Recent Volcanic
and Fluvial Activity in the Region of Harmakhis Vallis, Mars
Glamoclija, Mihaela1, Gian
Gabriele Ori2, Lucia Marinangeli2, Goro Komatsu3,
Jouko Raitala4 (1) Department of Geological Science, Indiana
University; and International School of Planetary Sciences, Università
d’Annunzio, Bloomington, IN (2) IRSPS, Pescara, Italy (3) Università
d’Annunzio, Pescara, Italy (4) University of Oulu, Oulu, Finland
Geologic mapping and geomorphic analyses
of Harmakhis Vallis in the eastern Hellas region (lat. -35˚
to –42˚S; lon. 91˚ to 98˚E) were conduced to distinguish and
characterize geologic units and processes that operated in the source region of
Harmakhis Vallis and its vicinity. Long and complex history of degradation and
modification involves mass wasting processes, volcanism and fluvial activity;
confronting effects of climate-induced slow mass-wasting processes with
temporary high geothermal variations caused by impact events and volcanism in
the area. Our analyses of currently available imagery from the area (Viking
imagery, MOLA altimetry, wide and narrow angle MOC images, THEMIS VIS and IR
(nighttime and daytime) images, HRSC: H0038, H0528 images, and stereo-derived
topography) revealed evidence for a recent geothermal excursion with small spatial
exposure. This recent, temporary, and a space-limited relatively high
geothermal anomaly was most likely caused by reactivation of volcanic sources
during the most recent history of the region. Its importance is not solely as
“a witness” of the recent hydrothermal activity resurged within last
approximately 400,000 years on the plain; but also to give support to more
detail researches of the Harmakhis Vallis region and other volcanic provinces
on Mars that may be of a high astrobiological interest.
Further analyses of new MOC narrow angle
images and incorporation of OMEGA data may provide information of the physical
and chemical properties of the surface material to further refine knowledge of
types, distribution, and origin of geologic units in the area.