Honey, I Shrunk the Face...!
By Richard C. Hoagland
1998 The Enterprise Mission
On April 5, 1998, NASA, JPL, and Dr. Michael Malin, Principle Investigator
for imaging on the Mars Global Surveyor spacecraft, collaborated in the
first major effort since the Viking missions to secure a new image of
the Cydonia Mensae region of the planet. This site has been the center
of a controversy which has simmered for over a generation: did NASA, over
20 years ago, find -- and then ignore -- bonafide evidence of extraterrestrial
ruins ... right next door? The first of three scheduled image strips that
are supposed to answer that 20-year old question, after being taken Sunday
morning, was officially released by NASA 36 hours later -- Monday morning,
April 6.
Immediately, a major controversy erupted -- over both the extraordinarily
poor quality of this initial Mars Surveyor image of Cydonia, as well as
the technical history of the "raw" data underlying that new image; the
latest evidence being that the image released Monday might not be "raw
data" at all--
But in fact, a second generation, reduced-resolution copy
of the original Mars Surveyor "Mars Orbiter Camera" Cydonia photograph!
The Mars Orbiter Camera -- above], according
to data published by the camera's Principal Investigator, Dr. Michael
Malin, in its "narrow-angle mode" is composed of a single line of detectors
-- a "2048 Element Line Scan CCD Array." The Camera produces images by
electronically "cross-track sampling" the array, while the physical motion
of the spacecraft around the planet moves the entire line of detectors
over the Martian surface at right angles to that scan [left].
Inevitably, each individual CCD element in such an array
possesses slightly varying sensitivity compared to its neighboring elements,
across the width of the detector. Thus, any image produced by the "line-scan
CCD array" will inevitably display a series of irregularly-spaced, vertical
bright and dark lines -- like scratches on an old print of "Casablanca"
-- stretching the length of the entire image at right angles to the scan
(below).
Normally, these vertical irregularities are removed from
the final image by appropriate computer processing; however, in "raw"
or incompletely processed images, these "lines" can serve as unique "detector
fingerprints" of that particular CCD array; no two line-scan cameras will
imprint the same spacing, intensity, or number of such lines on any of
its images. Thus, like matching bullet markings in a murder investigation
through a "ballistics test," comparing lines on various CCD line-scan
camera images can uniquely determine crucial aspects of those images --
including which camera took which image.
The idea of using this intrinsic "flaw" in line-scan CCD
cameras specifically to check on the current Cydonia photography, came
to our attention during a recent Art Bell show; we were engaged in a discussion
of the execrable photometric quality of the "raw" (and later, "enhanced")
versions of the Cydonia imagery, when it occurred to me that the CCD imperfections
inevitably present in CCD line-scan cameras could be used as a means of
verifying the ultimate source of all images taken with the Mars Surveyor
camera.
The next day a listener (Fred Hoddick), acting on our conversation
about these "CCD idiosyncracies" (as applied to Dr. Malin's camera), began
a serious investigation of the earlier Mars Surveyor imagery archived
on Dr. Malin's Website [link to Malin's Website]. His results, sent to
Enterprise for verification, can only be described as "startling."
Fred Hoddick discovered that, indeed, Dr. Malin's Narrow-Angle
Mars Orbiter Camera imprints a unique "line-scan fingerprint"on every
Mars Surveyor photograph; one such image he investigated -- "MOC568174924.8003"
-- was acquired by the Mars Surveyor spacecraft on orbit 80: a close-up
section of the spectacular "Vallis Marineris,' the so-called "Grand Canyon
of Mars." In comparing the "line-scan signature" visible in narrow-angle
image "8003" with the pattern of faint lines seen in the "raw" version
of the MGS Cydonia image "22003" (see close-up comparisons, below), Hoddick
indeed made a major, startling discovery--
That the spatial dimensions of the Mars Surveyor image
of Cydonia released by JPL are only half of what should have been acquired!
By following the green lines in the diagram and the "image
slice" comparisons with earlier MGS frame "8003" (above), it can easily
be seen that the final display-resolution of the so-called "raw" Cydonia
image "22003" is only half what should have been acquired; the documentation
supplied with Dr. Malin's camera (see above) clearly states that the full
resolution of a Narrow-Angle frame is supposed to be--
2048 picture elements wide.
Thus, the "raw" frame displayed on all the NASA Websites only presents
half the spatial resolution data apparently originally imaged by the camera
... radically reducing our ability to detect (if not unambiguously identify!)
any artificial sub-structures present in the image.
