O Hesperiano é um sistema geológico e período inicial do planeta Marte caracterizado por atividade vulcânica generalizada e inundações catastróficas que esculpiram canais de fluxo imensos através da superfície.[1][2][3] O Hesperiano é um período intermediário e transitório da história marciana.[4][5]
- Boyce, Joseph M. (2008). The Smithsonian Book of Mars. Old Saybrook, CT: Konecky & Konecky. ISBN 978-1-58834-074-0
- Carr, Michael H. (2006). The Surface of Mars. Cambridge, UK: Cambridge University Press. ISBN 978-0-521-87201-0
- S. McMahon, T. Bosak, J. P. Grotzinger, R. E. Milliken, R. E. Summons, M. Daye, S. A. Newman, A. Fraeman, K. H. Williford, D. E. G. Briggs. A Field Guide to Finding Fossils on Mars. Journal of Geophysical Research: Planets; DOI: 10.1029/2017JE005478 (2018)
- Tanaka, K.L. (1986). The Stratigraphy of Mars. J. Geophys. Res., Seventeenth Lunar and Planetary Science Conference Part 1, 91(B13), E139–E158, doi:10.1029/JB091iB13p0E139. http://adsabs.harvard.edu/full/1986LPSC...17..139T.
- Hartmann, W.K.; Neukum, G. (2001). Cratering Chronology and Evolution of Mars. In Chronology and Evolution of Mars, Kallenbach, R. et al. Eds., Space Science Reviews, 96: 105–164.
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