OBSERVING 9P/Tempel 1 THE TARGET OF DEEP IMPACT

Nicolas Biver 03 July 2005


TOPICS

Magnitude estimates of 9P and drawings Sky Maps for 9P/Tempel 1 Deep Impact home page
Trajectory and impact visibility Predictions for 4 July 2005 Radio observation results

Other useful links:

Nasa Deep Impact page
Space and Ground based observations highlights
Program of comet monitoring with Small Telescope (CCD)
Other Amateur observations
Nasa live coverage

Orbit and viewing conditions of impact

Current Earth time of impact is 4 July 2005 5:52:15+-17sec UTC

Trajectory of Deep Impact (red), Rosetta (purple) 9P/Tempel 1 (blue) and Earth (black). Dotted lines: below ecliptic materialized by the cyan grid (0.2/0.02 AU step)

( French version and higher resolution French version )

Earth as seen from 9P/Tempel 1 at the time of Deep Impact encounter: regions visible in the dark shaded part of the Earth can see the impact during night time hours (e.g. Polynesia, Hawaii in twilight, North-West America)

Based on a paper published in "L'Astronomie" vol. 119, 308-311 (Juin 2005)

Possible Brightness Outburst

Here is an estimate of the surge of brightness of comet 9P/Tempel 1 after the impact on 4.244 July 2005, hypotheses are:
  • (1) Dust follows the release of gas (i.e. dust column density stays proportionnal to gas one);
  • (2) Amount of material released corresponds to a hemispherical shape crater of diameter 138m, depth 30m: 240000 m3 => 120000 tons (50% dust + 50% ice)
  • (3) grain size distribution: 1um - 1cm, dN(r) # dr/r3 (lifetime 5s - 13h)
  • (4) "Nuclear magnitude": aperture 3"
  • (5) "Total magnitude": coma 2'

    There is no "forecast" here for what will hapen later to the comet (e.g. new active zone, runaway increase of new active area (e.g. tanks to crystalization of amorphous water ice,...), partial break-up or.... Nothing significant!)
    Based on a paper published in "L'Astronomie" vol. 119, 308-311 (Juin 2005)

    Some results of IRAM-30m observations



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    observations always in progress... Nicolas Biver - 3 July 2005