Water vapor escape from Earth's atmosphere into space is minimal, with the dominant loss mechanism being sequestration rather than atmospheric escape. Due to Earth's temperature conditions, water vapor and carbon dioxide are primarily stored in the hydrosphere and lithosphere, particularly as liquid water in oceans, which reduces atmospheric density. Estimates suggest that while hydrogen and oxygen may be lost, intact water molecules are unlikely to escape. Future projections indicate that significant water loss may occur only when the Sun's brightness increases by 10% over the next billion years, suggesting that current water loss rates are very low.