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Dating : Depending on my age, where I live, and my interest

h2>Dating : Depending on my age, where I live, and my interest

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The outlook for the biosphere is equally bleak when there is insufficient heating from the decay of radioactive elements. In this case, volcanism is quieted, but so is the planet’s dynamo. There is simply not enough heat to sustain convection and without it, there is no magnetic field. Mars may have suffered this fate early in its history which explains its relatively thin atmosphere and weak magnetic field today.

Heat is drawn out of the planets interior to the surface where we see it in the form of volcanoes. It also drives plate tectonics, the massive rock recycling system that takes cold, solid rock from the surface and melts it at depth. It’s the process by which continents move and mountain ranges are built. Poetic, sure, but convection within Earth’s interior also serves a vital function to the preservation of life on the surface: dynamism. Earth’s liquid outer core is mainly composed of iron. As the liquid iron moves, it generates the planet’s magnetic field. This magnetic field protects Earth’s atmosphere from degradation by the Sun’s solar winds. Without it, Earth would lose its atmosphere and life on this planet would disappear with it.

Tidal friction can generate enough heat to maintain liquid water even without an atmosphere. Another of Jupiter’s moons, Europa, may have a liquid water ocean underneath its icy exterior, yet it’s nowhere near the Goldilocks zone. However, the thick layer of ice surrounding the moon could protect alien life living within its watery depths.
In March of this year I found myself staring out over a sea of clouds from the top of Mount Taranaki on the north island of New Zealand. At the time, I was only thinking about putting one foot in front of the other as I climbed the steep scree field on the mountain’s north side. That, and the pack of Tim Tams I had stashed away for a small celebration at the summit. I definitely wasn’t thinking about radioactive isotopes, but maybe I should have been. Without the heat and energy generated from the radioactive decay of these tiny atoms, the mountain I was climbing might not exist — and neither would I.
Add specificity to make your writing more engaging and more accurate with less chance of being misunderstood. Being specific is an example where more words are better. You’ll attract more readers, more fans, more responses.

There are a lot of naturally occurring radioactive elements, but most of them are rare on our planet. The three most common radioactive elements on Earth are potassium, thorium, and uranium. Potassium is most common at the surface — it’s what makes bananas and granite counter tops slightly radioactive — but thorium and uranium are the two that matter most to Earth’s dynamism.

Volcanoes like Mount Taranaki are part of a complex interaction between the ground we stand on, the air we breath, and every living thing on this planet. If you’ve ever felt an earthquake or seen lava cascading into the ocean in Hawaii, you know our planet is alive and active. The geologic activity we see on the surface is evidence of the convection going on within Earth’s mantle — the semi-solid layer of rock that makes up the bulk of our planet’s interior — as it transfers heat away from the liquid outer core.Earth still retains some residual heat from its formation 4.5 billion years ago, but that alone is not sufficient to sustain life on our planet. New research from the University of California — Santa Cruz shows that the key to Earth’s internal heat, and the preservation of its atmosphere and biosphere, is isotopic radioactive decay.Add specificity to make your writing more engaging and more accurate with less chance of being misunderstood. Being specific is an example where more words are better. You’ll attract more readers, more fans, more responses.
While there are a tantalizing number of possibilities for how life could exist on other planets, we’re perhaps most interested in life that would somehow resemble what we know on Earth. It’s easier for us to imagine ourselves stepping foot on an alien world with a breathable atmosphere than exploring the inky black depths of Europa’s hidden ocean, even though the latter is far more likely. Now we have a new set of criteria to narrow the search.
While the plethora of relationships in your life function on different levels, they also all require certain factors, behaviours, and actions on your part to work well for all involved parties.

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In order to understand how radioactive decay affects Earth’s heating and internal convection, researchers modeled three different scenarios: excessive heating from radioactivity, minimal heating, and the base case of Earth as it is. Using the base case, the model accurately predicted active plate tectonics and an internal dynamo capable of generating a magnetic field.

Here’s where things get interesting. When the researchers increased the amount of heating from radioactive decay, volcanism increased, but the amount of internal convection generated was insufficient to create a magnetic field. There was too much heat at the planet’s surface to allow the internally generated heat to dissipate. Heat alone is not enough to create a dynamo. There has to be a large enough temperature gradient between the hot core and cool rocks near the surface for convection to take place. Life on this planet doesn’t have a great track record of surviving periods of intense volcanism as proposed by this model, but losing our atmosphere to the solar winds certainly wouldn’t help.

Our planet exists in the so-called Goldilocks zone where water is liquid at the planet’s surface because it’s not too hot and not too cold. What this research shows, is that that alone is not enough. For life to exist as we know it, there has to be just the right amount of heating from the decay of radioactive elements to sustain a dynamo, too. The dynamo is critical to preserving the planet’s atmosphere and the life that depends on it.

It’s possible, though, that life could exist on other planets in completely novel ways. Another source of planetary heat is tidal heating, which occurs when orbital and rotational energy (from a moon orbiting around its planet, for example) are dissipated as heat. Jupiter’s moon, Io, is the most geologically active body in our solar system despite being about the same size as our moon. If it weren’t for its proximity to Jupiter and its other moons, it would be frozen solid. Instead, Io could remain geologically active for billions of years.

While there are a tantalizing number of possibilities for how life could exist on other planets, we’re perhaps most interested in life that would somehow resemble what we know on Earth. It’s easier for us to imagine ourselves stepping foot on an alien world with a breathable atmosphere than exploring the inky black depths of Europa’s hidden ocean, even though the latter is far more likely. Now we have a new set of criteria to narrow the search.

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