Seeds of life among the stars: MIT scientists find complex carbon molecules in a distant cloud, pointing to clues to Earth’s beginnings!
Oct 26, 2024, 11:44 IST
Scientists have uncovered a tantalising clue to the origins of life on Earth, finding complex organic molecules in a distant interstellar cloud.
A team of researchers led by MIT has detected pyrene, a large molecule composed of carbon and hydrogen, within the Taurus Molecular Cloud. This discovery is significant as it suggests that complex organic molecules, the building blocks of life, were present in the early stages of our Solar System.
Pyrene, a polycyclic aromatic hydrocarbon (PAH), is a relatively large and stable molecule. Its presence in interstellar space challenges the conventional belief that complex molecules cannot survive the harsh conditions of star formation. The detection of pyrene indicates that these molecules can endure and even thrive in the extreme environments of space.
The discovery of pyrene is particularly exciting because it aligns with previous findings from the asteroid Ryugu, where significant amounts of pyrene were identified. This suggests that these molecules may have been inherited from the interstellar cloud that preceded our Solar System.
While pyrene itself is difficult to detect directly, scientists utilise a tracer molecule called 1-cyanopyrene. By observing the radio emissions of 1-cyanopyrene, researchers were able to infer the presence of pyrene in the Taurus Molecular Cloud.
The implications of this discovery are profound. It strengthens the hypothesis that complex organic molecules, essential for the emergence of life, were delivered to Earth through comets, asteroids, or interstellar dust. This cosmic infusion of organic matter may have provided the initial spark for the development of life on our planet.
As scientists continue to explore the universe, we may uncover even more complex molecules and gain deeper insights into the origins of life. This latest discovery brings us one step closer to unravelling the mysteries of our cosmic origins and the potential for life elsewhere in the universe.
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A team of researchers led by MIT has detected pyrene, a large molecule composed of carbon and hydrogen, within the Taurus Molecular Cloud. This discovery is significant as it suggests that complex organic molecules, the building blocks of life, were present in the early stages of our Solar System.
Pyrene, a polycyclic aromatic hydrocarbon (PAH), is a relatively large and stable molecule. Its presence in interstellar space challenges the conventional belief that complex molecules cannot survive the harsh conditions of star formation. The detection of pyrene indicates that these molecules can endure and even thrive in the extreme environments of space.
The discovery of pyrene is particularly exciting because it aligns with previous findings from the asteroid Ryugu, where significant amounts of pyrene were identified. This suggests that these molecules may have been inherited from the interstellar cloud that preceded our Solar System.
While pyrene itself is difficult to detect directly, scientists utilise a tracer molecule called 1-cyanopyrene. By observing the radio emissions of 1-cyanopyrene, researchers were able to infer the presence of pyrene in the Taurus Molecular Cloud.
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As scientists continue to explore the universe, we may uncover even more complex molecules and gain deeper insights into the origins of life. This latest discovery brings us one step closer to unravelling the mysteries of our cosmic origins and the potential for life elsewhere in the universe.