Cargando…
Deriving iron contents from past and future Venus surface spectra with new high-temperature laboratory emissivity data
In situ information on the surface composition of Venus is based on measurements of a small number of landing sites. In the laboratory, we measured the emissivity of a range of igneous rocks at temperatures up to 480°C. We show that high-temperature laboratory spectra of basalts are consistent with...
| Autores principales: | , , , |
|---|---|
| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
American Association for the Advancement of Science
2021
|
| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7810366/ https://www.ncbi.nlm.nih.gov/pubmed/33523894 http://dx.doi.org/10.1126/sciadv.aba9428 |