LITTLE BIG TRACTOR Little only in size. Tigre 4000 is the isodiametric Antonio Carraro tractor which most perfectly unites compactness and technology. A factotum designed for little agricultural lots, gardens, greenhouses, as well as parks, sport fields, municiapalities.
The 4-wheel drive and the ACTIO™ chassis contribute to comfort and safety: traction and grip are always constant. Tigre is equipped with synchronized PTO. The lifting system offers a 3 point-hitch and adjustable vertical tie-rods, with a lifting capacity up to 850 Kg. Dashboard - The elegant, technological and backlit analogue/ digital dashboard, a multi-purpose on-board instrument featuring a modern design, is integrated into the dashboard panel and protected by an anti-glare dome. The instrument constantly controls of all functions with highvisibility LED signalling even in direct sunlight.
Seat - Fitted with safety belts and height and comfort adjustments, it is also available with pneumatic suspension on request. Steering - The sensitive and precise hydrodrive power-assisted steering assures excellent manoeuvrability and maximum comfort. The Load Sensing (T4400F) system guarantees safety and efficiency in all conditions and optimises hydraulic flow at all times. The minimum steering radius reduces the number of manoeuvres and, consequently, work time. Download buku dale carnegie bahasa indonesia pdf. Control levers - All the controls are ergonomically positioned in a logical sequence. Power lift - Powerful three-point hitch with two external cylinders, elevated lifting capacity, cat. 1 - 1N, adjustable tie-rods.
Brakes - Drum service brakes (floating on the T4400F) acting on the rear wheels. Independent (opt. On the T4000) and simultaneous braking. Roll-bars - Front pull-down, featuring a low-profile design and integrated into the tractor chassis to allow manoeuvring in the tightest of spaces. Rear fixed, integrated into the multi-purpose number plate holder and distributor support panel. Lighting assemblies - The new front headlights feature halogen bulbs giving off a brilliant, white, wide and deep beam.
This article is about Antonio Carraro. For Carraro Agritalia, see.
Antonio Carraro Founded 1960 Antonio Carraro Headquarters Veneto, Website Antonio Carraro was founded in 1960 when Antonio set up his own company in Veneto, apart from his brothers who were part of Agritalia, formerly Giovanni Carraro. Antonio decided specialized in and machinery.
In 1964, the first Antonio Carraro was developed. In 2004, Antonio Carraro began building tractors for. In 2006, an agreement was signed that strengthened the ties to Carraro Agritalia, and Antonio Carraro began to distribute Carraro (Agritalia) tractors under the Antonio Carraro brand.
Contents Models Antonio Carraro Tractor Models Model Year(s) Produced Engine Type Misc Notes Photo 1982 62 3 cil 3995 cc 38 hp (28 kW) 38 hp (28 kW) 47 hp (35 kW) 48 hp (36 kW) 63 hp (47 kW) 60 hp (45 kW) 64 hp (48 kW) 64 hp (48 kW) 64 hp (48 kW) 64 hp (48 kW) 69 hp (51 kW) 70 hp (52 kW) 70 hp (52 kW) 70 hp (52 kW) 70 hp (52 kW) 70 hp (52 kW) 70 hp (52 kW) 75 hp (56 kW) 68 hp (51 kW) 75 hp (56 kW) 75 hp (56 kW) 75 hp (56 kW) 75 hp (56 kW) 75 hp (56 kW) 87 hp (65 kW) 83 hp (62 kW) 83 hp (62 kW) 83 hp (62 kW) 83 hp (62 kW) 81 hp (60 kW) 81 hp (60 kW) 83 hp (62 kW) 83 hp (62 kW).
Earth's crust close X home chemical composition chemical compound crystal earth's crust inorganic compound mineralogy mineraloid rock silicate minerals silicon 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.
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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.
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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.