#molecular-clouds

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#star-formation

Stars - NASA Science

Stars form in molecular clouds, eventually leading to protostars and stellar clusters.
Main sequence stars undergo nuclear fusion, with gradual changes throughout their lifecycle.
The supernova explosion marks the death of a star, leaving behind dense remnants.

3D-Printed Cosmic Clouds Unravel the Mysteries of Star Formation

Molecular clouds in space contain intricate structures like filaments and cores, vital for understanding star formation.

Stars - NASA Science

Stars form in molecular clouds, eventually leading to protostars and stellar clusters.
Main sequence stars undergo nuclear fusion, with gradual changes throughout their lifecycle.
The supernova explosion marks the death of a star, leaving behind dense remnants.

3D-Printed Cosmic Clouds Unravel the Mysteries of Star Formation

Molecular clouds in space contain intricate structures like filaments and cores, vital for understanding star formation.
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High-temperature 205Tl decay clarifies 205Pb dating in early Solar System - Nature

Short-lived radioactive nuclei provide insights into the early Solar System's formation and nucleosynthetic history.
The isolation time of Solar System materials was confirmed to be between 9-26 Myr before solar birth.
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