The appearance of part of this area in a natural color aerial
photo (somewhat overly red-brown in its printing) is seen in
here.
In the field, the same area is seen to consist of gentle rolling terrain covered sporadically by cedar and sagebrush;
in the satellite image this vegetation does not stand out as blotches of red suggesting that cedar has a weak reflectance response in the near-IR.
A published geologic map (Stringham and Brooke, 1962) of this
area indicates a wide variety of alteration types have developed
here. Their report states that mineralization consists of pyrite
and chalcopyrite (copper-bearing), the latter of insufficient
grade (amounts) to be minable. Alteration is confined to a group
of volcanic rocks called andesites which, after emplacement and
cooling, were subjected to volcanic gases and hot solutions that
modified some of the lava rocks. One alteration type is kaolinite,
a common clay mineral much sought after for ceramics, that is
light brownish-white at this location. A second light-gray mineral
is alunite, a hydrous potassium aluminum sulphate. The principal
alteration mineral is hematite, the anhydrous iron oxide, which
is a medium grayish red in color; minor amounts of limonite are
present but the yellow-brown color of the space image corresponds
mainly to altered hematite rather than the similar gossan. Very
white areas of siliceous sinter are scattered about and a few
areas actually contain native sulphur derived from the breakdown
of the original sulphides. In the ground based photograph above,
the light patch coincides with mainly a kaolinite-alunite (k/a)
mix and the reddish area is hematitic staining on weathered volcanics.
To appreciate their general distribution in this subscene, examine
the map below, a simplified version of the published map, itself
too detailed to reproduce well on this Web Page. This map can
be printed out with your Web Browser for ease of reference in
studying the images below.
We will now peruse a set of images prepared to illustrate how
remote sensing data can be applied effectively in mineral exploration.
Suppose, to start, that you are a modern-day prospector searching
for some metal (gold is the obvious choice but copper is often
the more likely find). If you had chosen a large region in which
to hunt, you would be grateful for Landsat imagery that encompasses
many thousands of square miles. Even in a full scene, the anomalous
color in the White Mountain area (as this alteration district
is known by) would grab your attention because it is typical of
a gossan signature. Your first logical step would be to zoom in
on your image processor to the immediate area showing this signature
in a natural color (bands 1-3) rendition. Dark areas in the subscene
relate mainly to the volcanics. On the left side, the map shows
these to be basalts (an almost blackish rock typical of Hawaiian
volcanism and of the Snake River volcanic plains of Idaho); those
at the top and bottom are somewhat lighter (but still dark grayish-brown)
andesites (typical of volcanoes in the western U.S. such as Mt.
St. Helens). White Mountain stands out on the right in light bluish-gray
tones; it contains a radial pattern that corresponds to furrowed
gullies draining down from its central peak. The main alteration
zones make up a pattern with an E-W branch that meets a N-S segment
on the left. Most of this alteration is displayed in the yellow-browns
seen in the regional subscene. Other zones are much lighter (sort
of tan) in this image. These two principal zonal types broadly
match the hematite and k/a areas on the generalized map shown
above. Areas on that map identified as alluvium (soil and loose
surface debris) show up in several variant colors in the subscene.
Those with a color similar to the hematite are alluvial deposits
derived from the altered hematitic zones. (An equivalent subscene
made from bands 2,3,4 [not reproduced here] contains very little
discrete red patches, confirming the sparsity of active, reflectant
vegetation.)
Code 935, Goddard Space Flight Center, NASA
Written by: Nicholas M. Short, Sr. email: nmshort@epix.net
and
Jon Robinson email: Jon.W.Robinson.1@gsfc.nasa.gov
Webmaster: Bill Dickinson Jr. email: rstwebmaster@gsti.com
Web Production: Christiane Robinson, Terri Ho and Nannette Fekete
Updated: 1999.03.15.