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Experimental results from the ST7 mission on LISA Pathfinder
- Source :
- Phys.Rev.D, Phys.Rev.D, 2018, 98 (10), pp.102005. ⟨10.1103/PhysRevD.98.102005⟩, BASE-Bielefeld Academic Search Engine, Physical Review D, Physical Review D, American Physical Society, 2018, 98 (10), pp.102005. ⟨10.1103/PhysRevD.98.102005⟩
- Publication Year :
- 2018
- Publisher :
- HAL CCSD, 2018.
-
Abstract
- The Space Technology 7 Disturbance Reduction System (ST7-DRS) is a NASA technology demonstration payload that operated from January 2016 through July of 2017 on the European Space Agency's LISA Pathfinder spacecraft. The joint goal of the NASA and ESA missions was to validate key technologies for a future space-based gravitational wave observatory targeting the source-rich milliHertz band. The two primary components of ST7-DRS are a micropropulsion system based on colloidal micro-Newton thrusters (CMNTs) and a control system that simultaneously controls the attitude and position of the spacecraft and the two free-flying test masses (TMs). This paper presents our main experimental results and summarizes the overall the performance of the CMNTs and control laws. We find that the CMNT performance to be consistent with pre-flight predictions, with a measured system thrust noise on the order of $100\,\textrm{nN}/\sqrt{\textrm{Hz}}$ in the $1\,\textrm{mHz}\leq f \leq 30\,\textrm{mHz}$ band. The control system maintained the TM-spacecraft separation with an RMS error of less than 2$\,$nm and a noise spectral density of less than $3\,\textrm{nm}/\sqrt{\textrm{Hz}}$ in the same band. Thruster calibration measurements yield thrust values consistent with the performance model and ground-based thrust-stand measurements, to within a few percent. We also report a differential acceleration noise between the two test masses with a spectral density of roughly $3\,\textrm{fm}/\textrm{s}^2/\sqrt{\textrm{Hz}}$ in the $1\,\textrm{mHz}\leq f \leq 30\,\textrm{mHz}$ band, slightly less than twice as large as the best performance reported with the baseline LISA Pathfinder configuration and below the current requirements for the Laser Interferometer Space Antenna (LISA) mission.
- Subjects :
- detector: technology
Space technology
Gravitational-wave observatory
Physics and Astronomy (miscellaneous)
engineering
FOS: Physical sciences
Thrust
Astronomy & Astrophysics
01 natural sciences
7. Clean energy
Noise (electronics)
Physics, Particles & Fields
cosmic rays
0103 physical sciences
Experiments in gravity
thrust
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Aerospace engineering
noise: acceleration
010306 general physics
010303 astronomy & astrophysics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
activity report
Physics
LISA
Science & Technology
Spacecraft
density: spectral
business.industry
Payload
Noise spectral density
Pathfinder
Physical Sciences
control system
business
Astrophysics - Instrumentation and Methods for Astrophysics
cosmology
performance
Subjects
Details
- Language :
- English
- ISSN :
- 15507998 and 15502368
- Database :
- OpenAIRE
- Journal :
- Phys.Rev.D, Phys.Rev.D, 2018, 98 (10), pp.102005. ⟨10.1103/PhysRevD.98.102005⟩, BASE-Bielefeld Academic Search Engine, Physical Review D, Physical Review D, American Physical Society, 2018, 98 (10), pp.102005. ⟨10.1103/PhysRevD.98.102005⟩
- Accession number :
- edsair.doi.dedup.....a91421fe431723cd0ed34dca063fb086
- Full Text :
- https://doi.org/10.1103/PhysRevD.98.102005⟩