Apparent magnitude / absolute magnitude / luminosity

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SUMMARY

The discussion clarifies the distinctions between luminosity, apparent magnitude, and absolute magnitude in astronomy. Luminosity refers to the total power output of a star across all wavelengths of electromagnetic radiation, while apparent magnitude is primarily concerned with visible light, making it a subjective measure. The term bolometric luminosity is used when considering all wavelengths, and specific bands are denoted with subscripts, such as m_B for the B band. This understanding is crucial for accurate astronomical measurements and interpretations.

PREREQUISITES
  • Understanding of electromagnetic radiation and its spectrum
  • Familiarity with astronomical terminology, including magnitude and luminosity
  • Knowledge of logarithmic scales and their applications in astronomy
  • Basic comprehension of photometric systems and passbands
NEXT STEPS
  • Research bolometric luminosity and its significance in stellar classification
  • Study the differences between apparent and absolute magnitude in detail
  • Learn about photometric systems and how they define various bands, such as the B band
  • Explore the concept of bolometric magnitude and its applications in astrophysics
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Astronomy students, astrophysicists, and anyone interested in understanding stellar properties and measurements in the context of electromagnetic radiation.

mtig
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Hello,

When we talk about the luminosity, apparent magnitude or absolute magnitude of a star, are we talking about all wavelengths of EM radiation or just a certain range?

I've read that luminosity is basically the power output of all types of radiation, but the apparent magnitude scale is subjective implying that it only accounts for visible light.
 
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Wikipedia's definition says, "In astronomy, magnitude is a logarithmic measure of the brightness of an object, measured in a specific wavelength or passband, usually in the visible or near-infrared spectrum." This is correct, in that we are usually talking about the radiation in a specific band. When no band is specified, it is usually assumed that the band is visible light. If the radiation at all wavelengths is included, then we usually call the quantity bolometric luminosity or bolometric magnitude. If it is a specific band, then there will often be a subscript, such as m_B, which would be the magnitude in the B band of wavelengths.
 
phyzguy said:
Wikipedia's definition says, "In astronomy, magnitude is a logarithmic measure of the brightness of an object, measured in a specific wavelength or passband, usually in the visible or near-infrared spectrum." This is correct, in that we are usually talking about the radiation in a specific band. When no band is specified, it is usually assumed that the band is visible light. If the radiation at all wavelengths is included, then we usually call the quantity bolometric luminosity or bolometric magnitude. If it is a specific band, then there will often be a subscript, such as m_B, which would be the magnitude in the B band of wavelengths.
Ok thank you.
 

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