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Metal Evolution is a 2011 documentary series directed by anthropologist and filmmaker Sam Dunn and director, producer and music supervisor Scot McFadyen about heavy metal subgenres, with new episodes airing every Friday at 10 pm EST on MuchMore [1] [2] and Saturday at 10pm EST on VH1 Classic. [3]
Evolution of metal ions in biological systems refers to the incorporation of metallic ions into living organisms and how it has changed over time. Metal ions have been associated with biological systems for billions of years, but only in the last century have scientists began to truly appreciate the scale of their influence.
A new version was presented in the related TV series Metal Evolution which included a new "Pre-Metal" field that listed non-metal bands that had an influence on heavy metal and also listed additional bands as examples of the various subgenres. The film's flow chart of metal genres. Early Metal (1966–1971)
Metallurgy derives from the Ancient Greek μεταλλουργός, metallourgós, "worker in metal", from μέταλλον, métallon, "mine, metal" + ἔργον, érgon, "work" The word was originally an alchemist's term for the extraction of metals from minerals, the ending -urgy signifying a process, especially manufacturing: it was discussed in this sense in the 1797 Encyclopædia ...
Dunn co-directed and hosted the biggest-ever TV series on the history of heavy metal, Metal Evolution, which reached #1 on VH1 Classic (USA) and M3 (Canada), and most-recently co-directed the Netflix original series Hip-Hop Evolution which has been awarded a Peabody, [2] an International Emmy, [3] and a Canadian Screen Award.
While it is, in many aspects, similar to post-rock, post-metal tends to include lower-tuned guitars, distorted guitar(s), heavy atmospherics, gradual evolution of song structure, and a minimal emphasis on vocals. Post-metal stresses emotion, contrasting the ambiance of post-rock with the weight and bombast of metal.
A timeline of events specifically related to the origin and evolution of hard rock and heavy metal starting from the 1960s and continuing up to present day. Subcategories This category has the following 2 subcategories, out of 2 total.
These became commonly known as population I (metal-rich) and population II (metal-poor) stars. A third, earliest stellar population was hypothesized in 1978, known as population III stars. [13] [14] [15] These "extremely metal-poor" (XMP) stars are theorized to have been the "first-born" stars created in the Universe.