Solar constant is defined as energy received by Earth per `cm^(2)` per minute. Find the dimensions of solar constant.

Options

A. `[ML^(2)T^(-3)]`
B. `[M^(2)L^(0)T^(-1)]`
C. `[MT^(-3)]`
D. `[MLT^(-2)]`

Explanation

(c) Unit `=("energy")/(cm^(2)"minute")=([ML^(2)T^(-2)])/([L^(2)T])`
`:.` The dimensions of solar constant `=[MLT^(-3)]`