Read the following excerpt from an academic history of nineteenth-century astrophysics:
"Although Gustav Kirchhoff’s 1859 formulation of spectral analysis enabled astronomers to identify chemical elements in the solar atmosphere, it was not until the development of gelatin-silver bromide photographic plates in the late 1870s that solar spectrographs could record spectral line shifts faint enough to verify Doppler-effect measurements of solar rotation."
True or False: Prior to the late 1870s, astronomers could identify chemical elements in the solar atmosphere using spectral analysis, but solar spectrographs lacked the sensitivity required to record line shifts subtle enough to verify Doppler-effect measurements of solar rotation.
Answer: Answer