File:Luhman16.png

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Summary

Description
English: Binary brown-dwarf system 6.5 ly away in the constellation Vela - The primary is of spectral type L7.5 and has 33 times Jupiter's mass - The secondary of type T0.5 has 29 times Jupiter's mass and exhibit patchy global clouds that obscure parts of its surface - The brown dwarfs are separated by 3 AU and orbit in a 27 year period -
Date
Source Own work
Author Pablo Carlos Budassi

Image processed and rendered especially for Wikimedia.org by Pablo Carlos Budassi. Please mention original author's name along with each image copy you use. Suggestions for improving this image are welcome. Please contact me for any comments or suggestions: pablocarlosbudassi@gmail.com fb https://www.facebook.com/pablocarlosbudassi/ tw https://twitter.com/budassiuniverse ig https://www.instagram.com/pablocarlosbudassi/ yt https://www.youtube.com/channel/UCPOu7Xqg4jqrO4o3MZm-Baw

This image and the description are part of the project "The Celestial Zoo": https://www.facebook.com/thecelestialzoo/ https://instagtam.com/thecelestialzoo[dead link]

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Captions

Artist's conception of Luhman 16 binary star system.

9 August 2020

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current20:44, 15 September 20201,560 × 1,499 (619 KB)CelestialobjectsUploaded own work with UploadWizard

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