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Lambda Ursae Majoris and Star

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

Difference between Lambda Ursae Majoris and Star

Lambda Ursae Majoris vs. Star

Lambda Ursae Majoris (λ Ursae Majoris, abbreviated Lambda UMa, λ UMa), formally named Tania Borealis, is a star in the northern circumpolar constellation of Ursa Major. A star is a luminous spheroid of plasma held together by self-gravity.

Similarities between Lambda Ursae Majoris and Star

Lambda Ursae Majoris and Star have 15 things in common (in Unionpedia): Apparent magnitude, Arabic, Bayer designation, Centre de données astronomiques de Strasbourg, Chinese astronomy, Effective temperature, Giant star, IAU Working Group on Star Names, International Astronomical Union, Latin, Main sequence, Parallax, Stellar atmosphere, Stellar classification, Stellar evolution.

Apparent magnitude

Apparent magnitude is a measure of the brightness of a star or other astronomical object.

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Arabic

Arabic (اَلْعَرَبِيَّةُ, or عَرَبِيّ, or) is a Central Semitic language of the Afroasiatic language family spoken primarily in the Arab world.

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Bayer designation

A Bayer designation is a stellar designation in which a specific star is identified by a Greek or Latin letter followed by the genitive form of its parent constellation's Latin name.

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Centre de données astronomiques de Strasbourg

The Centre de Données astronomiques de Strasbourg (CDS; English translation: Strasbourg Astronomical Data Centre) is a data centre which collects and distributes astronomical information.

Centre de données astronomiques de Strasbourg and Lambda Ursae Majoris · Centre de données astronomiques de Strasbourg and Star · See more »

Chinese astronomy

Astronomy in China has a long history stretching from the Shang dynasty, being refined over a period of more than 3,000 years.

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Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation.

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Giant star

A giant star has a substantially larger radius and luminosity than a main-sequence (or dwarf) star of the same surface temperature.

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IAU Working Group on Star Names

The International Astronomical Union (IAU) established a Working Group on Star Names (WGSN) in May 2016 to catalog and standardize proper names for stars for the international astronomical community.

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International Astronomical Union

The International Astronomical Union (IAU; Union astronomique internationale, UAI) is an international non-governmental organization (INGO) with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach, education, and development through global cooperation.

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Latin

Latin (lingua Latina,, or Latinum) is a classical language belonging to the Italic branch of the Indo-European languages.

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Main sequence

In astronomy, the main sequence is a classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive band.

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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 half-angle of inclination between those two lines.

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Stellar atmosphere

The stellar atmosphere is the outer region of the volume of a star, lying above the stellar core, radiation zone and convection zone.

Lambda Ursae Majoris and Stellar atmosphere · Star and Stellar atmosphere · See more »

Stellar classification

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

Lambda Ursae Majoris and Stellar classification · Star and Stellar classification · See more »

Stellar evolution

Stellar evolution is the process by which a star changes over the course of its lifetime and how it can lead to the creation of a new star.

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The list above answers the following questions

Lambda Ursae Majoris and Star Comparison

Lambda Ursae Majoris has 38 relations, while Star has 412. As they have in common 15, the Jaccard index is 3.33% = 15 / (38 + 412).

References

This article shows the relationship between Lambda Ursae Majoris and Star. To access each article from which the information was extracted, please visit: