File:Brown dwarf type T.jpg
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Summary
[edit]DescriptionBrown dwarf type T.jpg |
English: Brown dwarfs (also called failed stars) are substellar objects that are not massive enough to sustain nuclear fusion of ordinary hydrogen into helium in their cores, unlike a main-sequence star. Instead, they have a mass between the most massive gas giant planets and the least massive stars, approximately 13 to 80 times that of Jupiter. However, they can fuse deuterium and the most massive ones (> 65 MJ) can fuse lithium.
Astronomers classify self-luminous objects by spectral class, a distinction intimately tied to the surface temperature, and brown dwarfs occupy types M, L, T, and Y. As brown dwarfs do not undergo stable hydrogen fusion, they cool down over time, progressively passing through later spectral types as they age. Despite their name, to the naked eye, brown dwarfs would appear in different colors depending on their temperature. The warmest ones are possibly orange or red, while cooler brown dwarfs would likely appear magenta or black to the human eye. Brown dwarfs may be fully convective, with no layers or chemical differentiation by depth. As brown dwarfs have relatively low surface temperatures, they are not very bright at visible wavelengths, emitting most of their light in the infrared. However, with the advent of more capable infrared detecting devices, thousands of brown dwarfs have been identified. The nearest known brown dwarfs are located in the Luhman 16 system, a binary of L- and T-type brown dwarfs about 6.5 light-years from the Sun. Luhman 16 is the third closest system to the Sun after Alpha Centauri and Barnard's Star. |
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Source | Own work |
Author | Pablo Carlos Budassi |
Planet concept illustrated especially for Wikimedia Commons by Pablo Carlos Budassi. Source: https://www.pablocarlosbudassi.com/2021/02/planet-types.html Background image by ESO/Serge Brunier: https://commons.wikimedia.org/wiki/File:ESO_-_Milky_Way.jpg Suggestions for improving this image are welcome: pablocarlosbudassi@gmail.com
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current | 14:10, 15 August 2023 | 1,080 × 1,080 (321 KB) | Celestialobjects (talk | contribs) | Uploaded own work with UploadWizard |
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Image title |
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Author | Pablo Carlos Budassi |
Copyright holder |
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Headline | Artist's impression of a brown dwarf |
Credit/Provider | Created by artist Pablo Carlos Budassi in 2023 (@pablocarlosbudassi) |
Source | https://pablocarlosbudassi.com |
Usage terms |
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Date and time of data generation | 26 March 2021 |
Width | 1,080 px |
Height | 1,080 px |
Bits per component |
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Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS6 (Macintosh) |
File change date and time | 15:10, 9 August 2023 |
Exif version | 2.21 |
Color space | sRGB |
Date metadata was last modified | 12:10, 9 August 2023 |
Date and time of digitizing | 09:09, 30 May 2008 |
Unique ID of original document | xmp.did:0080117407206811B65FEE6CD4839DCA |
Type of item | 13000000 science and technology |
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Contact information | pablocarlosbudassi@gmail.com
www.pablocarlosbudassi.com https://www.pablocarlosbudassi.com/2021/02/planet-types.html Provincia del Chaco 2925 P.A. Mendoza, Mendoza, M5502 Argentina |