Answer:
Once the fusion reactions begin, they exert an outward pressure. As long as the inward force of gravity and the outward force generated by the fusion reactions are equal, the star remains stable.First, stars fuse hydrogen atoms into helium. Helium atoms then fuse to create beryllium, and so on, until fusion in the star's core has created every element up to iron.
Answer:
I would say B
Explanation:
its not A and im pretty sure its not C so i would say B. Sorry if im wrong.
Hi!
I don't have access to your grid, but iI can make my own to show you how to do it!
Please see attachment
on the y axis you can only use the relevant values - between 68 and 74; this way you can see more detail than if you'd used between 0 and 75.
You just need to plot the numbers and connect the line! (I did it with ms excel)
estimating geoacoustic properties of sediments with a wide grain-size distribution using sediment organic content and the viscous grain shearing model
Interstitial organic matter (OM) is a common component of marine sediment and is frequently measured across a variety of fields.
It is especially common in sediments with high silt/clay fractions. OM hasn't been accounted for in sediment acoustics models despite the fact that it suspends silt and clay particles in the sediment matrix, adheres to mineral surfaces, and typically lives between mineral contacts, all of which are thought to affect geoacoustic characteristics.
Recent research on sediments from the Baltic Sea, Texas, seagrass-bearing sediments, and mud banks in Brazil has demonstrated that OM content (OC) corresponds strongly with sediment geoacoustic characteristics, including porosity and index of impedance.
Learn more about sediments here
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