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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. 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 ...

  6. Hulse–Taylor pulsar - Wikipedia

    en.wikipedia.org/wiki/Hulse–Taylor_pulsar

    Evidence of orbital decay in PSR B1913+16. [7] The data points indicate the observed change in the time of periastron with date, relative to a system not undergoing decay. The parabola illustrates the theoretically expected change according to general relativity .

  7. WASP-4b - Wikipedia

    en.wikipedia.org/wiki/WASP-4b

    The planet's orbital period appears to be decreasing at a rate of 7.33 ± 0.71 milliseconds per year, suggesting that its orbit is decaying, with a decay timescale of 15.77 ± 1.57 million years. The anomalously high rate of orbital decay of WASP-4b is poorly understood as of 2021.

  8. TrES-3b - Wikipedia

    en.wikipedia.org/wiki/TrES-3b

    It has an orbital period of just 31 hours and nearly twice the mass of Jupiter. The planet TrES-3b is named Umbäässa. The name was selected in the NameExoWorlds campaign by Liechtenstein, during the 100th anniversary of the IAU. In the local dialect of southern Liechtenstein, Umbäässa is a small and barely visible ant. [2] [3]

  9. WASP-103 - Wikipedia

    en.wikipedia.org/wiki/WASP-103

    Orbital decay was not detected by 2020. [9] In early 2022, the planet was popularized because of its shape similar to a potato. [10] The planetary atmosphere contains water, and possibly hydrogen cyanide, titanium(II) oxide, or sodium. [11] The planet has an elevated carbon to oxygen molar fraction of 0.9 [3] or 1.35 +0.14