When this blatant spatial "image tampering" is added to
the extremely limited grey scale presented in the same MGS "raw" image
(see graphic, right) -- which demonstrates that only about 42 grey values
are represented out of a possible 256 -- the result is an extremely "noisy"
imaging enhancement (right-hand strip). Because of the "morning light"
aspect of this MGS Cydonia photography (as compared to the "late afternoon"
lighting of the original Viking Cydonia images), this reduced number of
grey levels further distorts the "raw" Mars Surveyor Cydonia image ...
without a great deal of effort, effectively eliminating meaningful comparisons
with the previous Viking data. This comparison is further hampered by
NASA's choice of the spacecraft imaging angle -- oblique -- as opposed
to Viking's overhead "frontal" view (below).
Finally, NASA's curious 1st choice of imaging enhancement tools for this
bland image -- "High-Pass filtering -- effectively eliminated almost all
remaining "grey scale information" in this initial Surveyor picture of
Cydonia -- reducing NASA's first version of "the Face" from Mars Surveyor
to a black and white "cartoon" ... what Art Bell termed whimsically (and
somewhat presciently ...) "the Catbox image."
No wonder Dan Rather, after one look Monday afternoon,
pronounced it "just another hill ... case closed!"
Michael
Malin's response to the posting of our "mysteriously reduced-resolution"
discovery came quickly:
Mars Global Surveyor Mars Orbiter Camera
Why is the image of Cydonia only 1024 pixels wide?
This question has been asked a great deal over the past few
days. The field-of-view of the MOC is 0.44 , and at the range of the
Cydonia image, this translated to about 3.1 km (1.9 miles). The viewing
angle was about 45 , so the projected width of the field was about 4.4
km (3 mi). The narrow angle detector is 2048 pixels across, so the intrinsic
resolution was about 2.1 m/pixel. The maximum images size (in bytes)
is 9.8 MBytes, or 2048 X 4800 pixels. At 2.1 m/pixel, this permitted
a down-track field of view of 11 km. Considering the uncertainties in
pointing of the spacecraft, this 11 km downtrack dimension was considered
insufficient to insure a reasonable chance of hitting the target.
There are two ways of extending the downtrack dimension.
First, we can use "lossless" compression to extend the distance by a
factor of about 1.8. We do this with most of the MOC images. However,
losses within the communication system occasionally create black bands
(accounting for the loss of about 7-15% of the data) through the images.
The MGS Project felt such losses would not be tolerable in the Cydonia
images. The second way to increase downtrack dimension is to decrease
resolution. If you sum the pixels two by two (that is, replace four
pixels--two across by two down--with the average of the four), you can
extend the image downtrack by a factor of four. This then changes the
dimensions of the image from 2048 X 4800 to 1024 X 9600, and the images
covers the same 4.8 km width but extends somewhat over 44 km downtrack.
The resolution is lower (4.3 m/pixel vs. 2.1 m/pixel), but the image
covers much more ground.
Since this resolution was still substantially better
than the best Viking image (by about a factor of ten), the Project decided
this was the best compromise in coverage and protection against data
loss.
Nice try, Michael -- but no cigar.
After Malin's "response," I spoke with Dr.
Thomas Van Flandern, former Head of the Celestial Mechanics Branch
of the U.S. Naval Observatory, and a world authority on orbital mechanics.
He confirmed my own impressions regarding NASA's main difficulties in
its attempted "targeted Mars observations": that the primary navigation
problem in securing Mars Surveyor re-imaging of Cydonia (as well as that
of Vikings 1&2, and Mars Pathfinder) was "cross-track" (east/west) error,
not uncertainties in "downtrack" (north/ south) spacecraft positioning.
This was due to the MGS discovery (during the attempted rephotography
of Viking) of east/west errors in the map positioning of Mars' "prime
meridian" of up to 10 miles!
Thus, to extend the downrange "footprint" of Surveyor's
imaging, from slightly under 7 miles to 26 miles, in an ostensible effort
to guarantee successfully re-imaging "the Face" -- but at the cost of
cutting the surface resolution in the Camera in half -- simply doesn't
make sense; by NASA's own acknowledgments, the primary uncertainty in
knowing the location of the targets was at right angles to this "increased
imaging footprint." For a north/south, polar orbiting spacecraft such
as MGS, increasing the "downrange" imaging would have zero effect on the
(acknowledged) major cross-track (east/west) errors.
(Such a strategy, however, would make sense if you wanted
to decrease the odds of actually recognizing something "interesting" in
your field of view ... if you succeeded.)
