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What (who) is neptunian$52189$ - definition
![[[Euler diagram]] showing the types of bodies in the Solar System.](https://commons.wikimedia.org/wiki/Special:FilePath/Euler-Diagram bodies in the Solar System.jpg?width=200 "[[Euler diagram]] showing the types of bodies in the Solar System.")
![[[Pluto]] imaged by ''[[New Horizons]]''](https://commons.wikimedia.org/wiki/Special:FilePath/Pluto in True Color - High-Res.jpg?width=200 "[[Pluto]] imaged by ''[[New Horizons]]''")
![Size comparison between the [[Moon]], Neptune's moon Triton, Pluto, several large TNOs, and the asteroid Ceres. Their respective shapes are not represented.](https://commons.wikimedia.org/wiki/Special:FilePath/Selected Planemos.svg?width=200 "Size comparison between the [[Moon]], Neptune's moon Triton, Pluto, several large TNOs, and the asteroid Ceres. Their respective shapes are not represented.")
![Pholus]] are not trans-Neptunian.](https://commons.wikimedia.org/wiki/Special:FilePath/TheTransneptunians Color Distribution.svg?width=200 "Pholus]] are not trans-Neptunian.")
![245}}'s orbit librating in a 2:9 resonance with [[Neptune]]](https://commons.wikimedia.org/wiki/Special:FilePath/2015RR245 resonance.gif?width=200 "245}}'s orbit librating in a 2:9 resonance with [[Neptune]]")
![Orcus]] and [[Pluto]] in a [[rotating frame]] with a period equal to [[Neptune]]'s [[orbital period]] (holding Neptune stationary)](https://commons.wikimedia.org/wiki/Special:FilePath/OrcusandPlutoRotatingFrame.gif?width=200 "Orcus]] and [[Pluto]] in a [[rotating frame]] with a period equal to [[Neptune]]'s [[orbital period]] (holding Neptune stationary)")
![Ixion]]](https://commons.wikimedia.org/wiki/Special:FilePath/ThePlutinos Size Albedo Color2.svg?width=200 "Ixion]]")
![[[Jacques Babinet]], an early proponent of a trans-Neptunian planet](https://commons.wikimedia.org/wiki/Special:FilePath/Jacques Babinet.jpg?width=200 "[[Jacques Babinet]], an early proponent of a trans-Neptunian planet")
Wikipedia
A clastic dike is a seam of sedimentary material that fills an open fracture in and cuts across sedimentary rock strata or layering in other rock types. Clastic dikes form rapidly by fluidized injection (mobilization of pressurized pore fluids) or passively by water, wind, and gravity (sediment swept into open cracks). Diagenesis may play a role in the formation of some dikes. Clastic dikes are commonly vertical or near-vertical. Centimeter-scale widths are common, but thicknesses range from millimetres to metres. Length is usually many times width.
Clastic dikes are found in sedimentary basin deposits worldwide. Formal geologic reports of clastic dikes began to emerge in the early 19th century.
Terms synonymous with clastic dike include: clastic intrusion, sandstone dike, fissure fill, soft-sediment deformation, fluid escape structure, seismite, injectite, liquefaction feature, neptunian dike (passive fissure fills), paleoseismic indicator, pseudo ice wedge cast, sedimentary insertion, sheeted clastic dike, synsedimentary filling, tension fracture, hydraulic injection dike, and tempestite.
