Artist's Concept of Aurorae and Ganymede

Artist's Concept of Aurorae and Ganymede

This is an artist's concept of the moon Ganymede as it orbits the giant planet Jupiter. NASA's Hubble Space Telescope observed aurorae on the moon that are controlled by Ganymede's magnetic fields. Two auroral ovals can be seen over northern and southern mid-latitudes. Hubble measured slight shifts in the auroral belts due to the influence of Jupiter's own immense magnetic field. This activity allows for a probe of the moon's interior. The presence of a saline ocean under the moon's icy crust reduces the shifting of the ovals as measured by Hubble. As on Earth, Ganymede's aurorae are produced by energetic charged particles causing gases to fluoresce.

Credits

Illustration Credit: NASA, ESA, and G. Bacon (STScI);
Science Credit: NASA, ESA, and J. Saur (University of Cologne, Germany)

About The Data
Data Description The image was created from Hubble data from the following proposal: PI: J. Saur (University of Cologne, Germany), P. Feldman and D. Strobel (JHU), K. Retherford (SwRI), M. McGrath (NASA/MSFC), and S. Duling (University of Cologne, Germany). The science team includes: J. Saur and S. Duling (University of Cologne, Germany), L. Roth (SwRI/University of Cologne, Germany), D. Strobel and P. Feldman (JHU), U. Christensen (Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany), K. Retherford (SwRI), M. McGrath (NASA/MSFC), F. Musacchio, A. Wennmacher, and F. Neubauer (University of Cologne, Germany), and S. Simon (Georgia Institute of Technology, Atlanta), and O. Hartkorn (University of Cologne, Germany).
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  • Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.

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