2017 Cassini flyby allows first accurate estimate of weight and age of Saturn’s rings — ScienceDaily

One of many final acts of NASA’s Cassini spacecraft earlier than its dying plunge into Saturn’s hydrogen and helium ambiance was to coast between the planet and its rings and allow them to tug it round, basically appearing as a gravity probe.

Exact measurements of Cassini’s closing trajectory have now allowed scientists to make the primary correct estimate of the quantity of fabric within the planet’s rings, weighing them primarily based on the energy of their gravitational pull.

That estimate — about 40 p.c of the mass of Saturn’s moon Mimas, which itself is 2,000 occasions smaller than Earth’s moon — tells them that the rings are comparatively latest, having originated lower than 100 million years in the past and maybe as lately as 10 million years in the past.

Their younger age places to relaxation a long-running argument amongst planetary scientists. Some thought that the rings fashioned together with the planet four.5 billion years in the past from icy particles remaining in orbit after the formation of the photo voltaic system. Others thought the rings had been very younger and that Saturn had, sooner or later, captured an object from the Kuiper belt or a comet and regularly diminished it to orbiting rubble.

The brand new mass estimate is predicated on a measurement of how a lot the flight path of Cassini was deflected by the gravity of the rings when the spacecraft flew between the planet and the rings on its closing set of orbits in September 2017. Initially, nonetheless, the deflection didn’t match predictions primarily based on fashions of the planet and rings. Solely when the workforce accounted for very deep flowing winds in ambiance on Saturn — one thing unattainable to look at from area — did the measurements make sense, permitting them to calculate the mass of the rings.

“The primary time I regarded on the information I did not consider it, as a result of I trusted our fashions and it took some time to sink in that there was some impact that modified the gravity area that we had not thought-about,” stated Burkhard Militzer, a professor of earth and planetary science on the College of California, Berkeley, who fashions planetary interiors. “That turned out to be huge flows within the ambiance at the least 9,000 kilometers deep across the equatorial area. We thought preliminarily that these clouds had been like clouds on Earth, that are confined to a skinny layer and comprise virtually no mass. However on Saturn they’re actually huge.”

In addition they calculated that the floor clouds at Saturn’s equator rotate four p.c quicker than the layer 9,000 kilometers (about 6,000 miles) deep. That deeper layer takes 9 minutes longer to rotate than do the cloud tops on the equator, which go across the planet as soon as each 10 hours, 33 minutes.

“The invention of deeply rotating layers is a stunning revelation in regards to the inside construction of the planet,” stated Cassini venture scientist Linda Spilker of NASA’s Jet Propulsion Laboratory in Pasadena, California. “The query is what causes the extra quickly rotating a part of the ambiance to go so deep and what does that inform us about Saturn’s inside.”

Militzer additionally was in a position to calculate that the rocky core of the planet should be between 15 and 18 occasions the mass of Earth, which has similarities to earlier estimates.

The workforce, led by Luciano Iess on the Sapienza College of Rome, Italy, reported their outcomes right now within the journal Science.

Did rings come from icy comet?

Earlier estimates of the mass of Saturn’s rings — between one-half and one-third the mass of Mimas — got here from finding out the density waves that journey across the rocky, icy rings. These waves are attributable to the planet’s 62 satellites, together with Mimas, which creates the so-called Cassini division between the 2 largest rings, A and B. Mimas is clean and spherical, 246 kilometers in diameter. It has a big effect crater that makes it resemble the Demise Star from the Star Wars films.

“Individuals did not belief the wave measurements as a result of there is perhaps particles within the rings which might be huge however usually are not taking part within the waves,” Militzer stated. “We at all times suspected there was some hidden mass that we couldn’t see within the waves.”

Fortunately, as Cassini approached the top of its life, NASA programmed it to carry out 22 dives between the planet and the rings to probe Saturn’s gravity area. Earth-based radio telescopes measured the spacecraft’s velocity to inside a fraction of a millimeter per second.

The brand new ring mass worth is within the vary of earlier estimates and permits the researchers to find out their age.

These age calculations, led by Philip Nicholson of Cornell College and Iess, constructed on a connection that scientists had beforehand made between the mass of the rings and their age. Decrease mass factors to a youthful age, as a result of the rings are initially made from ice and are vivid however over time turn into contaminated and darkened by interplanetary particles.

“These measurements had been solely doable as a result of Cassini flew so near the floor in its closing hours,” Militzer stated. “It was a basic, spectacular strategy to finish the mission.”


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