by AVAO » Sat Nov 04, 2023 4:35 pm
Chris Peterson wrote: ↑Sat Nov 04, 2023 2:07 pm
johnnydeep wrote: ↑Sat Nov 04, 2023 1:49 pm
Chris Peterson wrote: ↑Sat Nov 04, 2023 1:22 pm
There is no evidence of "exploded planets" in the Solar System (and no physics to explain such a thing). Asteroids are remnants of material that failed (probably due to gravitational resonance zones created by the gas giants) to coalesce into planets. The total mass of all the asteroids in the Solar System is about 3% of the mass of the Moon. Nowhere near enough material to point back to any planet.
I won't comment on the "exploded planet" theory (however unlikely it may be), but on the OP's statement about "belts". Each of these asteroids does indeed appear to have an "equatorial" belt or ridge, though the ridge on Dinkinesh itself is much more obvious than the ridge - if it is in fact more than an accidental artifact of perspective - on its moon. A few other moons of planets also exhibit ridges. Is there a good explanation for them?
Because they rotate. That means there are different forces present at the equator than near the poles... and in the common case of these things being "rubble piles" it isn't unexpected for material to accumulate around the equator. The YORP effect can result in asteroids spinning up, creating increased distortion and eventually the ejection of material and possible formation of a binary (as with today's APO). Here's an example of such a system being simulated mathematically:
.
Click to play embedded YouTube video.
Well, I'm not entirely convinced by the simulation, as the belt formation would have to continuously decrease towards the poles. For many moons, however, the belt can be defined as an equatorial bulge untill only a very narrow ridge, with a clear and independent shape, as we can see for example on Saturn's moons Pan or Iapetus. The simulation cannot or only insufficiently explain these phenomena.
"New image of Saturn’s tiny moon Pan, which orbits inside the Encke Gap of Saturn’s rings. A thin “skirt” or ridge of material surrounds the moon’s equator, giving it a "ravioli shaped" appearance. Photo Credit: NASA/JPL-Caltech/Space Science Institute/Ian Regan"
Credit: Saturn moon Iapetus NASA/JPL/Space Science Institute
Credit: Saturn moon Iapetus NASA/JPL/Space Science Institute
Somewhat less clearly recognizable:
This image of Atlas was taken by Cassini’s narrow-angle camera during a close flyby on April 12, 2017. Image credit: NASA / JPL-Caltech / Space Science Institute.
[quote="Chris Peterson" post_id=334855 time=1699106833 user_id=117706]
[quote=johnnydeep post_id=334853 time=1699105797 user_id=132061]
[quote="Chris Peterson" post_id=334852 time=1699104129 user_id=117706]
There is no evidence of "exploded planets" in the Solar System (and no physics to explain such a thing). Asteroids are remnants of material that failed (probably due to gravitational resonance zones created by the gas giants) to coalesce into planets. The total mass of all the asteroids in the Solar System is about 3% of the mass of the Moon. Nowhere near enough material to point back to any planet.
[/quote]
I won't comment on the "exploded planet" theory (however unlikely it may be), but on the OP's statement about "belts". Each of these asteroids does indeed appear to have an "equatorial" belt or ridge, though the ridge on Dinkinesh itself is much more obvious than the ridge - if it is in fact more than an accidental artifact of perspective - on its moon. A few other moons of planets also exhibit ridges. Is there a good explanation for them?
[/quote]
Because they rotate. That means there are different forces present at the equator than near the poles... and in the common case of these things being "rubble piles" it isn't unexpected for material to accumulate around the equator. The YORP effect can result in asteroids spinning up, creating increased distortion and eventually the ejection of material and possible formation of a binary (as with today's APO). Here's an example of such a system being simulated mathematically:
.
[youtube]https://www.youtube.com/watch?v=nzyettXkIqY[/youtube]
[/quote]
Well, I'm not entirely convinced by the simulation, as the belt formation would have to continuously decrease towards the poles. For many moons, however, the belt can be defined as an equatorial bulge untill only a very narrow ridge, with a clear and independent shape, as we can see for example on Saturn's moons Pan or Iapetus. The simulation cannot or only insufficiently explain these phenomena.
[img2]https://www.americaspace.com/wp-content/uploads/2017/03/32496709034_51f9a2b51f_b.jpg[/img2]
[size=75]"New image of Saturn’s tiny moon Pan, which orbits inside the Encke Gap of Saturn’s rings. A thin “skirt” or ridge of material surrounds the moon’s equator, giving it a "ravioli shaped" appearance. Photo Credit: NASA/JPL-Caltech/Space Science Institute/Ian Regan"[/size]
[img2]
https://encrypted-tbn0.gstatic.com/images?q=tbn:ANd9GcT9Qsw3yiADVl517734k7qdp1qHaV0eUmSMcCes3KQe7X2P1UD_a7gkV3NU5z5VyuWMn7Q&usqp=CAU[/img2]
[img2]https://science.nasa.gov/_ipx/w_4096&f_webp/https://smd-cms.nasa.gov/wp-content/uploads/2023/09/PIA06166-1.jpg%3Fw=1380[/img2]
[size=75]Credit: Saturn moon Iapetus NASA/JPL/Space Science Institute[/size]
[img]https://www.researchgate.net/profile/Alice-Quillen/publication/311586231/figure/fig5/AS:613885228875777@1523373052058/An-image-of-the-ridge-of-Iapetus-taken-from-around-62-000-km-in-September-2007-by-the.png[/img]
[size=75]Credit: Saturn moon Iapetus NASA/JPL/Space Science Institute[/size]
Somewhat less clearly recognizable:
[img2]https://cdn.sci.news/images/2017/04/image_4786_1-Atlas.jpg[/img2]
[size=75]This image of Atlas was taken by Cassini’s narrow-angle camera during a close flyby on April 12, 2017. Image credit: NASA / JPL-Caltech / Space Science Institute.[/size]