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Quadruple Saturn Moon Transit Snapped by Hubble

The headshot image of NASA Hubble Mission Team

NASA Hubble Mission Team

Goddard Space Flight Center

Mar 17, 2009
Article
Quadruple Saturn Moon Transit Snapped By Hubble
On February 24, 2009, the Hubble Space Telescope took a photo of four moons of Saturn passing in front of their parent planet. In this view, the giant orange moon Titan casts a large shadow onto Saturn's north polar hood. Below Titan, near the ring plane and to the left is the...

Saturn's comparatively paper-thin rings are tilted edge on to Earth every 15 years. Because the orbits of Saturn's major satellites are in the ring plane, too, this alignment gives astronomers a rare opportunity to capture a truly spectacular parade of celestial bodies crossing the face of Saturn. Leading the parade is Saturn's giant moon Titan - larger than the planet Mercury. The frigid moon's thick nitrogen atmosphere is tinted orange with the smoggy byproducts of sunlight interacting with methane and nitrogen. Several of the much smaller icy moons that are closer in to the planet line up along the upper edge of the rings. Hubble's exquisite sharpness also reveals Saturn's banded cloud structure.

Related Images & Videos

Quadruple Saturn Moon Transit Snapped By Hubble

Quadruple Saturn Moon Transit Snapped By Hubble

On February 24, 2009, the Hubble Space Telescope took a photo of four moons of Saturn passing in front of their parent planet. In this view, the giant orange moon Titan casts a large shadow onto Saturn's north polar hood. Below Titan, near the ring plane and to the left is the...

HST Image of Saturn Moon Transits

HST Image of Saturn Moon Transits

This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's...

HST Image of Saturn: February 24, 2009 12:12 UT

HST Image of Saturn: February 24, 2009 12:12 UT

HST Image of Saturn: February 24, 2009 14:25 UT

HST Image of Saturn: February 24, 2009 14:25 UT

HST Image of Saturn: February 24, 2009 15:27 UT

HST Image of Saturn: February 24, 2009 15:27 UT

Closeup of Quadruple Saturn Moon Transit

Closeup of Quadruple Saturn Moon Transit

This close-up view of Saturn's disk captures the transit of several moons across the face of the gas giant planet. The giant orange moon Titan – larger than the planet Mercury – can be seen at upper right. The white icy moons that are much closer to Saturn, hence much closer to...

Compass and Scale Image of Saturn

Compass and Scale Image of Saturn

Annotated Image of Saturn's Rings and Moons

Annotated Image of Saturn's Rings and Moons

Photo Sequence of Saturn: February 24, 2009

Photo Sequence of Saturn: February 24, 2009

Saturn's Rings Viewed from Earth

Saturn's Rings Viewed from Earth

As Saturn travels around its orbit, Hubble sees a different view of the tilted rings from a position near Earth. The rings nearly disappear twice during Saturn's approximately 30-year orbit, because we see them edge on and they are extremely thin relative to their diameter.

Saturn Quadruple Transit Science Visualization

Saturn Quadruple Transit Science Visualization

This Hubble movie shows four of Saturn's moons moving across the face of their parent planet on February 24, 2009. Icy moons Enceladus and Dione are on the far left, while the large orange moon Titan and icy Mimas are on the right.

Saturn Quadruple Transit Science Visualization (Narrated)

Saturn Quadruple Transit Science Visualization (Narrated)

This Hubble movie shows four of Saturn's moons moving across the face of their parent planet on February 24, 2009. Icy moons Enceladus and Dione are on the far left, while the large orange moon Titan and icy Mimas are on the right.

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Last Updated
Mar 20, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Credits

NASA,ESA, and theHubble Heritage Team (STScI/AURA);
Acknowledgment: M.H. Wong (STScI/UC Berkeley) and C. Go (Philippines)

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