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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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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:
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The 250,000 Ton Punch
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Everything I need to know I learned through Googling. |
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |
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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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Moderations in purple Fame, glory adventure, a cyber warrior craves not these things. |
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Everything I need to know I learned through Googling. |
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The 250,000 Ton Punch Quote:
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From Sticks reference: Quote:
Bad science!
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jwj It's ok not to know. We should try harder to find out. |
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |
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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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jwj It's ok not to know. We should try harder to find out. |
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Lighten up! This is a stellar board! Author: duh. "The Sun, with all the planets revolving around it, and depending on it, can still ripen a bunch of grapes as though it had nothing else in the universe to do..." Author: Galileo supposedly. |
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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. Read more
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`Irony` actually does mean `metal like`... |
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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. Rea more (subscription, PDF)
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`Irony` actually does mean `metal like`... |
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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 Bob Clark |