HD 93129 and Supergiant star

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

Difference between HD 93129 and Supergiant star

HD 93129 vs. Supergiant star

HD 93129 is a triple star system in the Carina Nebula, with all three components being hot O class stars amongst the most luminous stars in the Milky Way. Supergiants are among the most massive and most luminous stars.

Similarities between HD 93129 and Supergiant star

HD 93129 and Supergiant star have 3 things in common (in Unionpedia): O-type main-sequence star, Open cluster, Wolf–Rayet star.

O-type main-sequence star

An O-type main-sequence star (O V) is a main-sequence (core hydrogen-burning) star of spectral type O and luminosity class V. These stars have between 15 and 90 times the mass of the Sun and surface temperatures between 30,000 and 50,000 K. They are between 40,000 and 1,000,000 times as luminous as the Sun.

HD 93129 and O-type main-sequence star · O-type main-sequence star and Supergiant star · See more »

Open cluster

An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age.

HD 93129 and Open cluster · Open cluster and Supergiant star · See more »

Wolf–Rayet star

Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of highly ionised helium and nitrogen or carbon.

HD 93129 and Wolf–Rayet star · Supergiant star and Wolf–Rayet star · See more »

The list above answers the following questions

What HD 93129 and Supergiant star have in common
What are the similarities between HD 93129 and Supergiant star

HD 93129 and Supergiant star Comparison

HD 93129 has 26 relations, while Supergiant star has 74. As they have in common 3, the Jaccard index is 3.00% = 3 / (26 + 74).

References

This article shows the relationship between HD 93129 and Supergiant star. To access each article from which the information was extracted, please visit:

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