One of the instruments on the spacecraft measured a stream of hydrogen molecules flowing away from the moon over its north pole. Another instrument measured the presence of an Ionosphere, a part of the atmosphere that is filled with ions. If lightweight hydrogen escapes easily from Ganymede’s low gravity, it must be replenished continuously due to an active process at the surface. Terrestrial observations, such as this image of ozone from the Hubble Space Telescope have suggested that Ganymede may have a substantial trapped component of oxygen under the surface. Ozone is an important constituent of the Earth’s atmosphere. Calculations show that the trapped atmospheric component may be as large as the atmosphere of Mars. Ground based telescopes show other components of the atmosphere.
Even though Ganymede and Callisto have thin atmospheres, there does not seem to be a Ganymede or Callisto torus, the way there is at Europa and Io.
One of the instruments on the spacecraft measured a stream of hydrogen molecules flowing away from the moon over its north pole. Another instrument measured the presence of an Ionosphere, a part of the atmosphere that is filled with ions. If molecules are leaving Ganymede all the time, that means they have to be replaced all the time, and that means there must be an active process that is creating the atmosphere. This image from the Hubble Space Telescope shows ozone on Ganymede. Ozone is an important constituent of the Earth’s atmosphere.
Even though Ganymede and Callisto have thin atmospheres, there does not seem to be a Ganymede or Callisto torus, the way there is at Europa and Io.
Page created September 20, 2003 by Jennifer Bergman.
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