Stellar attitude determination accuracy with multiple-star-tracking advanced star tracker

Author(s):  
Rene Abreu
Sensors ◽  
2020 ◽  
Vol 20 (21) ◽  
pp. 6250
Author(s):  
Surabhi Agarwal ◽  
Elena Hervas-Martin ◽  
Jonathan Byrne ◽  
Aubrey Dunne ◽  
Jose Luis Espinosa-Aranda ◽  
...  

Star trackers are navigation sensors that are used for attitude determination of a satellite relative to certain stars. A star tracker is required to be accurate and also consume as little power as possible in order to be used in small satellites. While traditional approaches use lookup tables for identifying stars, the latest advances in star tracking use neural networks for automatic star identification. This manuscript evaluates two low-cost processors capable of running a star identification neural network, the Intel Movidius Myriad 2 Vision Processing Unit (VPU) and the STM32 Microcontroller. The intention of this manuscript is to compare the accuracy and power usage to evaluate the suitability of each device for use in a star tracker. The Myriad 2 VPU and the STM32 Microcontroller have been specifically chosen because of their performance on computer vision algorithms alongside being cost-effective and low power consuming devices. The experimental results showed that the Myriad 2 proved to be efficient and consumed around 1 Watt of power while maintaining 99.08% accuracy with an input including false stars. Comparatively the STM32 was able to deliver comparable accuracy (99.07%) and power measurement results. The proposed experimental setup is beneficial for small spacecraft missions that require low-cost and low power consuming star trackers.


1996 ◽  
Author(s):  
Kazuhide Noguchi ◽  
Koshi Sato ◽  
Ryouichi Kasikawa ◽  
Naoto Ogura ◽  
Keiken Ninomiya ◽  
...  

2014 ◽  
Vol 664 ◽  
pp. 298-303
Author(s):  
Yu Wang Lai ◽  
De Feng Gu ◽  
Jun Hong Liu ◽  
Wen Ping Li ◽  
Dong Yun Yi

The low-frequency error (LFE) of star tracker is the most critical problems in the high accuracy attitude determination for the satellite. In this paper a novel approach is proposed to identify and compensate the attitude measurement LFE of the star trackers. The main difficulty in the attitude LFE identification is to distinguish the attitude LFE from the attitude motion. To overcome this difficulty, the gyro data, which is sensitive to the attitude motion, was used to fit the measurement attitude data to obtain the reference attitude. It is shown that, the LFE can be identified by comparing the measurement attitude and the reference attitude. The attitude LFE repeated feature is characterized well by the proposed method. By utilizing the orbital repeated feature, the LFE of the star trackers can be estimated. Finally, a LFE compensation strategy is presented base on the LFE estimation results. The validity and efficiency of the proposed approach are demonstrated by the relative Euler angle results from two test star trackers on-board the STECE satellite.


1993 ◽  
Author(s):  
Luisa DeAntonio ◽  
Gabriel Udomkesmalee ◽  
James W. Alexander ◽  
Randel C. Blue ◽  
Edwin W. Dennison ◽  
...  

2021 ◽  
pp. 1-26
Author(s):  
H. Benzeniar

ABSTRACT The Algerian Space Agency has been active in the field of microsatellite engineering for more than 15 years and has successfully developed microsatellites under several know-how transfer technology programs, six to date. This paper presents the flight results and lessons learned from the attitude determination and control system (ADCS) flown on the ALSAT-2B satellite, an Earth observation microsatellite, by analysing the behaviour of the satellite from the initial attitude acquisition through the coarse pointing mode then the nominal mode, where the payload is first tested, and finally the orbit control mode. The spacecraft was launched on 26 September 2016 and placed into a 670km Sun-synchronous orbit with a solar local time at an ascending node of 22:15. The ADCS performance presented here mainly focuses on the launch and early operation results. ALSAT-2B includes four reaction wheels in a pyramidal configuration, three gyros, three Sun sensors, three magneto-torquers, one magnetometer, and one star tracker for agile and accurate attitude control. In addition, a propulsion system based on four 1N hydrazine thrusters is also used on board the microsatellite. The main new development in this platform compared with previous ones of the same type is the fusion of the star tracker and measurements by the three gyroscopes into one gyrostellar estimator that was implemented for the first time on ALSAT-2B, and the pyramidal configuration of the wheels, aiming to increase the angular momentum. The results obtained from the early launch operations for different ADCS modes are very encouraging and fulfil all the requirements set during design and testing. Currently, the satellite has accomplished its fourth year in orbit and is still operational and producing high-quality images.


2008 ◽  
Vol 56 (657) ◽  
pp. 480-491
Author(s):  
Takanori IWATA ◽  
Eiji HIROKAWA ◽  
Hiroki HOSHINO ◽  
Takeshi YOSHIZAWA ◽  
Koshi SATO ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document