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  • Infrared Radiation from Protostars: Understanding Early Stellar Evolution
    A newly formed protostar will radiate primarily in the infrared wavelength.

    Here's why:

    * Protostars are very young and still accreting material: They are surrounded by a dense cloud of gas and dust that absorbs most of the visible light they emit.

    * Infrared radiation can penetrate dust: Unlike visible light, infrared radiation can penetrate the dust surrounding the protostar and escape into space.

    * Protostars are relatively cool: Compared to mature stars, protostars are still relatively cool, with surface temperatures ranging from a few hundred to a few thousand Kelvin. This leads to peak emission in the infrared portion of the electromagnetic spectrum.

    As a protostar evolves and becomes hotter, its peak emission will shift towards shorter wavelengths, eventually into the visible light spectrum.

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