Illustration of the orbit (dashed line) of HD 93205 in the orbital plane with the primary set at coordinates (x = 0, y = 0) (left) and as a projected orbit assuming two likely inclination angles (right). Solid circles represent the primary and secondary stellar bodies. Stellar bodies and orbit sizes are to scale. Orbital phase increases counterclockwise (resp. clockwise) along the orbit in top right (resp. bottom right) illustration.