What is the typical $H_0$ value associated with measurements derived from the Early Universe (CMB analysis) within the $\Lambda$CDM model?

Answer

Approximately $67 \text{ km/s/Mpc}$.

Observations based on the Cosmic Microwave Background (CMB) within the standard $\Lambda$CDM model consistently predict an expansion rate around $67 \text{ km/s/Mpc}$.

What is the typical $H_0$ value associated with measurements derived from the Early Universe (CMB analysis) within the $\Lambda$CDM model?
astronomyuniversecosmologyexpansionHubble constant