Step 1: Understanding the Concept:
In spherical geometry, every great circle has two poles. A pole is a point that is equidistant from every point on the circumference of that circle. In Indian astronomy, the pole of the Ecliptic (the Sun's path) is called the Kadamba.
Step 2: Detailed Explanation of Assertion (A):
The Ecliptic (Kranti-vritta) is the fundamental plane for measuring planetary longitudes. To define planetary latitude (Shara), we need a reference point perpendicular to this plane. This point is the 'Kadamba' (Pole of the Ecliptic). Understanding the geometry between the center of the sphere, the circle, and its pole is the basis for all spherical transformations. Thus, (A) is correct.
Step 3: Detailed Explanation of Reason (R):
The Reason gives the mathematical property of a "Pole." By definition, in a sphere, the pole of a great circle is at an angular distance of one quadrant (90 degrees or one 'Trijya' arc) from every point on that circle.
- If you are at the North Pole of the Earth, the Equator is always 90 degrees away from you in every direction.
- Similarly, every point on the Ecliptic is exactly 90 degrees away from the Kadamba. This property is used to calculate planetary latitudes and to perform the 'Ayana-valana' (transformation between ecliptic and equatorial coordinates).
Step 4: Synthesis:
The Assertion identifies the points, and the Reason explains the unique geometric property (the 90-degree distance) that makes those points useful as coordinates.
Step 5: Final Answer:
Both are correct and (R) explains (A).