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Bubble streams in Titan’s seas as a product of liquid N2 + CH4 + C2H6 cryogenic mixture

Bubble streams in Titan’s seas as a product of liquid N2 + CH4 + C2H6 cryogenic mixture

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_02268643v1

Bubble streams in Titan’s seas as a product of liquid N2 + CH4 + C2H6 cryogenic mixture

About this item

Full title

Bubble streams in Titan’s seas as a product of liquid N2 + CH4 + C2H6 cryogenic mixture

Publisher

London: Nature Publishing Group UK

Journal title

Nature astronomy, 2017-05, Vol.1 (5), Article 0102

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

Titan, Saturn’s largest moon, is the only extraterrestrial body known to support stable liquid on its surface, in the form of seas and lakes that dot the polar regions. Many indications suggest that the liquid should be composed of a mixture of nitrogen, methane and ethane. Recent observations by Cassini’s Radio Detection and Ranging (RADAR) instru...

Alternative Titles

Full title

Bubble streams in Titan’s seas as a product of liquid N2 + CH4 + C2H6 cryogenic mixture

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_hal_primary_oai_HAL_hal_02268643v1

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_02268643v1

Other Identifiers

ISSN

2397-3366

E-ISSN

2397-3366

DOI

10.1038/s41550-017-0102

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