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 2 August 2024 by SafariScribe (talk).

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Declined by SafariScribe 4 seconds ago. Last edited by SafariScribe 4 seconds ago. Reviewer: Inform author.

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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 Nebule 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. 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. 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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