9 Persei and Perseus (constellation)

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

Difference between 9 Persei and Perseus (constellation)

9 Persei vs. Perseus (constellation)

9 Persei is a pulsating variable star in the constellation Perseus. Perseus is a constellation in the northern sky, being named after the Greek mythological hero Perseus.

Similarities between 9 Persei and Perseus (constellation)

9 Persei and Perseus (constellation) have 4 things in common (in Unionpedia): Apparent magnitude, Constellation, Iota Persei, Variable star.

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.

9 Persei and Apparent magnitude · Apparent magnitude and Perseus (constellation) · See more »

A constellation is a group of stars that are considered to form imaginary outlines or meaningful patterns on the celestial sphere, typically representing animals, mythological people or gods, mythological creatures, or manufactured devices.

9 Persei and Constellation · Constellation and Perseus (constellation) · See more »

Iota Persei

Iota Persei (Iota Per, ι Persei, ι Per) is a main sequence dwarf star in the constellation Perseus.

9 Persei and Iota Persei · Iota Persei and Perseus (constellation) · See more »

Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.

9 Persei and Variable star · Perseus (constellation) and Variable star · See more »

The list above answers the following questions

What 9 Persei and Perseus (constellation) have in common
What are the similarities between 9 Persei and Perseus (constellation)

9 Persei and Perseus (constellation) Comparison

9 Persei has 19 relations, while Perseus (constellation) has 160. As they have in common 4, the Jaccard index is 2.23% = 4 / (19 + 160).

References

This article shows the relationship between 9 Persei and Perseus (constellation). To access each article from which the information was extracted, please visit:

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