Evidence for a polar ethane cloud on Titan
Science
By: C.A. Griffith, P. Penteado, P. Rannou, R. Brown, V. Boudon, K. H. Baines, R. Clark, P. Drossart, B. Buratti, P. Nicholson, C.P. McKay, A. Coustenis, A. Negrao, and R. Jaumann
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Abstract
Spectra from Cassini's Visual and Infrared Mapping Spectrometer reveal the presence of a vast tropospheric cloud on Titan at latitudes 51?? to 68?? north and all longitudes observed (10?? to 190?? west). The derived characteristics indicate that this cloud is composed of ethane and forms as a result of stratospheric subsidence and the particularly cool conditions near the moon's north pole. Preferential condensation of ethane, perhaps as ice, at Titan's poles during the winters may partially explain the lack of liquid ethane oceans on Titan's surface at middle and lower latitudes.
Suggested Citation
Griffith, C., Penteado, P., Rannou, P., Brown, R., Boudon, V., Baines, K.H., Clark, R., Drossart, P., Buratti, B., Nicholson, P., McKay, C., Coustenis, A., Negrao, A., Jaumann, R., 2006, Evidence for a polar ethane cloud on Titan: Science, v. 313, no. 5793, p. 1620-1622, https://doi.org/10.1126/science.1128245.
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Evidence for a polar ethane cloud on Titan |
| Series title | Science |
| DOI | 10.1126/science.1128245 |
| Volume | 313 |
| Issue | 5793 |
| Year Published | 2006 |
| Language | English |
| Larger Work Type | Article |
| Larger Work Subtype | Journal Article |
| Larger Work Title | Science |
| First page | 1620 |
| Last page | 1622 |