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Hinrichs, John L., Lucey, Paul G. (2002) Temperature-Dependent Near-Infrared Spectral Properties of Minerals, Meteorites, and Lunar Soil. Icarus, 155 (1). 169-180 doi:10.1006/icar.2001.6754

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Reference TypeJournal (article/letter/editorial)
TitleTemperature-Dependent Near-Infrared Spectral Properties of Minerals, Meteorites, and Lunar Soil
JournalIcarus
AuthorsHinrichs, John L.Author
Lucey, Paul G.Author
Year2002 (January)Volume155
Issue1
PublisherElsevier BV
DOIdoi:10.1006/icar.2001.6754Search in ResearchGate
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Mindat Ref. ID6378410Long-form Identifiermindat:1:5:6378410:1
GUID0
Full ReferenceHinrichs, John L., Lucey, Paul G. (2002) Temperature-Dependent Near-Infrared Spectral Properties of Minerals, Meteorites, and Lunar Soil. Icarus, 155 (1). 169-180 doi:10.1006/icar.2001.6754
Plain TextHinrichs, John L., Lucey, Paul G. (2002) Temperature-Dependent Near-Infrared Spectral Properties of Minerals, Meteorites, and Lunar Soil. Icarus, 155 (1). 169-180 doi:10.1006/icar.2001.6754
In(2002, January) Icarus Vol. 155 (1) Elsevier BV

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Lucey, Paul G., Hinrichs, John, Kelly, Mary, Wellnitz, Dennis, Izenberg, Noam, Murchie, Scott, Robinson, Mark, Clark, Beth E., Bell, James F. (2002) Detection of Temperature-Dependent Spectral Variation on the Asteroid Eros and New Evidence for the Presence of an Olivine-Rich Silicate Assemblage. Icarus, 155 (1). 181-188 doi:10.1006/icar.2001.6747
Lucey, Paul G., Hinrichs, John, Kelly, Mary, Wellnitz, Dennis, Izenberg, Noam, Murchie, Scott, Robinson, Mark, Clark, Beth E., III, James F.Bell (2002) Detection of Temperature-Dependent Spectral Variation on the Asteroid Eros and New Evidence for the Presence of an Olivine-Rich Silicate Assemblage. Icarus, 160 (1). 224pp. doi:10.1006/icar.2002.6983
Hinrichs, J. L., Lucey, P. G., Robinson, M. S., Meibom, A., Krot, A. N. (1999) Implications of temperature-dependent near-IR spectral properties of common minerals and meteorites for remote sensing of asteroids. Geophysical Research Letters, 26 (12) 1661-1664 doi:10.1029/1999gl900334
Grundy, W (2002) The Temperature-Dependent Spectrum of Methane Ice I between 0.7 and 5 μm and Opportunities for Near-Infrared Remote Thermometry. Icarus, 155 (2). 486-496 doi:10.1006/icar.2001.6726
Veverka, J. (2002) NEAR at Eros. Icarus, 155 (1). 1-2 doi:10.1006/icar.2002.6824
Pieters, C (2002) Statistical Analysis of the Links among Lunar Mare Soil Mineralogy, Chemistry, and Reflectance Spectra. Icarus, 155 (2). 285-298 doi:10.1006/icar.2001.6749
Rivkin, A (2002) Near-Infrared Spectrophotometry of Phobos and Deimos. Icarus, 156 (1). 64-75 doi:10.1006/icar.2001.6767
Blewett, David T., Lucey, Paul G., Hawke, B.Ray, Ling, G.Gina, Robinson, Mark S. (1997) A Comparison of Mercurian Reflectance and Spectral Quantities with Those of the Moon. Icarus, 129 (1). 217-231 doi:10.1006/icar.1997.5785
Salisbury, John W., Basu, Abhijit, Fischer, Erich M. (1997) Thermal Infrared Spectra of Lunar Soils. Icarus, 130 (1). 125-139 doi:10.1006/icar.1997.5809
Davies, John K., Sykes, Mark V., Cruikshank, Dale P. (1993) Near-Infrared Photometry and Spectroscopy of the Unusual Minor Planet 5145 Pholus (1992AD). Icarus, 102 (1). 166-169 doi:10.1006/icar.1993.1040
Helfenstein, Paul, Veverka, Joseph, Hillier, John (1997) The Lunar Opposition Effect: A Test of Alternative Models. Icarus, 128 (1). 2-14 doi:10.1006/icar.1997.5726
 
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