Horologium (constellation) and Mira variable

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

Difference between Horologium (constellation) and Mira variable

Horologium (constellation) vs. Mira variable

Horologium is a faint constellation in the southern sky. Mira variables ("Mira", Latin, adj. - feminine form of adjective "wonderful"), named for the prototype star Mira, are a class of pulsating variable stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths.

Similarities between Horologium (constellation) and Mira variable

Horologium (constellation) and Mira variable have 3 things in common (in Unionpedia): Apparent magnitude, R Horologii, Red giant.

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 Horologium (constellation) · Apparent magnitude and Mira variable · See more »

R Horologii

R Horologii (also known as HD 18242) is a red giant star approximately 700 light-years away in the constellation Horologium.

Horologium (constellation) and R Horologii · Mira variable and R Horologii · See more »

Red giant

A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses) in a late phase of stellar evolution.

Horologium (constellation) and Red giant · Mira variable and Red giant · See more »

The list above answers the following questions

What Horologium (constellation) and Mira variable have in common
What are the similarities between Horologium (constellation) and Mira variable

Horologium (constellation) and Mira variable Comparison

Horologium (constellation) has 66 relations, while Mira variable has 66. As they have in common 3, the Jaccard index is 2.27% = 3 / (66 + 66).

References

This article shows the relationship between Horologium (constellation) and Mira variable. To access each article from which the information was extracted, please visit:

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