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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. 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.

  4. ZTF J153932.16+502738.8 - Wikipedia

    en.wikipedia.org/wiki/ZTF_J153932.16+502738.8

    The orbital period is decreasing at 2.373 × 10 −11 seconds per second giving a characteristic timescale of 210,000 years. [1] This decay is mostly due to the emission of gravitational waves, however 7% of the decay could be due to tidal losses. [1] The decay is predicted to go for 130,000 years when the orbital period should reach 5 minutes.

  5. Simplified perturbations models - Wikipedia

    en.wikipedia.org/wiki/Simplified_perturbations...

    Simplified Deep Space Perturbations (SDP) models apply to objects with an orbital period greater than 225 minutes, which corresponds to an altitude of 5,877.5 km, assuming a circular orbit. [ 3 ] The SGP4 and SDP4 models were published along with sample code in FORTRAN IV in 1988 with refinements over the original model to handle the larger ...

  6. Capture of Triton - Wikipedia

    en.wikipedia.org/wiki/Capture_of_Triton

    The event would have been "gentle and brief", as Triton is not subject to violent disruption or potentially dangerous post-capture orbital decay. Additionally, the prevalence of binaries among Kuiper belt objects , combined with the outward migration of Neptune early in the Solar System's history, ensures that an encounter between Neptune and a ...

  7. Accretion (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Accretion_(astrophysics)

    The planetesimals are massive enough that mutual gravitational interactions are significant enough to be taken into account when computing their evolution. [5] Growth is aided by orbital decay of smaller bodies due to gas drag, which prevents them from being stranded between orbits of the embryos.

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    mail.aol.com

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  9. Zero-propellant maneuver - Wikipedia

    en.wikipedia.org/wiki/Zero-propellant_maneuver

    Spacecraft experience orbital decay due to drag. To maintain their orbit, thrusters are used to reboost the spacecraft to a higher altitude. Because on board propellant capacity is limited, the spacecraft can only perform a limited number of momentum desaturations or reboosts.