2015
DOI: 10.1007/s11084-015-9410-0
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Organic Compounds in Circumstellar and Interstellar Environments

Abstract: Recent research has discovered that complex organic matter is prevalent throughout the Universe. In the Solar System, it is found in meteorites, comets, interplanetary dust particles, and planetary satellites. Spectroscopic signatures of organics with aromatic/aliphatic structures are also found in stellar ejecta, diffuse interstellar medium, and external galaxies. From space infrared spectroscopic observations, we have found that complex organics can be synthesized in the late stages of stellar evolution. Sho… Show more

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Cited by 8 publications
(4 citation statements)
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“…Carbon (C) is the 4th most abundant element in the Universe and highly complex organic compounds involving this element have been discovered on objects from the solar system and more distant galaxies (Kwok, 2009). Space remote sensing techniques, e.g., space infrared spectroscopy, have identified more than 150 molecules with stretching and bending modes of compounds with aromatic and aliphatic structures (Kwok, 2009(Kwok, , 2015. For research in astronomy, one of the most definite and surprising knowledge of molecular synthesis comes from circumstellar envelopes of evolved stars, from the asymptotic giant branch (AGB) stars to protoplanetary nebulae to planetary nebulae, over very short (∼10 3 yr) time scales.…”
Section: Pre-to Early Planetary Processmentioning
confidence: 99%
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“…Carbon (C) is the 4th most abundant element in the Universe and highly complex organic compounds involving this element have been discovered on objects from the solar system and more distant galaxies (Kwok, 2009). Space remote sensing techniques, e.g., space infrared spectroscopy, have identified more than 150 molecules with stretching and bending modes of compounds with aromatic and aliphatic structures (Kwok, 2009(Kwok, , 2015. For research in astronomy, one of the most definite and surprising knowledge of molecular synthesis comes from circumstellar envelopes of evolved stars, from the asymptotic giant branch (AGB) stars to protoplanetary nebulae to planetary nebulae, over very short (∼10 3 yr) time scales.…”
Section: Pre-to Early Planetary Processmentioning
confidence: 99%
“…For research in astronomy, one of the most definite and surprising knowledge of molecular synthesis comes from circumstellar envelopes of evolved stars, from the asymptotic giant branch (AGB) stars to protoplanetary nebulae to planetary nebulae, over very short (∼10 3 yr) time scales. Specifically, carbon is synthesized in the core of AGB stars by nucleosynthesis and then dredged up to the star surface, and, subsequently, new Cbearing molecules with increasing complexity are detected through infrared and millimeter-wave spectroscopy in the stellar winds ejected from these stars (Kwok, 2015). By these processes, simple molecules, such as acetylene (C 2 H 2 ), CN chains (HCN, HC 3 N, HC 5 N), and rings (C 3 H 2 ), are formed at first in the stellar winds of AGB stars, followed by the formation of di-acetylene, triacetylene, and the first aromatic molecule, benzene, in the proto-planetary nebula stage.…”
Section: Pre-to Early Planetary Processmentioning
confidence: 99%
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“…The advent of an atomistic understanding of chemistry at the beginning of the 20th century, however, dealt the death-blow to vitalism since there was nothing special to organic molecules as compared to their inorganic counterparts, apart from their higher structural complexity (a disputable claim in the light of some of the minerals we will discuss below) and no natural border between inorganic and organic chemistry could be defined. It is ironic that the detection of organic molecules in numerous extraterrestrial settings from the surface of Titan [3] through comet atmospheres [4] to interstellar space [5] is still systematically interpreted as evidence that the seed for life on Earth may have come from outer space rather than as showing that there is nothing special to complex hydrocarbons and that their synthesis is just chemistry.…”
Section: The Textbook Narrative: Life From Organic Moleculesmentioning
confidence: 99%