NASA Solarsystem Collection

Jupiter's Rings

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.

Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

02.24.2007

Solar System Exploration

SSE

Space

NASA

National Aeronautics and Space Administration

JPL

Jet Propulsion Laboratory

Planets

Voyager

Voyager 2

Galileo

Jupiter

Cassini

Imager

Voyager 1

New Horizons

Long Range Reconnaissance Imager

LORRI

Hubble Space Telescope (HST)

Jet Propulsion Laboratory

Jupiter

Jet Propulsion Laboratory (JPL)

1979

February 24, 2007

02-24-2007

1979

2007

SPD-SLRSY-5063

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