The Heatflow and Physical Properties Package (HP 3 ) radiometer is currently operating on Mars, observing two spots approximately 1 and 3 m north-north-west of the InSight lander. The instrument has primary sensors that are sensitive in the range of 8 to 14 μm and two more sensors with more narrow spectral ranges per field of view. The radiometer underwent radiometric and geometric calibration at DLR-Berlin; and on Mars radiometric self-calibration is performed regularly. The self-calibration confirms that one of the two primary sensors has been stable since the ground calibration, but environmental parameters that are likely associated with the thermal contact of sensor and instrument main body may have slightly changed. The other primary sensor has increased in sensitivity for an unknown reason but is still within expectation from the sensor design. The uncertainty of the two primary sensors is approximately 3 K at night, with somewhat larger errors in the late afternoon. This estimate includes the effect of sensitivity changes that would be too small to be reliably detected by the self-calibration.The HP 3 -RAD radiometer is based on the designs of the MASCOT Radiometer (Grott et al., 2017) on Hayabusa 2, of the MERTIS instrument on Bepi-Colombo (Hiesinger & Helbert, 2010;Walter et al., 2006), and of the MUPUS Thermal Mapper on Rosetta (Spohn et al., 2007(Spohn et al., , 2015. The HP 3 -RAD was radiometrically calibrated in a space simulation chamber under conditions simulating the Mars environment over 2 weeks in April 2017. Onboard calibration occurred regularly after landing starting in December 2018.