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  #181 (permalink)  
Old 20-February-2006, 05:30 PM
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Quote:
Originally Posted by Jerry Jensen
This article:

http://www.lpi.usra.edu/meetings/lpsc2006/pdf/2192.pdf

Clearly shows that the probe penetrated (thick dust? a cobwebby surface?) in the first three frames, THEN struck a (harder? more resilient) surface that caused it to emit a bright UV flash - but contrary to first reports, this flash was dimmer than expected (!?).

Since it took roughly 125ms before the bright flash occurred, my hypothesis that the dust or surface layer is only 1-3 meters thick is certainly wrong, and even though the angle of impact was 20-40 degrees, the probe must have penetrated quite deeply before the bright flash occurred.

Fascinating structure!

Ok, so we have to revise the time between the early flash and the second flash to 123 msec. That means the projectile could have travelled another 1254.6 m before the dust plume started to emerge. Or do you think the delay time is consistent with "implosive, excavating and funnelling" action as claimed by the experts?

Cheers.

P.S. The images are unreadable by my computer software, any solutions?
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  #182 (permalink)  
Old 23-February-2006, 06:13 AM
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The experts are saying there is 'layering', which I would assume means that when you get a bright flash after burrowing for 125ms, there was some kind of change in density or resiliency. I can't argue with that. I guess we will never really know.

You are not missing much by not seeing the images, just three very dim spots of light prior to the flash.
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  #183 (permalink)  
Old 20-March-2006, 07:25 AM
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Some Lunar and Planetary Science Conference (LPSC) 2006 Deep Impact-talk documents (PDF format):

A DEEP IMPACT MISSION CONTRIBUTION TO THE INTERNAL STRUCTURE OF JUPITER FAMILY COMETARY NUCLEI: THE TALPS OR “LAYERED PILE” MODEL

Quote:
Based on this proposal, a structural model for the interior, called here the Talps or ‘layered pile’ model, is presented for typical Jupiter family comet nuclei that has an inner core transitioning to an outer mantle consisting of a sequence of thin, randomly stacked, layers, each of limited area and, possibly showing small differences in composition, out to the surface. As presented here this model predicts a correlation between the radial distance and the average thickness of the layers. As long as gravity plays a minor role large nuclei are expected to have thicker surface layers and vice versa.
DEEP IMPACT: THE FIRST SECOND

Quote:
These frames witnessed the beginning of the conical ejecta plume’s expansion. In addition, they caught the expansion of a cloud of incandescent, probably liquid silicate, droplets that sprayed away from the impact site.
TEMPEL 1: SURFACE PROCESSES AND THE ORIGIN OF SMOOTH TERRAINS

Quote:
Deep Impact spacecraft [1] obtained high resolution views (better than 10m/pxl) of some 30% of the surface of comet 9P/Tempel 1. The images reveal the nucleus to be a geologically complex body with a) prominent layering, possibly of global extent, b) widespread preservation of apparent impact scars, c) strong evidence of scarp retreat and a diversity of slope morphologies, d) extensive smooth terrains strongly suggestive of flow deposits.
ASYMMETRY OF GASEOUS CO2 AND H2O IN THE INNER COMA OF COMET TEMPEL 1

Quote:
The distribution of the gas in the inner coma was mapped and an asymmetry was found in both the CO2 and H2O. The CO2 is more prevalent in the southern coma, while the H2O is more prevalent in the sunward direction. The ratio of CO2 compared to H2O is over a factor of 2 larger in the southern, anti-sunward direction than in any other region. Further study of this asymmetry will give insight to the chemistry of the near-nucleus ambient coma as well as the anisotropic outgassing of the nucleus.
GRAVITY OR STRENGTH? AN INTERPRETATION OF THE DEEP IMPACT EXPERIMENT

Quote:
So, either gravity or strength craters can be consistent with the observations. Thus, the observations to date do not discern between the relative importance of strength and gravity in the DI event.
DEEP IMPACT: EXCAVATING COMET TEMPEL 1

Quote:
The preliminary analysis of the data has already lead to significant, new understanding of cometary properties and behavior and this talk will summarize the present state of our understanding with details of some results in related talks.
WATER ICE ON TEMPEL 1: BEFORE, DURING, AND AFTER THE IMPACT EVENT

Quote:
Water ice was detected and mapped in all three phases of observations. We present the identification, spatial distribution, and particle size of water ice and trace its path during impact and in relation to the comet’s structure.
Others at: LPSC 2006: SPECIAL SESSION: RESULTS FROM THE DEEP IMPACT MISSION
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  #184 (permalink)  
Old 04-April-2006, 06:12 PM
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The 250,000 Ton Punch

