TY - GEN
T1 - Autonomous spacecraft navigation based on pulsar timing information
AU - Bernhardt, Mike Georg
AU - Becker, Werner
AU - Prinz, Tobias
AU - Breithuth, Ferdinand Maximilian
AU - Walter, Ulrich
PY - 2011
Y1 - 2011
N2 - We discuss the possibility of an autonomous navigation system for spacecraft that is based on pulsar timing data. Pulsars are rapidly rotating neutron stars that are observable as variable celestial sources of electromagnetic radiation. Their periodic signals have timing stabilities comparable to atomic clocks and provide characteristic temporal signatures that can be used as natural navigation beacons, quite similar to the use of GPS satellites for navigation on Earth. By comparing pulse arrival times measured on-board the spacecraft with predicted pulse arrivals at some reference location, the spacecraft position can be determined autonomously with accuracies on the order of 5 kilometres. For a spacecraft at a distance of 10 astronomical units from Earth (e.g., Earth-Saturn), this means an improvement by a factor of 8 compared to conventional methods. Therefore this new technology is an alternative to standard navigation based on radio tracking by ground stations, without the disadvantages of uncertainty increasing with distance from Earth and the dependence on ground control.
AB - We discuss the possibility of an autonomous navigation system for spacecraft that is based on pulsar timing data. Pulsars are rapidly rotating neutron stars that are observable as variable celestial sources of electromagnetic radiation. Their periodic signals have timing stabilities comparable to atomic clocks and provide characteristic temporal signatures that can be used as natural navigation beacons, quite similar to the use of GPS satellites for navigation on Earth. By comparing pulse arrival times measured on-board the spacecraft with predicted pulse arrivals at some reference location, the spacecraft position can be determined autonomously with accuracies on the order of 5 kilometres. For a spacecraft at a distance of 10 astronomical units from Earth (e.g., Earth-Saturn), this means an improvement by a factor of 8 compared to conventional methods. Therefore this new technology is an alternative to standard navigation based on radio tracking by ground stations, without the disadvantages of uncertainty increasing with distance from Earth and the dependence on ground control.
UR - http://www.scopus.com/inward/record.url?scp=82055188350&partnerID=8YFLogxK
U2 - 10.1109/ICSpT.2011.6064649
DO - 10.1109/ICSpT.2011.6064649
M3 - Conference contribution
AN - SCOPUS:82055188350
SN - 9781457718748
T3 - 2nd International Conference on Space Technology, ICST 2011
BT - 2nd International Conference on Space Technology, ICST 2011
T2 - 2nd International Conference on Space Technology, ICST 2011
Y2 - 15 September 2011 through 17 September 2011
ER -