Using its clear filter, the OSIRIS Narrow Angle also produced a 'light curve' of Comet 9P/Tempel 1. This shows how the comet's intensity varies in time, starting from impact.
The light curve shows that about 30 minutes after impact the brightness of the comet had increased by five times.
After this phase, scientists also noticed that the brightness level fluctuated for about one hour with no overall increase, then seemed to decrease, but much more slowly than the initial increase.
As more data come in from Rosetta, ESA scientists will be able to refine images and results.
 |  |
| | ESA's comet chaser (http://www.esa.int/SPECIALS/Rosetta/index.html) |
 |
 More about...

|
| | Rosetta factsheet (http://www.esa.int/esaSC/SEMJUZS1VED_index_0.html) |
 |
| | XMM-Newton factsheet (http://www.esa.int/esaSC/SEM14YS1VED_index_0.html) |
 |
| | Hubble factsheet (http://www.esa.int/esaSC/SEMB5E1A6BD_index_0.html) |
 |
| | NASA Deep Impact (http://www.nasa.gov/mission_pages/deepimpact/main/index.html) |
 |
| | ESO Deep Impact news (http://www.eso.org/outreach/press-rel/pr-2005/pr-15-05.html) |
 |
 Related articles

|
| | Life of a comet (http://www.esa.int/SPECIALS/Rosetta/SEM3NV0PGQD_0.html) |
 |
| | Tempel 1: Biography of a comet (http://www.esa.int/SPECIALS/Rosetta/SEMIUG0DU8E_0.html) |
 |
| | Rosetta monitors Deep Impact (http://www.esa.int/esaCP/SEMCOZ1DU8E_Expanding_0.html) |
 |
| | XMM-Newton to observe Deep Impact (http://www.esa.int/SPECIALS/Rosetta/SEMSZC2DU8E_0.html) |
 |
| | Hubble sees outburst from Deep Impact comet (http://www.esa.int/SPECIALS/Rosetta/SEMSBN5DIAE_0.html) |
 |
| | ESA observes Deep Impact from Earth (http://www.esa.int/SPECIALS/Rosetta/SEMNRO5DIAE_0.html) |
 |
| | Dust and gas from Comet 9P/Tempel 1 seen by ESA OGS (http://www.esa.int/SPECIALS/Rosetta/SEMQR06DIAE_0.html) |
 |
| | Tempel 1 is weak X-ray source, XMM-Newton confirms (http://www.esa.int/SPECIALS/Rosetta/SEMXA46DIAE_0.html) |
 |