To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

TOI-1431 b
Discovery
Discovered byTESS, MASCARA
Discovery date2021
Transit
Orbital characteristics
0.046
Eccentricity0
2.7 d
Inclination80.4
StarTOI-1431
Physical characteristics
Mean radius
1.49 RJ
Mass3.12 MJ
Temperature2700±2600 K

TOI-1431 b, also known as MASCARA-5b, is an Ultra-hot Jupiter exoplanet orbiting TOI-1431 in the constellation of Cepheus. It has an orbital period of 2.7 days.[1] Its dayside temperature is 2,700 K (2,427 °C), making it hotter than 40% of stars in our galaxy.[2] The nightside temperature is 2,600 K (2,300 °C).[3][4][5]

References

  1. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2023-09-05.
  2. ^ "Scientists uncover a 'hellish' planet so hot it could vaporize most metals". CNET. April 27, 2021. Retrieved April 27, 2021.
  3. ^ "'Hellish' new planet discovered". University of Southern Queensland. April 27, 2021. Retrieved April 27, 2021.
  4. ^ Brett Christopher Addison; et al. (2021), "TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars", Posters from the Tess Science Conference Ii (Tsc2: 64, arXiv:2104.12078, Bibcode:2021tsc2.confE..64A, doi:10.5281/zenodo.5126266, S2CID 240578462
  5. ^ Stangret, M.; et al. (2021), "The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions", Astronomy & Astrophysics, 654: A73, arXiv:2104.12414, Bibcode:2021A&A...654A..73S, doi:10.1051/0004-6361/202040100, S2CID 233393996
This page was last edited on 22 November 2023, at 05:32
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.