Mission
The AIM mission was selected in July 2002 with final approval in
May 2004. In mid-2003, Orbital Sciences Corporation was awarded the satellite
manufacturing contract for the AIM spacecraft from a university team led by
Hampton University with the University of Colorado’s Laboratory for Atmospheric
and Space Physics (LASP) managing satellite development.
Mating of the three stages of the Orbital Sciences Pegasus XL has
been underway at Vandenberg as of March 2007. AIM will undergo a series of
readiness tests to verify its state of health and the instruments will be
cleaned and calibrated. Technicians also will partially deploy the craft's solar
arrays for illumination testing.
AIM is scheduled to be mated to the
Pegasus XL during the second week of April, after which final inspections will
be conducted. Approximately one week later, after the test team performs a
launch countdown rehearsal and flight simulation, the payload fairing will be
installed around the spacecraft.
Two days before launch, the Pegasus
rocket with the AIM spacecraft will be transported to the Vandenberg runway
where it will be attached beneath the Orbital Sciences L-1011 carrier aircraft.
The expected mission life of AIM is 26 months.
Spacecraft:
Orbital Sciences Corporation (OSC) of Dulles, Virginia, USA is the prime
contractor to Hampton University (Center for Atmospheric Sciences/Hampton
University) for the spacecraft and payload integration. The AIM mission
employs the LeoStar-2 bus of OSC, a 3-axis stabilized zero momentum
platform. The Spacecraft structure (cylinder) has a diameter of 1.09 m and
a length of 1.4 m. Spacecraft power = 335 W (orbital average) using a
fixed GaAs solar array; S/C mass = 210 kg, design life of at least 2
years.
The AIM satellite has three instruments aboard: CIPS,
SOFIE and CDE.
1. CIPS is an instrument that will take images
of the clouds to determine when and where they form, and to document what they
look like.
2. SOFIE will measure the temperature and
composition of the mesosphere, which will tell scientists more
about the chemistry and movement of air in the mesosphere that
might lead to cloud formation or cloud dissipation.
3. CDE will measure how much dust enters the
mesosphere from meteors. It is possible that this dust is what
water vapor is freezing onto to form PMC’s and thus meteor dust is
an important component of cloud formation to understand.
About
Hampton University (HU) is NASA’s
main contractor for the AIM mission, but HU will be working along with many
other co-investigators at various universities and institutions.
The
Explorers Program Office at Goddard Space Flight Center, Greenbelt, Md. manages
this NASA-funded mission. The Center for Atmospheric Sciences at Hampton
University, Hampton, Virginia leads the mission. The Laboratory for Atmospheric
and Space Physics at the University of Colorado, Boulder built two of the
spacecraft's three instruments, manages the mission and will control the
satellite after launch. The Space Dynamics Laboratory of Utah State University,
Logan, built the third instrument. Orbital Sciences Corporation, Dulles,
Virginia designed, manufactured and tested the AIM spacecraft.
Did you know?
* NASA's SMEX (Small Explorer) program is designed to provide
frequent, low-cost access to space for a variety of missions.
* Noctilucent or "night-shining" clouds were first seen in 1885 about two
years after the powerful eruption of Krakatoa in Indonesia, which hurled plumes
of ash high into Earth's atmosphere. Crews aboard the International Space
Station routinely witness noctilucent clouds when flying over Australia and the
tip of South America.
Books:
The Chilling Stars: The New Theory of
Climate Change by Henrik Svensmark
from
Amazon.com,
Amazon.co.uk,
Amazon.ca
Explains the theory that sub-atomic particles from exploded stars have more
effect on the climate than manmade CO2. The conclusion stems from Svensmark's
research which has shown the previously unsuspected role that cosmic rays play
in creating clouds.