Nothing Special   »   [go: up one dir, main page]

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.
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

HD 149026 b

De Wikipedia, la enciclopedia libre

Smertrios

HD 149026 b (Visión artística)
Descubrimiento
Descubridor B. Sato, D. Fischer,
G. Henry et al. en telescopio Keck y
telescopio Subaru
Fecha 1 de julio de 2005
Método de detección Velocidad radial
Categoría planeta extrasolar
Estrella madre
Orbita a HD 149026
Constelación Hércules
Ascensión recta (α) 247,62341035048 grados sexagesimales
Declinación (δ) 38,347308581549 grados sexagesimales
Elementos orbitales
Inclinación 84,55 grados sexagesimales
Argumento del periastro 100 grados sexagesimales
Semieje mayor 0.042 UA
Excentricidad 0
Elementos orbitales derivados
Periastro o perihelio (2.453.530,751 DJ)
Semi-amplitud 43,2 ± 2,6 m/s
Período orbital sideral 2.8758882 ± 0.0000061[1]​ días
Características físicas
Masa 0.36 ± 0.03 MJúpiter
Radio 0.725 ± 0.03 RJúpiter
Características atmosféricas
Temperatura 2300 ± 200[2]​ K
[editar datos en Wikidata]

Smertrios, es un planeta extrasolar, que orbita la estrella Ogma. Es excepcional por poseer un núcleo planetario muy grande, y también por su elevada temperatura superficial, calculada en torno a 2300 kelvin.

Referencias

  1. ↑ Winn et al. (2008). Five New Transits of the Super-Neptune HD 149026b 675 (2). The Astrophysical Journal. pp. 1531 - 1537.  (web Preprint)
  2. ↑ Harrington, Joseph; Statia Luszcz, Sara Seager, Drake Deming & L. Jeremy Richardson (9 de mayo de 2007). The hottest planet. Nature advance online publishing. doi 10.1038/nature05863. 
Esta página se editó por última vez el 30 mar 2021 a las 01:48.
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