Earth and Space Sciences Regents practice

Earth and Space Sciences Regents, August 2025, question 2

The passage, Energy in the Sun, says that deuterium and helium-3 atoms in the Sun's core combine under very high temperatures and pressures to form helium-4 and release large amounts of energy. The Layers of the Sun Model shows four layers from the center outward: core, radiative zone, convection zone and photosphere. Its table says: core, nuclear reactions occur, 27 million degrees Fahrenheit (°F); radiative zone, serves as a passage for radiation energy from core to surface; convection zone, hot material rises to the surface and cools; photosphere, observable layer that gives off electromagnetic energy.
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What the figure shows

The passage, Energy in the Sun, says that deuterium and helium-3 atoms in the Sun's core combine under very high temperatures and pressures to form helium-4 and release large amounts of energy. The Layers of the Sun Model shows four layers from the center outward: core, radiative zone, convection zone and photosphere. Its table says: core, nuclear reactions occur, 27 million degrees Fahrenheit (°F); radiative zone, serves as a passage for radiation energy from core to surface; convection zone, hot material rises to the surface and cools; photosphere, observable layer that gives off electromagnetic energy.

How to think about it

The question has two parts: where the energy is made, and where it leaves the Sun. Use the Information About Layer column of the table for both. Then check each claim against both parts, not only one.

Which claim best describes where energy is produced in the Sun and how the energy is released into space?

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