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Chapter 3. Motions of the Earth Geography class 6 in English Medium ncert book solutions Chapter-Review

Chapter 3. Motions of the Earth Chapter-Review – Complete NCERT Book Solutions for Class 6 Geography (English Medium). Get all chapter explanations, extra questions, solved examples and additional practice questions for Chapter 3. Motions of the Earth Chapter-Review to help you master concepts and score higher.

Chapter 3. Motions of the Earth Geography class 6 in English Medium ncert book solutions Chapter-Review

Chapter 3. Motions of the Earth Geography class 6 in English Medium ncert book solutions Chapter-Review

NCERT Solutions for Class 6 Geography play an important role in helping students understand the concepts of the chapter Chapter 3. Motions of the Earth clearly. This chapter includes the topic Chapter-Review, which is essential from both academic and examination point of view. The solutions provided here are prepared strictly according to the latest NCERT syllabus and follow the guidelines of CBSE to ensure accuracy and relevance. Each question is explained in a simple and student-friendly manner so that learners can grasp the concepts without confusion. These NCERT Solutions are useful for regular study, homework help, and exam preparation. All textbook questions are solved step by step to improve problem-solving skills and conceptual clarity. Students of Class 6 studying Geography can use these solutions to revise important topics, understand difficult questions, and practise effectively before examinations. The chapter Chapter 3. Motions of the Earth is explained in a structured way, making it easier for students to connect the theory with the topic Chapter-Review. By studying these updated NCERT Solutions for Class 6 Geography, students can build a strong foundation, boost their confidence, and score better marks in school and board exams.

Chapter 3. Motions of the Earth

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Chapter-Review

Last Update On: 06 March 2026

 

Chapter - Review:


  • The phenomenon of day and night is because of the rotation of the earth. Had there been no rotation, one side of the earth would perpetually have night, and temperatures would have dropped in this half. The other half would forever have a day, and in this half, temperatures would have risen. In such cases, It wpould nort be possible to sustain life on earth.
  • Earth takes 24 hours to complete one rotation and this is known as earth day.
  • 23 hr 56 min 4 sec is the actual time taken to complete on rotation, but for convenience purposes, it is taken to be 24 hours.
  • The movement of the earth on its own axis around the sun is termed a revolution.
  • The earth moves around the sun in an elliptical - shaped orbit.
  • It takes 365.25 days to complete one revolution. This is the time taken by the earth to go round an elliptical orbit with the sun at a focus.
  • We consider 365 days as one year, and the rest one - fourth of a day is added up for every four years to give us one extra day. This day is added up to the fourth year, and the year has 366 days. This year is called a leap year. This day is added up to the month of february.
  • In a leap year, february has 29 days instead of 28 days.
  • Seasons change due to change in the position of the Earth around the sun.
  • Because of the change in the position of earth, a year is divided into summer, winter, spring and autumn.
  • Summer solstice begins on 21st June in the Northern Hemisphere.
  • On this day, the Northern Hemisphere is tilted towards he sun.
  • Sun rays fall on the Tropic of cancer.
  • The North pole is inclined towards the sun and areas beyound the Arctic Circle experience continuous daylight for about six months.
  • The longest day and shortest night occur on 21st June, the summer Solstice.
  • The conditions in the Southern Hemisphere are reversed, and it is winter season there.
  • Winter solstice occurs on the 22nd of  December in the Northern Hemisphere.
  • The Southern Hemisphere at this time is tilted towards the sun.
  • The Sunrays fall on the Tropic of Capricorn in the Southern Hemisphere.
  • The Southern Hemisphere has loger days during this period and shorter night.
  • The conditions are reversed in the northern hemisphere.
  • The direct rays of the sun fall on the equator on 21st March and 23rd September.
  • The whole Earth experiences equal days and equal night because neither of the poles is tilted towards the sun.
  • On 23rd September, it is autumn season in the Northern hemisphere and spring season in the Southern hemisphere.
  • The opposite is the caes on 21st march when it is spring in the Northern hemisphere and autumn in the Southern hemisphere.
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