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
Languages
Recent
Show all languages
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

Kepler-451b
Discovery
Discovery siteKepler Space Observatory
Discovery date2015
Eclipse Timing Variations
Orbital characteristics
0.92 ± 0.02 AU (137,600,000 ± 3,000,000 km)[1]
Eccentricitynull
416±2 d[1]
Star2MASS J19383260+4603591 A/B
Physical characteristics
Mass604±32[1] MEarth

Kepler-451b, also known as 2MASS J19383260+4603591 b, is a circumbinary exoplanet orbiting the two stars 2MASS J19383260+4603591. It has a mass of 604±32 Earth Masses or 1.9±0.1 Jupiter Masses. It was discovered using Eclipse Timing Variations by the Kepler space telescope in 2015.[2]

The existence of the planet was disputed in 2020 though,[3] but in 2022 a confirmation was announced.[4]

References

  1. ^ a b c "2MASS J19383260+4603591 b/Kepler-451 b CONFIRMED PLANET OVERVIEW PAGE". NASA Exoplanet Archive. Retrieved 2015-10-08.
  2. ^ Detection of a planet in the sdB + M dwarf binary system 2M 1938+4603
  3. ^ Krzesinski, J.; Blokesz, A.; Siwak, M.; Stachowski, G. (2020), "The quest for planets around subdwarfs and white dwarfs from Keplerspace telescope fields", Astronomy & Astrophysics, 642: A105, arXiv:2009.02749, doi:10.1051/0004-6361/202038121, S2CID 221516872
  4. ^ Esmer, Ekrem Murat; Baştürk, Özgür; Selam, Selim Osman; Aliş, Sinan (2022), "Detection of two additional circumbinary planets around Kepler-451", Monthly Notices of the Royal Astronomical Society, 511 (4): 5207–5216, arXiv:2202.02118, doi:10.1093/mnras/stac357


This page was last edited on 27 December 2023, at 02:02
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.