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Paolozzi, A., Ciufolini, I., Gabrielli, A., Paris, C., and Sindoni, G., 2015. Lares Mission: Engineering Aspects. Aerotecnica Missili & Spazio, 94(1):23–30, doi:10.1007/BF03404685.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2015AeMiS..94...23P,
author = {{Paolozzi}, A. and {Ciufolini}, I. and {Gabrielli}, A. and {Paris}, C. and {Sindoni}, G.},
title = "{Lares Mission: Engineering Aspects}",
journal = {Aerotecnica Missili \& Spazio},
year = 2015,
month = jan,
volume = {94},
number = {1},
pages = {23-30},
abstract = "{LARES is a satellite of the Italian Space Agency, successfully launched
with the new VEGA launcher in the occasion of its inaugural
flight, VV01. It was put in a circular orbit at 1450 km
altitude. This altitude was required to reduce atmospheric drag,
whereas the satellite was designed to minimize the non-
gravitational perturbations acting on the surface of the
satellite. This was of paramount importance because the mission
objective is to test Einstein general relativity, and any
unmodeled effect could spoil the accuracy of the relativistic
measurement. With the optimal design achieved, this non-
gravitational unmodeled effects are maintained below 1\% of
frame-dragging or Lense-Thirring effect. This effect is the
orbital node shift induced by the Earth rotation as predicted by
general relativity. To achieve the accuracy required for the
test, it was conceived a constellation of three laser ranged
satellites (LAGEOS 1, LAGEOS 2 and LARES) along with the latest
determination of the Earth gravitational field by GRACE
satellite. The satellite is a passive system and embedded with
92 Cube Corner Reflectors that have the properties of reflecting
back to the emitting ground station the laser pulses, thus
allowing its precise orbital determination. In this paper
engineering aspects of the mission will be addressed.}",
doi = {10.1007/BF03404685},
adsurl = {https://ui.adsabs.harvard.edu/abs/2015AeMiS..94...23P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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