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  2. Magnetic field of Mars - Wikipedia

    en.wikipedia.org/wiki/Magnetic_field_of_Mars

    The magnetic field of Mars is the magnetic field generated from Mars's interior. Today, Mars does not have a global magnetic field. However, Mars did power an early dynamo that produced a strong magnetic field 4 billion years ago, comparable to Earth's present surface field. After the early dynamo ceased, a weak late dynamo was reactivated (or ...

  3. Magnetopause - Wikipedia

    en.wikipedia.org/wiki/Magnetopause

    If the pressure from particles within the magnetosphere is neglected, it is possible to estimate the distance to the part of the magnetosphere that faces the Sun.The condition governing this position is that the dynamic ram pressure from the solar wind is equal to the magnetic pressure from the Earth's magnetic field: [note 1] (()) where and are the density and velocity of the solar wind, and ...

  4. Spacecraft magnetometer - Wikipedia

    en.wikipedia.org/wiki/Spacecraft_magnetometer

    A low field vector-helium magnetometer was equipped on the Mariner 4 spacecraft to Mars like the Venus probe a year earlier, no magnetic field was detected. [16] Mariner 5 used a similar device For this experiment a low-field helium magnetometer was used to obtain triaxial measurements of interplanetary and Venusian magnetic fields.

  5. Crustal magnetism - Wikipedia

    en.wikipedia.org/wiki/Crustal_magnetism

    Crustal magnetism map of Mars. Crustal magnetism is the magnetic field of the crust of a planetary body. [1] [2] The crustal magnetism of Earth has been studied; in particular, various magnetic crustal anomalies have been studied. [1]

  6. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    Mars also has a complicated ionosphere that interacts with the solar wind particles, extreme UV radiation and X-rays from Sun, and the magnetic field of its crust. [143] [144] The exosphere of Mars starts at about 230 km and gradually merges with interplanetary space. [2] The solar wind accelerates ions from Mars' upper atmosphere into space

  7. Eridania quadrangle - Wikipedia

    en.wikipedia.org/wiki/Eridania_quadrangle

    At about 3.93 billion years ago Mars became a one plate planet with a superplume under Tharsis. [42] [43] [44] When molten rock containing magnetic material, such as hematite (Fe 2 O 3), cools and solidifies in the presence of a magnetic field, it becomes magnetized and takes on the polarity of the background field. This magnetism is lost only ...

  8. Terra Sirenum - Wikipedia

    en.wikipedia.org/wiki/Terra_Sirenum

    Researchers believe these magnetic stripes on Mars are evidence for a short, early period of plate tectonic activity. When the rocks became solid they retained the magnetism that existed at the time. A magnetic field of a planet is believed to be caused by fluid motions under the surface.

  9. Phaethontis quadrangle - Wikipedia

    en.wikipedia.org/wiki/Phaethontis_quadrangle

    When the rocks became solid they retained the magnetism that existed at the time. A magnetic field of a planet is believed to be caused by fluid motions under the surface. [54] [55] [56] However, there are some differences, between the magnetic stripes on Earth and those on Mars. The Martian stripes are wider, much more strongly magnetized, and ...

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