And the spectacular success of the JPL Navigation Team confirms this:
after all of Malin's "explanation," the actual location of "the Face"
in the image JPL released (right) is almost dead center of the "downrange"
footprint, and just left of the east/west "cross-track." (In the words
of one of Malin's own associates on Monday afternoon: "We nailed it!")
And other "nagging inconsistencies" also remain ...
If "trading off" imaging resolution for a larger photographic
footprint was a deliberate pre-Cydonia strategy reached by the entire
Project ... why didn't anyone at NASA (including Michael Malin) tell us
before the Cydonia attempt?; why did they wait to offer an explanation
for this "surprise" ... until after we discovered it?
This pattern of grudgingly responding to "anomalous details"
surrounding the Cydonia rephotography -- and only after they've been pointed
out -- is not only increasingly suspicious ... it is highly uncharacteristic
of prior NASA behavior as a whole; NASA used to be the one government
agency which apparently loved releasing "truck loads" of details about
its most arcane activities (some reporters complained, especially during
Apollo, about too much detail): everything from the weight of the crawler
which carried the Saturn V rocket to the launch pad ... to what the astronauts
ate for breakfast ... two days before the launch!
But on the rephotography of Cydonia, NASA's usually copious
flood of technical detail has mysteriously dried up ...
Responding to the major criticisms that greeted the first
"raw" Cydonia image -- that it simply was too dark -- Dr. Malin posted
on his Website (but only after we had presented our histogram analysis
-- above) his own assessment, data claiming that the MGS raw image in
fact "wasn't all that dark ..."; Malin attempted to compare [link to Malin's
Website] the new MOC data of Cydonia with the 22 year-old Viking image
histograms, insisting that in truth "the MOC data actually have more grey
levels than the Viking images ..." There is only one small problem with
Dr. Malin's analysis--
In order to support his claim, Malin had to compare "apples
and oranges": the raw "high-sun angle" MOC "morning light" image (22003)
to the raw "low-sun angle" 35 A series of Cydonia images from Viking.
And the sun-angle difference between the Viking imagery he used and Mars
Surveyor's image ... is almost a factor of three lower..!
The Viking image Malin chose to highlight (35A70) was taken
just before local "Martian sunset" -- with long shadows (~10 degrees),
of an intrinsically dark, relatively contrastless scene; in stark contrast
(pun intended ...), the raw Mars Surveyor Cydonia "strip image" was taken
at about 10:00AM "local Cydonia time" -- with a sun-angle comparable to
the high-sun angle (~30 degrees) of the 70A series of raw Viking frames
... which (although he published a revealing histogram
from 70A13) Dr. Malin for some reason conspiciously chose not to focus
on ...
A simple comparison tells why: the visual scene brightness between the
two equally-lit images (see right) reveals an apparently completely different
scene; the
raw Viking image is clearly -- even to the naked eye -- much brighter,
and has far more crucial contrast, than the Mars Surveyor record of the
same scene 22 years later, with ostensibly a far better privately-developed
camera!
The difference is literally "night and
day!"
The histogram comparisons reveal the numbers behind this startling comparison
(left); not only are there simply more shades of grey in the image taken
with the "primitive," 20-year old "vidicon tube" TV technology of Viking
(with the sun at essentially the same elevation angle above the horizon!),
but you don't even need a computer to measure it--
Just look!
Another of the "Malin explanations" for why the Mars Surveyor
image is so dark was "Martian weather."
After initially
writing"... fortuitously, the area imaged was relatively clear," he
then immediately contradicted himself by also stating "the low contrast
of the raw MOC high resolution image ... suggests haze or fog over much
of the area."
Of the two main problems with this explanation, the first can be seen
in the simultaneous wide-angle, color MGS image that was taken of the
larger Cydonia region that same morning (right). The intrinsic brightness
of this image -- which is caused by well-known "Lambert scattering" from
clouds and haze -- belies the anomalous "darkness" of the "raw" Cydonia
high-resolution frame (outline).
The second problem with MOC 22003, given this wide-angle
confirmation of at least some haze over Cydonia that morning, is the fact
that the 2048 Narrow Angle Camera CCD detectors (see Camera graphic --
above) have a spectral (color) sensitivity from about 5000 Angstroms (green
light) to below 9000 Angstroms (in the infrared). Infrared radiation effectively
cuts through haze--
So ...
Why was the long-awaited April 5 Mars Surveyor image
of Cydonia so damned dark -- compared to a much more primitive Viking
television image of 20 years ago ... 70A13?!
All this notwithstanding, we are left with a growing suspicion:
that this first Mars Surveyor, extremely poor quality, Cydonia image ...
might not in fact be all that "raw"...
