What does the constant k in Kepler’s third law (T2\=kr3) depend on for satellites?
T2 = 4π2GMEr3 for satellites, where k = 4π2GME. Thus, k depends on the mass of the central body (Earth) and universal constants, not the satellite’s mass. As per NCERT, applying relevant law/formula with correct units and sign convention leads to Mass of the central body. This satisfies dimensional consistency and physical conditions given, so option B is scientifically correct.
Ref: Halliday & Resnick, Fundamentals of Physics, 11th ed., Chapter 13: Gravitation.