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  2. Gravity science (Juno) - Wikipedia

    en.wikipedia.org/wiki/Gravity_Science_(Juno)

    Jupiter shown in the image 'Jupiter Marble' as recorded by Juno The Gravity Science experiment and instrument set aboard the Juno Jupiter orbiter is designed to monitor Jupiter 's gravity. [ 1 ] [ 2 ] [ 3 ] It maps Jupiter's gravitational field , which will allow the interior of Jupiter to be better understood. [ 3 ]

  3. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    ^ Surface gravity derived from the mass m, the gravitational constant G and the radius r: Gm/r 2. ^ Escape velocity derived from the mass m, the gravitational constant G and the radius r: √ (2Gm)/r. ^ Orbital speed is calculated using the mean orbital radius and the orbital period, assuming a circular orbit. ^ Assuming a density of 2.0

  4. Gravity map - Wikipedia

    en.wikipedia.org/wiki/Gravity_map

    Surface gravity mapping is often used to map out gravity anomalies such as a Bouguer anomaly or isostatic gravity anomalies. [1] Derivative gravity maps are an extension of standard gravity maps, involving mathematical analysis of the local gravitational field strength, to present data in analogous formats to a geologic map. [1]

  5. Juno (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Juno_(spacecraft)

    Precisely map Jupiter's gravitational field to assess the distribution of mass in Jupiter's interior, including properties of its structure and dynamics. Precisely map Jupiter's magnetic field to assess the origin and structure of the field, and the depth at which the planet's magnetic field is created.

  6. Geopotential spherical harmonic model - Wikipedia

    en.wikipedia.org/wiki/Geopotential_spherical...

    However, a spherical harmonics series expansion captures the actual field with increasing fidelity. If Earth's shape were perfectly known together with the exact mass density ρ = ρ(x, y, z), it could be integrated numerically (when combined with a reciprocal distance kernel) to find an accurate model for Earth's gravitational field. However ...

  7. Galilean moons - Wikipedia

    en.wikipedia.org/wiki/Galilean_moons

    The current model is that the moons experience tidal heating as a result of the gravitational field of Jupiter in inverse proportion to the square of their distance from the giant planet. In all but Callisto this will have melted the interior ice, allowing rock and iron to sink to the interior and water to cover the surface.

  8. GRACE and GRACE-FO - Wikipedia

    en.wikipedia.org/wiki/GRACE_and_GRACE-FO

    High-resolution static gravity fields estimated from GRACE data have helped improve the understanding of global ocean circulation. The hills and valleys in the ocean's surface (ocean surface topography) are due to currents and variations in Earth's gravity field. GRACE enables separation of those two effects to better measure ocean currents and ...

  9. Exploration of Io - Wikipedia

    en.wikipedia.org/wiki/Exploration_of_Io

    Global image of Jupiter's moon Io acquired by Juno's JunoCam camera on 30 December 2023. The Juno spacecraft was launched in 2011 and entered orbit around Jupiter on July 5, 2016. Juno ' s mission is primarily focused on improving our understanding of Jupiter's interior, magnetic field, aurorae, and polar atmosphere. [88]