Deep Impact (Discovery 7) --> EPOXI |
USA |
International Sat. nº: |
USA satellite nº: |
Launch data:
| Designation | 28517 / 05001A |
| Launch date | 12 Jan 2005 - 18:47:08 UT |
| Launch site | CC, SLC-17B |
| Launch vehicle |
Delta 7925-9.5 (#D311) |
| Mission | Comet impact and flyby |
| Heliocentric orbit |
| Perihelion / Aphelion | 0.981 x 1.628 |
| Incl. to ecliptic | 0.6 ° |
| Period | min |
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Deep Impact (with Impactor) [Ball]
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Spacecraft data:
| Prime contractor | Ball Aerospace, JPL |
| Operator | NASA |
| Platform | |
| Mass at launch: |
| Fly-by spacecraft | 601 kg (86 kg of propellant) |
| Impactor | 372 kg (8 kg of propellant) dim: 1 dia, 1 long |
| Launch Mass | 973 kg |
| Basic shape | Box + panel |
| Dimension | 3.3 x 1.7 x 2.3 2.8 span |
| Solar array | |
| Stabilization | |
| DC power | |
| Design lifetime | |
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Description:
The objectives of the Deep Impact mission are to rendezvous with comet
P/Tempel-1 and launch a projectile into the comet nucleus. Observations will
then be made of the ejecta, much of which will represent pristine material from
the interior of the comet, the crater formation process, the resulting crater,
and any outgassing from the nucleus, particularly the newly exposed surface.
This project was selected as a Discovery class mission in July, 1999.
Deep Impact is a two-part spacecraft, comprising a Fly-by spacecraft and an Impactor. The Impacter is a 372 kg cylindrical copper attached to a flyby bus, the launch mass of the flyby bus and impactor is 973 kg. The Fly-by
spacecraft is a box-shaped honeycombed aluminum framework with a flat
rectangular Whipple debris shield mounted on one side to protect components
during comet close approach. Mounted on the framework are one high- and one
medium-resolution instrument, each of which consists of an imaging camera and an
infrared spectrometer which will be used to observe this ejected ice and dust,
much of which will be exposed to space for the first time in over 4 billion
years. The medium resolution camera has a field of view (FOV) of 0.587 degrees
and a resolution of 7 m/pixel at 700 km distance and is used for navigation and
context images. The high resolution camera has a FOV of 0.118 degrees and a
resolution of 1.4 m/pixel at 700 km. The infrared spectrometers cover the range
from 1.05 to 4.8 micrometers with FOV of 0.29 degrees (hi-res) and 1.45 degrees
(lo-res). The total flyby bus instrument payload has a mass of 90 kg.
The flyby spacecraft measures approximately 3.2 m x 1.7 m x 2.3 m, is
three-axis stabilized and uses a hydrazine propulsion system. Communications
with the ground from the flyby bus are via X-band (8.000 MHz) through a 1 meter
diameter parabolic dish antenna mounted on a 2-axis gimbal and via S-band
between the impactor and flyby spacecraft. The maximum data rate will be 400
kbps. Power of 620 W at the encounter is provided by a 7.5 square meter solar
array and stored in a small NiH2 battery. The projectile is made of copper so it
will be easily identifiable in the spectra after the projectile is largely
vaporized and mixed in with the comet ejecta on impact. The impactor is equipped
with an Impactor Targeting Sensor, an imager which provides knowledge for
autonomous control and targeting, and a cold-gas attitude control system.
Mission:
- The Boeing Delta 7925 rocket reached a 167 x 167 km x 29.7
deg parking orbit at 18:56 UT, and then restarted at 19:11 UT to enter a
163 x 4170 km orbit. The third stage separated and burned at 19:14 UT,
and after separation at 19:21 UT there were four objects on an Earth
escape trajectory: the PAM-D third stage, two despin weights, and the
Deep Impact probe.
- By Jan 19, 2005 the probe was 1.9 million km
from Earth and on track to enter a 0.981 x 1.628 AU solar orbit
inclined 0.6 deg to the ecliptic.
- The 372 kg Impactor spacecraft separated from the DI Flyby vehicle at 06:00
UT on Jul 3, 2005. Impactor hit comet 9P/Tempel 1 at 10.2 km/s at 0544:58
UT on Jul 4, 2005 as the DI Flyby spacecraft sent back spectacular pictures
of the resulting plume. Flyby passed about 500 km from the comet at 05:59
UT, at which time it was in 'shields up' mode pointing away from the
comet to protect itself from the plume.
- The comet and spacecraft will be about 0.89 AU
from Earth and 1.5 AU from the Sun during the encounter. Real time return of
selected impactor images and flyby images and spectra will be returned to Earth
during the encounter. Primary data return will be over the first day after
encounter, with a 28 day supplemental data return period. Earth-based
observatories will also study the impact. The spacecraft will range over a
distance of 0.93 to 1.56 AU from the Sun during the mission. End of mission is
scheduled for August 2005.
- Name changed into EPOXI in 2007 for an extended mission.
- The Deep Impact (EPOXI) spacecraft flew 700 km from comet 103P/Hartley
at around 14:01 UTC on Nov 4, 2010. It revealed an active cometary nucleus
with rough and smooth areas, and jets coming from the rough areas.
- The Deep Impact/EPOXI mission has come to an end. Last contact with the Deep Impact Flyby spacecraft was on Aug 11, 2013
and attempts to revive it have been abandoned.
In Oct 2012 the probe was targeted towards minor planet (163249) 2002 GT, which it might have reached in 2020. DIF is
in a 0.97 x 1.21 AU x 3.2 deg heliocentric orbit.
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Ref.: #3(SD391), #7(JR543-550,634,686), #14, #81, #206 - update: 02.11.13
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