PIA02142 Tempel 1 bottom sharped


Autor:
NASA / Jet Propulsion Laboratory / University of Maryland
Formát:
1600 x 1600 Pixel (430492 Bytes)
Popis:

This image shows comet Tempel 1 before Deep Impact's probe smashed into its surface. It is a composite of images taken by the probe's impactor targeting sensor. The Sun is to the right of the image and reveals terrain varying in brightness by a factor of two. Shadows and bright areas indicate surface topography. Smooth regions with no features (lower left and upper right) are probably younger than rougher areas with circular features, which are probably impact craters. The probe crashed between the two dark-rimmed craters near the center and bottom of the comet.

The comet nucleus is estimated to be about 5 kilometers (3.1 miles) across and 7 (4.3 miles) kilometers tall.

This composite image was built up from scaling all images to 5 meters/pixel, and aligning images to fixed points. Each image at closer range, replaced equivalent locations observed at a greater distance. The impact site has the highest resolution because images were acquired until about 4 sec from impact or a few meters from the surface.

In the annotated version (see "Other versions" below), arrows a and b point to large, smooth regions. The impact site is indicated by the third large arrow. Small arrows highlight a scarp that is bright due to illumination angle, which shows the smooth area to be elevated above the extremely rough terrain. The scale bar is 1 km and the two arrows above the nucleus point to the sun and the rotational axis of the nucleus. Celestial north is near the rotational pole.

The original NASA image has been modified by cropping, and by sharpening of the lower 640 pixels.
Licence:
Public domain
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9P/Tempel

9P/Tempel 1 je kometa patřící do Jupiterovy rodiny. Objevil ji 3. dubna 1867 francouzský astronom Ernst Wilhelm Leberecht Tempel. Tato krátkoperiodická kometa prošla dne 15. května téhož roku v minimální vzdálenost 0,568 AU od Země a 24. května perihelem své dráhy ve vzdálenosti 1,562 AU od Slunce. Naposledy při tomto přiblížení ke Slunci byla pozorována 27. srpna 1867. Pětiměsíční sledování však stačilo, aby byla dostatečně přesně zjištěna její dráha. .. pokračovat ve čtení