The gravitational constant \( G \) appears in Newton's law of gravitation:
\[
F = \frac{G m_1 m_2}{r^2}
\]
where:
- \( F \) is the force with dimensional formula \( [M L T^{-2}] \)
- \( m_1 \) and \( m_2 \) are masses with dimensional formula \( [M] \)
- \( r \) is the distance with dimensional formula \( [L] \)
The dimensional formula of \( G \) can be derived as follows:
\[
[F] = \frac{[G] [M]^2}{[L]^2}
\]
Substituting the dimensional formulas:
\[
[M L T^{-2}] = \frac{[G] M^2}{L^2}
\]
Solving for \( [G] \):
\[
[G] = \frac{M L^3 T^{-2}}{M^2} = M^{-1} L^3 T^{-2}
\]
Thus, the dimensional formula of \( G \) is:
\[
[G] = M^{-1} L^3 T^{-2}
\]
Therefore, comparing this with \( M^a L^b T^c \), we get:
\[
a = -1, \quad b = 3, \quad c = -2
\]
Thus, the correct values of \( a \), \( b \), and \( c \) are \( -1, 3, -2 \).
\[
\boxed{(-1, 3, -2)}
\]