Basics of Photometry and Magnitudes

In summary, it is not possible to calculate the absolute or apparent magnitude of a star using only its photometric magnitudes. Additional information, such as the star's distance, is needed for these calculations.
  • #1
piareround
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http://www.exoplanet.eu/catalog-all.php?&mode=0&more=yes". On one of the this it has for the for each exoplanet, in the list it gives the information about the parent star's properties especially its phototemetry. Specifically it lists star's the V-order, I-order, H-order, J-order, and K-order magnitude; however, it does not list the star's absolute magnitude, or luminosity.

Is their a way to calculate the absolute or apparent magnitude of the parent star from its photometric magnitudes? If so do how?
 
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  • #2
Unfortunately, it is not possible to calculate the absolute or apparent magnitude of a star based solely on its photometric magnitudes. Photometric magnitudes measure the amount of light that is received from a star in different bands of the electromagnetic spectrum, but they do not tell us how far away the star is. The only way to calculate the absolute magnitude of a star is to know its distance from Earth. This information can be obtained from other sources, such as astrometric or parallax measurements, which measure the angular shift of the star's position in the sky as the Earth moves around its orbit.
 

Related to Basics of Photometry and Magnitudes

1. What is photometry?

Photometry is the branch of science that deals with the measurement of light and its properties, such as intensity and color.

2. What is a magnitude in photometry?

A magnitude is a unit of measurement used in photometry to describe the brightness of an object, typically a star. The lower the magnitude, the brighter the object.

3. How is apparent magnitude different from absolute magnitude?

Apparent magnitude is a measure of how bright an object appears to us on Earth, while absolute magnitude is a measure of how bright an object would appear if it were located at a standard distance of 10 parsecs (32.6 light years) from Earth.

4. What is the difference between magnitude and luminosity?

Magnitude is a measure of how bright an object appears to us, while luminosity is a measure of the total amount of light that an object emits. Luminosity takes into account the distance of the object, while magnitude does not.

5. How is photometry used in astronomy?

Photometry is used in astronomy to measure the brightness of celestial objects, such as stars and galaxies. This information can then be used to study the properties and evolution of these objects.

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