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
Spanish 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.
Great Wikipedia has got greater.
.
Leo
Newton
Brights
Milds

Archivo:NASA-JPL-Caltech - Double the Rubble (PIA11375) (pd).jpg

De Wikipedia, la enciclopedia libre

Ver la imagen en su resolución original ‎(3000 × 1600 píxeles; tamaño de archivo: 2,15 MB; tipo MIME: image/jpeg)

Resumen

Descripción
English: This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.

Epsilon Eridani is located about 10 light-years away in the constellation Eridanus. It is visible in the night skies with the naked eye.

The system's inner asteroid belt appears as the yellowish ring around the star, while the outer asteroid belt is in the foreground. The outermost comet ring is too far out to be seen in this view, but comets originating from it are shown in the upper right corner.

Astronomers think that each of Epsilon Eridani's asteroid belts could have a planet orbiting just outside it, shepherding its rocky debris into a ring in the same way that Jupiter helps keep our asteroid belt confined. The planet near the inner belt was previously identified in 2000 via the radial velocity, or "star wobble," technique, while the planet near the outer belt was inferred when Spitzer discovered the belt.

The inner belt orbits at a distance of about 3 astronomical units from its star —or about the same position as the asteroid belt in our own solar system (an astronomical unit is the distance between Earth and our sun). The second asteroid belt lies at about 20 astronomical units from the star, or a position comparable to Uranus in our solar system. The outer comet ring orbits from 35 to 90 astronomical units from the star; our solar system's analogous Kuiper Belt extends from about 30 to 50 astronomical units from the sun.
Français : A traduire...
Fecha Fecha desconocida
Unknown date
Fuente Double the Rubble
Autor NASA/JPL-Caltech
Este archivo fue catalogado por
Jet Propulsion Lab
de la Administración Nacional de Aeronáutica y del Espacio (NASA) de los Estados Unidos de Américabajo el identificador de foto: PIA11375.

Esta etiqueta no indica el estado de los derechos de autor del trabajo adjunto. Se requiere una etiqueta de derechos de autor normal. Para más información vea Commons:Sobre las licencias.
Otros idiomas:

العربية ∙ беларуская (тарашкевіца) ∙ български ∙ català ∙ čeština ∙ dansk ∙ Deutsch ∙ English ∙ español ∙ فارسی ∙ français ∙ galego ∙ magyar ∙ հայերեն ∙ Bahasa Indonesia ∙ italiano ∙ 日本語 ∙ македонски ∙ മലയാളം ∙ Nederlands ∙ polski ∙ português ∙ русский ∙ sicilianu ∙ slovenščina ∙ Türkçe ∙ українська ∙ 简体中文 ∙ 繁體中文 ∙ +/−

Licencia

Public domain Este archivo es de dominio público porque fue creado por la NASA. Las políticas sobre copyright de la NASA estipulan que «el material de la NASA no está protegido con copyright a menos que se indique lo contrario». (Políticas sobre copyright de la NASA o Políticas sobre la utilización de imágenes del Jet Propulsion Laboratory).
Advertencias:

Historial del archivo

Haz clic sobre una fecha y hora para ver el archivo tal como apareció en ese momento.

Fecha y horaMiniaturaDimensionesUsuarioComentario
actual21:49 13 feb 2017Miniatura de la versión del 21:49 13 feb 20173000 × 1600 (2,15 MB)David Levyrecompressed TIFF file
05:57 7 nov 2011Miniatura de la versión del 05:57 7 nov 20113000 × 1600 (4,11 MB)OgreBot(BOT): Reverting to most recent version before archival
05:57 7 nov 2011Miniatura de la versión del 05:57 7 nov 20113000 × 1600 (625 kB)OgreBot(BOT): Uploading old version of file from en.wikipedia; originally uploaded on 2008-10-27 21:14:20 by Cookbutter
18:51 14 nov 2008Miniatura de la versión del 18:51 14 nov 20083000 × 1600 (4,11 MB)ComputerHotline{{Information |Description={{en|1=This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previous

Uso global del archivo

Las wikis siguientes utilizan este archivo:

Obtenido de «https://es.wikipedia.org/wiki/Archivo:NASA-JPL-Caltech_-_Double_the_Rubble_(PIA11375)_(pd).jpg»
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