Infrared radiation is referred to as a heat signature because it effectively transfers energy to internal molecular vibrations, resulting in heat. Most objects at typical temperatures emit predominantly infrared radiation, making it a reliable indicator of temperature. The concept of blackbody radiation further clarifies this relationship, as it describes how objects emit radiation based on their temperature. While very hot objects like stars emit significant visible light, they still produce a substantial amount of infrared radiation. Thus, measuring infrared emissions provides valuable insights into the thermal characteristics of various objects.