Long afterglow materials have been studied continuously due to its unique mechanisms of light storage and luminescence. The long afterglow materials will undergo three stages of absorption, energy transfer, and luminescence to release the energy in the form of long-term continuous luminescence after removing the excitation source. 1 The long afterglow is determined by the luminescence center. At present, only some rareearth ions (Ce 3+ , Pr 3+ , Sm 3+ , Eu 2+ , Eu 3+ , Tb 3+ , Dy 3+ , Tm 3+ , Yb 2+ , Yb 3+ , etc.), transition-metal ions (Cr 3+ , Mn 2+ , Mn 4+ , Ti 4+ , etc.), main group elements (Bi 3+ , etc.), and some crystal defects show their characteristic phosphorescence. 2-7 Since Matsuzawa et al. discovered the continuous luminescence of SrAl 2 O 4 :Eu 2+ , Dy 3+ more than 20 years ago, this material has attracted extensive attention. Many other long afterglow material systems have been also discovered and studied successively, including sulfide, aluminate, silicate, gallate, and so on. 8 Among them, green luminescent materials such as SrAl 2 O 4 :Eu 2+ , Dy 3+ and blue luminescent materials such as CaAl 2 O 4 :Eu 2+ , Nd 3+ have been mature and commercialized in many application fields due to their excellent afterglow performance, however, the research and development of long afterglow materials that can produce red and near-infrared emission are still relatively scarce. 9 Cr-doped zinc gallate has good long afterglow emissions in red and near-infrared regions. [10][11][12][13] Spinel ZnGa 2 O 4 has a wide band gap (4.4-5.0 eV), high chemical stability, and thermal stability. [14][15][16][17][18] In the process of practical application, long afterglow materials will confront harsh environments