It is a pleasure and a privilege for me to participate in this symposium in honor of Professor Rowland. My talk will deal with astronomical applications of spectroscopy, and will have two parts. First, I shall talk about the Copernicus satellite, mainly because it used a Rowland spectrometer, which was uniquely qualified for the purpose we had in mind. Second, I shall say a few words about the two spectrometers on the Hubble Space Telescope; these instruments do not use Rowland mountings, but are of interest because they offer such enormous promise for future research. MY own interest in spectroscopy emphasizes the ultraviolet wavelengths, because in the study of interstellar matter the universe opens up below 3000 A. It opens up a little wider below 1600 A, and even more in the region between 900 and 1250 A, the region in which the Copernicus satellite principally contributed to the study of interstellar lines. Fiqure 1 is an optical diagram of the spectrometer on Copernicus, which will be familiar in principle, I am sure, to all of you. The light passes through a narrow entrance slit and strikes the concave grating: the spectrum is then brought to a focus on the Rowland circle, about one meter in diameter. I shall say nothing about the Copernicus spacecraft, but I will say just a few words about the spectrometer exit slits, since these were of somewhat unusual design.