My Assistant
Small Body Grooves, Theories for the formation of grooves on Lutetia and Phobos |
Jul 10 2010, 09:15 PM
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#1
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Solar System Cartographer ![]() ![]() ![]() ![]() Group: Members Posts: 10265 Joined: 5-April 05 From: Canada Member No.: 227 |
The best set of grooves on any object since Phobos. This has to put an end to the 'grooves caused by Mars ejecta' argument. fantastic object and a wonderful data set. And this is just the highest priority data, all the rest still to come.
Phil -------------------- ... because the Solar System ain't gonna map itself.
Also to be found posting similar content on https://mastodon.social/@PhilStooke Maps for download (free PDF: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf NOTE: everything created by me which I post on UMSF is considered to be in the public domain (NOT CC, public domain) |
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Jul 11 2010, 06:25 AM
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#2
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Junior Member ![]() ![]() Group: Members Posts: 22 Joined: 8-March 10 Member No.: 5252 |
The best set of grooves on any object since Phobos. This has to put an end to the 'grooves caused by Mars ejecta' argument. fantastic object and a wonderful data set. And this is just the highest priority data, all the rest still to come. Phil The similarities with Phobos are striking, the photos clearly show two families of roughly parallel grooves, in two different planes. But the grooves seem to have been obliterated over most of the surface by later big impacts. Once again I have to say they look like the tracks of intersection with rings, edge on. What else could carve a long smooth trench on the surface of a large object in space? Where Lutetia might have encountered rings is not going to be easy to answer, the chaos of the early Solar System is way beyond our scrutiny. The grooves do seem to be very old features, pockmarked with small craters, as well as restricted to areas clear of debris from the big ones. |
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Jul 16 2010, 08:13 AM
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#3
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Junior Member ![]() ![]() Group: Members Posts: 22 Joined: 8-March 10 Member No.: 5252 |
I will try to get hold of The New Solar System. Thanks for the leads on the mechanisms for ring decay.
I'm skeptical about the idea of decaying rings being the origin of the grooves. How could a decaying ring leave a family of grooves, parallel but separated by gaps many times the width of a groove? These are most apparent on Phobos, but Lutetia has them as well. If the ring orbits the center of gravity and decays onto the surface of a non-rotating body, it would leave a single groove all the way around. If the main body was rotating, and the ring was at high inclination to the equator, the groove would be smeared out. I can't see a mechanism for the creation of families of grooves, which in the case of Phobos, peter out on one hemisphere. |
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Jul 16 2010, 01:09 PM
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#4
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![]() Member ![]() ![]() ![]() Group: Members Posts: 656 Joined: 20-April 05 From: League City, Texas Member No.: 285 |
...How could a decaying ring leave a family of grooves, parallel but separated by gaps many times the width of a groove? These are most apparent on Phobos, but Lutetia has them as well. If the ring orbits the center of gravity and decays onto the surface of a non-rotating body, it would leave a single groove all the way around. If the main body was rotating, and the ring was at high inclination to the equator, the groove would be smeared out. ... I would guess that the ring/surface intersection events are episodic (probably chaotically so). Once the ring begins intersecting the surface, the interaction would throw-up debris which would cause a rapid decay/depletion of the portion of the ring immediately closest to the surface, creating a distinct groove. Over time, this would repeat as the ring continues to decay. Yes, if the ring were equatorial this process would lead to a single ridge about the equator, however the grazing impacts hypothesized to create these rings are unlikely to be oriented on the equator, so they would be expected to have some random orientation to the pole. Rings generated by grazing impacts would be categorically distinct from planetary rings which derive from the breakup of (typically) equatorially orbiting satellites. I'd love to try doing a simulation to validate the theory, as opposed to the mental simulation I'm doing here, but lack the resources. Perhaps the folks who worked on the Iapetus ring-intersection model would like to give it a go |
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Jul 17 2010, 04:56 AM
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#5
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Junior Member ![]() ![]() Group: Members Posts: 22 Joined: 8-March 10 Member No.: 5252 |
I would guess that the ring/surface intersection events are episodic (probably chaotically so). ... Our best example of a grooved body is Phobos. 28Km long, escape velocity ~ 11m/sec. Any ring around Phobos would have been in slow motion, and tenuous since most of the debris from impacts would have escaped. Hardly the stuff to carve those trenches. |
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Jul 19 2010, 01:08 PM
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#6
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![]() Member ![]() ![]() ![]() Group: Members Posts: 656 Joined: 20-April 05 From: League City, Texas Member No.: 285 |
... Any ring around Phobos would have been in slow motion, and tenuous since most of the debris from impacts would have escaped... Phobos may be something of a special case, since it's in orbit around a substantial planet. As has been suggested elsewhere, grooves on Phobos may be due to intersection with a ring around Mars. |
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