The reflection spectrum of liquid sulfur: Implications for Io
The spectral reflectance from 0.38 to 0.75 μm of a column of liquid sulfur has been measured at several temperatures between the melting point (∼118° C) and 173°C. Below 160°C the spectral reflectance was observed to vary reversibly as a function of temperature, independent of the previous thermal h...
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| Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 1983-12, Vol.56 (3), p.409-413 |
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| container_title | Icarus (New York, N.Y. 1962) |
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| creator | Nelson, Robert M. Pieri, David C. Baloga, Stephen M. Nash, Douglas B. Sagan, Carl |
| description | The spectral reflectance from 0.38 to 0.75 μm of a column of liquid sulfur has been measured at several temperatures between the melting point (∼118°
C) and 173°C. Below 160°C the spectral reflectance was observed to vary reversibly as a function of temperature, independent of the previous thermal history of the column. Once the temperature exceeded 160°C, the spectrum would not change given a subsequent decrease in temperature. The spectral reflectance of the liquid-sulfur column at all temperatures was very low (10–19%). Combining this information with Voyager spectrophotometry of Jupiter's satellite Io, it is concluded that liquid sulfur at any temperature on Io's surface would be classified as a “black area” according to the standards used by the Voyager imaging team in their spectrophotometric analysis (
L. Soderblom, T. V. Johnson, D. Morrison, E. Danielson, B. L. Smith, J. Veverka, A. Cook, C. Sagan, P. Kupferman, D. Pieri, J. Mosher, C. Avis, J. Gradie, and T. Clancy (1980).
Geophys. Res. Lett.
7, 963–966). |
| doi_str_mv | 10.1016/0019-1035(83)90162-8 |
| format | Article |
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L. Soderblom, T. V. Johnson, D. Morrison, E. Danielson, B. L. Smith, J. Veverka, A. Cook, C. Sagan, P. Kupferman, D. Pieri, J. Mosher, C. Avis, J. Gradie, and T. Clancy (1980).
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L. Soderblom, T. V. Johnson, D. Morrison, E. Danielson, B. L. Smith, J. Veverka, A. Cook, C. Sagan, P. Kupferman, D. Pieri, J. Mosher, C. Avis, J. Gradie, and T. Clancy (1980).
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C) and 173°C. Below 160°C the spectral reflectance was observed to vary reversibly as a function of temperature, independent of the previous thermal history of the column. Once the temperature exceeded 160°C, the spectrum would not change given a subsequent decrease in temperature. The spectral reflectance of the liquid-sulfur column at all temperatures was very low (10–19%). Combining this information with Voyager spectrophotometry of Jupiter's satellite Io, it is concluded that liquid sulfur at any temperature on Io's surface would be classified as a “black area” according to the standards used by the Voyager imaging team in their spectrophotometric analysis (
L. Soderblom, T. V. Johnson, D. Morrison, E. Danielson, B. L. Smith, J. Veverka, A. Cook, C. Sagan, P. Kupferman, D. Pieri, J. Mosher, C. Avis, J. Gradie, and T. Clancy (1980).
Geophys. Res. Lett.
7, 963–966).</abstract><cop>Legacy CDMS</cop><pub>Elsevier Inc</pub><doi>10.1016/0019-1035(83)90162-8</doi><tpages>5</tpages></addata></record> |
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| identifier | ISSN: 0019-1035 |
| ispartof | Icarus (New York, N.Y. 1962), 1983-12, Vol.56 (3), p.409-413 |
| issn | 0019-1035 1090-2643 |
| language | eng |
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| source | Elsevier ScienceDirect Journals Complete; NASA Technical Reports Server |
| subjects | Astronomy Earth, ocean, space Exact sciences and technology Jupiter Planets, their satellites and rings. Asteroids Solar system |
| title | The reflection spectrum of liquid sulfur: Implications for Io |
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