INSTRUMENT_HOST_DESC |
Instrument Host Overview
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This description was provided by Dr. Michael A'Hearn, the
principal investigator for the Deep Impact mission.
The Deep Impact Impactor vehicle is a complete spacecraft with a
CCD-based camera and telescope called the Impactor Targeting
Sensor (ITS) for both scientific imaging and auto-navigation, a
complete attitude control subsystem using hemispherical
resonator gyros, a star tracker, and a complete, hydrazine-based
propulsion system. Electrical power is supplied by an internal
battery since the expected operating lifetime is very short (24
hours).
The Impactor is mechanically and electrically attached to the
Flyby spacecraft and both launch together and fly together until
one day before the impact event. On July 3, 2005, the impactor
is released and pushed away from the Flyby at a distance of
864,000 km from comet Tempel 1. The auto-navigation system
takes control and maneuvers the Impactor to ensure an impact on
an illuminated portion of the cometary nucleus. On July 4,
2005, the impactor hits the nucleus at a relative speed of 10.2
km/s. The 360-kg Impactor releases 19 gigajoules of kinetic
energy to excavate a crater on the surface of the nucleus.
The estimated time of impact is 05:44:36 UT (Earth-received
time 05:52:02 UT), as reported by A'Hearn et al. (2005)
[AHEARNETAL2005A].
About half of the mass of the Impactor is copper, a noble metal,
which minimizes chemical reactions that could lead to species
that contaminate the spectrum with bright lines. About half this
copper is in a spherical cap at the 'front' of the impactor.
This cap is made of chamfered discs that are internally hollowed
much like a lightweight telescope mirror to reduce the density
by a factor two or so from the bulk density of copper.
Data taken by the ITS are white-light images and are used by the
onboard software for auto-navigation and transmitted to the
Flyby over an S-band link at 60 kilobits per seconds (kbps).
Attitude control and minor trajectory corrections are performed
using a small hydrazine propulsion subsystem.
In the last minute before impact, long after the last trajectory
maneuver, the project expects the optics to be destroyed by dust
impacts, either by sandblasting by small particles or by the
impact of a large particle that cracks the primary mirror of the
ITS telescope. If the optics survive, the last image will have
a resolution of 20-cm per pixel.
System Requirement Specifications for the Impactor are:
Image Data Volume : Approximately 17 megabytes
Pointing Accuracy : 2 milliradian 3-sigma
Pointing Knowledge : 150 microradian, 3 axes, 3-sigma
Targeting Accuracy : 300 m 3-sigma with respect to the
center of brightness of the nucleus
Telecom Band : S-Band
Data Rate to Flyby : 64 kbps
Command Rate : 16 kbps
Energy Storage : 2.8 kilowatt-hr for 24 hr mission
Propulsion : 25 m/s delta-velocity
For further descriptions of the impactor spacecraft, the
anticipated flight data, and the cratering experiment, see
A'Hearn, et al. (2005) [AHEARNETAL2005], Blume (2005)
[BLUME2005], Hampton, et al. (2005) [HAMPTONETAL2005], Klaasen,
et al. (2005) [KLAASENETAL2005], Richardson, et al. (2005)
[RICHARDSONETAL2005], and Schultz and Ernst (2005)
[SCHULTZ&ERNST2005].
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