By understanding the dynamics and structure of the space environment carved out by the Sun and its continuously-emitted solar wind, we better place our Sun in its context as a star and the ability of exoplanets to support life within a stellar environment that, for example, shields us from lethal galactic cosmic rays. NASA's IMAP mission will provide unprecedented observations, understanding, and discovery of the structure and properties of 'clouds' of plasma that lie at the collision of the solar wind that is continuously emitted from the Sun and the cold material of the interstellar medium through which the Sun is moving. With special glasses to see neutral hydrogen atoms rather than light, three unique imagers aboard IMAP will provide sky maps of energetic hydrogen emitted from plasmas within these distant regions of the heliosphere. We report the first data from the high energy neutral atom imager, IMAP-Hi.