Close-Up of Bright Nucleus in Comet P/Shoemaker-Levy 9

Close-Up of Bright Nucleus in Comet P/Shoemaker-Levy 9

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Fast Facts
News release ID: STScI-1993-22
Release Date: Oct 18, 1993
Image Use: Copyright
About this image

This is an enlargement of a NASA Hubble Space Telescope image of the "brightest nucleus" in a string of approximately 20 objects that comprise comet P/Shoemaker-Levy 9. The comet is hurtling toward a July I994 collision with the giant planet Jupiter.

Hubble's high resolution shows that this bright region is actually a group of at least four separate pieces. The HST images allow for the best separation of the individual nuclei and their surrounding halo of dust (comae), which results in a better estimate of the nuclear sizes.

The image was taken with the Wide Field and Planetary Camera (WFPC), in PC mode, on July 1, 1993. The Hubble observations show that the cometary nuclei are probably less than three miles (5 km) across, as opposed to earlier estimates of nine miles (I4 km).

The new Hubble data show that the impacts will unleash only 1/10th to 1/100th as much energy as thought previously. However, even with these new size estimates, the total energy of the July I994 collisions will be equivalent to I00 million megatons of TNT.

Annotated Observations, Jupiter, Planets, Solar System


Dr. H. A. Weaver and Mr. T. E. Smith, STScI NASA