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.

How to transfigure the Wikipedia

Would you like Wikipedia to always look as professional and up-to-date? We have created a browser extension. It will enhance any encyclopedic page you visit with the magic of the WIKI 2 technology.

Try it — you can delete it anytime.

Install in 5 seconds
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.
Great Wikipedia has got greater.
.
Leo
Newton
Brights
Milds

Kepler-560b

From Wikipedia, the free encyclopedia

Kepler-560b
Discovery[1]
Discovered byKepler space telescope
Discovery date10 May 2016
Transit
Designations
KOI-463.01, Kepler-560 Bb, KIC 8845205 b
Orbital characteristics
0.0899+0.0031
−0.0062 AU[2]
Eccentricity0.17[3]
18.4776196+0.0000130
−0.0000132 d[3]
Inclination89.606°+0.0031°
−0.094°[2]
StarKepler-560 B
Physical characteristics
Mean radius
1.93+0.15
−0.14 R🜨[3]
Temperature298+22
−32 K[2]

Kepler-560b, or more correctly Kepler-560 Bb,[4] is a confirmed exoplanet orbiting the secondary star of the binary star system Kepler-560.[3][5] It is only 287 light-years away.[6] Though not listed in the Habitable Exoplanets Catalog, one study gives the planet an 85% chance of being in the habitable zone.[2]

Size comparison
Earth Kepler-560b
Exoplanet

YouTube Encyclopedic

  • 1/3
    Views:
    1 592
    14 309
    124 622
  • 3. KEPLER MISSION | MASTERING SCIENCE & TECHNOLOGY | LETS LEARN | NEO IAS
  • Upgrading Acer aspire E14 HDD to SSD
  • 50 PREGUNTAS DE CIENCIA GENERAL | Nivel Difícil ✅

Transcription

See also

References

  1. ^ Morton, Timothy D.; Bryson, Stephen T.; Coughlin, Jeffrey L.; Rowe, Jason F.; Ravichandran, Ganesh; et al. (May 2016). "False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives". The Astrophysical Journal. 822 (2): 86. arXiv:1605.02825. Bibcode:2016ApJ...822...86M. doi:10.3847/0004-637X/822/2/86. S2CID 20832201.
  2. ^ a b c d Torres, Guillermo; et al. (December 2017). "Validation of Small Kepler Transiting Planet Candidates in or near the Habitable Zone". The Astronomical Journal. 154 (6): 264. arXiv:1711.01267. Bibcode:2017AJ....154..264T. doi:10.3847/1538-3881/aa984b. S2CID 73678176.
  3. ^ a b c d Mann, Andrew W.; et al. (June 2017). "The Gold Standard: Accurate Stellar and Planetary Parameters for Eight Kepler M Dwarf Systems Enabled by Parallaxes". The Astronomical Journal. 153 (6): 267. arXiv:1705.01545. Bibcode:2017AJ....153..267M. doi:10.3847/1538-3881/aa7140. S2CID 119325474.
  4. ^ "Kepler-560 b". NASA Exoplanet Archive. Retrieved 22 January 2021.
  5. ^ "Open Exoplanet Catalogue - Kepler-560 b". www.openexoplanetcatalogue.com. Retrieved 2021-01-22.
  6. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2021-01-22.
Stub icon

This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it.

This page was last edited on 24 November 2023, at 04:41
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.
Contact WIKI 2
Introduction
Terms of Service
Privacy Policy