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A-type main-sequence star and HD 15082

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

Difference between A-type main-sequence star and HD 15082

A-type main-sequence star vs. HD 15082

An A-type main-sequence star (A V) or A dwarf star is a main-sequence (hydrogen-burning) star of spectral type A and luminosity class V. These stars have spectra which are defined by strong hydrogen Balmer absorption lines. HD 15082 (also known as WASP-33) is a star located roughly 380 light years away in the northern constellation of Andromeda.

Similarities between A-type main-sequence star and HD 15082

A-type main-sequence star and HD 15082 have 4 things in common (in Unionpedia): Effective temperature, Exoplanet, Star, Stellar classification.

Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation.

A-type main-sequence star and Effective temperature · Effective temperature and HD 15082 · See more »

Exoplanet

An exoplanet or extrasolar planet is a planet outside our solar system.

A-type main-sequence star and Exoplanet · Exoplanet and HD 15082 · See more »

Star

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

A-type main-sequence star and Star · HD 15082 and Star · See more »

Stellar classification

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

A-type main-sequence star and Stellar classification · HD 15082 and Stellar classification · See more »

The list above answers the following questions

A-type main-sequence star and HD 15082 Comparison

A-type main-sequence star has 38 relations, while HD 15082 has 28. As they have in common 4, the Jaccard index is 6.06% = 4 / (38 + 28).

References

This article shows the relationship between A-type main-sequence star and HD 15082. To access each article from which the information was extracted, please visit:

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