Space Situational Awareness
AFSPC explores Allen Telescope Array for Space Surveillance View official AFSPC press release here
An important and high visibility mission of the United States Air Force Space Command
(AFSPC) is Space Surveillance. Knowing exactly where orbiting objects are located in
space at any given instant is key to ensuring safe space operations. The significance
of the mission has become even more acute with the recent collision of an Iridium
Satellite and an inoperable Russian Cosmos Satellite, which destroyed both satellites
and created two large fields of space debris. This debris will be a risk to other
satellites for years to come as the debris fields expand and their orbits degrade toward
Earth.
AFSPC is one of a few organizations responsible for obtaining and maintaining the
awareness needed for successful and safe space operations. The command develops,
maintains and shares a comprehensive and accurate catalog of orbiting space objects,
while constantly seeking methods to improve their Space Surveillance Network (SSN), a
global network of radar and optical sensors that detect and track orbiting space
objects. AF Space Command is exploring opportunities in academia and the commercial
sector that could provide suitable cost-effective means for augmenting the Space
Command's Space Surveillance mission.
The Allen Telescope Array (ATA), located at the
Hat Creek Radio Observatory, 290 miles northeast of San Francisco, California is a tool
with strong potential for use by AFSPC in support of the Department of Defense’s Space
Surveillance mission. The ATA is a radio interferometer that is dedicated to
cutting-edge astronomical research. This array of antennas is optimized to receive and
process a very wide portion of the radio spectrum and can stare at many areas of the sky
at once.
AFSPC, through the Space Innovation and Development Center (SIDC), is currently
researching the possible use of the ATA to augment the already extensive sensors of the
Space Surveillance Network, potentially leveraging the array to help increase space
situational awareness. Initial demonstrations show promise for the ATA to track
transmitting satellites in Low Earth Orbit, Medium Earth Orbit and, most promising, in
Geosynchronous Orbit (GEO), which is home to the most costly, highly-utilized, and vital
satellites that orbit the earth. A collision and subsequent debris field in GEO could
permanently remove the GEO belt from worldwide use.
AFSPC is working with the SETI Institute, and its partner, the Radio Astronomy
Laboratory at the University of California, Berkeley. These partners currently operate
the ATA. The effort is to demonstrate the array’s capability of accurately surveying
the GEO belt by demonstrating the array’s capability of precisely locating objects in
that area, in an effort to avoid a devastating collision in GEO. The ATA may prove to
be a viable and sensitive SSN sensor, capable of all-weather, day and night operations,
and will hopefully lead to improved space safety.
Questions and Answers -- Use of the Allen Telescope Array for Space
SurveillanceQ1. What is the degree to which SETI Institute is collaborating with the Air Force
here?
A1. AF Space Command is exploring opportunities in academia and the commercial sector
that could provide suitable cost-effective means for augmenting the Space Command's
Space Surveillance mission. The Allen Telescope Array (ATA) could be an important tool
to support the Department of Defense’s Space Surveillance mission. The significance of
this mission has become even more acute with the recent collision of two satellites and
the resulting danger posed to the International Space Station, the Hubble Telescope and
other satellites in low earth orbit.
Q2. How can the Allen Telescope Array complement the Air Force's existing
sensors?
A2. The ATA has numerous unique capabilities for astronomy and SETI research, and
because it is the first instrument of its type, some of its capabilities may enhance Air
Force daylight space surveillance capabilities.
Q3. What would SETI Institute get from such a collaboration?
A3. If the ATA proves to be a valued contributing sensor, it could provide a potential
additional use of the array and, concurrently, an additional source of long term funds
to assist in the operations and support cost of sustaining the array.
Q4. What tasks have been done by the ATA for AFSPC?
A4. The initial task completed was an assessment of the capability of the array to
accurately track orbiting objects, specifically GPS satellites. The GPS satellite
constellation was selected because the location of these satellites in space is well
known. Therefore by utilizing this data, the accuracy of the array’s observations could
be assessed. The ATA has observed GPS satellites to a relatively high accuracy, and the
accuracy is expected to improve as the array’s algorithms for satellite positional
determination are refined and as the array’s configuration is extended by the addition
of more antennas.
Q5. What do you foresee as some future tasks the ATA may conduct for AFSPC?
A5. Future tasks for the ATA will include demonstrating the capability to track objects
besides GPS. Additionally, tasks such as tracking objects during the daylight hours, or
with the sun or moon in field of view, will further demonstrate the capabilities of the
ATA as a sensor for the SSN. These demonstrations are important because many of the
current sensors have difficulty with light-pollution, which hampers observations. If
the ATA can demonstrate its capability to precisely locate satellites in all orbits,
during day or night, it increases it significance as a SSN sensor, and increases the
overall safety of space.
Q6. What are the future plans for the ATA?
A6. The SETI Institute and its partner, UC. Berkeley, plan to increase the size of the
array in stages. As the number of array elements increase, the sensitivity and
capability of the array also increases. This helps for both scientific and astronomical
research, and will also increase the capabilities of the ATA as a SSN sensor.
Q7. What are the plans for securing the funding needed to fill out the antenna
array?
A7. The SETI Institute and its partner, UC. Berkeley, have plans to increase the size of
the array in stages. Dependent upon the availability of funds, the first expansion to
128 dishes with additional control building and other support components, is expected to
cost between $18 -$20M. The next 128 (256 total) is budgeted at an additional $20M
($156K per dish).
Q8. Why is the Air Force interested in using this sensor as opposed to
others?
A8. The unique design of the Allen Telescope Array (ATA) is intriguing to the Air Force
because it provides a similar sensitivity to a very large dish antenna, but at a cheaper
cost for the same collecting area. This is known as a Large-Number Small-Diameter
concept, and fits well with the Air Force’s goal of conducting its mission in a fiscally
responsible manner.
The AF working with the ATA may be a natural win-win relationship. Specifically, the
AF requires additional sensors to observe orbiting objects during the daytime, because
many of its Electric-Optical (EO) sensors are affected by light pollution during the
day, which limits the observations that can be conducted at that time. The ATA's
primary missions, searching for extraterrestrial life and scientific research, are most
often conducted at night, because this gives them the best pointing stability and avoids
decrease in the strength of narrow band signals due to scattering by the solar wind.
Operating the ATA during the daylight hours for the AF allows the array to be more fully
utilized while not detracting from its scientific and SETI goals, and may provide the AF
with vital daytime observations.
To be utilized as a viable long-term sensor for the SSN, the ATA has to demonstrate
many characteristics besides accurately being able to observe orbiting satellites. Its
data have to be consistent, timely, precise, sensitive, and have a throughput that makes
it worth the cost of a long-term investment by the Air Force. If these factors
demonstrate themselves, the ATA may be integrated into the SSN to help to ensure the
safety of flight of objects in space.
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