Macroscopic results
No structural anomalies and malformations were observed in the cerebella.
Body weight and relative cerebellum weights
The average body weights of young rats were lower than those of adult and old rats (P<0.05). Conversely, it was shown that the relative cerebellum weights were significantly greater in young rats compared to adult and old rats (P<0.05, Fig. 3).
Histological structure of the cerebellum
All age groups, it was observed that ten folium and they were numbered from I to X rostro-caudal direction. The secondary foliations were observed in the folia III, VI, and IX. Each folium exhibited distinct layers of gray matter (cortex) and white matter (medulla). In the central part of the cerebellum, there was a white matter region, referred to as the central alba.
The histology of the cerebellum was similar in all animals. Light microscopic analysis demonstrated that the cerebellar cortex comprises three layers (Fig. 4). The molecular cell layer (stratum moleculare), situated in the outermost, consisted of diminutive neurons and glial cells. The granular cell layer (stratum granulosum), located next to the medulla (substantia alba), had tiny neurons distinguished by heterochromatic nuclei and small amount of cytoplasm. The ganglioner layer (stratum gangliosum) comprises Purkinje cells organized in a single row located between the molecular and granular layers (Fig. 4D, 4E, 4F).
In the cerebellar tissue sections from the elderly rat group, edema, and demyelination were observed, particularly in the white matter (Fig. 5A, 5B). In the sections of this group, senescence pigment granules exhibiting positive reactions in PAS staining were observed in Purkinje cells, predominantly situated in the upper part of the perikaryon, adjacent to the initial dendritic branching (Fig. 5C, 5D).
Histometric measurement results
Average thicknesses of the cortical layers
Histometric examinations of foliums revealed that the molecular layer thickness was increased in adults compared to the young and old rats, however, the granular layer thickness was lower in the young age group. The adult rats had the thickest cortex. The difference between the groups was statistically significant (Fig. 6, P<0.05).
Average folium heights
Analysis of the folium height in the adult rats revealed a consistent reduction throughout the aging process (Fig. 7). The highest folium I, IXA, IXB, IXC, and X were identified in the adult rats, compared to the old rats (P<0.05). The highest folium VIB was identified in the adult rats, and difference between young and adult animals was statistically significant (P<0.05). The highest folium VII and VIII were identified in the young age group (P<0.05) whereas the smallest foliums IXC and X were identified in the old rat group (P<0.05). Although the differences were not statistically significant (P>0.05), the highest folium II, IIIA, and IIIB were observed in adult rats, the highest folium V and VIA were identified in young rats, and the smallest folium IV was found in old rats.
Average folium widths
According to the results obtained from the average folium widths, the widest folium I, II, IIIB, VII, and VIII were observed in adults, and differences among the folium I, VII, and VIII were statistically significant (P<0.05); conversely, the widths of folium II and IIIB were similarly to both young and old rats (P>0.05). The largest folium IXB was observed in the old rats (P<0.05) while the narrowest folium VII, VIII, and X were identified in the old rats (P<0.05). However, folium X was similar in both young and adult rats (P>0.05). The narrowest folium IIIA and IXA were detected in young rats, whilst the widest foliums V and VIA were found in old rats. Although the widths of these foliums typically increase with age, it was observed that the maximum widths of foliums IV and IXC were recorded in young rats, whereas the width values in adult and elderly rat groups were comparable and diminished with age (Fig. 8).
Immunohistochemical results
Astrocytic soma and processes stained for GFAP were identified as dark brown and GFAP-immunoreactive (GFAP-IR) cells exhibited star-shaped. In contrast to the young and adult groups, astrocytes in the cerebellar tissue sections of the old rats exhibited hypertrophy, hyperplasia, and increased staining intensity. In old rats, the cytoplasmic extensions of astrocytes were more abundant and interwoven with each another (Fig. 9F, 9I, 9L). GFAP-immunoreactive astrocytes were identified in the granular layer and white matter of each folium in the cerebellar tissue, as well as in the central white matter regions situated along the mid-vermal line of the cerebellum (Fig. 9). GFAP-IR cellular extensions were also observed in the molecular layer (Fig. 9D, 9E, 9F).
The assessments revealed the greatest quantity of GFAP-IR astrocytes in the granular layer of the foliums in old rats (Fig. 9F, 9I). GFAP-IR astrocyte numbers in the granular layer of folium I, II, III, IV, V, VIII, IX, and X exhibited a significant increase in the old rat compared to the young and adult animals. Conversely, in folium VI and VII, the number of GFAP-IR astrocytes varied among all groups, showing significant increases in the order to the young, adult, and old groups, respectively (P<0.05, Fig. 10).
In white matter of cerebellar vermis, the highest number of GFAP-IR astrocytes was observed in old rats (Fig. 9I). The number of GFAP-IR astrocytes in folium I, II, and VII showed significant increases in all age groups. In folium III, IV, V, VI, VIII, and IX, the enhancement was significantly greater in the old rats compared to the young and adult (P<0.05). In folium X, the statistically significant change was observed solely between the young and old rat (P<0.05). The mean GFAP-IR astrocyte number in the stratum granulosum and white matter of the foliums are presented in Fig. 10 and Fig. 11.
The evaluation of total GFAP-IR astrocyte counts in the cerebellar folia (stratum granulosum + substansia alba) revealed significant differences in folia I, II, VI, VII, and X among all age groups, with the highest number observed in the old-rats. Additionally, significant increase density of GFAP-IR astrocyte was noted in the other folia (III, IV, V, VIII, and IX) in the old rat group compared to the young and adult groups (P<0.05, Fig. 12).
Analysis of GFAP-IR astrocyte number in the central alba region of the mid-vermal sections of the cerebellum revealed that the old rat group exhibited the highest values (Fig. 9L, P<0.05, Fig. 13).