Durchmusterung and Sigma Cassiopeiae

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

Difference between Durchmusterung and Sigma Cassiopeiae

Durchmusterung vs. Sigma Cassiopeiae

In astronomy, Durchmusterung or Bonner Durchmusterung (BD), is the comprehensive astrometric star catalogue of the whole sky, compiled by the Bonn Observatory (Germany) from 1859 to 1903. Sigma Cassiopeiae (σ Cas, σ Cassiopeiae) is a binary star in the constellation Cassiopeia.

Similarities between Durchmusterung and Sigma Cassiopeiae

Durchmusterung and Sigma Cassiopeiae have 3 things in common (in Unionpedia): Apparent magnitude, Durchmusterung, Smithsonian Astrophysical Observatory Star Catalog.

Apparent magnitude

The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.

Apparent magnitude and Durchmusterung · Apparent magnitude and Sigma Cassiopeiae · See more »

Durchmusterung

In astronomy, Durchmusterung or Bonner Durchmusterung (BD), is the comprehensive astrometric star catalogue of the whole sky, compiled by the Bonn Observatory (Germany) from 1859 to 1903.

Durchmusterung and Durchmusterung · Durchmusterung and Sigma Cassiopeiae · See more »

Smithsonian Astrophysical Observatory Star Catalog

The Smithsonian Astrophysical Observatory Star Catalog is an astrometric star catalogue.

Durchmusterung and Smithsonian Astrophysical Observatory Star Catalog · Sigma Cassiopeiae and Smithsonian Astrophysical Observatory Star Catalog · See more »

The list above answers the following questions

What Durchmusterung and Sigma Cassiopeiae have in common
What are the similarities between Durchmusterung and Sigma Cassiopeiae

Durchmusterung and Sigma Cassiopeiae Comparison

Durchmusterung has 42 relations, while Sigma Cassiopeiae has 37. As they have in common 3, the Jaccard index is 3.80% = 3 / (42 + 37).

References

This article shows the relationship between Durchmusterung and Sigma Cassiopeiae. To access each article from which the information was extracted, please visit:

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