Understanding ice composition is crucial in star and planet formation. To investigate ices in young stellar objects (YSOs), we can utilize ALMA, JWST, and the upcoming SPHEREx mission. ALMA observations reveal sublimated complex organic molecules, while JWST provides detailed ice absorption spectra. SPHEREx will perform all-sky ice mapping. We emphasize burst accretion, where episodic increases in accretion rates cause ices to sublimate, revealing their composition. YSOs gain mass through episodic accretion, causing luminosity variability. Catching burst events by monitoring YSOs allows for detailed ice composition studies. Identifying bursting YSOs at different evolutionary stages will enable us to track ice evolution from early star formation to planet formation, enhancing our understanding of surface chemistry.