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Subjects

Geography

The heat budget of the earth

पृथ्वी का ऊष्मा बजट

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.

TOPIC PRACTICE

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Up to 25 questions from this page. Select your focus, then start.

25 questions

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Medium · Level 5
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  1. Surface absorption decreases
  2. Terrestrial radiation comes from the Sun
  3. Earth stops creating energy
  4. The atmosphere disappears
Medium · Level 5
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  1. The natural greenhouse effect keeps Earth warm enough for life
  2. The greenhouse effect blocks the Sun
  3. The greenhouse effect occurs only in oceans
  4. The greenhouse effect has no relation with temperature
Medium · Level 5
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  1. Scattering and reflection may increase
  2. The Sun's temperature will always decrease
  3. Earth's revolution will become faster
  4. Terrestrial radiation will stop forming
Medium · Level 5
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  1. Energy imbalance can cause temperature change
  2. Energy balance has no relation with temperature
  3. Only rivers change climate
  4. Solar radiation does not reach Earth
Medium · Level 5
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  1. It retains part of incoming solar radiation within the atmosphere
  2. It moves Earth away from the Sun
  3. It sends all longwaves to the Moon
  4. It stops ocean currents
Medium · Level 5
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  1. Shortwave from Sun to Earth and longwave from Earth to space
  2. Shortwave from Earth to Sun and sound from Sun to Earth
  3. Longwave from Moon to Earth and rain from Earth to Sun
  4. Clouds from ocean to Sun and soil from Sun to Earth
Medium · Level 5
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  1. Energy is stored as latent heat during evaporation
  2. Moisture creates the Sun
  3. Moisture always makes albedo zero
  4. Moisture changes Earth's axis
Medium · Level 5
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  1. Pressure differences and winds
  2. Only rock layers
  3. Permanent calmness of seas
  4. End of solar energy
Medium · Level 5
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  1. Temperature range could become very large
  2. Temperature range will always remain zero
  3. Day and night will end
  4. The Sun will not give radiation
Medium · Level 5
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  1. On energy input and output remaining nearly equal
  2. Only on the number of mountains
  3. Only on length of rivers
  4. Only on population growth
Medium · Level 5
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  1. Black asphalt road
  2. Fresh snow
  3. White cloud
  4. Bright icy peak
Medium · Level 5
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  1. Because some regions have heat surplus and others have heat deficit
  2. Because there is no radiation on Earth
  3. Because the Sun heats only the poles
  4. Because oceans are fixed rocks
Medium · Level 5
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  1. Low moisture and clear sky allow heat to gain and escape quickly
  2. The Sun does not rise there
  3. Clouds are always thick there
  4. Sand does not emit longwave radiation
Medium · Level 5
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  1. Because energy balance affects temperature pressure and winds
  2. Because it only tells population
  3. Because it tells soil age
  4. Because it only measures ocean depth
Medium · Level 5
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  1. Twenty seven units
  2. Two units
  3. Fourteen units
  4. Fifty one units
Medium · Level 5
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  1. Seventeen units
  2. Two units
  3. Forty eight units
  4. Sixty five units
Medium · Level 5
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  1. Six units
  2. Fifty one units
  3. Thirty four units
  4. Sixty five units
Medium · Level 5
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  1. One unit
  2. Two units
  3. Fourteen units
  4. Seventeen units
Medium · Level 5
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  1. It heats the surface and becomes the basis of terrestrial radiation
  2. It is completely reflected into space
  3. It is stored only in clouds
  4. It changes into sound energy
Medium · Level 5
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  1. The atmosphere also directly takes some incoming solar energy
  2. The atmosphere takes no energy
  3. Only the surface takes all energy
  4. The Moon heats the atmosphere
Medium · Level 5
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  1. Longwave terrestrial radiation
  2. Shortwave solar radiation
  3. Sound wave
  4. Ocean current
Medium · Level 5
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  1. Absorption of terrestrial longwave radiation
  2. Complete reflection of solar shortwaves
  3. Freezing of seawater
  4. Formation of mountains
Medium · Level 5
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  1. From fourteen units solar absorption and thirty four units terrestrial absorption
  2. From twenty seven units clouds and two units surface
  3. From seventeen units surface and six units scattering
  4. From fifty one units surface and thirty five units reflection
Medium · Level 5
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  1. By thirty five reflected seventeen direct and forty eight atmospheric energy
  2. By fifty one surface and fourteen atmospheric energy
  3. By twenty seven cloud and six scattering
  4. Only by sixty five absorbed energy
Medium · Level 5
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  1. Radiative balance
  2. Ocean salinity
  3. Wind direction
  4. Rainfall distribution

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