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Geography

The heat budget of the earth

Class 11 Geography explores the heat budget of the Earth as the balance between incoming solar radiation and outgoing terrestrial radiation. Students learn how the atmosphere, land, oceans, clouds, and ice reflect, absorb, store, and redistribute heat, and why the Earth’s average temperature remains broadly stable. The topic connects this balance with the greenhouse effect, latitudinal differences in heating, and the movement of heat through the atmosphere and oceans.

Medium · Level 8 · 25 questions

TOPIC PRACTICE

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25 questions

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  1. Clouds can reflect a substantial part of incoming solar energy back into space
  2. Clouds draw all energy from Earth's surface
  3. Clouds create Earth's longwave energy
  4. Clouds eliminate the solar constant
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  1. Surface reflection is less than cloud reflection
  2. The surface sends all energy into space
  3. The surface sends solar energy to the Sun as longwave radiation
  4. The surface always has zero albedo
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  1. Solar radiation reaching the surface
  2. Terrestrial radiation arriving from the Sun
  3. Energy absorbed by the oceans
  4. Earth's temperature remaining at zero at all times
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  1. Terrestrial longwave radiation, sensible heat transfer, and latent heat transfer
  2. River deposition and earthquakes
  3. The Moon's revolution around Earth
  4. An increase in the solar constant
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  1. Atmospheric window
  2. Solar constant
  3. Rain shadow
  4. Ocean salinity
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  1. An energy surplus develops, creating a tendency for warming
  2. An energy deficit develops, causing immediate cooling
  3. Solar radiation will stop
  4. Albedo will necessarily increase
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  1. There is less cloud absorption and downward re-emission of longwave radiation
  2. The Sun shines more strongly at night
  3. The surface stops emitting radiation
  4. The atmosphere completely disappears at night
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  1. Daytime temperatures may be lower and nighttime temperatures higher, reducing the range.
  2. Temperatures will rise without limit during both day and night.
  3. Nighttime temperature will always be zero.
  4. Clouds will make incoming solar energy increase completely.
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  1. Less incoming solar energy is reflected, so more is absorbed by the surface.
  2. Outgoing longwave radiation stops completely.
  3. The solar constant becomes zero.
  4. The atmosphere stops receiving or exchanging energy.
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  1. Positive feedback: lower albedo leads to greater energy absorption, which can cause further warming and snow loss.
  2. Negative feedback: the Sun stops supplying energy as soon as snow melts.
  3. No feedback: snow and the exposed surface reflect exactly the same amount of sunlight.
  4. Positive feedback: snow has no albedo, so losing it reduces absorption.
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  1. Less direct escape of longwave energy to space
  2. A complete end to incoming solar energy
  3. Surface reflection becoming zero
  4. A decrease in ocean depth
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  1. They can absorb and store substantial heat
  2. They reflect all incoming energy
  3. They form clouds that stop rainfall
  4. They eliminate solar radiation
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  1. It changes albedo, moisture, evapotranspiration, and heat storage.
  2. It changes Earth’s distance from the Sun.
  3. It breaks Earth’s axis.
  4. It makes the atmosphere disappear.
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  1. Because moving air also transfers heat vertically.
  2. Because convection creates solar energy.
  3. Because convection makes albedo permanent.
  4. Because convection makes Earth solid.
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  1. It transports some surplus heat from low latitudes toward higher latitudes.
  2. The poles produce solar energy.
  3. There is no longwave radiation at the equator.
  4. Oceans are fixed rocks.
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  1. Global atmospheric and oceanic circulation
  2. River deposition alone
  3. Mountain building alone
  4. Soil formation alone
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  1. On a moist surface where enough water is available
  2. On a completely dry rocky surface
  3. In a snowy area with high albedo
  4. During a sunless night
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  1. Moisture, heat capacity, atmospheric conditions, and energy transfer also affect it
  2. Albedo has no relation to temperature
  3. Solar energy does not reach Earth
  4. Earth never emits longwave radiation
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  1. Between the surface and nearby air in contact with it
  2. Between the Sun and the Moon
  3. Between the ocean floor and outer space
  4. Between Earth’s core and the stars
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  1. Only emission of heat from Earth's surface
  2. Reflection by clouds and the surface, together with scattering by the atmosphere
  3. Only absorption by the oceans
  4. Only the release of latent heat
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  1. Net solar absorption decreases
  2. Net solar absorption remains unchanged
  3. Net solar absorption increases
  4. Terrestrial radiation stops
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  1. Because Earth is hotter than the Sun
  2. Because greenhouse gases absorb radiation selectively at different wavelengths
  3. Because clouds block only sound
  4. Because oceans do not emit longwave radiation
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  1. Because some energy is used for evaporation, transferred to the atmosphere as sensible heat, and emitted as longwave radiation
  2. Because energy is immediately destroyed
  3. Because the surface cannot interact with energy
  4. Because the Sun pulls the absorbed energy back
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  1. All the energy is being reflected
  2. Some energy is being used for evaporation or transferred elsewhere
  3. Solar radiation has not reached Earth
  4. The atmosphere is completely absent
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  1. The tendency toward cooling will increase
  2. The tendency toward warming may strengthen
  3. The energy balance will necessarily become zero
  4. Terrestrial radiation will become impossible

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