Andromeda (constellation) and HD 16175

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

Difference between Andromeda (constellation) and HD 16175

Andromeda (constellation) vs. HD 16175

Andromeda is one of the 48 constellations listed by the 2nd-century Greco-Roman astronomer Ptolemy and remains one of the 88 modern constellations. HD 16175 is a 7th magnitude G-type star with temperature about 6000 K located approximately 190 light-years away in the Andromeda constellation.

Similarities between Andromeda (constellation) and HD 16175

Andromeda (constellation) and HD 16175 have 4 things in common (in Unionpedia): Apparent magnitude, Exoplanet, Light-year, 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.

Andromeda (constellation) and Apparent magnitude · Apparent magnitude and HD 16175 · See more »

Exoplanet

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

Andromeda (constellation) and Exoplanet · Exoplanet and HD 16175 · See more »

Light-year

The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.

Andromeda (constellation) and Light-year · HD 16175 and Light-year · See more »

Star

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

Andromeda (constellation) and Star · HD 16175 and Star · See more »

The list above answers the following questions

What Andromeda (constellation) and HD 16175 have in common
What are the similarities between Andromeda (constellation) and HD 16175

Andromeda (constellation) and HD 16175 Comparison

Andromeda (constellation) has 161 relations, while HD 16175 has 19. As they have in common 4, the Jaccard index is 2.22% = 4 / (161 + 19).

References

This article shows the relationship between Andromeda (constellation) and HD 16175. To access each article from which the information was extracted, please visit:

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