User:Sgeureka/Sandbox
You don't need to be Editor-In-Chief to add or edit content to WikiDoc. You can begin to add to or edit text on this WikiDoc page by clicking on the edit button at the top of this page. Next enter or edit the information that you would like to appear here. Once you are done editing, scroll down and click the Save page button at the bottom of the page.
Quick
Template:Signpost-subscription
|
|
[[Image:Westminstpalace.jpg|thumb|100px|right|The Palace of Westminster]]
{{fact|date=November 2009}}
{{inuse}}
{{TOCright}}
Ancient (Stargate)#Language and writing system
| {{sgcite|Lost City|show=all}} | – Template:Sgcite |
| {{sgcite|The Brotherhood|SGA|show=all}} | – Template:Sgcite |
| {{sgcite|Lost City|show=ref}} | – Template:Sgcite |
Disambiguation
- Disambig page style repair: ([[Wikipedia:WikiProject Disambiguation|you can help!]]), see Talk page ("Cleanup")
- [[MoS:DAB#Examples of individual entries that should not be created]]
- WP:DAB#Lists: Lists of articles of which the disambiguated term forms only a part of the article title don't belong here. Disambiguation pages are not search indices. Do not add links that merely contain part of the page title (where there is no significant risk of confusion).
- Wikipedia talk:Manual of Style (disambiguation pages)/Archive 28#.7B.7BSurname.7D.7D - {{surname}} debate
- {{db-redirtypo}} - accidentally created in disambigation page cleanup process; new typo-less redirect has been created instead
- User:Kevinkor2/Research into names of Wikipedia articles
- Wikipedia:Naming conventions (people)#Qualifier between brackets or parentheses
<ref>
<ref>{{cite web |url=http://www.gateworld.net/articles/interviews/wright02.shtml |title=Wright on Target |date=[[March 14]], [[2007]] |publisher=GateWorld.net |accessdate=2006-07-17}}</ref> [1]
<ref>MGM (December 04, 2006). ''[http://www.mgm.com/news/pr4.php MGM Acquires Worldwide Rights to Hysterical Dark Comedy A Dog's Breakfast]''. Press release.</ref> [2]
<div class="small"> <references/> </div>
<div class="references-small" style="-moz-column-count:2; column-count:2;"> <references/> </div>
- ↑ Wright on Target. GateWorld.net (March 14, 2007). Retrieved on 2007-03-11.
- ↑ MGM (December 04, 2006). MGM Acquires Worldwide Rights to Hysterical Dark Comedy A Dog's Breakfast. Press release.
Templates
- See also: User:Sgeureka/Template
- {{R from title without diacritics}}
- {{R from incomplete disambiguation}}
- {{historical}}
- {{R from surname}}
- {{Copy to Wiktionary}}
Now: Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample
Pastel colors: Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample
With images etc.: Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample Template:Wikipedia:Template standardisation/colorsample
The Sun (Latin: Sol) is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for about 99.8% of the solar system's mass. Energy from the Sun—in the form of sunlight—supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather.
The Sun is composed of hydrogen (about 74% of its mass, or 92% of its volume), helium (about 25% of mass, 7% of volume), and trace quantities of other elements. The Sun has a spectral class of G2V. G2 implies that it has a surface temperature of approximately 5,780 K (or approximately 5,515 degrees Celsius / 9,940 Fahrenheit), giving it a white color which, because of atmospheric scattering, appears yellow as seen from the surface of the Earth. This is a subtractive effect, as the preferential scattering of blue photons (causing the sky color) removes enough blue light to leave a residual reddishness that is perceived as yellow. (When low enough in the sky, the Sun appears orange or red, due to this scattering.)
