NASA's Hubble Space Telescope observed a pair of auroral belts encircling the Jovian moon Ganymede. The belts were observed in ultraviolet light by the Space Telescope Imaging Spectrograph and are colored blue in this illustration. They are overlaid on a visible-light image of Ganymede taken by NASA's Galileo orbiter. The locations of the glowing aurorae are determined by the moon's magnetic field, and therefore provide a probe of the moon's interior, where the magnetic field is generated. The amount of rocking of the magnetic field, caused by its interaction with Jupiter's own immense magnetosphere, provides evidence that the moon has a subsurface ocean of saline water.
Credits
NASA, ESA, and J. Saur (University of Cologne, Germany);Ganymede Globe Credit: NASA, JPL, and the Galileo Project
| About The Object | |
|---|---|
| Object Name | Ganymede |
| Object Description | Jovian Moon: Jupiter has a diameter of roughly 88,789 miles (142,984 km) at the equator. Ganymede has a diameter of 3,270 miles (5,262 km). |
| Distance | The semi-major axis of Jupiter's orbit about the Sun is 5.2 astronomical units (483 million miles or 778 million km). Ganymede orbits at a mean distance of 665,000 miles (1 million km) from Jupiter. |
| 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). |
| Instrument | HST>STIS |
| About The Image | |
| Compass Image |  |
| 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 |
|
| 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. |
