We present the UV-to-NIR size evolution of a sample of 161 quiescent galaxies (QGs) with M_*>10^{10}M_\odot over 0.5<z<5. With deep multi-band NIRCam images in GOODS-South from JADES, we measure the effective radii (R_e) of the galaxies at rest-frame 0.3, 0.5 and 1\mu m. On average, QGs are 45% (15%) more... Show more