29) Estimate the distance to the North Star if it has an absolute magnitude of -3.2 and an apparent magnitude of 1.99.
29) Estimate the distance to the North Star if it has an absolute magnitude of -3.2 and an apparent magnitude of 1.99.
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Concept and Principle:
- In astronomy when studying a star or any celestial object we use two different magnitudes. Apparent and absolute magnitudes.
- The apparent magnitude of a celestial object is the brightness measured by an observer at a specific distance from the object. If an object is closer it will have a larger apparent magnitude. Two objects can have the same apparent magnitude.
- The absolute magnitude on the other hand is the magnitude of a star if it was observed from a distance of 10 parsecs. Thus absolute magnitude allows astronomers a parameter to compare stars based on their magnitudes.
- The distance to a celestial object can be calculated if both of these magnitudes are known. The distance magnitude formula is given by,
Here d is the distance to the celestial object, m is the apparent magnitude, and M is the absolute magnitude.
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