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Observaciones ultravioleta de Ganímedes realizadas por el Hubble en 1998

In 1998, Hubble's Space Telescope Imaging Spectrograph (STIS) took these first ultraviolet (UV) images of Ganymede, which revealed a particular pattern in the observed emissions from the moon's atmosphere. The moon displays auroral bands that are somewhat similar to aurora ovals...

Fecha
Jan 1, 2021
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2021-033-01fak3ek6kgra8njwgdsa7kmy7
Por

In 1998, Hubble's Space Telescope Imaging Spectrograph (STIS) took these first ultraviolet (UV) images of Ganymede, which revealed a particular pattern in the observed emissions from the moon's atmosphere. The moon displays auroral bands that are somewhat similar to aurora ovals observed on Earth and other planets with magnetic fields. This was an illustrative evidence for the fact that Ganymede has a permanent magnetic field. The similarities in the ultraviolet observations were explained by the presence of molecular oxygen (O2). The differences were explained at the time by the presence of atomic oxygen (O), which produces a signal that affects one UV color more than the other.

Credits

Science

NASA, ESA, Lorenz Roth (KTH)

Detalles de la imagen

About The Object
Object NameGanymede
Object DescriptionSatellite of Jupiter
DistanceOver 600 million kilometers away from Earth.
About The Data
InstrumentSTIS

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Fuente

La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

Ver en NASA.gov

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