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Image taken by Giovanni Sostero
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| Comments: |
This panel illustrate the steep variation of the Afrho quantity (a proxy of the dust abundance) Vs. the distance from the nucleus. The contribution of the nucleus has not been removed jet. |
| Image Date (UTC): |
2005-03-14 |
| Image Time (UTC): |
00:10:00 |
| Exposure: |
7x180 sec |
| Filter: |
Red |
| Field of View: |
26 to 12 x 18 to 8 arcmins |
| Observing Site: |
Remanzacco Observatory |
| Observing Equipment: |
10/18/6" f/from 5.2 up to 7/4.5/6 Meade/Marcon/Intes SCT/newtonian/Maksutov |
| Days After Perihelion: |
-113.29 |
| Heliocentric Distance: |
1.863 |
| Geocentric Distance: |
0.933 |
| Sun-Comet-Earth Angle: |
15.23 |
STSP Coordinator: Stef McLaughlin
Webmaster: Elizabeth Warner
Last Updated: Wednesday August 29, 2007
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