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61 Cygni and Main sequence

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

Difference between 61 Cygni and Main sequence

61 Cygni vs. Main sequence

61 Cygni Not to be confused with 16 Cygni, a more distant system containing two G-type stars harboring the gas giant planet 16 Cygni Bb. In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.

Similarities between 61 Cygni and Main sequence

61 Cygni and Main sequence have 14 things in common (in Unionpedia): Apparent magnitude, Binary star, Brown dwarf, Dwarf star, Earth, Jupiter, K-type main-sequence star, Parallax, Sirius, Stellar classification, Stellar magnetic field, Stellar rotation, Sun, Variable 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.

61 Cygni and Apparent magnitude · Apparent magnitude and Main sequence · See more »

Binary star

A binary star is a star system consisting of two stars orbiting around their common barycenter.

61 Cygni and Binary star · Binary star and Main sequence · See more »

Brown dwarf

Brown dwarfs are substellar objects that occupy the mass range between the heaviest gas giant planets and the lightest stars, having masses between approximately 13 to 75–80 times that of Jupiter, or approximately to about.

61 Cygni and Brown dwarf · Brown dwarf and Main sequence · See more »

Dwarf star

A dwarf star is a star of relatively small size and low luminosity.

61 Cygni and Dwarf star · Dwarf star and Main sequence · See more »

Earth

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

61 Cygni and Earth · Earth and Main sequence · See more »

Jupiter

Jupiter is the fifth planet from the Sun and the largest in the Solar System.

61 Cygni and Jupiter · Jupiter and Main sequence · See more »

K-type main-sequence star

A K-type main-sequence star (K V), also referred to as an orange dwarf or K dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow G-type main-sequence stars.

61 Cygni and K-type main-sequence star · K-type main-sequence star and Main sequence · See more »

Parallax

Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight, and is measured by the angle or semi-angle of inclination between those two lines.

61 Cygni and Parallax · Main sequence and Parallax · See more »

Sirius

Sirius (a romanization of Greek Σείριος, Seirios,."glowing" or "scorching") is a star system and the brightest star in the Earth's night sky.

61 Cygni and Sirius · Main sequence and Sirius · See more »

Stellar classification

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

61 Cygni and Stellar classification · Main sequence and Stellar classification · See more »

Stellar magnetic field

A stellar magnetic field is a magnetic field generated by the motion of conductive plasma inside a star.

61 Cygni and Stellar magnetic field · Main sequence and Stellar magnetic field · See more »

Stellar rotation

Stellar rotation is the angular motion of a star about its axis.

61 Cygni and Stellar rotation · Main sequence and Stellar rotation · See more »

Sun

The Sun is the star at the center of the Solar System.

61 Cygni and Sun · Main sequence and Sun · See more »

Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.

61 Cygni and Variable star · Main sequence and Variable star · See more »

The list above answers the following questions

61 Cygni and Main sequence Comparison

61 Cygni has 121 relations, while Main sequence has 127. As they have in common 14, the Jaccard index is 5.65% = 14 / (121 + 127).

References

This article shows the relationship between 61 Cygni and Main sequence. To access each article from which the information was extracted, please visit:

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