This audiobook is narrated by a digital voice.

The concept of planetary habitability revolves around the potential of a celestial body to support life, particularly life as we understand it—carbon-based organisms that require water, energy, and stable environmental conditions. Habitability does not necessarily imply that life exists on a planet, but rather that the conditions are right for life to emerge and persist over time. Scientists assess various planetary characteristics to determine whether a world could be considered habitable, and this assessment has become a cornerstone in the search for life beyond Earth.

Historically, the idea of habitability has evolved alongside our understanding of astronomy and biology. In ancient times, Earth was considered unique and central to the universe. However, as telescopes improved and our grasp of planetary science deepened, it became apparent that Earth might be one of many planets capable of supporting life. The discovery of exoplanets—planets orbiting stars outside our solar system—has dramatically expanded the scope of the habitability discussion. Today, thousands of exoplanets have been identified, and scientists continue to analyze their features to assess whether any of them resemble Earth in critical ways.

At the core of defining habitability is a set of criteria based on what we know about life on Earth. These include the presence of liquid water, a stable source of energy, and a range of environmental factors such as temperature, atmospheric pressure, and chemical composition. While Earth serves as our primary model for habitability, researchers remain open to the possibility that life could exist under different conditions, perhaps even in environments previously deemed inhospitable.