Its spectrum contains lines of ionized and neutral metals as well as very weak hydrogen lines. The V (Roman five) suffix indicates that the Sun, like most stars, is a main sequence star. This means that it generates its energy by nuclear fusion of hydrogen nuclei into helium and is in a state of hydrostatic equilibrium, neither contracting nor expanding over time. There are more than 100 million G2 class stars in our galaxy. Because of logarithmic size distribution, the Sun is actually brighter than 85% of the stars in the galaxy, most of which are red dwarfs.[3]
The Sun orbits the center of the Milky Way galaxy at a distance of approximately 26,000 light-years from the galactic center, completing one revolution in about 225–250 million years. The orbital speed is 217 km/s (135 mi/s), equivalent to one light-year every 1,400 years, and one AU every 8 days.[4]
It is currently travelling through the Local Interstellar Cloud in the low-density Local Bubble zone of diffuse high-temperature gas, in the inner rim of the Orion Arm of the Milky Way Galaxy, between the larger Perseus and Sagittarius arms of the galaxy. Of the 50 nearest stellar systems within 17 light years from the Earth, the sun ranks 4th in absolute magnitude as a fourth magnitude star (M=4.83).
| This article or section is in need of attention from an expert on the subject. Please help recruit one or improve this article yourself. See the talk page for details. Please consider using {{Expert-subject}} to associate this request with a WikiProject |
| This article or section is in need of attention from an expert on the subject. Please help recruit one or improve this article yourself. See the talk page for details. Please consider using {{Expert-subject}} to associate this request with a WikiProject |
| This article may be too long. Please discuss this issue on the talk page and help summarize or split the content into subarticles of an article series. |
| Image:Crystal 128 clock.png | This section is actively undergoing a major edit for a short while. As a courtesy, please do not edit this section while this message is displayed. The person who added this notice will be listed in its edit history. If this section has not been edited recently, please remove this template. This message is intended to help reduce edit conflicts; please remove it between editing sessions to allow others to improve the article. |
The Sun (Latin: Sol) is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for about 99.8% of the solar system's mass. Energy from the Sun—in the form of sunlight—supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather.
The Sun is composed of hydrogen (about 74% of its mass, or 92% of its volume), helium (about 25% of mass, 7% of volume), and trace quantities of other elements. The Sun has a spectral class of G2V. G2 implies that it has a surface temperature of approximately 5,780 K (or approximately 5,515 degrees Celsius / 9,940 Fahrenheit), giving it a white color which, because of atmospheric scattering, appears yellow as seen from the surface of the Earth. This is a subtractive effect, as the preferential scattering of blue photons (causing the sky color) removes enough blue light to leave a residual reddishness that is perceived as yellow. (When low enough in the sky, the Sun appears orange or red, due to this scattering.)
Its spectrum contains lines of ionized and neutral metals as well as very weak hydrogen lines. The V (Roman five) suffix indicates that the Sun, like most stars, is a main sequence star. This means that it generates its energy by nuclear fusion of hydrogen nuclei into helium and is in a state of hydrostatic equilibrium, neither contracting nor expanding over time. There are more than 100 million G2 class stars in our galaxy. Because of logarithmic size distribution, the Sun is actually brighter than 85% of the stars in the galaxy, most of which are red dwarfs.[5]
The Sun orbits the center of the Milky Way galaxy at a distance of approximately 26,000 light-years from the galactic center, completing one revolution in about 225–250 million years. The orbital speed is 217 km/s (135 mi/s), equivalent to one light-year every 1,400 years, and one AU every 8 days.[4]
It is currently travelling through the Local Interstellar Cloud in the low-density Local Bubble zone of diffuse high-temperature gas, in the inner rim of the Orion Arm of the Milky Way Galaxy, between the larger Perseus and Sagittarius arms of the galaxy. Of the 50 nearest stellar systems within 17 light years from the Earth, the sun ranks 4th in absolute magnitude as a fourth magnitude star (M=4.83).
| This article or section is in need of attention from an expert on the subject. Please help recruit one or improve this article yourself. See the talk page for details. Please consider using {{Expert-subject}} to associate this request with a WikiProject |
|
|
This article or section is in need of attention from an expert on the subject. Please help recruit one or improve this article yourself. See the talk page for details. Please consider using {{Expert-subject}} to associate this request with a WikiProject |
|
|
This article may be too long. Please discuss this issue on the talk page and help summarize or split the content into subarticles of an article series. |
| This section is actively undergoing a major edit for a short while. As a courtesy, please do not edit this section while this message is displayed. The person who added this notice will be listed in its edit history. If this section has not been edited recently, please remove this template. This message is intended to help reduce edit conflicts; please remove it between editing sessions to allow others to improve the article. |
The Sun (Latin: Sol) is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for about 99.8% of the solar system's mass. Energy from the Sun—in the form of sunlight—supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather.
