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  2. Wikipedia:Reference desk/Archives/Science/2024 October 19 ...

    en.wikipedia.org/wiki/Wikipedia:Reference_desk/...

    1.1 Falling into Jupiter. 4 comments. 1.2 Since neutrinos (and dark matter) don't interact with light, so what should happen when light comes across them? 19 comments.

  3. Comet Shoemaker–Levy 9 - Wikipedia

    en.wikipedia.org/wiki/Comet_Shoemaker–Levy_9

    The first impact occurred at 20:13 UTC on July 16, 1994, when fragment A of the [comet's] nucleus slammed into Jupiter's southern hemisphere at about 60 km/s (35 mi/s). Instruments on Galileo detected a fireball that reached a peak temperature of about 24,000 K (23,700 °C; 42,700 °F), compared to the typical Jovian cloud-top temperature of ...

  4. Stability of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Stability_of_the_Solar_System

    At one point, the two may fall into sync, at which time Jupiter's constant gravitational tugs could accumulate and pull Mercury off course, with 1–2% probability, 3–4 billion years into the future. This could eject it from the Solar System altogether [1] or send it on a collision course with Venus, the Sun, or Earth. [10]

  5. Impact events on Jupiter - Wikipedia

    en.wikipedia.org/wiki/Impact_events_on_Jupiter

    The first impact occurred at 20:13 UTC on July 16, 1994, when fragment A of the [comet's] nucleus slammed into Jupiter's southern hemisphere at about 60 km/s (35 mi/s). Instruments on Galileo detected a fireball that reached a peak temperature of about 24,000 K (23,700 °C; 42,700 °F), compared to the typical Jovian cloud-top temperature of ...

  6. Europa Clipper - Wikipedia

    en.wikipedia.org/wiki/Europa_Clipper

    The probe will then arc (reach aphelion) beyond Jupiter's orbit on October 4, 2029 [121] before slowly falling into Jupiter's gravity well and executing its orbital insertion burn in April 2030. [122] As of 2014, the trajectory in the Jupiter system is planned as follows.

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  8. Equations for a falling body - Wikipedia

    en.wikipedia.org/wiki/Equations_for_a_falling_body

    For astronomical bodies other than Earth, and for short distances of fall at other than "ground" level, g in the above equations may be replaced by (+) where G is the gravitational constant, M is the mass of the astronomical body, m is the mass of the falling body, and r is the radius from the falling object to the center of the astronomical body.

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