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Over the weekend of 9-10 July 2005 a team of UK and US scientists, led by Dr. Dick Willingale of the University of Leicester, used NASAE28099s Swift satellite to observe the collision of NASA's Deep Impact spacecraft with comet Tempel 1. The Swift observations show that the comet grew brighter and brighter in X-ray light after the impact, with the X-ray outburst lasting a total of 12 days.
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  #185 (permalink)  
Old 04-April-2006, 09:45 PM
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Quote:
Originally Posted by ToSeek
Quote:
"The Swift observations reveal that far more water was liberated and over a longer period than previously claimed," said Dick Willingale.
Also, just curious, why are there two x-ray peaks in their graph - rotation?
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  #186 (permalink)  
Old 05-April-2006, 10:01 AM
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Here is how this is reported on the BBC website

This extra water being given off, is it enough to change it's trajectory The told us this would be safe
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  #187 (permalink)  
Old 05-April-2006, 03:20 PM
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Quote:
Originally Posted by Sticks
Here is how this is reported on the BBC website

This extra water being given off, is it enough to change it's trajectory The told us this would be safe
By my reckoning, even the 250,000 metric tons of water is less than a billionth of the total mass of the comet. It shouldn't make a significant difference.
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  #188 (permalink)  
Old 05-April-2006, 04:11 PM
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I only mention this, because one of the ideas to steer rouge comets off of collision course was to use a large reflector to create a jet to nudge it onto a different heading.
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  #189 (permalink)  
Old 05-April-2006, 05:56 PM
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Quote:
Originally Posted by ToSeek
By my reckoning, even the 250,000 metric tons of water is less than a billionth of the total mass of the comet. It shouldn't make a significant difference.
And the 250000 tonnes total over the impact-related outburst duration, should be compared to the normal non-impacted rate of 16000 tonnes per day.

The 250,000 Ton Punch
Quote:
Tempel 1 is usually a rather dim, weak comet with a water production rate of 16,000 tonnes per day. However, after the Deep Impact probe hit the comet this rate increased to 40,000 tonnes per day over the period 5-10 days after impact. Over the duration of the outburst, the total mass of water released by the impact was 250,000 tonnes.
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  #190 (permalink)  
Old 06-April-2006, 04:45 AM
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Quote:
Originally Posted by ToSeek
After seeing the plots, this is quite an incredible claim: All there is, is a shift in the background, a shift that never returned to the original baseline. They are integrating all the noise in this background shift, and calling it Deep Impact water. There is not even a hint of a Gaussian distribution. Baseline shifts can be anything from and including the solar wind, to calibration errors, to a dustier environment that may or may not contain copious amounts of moisture.

From Sticks reference:
Quote:
"All this is supposition; all we know is that when we put in the numbers we seem to get an excess coming off of about two and a half times over the quiescent level."
No, they don't see anything "coming off", 'coming off' implies a rise, a distribution, a pattern, not a shift from the expected baseline.

Bad science!
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  #191 (permalink)  
Old 06-April-2006, 02:35 PM
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Quote:
Originally Posted by Jerry Jensen
After seeing the plots, this is quite an incredible claim: All there is, is a shift in the background, a shift that never returned to the original baseline. They are integrating all the noise in this background shift, and calling it Deep Impact water. There is not even a hint of a Gaussian distribution. Baseline shifts can be anything from and including the solar wind, to calibration errors, to a dustier environment that may or may not contain copious amounts of moisture.
I am curious why their graph shows two peaks. Is this to be expected? Is the valley due to a leeward orientation (in the shadow)?
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  #192 (permalink)  
Old 06-April-2006, 03:15 PM
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Quote:
Originally Posted by George
I am curious why their graph shows two peaks. Is this to be expected? Is the valley due to a leeward orientation (in the shadow)?
Good question - looking at the timing, the two peaks are both associated with the original plume. When I looked at the data, I assumed both of these peaks were picked up by other observers as well, because they are in the time frame very near to the impact. My guess is that as the heavier particles were pulled back by gravity, the lighter and gaseous elements became more exposed - the distribution should be more gaussian, but since the sampling times are hours apart, the true nature of the distribution is lost. If the conclusion of the Liecester scientists is based upon this second peak, and not the shift in the baseline, the conclusion is much more robust.