The Sun is composed of hydrogen (about 74% of its mass, or 92% of its volume), helium (about 25% of mass, 7% of volume), and trace quantities of other elements. The Sun has a spectral class of G2V. G2 implies that it has a surface temperature of approximately 5,780 K (or approximately 5,515 degrees Celsius / 9,940 Fahrenheit), giving it a white color which, because of atmospheric scattering, appears yellow as seen from the surface of the Earth. This is a subtractive effect, as the preferential scattering of blue photons (causing the sky color) removes enough blue light to leave a residual reddishness that is perceived as yellow. (When low enough in the sky, the Sun appears orange or red, due to this scattering.)
Its spectrum contains lines of ionized and neutral metals as well as very weak hydrogen lines. The V (Roman five) suffix indicates that the Sun, like most stars, is a main sequence star. This means that it generates its energy by nuclear fusion of hydrogen nuclei into helium and is in a state of hydrostatic equilibrium, neither contracting nor expanding over time. There are more than 100 million G2 class stars in our galaxy. Because of logarithmic size distribution, the Sun is actually brighter than 85% of the stars in the galaxy, most of which are red dwarfs.[6]
The Sun orbits the center of the Milky Way galaxy at a distance of approximately 26,000 light-years from the galactic center, completing one revolution in about 225–250 million years. The orbital speed is 217 km/s (135 mi/s), equivalent to one light-year every 1,400 years, and one AU every 8 days.[4]
It is currently travelling through the Local Interstellar Cloud in the low-density Local Bubble zone of diffuse high-temperature gas, in the inner rim of the Orion Arm of the Milky Way Galaxy, between the larger Perseus and Sagittarius arms of the galaxy. Of the 50 nearest stellar systems within 17 light years from the Earth, the sun ranks 4th in absolute magnitude as a fourth magnitude star (M=4.83).
Links
Wikimedia tools
- MartinBot Trigger/Revert Log
- User:Sgeureka Wiki contribution statistics
- Lists the mainspace articles created by Sheynhertz-Unbayg
- http://en.wikipedia.org/w/index.php?title=Special:Log&user=Sheynhertz-Unbayg
Wiki links
- meta:ParserFunctions
- commons:Category:Vote_symbols
- Wikipedia:Administrators' noticeboard/Removal of images from lists of episodes
- Deletion:
- Wikipedia:Example requests for permission - for requesting permission to re-use somebody else's content in Wikipedia
- Wikipedia:Template messages/General
- Template:Infobox Film
- Template:Template sandbox
- Category:Articles in translation
- Category:Aspergian Wikipedians
- Statistics:
- Wikipedia:Service awards
- User:Tony1/How to satisfy Criterion 1a - Featured articles
Personal subpages
To work into articles
- http://www.hollywoodreporter.com/hr/content_display/film/news/e3ib1ebc09603fb86d2fb56fdc5fe936f8d and http://www.worldscreen.com/newscurrent.php?filename=mgm070307.htm - provide source for ADB "buzz in SG fandom", not necessary
- Wikipedia:Mediation Cabal/Cases/2006-02-10 Carnivàle - what does the end of Carnivàle mean?
