After 35 years into a career that spans 35 albums recorded for seven labels, you'd think might get a little complacent. Thankfully the opposite is true, as 2001's is the artist's most daring musical departure and arguably greatest achievement to date. Mining the rich catalog for 12 of its 13 tracks (the closing is a traditional gospel tune) and bringing himself along as producer has resulted in a stunning collection that stands as one of the best in 's bulging catalog. Never a songwriter, the singer/guitarist/harmonica bluesman has maintained a knack for picking top-notch material from the rich blues tradition without resorting to the hoary, over-covered classics of the genre. It's that quality that transforms these tunes into songs, regardless of their origin.

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His history of working with exceptional session musicians is also legendary, and this album's band, which features sideman on keyboards, harmonica wiz, longtime associate on bass, and himself poking around on various songs, is perfect for the spooky, swampy feel he effortlessly conjures here. Choosing from a wide variety of ' material, infuses these unusual tracks with a bluesman's spirit and a crackling energy that practically reinvents the songs, instilling them with an ominous, rhythmic swampy feel. The producer contributes two new tracks ('2:19' and 'Fannin' Street,' the latter is the album's only acoustic cut) that maintain the creepy but upbeat voodoo spirit that trickles and twists throughout. Radhe mujhe tumse mohabbat hai mp3 song download. Sings with a renewed spirit, adding a smoother but no less intense edge than ' typical rusty razor blade soaked whisky growl.

John Hammond Wicked Grin Rarlabs

With his dusky croon and idiosyncratic delivery, tears into this material with relish, spitting out the often offbeat, stream of consciousness lyrics as if he wrote them himself. Only the slow, ambling blues of 'Murder in the Red Barn' would comfortably slot into 's existing oeuvre; the remainder push the bluesman into previously uncharted territory with results that reveal fascinating layers of his own interpretive abilities. An experiment whose success will hopefully yield another volume, this partnership of and brings out the best in both artists' substantial talents.

The crust of the Earth is composed of a great variety of igneous, metamorphic, and sedimentary rocks. The crust is underlain by the mantle. The upper part of the mantle is composed mostly of peridotite, a rock denser than rocks common in the overlying crust. The boundary between the crust and mantle is conventionally placed at the Mohorovi?i?

Discontinuity, a boundary defined by a contrast in seismic velocity. The crust occupies less than 1% of Earth's volume.1 The oceanic crust of the sheet is different from its continental crust. The oceanic crust is 5 km (3 mi) to 10 km (6 mi) thick2 and is composed primarily of basalt, diabase, and gabbro. The continental crust is typically from 30 km (20 mi) to 50 km (30 mi) thick and is mostly composed of slightly less dense rocks than those of the oceanic crust. Some of these less dense rocks, such as granite, are common in the continental crust but rare to absent in the oceanic crust.

Partly by analogy to what is known about the Moon, Earth is considered to have differentiated from an aggregate of planetesimals into its core, mantle and crust within about 100 million years of the formation of the planet, 4.6 billion years ago. The primordial crust was very thin and was probably recycled by much more vigorous plate tectonics and destroyed by significant asteroid impacts, which were much more common in the early stages of the solar system. Earth has probably always had some form of basaltic crust, but the age of the oldest oceanic crust today is only about 200 million years. In contrast, the bulk of the continental crust is much older. The oldest continental crustal rocks on Earth have ages in the range from about 3.7 to 4.28 billion years 45 and have been found in the Narryer Gneiss Terrane in Western Australia, in the Acasta Gneiss in the Northwest Territories on the Canadian Shield, and on other cratonic regions such as those on the Fennoscandian Shield. Some zircon with age as great as 4.3 billion years has been found in the Narryer Gneiss Terrane.

A theoretical protoplanet named 'Theia' is thought to have collided with the forming Earth, and part of the material ejected into space by the collision accreted to form the Moon. As the Moon formed, the outer part of it is thought to have been molten, a “lunar magma ocean.” Plagioclase feldspar crystallized in large amounts from this magma ocean and floated toward the surface. The cumulate rocks form much of the crust. The upper part of the crust probably averages about 88% plagioclase (near the lower limit of 90% defined for anorthosite): the lower part of the crust may contain a higher percentage of ferromagnesian minerals such as the pyroxenes and olivine, but even that lower part probably averages about 78% plagioclase.9 The underlying mantle is denser and olivine-rich. The thickness of the crust ranges between about 20 and 120 km.

Crust on the far side of the Moon averages about 12 km thicker than that on the near side. Estimates of average thickness fall in the range from about 50 to 60 km.

Most of this plagioclase-rich crust formed shortly after formation of the moon, between about 4.5 and 4.3 billion years ago. Perhaps 10% or less of the crust consists of igneous rock added after the formation of the initial plagioclase-rich material. The best-characterized and most voluminous of these later additions are the mare basalts formed between about 3.9 and 3.2 billion years ago. Minor volcanism continued after 3.2 billion years, perhaps as recently as 1 billion years ago. There is no evidence of plate tectonics.

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