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  2. Pulsar - Wikipedia

    en.wikipedia.org/wiki/Pulsar

    X-ray pulsar-based navigation and timing (XNAV) or simply pulsar navigation is a navigation technique whereby the periodic X-ray signals emitted from pulsars are used to determine the location of a vehicle, such as a spacecraft in deep space. A vehicle using XNAV would compare received X-ray signals with a database of known pulsar frequencies ...

  3. Studebaker US6 2½-ton 6×6 truck - Wikipedia

    en.wikipedia.org/wiki/Studebaker_US6_2½-ton_6×6...

    The Studebaker US6 was a series of 2 + 1 ⁄ 2-ton 6×6 and 5-ton 6×4 trucks manufactured by the Studebaker Corporation and REO Motor Car Company during World War II.The basic cargo version was designed to transport a 2 + 1 ⁄ 2-short-ton (5,000 lb; 2,300 kg) cargo load over any type of terrain in any weather.

  4. Alvis Stalwart - Wikipedia

    en.wikipedia.org/wiki/Alvis_Stalwart

    The Stalwart, formally classified by the British Army as Truck, High Mobility Load Carrier (HMLC), 5 Ton, 6 x 6, Alvis Stalwart and informally known by servicemen as the Stolly, and by former RCT as the Stally, [1] is a highly mobile amphibious military truck.

  5. List of Subaru engines - Wikipedia

    en.wikipedia.org/wiki/List_of_Subaru_engines

    Subaru EK engine summary Cooling Stroke Name Displacement Bore × Stroke Output Compression Ratio Applications Air Two: EK31 356 cm 3 (21.7 cu in): 61.5 mm × 60.0 mm (2.42 in × 2.36 in)

  6. PSR B1937+21 - Wikipedia

    en.wikipedia.org/wiki/PSR_B1937+21

    PSR B1937+21 is a pulsar located in the constellation Vulpecula a few degrees in the sky away from the first discovered pulsar, PSR B1919+21. [1] The name PSR B1937+21 is derived from the word "pulsar" and the declination and right ascension at which it is located, with the "B" indicating that the coordinates are for the 1950.0 epoch.

  7. Crab Pulsar - Wikipedia

    en.wikipedia.org/wiki/Crab_Pulsar

    The Crab Pulsar was the first pulsar for which the spin-down limit was broken using several months of data of the LIGO observatory. Most pulsars do not rotate at constant rotation frequency, but can be observed to slow down at a very slow rate (3.7 × 10 −10 Hz/s in case of the Crab). This spin-down can be explained as a loss of rotation ...

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