The characteristics of photoelectron emission (PE) and X-ray photoelectron spectroscopy of iron surfaces scratched in different environments were investigated. The scratching environments were air, water, and organic liquids. The PE quantum yields (emitted electrons/photon), Y FD and Y s , were obtained in 2 ways of irradiation of the surface with photon energies: during the light wavelength scan in the range of 300 to 200 nm at 25°C, 200°C, and 339°C and during temperature increase and subsequent decrease scans in the range of 25°C to 339°C under 210-nm-light irradiation,where αA is called the electron photoemission probability, A is identical to the Richardson constant, E p is the incident photon energy, and ϕ is the photothreshold, was applied to the wavelength scan data to obtain αA and ϕ. Additionally, the emission intensity at 210-nm wavelength (I 210 ) and the total number of emitted electrons (N T ) were obtained during the wavelength scan. Arrhenius activation energies obtained for αA, I 210 , and N T were ΔE αA = 0.113 to 0.074 eV, ΔE 210 = 0.085 to 0.054 eV, and ΔE NT = 0.088 to 0.053 eV, respectively. The ΔE 210 and ΔE NT increased with ΔE αA . The dependence of ΔE 210 , ΔE NT , and ΔE αA on the environments was completely different from that of ΔE aUp1 values for the Y s during the temperature increase scan (Up1 scan), which were previously reported to be in the 0.212-to 0.035-eV range. The PE characteristics were explained from the dependence on the O1s component ratio of Z O = O 2− /(OH − + O 2− ) and the acid-base interaction between the surface Fe −OH groups and the molecules of the liquid environments. KEYWORDS Arrhenius activation energy, electron photoemission probability, photoelectron emission, real iron surface, scratching environment, XPS 1 | INTRODUCTION Much attention has been given to studying electron transfer and electronic excitation in the overlayers of real metallic surfaces in more detail in the fields of tribology, lubrication, adhesion, and corrosion. However, little is known about the behavior of electron transfer in superficial layers owing to the difficulties associated with experimental measurements of such electrons. Photoelectron emission (PE) occurs when photons are absorbed by electrons, leading to the release of these photon-absorbing electrons from the surface. The theoretical basis of PE is well captured by Spicer's 3-step model, 1 which prescribes that the emission process occurs in 3 successive steps: (a) optical excitation, (b) transport of excited electrons to the surface, and (c) release of excited electrons into vacuum. Furthermore, this theory relates photoemission to the parameters of the emitter, such as the optical absorption coefficient, electron scattering mechanisms, and height of the potential barrier at the surface. 2 For real iron surfaces, however, little electron emission is observed at temperatures close to room temperature, even in response to irradiation by photons with an energy greater than the work function of the