User:Tomruen

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Contact[edit]

Self

Hi, my name is Tom Ruen. If you'd like to contact me, try out the form at: Special:Emailuser/tomruen

I also edit from User:SockPuppetForTomruen, mostly for eclipses.

My work here[edit]

I first came on here to edit on April 28, 2004 (19 years ago now!) It is an addicting idea to try to add to something much bigger than I could ever do. I am a little skeptical over the idea of freedom to change anything, but overall I'm very impressed by the quality of articles and I have faith good work is being done and I can add to it.

There are many quality websites out there and it seems silly to duplicate too much. I like the idea of learning about something and testing my knowledge by trying to share it. For me that motivates much of my efforts here.

Primary topics I've worked on include geometry, and astronomy.

My specialty has primarily been image generation, perhaps because I've found so many articles where useful images were absent. I try to make quality images, but I will compromise perfection for meaningful improvement. I'm happy if anyone can replace my images with better ones.

Active work and subpages[edit]

About me[edit]

Pictures[edit]

EarthMoonCharonCharonNixNixKerberosKerberosStyxStyxHydraHydraPlutoPlutoDysnomiaDysnomiaErisErisNamakaNamakaHi'iakaHi'iakaHaumeaHaumeaMakemakeMakemakeMK2MK2XiangliuXiangliuGonggongGonggongWeywotWeywotQuaoarQuaoarSednaSednaVanthVanthOrcusOrcusActaeaActaeaSalaciaSalacia2002 MS42002 MS4File:10 Largest Trans-Neptunian objects (TNOS).png
Artistic comparison of Pluto, Eris, Makemake, Haumea, Gonggong (2007 OR10), Sedna, Quaoar, Orcus, 2002 MS4, and Salacia.

Links[edit]

Wiki news[edit]

  • [3] Jimmy Wales is founder of Wikipedia, the self-organizing, self-correcting, ever-expanding, and thoroughly addictive encyclopedia of the future. In this presentation, he explains how Wikipedia's collaborative system works, and why it succeeds. (Recorded July 2005 in Oxford, UK. Duration: 20:47)
  • Jimmy Wales’s benevolent Wikipedia wisdom By DAVID HOROVITZ 07/01/2011
Nemo
Nemo
Tarantula Nebula
The Tarantula Nebula, also known as 30 Doradus, is a large H II region in the Large Magellanic Cloud (LMC). It is one of the largest H II regions in the Local Group, with an estimated diameter around 650 to 1860 light years. It is around 160,000 light-years from Earth and has apparent magnitude of 8. The Tarantula Nebula was first observed by Nicolas-Louis de Lacaille during an expedition to the Cape of Good Hope between 1751 and 1753. This high-resolution photograph was taken by the Hubble Space Telescope and shows the star-forming region of Tarantula Nebula with the R136 super star cluster at its center.Photograph credit: NASA, ESA, Space Telescope Science Institute