Draft:Proplyd 133-353

Proplyd 133-353
	Artist interpretation of Proplyd 133-353
Discovery
Discovery date	2016
Physical characteristics
Equatorial radius	7.4 RJ
Mass	13.0 MJ
Mean density	Unknown
Temperature	2,450K

Submission declined on 7 September 2024 by Dr vulpes (talk).

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Declined by Dr vulpes 2 months ago. Last edited by Citation bot 45 days ago. Reviewer: Inform author.

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Submission declined on 2 August 2024 by SafariScribe (talk).

This submission is not adequately supported by reliable sources. Reliable sources are required so that information can be verified. If you need help with referencing, please see Referencing for beginners and Citing sources.

Declined by SafariScribe 3 months ago.

Comment: Article needs more sources, try looking on Google Scholar or Archive.org. If you need help feel free to leave a message on my talk page. Dr vulpes (Talk) 07:46, 7 September 2024 (UTC)

Comment: Wikipedia cannot cite itself, hence unreliable. Safari Scribe^{Edits! Talk!} 18:26, 2 August 2024 (UTC)

Proplyd 133-353 is possibly the largest known exoplanet^[1]. This celestial body is likely a sub-brown dwarf/rouge planet. Proplyd 133-353 is likely not able to fuse deuterium disqualifying it from being a brown dwarf, the mass limit for deuterium fusion is slightly over 13M_J^[2] and Proplyd 133-353's mass is likely under this threshold. Proplyd likely has a photoevaporating disk as shown in the graphic on the right. Proplyd 133-353 is also a very young exoplanet with an age of just 500,000^[3] years making it one of the youngest exoplanets known.

Location

Located in the Orion Nebula Cluster^[3], Proplyd 133-353 is approximately 1,265.5^[3] light years away.

References

^ "List of largest exoplanets", Wikipedia, 2024-07-27, retrieved 2024-08-02
^ Spiegel, David S.; Burrows, Adam; Milsom, John A. (January 2011). "The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets". The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. ISSN 0004-637X.
^ ^a ^b ^c "Proplyd 133-353". Exoplanets, Planets, and Fan made Exoplanets and Planets Wiki. Retrieved 2024-08-02.

[1] "List of largest exoplanets", Wikipedia, 2024-07-27, retrieved 2024-08-02

[2] Spiegel, David S.; Burrows, Adam; Milsom, John A. (January 2011). "The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets". The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. ISSN 0004-637X.

[:0-3] "Proplyd 133-353". Exoplanets, Planets, and Fan made Exoplanets and Planets Wiki. Retrieved 2024-08-02.

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