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

HIP 41378 d

From Wikipedia, the free encyclopedia

HIP 41378 d
Discovery
Discovery dateJune 2016
Transit
Orbital characteristics
0.88 ± 0.01 au
278.3618 ± 0.0005[1][2] d
StarHIP 41378[2]
Physical characteristics
Mean radius
3.54±0.06 R🜨
Mass<4.6[1] M🜨

HIP 41378 d (also known as EPIC 211311380 d) is an exoplanet orbiting around the F-type star HIP 41378. It has a radius about 3.5 times that of Earth.[2] Planetary orbit is significantly inclined to the equatorial plane of the parent star, misalignment been equal to 57.1+26.4
−17.9°.[3]

YouTube Encyclopedic

  • 1/1
    Views:
    1 775
  • Exoplanets and the Hidden Universe - Astronomy on Tap - 5/18/20

Transcription

See also

References

  1. ^ a b Santerne, A.; Malavolta, L.; Kosiarek, M. R.; Dai, F.; Dressing, C. D.; Dumusque, X.; Hara, N. C.; Lopez, T. A.; Mortier, A.; Vanderburg, A.; Adibekyan, V.; Armstrong, D. J.; Barrado, D.; Barros, S. C. C.; Bayliss, D.; Berardo, D.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Brown, D. J. A.; Buchhave, L. A.; Butler, R. P.; Collier Cameron, A.; Cosentino, R.; Crane, J. D.; Crossfield, I. J. M.; Damasso, M.; Deleuil, M. R.; Delgado Mena, E.; et al. (2019). "An extremely low-density and temperate giant exoplanet". arXiv:1911.07355 [astro-ph.EP].
  2. ^ a b c "HIP 41378 d CONFIRMED PLANET OVERVIEW PAGE". NASA Exoplanet Archive. Retrieved 2016-07-08.
  3. ^ Grouffal, S.; Santerne, A.; Bourrier, V.; Dumusque, X.; Triaud, A. H. M. J.; Malavolta, L.; Kunovac, V.; Armstrong, D. J.; Attia, O.; Barros, S. C. C.; Boisse, I.; Deleuil, M.; Demangeon, O. D. S.; Dressing, C. D.; Figueira, P.; Lillo-Box, J.; Mortier, A.; Nardiello, D.; Santos, N. C.; Sousa, S. G. (2022), "Rossiter-Mc Laughlin detection of the 9-month period transiting exoplanet HIP41378 D", Astronomy & Astrophysics, 668: A172, arXiv:2210.14125, doi:10.1051/0004-6361/202244182, S2CID 253107437


Stub icon

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

This page was last edited on 24 February 2023, at 05:15
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