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The ESO 3.6 m Telescope is an optical reflecting telescope run by the European Southern Observatory at La Silla Observatory, Chile since 1977, with a clear aperture of about 3.6 metres (140 in) and 8.6 m 2 (93 sq ft) area.
3.74 m (12 ft 3 in) Gradignan: June 4, 1905 [5] 2 3.78 m (12 ft 4 + 3 ⁄ 4 in) Leroy Samse United States: Chicago: June 2, 1906 [5] 1 3.79 m (12 ft 5 in) Walter Dray: New Haven: May 18, 1907 [5] 1 3.82 m (12 ft 6 + 1 ⁄ 4 in) Philadelphia: April 25, 1908 [5] 2 3.855 m (12 ft 7 + 3 ⁄ 4 in) Alfred Gilbert: June 6, 1908 [5] 1 3.86 m (12 ft 7 ...
Holden has built its own 3.2 L (3,195 cc) version of the High Feature engine in Australia produced between 2005 and 2010 with a bore and stroke of 89 mm × 85.6 mm (3.50 in × 3.37 in). Branded with the Alloytec name like the 3.6L version, this version produces 227 hp (169 kW; 230 PS) at 6600 rpm and 297 N⋅m (219 lb⋅ft) at 3200 rpm.
The 3.6m Devasthal (Hindi: देवस्थल) Optical Telescope is a clear-aperture Ritchey–Chrétien telescope built by Aryabhatta Research Institute of Observational Sciences (ARIES) and is located at the Devasthal Observatory site near Nainital, Kumaon, India. [1] ARIES operates another 1.3m telescope at the same location.
The following is a list of the longest private passenger vehicles of any global marque sold to individuals. The list includes light trucks as many SUV and other light trucks rank among the world's longest passenger vehicles.
By default, the output value is rounded to adjust its precision to match that of the input. An input such as 1234 is interpreted as 1234 ± 0.5, while 1200 is interpreted as 1200 ± 50, and the output value is displayed accordingly, taking into account the scale factor used in the conversion.
Drone video shows the town of Hamburg, N.Y. covered in snow on Friday morning after a lake-effect snow band dumped 33 inches in a 24-hour period. AccuWeather 4 hours ago
The HARPS can attain a precision of 0.97 m/s (3.5 km/h), [2] making it one of only two instruments worldwide with such accuracy. [citation needed] This is due to a design in which the target star and a reference spectrum from a thorium lamp are observed simultaneously using two identical optic fibre feeds, and to careful attention to mechanical stability: the instrument sits in a vacuum vessel ...