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Large Magellanic Cloud and Orders of magnitude (length)

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

Difference between Large Magellanic Cloud and Orders of magnitude (length)

Large Magellanic Cloud vs. Orders of magnitude (length)

The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way. The following are examples of orders of magnitude for different lengths.

Similarities between Large Magellanic Cloud and Orders of magnitude (length)

Large Magellanic Cloud and Orders of magnitude (length) have 21 things in common (in Unionpedia): Andromeda Galaxy, Astronomy & Astrophysics, Canis Major Overdensity, Globular cluster, Kilometre, Light-year, Local Group, Milky Way, Moon, Orders of magnitude (length), Parsec, Sagittarius Dwarf Spheroidal Galaxy, Satellite galaxy, Second, Small Magellanic Cloud, SN 1987A, Spiral galaxy, Supernova, Tarantula Nebula, The Astronomical Journal, The Astrophysical Journal.

Andromeda Galaxy

The Andromeda Galaxy, also known as Messier 31, M31, or NGC 224, is a spiral galaxy approximately 780 kiloparsecs (2.5 million light-years) from Earth, and the nearest major galaxy to the Milky Way.

Andromeda Galaxy and Large Magellanic Cloud · Andromeda Galaxy and Orders of magnitude (length) · See more »

Astronomy & Astrophysics

Astronomy & Astrophysics is a peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics.

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Canis Major Overdensity

The Canis Major Dwarf Galaxy (CMa Dwarf) or Canis Major Overdensity (CMa Overdensity) is a disputed dwarf irregular galaxy in the Local Group, located in the same part of the sky as the constellation Canis Major.

Canis Major Overdensity and Large Magellanic Cloud · Canis Major Overdensity and Orders of magnitude (length) · See more »

Globular cluster

A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite.

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Kilometre

The kilometre (International spelling as used by the International Bureau of Weights and Measures; SI symbol: km; or) or kilometer (American spelling) is a unit of length in the metric system, equal to one thousand metres (kilo- being the SI prefix for). It is now the measurement unit used officially for expressing distances between geographical places on land in most of the world; notable exceptions are the United States and the road network of the United Kingdom where the statute mile is the official unit used.

Kilometre and Large Magellanic Cloud · Kilometre and Orders of magnitude (length) · 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.

Large Magellanic Cloud and Light-year · Light-year and Orders of magnitude (length) · See more »

Local Group

The Local Group is the galaxy group that includes the Milky Way.

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Milky Way

The Milky Way is the galaxy that contains our Solar System.

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Moon

The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.

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Orders of magnitude (length)

The following are examples of orders of magnitude for different lengths.

Large Magellanic Cloud and Orders of magnitude (length) · Orders of magnitude (length) and Orders of magnitude (length) · See more »

Parsec

The parsec (symbol: pc) is a unit of length used to measure large distances to astronomical objects outside the Solar System.

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Sagittarius Dwarf Spheroidal Galaxy

The Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph), also known as the Sagittarius Dwarf Elliptical Galaxy (Sgr dE or Sag DEG), is an elliptical loop-shaped satellite galaxy of the Milky Way.

Large Magellanic Cloud and Sagittarius Dwarf Spheroidal Galaxy · Orders of magnitude (length) and Sagittarius Dwarf Spheroidal Galaxy · See more »

Satellite galaxy

A satellite galaxy is a smaller companion galaxy that travels on bound orbits within the gravitational potential of a more massive and luminous host galaxy (also known as the primary galaxy).

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Second

The second is the SI base unit of time, commonly understood and historically defined as 1/86,400 of a day – this factor derived from the division of the day first into 24 hours, then to 60 minutes and finally to 60 seconds each.

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Small Magellanic Cloud

The Small Magellanic Cloud (SMC), or Nubecula Minor, is a dwarf galaxy near the Milky Way.

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SN 1987A

SN 1987A was a peculiar type II supernova in the Large Magellanic Cloud, a dwarf galaxy satellite of the Milky Way.

Large Magellanic Cloud and SN 1987A · Orders of magnitude (length) and SN 1987A · See more »

Spiral galaxy

Spiral galaxies form a class of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae(pp. 124–151) and, as such, form part of the Hubble sequence.

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Supernova

A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.

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Tarantula Nebula

The Tarantula Nebula (also known as 30 Doradus) is an H II region in the Large Magellanic Cloud (LMC).

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The Astronomical Journal

The Astronomical Journal (often abbreviated AJ in scientific papers and references) is a peer-reviewed monthly scientific journal owned by the American Astronomical Society and currently published by IOP Publishing.

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The Astrophysical Journal

The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.

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The list above answers the following questions

Large Magellanic Cloud and Orders of magnitude (length) Comparison

Large Magellanic Cloud has 82 relations, while Orders of magnitude (length) has 843. As they have in common 21, the Jaccard index is 2.27% = 21 / (82 + 843).

References

This article shows the relationship between Large Magellanic Cloud and Orders of magnitude (length). To access each article from which the information was extracted, please visit:

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