 Solution

An Earth analogue has an iron-silicate interior and a thin secondary nitrogen-dominated atmosphere with water and carbon dioxide. Contextual coexistence of oxygen or ozone with methane and surface-water indicators would be a target biosignature. Its small scale height and extreme reflected-light contrast put a true Sun-Earth analogue beyond routine current atmospheric work, but future large direct-imaging missions and the Extremely Large Telescope target nearby terrestrial planets.

A temperate M-dwarf rocky planet has a similar solid interior but may retain carbon-dioxide, nitrogen, or water atmospheres under synchronous rotation. Water, carbon dioxide, methane, and contextual oxygen chemistry are observable targets. Its small host gives deeper transits, so the James Webb Space Telescope and large ground telescopes can test nearby systems, although stellar activity and atmospheric erosion complicate interpretation.

A Hycean planet or water-rich sub-Neptune has a water-rich interior or ocean below a hydrogen-rich atmosphere. Methane, carbon dioxide, ammonia, water, and proposed sulfur-bearing biosignatures must be interpreted against abiotic photochemistry. Its large radius and hydrogen scale height make transmission spectroscopy comparatively favorable for JWST and future Ariel space telescope surveys, but whether a clement ocean exists beneath the atmosphere remains model-dependent.