Serpens and Slowly pulsating B-type star

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

Difference between Serpens and Slowly pulsating B-type star

Serpens vs. Slowly pulsating B-type star

Serpens ("the Serpent", Greek Ὄφις) is a constellation of the northern hemisphere. A slowly pulsating B-type star (SPB), formerly known as a 53 Persei variable, is a type of pulsating variable star.

Similarities between Serpens and Slowly pulsating B-type star

Serpens and Slowly pulsating B-type star have 8 things in common (in Unionpedia): Algol variable, American Association of Variable Star Observers, Apparent magnitude, Beta Cephei variable, Spectral line, Stellar classification, Variable star, 25 Serpentis.

Algol variable

Algol variables or Algol-type binaries are a class of eclipsing binary stars that are related to the prototype member of this class, β Persei (Beta Persei, Algol) from an evolutionary point of view.

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American Association of Variable Star Observers

Since its founding in 1911, the American Association of Variable Star Observers (AAVSO) has coordinated, collected, evaluated, analyzed, published, and archived variable star observations made largely by amateur astronomers and makes the records available to professional astronomers, researchers, and educators.

American Association of Variable Star Observers and Serpens · American Association of Variable Star Observers and Slowly pulsating B-type star · See more »

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.

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Beta Cephei variable

Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations of the stars' surfaces, thought due to the unusual properties of iron at temperatures of 200,000 K in their interiors.

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Spectral line

A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies.

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Stellar classification

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

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Variable star

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

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25 Serpentis

25 Serpentis is a star system in the constellation of Serpens Caput.

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The list above answers the following questions

What Serpens and Slowly pulsating B-type star have in common
What are the similarities between Serpens and Slowly pulsating B-type star

Serpens and Slowly pulsating B-type star Comparison

Serpens has 228 relations, while Slowly pulsating B-type star has 35. As they have in common 8, the Jaccard index is 3.04% = 8 / (228 + 35).

References

This article shows the relationship between Serpens and Slowly pulsating B-type star. To access each article from which the information was extracted, please visit:

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