Why the measured cosmological constant is small

In a quest to explain the small value of the today’s cosmological constant, following the approach introduced in [1], we show that the theoretical value of cosmological constant is consistent with its observational value. In more detail, we study the Freidmann-Lama^{\i}tre-Robertson-Walker cosmology embedded isometrically in an $11$-dimensional ambient space. The field equations determines $\mathrm{\Lambda }$ in terms of other measurable fundamental constants. Specifically, it predicts that the cosmological constant measured today be $\mathrm{\Lambda }{L}_{\text{Pl}}^2=2.56\times {10}^{-122}$, as observed.