An exoplanet with 0.5 Earth masses and 0.8 Earth radii could potentially support a large body of liquid water, such as an ocean, despite having low atmospheric pressure of 0.10 bar. The saturation pressure at 285 K indicates that a significant portion of the atmosphere could be water vapor, allowing for the possibility of an ocean comparable to or larger than the Indian Ocean. The planet's escape velocity suggests that its atmosphere could persist for billions of years, even with some hydrogen loss. The composition of the atmosphere, including nitrogen, oxygen, and carbon dioxide, along with the planet's density and potential for plate tectonics, supports the idea of a stable climate conducive to liquid water. Ultimately, there are no inherent limits on the size of the ocean, as long as it does not exceed the planet's surface area.