Timelines
Stargate SG-1
<timeline> TimeAxis = orientation:horizontal format:yyyy ImageSize = width:800 height:300 PlotArea = width:750 height:250 bottom:20 left:20
Colors =
id:canvas value:rgb(0.97,0.97,0.97) id:grid1 value:rgb(0.86,0.86,0.86) id:grid2 value:gray(0.8) id:bars value:rgb(0.96,0.96,0.6) id:leader value:kelleygreen id:2ic value:yellowgreen id:goodsoul value:magenta id:alien value:lightorange id:general value:yellow id:doctor value:oceanblue
BackgroundColors = canvas:canvas
Period = from:1997 till:2010 ScaleMajor = unit:year increment:1 start:1997.0 gridcolor:grid1
bardata=
bar:General text: bar:Leader text: bar:Carter text: bar:Goodsoul text: bar:Teal'c text: bar:Vala text: bar:Doctor text:
plotdata=
- set defaults
width:25 fontsize:L align:left anchor:from textcolor:black fontsize:S mark:(line,white) width:25 shift:(5,-5)
bar:General color:general from:1997.5 till:2004.5 text:"Hammond"
bar:General color:general from:2005.5 till:2007.5 text:"Landry"
bar:Leader color:leader from:1997.5 till:2004.5 text:"O'Neill" from:2005.5 till:2007.5 text:"Mitchell"
bar:Leader color:general from:2004.5 till:2005.5 text:"O'Neill"
bar:Carter color:2ic from:1997.5 till:2004.5 text:"Carter"
bar:Carter color:leader from:2004.5 till:2005.5 text:"Carter"
bar:Carter color:leader from:2005.75 till:2007.5 text:"Carter"
bar:Goodsoul color:goodsoul from:1997.5 till:2002.5 text:"Jackson" from:2003.5 till:2007.50 text:"Jackson"
bar:Goodsoul color:alien from:2002.5 till:2003.5 text:"Jonas"
bar:Teal'c color:alien from:1997.5 till:2007.5 text:"Teal'c"
bar:Vala color:alien from:2005.5 till:2005.75 text:"Vala" from:2006.5 till:2007.5 text:"Vala"
bar:Doctor color:doctor from:1997.75 till:2004.25 text:"Fraiser" from:2005.5 till:2007.5 text:"Lam"
</timeline>
Stargate Atlantis
<timeline> TimeAxis = orientation:horizontal format:yyyy ImageSize = width:800 height:300 PlotArea = width:750 height:250 bottom:20 left:20
Colors =
id:canvas value:rgb(0.97,0.97,0.97) id:grid1 value:rgb(0.86,0.86,0.86) id:grid2 value:gray(0.8) id:bars value:rgb(0.96,0.96,0.6) id:leader value:kelleygreen id:2ic value:yellowgreen id:scientist value:magenta id:alien value:lightorange id:general value:yellow id:doctor value:oceanblue
BackgroundColors = canvas:canvas
Period = from:1997 till:2010 ScaleMajor = unit:year increment:1 start:1997.0 gridcolor:grid1
bardata=
bar:Boss text: bar:Leader text: bar:2IC text: bar:Scientist text: bar:Teyla text: bar:Doctor text:
plotdata=
- set defaults
width:25 fontsize:L align:left anchor:from textcolor:black fontsize:S mark:(line,white) width:25 shift:(5,-5)
bar:Boss color:general from:2004.5 till:2007.5 text:"Weir"
bar:Leader color:leader from:2004.5 till:2008.5 text:"Sheppard"
bar:2IC color:2ic from:2004.5 till:2005.5 text:"Ford"
bar:2IC color:alien from:2005.5 till:2008.5 text:"Ronon"
bar:Scientist color:scientist from:2004.5 till:2008.5 text:"McKay"
bar:Teyla color:alien from:2004.5 till:2008.5 text:"Teyla"
bar:Doctor color:doctor from:2004.5 till:2007.25 text:"Beckett" from:2007.25 till:2008.5 text:"Keller"
</timeline>
Real Sandbox
Userboxes
Blablabla Template:User servertime Template:User Wikipedian For Template:User contrib |
| Year | Championship | Opponent in Final | Score in Final |
| 1985 | Wimbledon | Image:Flag of South Africa.svg/ Image:Flag of the United States.svg Kevin Curren | 6-3, 6-7, 7-6, 6-4 |
| 1986 | Wimbledon (2) | Image:Flag of Germany.svg Ivan Lendl | 6-4, 6-3, 7-5 |
| 1989 | Wimbledon (3) | Image:Flag of Sweden.svg Stefan Edberg | 6-0, 7-6, 6-4 |
| 1989 | U.S. Open | Image:Flag of Germany.svg Ivan Lendl | 7-6, 1-6, 6-3, 7-6 |
| 1991 | Australian Open | Image:Flag of Germany.svg Ivan Lendl | 1-6, 6-4, 6-4, 6-4 |
| 1996 | Australian Open (2) | Image:Flag of the United States.svg Michael Chang | 6-2, 6-4, 2-6, 6-2 |
