Thanks, Luis.
Yes. The layout of the features on the Moon, as seen in projection in
the sky, is completely determined by the date, time and location of
the observation.
Identifying any two points, ideally as widely spaced as possible,
defines the rotation and magnification of your image; and once those
two points have been located, the expected locations of all others
(such as "M5" and the LCROSS impact targets) are known relative to
them.
For LTVT to make a successful "calibration" it needs valid data in the
lon/lat and x/y (pixel) boxes for the two points. Usually this is
done by clicking on images, but it is possible to enter the data
manually.
For example, for the south pole image you recently uploaded
(MARTINEZ20090401+0432UT+SOUTH+POLE.jpg) the points I identified were
lon=41.957 lat=-84.283 (a small crater on Leibnitz Beta) at x=258
y=176, and lon=36.686 lat=-51.266 (the small crater Vlacq K) at x=594
y=385. If you copy this information into the boxes (along with the
correct date and location information) your will get the same
calibration. These points were taken from the special "dot file" of
control points in "1994 ULCN Supplement v2.csv" at:
http://ltvt.wikispaces.com/dot+files
The error message you are getting sounds like you may be clicking on
pixel locations without *first* entering the lon/lat of the point you
are clicking on. When you click on the second point LTVT checks to
make sure that it differs from the first point in *both* lon/lat and x/
y location. If they aren't different points LTVT can't determine the
scale and rotation of the image.
If you are using control points copied from the main screen, it helps
greatly to have a good set of reference images to know what those
points look like under a variety of lighting conditions. There is an
increasing set of links to full disk images suitable for this purpose
at:
http://ltvt.wikispaces.com/Calibrated+Full+Disk+Images
and you can add some (or all) of these to the set of calibrated images
on your hard drive. There is also a new "Clementine Basemap V2" and a
Lunar Orbiter map available at Map-a-Planet, which you can download as
texture files:
http://ltvt.wikispaces.com/Texture+Files
These have very good registration, and if you can recognize a feature
that appears on your photos in them, you can set the "reference point"
on that feature (with a right-click of the mouse) and copy its lon/lat
as a control point for the calibration.
After you download these files, you use the Files...Change External
File Associations... menu:
http://ltvt.wikispaces.com/File+Associations+Menu
to use them for the display. You also use it to display special dot
files, such as the one mentioned above.
-- Jim
> LTVT_Image 04012009 south pole.bmp
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