In which region of the sun does energy move through circulating currents of gases? photosphere corona core radiative zone chromosphere convective zone

The convective zone  is the region of the Sun in which energy move through circulating currents of gases.

The convective zone is the outer most region of the interior of the Sun where energy is transported by circulating currents of gases (in a process called convection). The convection zone extends from the visible surface of the sun to a depth of about 200,000 km. The upper layer of this region, which is known as photosphere is where light (photons) is usually produced.

this age may represent the age of the earth's accretion, of core formation, or of the material from which the earth formed. this dating is based on evidence from radiometric age-dating of meteorite material and is consistent with the radiometric ages of the oldest-known terrestrial and lunar samples.