But if I am interpreting the articles correctly, they are doing a mole count in the baseline shift, AFTER the peaks desolved - they are integrating a much larger area than the initial (second) peak, and that is not valid. It is like measuring the grains of moisture in the air after a tyre burst, and saying "Oh, there is more moisture in the air now than there was before the tyre burst - that tyre must have been full of water."
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  #193 (permalink)  
Old 06-April-2006, 04:37 PM
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Quote:
Originally Posted by Jerry Jensen
...if I am interpreting the articles correctly, they are doing a mole count in the baseline shift, AFTER the peaks desolved - they are integrating a much larger area than the initial (second) peak, and that is not valid. It is like measuring the grains of moisture in the air after a tyre burst, and saying "Oh, there is more moisture in the air now than there was before the tyre burst - that tyre must have been full of water."
Interesting. I would have guessed they would have taken their peak megawatt value and equate it to tonnage, but I am a novice on such things, admittedly.
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  #194 (permalink)  
Old 14-July-2006, 08:12 PM
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Scientists Gaining Clearer Picture of Comet Makeup and Origin

Scientists are getting their best understanding yet of the makeup of comets – not only of the materials inside these planetary building blocks, but also of the way they could have formed around the Sun in the solar system’s earliest years.

When NASA’s Deep Impact spacecraft slammed into comet Tempel 1 on July 4, 2005, the collision sent tons of pristine materials into space and gave astronomers from around the world, using ground- and space-based telescopes, the first look “inside” a comet. From that sample, over the past several months, scientists who used the imaging spectrometer on NASA’s Spitzer Space Telescope have refined their models of what a comet is made of and how it comes together.

"Spitzer’s spectral observations of the impact at Tempel 1 not only gave us a much better understanding of a comet’s makeup, but we now know more about the environment in the solar system at the time this comet was formed" - Dr. Carey Lisse of the Johns Hopkins University Applied Physics Laboratory.

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  #195 (permalink)  
Old 14-July-2006, 08:21 PM
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Title: Spitzer Spectral Observations of the Deep Impact Ejecta
Authors: C. M. Lisse, J. VanCleve, A. C. Adams, M. F. Ahearn, Y. R. Fernández, T. L. Farnham, L. Armus, C. J. Grillmair, J. Ingalls, M. J. S. Belton, O. Groussin, L. A. McFadden, K. J. Meech, P. H. Schultz, B. C. Clark, L. M. Feaga, J. M. Sunshine

Spitzer Space Telescope imaging spectrometer observations of comet 9P/Tempel 1 during the Deep Impact encounter returned detailed, highly structured 5 - 35 µm spectra of the ejecta. Emission signatures due to amorphous silicates and carbon, and crystalline silicates, carbonates, phyllosilicates, PAHS, water gas/ice, sulphides were found. Good agreement is seen between the ejecta spectra and the material emitted from comet C/1995 O1 (Hale-Bopp) and the circumstellar material around the young stellar object HD100546. The atomic abundance of the observed material is consistent with solar and C1 abundances, and the D/G ratio was determined to be = 1.3. The presence of the observed mix of materials requires efficient methods of annealing amorphous silicates, and mixing of high- and low-temperature phases over large distances in the early proto-solar nebula.

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  #196 (permalink)  
Old 18-July-2006, 04:27 PM
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Default Carbonates and clays in Tempel I: Science report

We discussed on this forum before the observations of Lisse et.al. that the Deep Impact mission showed carbonates and clays within Temple I.
The results have now been published in Science:

Scientists Gaining Clearer Picture of Comet Makeup and Origin
by Staff Writers
Laurel MD (SPX) Jul 16, 2006
"From its orbit, Spitzer's infrared spectrograph closely observed the materials ejected from Tempel 1 when Deep Impact's probe dove into the comet's surface. Astronomers spotted the signatures of solid chemicals never seen before in comets, such as carbonates (chalk) and smectite (clay), metal sulfides (such as fool's gold), and carbon-containing molecules called polycyclic aromatic hydrocarbons, commonly found in barbecue grills or automobile exhaust on Earth.
"Lisse said the clay and carbonates were surprises because they typically require liquid water to make - and liquid water isn't found in the regions of deep space where comets form. Also surprising was the superabundance of crystalline silicates, material formed only at red-hot temperatures found inside the orbit of Mercury."
http://www.spacedaily.com/reports/Sc...rigin_999.html

Spitzer Spectral Observations of the Deep Impact Ejecta.
Published Online July 13, 2006
Science DOI: 10.1126/science.1124694
http://www.sciencemag.org/cgi/conten...ract/1124694v1


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  #197 (permalink)  
Old 18-July-2006, 07:16 PM
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Hum,
see also this
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  #198 (permalink)  
Old 18-July-2006, 09:44 PM
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Thread containing last two posts merged with this thread.
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