Dunno, im not a christian
<span>Thermal energy is transferred from hot places to cold places by convection. Convection occurs when warmer areas of a liquid or gas rise to cooler areas in the liquid or gas. Cooler liquid or gas then takes the place of the warmer areas which have risen higher. This results in a continous circulation pattern. Water boiling in a pan is a good example of these convection currents. Another good example of convection is in the atmosphere. The earth's surface is warmed by the sun, the warm air rises and cool air moves in.
</span><span>Convection is the movement of heat through gases or liquids. Heat from the sun heats the air which can account for A and D, but a lot of the Earth's heat is distributed by the ocean. Water has a high specific heat which can absorb a lot of heat in one place, and distribute it in a colder place evening out the Earth's temperatures a bit.
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So, the answer would be
<span>through the greenhouse effect
And could also be </span><span>through the movement of winds and currents</span>
The majority of the smaller islands in the Pacific are made up of build-up of coral deposits.
<h3>What do we find in the smaller islands of the Pacific?</h3>
Even though these islands are usually created as a result of volcanic activity, we find that they are composed of coral deposits.
These coral deposits come about as a result of a buildup over centuries which made these islands quite important in preservation efforts.
Find out more on coral deposits at brainly.com/question/13195203.
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Wind patterns, ocean currents, proximity to large bodies of water (i.e. seas and oceans), and elevation all impact climate patterns through a variety of factors. These factors largely impact the flow of energy and heat from the sun across the Earth's surface through processes of convection. For example the "Jet Stream" in the United States is a wind pattern that carries air and weather patterns across the United States and its flow shifts directions depending on seasons. Another is the Gulf Stream which brings warm currents from the Caribbean and Central American up the American coast and out into the Atlantic ocean warming the temperatures of the coastal water ways and also impacting the climate of the land near it.
Explanation:
Abstract
Most planetary systems are formed within stellar clusters, and these environments can shape their properties. This paper considers scattering encounters between solar systems and passing cluster members, and calculates the corresponding interaction cross-sections. The target solar systems are generally assumed to have four giant planets, with a variety of starting states, including circular orbits with the semimajor axes of our planets, a more compact configuration, an ultracompact state with multiple mean motion resonances, and systems with massive planets. We then consider the effects of varying the cluster velocity dispersion, the relative importance of binaries versus single stars, different stellar host masses, and finite starting eccentricities of the planetary orbits. For each state of the initial system, we perform an ensemble of numerical scattering experiments and determine the cross-sections for eccentricity increase, inclination angle increase, planet ejection, and capture. This paper reports results from over 2 million individual scattering simulations. Using supporting analytic considerations, and fitting functions to the numerical results, we find a universal formula that gives the cross-sections as a function of stellar host mass, cluster velocity dispersion, starting planetary orbital radius, and final eccentricity. The resulting cross-sections can be used in a wide variety of applications. As one example, we revisit constraints on the birth aggregate of our Solar system due to dynamical scattering and find N ≲ 104 (consistent with previous estimates).