The Fast
and Easy Image Suggestion Tutorial
If you want to suggest a
target area on Mars for HiRISE, but you want to let the scientists decide on
the "extras", like the time of year that the image is taken, you can use this
tutorial to walk you through it.
If you have more time and want to use all of the advanced features of
the Image Suggestion site, go here. The fast and easy tutorial will take you
through all of the basics you need to get started finding and suggesting areas
on Mars for HiRISE to image. Now let's get started!
(Also on this page you can select different maps to
view this region. You may
experiment with this if you like.
If you click on the "MOC/THEMIS" button at the upper left, it will allow
to you see the more detailed images from MOC
or THEMIS. You do not need to use this
to suggest a site, but if you want to check it out, go here for more information.)
Here is a brief description
of what each of these scientific areas cover. Click on the term to go to a link with more information
about the scientific theme.
v Climate Change: any features, deposits or landforms indicative of changing climatic
regimes.
v Eolian Processes: refers to features or processes involving wind erosion or
deposition. Examples include:
dunes, wind streaks, dust devils.
v Fluvial
Processes: refers to surface and
subsurface water flow processes involving the formation and subsequent
development of channels, rivers or streams and the valley systems in which they
flow or once flowed. Water is
critical for life as we know it, so the presence of water in streams or gullies
on Mars suggests that there was water on the surface of Mars at one point. Persistent surface and subsurface water
flow could have potentially created habitable regions in the planet's past.
v Future Exploration/Landing Sites: Understanding past landing sites from orbit or to
target areas of potential future landing sites for further study.
v Geologic
Contacts/Stratigraphy: refers to the description, correlation,
classification of stratigraphic layers and their depositional environments.
Also refers to the geologic boundaries between two different layers, surface
units, materials, or features.
v Glacial Processes: refers to the landforms, features and materials produced
by glacial or ice sheet activity. Examples include: moraines, eskers, kettles,
kames.
v Hydrothermal
Processes: refers to processes
involving hot ( or above ambient temperature) water at or near the
surface. Many hydrothermal areas
have been heated by hot magma bodies beneath the surface of the planet, such as
the hot springs in Yellowstone National Park on Earth. There may have been significant
hydrothermal activity near the volcanoes or impact craters on Mars in the
past.
v Impact Processes: refers to the processes involved in meteorite impacts and the
subsequent formation of impact craters and basins and related features to the surface
of the planet.
v Landscape
Evolution: different landforms
and processes that affect the overall changes in a region's or landscape's
shape and elevation over time. Many of the features on Mars look similar to
those seen on Earth, but many are quite different. Understanding the origin of the unusual features can tell us
about the history of the planet.
v Mass Wasting
Processes: refers to the movement of sediment and rock material
downslope by gravitational forces.
Downslope movement may be slow as in creep and solifluction or may be
rapid as in landslides, rockfalls, rockslides and debris flows.
v Periglacial Processes: refers to landforms or features that form at the
margins of former and existing ice sheets and glaciers. Environments where
frost action is important and induced by a periglacial climate beyond the
margin of an ice sheet. Such
landforms include: pingos, polygons, and a variety of patterned ground.
v Polar
Geology: (detailed version) studies of the polar
caps. Understanding the polar caps
on Mars can help us better understand past climate changes on Mars.
v Seasonal Processes: refers to any processes, landforms or features that
change with the season. Examples
include: the sublimation of the polar ice caps, presence of seasonal frosts,
landforms or features that change shape, color or are present with the season.
v Sedimentary/Layering
Processes: refers to the
deposition or erosion of sediment layers in lakes or oceans, layers formed by
deposition of ash from volcanic eruptions or layers from cyclic changes in the
amount of dust in the atmosphere.
v Surface Properties: refers to understanding the physical and chemical
composition of the surface. For example: the nature and abundance of rocks on
the surface and the materials that comprise the surface.
v Tectonic
Processes: refers to deformation of the planets surface into
fractures, lineaments, grabens and faults caused compression, shearing or
expansion of the planet's crust by volcanic, impact or sedimentary processes.
v Volcanic
Processes: (detailed version) refers to the processes
involved in volcano formation and lava emplacement on the surface of the
planet. Much of Mars is covered in
volcanic rocks, and ancient lava flows can be observed over much of the planet. Volcanoes also greatly affect the
atmosphere due to the eruption of gasses, and this could have had a large
impact on past climate.
(You
can leave the rest of the parameters at the defaults and a scientist will
select the appropriate parameters if the site is selected. If you want to learn more about
modifying the parameters, go to the Advanced Tutorial here.)