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originally posted by: Phage
a reply to: gortex
Au Contrair. Just give us a couple of centuries.
originally posted by: wildespace
For the record, the Very Large Telescope in Chile has 4 times the resolution of the Hubble Telescope (8 meters versus 2). Granted, it's not positioned in space to avoid atmospheric disturbances, but it manages to counter them using a sophisticated system of adaptive optics and interferometry.
VLT could probably produce a better image of Mars than the Hubble.
You can now officially call me the resident party-pooper!
originally posted by: smurfy
a reply to: gortex
NASA sure has pulled out the stops in the treatment of these images. The blue is more vivid, the brown/red has more shades, even a little more blue to white of the clouds covering the brown surface and it could almost be looking at Earth with Africa peeking through. 'Only' missing in the illusion is the deep blue where there is no land, just water. Don't you just wish?
This image is a composite of separate exposures acquired by the WFC3/UVIS instrument. Several filters were used to sample various wavelengths. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:
F275W (275nm) purple
F410M (410nm) blue
F502N (502nm) green
F673N (673nm) red
We propose to observe Mars near opposition, which occurs on 22 May 2016, to obtain WFC3/UVIS multi-color imaging. Mars will be near the Earth evenly illuminated by the Sun, which is ideal for our observations. It will also be easily visible to the public in the nighttime sky. At opposition, Mars will be at a distance of 0.51 AU, and its disk will subtend a diameter of 18.4 arcsec. Within our one HST orbit, we will sweep through a set of four WFC3 filters (F275W, F410M, F502N, F673N) several times each, and include a small dither shift, to mitigate cosmic rays and detector artifacts. Mars will easily fit within the 1K subarray, which will minimize CTE effects and allow us to obtain over 20 exposures per orbit. We hedge a bit with exposure timess for each filter, since it is difficult to know in advance which Mars features might be prominent at the time of the observation (e.g. polar caps, clouds). Exposure times will generally be short, but some may saturate in spots, and we also use post-flash for some of the shotest exposures. We obtained approval to specify BLADE=A for all exposures to mitigate shutter-driven vibrations. The Hubble Heritage team imaged Mars at opposition in 2007 with WFPC2 (HST program 11361). We used filters F410M, F502N, and F673N. In this proposal we have included a wide UV filter (F275W) which also does not require very long exposures times and could reveal interesting Martian cloud structure. Opposition will be near the end of the aphelion cloud belt season, which was originally discovered using HST. We would like to schedule this observation a week or so before the opposition date, so the public release can coincide with the opposition.
And you would know this for certain? Non intervention by us? Non intervention by, anyone?
originally posted by: gortex
a reply to: bobs_uruncle
It's natural Mars, no intervention from us.
originally posted by: wildespace
originally posted by: smurfy
a reply to: gortex
NASA sure has pulled out the stops in the treatment of these images. The blue is more vivid, the brown/red has more shades, even a little more blue to white of the clouds covering the brown surface and it could almost be looking at Earth with Africa peeking through. 'Only' missing in the illusion is the deep blue where there is no land, just water. Don't you just wish?
It's not strictly a true-colour image. The Hubble used four filters for this, including violet and UV.
This image is a composite of separate exposures acquired by the WFC3/UVIS instrument. Several filters were used to sample various wavelengths. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:
F275W (275nm) purple
F410M (410nm) blue
F502N (502nm) green
F673N (673nm) red
I think the clouds appear so bright and vivid here because they reflect lots of UV back from the Sun.
~~~
In case anyone's interested, here's the official proposal for taking this image: www.stsci.edu...
We propose to observe Mars near opposition, which occurs on 22 May 2016, to obtain WFC3/UVIS multi-color imaging. Mars will be near the Earth evenly illuminated by the Sun, which is ideal for our observations. It will also be easily visible to the public in the nighttime sky. At opposition, Mars will be at a distance of 0.51 AU, and its disk will subtend a diameter of 18.4 arcsec. Within our one HST orbit, we will sweep through a set of four WFC3 filters (F275W, F410M, F502N, F673N) several times each, and include a small dither shift, to mitigate cosmic rays and detector artifacts. Mars will easily fit within the 1K subarray, which will minimize CTE effects and allow us to obtain over 20 exposures per orbit. We hedge a bit with exposure timess for each filter, since it is difficult to know in advance which Mars features might be prominent at the time of the observation (e.g. polar caps, clouds). Exposure times will generally be short, but some may saturate in spots, and we also use post-flash for some of the shotest exposures. We obtained approval to specify BLADE=A for all exposures to mitigate shutter-driven vibrations. The Hubble Heritage team imaged Mars at opposition in 2007 with WFPC2 (HST program 11361). We used filters F410M, F502N, and F673N. In this proposal we have included a wide UV filter (F275W) which also does not require very long exposures times and could reveal interesting Martian cloud structure. Opposition will be near the end of the aphelion cloud belt season, which was originally discovered using HST. We would like to schedule this observation a week or so before the opposition date, so the public release can coincide with the opposition.
originally posted by: OneBigMonkeyToo
a reply to: Aliensun
No-one has said you can't, it's just you can't get high resolution close ups with it. Using Hubble to get high resolution images of nearby objects is like trying to watch your living room TV through binoculars.
originally posted by: Phage
a reply to: Aliensun
I remember when the officials said that the Hubble could not image Mars or the Moon.
I don't remember that. In fact there are a couple of Hubble image of the Moon in an article from 2005.
Now, the U.S. is planning another pioneering journey, this time to the moon and beyond. To prepare, NASA scientists are using the Hubble Space Telescope to hunt for resources, such as oxygen, that are essential for people to survive and to sustain their existence on the lunar surface. Hubble's preliminary observations and results are promising.
www.nasa.gov...
Mars:1999
Or, to simplify:
heritage.stsci.edu...
originally posted by: OneBigMonkeyToo
a reply to: MysterX
As a Brit I also don't care about NASA, however you made a claim stating that NASA said it couldn't image the Moon in the late 1990's and I do care about accuracy and truth.
I could actually be bothered to check that and found photos of the moon taken by Hubble in the late 1990s.
What you remember NASA saying they could do and what NASA actually did are two different things. If you want to prove that you aren't going senile in your old age, I'd check through all the stuff you think you have stored.
I remember the NASA replies of the late 90's, early 2000's consisting of "Hubble cannot image Lunar, as the albedo or reflectivity of the moons surface, would damage Hubble's sensitive imaging subsystems as it is too bright.