Cassini spots tiny moon, begins to tilt orbit

Cassini spots tiny moon, begins to tilt orbit
This raw, unprocessed image was taken by NASA's Cassini spacecraft on May 20, 2012. The camera was pointing toward Methone. Credit: NASA/JPL-Caltech/SSI

(Phys.org) -- NASA's Cassini spacecraft made its closest approach to Saturn's tiny moon Methone as part of a trajectory that will take it on a close flyby of another of Saturn's moons, Titan. The Titan flyby will put the spacecraft in an orbit around Saturn that is inclined, or tilted, relative to the plane of the planet's equator. The flyby of Methone took place on May 20 at a distance of about 1,200 miles (1,900 kilometers). It was Cassini's closest flyby of the 2-mile-wide (3-kilometer-wide) moon. The best previous Cassini images were taken on June 8, 2005, at a distance of about 140,000 miles (225,000 kilometers), and they barely resolved this object.

Also on May 20, Cassini obtained images of Tethys, a larger Saturnian moon that is 660 miles (1,062 kilometers) across. The spacecraft flew by Tethys at a distance of about 34,000 miles (54,000 kilometers).

Cassini's encounter with Titan, Saturn's largest moon, on May 22, is the first of a sequence of flybys that will put the spacecraft into an inclined orbit. At closest approach, Cassini will fly within about 593 miles (955 kilometers) of the surface of the hazy Titan. The flyby will angle Cassini's path around Saturn by about 16 degrees out of the equatorial plane, which is the same plane in which Saturn's rings and most of its moons reside.

Cassini spots tiny moon, begins to tilt orbit
This raw, unprocessed image was taken by NASA's Cassini spacecraft on May 20, 2012. The camera was pointing toward Tethys at approximately 81,580 miles (131,290 kilometers) away. Credit: NASA/JPL/Space Science Institute

Cassini's onboard don't have the capability to place the spacecraft into orbits so inclined. But mission designers have planned trajectories that take advantage of the exerted by Titan to boost Cassini into inclined orbits. Over the next few months, Cassini will use several flybys of Titan to change the angle of its inclination, building one on top of the other until Cassini is orbiting Saturn at around 62 degrees relative to the equatorial plane in 2013. Cassini hasn't flown in orbits this inclined since 2008, when it orbited at an angle of 74 degrees.

This set of inclined orbits is expected to provide spectacular views of the rings and poles of Saturn. Further studies of Saturn's other moons will have to wait until around 2015, when Cassini returns to an equatorial .

"Getting Cassini into these inclined orbits is going to require the same level of navigation accuracy that the team has delivered in the past, because each of these Titan flybys has to stay right on the money," said Robert Mitchell, Cassini program manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "However, with nearly eight years of experience to rely on, there's no doubt about their ability to pull this off." 

Cassini discovered Methone and two other small moons, Pallene and Anthe, between the orbits of Mimas and Enceladus between 2004 and 2007. The three tiny moons, called the Alkyonides group, are embedded in Saturn's E ring, and their surfaces are sprayed by ice particles originating from the jets of water ice, water vapor and organic compounds emanating from the south polar area of Enceladus.


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Cassini, Saturn Moon Photographer

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rah
May 23, 2012
I don't know why they haven't made a movie about these spacecraft engineers. I know it's a bit on the geeky side, but it would be hugely popular if made right. No exaggerations would be necessary, just a plain language explanation of what they have been doing everyday for many years.

yyz
May 23, 2012
"The three tiny moons, called the Alkyonides group, are embedded in Saturn's E ring, and their surfaces are sprayed by ice particles originating from the jets of water ice, water vapor and organic compounds emanating from the south polar area of Enceladus."

This process is probably responsible for the smooth surface of Methone in this image. No large craters are visible on this tiny 3km-wide moon. Few craters are visible at all. If not for resurfacing with material from Enceladus (and the Methone Ring Arc the moon orbits within), the surface would look as pockmarked and ragged as Tethys.

Jason Major at Universe Today has created a color version of this Cassini image of Methone: http://www.univer...hone.jpg

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