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Hubble's View of Deep Impact.


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Hubble's view of the Deep Impact collision.
Hubble's view of the Deep Impact collision. Image credit: Hubble.

The powerful Hubble Space Telescope was on hand to watch the collision between Deep Impact and Comet Tempel 1. Even though Hubble is one of the most sensitive Telescopes available, the shroud of dust and gas surrounding Tempel 1 obscures a view of the comet's nucleus. Hubble was able to see the flash from the impact, making the Comet 4 times as bright, and then an expanding fan of debris moving away from the comet.

The NASA/ESA Hubble Space Telescope captured the dramatic effects of the collision early on 4 July between the Deep Impact impactor spacecraft and Comet 9P/Tempel 1.

This sequence of images shows the Comet before and after the impact. The image at left shows the Comet just minutes before the impact. The encounter occurred at 07:52 CEST (05:52 UT/GMT).

In the middle image, captured 15 minutes after the collision, Tempel 1 appears four times brighter than in the pre-impact photograph.

Astronomers noticed that the inner cloud of dust and gas surrounding the comet's nucleus increased by about 200 kilometres in size.

The impact caused a brilliant flash of light and a constant increase in the brightness of the inner cloud of dust and gas.

Hubble continued to monitor the comet, snapping another image (at right) 62 minutes after the encounter. In this photograph, the gas and dust ejected during the impact are expanding outward in the shape of a fan.

The fan-shaped debris is travelling at about 1800 kilometres an hour, or twice as fast as the speed of a commercial jet. The debris extends about 1800 kilometres from the nucleus.

The potato-shaped Comet is 14 kilometres wide and 4 kilometres long. Tempel 1's nucleus is too small even for the Hubble telescope to resolve.

The visible-light images were taken by the high-resolution camera on Advanced Camera for Surveys instrument. The Hubble Space Telescope is a project of international co-operation between ESA and NASA.




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