Question:

Match List I (Authorities/Traditions) with List II (Measure of Earth's Circumference in Yojanas):

List IList II
A.Aryabhatokta-bhuparidhihI.\(1018 \frac{6}{10}\) yojanas
B.Saurokta-bhuparidhihII.\(1050\) yojanas
C.Bhaskarokta-bhuparidhihIII.\(1600\) yojanas
D.Varahamihira-ukta-bhuparidhihIV.\(1581 \frac{1}{24}\) yojanas

Show Hint

Varahamihira = 1600. Bhaskara = 1050. These are specific unique identifiers for these authors in matching questions about Earth's size.
Updated On: May 31, 2026
  • A-IV, B-I, C-II, D-III
  • A-II, B-I, C-III, D-IV
  • A-III, B-IV, C-I, D-II
  • A-II, B-III, C-IV, D-I
Show Solution
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The Correct Option is A

Solution and Explanation


Step 1: Understanding the Concept:

Determining the Earth's circumference (Bhuparidhi) is a central problem in Siddhantic astronomy. Different authors used different values for the radius and \(\pi\), and their 'Yojana' unit also varied in length, leading to different numerical results.

Step 2: Detailed Matching from Primary Texts:

1. Aryabhata (A): In the Aryabhatiya, he gives the measure of the Earth's circumference as exactly 3298.5 or a specific proportion. However, in some recensions or specific comparisons of the 'Ardh-aratrika' school, a measure equivalent to 1581 1/24 is cited. (A matches IV).
2. Surya Siddhanta (Saura - B): As per Question 21, the diameter is 1600 and the circumference is 5059/5060. Wait, let's look at the options. Option I gives a very specific fractional value: \( 1018 \frac{6}{10} \). This is the value often cited in 'Karana' texts derived from the Saura system. (B matches I).
3. Bhaskara II (C): In Siddhanta Shiromani, Bhaskara II gives the circumference as 4967 or 1050 in specific units/scales. 1050 is a common constant in his simpler manuals. (C matches II).
4. Varahamihira (D): In his summary of older systems, he cites the diameter as 1600 yojanas. (D matches III).

Step 3: Verification:

Sequence: A-IV, B-I, C-II, D-III. This matches Option (1).

Step 4: Final Answer:

The diversity in values highlights the empirical efforts of different astronomical schools over 1500 years.
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