Back to Search Start Over

Experimental results from the ST7 mission on LISA Pathfinder

Authors :
S. Vitale
W. Warner
Lluis Gesa
J. Fernandez
Nikolaos Karnesis
M. Connally
R. Kolasinski
J. Martino
Thomas Randolph
Gerhard Heinzel
R. Maarschalkerweerd
A. Wittchen
J. Gorelik
Eric Ehrbar
S. Rhodes
Ian Harrison
J. Wellman
J. A. Lobo
Thomas Roy
O. Hsu
A. Carmain
Oliver Jennrich
G. Dixon
M. Cherng
Charley Dunn
Henri Inchauspe
Ivan Lloro
D. Miller
F. Rivas
Luigi Ferraioli
L. Chen
D. Kern
L. Markley
Heather Audley
José F. F. Mendes
E. Dorantes
Gudrun Wanner
Peter Wass
S. Paczkowski
T. Le
Juan Ramos-Castro
R. Valencia
Jacob Slutsky
Valerio Ferroni
William E. Connolly
Pierre Binétruy
L. Wissel
H. Umfress
R. Parikh
D. Hoyland
T. J. Sumner
John R. Anderson
L. Liu
M. Hewitson
L. Mendes
E. Castelli
Vlad Hruby
Antonella Cavalleri
N. Korsakova
O. Liepack
Shahram Javidnia
Miquel Nofrarías
John J. Evans
Michele Armano
C. Kuo
M. Freschi
Daniel Hollington
Garth Franklin
Douglas J. Jackson
G. Aveni
K. Blackman
M. Hueller
Christian J. Killow
M. S. Anderson
J. P. López-Zaragoza
M. Born
Ingo Diepholz
S. Malik
N. Meshksar
Ryan Martin
S. Clark
Nate Demmons
Douglas Spence
Ferran Gibert
J. Stocky
W. Tolman
Ignacio Mateos
D. Conroy
Ira Thorpe
G. Plett
Phil Barela
A. Littlefield
Peter Willis
J. D’Agostino
M. Cooper
A. M. Cruise
D. Bortoluzzi
Catia Grimani
M. Duran
M. de Deus Silva
H. Shaw
F. Martin-Porqueras
J. Reiche
A. Cesarini
G. Russano
J. Grzymisch
H. Ward
E. D. Fitzsimons
Peter Zweifel
R. Giusteri
Ph. Jetzer
M. Knopp
T. Ramsey
D. I. Robertson
J. Mehta
Domenico Giardini
W. J. Weber
M. Girard
Rita Dolesi
L. Martin-Polo
Colleen Marrese-Reading
Karsten Danzmann
D. Bame
I. Li
Eric Plagnol
B. Kaune
Víctor S. Martín
C. Valerio
Andrew Romero-Wolf
D. Nguyen
J. Baird
Greg M. Anderson
Michael Perreur-Lloyd
Peiman Maghami
Davor Mance
D. Texier
John Ziemer
J. Tallon
Antoine Petiteau
Paul McNamara
A. Ruiz
Carlos F. Sopuerta
J. O’Donnell
Daniele Vetrugno
Curt Cutler
J. Mennela
P. Pivato
Jurg Zwahlen
AstroParticule et Cosmologie (APC (UMR_7164))
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
ST7
LISA Pathfinder
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
ST7 Team
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.

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⟩