  Giant planets within the habitable zones of the closest several stars can
currently be imaged with ground-based telescopes. Within the next decade, the
Extremely Large Telescopes (ELTs) will begin to image the habitable zones of a
greater number of nearby stars with much higher sensitivity$-$ potentially
imaging exo-Earths around the closest stars. To determine the most promising
candidates for observations over the next decade, we establish a theoretical
framework for the direct detectability of Earth$-$ to super-Jovian-mass
exoplanets in the mid-infrared based on available atmospheric and evolutionary
models. Of the 83 closest BAFGK type stars, we select 37 FGK type stars within
10 pc and 34 BA type stars within 30 pc with reliable age constraints. We
prioritize targets based on a parametric model of a planet's effective
temperature based on a star's luminosity, distance, and age, and on the
planet's orbital semi-major axis, radius, and albedo. We then predict the most
likely planets to be detectable with current 8-meter telescopes and with a 39-m
ELT with up to 100 hours of observation per star. Putting this together, we
recommend observation times needed for the detection of habitable-zone
exoplanets spanning the range of very nearby temperate Earth-sized planets to
more distant young giant planets. We then recommend ideal initial targets for
current telescopes and the upcoming ELTs.
