Mira variable and S Persei

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

Difference between Mira variable and S Persei

Mira variable vs. S Persei

Mira variables ("Mira", Latin, adj. - feminine form of adjective "wonderful"), named for the prototype star Mira, are a class of pulsating variable stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths. S Persei is a red supergiant located near the Double Cluster in Perseus, north of the cluster NGC 869.

Similarities between Mira variable and S Persei

Mira variable and S Persei have 2 things in common (in Unionpedia): Apparent magnitude, Semiregular 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.

Apparent magnitude and Mira variable · Apparent magnitude and S Persei · See more »

Semiregular variable star

Semiregular variable stars are giants or supergiants of intermediate and late spectral type showing considerable periodicity in their light changes, accompanied or sometimes interrupted by various irregularities.

Mira variable and Semiregular variable star · S Persei and Semiregular variable star · See more »

The list above answers the following questions

What Mira variable and S Persei have in common
What are the similarities between Mira variable and S Persei

Mira variable and S Persei Comparison

Mira variable has 66 relations, while S Persei has 29. As they have in common 2, the Jaccard index is 2.11% = 2 / (66 + 29).

References

This article shows the relationship between Mira variable and S Persei. To access each article from which the information was extracted, please visit:

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