G-type main-sequence star and Lambda Arietis

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

Difference between G-type main-sequence star and Lambda Arietis

G-type main-sequence star vs. Lambda Arietis

A G-type main-sequence star (Spectral type: G-V), often (and imprecisely) called a yellow dwarf, or G dwarf star, is a main-sequence star (luminosity class V) of spectral type G. Such a star has about 0.84 to 1.15 solar masses and surface temperature of between 5,300 and 6,000 K., G. M. H. J. Habets and J. R. W. Heintze, Astronomy and Astrophysics Supplement 46 (November 1981), pp. Lambda Arietis (λ Ari, λ Arietis) is the Bayer designation for a double star in the northern constellation of Aries.

Similarities between G-type main-sequence star and Lambda Arietis

G-type main-sequence star and Lambda Arietis have 3 things in common (in Unionpedia): Apparent magnitude, Earth, Stellar classification.

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 G-type main-sequence star · Apparent magnitude and Lambda Arietis · See more »

Earth

Earth is the third planet from the Sun and the only astronomical object known to harbor life.

Earth and G-type main-sequence star · Earth and Lambda Arietis · See more »

Stellar classification

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

G-type main-sequence star and Stellar classification · Lambda Arietis and Stellar classification · See more »

The list above answers the following questions

What G-type main-sequence star and Lambda Arietis have in common
What are the similarities between G-type main-sequence star and Lambda Arietis

G-type main-sequence star and Lambda Arietis Comparison

G-type main-sequence star has 57 relations, while Lambda Arietis has 22. As they have in common 3, the Jaccard index is 3.80% = 3 / (57 + 22).

References

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

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