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  2. Orbital decay - Wikipedia

    en.wikipedia.org/wiki/Orbital_decay

    Orbital decay is a gradual decrease of the distance between two orbiting bodies at their closest approach (the periapsis) over many orbital periods. These orbiting bodies can be a planet and its satellite , a star and any object orbiting it, or components of any binary system .

  3. Template:WikiProject Google/doc - Wikipedia

    en.wikipedia.org/.../Template:WikiProject_Google/doc

    This is a documentation subpage for Template:WikiProject Google. It may contain usage information, categories and other content that is not part of the original template page. Usage

  4. Template:Google books - Wikipedia

    en.wikipedia.org/wiki/Template:Google_books

    Citer, hosted on the Wikimedia Toolforge, can be used to convert Google Books URLs—as well as many other forms of universal identifiers (DOI, ISBN, PMID,etc.)—into full {} transclusions. The above documentation is transcluded from Template:Google books/doc .

  5. Outer space - Wikipedia

    en.wikipedia.org/wiki/Outer_space

    The energy required to reach Earth orbital velocity at an altitude of 600 km (370 mi) is about 36 MJ/kg, which is six times the energy needed merely to climb to the corresponding altitude. [93] The escape velocity required to pull free of Earth's gravitational field altogether and move into interplanetary space is about 11,200 m/s (40,300 km/h ...

  6. UAH satellite temperature dataset - Wikipedia

    en.wikipedia.org/wiki/UAH_satellite_temperature...

    The sensors deteriorate over time, and corrections are necessary for satellite drift and orbital decay. Particularly large differences between reconstructed temperature series occur at the few times when there is little temporal overlap between successive satellites, making intercalibration difficult.

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    www.aol.com/games/play/arcade-bomb/orbital-decay

    Discover the best free online games at AOL.com - Play board, card, casino, puzzle and many more online games while chatting with others in real-time.

  8. PSR J0737−3039 - Wikipedia

    en.wikipedia.org/wiki/PSR_J0737%E2%88%923039

    The orbital decay and the speedup of the orbital period was tested to follow the quadrupole formula with a great precision of 0.013% mainly because of the unique characteristics of the system which has two pulsars, is nearby and possesses an inclination close to 90°. [7] [8] [9]

  9. Space debris - Wikipedia

    en.wikipedia.org/wiki/Space_debris

    At higher altitudes, where air drag is less significant, orbital decay takes longer. Slight atmospheric drag , lunar perturbations , Earth's gravity perturbations, solar wind , and solar radiation pressure can gradually bring debris down to lower altitudes (where it decays), but at very high altitudes this may take centuries. [ 57 ]