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Originally posted by zorgon
Well if that was true about the lower gravity and the thinner atmosphere... then the same would apply on the Moon even more so because it supposedly has less gravity that Mars and an even thinner atmosphere...
So we should see dust floating around the Lunar atmosphere for long periods of time as well, by that logic, should we not?
We use what we want to, and when I have to write in English I prefer the real English to its "lite" version.
Originally posted by zorgon
Ah well here in America we say skeptic and true color.. I wasn't aware that Portugal used Queen's English
On a clear day (meaning a dust free atmosphere) I think I would see a blueish sky, but judging by the photos I don't know if it would be a darker blue or a lighter blue, seeing that in some photos the sky looks white.
So what colour do you think the Martian sky looks like if you were standing on Mars on a clear day at noon? And would that be a 'true colour' or a 'false colour'
No, I see I wasn't clear.
Originally posted by zorgon
Well if that was true about the lower gravity and the thinner atmosphere... then the same would apply on the Moon even more so because it supposedly has less gravity that Mars and an even thinner atmosphere...
No, because of what I said above and because there isn't a easy way to get the Moon dust high enough, there are no strong winds on the Moon and there is no other way (that we know) to send the dust that high.
So we should see dust floating around the Lunar atmosphere for long periods of time as well, by that logic, should we not?
So I am not sure why so many are having issues understanding this
Panchromatic (nm) 675±90 -Nadir, 2 stereo, 2 photometric
Near-IR (nm) 970±45
Red (nm) 750±20
Green (nm) 530±45
Blue (nm) 440±45
Left camera:
Empty slot (sharpest)
L1 750 nm (Near IR/ Red Stereo L)
L2 670 nm (Deep red - Geology)
L3 600 nm (CCD Pickup Red)
L4 530 nm (CCD Pickup Green)
L5 480 nm (CCD Pickup Blue)
L6 430 nm high pass (UV/ Blue Stereo L)
L7 440 nm + Solar Neutral Density
Right camera:
R1 430 nm high-pass (Near UV/ Blue Stereo R)
R2 750 nm (Near IR/ Red Stereo R)
R3 800 nm (Near IR - Geology)
R4 860 nm (IR - Geology)
R5 900 nm (IR - Geology)
R6 930 nm (Far IR - Geology)
R7 980 nm low pass (Far IR - Geology)
R8 880 nm + Solar Neutral Density
Originally posted by zorgon
Originally posted by thesneakiod
Nice. Why though do NASA portray mars as a red planet?
Dunno Same reason NASA colors Venus in a bright 'lava orange'?
The older viking images were correct... so why the change to 'NASA red'
edit on 18-11-2010 by zorgon because: No way am I filling this out
Originally posted by ArMaP
Originally posted by DJW001
Given that Mars' atmosphere is much thinner than Earth's, I would expect that it would be dark purple-blue overhead with a permanent reddish tinge around the horizon where the light passes through more of the atmosphere. Think twilight in Los Angeles.
Originally posted by ArMaP
OK, let's see if with some pictures I can explain better what I said before.
These are the photos used to create the colour version of that image.
For the red channel.
For the green channel, taken 143 seconds after.
For the blue channel, taken 135 seconds after the previous photo and 278 seconds after the first.
(All images are bigger than they appear here, click for full size)
In the first (red) photo there is nothing visible on that area where we can see the green dust (or whatever), but in the second photo (green) we can see what looks like a wide dust-devil. In the third photo we can see that the dust-devil has moved to the left, and looks fainter than in the previous photo, so it was probably loosing energy and disappearing at the time.
As anyone that knows how these RGB images are created knows, something that appears only in one of the images will appear in the final image as being of the colour for the channel in which the object was visible, so the joining of these three images should show a green dust-devil at the middle of the image and a fainter blue dust-devil to the left, and that is what we see.
This is the final result of using the above images to make a colour version.
(Click for full size)
Although faint, it's visible that there is a blue "mist" to the left of the green "swamp gas", as predicted by what was visible on the greyscale images.
That is why I think that this is really an image artefact and not a green dust, mist or gas, it's just the result of how these images are made.
PS: yes, that's a blue sky, before someone asks.
These are the radiometrically corrected images, they give much better looking results.
Originally posted by Krusty the Klown
I notice that that the Martian sky is blue in these two images..... is that normal?
An angry looking sky is captured in a movie clip consisting of 10 frames taken by the Surface Stereo Imager on NASA's Phoenix Mars Lander. The clip accelerates the motion. The images were take around 3 a.m. local solar time at the Phoenix site during Sol 95 (Aug. 30), the 95th Martian day since landing. The swirling clouds may be moving generally in a westward direction over the lander.
This sequence combines 32 images of clouds moving eastward across a Martian horizon. The Surface Stereo Imager on NASA's Phoenix Mars Lander took this set of images on Sept. 18, 2008, during early afternoon hours of the 113th Martian day of the mission. The view is toward the north. The actual elapsed time between the first image and the last image is nearly half an hour. The numbers inset at lower left are the elapsed time, in seconds, after the first image of the sequence. The particles in the clouds are water-ice, as in cirrus clouds on Earth.