4K Intel Video Editing Computer - One year update! @happyfoxproductions

Happyfox Productions | 4K Intel Video Editing Computer - One year update! @happyfoxproductions | Uploaded November 2016 | Updated October 2024, 7 hours ago.
Hey guys I just wanted to put out a quick update video on my "Monster Computer" that I built last year. I am very happy with it and as a first time build It came out not bad!
Here are the specs
Processor: Intel Core I7 5960X 8 core processor
Motherboard: ASUS X99 PRO 3.1 boost
Graphics Card: MSI GeForce GTX 980Ti 6G
RAM: GSKILL RIPJAW SERIES DDR4 32 GIG
Liquid Cooler: NZXT X61 Liquid Cooler
Hard drive array: 4 Samsung SSD's
Western Digital Black 4TB internal drive
2 NZXT case fans
Case: NZXT H630 white full tower ATX case
PSU: 1,000 Watt EVGA Fully Modular Power Supply
Optical Drive: LG Bluray, DVD, CD read write drive
Operating System: Windows 10Pro OEM
Peripherals: Microsoft ergonomic keyboard
JBL LSR LSR 305 studio monitors
ISO Acoustics stands
Focusrite 2i4 Audio interface
Screen: Asus PB278 2K monitor

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$How the Telescope Revolutionized the World Our National History Day Project for the 2012 NHD competition. By John Haug, Justin Melson, Justin Remulla. How the Telescope Revolutionized the World A telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic radiation (such as visible light). The first known practical telescopes were invented in the Netherlands at the beginning of the 17th century, using glass lenses. They found use in terrestrial applications and astronomy. Within a few decades, the reflecting telescope was invented, which used mirrors. In the 20th century many new types of telescopes were invented, including radio telescopes in the 1930s and infrared telescopes in the 1960s. The word telescope now refers to a wide range of instruments detecting different regions of the electromagnetic spectrum, and in some cases other types of detectors. The word telescope (from the Greek τῆλε, tele far and σκοπεῖν, skopein to look or see; τηλεσκόπος, teleskopos far-seeing) was coined in 1611 by the Greek mathematician Giovanni Demisiani for one of Galileo Galileis instruments presented at a banquet at the Accademia dei Lincei.[1][2][3] In the Starry Messenger, Galileo had used the term perspicillum. The earliest recorded working telescopes were the refracting telescopes that appeared in the Netherlands in 1608. Their development is credited to three individuals: Hans Lippershey and Zacharias Janssen, who were spectacle makers in Middelburg, and Jacob Metius of Alkmaar.[4] Galileo heard about the Dutch telescope in June 1609, built his own within a month,[5] and greatly improved upon the design in the following year. The idea that the objective, or light-gathering element, could be a mirror instead of a lens was being investigated soon after the invention of the refracting telescope.[6] The potential advantages of using parabolic mirrors—reduction of spherical aberration and no chromatic aberration—led to many proposed designs and several attempts to build reflecting telescopes.[7] In 1668, Isaac Newton built the first practical reflecting telescope, of a design which now bears his name, the Newtonian reflector. The invention of the achromatic lens in 1733 partially corrected color aberrations present in the simple lens and enabled the construction of shorter, more functional refracting telescopes. Reflecting telescopes, though not limited by the color problems seen in refractors, were hampered by the use of fast tarnishing speculum metal mirrors employed during the 18th and early 19th century—a problem alleviated by the introduction of silver coated glass mirrors in 1857,[8] and aluminized mirrors in 1932.[9] The maximum physical size limit for refracting telescopes is about 1 meter (40 inches), dictating that the vast majority of large optical researching telescopes built since the turn of the 20th century have been reflectors. The largest reflecting telescopes currently have objectives larger than 10 m (33 feet). The 20th century also saw the development of telescopes that worked in a wide range of wavelengths from radio to gamma-rays. The first purpose built radio telescope went into operation in 1937. Since then, a tremendous variety of complex astronomical instruments have been developed.$