In 40 million years, Mars may have a ring (and one fewer moon)

November 24, 2015 by Karen Kaplan, Los Angeles Times
Phobos, the larger of Mars' moons, imaged from a distance of 6,800 kilometers. The Stickney impact crater dominates one hemisphere of the moon (HiRISE image PSP_007769_9010, taken March 23, 2008. Credit: NASA/JPL/University of Arizona

Nothing lasts forever - especially Phobos, one of the two small moons orbiting Mars. The moonlet is spiraling closer and closer to the Red Planet on its way toward an inevitable collision with its host. But a new study suggests that pieces of Phobos will get a second life as a ring around the rocky planet.

In our solar system, the only planets with rings are the gas giants - Jupiter, Saturn, Uranus and Neptune. The study, published Monday in the journal Nature Geoscience, suggests this wasn't always the case. However, the study authors say this is probably the last time a will have a chance to sport a ring.

A moon - or moonlet - in orbit around a planet has three possible destinies. If it is just the right distance from its host, it will stay in orbit indefinitely. If it's beyond that point of equilibrium, it will slowly drift away. (This is the situation with the moon; as it gradually pulls away from Earth, its orbit is growing by about 1.5 inches per year.) And if a moon starts out on the too-close side, its orbit will keep shrinking until there is no distance left between it and its host planet.

That will be the ultimate fate of Phobos, as astronomers have known for decades. But Benjamin Black and Tushar Mittal, both planetary scientists at the University of California, Berkeley, wanted to get a clearer picture of what this end would look like.

A lot depends on what Phobos is made of. To find out, Black and Mittal compared spectral data from the small moon with data from other rocky objects. The closest match they found was with a class of meteorites known as CM carbonaceous chondrites - especially those that fell on Canada's frozen Tagish Lake in January of 2000.

Such objects aren't especially strong, the study authors wrote. Phobos has the added weakness of having a low density, which suggests it's very porous, they noted.

Phobos also had the misfortune of getting slammed by a large object that left a roughly 6-mile-wide crater, which covers nearly half of the moonlet's diameter. That impact undermined the moon's integrity even further.

To determine the "rock mass strength" of Phobos, Black and Mittal used a model employed by engineers who work on massive underground construction projects on Earth. That model suggests that tidal stresses exerted by Mars will break apart the weakest parts of Phobos in 20 million to 40 million years, when the moonlet is about 3,400 miles away from the planet's surface.

These Phobos fragments will form a ring with a density similar to some of the rings around Saturn. The Martian ring will last for at least 1 million years - and perhaps for as long as 100 million years, according to the study.

Mars could gain a ring in 10-20 million years when its moon Phobos is torn to shreds by Mars gravity. Credit: Tushar Mittal using Celestia 2001-2010, Celestia Development Team.

The rest of Phobos will probably remain intact, until it hits the Martian surface. But it won't be a direct impact; instead, the moonlet's remains will strike at an oblique angle, skipping along the surface like a smooth stone on a calm lake.

This has probably happened before - scientists believe a group of elliptical craters on the Martian surface were caused by a small moon that skidded to its demise. (If this were to happen on Earth, our planet's greater mass would produce a crash as big as the one that wiped out the dinosaurs, the researchers noted as an aside.)

Of course, neither Black nor Mittal will be around in 40 million years to find out if their predictions are correct. But any of three proposed NASA missions - PADME, PANDORA or MERLIN - would provide more data to hone their calculations.

Assuming they are right, one implication is that there used to be more moons in close orbits around their host planets. Moons that were bigger than Phobos would have broken apart to form rings or crashed into their hosts already.

"It is not a coincidence that Phobos is the only surviving inwardly migrating Martian satellite," they wrote. "Phobos thus offers the last possible glimpse" of the events that led to "ring formation early in our solar system's history."

Explore further: Mars' moon Phobos is slowly falling apart

More information: Benjamin A. Black et al. The demise of Phobos and development of a Martian ring system, Nature Geoscience (2015). DOI: 10.1038/ngeo2583

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6 comments

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Shootist
4.7 / 5 (3) Nov 24, 2015
In 40 million years Mars will have a series of new impact basins to rival Utopia and Hellas,
wduckss
1 / 5 (4) Nov 24, 2015
The body in proper orbit does not fall on the planet, star or galaxy center (do not exist astronomical evidence).
Supposedly, the collision of a larger body with the Earth originated is the moon (where's the ring?).
In our system has, a lot of satellites, why it is Phobos exception, only to form a the article?
Enthusiastic Fool
4.3 / 5 (6) Nov 24, 2015
@Shootist
In 40 million years Mars will have a series of new impact basins to rival Utopia and Hellas,

Or if the composition is as fragile as implied Mars might just have a giant strewn field. It sure would be awesome to witness such a spectacle.

If Phobos lands in the Valle Marineris is it a 3-point shot or a dunk? Who gets the points?

@wduckss
The body in proper orbit does not fall on the planet


I believe the article enumerates the possibilities for orbit including decay and escape options. There's several factors that can act on an object to destabilize an orbit. Another moon for example, magnetic drag between the 2 objects, trace friction from the interplanetary medium, or maybe even iterations based on the orbiting object's composition such as an inducing a wobble or thermal dissipation like in the Pioneer Anomaly. I don't think an absolutist point of view is appropriate given our experiences with orbital mechanics.
wduckss
1 / 5 (5) Nov 25, 2015
Enthusiastic Fool "Another moon for example, magnetic drag between the 2 objects, trace friction from the interplanetary medium, or maybe even iterations based on the orbiting object's composition such as an inducing a wobble or thermal dissipation like in the Pioneer Anomaly. I don't think.."


Enumeration and listing more options = ignorance of the orbit of the body. Where is foothold in evidence?
See: The forbidden article: Gravity and anti-gravity http://www.svemir....html#5b
marko
not rated yet Nov 25, 2015
Why can't Phobos be fitted with rocket boosters that will restore its orbit over Mars.

Over 40 million years, there should be lots of time to gradually correct the orbit of the moon.

Perhaps using local materials and solar or nuclear energy, a suitable reaction motor could be built on Phobos.

Alternatively, a powerful laser beam from mars could selectively ablate Phobos, and boost its orbit that way.

Destroying a moon to make a planetary ring seems wasteful, especially if humans have already colonised Mars.
mreda14
1 / 5 (1) Nov 29, 2015
Speculations and waste of the American tax payer money.

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