Issue |
A&A
Volume 593, September 2016
|
|
---|---|---|
Article Number | A34 | |
Number of page(s) | 10 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/201628869 | |
Published online | 06 September 2016 |
Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique: A test case of the Mars Express Phobos fly-by
1 California Institute of
Technology, 1200 E California
Blvd, Pasadena, CA 91125, USA
e-mail: duev@caltech.edu
2 Joint Institute for VLBI ERIC,
PO Box 2,
7990 AA
Dwingeloo, The
Netherlands
3 Sternberg Astronomical Institute,
Lomonosov Moscow State University, Universitetsky av. 13, 119991
Moscow,
Russia
4 ASTRON, The Netherlands Institute for
Radio Astronomy, Postbus
2, 7990 AA,
Dwingeloo, The
Netherlands
5 Aalto University, School of
Electrical Engineering, Department of Radio Science and Engineering,
02150
Espoo,
Finland
6 Department of Astrodynamics and Space
Missions, Delft University of Technology, 2629 HS
Delft, The
Netherlands
7 Shanghai Astronomical Observatory,
80 Nandan Road,
200030
Shanghai, PR
China
8 Carnegie Mellon University,
5000 Forbes Ave,
Pittsburgh, PA
15213,
USA
9 Institute for Space Sciences,
Atomistilor 409, PO Box
MG-23, 077125
Bucharest-Magurele,
Romania
10 Royal Observatory of Belgium,
Ringlaan 3,
1180
Brussels,
Belgium
11 CNES/GRGS, OMP 14 avenue Édouard
Belin 31400
Toulouse,
France
12 IMCCE, Observatoire de Paris, PSL
Research University, CNRS-UMR 8028 du CNRS, UPMC, Lille-1, 77 Av. Denfert-Rochereau,
75014
Paris,
France
13 Observatorio de Yebes (IGN),
Apartado 148,
19180
Guadalajara,
Spain
14 Hartebeesthoek Radio Astronomy
Observatory, 1740
Krugersdorp, South
Africa
15 Federal Agency for Cartography and
Geodesy, Geodetic Observatory of Wettzell, 60598
Frankfurt Am Main,
Germany
16 Department of Earth and Space
Sciences, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
17 National Institute for
Astrophysics, Radio Astronomy Institute, Radio Observatory Medicina,
75500
Medicina,
Italy
18 Institute of Applied Astronomy,
Russian Academy of Sciences, Kutuzova Embankment 10, 191187
Saint-Petersburg,
Russia
19 School of Physical Sciences,
University of Tasmania, Private Bag
37, 7001
Hobart,
Australia
20 CSIRO Astronomy and Space Science,
Australia Telescope National Facility, Narrabri
NSW
2390,
Australia
21 Institute for Radio Astronomy and
Space Research, Auckland University of Technology, Private Bag 92006, 1142
Auckland, New
Zealand
22 Xinjiang Astronomical Observatory,
Chinese Academy of Sciences, 830011
Urumqi, PR
China
23 Yunnan Astronomical Observatory,
Chinese Academy of Sciences, 650011
Kunming, PR
China
24 Metsähovi Radio Observatory, Aalto
University, 02540
Kylmälä,
Finland
25 European Space Agency, ESA/ESTEC
Scientific Support Office, 2200AG
Noordwijk, The
Netherlands
Received:
7
May
2016
Accepted:
31
May
2016
Context. The closest ever fly-by of the Martian moon Phobos, performed by the European Space Agency’s Mars Express spacecraft, gives a unique opportunity to sharpen and test the Planetary Radio Interferometry and Doppler Experiments (PRIDE) technique in the interest of studying planet–satellite systems.
Aims. The aim of this work is to demonstrate a technique of providing high precision positional and Doppler measurements of planetary spacecraft using the Mars Express spacecraft. The technique will be used in the framework of Planetary Radio Interferometry and Doppler Experiments in various planetary missions, in particular in fly-by mode.
Methods. We advanced a novel approach to spacecraft data processing using the techniques of Doppler and phase-referenced very long baseline interferometry spacecraft tracking.
Results. We achieved, on average, mHz precision (30 μm/s at a 10 s integration time) for radial three-way Doppler estimates and sub-nanoradian precision for lateral position measurements, which in a linear measure (at a distance of 1.4 AU) corresponds to ~50 m.
Key words: techniques: interferometric / techniques: miscellaneous / methods: data analysis / astrometry
© ESO, 2016
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