Properties and Spectral Characteristics of Celestial Bodies Quiz

Temperature determines the color of a celestial body.

Redshift indicates an increase in the wavelength of light emitted by a celestial body.

An emission spectrum refers to a spectrum formed by the emission of specific wavelengths of light.

Temperature is the primary characteristic used to classify stars into different spectral types.

Astronomers use stellar spectroscopy as the primary method to measure the temperature of stars.

Spectral lines are formed by the absorption or emission of specific wavelengths of light.

The temperature of the celestial body primarily affects the width of spectral lines.

Type O stars correspond to the hottest stars.

Black holes emit the most intense radiation among celestial bodies.

The shift of spectral lines helps astronomers determine a celestial body's radial velocity.

Absorption is associated with the formation of absorption lines in a spectrum.

Pressure is the primary factor determining the width of absorption lines in a celestial body's spectrum.

Astronomers determine the composition of celestial bodies by analyzing their spectra.

The primary purpose of spectroscopy in astronomy is to determine the composition and properties of celestial bodies.

Main sequence stars emit a continuous spectrum.

Temperature is the primary factor determining the color of a main sequence star.

Astronomers observe celestial bodies across different wavelengths to understand their internal structure and composition.