Types of spectra (a) Before passing the solar atmosphere, why does the solar radiation have a continuous spectrum? Solar atmosphere (b) The right figure is a schematic drawing of the Sun. oB If the telescope zooms in on Position B, which kind of spectrum (emission, absorption, or continuous) o A is most likely observed? (c) The solar atmosphere is very faint compared with the solar disk (i.e. the orange circle in the figure) and it is therefore not easy to observe the spectrum of Position B. Suggest an astronomical event that is suitable for the observation of this spectrum.
Types of spectra (a) Before passing the solar atmosphere, why does the solar radiation have a continuous spectrum? Solar atmosphere (b) The right figure is a schematic drawing of the Sun. oB If the telescope zooms in on Position B, which kind of spectrum (emission, absorption, or continuous) o A is most likely observed? (c) The solar atmosphere is very faint compared with the solar disk (i.e. the orange circle in the figure) and it is therefore not easy to observe the spectrum of Position B. Suggest an astronomical event that is suitable for the observation of this spectrum.
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
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
Transcribed Image Text:2.
Турes of spectra
(a)
Before passing the solar atmosphere, why does the solar radiation have a
continuous spectrum?
Solar atmosphere
(b) The right figure is a schematic drawing of the Sun.
o B
If the telescope zooms in on Position B, which kind
of spectrum (emission, absorption, or continuous)
o A
is most likely observed?
(c) The solar atmosphere is very faint compared with
the solar disk (i.e. the orange circle in the figure)
and it is therefore not easy to observe the spectrum of Position B. Suggest an
astronomical event that is suitable for the observation of this spectrum.
(d) State two pieces of info that can be measured/found by using stellar spectrum.
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