Test object with a mass up to 50 kg
Frequency range 5 Hz … 4 kHz
Max acceleration* 720 m/s² (sine vibration)
Max acceleration* 480 m/s² (random vibration)
Max force 1,5 kN
EVS-EN 60068-2-6:2008
EVS-EN 60068-2-64:2008
ECSS-E-ST-10-03C
* Depends on the mass of the test object
Mechanical shock
Mechanical shock response spectrum up to 98 000 m/s2
Frequency range 1 Hz … 10 kHz
Test object with a mass up to 26 kg
ECSS-E-ST-10-03C
Thermal vacuum
Lowest pressure 5×10⁻⁷ hPa
Temperature range (-40...+150) °C
Chamber dimensions Ø 650 mm × 650 mm
ECSS-E-ST-10-03C
Climatic conditions
Temperature (-40…+150) °C
Relative air humidity* (30…90) %
Chamber dimensions 400 mm × 470 mm × 345 mm
ECSS-E-ST-10-03C
* Depends on the temperature
Electromagnetic compatibility
Immunity and emission
Frequency range 30 MHz …18 GHz
Distance from test object 1 m
Size of uniform field area 0,5 m × 0,5 m
Chamber dimensions 4 m × 3 m × 2,5 m
IEC/EN 61000-4-3
ECSS-E-ST-20-07C
Electrostatic discharge
Test voltage range ± (1...30) kV
IEC/EN 61000-4-2
ISO 10605
Current shortcomings in our understanding of dark matter distribution in our Galaxy and ongoing strategies for using the Milky Way to investigate the particle physics model for DM are discussed.
We are excited to announce the upcoming stellar spectroscopy workshop hosted by Tartu Observatory under the EXOHOST project, and we invite you to join us on 27–28 September in Tõravere or Zoom.
The cosmic web is vital for studying dark matter and the cosmological model and understanding galaxy evolution. However, detecting the cosmic web from observations is a complex task.