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NCERT Solutions

Lunar, Solar and Luni-Solar Calendars (11.2.1–11.2.3)"Keeping Time with the Skies"

8 questions✓ Free · step-by-step
  1. 13 marks

    How does a lunar calendar work, and why does it fall out of sync with the seasons over time?

    Hint. 12 lunar months of ~29.5 days each add up to less than a full solar year.

    ✦ A lunar calendar uses the day as its shortest unit, a month of about 29.5 days, and a lunar year of 12 lunar months. Since 12 lunar months add up to only about 354 days, while the seasons repeat on an approximately 365-day cycle, a lunar year falls about 11 days short of a solar year every time — so the same lunar month drifts steadily against the seasons from one lunar year to the next, never staying synchronised.

  2. 22 marks

    State the basic Gregorian leap year rule, and explain why it's needed.

    Hint. The solar year isn't a clean number of days — the leftover fraction has to go somewhere.

    ✦ In the Gregorian calendar, if a year is divisible by four, an extra leap day (29 February) is added, making that February 29 days instead of 28. This is needed because Earth actually takes nearly an extra quarter-day beyond 365 days to complete one revolution around the Sun — these extra quarter-days accumulate to roughly one full day every four years, and the leap day keeps the calendar synchronised with the seasons instead of slowly drifting.

  3. 33 marks

    A step further: why does the Gregorian calendar skip leap years in 1700, 1800 and 1900, but not in 1600 or 2000?

    Hint. Adding a leap day every four years actually overcorrects by a small amount — the century rule fixes that overcorrection.

    ✦ Adding a day every four years corrects for slightly more than the true extra time Earth takes, so over centuries this would push the calendar too far ahead of the seasons. To fix this, leap years are skipped every 100 years (as in 1700, 1800, 1900) — but skipping ALL century years would then make the calendar lag slightly behind, so every 400 years the leap year is added back in after all (as in 1600 and 2000). This two-level correction keeps the Gregorian calendar closely matched to the seasons over very long stretches of time.

  4. 43 marks

    Distinguish the tropical year from the sidereal year, and state which one the Gregorian calendar is based on.

    Hint. One is measured equinox-to-equinox; the other by the same stars returning to the same position at sunset.

    ✦ The tropical year is the time between successive spring equinoxes, and it is what the Gregorian calendar is based on. The sidereal year is the time for the same stars to rise again at sunset — Earth's true orbital period relative to the distant stars. The sidereal year is longer than the tropical year by a mere 20 minutes, which is why the difference between the two takes a very long time to become noticeable.

  5. 52 marks

    Why do modern astronomers prefer the sidereal year over the tropical year for tracking Earth's position in its orbit?

    Hint. One year length is tied to the equinox (a point that itself slowly shifts); the other is tied to the fixed background of distant stars.

    ✦ The sidereal year measures Earth's return to the same position relative to the distant, effectively fixed stars, which gives a direct, physically stable measure of one true orbit around the Sun — this is exactly why the chapter notes astronomers use the sidereal year specifically to keep track of the Earth's position in its orbit, even though the everyday calendar itself runs on the tropical year.

  6. 63 marks

    Our scientific heritage: what are Uttarayan and Dakshinayan, and how could ancient observers detect this pattern without knowing Earth orbits the Sun?

    Hint. The chapter ties this to where exactly on the horizon the Sun rises across the year.

    ✦ Careful observation shows the Sun does not always rise exactly in the East: in summer it rises a little north of East, and in winter a little south of East, with the extremes occurring at the solstices (around 21 June and 21 December). The Sun's apparent northward drift from December to June is called Uttarayan, and its apparent southward drift from June to December is Dakshinayan. Ancient observers, even without knowing Earth revolves around the Sun, could track this real, repeating pattern purely by noting where on the horizon the Sun rose, day after day, year after year — because patient sky-watching alone was enough to reveal the cycle.

  7. 72 marks

    What ancient Indian sources does the chapter cite as evidence for tracking this solstice pattern, and what do they record?

    Hint. One is a Vedic text quoted directly in Sanskrit; the other links the winter solstice to a specific constellation.

    ✦ The chapter quotes the Taittirīya Saṁhitā (verse 6.5.3), which records that 'the Sun moves southwards for six months and northwards for six months.' It also cites the Surya Siddhanta, which noted that the constellation Capricorn (called Makar in India) framed the Sun's position in the background around the winter solstice, which is why that month is still called Makar in the Indian calendar today.

  8. 83 marks

    What is a luni-solar calendar, and what is Adhika Maasa? Why does a luni-solar calendar need it but a purely solar calendar doesn't?

    Hint. 12 lunar months fall short of a solar year by about 11 days every year — that shortfall has to be corrected periodically.

    ✦ A luni-solar calendar primarily counts days and months using the Moon's phases, but makes periodic adjustments to stay in step with the solar year's cycle of seasons. Because 12 lunar months add up to only 354 days — about 11 days short of the solar year — this shortfall accumulates until, every 2–3 years, it becomes close to a full month; at that point an extra month, called Adhika Maasa (intercalary month), is inserted to catch the calendar back up. A purely solar calendar doesn't need this because it is already built directly from the 365-day solar year, with no lunar-month shortfall to correct.

Solutions written by the tuition.in editorial team and checked against NCERT Curiosity — Textbook of Science for Grade 8, Chapter 11 (hecu111.pdf), Reprint 2026-27, pages 170-189. Questions are referenced from the NCERT textbook for identification.

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