SL9 Impact Surprise


Donald Savage July 7, 1994 NASA Headquarters, Washington, DC.

"Because of its small size, most scientists do not expect to witness
significant visible effects from the impact of the first fragment,
nor to detect significant after-effects in the planet's
atmosphere."

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Paul Weissman July 13, 1994 in _Nature_ July 14, article titled: 
"The Big Fizzle is Coming"

"Each snowball will individually ablate and burn up like a meteor in
Jupiter's upper atmosphere. Lacking the momentum and the structural
integrity of a single solid body, they will likely not penetrate
deeper into the atmosphere where they might explode with
multi-thousands of megatons of energy.

Thus the giant impacts will produce a spectacular meteor shower, but
not the massive fireball explosions that have been predicted by some
researchers. The impacts will be a cosmic fizzle."


BAM!


(12 minute sequence of a plume near Jupiter's limb from fragment A.)

These sequence of images show evidence for a plume near the terminator of Jupiter at the time of the A impact. A bright feature appears 1000-1500 km above the limb of Jupiter at 20:18:17 in the 953nm filter. (An image at 20:15:17 did not show a detached feature.) A possible interpretation was that the feature was visible by reflected sunlight, and the apparent detachment is due to the shadow of Jupiter on the plume. During the temporal sequence from top to bottom, spreading of the feature is clearly resolved. The feature is visible at wavelengths ranging from the ultraviolet through the near infrared. Photo Credit: HST Jupiter Imaging Science Team



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Last Modified by Amara Graps on 26 November 2003.
© Copyright Amara Graps, 1995-2003.