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User:Brothejr

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Retired
This user is no longer active on Wikipedia.

If you have come to this page looking for some major conspiracy then before you go on further: I don’t know if aliens are real, who knows who killed JFK, and I’m pretty sure Tupac is dead!

What I am here for[edit]

I originally came here due to Wikipedia appearing in the news due to certain outside events. After a short bit, I saw various bits of vandalism and POV pushing going on and decided that reverting vandalism appealed to me. I am not some elite editor who posts all the articles they have started and worries about how long they've been a part of Wikipedia, nor am I some highfalutin expert who worries that no one recognizes me as an expert. My main concern is keeping the vandalism down to a minimum and reading good articles. I'm not after glory, barn stars, medals, etc. I am just here to keep things working and stay semi in the background.

About myself[edit]

Here goes: I grew up in Skaneateles New York. I enrolled at State University of New York at Oneonta where I joined the co-ed voluntary service fraternity Alpha Phi Omega and graduated with a degree in English.

For a short time, I was a door-to-door insurance salesman. After that frightening experience, I enlisted in the U.S. Navy in August 2001. I was then transferred to Naval Submarine Base New London in Groton Ct where I was stationed on board the USS Pittsburgh (SSN-720) as a Sonar Technician. I changed rates and became a U.S. Navy Quartermaster. I was then transferred to Naval Station Norfolk, Norfolk, VA where I was stationed on board the USS Shreveport (LPD-12). From there I had been honorably discharged and currently I work in the civilian nuclear power industry.

Some of my many myriad of hobbies have been: amateur photography, asylum history, creative writing, and much more than I can remember right now.

Web pages I run[edit]

I am also on:

Picture of the Day[edit]

Heart Nebula
The Heart Nebula is an emission nebula, 7500 light years from Earth, located in the Perseus Arm of the Milky Way in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787. Spanning almost 2 degrees in the sky, its shape is driven by stellar winds from the hot stars in its core. The nebula displays glowing ionized hydrogen gas and darker dust lanes, and is also made up of ionised oxygen and sulfur gasses, which cause rich blue and orange colours to be seen in narrowband images. This photograph of the Heart Nebula, with the Fish Head Nebula also visible in the top right corner, is a narrowband image captured on a 70mm scope with a capture period of around 44 hours.Photograph credit: Ram Samudrala

Some reference links for myself[edit]