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Apparent magnitude and Catalog of Components of Double and Multiple Stars

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Apparent magnitude and Catalog of Components of Double and Multiple Stars

Apparent magnitude vs. Catalog of Components of Double and Multiple Stars

The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth. The Catalog of Components of Double and Multiple Stars, or CCDM, is an astrometric star catalogue of double and multiple stars.

Similarities between Apparent magnitude and Catalog of Components of Double and Multiple Stars

Apparent magnitude and Catalog of Components of Double and Multiple Stars have 3 things in common (in Unionpedia): Double star, Star, Stellar classification.

Double star

In observational astronomy, a double star or visual double is a pair of stars that appear close to each other in the sky as seen from Earth when viewed through an optical telescope.

Apparent magnitude and Double star · Catalog of Components of Double and Multiple Stars and Double star · See more »

Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

Apparent magnitude and Star · Catalog of Components of Double and Multiple Stars and Star · See more »

Stellar classification

In astronomy, stellar classification is the classification of stars based on their spectral characteristics.

Apparent magnitude and Stellar classification · Catalog of Components of Double and Multiple Stars and Stellar classification · See more »

The list above answers the following questions

Apparent magnitude and Catalog of Components of Double and Multiple Stars Comparison

Apparent magnitude has 159 relations, while Catalog of Components of Double and Multiple Stars has 11. As they have in common 3, the Jaccard index is 1.76% = 3 / (159 + 11).

References

This article shows the relationship between Apparent magnitude and Catalog of Components of Double and Multiple Stars. To access each article from which the information was extracted, please visit:

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