of carbon dioxide and has a pressure less than 1 %...
- 18N.2.HL.TZ0.8c.iii: The atmosphere of Mars is composed mainly of carbon dioxide and has a pressure less than 1 %...
-
18N.2.SL.TZ0.6b:
Determine, in K, the mean surface temperature of Mars. Assume that Mars acts as a black body.
- 19M.2.HL.TZ2.7a: Show that the intensity radiated by the oceans is about 400 W m-2.
- 19M.2.SL.TZ1.6a.ii: Another black body is on the Moon’s surface at point B. Outline, without calculation, why...
- 21N.2.HL.TZ0.6a.iii: Show that the equilibrium surface temperature of Titan is about 90 K.
- 19M.2.SL.TZ2.7a: Show that the intensity radiated by the oceans is about 400 W m-2.
- 19M.2.SL.TZ2.7b: Explain why some of this radiation is returned to the oceans from the atmosphere.
- 19M.1.SL.TZ2.30: The orbital radius of the Earth around the Sun is 1.5 times that of Venus. What is the...
-
19M.2.SL.TZ1.6a.i:
A black body is on the Moon’s surface at point A. Show that the maximum temperature that this body can reach is 400 K. Assume that the Earth and the Moon are the same distance from the Sun.
-
18M.2.HL.TZ1.6c.ii:
Discuss how the frequency of the radiation emitted by a black body can be used to estimate the temperature of the body.
- 17M.1.HL.TZ1.23: An object can lose energy through I. conductionII. convectionIII. radiation What are...
-
18M.1.SL.TZ2.30:
Mars and Earth act as black bodies. The and .
What is the value of ?
A.
B.
C.
D.
-
17M.1.SL.TZ2.29:
A room is at a constant temperature of 300 K. A hotplate in the room is at a temperature of 400 K and loses energy by radiation at a rate of P. What is the rate of loss of energy from the hotplate when its temperature is 500 K?
A. P
B. P
C. P
D. P
- 18M.1.SL.TZ1.30: The diagram shows a simple climate model for the Earth. What does this model predict for...
-
17M.1.SL.TZ1.30:
The average surface temperature of Mars is approximately 200 K and the average surface temperature of Earth is approximately 300 K. Mars has a radius half that of Earth. Assume that both Mars and Earth act as black bodies.
What is ?
A. 20
B. 5
C. 0.2
D. 0.05 - 19N.1.SL.TZ0.30: What is meant by the statement that the average albedo of the Moon is 0.1? A. 10% of the...
-
18M.2.HL.TZ1.6c.iii:
Calculate the peak wavelength in the intensity of the radiation emitted by the ice sample.
-
18N.2.HL.TZ0.8c.ii:
Determine, in K, the mean surface temperature of Mars. Assume that Mars acts as a black body.
-
20N.1.SL.TZ0.26:
The average temperature of the surface of a planet is five times greater than the average temperature of the surface of its moon. The emissivities of the planet and the moon are the same. The average intensity radiated by the planet is . What is the average intensity radiated by its moon?
A.
B.
C.
D.
-
21M.1.SL.TZ2.29:
A black-body radiator emits a peak wavelength of and a maximum power of . The peak wavelength emitted by a second black-body radiator with the same surface area is . What is the total power of the second black-body radiator?
A.
B.
C.
D.
-
17N.1.SL.TZ0.28:
A black body emits radiation with its greatest intensity at a wavelength of Imax. The surface temperature of the black body doubles without any other change occurring. What is the wavelength at which the greatest intensity of radiation is emitted?
A. Imax
B.
C.
D.
-
21M.2.SL.TZ1.4a.i:
Explain why the power incident on the planet is
-
21M.2.SL.TZ1.4b:
On average, the Moon is the same distance from the Sun as the Earth. The Moon can be assumed to have an emissivity e = 1 and an albedo = 0.13. The solar constant is 1.36 × 103 W m−2. Calculate the surface temperature of the Moon.
-
17N.2.SL.TZ0.5b.i:
Determine the mean temperature of the Earth.
-
18N.2.HL.TZ0.8c.i:
Show that the intensity of solar radiation at the orbit of Mars is about 600 W m–2.
-
21M.2.SL.TZ1.4a.ii:
The albedo of the planet is . The equilibrium surface temperature of the planet is T. Derive the expression
where e is the emissivity of the planet.
-
21M.1.SL.TZ1.29:
A black body at temperature T emits radiation with peak wavelength and power P. What is the temperature of the black body and the power emitted for a peak wavelength of ?
- 21M.1.SL.TZ1.30: In a simple climate model for a planet, the incoming intensity is 400 W m−2 and the...
- 21M.1.SL.TZ2.30: What is the main role of carbon dioxide in the greenhouse effect? A. It absorbs incoming...
-
18N.2.SL.TZ0.6a:
Show that the intensity of solar radiation at the orbit of Mars is about 600 W m–2.
-
17M.1.HL.TZ1.25:
The average albedo of glacier ice is 0.25.
What is ?
A. 0.25
B. 0.33
C. 2.5
D. 3.0
- 19M.1.SL.TZ1.29: A beaker containing 1 kg of water at room temperature is heated on a 400 W hot plate. The...
- 19M.2.HL.TZ2.7b: Explain why some of this radiation is returned to the oceans from the atmosphere.
- 19M.2.HL.TZ2.7ci: Calculate the additional intensity that must be lost by the oceans so that the water...
- 19M.2.HL.TZ2.7cii: Suggest a mechanism by which the additional intensity can be lost.
-
19M.2.SL.TZ1.6b:
The albedo of the Earth’s atmosphere is 0.28. Outline why the maximum temperature of a black body on the Earth when the Sun is overhead is less than that at point A on the Moon.
-
18M.2.SL.TZ1.6c.i:
State what is meant by thermal radiation.
-
18M.2.SL.TZ1.6c.ii:
Discuss how the frequency of the radiation emitted by a black body can be used to estimate the temperature of the body.
- 18M.1.HL.TZ1.24: The dashed line on the graph shows the variation with wavelength of the intensity of solar...
- 21N.1.SL.TZ0.30: Which is correct for a black-body radiator? A. The power it emits from a unit surface area...
- 21N.2.SL.TZ0.6a.iii: Show that the equilibrium surface temperature of Titan is about 90 K.
-
21N.2.SL.TZ0.6a.ii:
Titan has an atmosphere of nitrogen. The albedo of the atmosphere is 0.22. The surface of Titan may be assumed to be a black body. Explain why the average intensity of solar radiation absorbed by the whole surface of Titan is 3.1 W m−2
-
21N.2.HL.TZ0.6a.ii:
Titan has an atmosphere of nitrogen. The albedo of the atmosphere is 0.22. The surface of Titan may be assumed to be a black body. Explain why the average intensity of solar radiation absorbed by the whole surface of Titan is 3.1 W m−2.
- 22M.2.SL.TZ1.2d.i: State how energy is transferred from the inside of the metal pipe to the outside of the metal...
-
22M.2.SL.TZ1.2d.iii:
Describe one other method by which significant amounts of energy can be transferred from the pipe to the surroundings.
-
22M.2.SL.TZ1.2d.ii:
The missing section of insulation is 0.56 m long and the external radius of the pipe is 0.067 m. The emissivity of the pipe surface is 0.40. Determine the energy lost every second from the pipe surface. Ignore any absorption of radiation by the pipe surface.