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The constellation Libra marked on a naked eye view. Overall, there are 83 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5. [a] [2] The brightest stars in Libra form a quadrangle that distinguishes it for the unaided observer. Traditionally, Alpha and Beta Librae are considered to represent the scales ...
This image is a derivative work of the following images: File:Libra_constellation_map.png licensed with Cc-by-sa-3.0-migrated, GFDL 2005-01-07T17:44:15Z Maximaximax 378x332 (15793 Bytes) Libra constellation (from en:) {{GFDL}} Uploaded with derivativeFX
α Librae (Latinised to Alpha Librae) is the system's Bayer designation.. Zubenelgenubi / ˌ z uː b ən ɛ l dʒ ə ˈ n uː b i /, also rendered Zuben Elgenubi, derives from the Arabic ّالزُبَانَى الجَنُوبِي al-zubānā al-janūbiyy "the southern claw", which was coined before Libra was recognized as a constellation distinct from Scorpius.
Constellation map. Subcategories. This category has the following 2 subcategories, out of 2 total. ... Libra (constellation) * List of stars in Libra; 0–9. 2MASS ...
NGC 5915 is a barred spiral galaxy in the constellation of Libra. Its velocity with respect to the cosmic microwave background is 2449 ± 13 km/s, which corresponds to a Hubble distance of 36.12 ± 2.54 Mpc (∼118 million light-years). [1] It was discovered by British astronomer John Herschel on 5 June 1836. [2]
A celestial map by the Dutch cartographer Frederik de Wit, 1670. A star chart is a celestial map of the night sky with astronomical objects laid out on a grid system. They are used to identify and locate constellations, stars, nebulae, galaxies, and planets. [1] They have been used for human navigation since time immemorial. [2]
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NGC 5861 is an intermediate spiral galaxy in constellation Libra. It is located at a distance of about 85 million light years from Earth, which, given its apparent dimensions, means that NGC 5861 is about 80,000 light years across. Center image by Hubble Space Telescope. The galaxy features two long spiral arms that dominate the optical disk. [2]
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