Studies of water vapor in the atmospheres of Venus, Mars and Earth by spectroscopic techniques are being made routinely with different instruments on board of interplanetary missions like Mars-Express, Venus-Express and many others as well as with a lot of spacecrafts on the Earth’ orbit. Accessibility of detailed spectroscopic information in a wide range is then of crucial importance to retrieve reliable results with these instruments. Unlike Earth, Mars and Venus have the CO 2 -rich planetary atmospheres that require line shape parameters for HDO–CO 2 broadening.In this paper a new linelist for HD 16 O is presented. This linelist covers the range of 0.00065–25,660cm −1 and is significantly more complete than other databases presently available. All lines with intensities (for 100% abundance) greater than 10 −30 cm/molecule at 296K are included. Wavenumbers for 43% (about 300,000) of all lines were evaluated at a level of the best experimental accuracy. For each transition the line shape parameters such as halfwidth and temperature exponent are provided for the case of HDO–air, HDO–HDO, and HDO–CO 2 broadening. The final linelist contains more than 700,000 HD 16 O lines and is presented in HITRAN-compatible format.