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High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko

High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_insu_01362335v1

Publication information

Publisher

Nature Publishing Group

Subjects

Subjects and topics

More information

Scope and Contents

Contents

The presence of solid carbonaceous matter in cometary dust was established by the detection of elements such as carbon, hydrogen, oxygen and nitrogen in particles from comet 1P/Halley1, 2. Such matter is generally thought to have originated in the interstellar medium3, but it might have formed in the solar nebula—the cloud of gas and dust that was...

Alternative Titles

Full title

High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_hal_primary_oai_HAL_insu_01362335v1

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_insu_01362335v1

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature19320

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