Robotics in SRC PAS - LEMUR
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Written by Rafał Przybyła   
Space agencies and companies work on the program of sending into the orbit autonomous servicing satellites, which could repair  damaged commercial satellites. In October 2011 Space Mechatronics and Robotics Laboratory started the project "Design and construction of a prototype of the manipulator as a key component of the satellite orbit servicing system" implemented under the LEADER II program of National Centre for Research and Development. LEMUR, the name of the project was chosen by voting of the project team members.
 
Last Updated on Thursday, 25 April 2013 10:01
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History
1976
- 20 September:the Polish Academy of Sciences Presidium establishes the Space Research Centre

1977
- 1 February: the Space Research Centre officially begins its activity.
The scientific staff is a combination of small research groups from the Institute of Geophysics, the Astronomical Observatory of Warsaw University, the Warsaw University of Technology and the Institute of Mathematical Machines. The Centre  also includes the Astronomical Observatory in Borowiec (now the Astrogeodynamic Observatory) near Poznań and the Wrocław Heliophysics Labolatory of the PAS Institute of Astronomy (now the Solar Physics Division.)
Last Updated on Wednesday, 07 November 2012 12:18
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Mission
Mission

“The bright ideas of scientists have to be matched by the creativity of engineers and very high management standards”

The Space Research Centre is an interdisciplinary research institute of the Polish Academy of Sciences, established to conduct scientific research and activities in order to develop the space industry in Poland.

Our mission is the development and dissemination of space activities, which might help our country in achieving the image of the state actively involved in space research at world level and the creation of satellite technologies.

Last Updated on Wednesday, 07 November 2012 12:19
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Our research

our research

The smallest dust grains in the circumsolar dust cloud are the nanodust particles, i.e., the dust grains with the sizes of a few to a few tens millionth parts of millimeter. They are so small they include just several dozen thousands of atoms.

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Interplanetary space is filled with magnetized plasma from the Sun (the solar wind) and interstellar gas, mainly hydrogen and helium, which continuously flows through the heliosphere. The interstellar atoms are ionized by extreme ultraviolet radiation and the solar wind. In result of ionization of the interstellar atoms, new ions in the solar wind are created.

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The heliosphere is a region in the interstellar space filled with the solar wind plasma, emitted by the Sun. Since the Sun is traversing a partly ionized, magnetized cloud of interstellar gas, the solar wind expansion must be eventually arrested at a certain distance to the Sun. This happens in the locations where the solar wind pressure becomes equal to the pressure of the interstellar matter. Ultimately, however, the solar wind matter cannot accumulate infinitely inside the heliosphere and must find an exit path to the interstellar space. But where exactly is this path located? And is there just one evacuation path or more? These questions cannot be answered directly because up to now there have been just two active space probes – Voyager 1 and 2 – to reach the boundary regions of the heliosphere, and this happened in the regions least suspect of being anywhere close to the solar wind evacuation path. Therefore, answering these question can only be done by remote-sensing measurements and theoretical modeling.

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CBK PAN will participate in a NASA space mission Interstellar Mapping and Acceleration Probe (IMAP), scheduled for launch in 2024. The selection of the winning proposal submitted in response to the Announcement of Opportunity released in 2017, was announced in Washington DC on June 1, 2018 (https://www.nasa.gov/press-release/nasa-selects-mission-to-study-solar-wind-boundary-of-outer-solar-system).

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