News and Events (in Russian for the time being)

Using data gathered by Russian LEND neutron telescope onboard NASA's Lunar Reconnaissance Orbiter, IKI scientists studied water ice distribution within lunar polar craters Cabeus and Galimov.

In 2024, IKI scientists and their colleagues completed the analysis of the data from the Milky Way central region deep survey and the first five all-sky surveys (2019–2022) made by Mikhail Pavlinsky ART-XC telescope onboard Spektr-RG X-ray observatory.

New model developed by IKI astrophysicists and their colleagues and based on the data of SRG/eROSITA X-ray telescope, links the bright structure seen in our Galaxy to bubbles of hot gas that emerge from star-formation regions like smoke from the chimney.

Having measured HCl and water ice abundance in Martian atmosphere with the ACS spectrometer onboard TGO mission, scientists showed that it is HCl uptake onto water ice cloud particles that can swiftly reduce the content of HCl in the atmosphere.

Plasma parameters on the borders of the heliosphere help small interstellar dust particles permeate deep into Solar system, according to a new model developed by IKI researchers Egor Godenko and Vladislav Izmodenov. This also suggest that we can study the properties of interstellar matter by measuring its characteristics in our closest neighbourhood.

New model developed by IKI scientists and their colleagues from Ioffe Institute sheds new light on the origin of W50 giant radio nebula, which hides the most reknown X-ray object of our Galaxy – SS433 microquasar.

On August 8, 2024 BTN-M1 instrument onboad Russian segment of the ISS resumed gamma-ray bursts (GRBs) monitoring together with Russian neutron spectrometer HEND (onboard NASA's Mars Odyssey mission). Just the day after they detected new GRB240809A from hypernova at a distance z ~ 1.5.

Using data from ACS spectrometer onboard TGO spacecraft, IKI scientist Ekaterina Starichenko and her colleagues studied gravity waves in Martian atmosphere, from the surface to the 160-km height, and the effect, which seasonal changes and dust storms have upon them. Results were published in the Astronomy&Astrophysics.

Scientists from Institute of Volcanology and Seismology, Computing Center of the RAS Far-Eastern Branch, IKI and Planeta Center For Space Hydrometeorology made the discovery, using satellite data and VolSatView infromation system. By the early June, 2024 the dome was already 100 meter high.

On 20th May 2024 IKI instuments, working near the Red Planet, caught it and stayed safe.