Population III star in the context of "Globular cluster"

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⭐ Core Definition: Population III star

In 1944, Walter Baade categorized groups of stars within the Milky Way into stellar populations.In the abstract of the article by Baade, he recognizes that Jan Oort originally conceived this type of classification in 1926.

Baade observed that bluer stars were strongly associated with the spiral arms, and yellow stars dominated near the central galactic bulge and within globular star clusters. Two main divisions were deemed population I and population II stars, with another newer, hypothetical division called population III added in 1978.

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Population III star in the context of James Webb Space Telescope

The James Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy. It is the largest telescope in space, and is equipped with high-resolution and high-sensitivity instruments, allowing it to view objects too old, distant, or faint for the Hubble Space Telescope. This enables investigations across many fields of astronomy and cosmology, such as observation of the first stars and the formation of the first galaxies, and detailed atmospheric characterization of potentially habitable exoplanets.

Although the Webb's mirror diameter is 2.7 times larger than that of the Hubble Space Telescope, it only produces images of comparable resolution because it observes in the infrared spectrum, of longer wavelength than the Hubble's visible spectrum. The longer the wavelength the telescope is designed to observe, the larger the information-gathering surface (mirrors in the infrared spectrum or antenna area in the millimeter and radio ranges) required for the same resolution.

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