One of the main problems with accepting NASA's assertion
that it is, is the growing litany of "ad hoc" explanations NASA has offered
after the fact for increasing numbers of technical discrepancies we have
discovered and documented with this image -- such as Dr. Malin's somewhat
tortured description (above) for why "lossless compression" wasn't used
this time within his camera, because of a possible loss of between "7
and 15% of the data ..." But, instead, a certain, 400% reduction in total
surface resolution was somehow deemed "acceptable."
What, prey tell, is the relationship between applying a
"lossless" compression algorithm in the camera on-board Mars Surveyor
... and experiencing an overall spacraft "communications loss?"; how does
reducing image resolution (as a substitute for this on-board "lossless"
data compression) thereby reduce those "losses within the communication
system [that] occasionally create black bands ..?"
And doesn't reducing overall data acquisition by a certain
400 percent (the effect of the 4-to-1 pixel averaging described by Dr.
Malin!) seem a disproportionate response to a potential communications
problem which might result in losing a mere " 7-15%?"
(Incidentally, I presume these pesky MGS "communications
losses" are in the transmission of the imaging data to Earth, not some
internal spacecraft problem between systems. If that is, indeed, the case,
in every previous planetary mission I have ever known, losses in telemetry
to Earth have been made up by either redundant error-correcting codes,
or, by simply retransmitting the same data a second time. And, even if
the problem is internal, with no other data in the camera buffer for April
5 except the Cydonia image, why couldn't Dr. Malin simply have retransmitted
the same image later ... thus making up for any losses in the first transmission?
As far back as I can remember, such redundant procedures have been standard
on all previous NASA planetary missions.)
And finally, there is the little matter of the "corrected
caption" on JPL's own Website.
CYDONIA PHOTO CAPTION
as stated on: Mon 04/06/98 10:30 AM PDT Image dimensions:
1024 X 19200 pixels, 4.42 km X 82.94 km
This was a typographical error for which we appologize
[sic].
Actual image dimensions: 1024 X 9600 pixels, 4.42 km
X 41.5 km
Somehow, it's hard to imagine anyone typing "19200" in
place of "9600" -- even in a government contracted typing pool at JPL.
But--
If the original transmitted imaging resolution from Dr.
Malin's camera was 2048 pixels across, subsequently "downsized" on Earth
to 1024, then the corresponding "downtrack" dimension would have been
precisely 19200 pixels -- exactly what the original NASA caption read
... exactly consistent with our discovery that "MOC 22003" is somehow
missing 400 percent of its expected resolution.
The only question remaining: was the resolution deliberately
"traded off" at Mars in Dr. Malin's camera (as he claims), or was it quietly
reduced in the production of a second generation copy -- the impossibly
bad "raw" image we were given Monday -- of the original, high-quality
2048 X 19200 image ... here on Earth?
Several hours after the JPL release of the "raw" Cydonia MGS
image, and several additional hours after the release of the "enhanced"
("Catbox") version that the media all took one look at ... and totally
dismissed--
A new Cydonia image suddenly appeared on all the NASA Websites
-- termed the "TJP
Enhancement".
Presented by a NASA geologist officially attached to the
Mars Pathfinder mission, this enhancement by Tim Parker was a staggering
improvement over JPL's first "high-pass filter" version. Unfortunately,
by the time Mr. Parker's partially rectified, grey-scale corrected version
-- confirming a startling "face-like" image at Cydonia -- was posted on
NASA's
official Websites all around the world.... no one in the media was
listening (or, apparently, even watching NASA's Websites).
Where did this remarkable "new" Cydonia image come from?
Was it merely another "enhancement" of the previous "raw" image released
that morning (as Parker insisted in his own "enhancement notes" accompanying
the image) ... or, was it drawn from data much closer to what Mars Surveyor
actually transmitted back to earth?
We may never know.
Which only underscores the point I've been attempting to
illustrate all week:
That, without appropriate and meticulous documentation
of the entire process -- from taking the photographs at Mars, to receiving,
enhancing and displaying them back here on Earth -- no one can make a
scientific assessment of what's waiting at Cydonia ... In terms of Mars
Surveyor, judging from our experience this week, we are still "light years"
from gaining access to such crucial, verifiable documentation.
So far, unlike any other area of Science, on the subject
of potential Life on Mars we're simply being asked by NASA (and its contractors)
"take our word ..."
When I was at CBS, covering Apollo, a correspondent in our unit
once wise-cracked in frustration that, " NASA' simply means Never A Straight
Answer ..."
I guess it still applies.
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