Transmission spectroscopy measures the transit depth as a function of wavelength, to detect the gases of the atmosphere that the starlight crosses at the planet’s limb. A secondary eclipse is the passage of a planet behind its star, half an orbit after the transit on a circular orbit; the drop of the system’s flux then measures the light of the planet’s day side.
বইগুলো এখনো বাংলা ভাষায় পাওয়া যায় না — ইংরেজি সংস্করণ দেখানো হচ্ছে।
Earth and Space Sciences · পরিভাষা
Transmission spectroscopy; secondary eclipse কী?
অন্য নাম: transmission spectroscopy · secondary eclipse