PIA09249: Jupiter's Rings

Jupiter’s Rings


 Click here for annotated version of Jupiter's Rings
Annotated Version

The New Horizons Long Range Reconnaissance Imager (LORRI) snapped this photo of Jupiter's ring system on February 24, 2007, from a distance of 7.1 million kilometers (4.4 million miles).

This processed image shows a narrow ring, about 1,000 kilometers (600 miles) wide, with a fainter sheet of material inside it. The faint glow extending in from the ring is likely caused by fine dust that diffuses in toward Jupiter. This is the outer tip of the "halo," a cloud of dust that extends down to Jupiter's cloud tops. The dust will glow much brighter in pictures taken after New Horizons passes to the far side of Jupiter and looks back at the rings, which will then be sunlit from behind.

Jupiter's ring system was discovered in 1979, when astronomers spied it in a single image taken by the Voyager 1 spacecraft. Months later, Voyager 2 carried out more extensive imaging of the system. It has since been examined by NASA's Galileo and Cassini spacecraft, as well as by the Hubble Space Telescope and large ground-based observatories.

Cataloging Keywords:

Name Value Additional Values
Target Jupiter Rings Halo, Jupiter, Sun
System Jupiter
Target Type Ring Planet, Sun
Mission New Horizons Cassini-Huygens, Galileo, Hubble Space Telescope (HST), Voyager
Instrument Host New Horizons Cassini Orbiter, Galileo Orbiter, Hubble Space Telescope (HST), Voyager 1, Voyager 2
Host Type Orbiter Flyby Spacecraft, Orbiting Telescope, Probe
Instrument Long Range Reconnaissance Imager (LORRI)
Extra Keywords Dust, Grayscale, Visual
Acquisition Date
Release Date 2007-04-02
Date in Caption 2007-02-24
Image Credit NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
Source photojournal.jpl.nasa.gov/catalog/PIA09249
Identifier PIA09249