SONY FX6 Cinematic Footage (with raw footage!) @happyfoxproductions

Uploaded October 2021 | Updated September 2026, 2 weeks ago

Here are a couple of shots I filmed with my new Sony FX6. I currently have the Sony 50 F/1.2 and Sony 24-105 F/4 lenses to go with it. I'm in love with this camera!
All shots were filmed with autofocus (I never touched the lens on any shot in this video, that is crazy! Especially cause most shots were shot at 1.2!)

Most shots are filmed XAVC-L in UHD or 1080P

Steady shots were filmed on my One Wheel or with my Glidecam HD2000

The footage at the end is the same sequence, just ungraded for reference.

Edited in Premiere Pro
Graded in Davinci Resolve
Additional film emulation with Dehancer pro (seriously the best film emulation software out there)

Follow for more!
Instagram: @justinmelson
Instagram: @happyfoxproductions
Facebook: Justin Melson

#SonyFX6
#cinematic
#Sony501.2lens

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SONY FX6 Cinematic Footage (with raw footage!)

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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.$

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