Ventspils International Radio Astronomy Centre

Engineering Research Institute Ventspils International Radio Astronomy Centre (ERI VIRAC) of Ventspils University of Applied Sciences (VUAS) is a science education center specializing in the implementation of high-quality future research services in the field of space technology and signal processing.

The video was shot by a creative group led by film director Juris Pakalnītis.

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The strategic goal of ERI VIRAC is to become a major science centre in observational radio astronomy and related theoretical astrophysics, a global provider of research in space physics and services in space technology, based on an internationally competitive, balanced, and sustainable team of researchers. Research and services employ an internationally competitive infrastructure for astronomical observations and deep-space communications.


VIRAC operates a radio telescope site in Irbene, equipped with two completely rotatable, parabolic antennas RT-32 and RT-16, as well as a Low-frequency array (LOFAR) station.

Insight into history

  • The Irbene radio antenna complex was founded on June 10, 1967, as a secret Soviet astronomy and communications center to spy on Western communications.
  • VIRAC, was founded by the Latvian Academy of Sciences under the name Ventspils International Radio Astronomy Center on July 22, 1994, when the State Commission from the Russian Federation took over from the former Soviet Union, at the time of the transfer, the Russian Federation’s military unit at Irbene, in the Ventspils region (military object “Star”).
  • Two years later, VIRAC was reorganized as a state-owned scientific non-profit organization, a limited liability company.
  • On December 16, 2004, VIRAC was incorporated into the Ventspils University College (now Ventspils University of Applied Sciences – VUAS) as the VUAS Scientific Institute, which was registered on November 25, 2005, in the Register of Scientific Institutions of the Republic of Latvia.
  • On March 1, 2010, VIRAC added a second VUAS scientific institute – the Engineering Research Center (IPC), replacing the name of the institute with the current one.
  • On March 18, 2010, the VIRAC as a VUAS unit was re-registered in the Register of Scientific Institutions of the Republic of Latvia.
  • In 2013, the VIRAC became a VUAS unit with its Scientific Council, whose activities are determined by the Senate of the VUAS.
  • In 2016, VIRAC was admitted to the European Radio Astronomy Observation Network (EVN) and Latvia – JIV-ERIC.
  • In 2019, VIRAC became a member of ILT.
  • In 2021, VIRAC telescopes start to be used for practical, non-research purposes.
  • In 2025, VIRAC provides first services to spacecraft missions in faraway space.


  • ERI VIRAC Scientific Council

    • Juris Freimanis (chair), leading researcher
    • Artis Aberfelds, leading researcher
    • Vairis Caune (external, VUAS Faculty of Information Technologies)
    • Juris Kalvāns, leading researcher
    • Matīss Maltisovs, leading researcher
    • Ivars Šmelds, leading researcher
    • Juris Žagars, visiting leading researcher

  • Astronomy and Astrophysics Department

    Galaxy

    Studies of the interstellar medium (ISM) and circumstellar envelopes (CE). The investigations deepen knowledge on the circulation of cosmic matter in our Galaxy and the properties of matter and processes in extreme conditions in deep space. A major VIRAC research direction is observations of galactic masers - laser-like radiation in the radio wavelength range. Natural cosmic masers primarily occur in massive star-forming regions. Masers of methanol CH3OH and excited hydroxyl OH* are regularly monitored and analyzed with VIRAC radio telescopes in single antenna mode, as well as with a single-baseline interferometer consisting of RT-16 and RT-32. Formaldehyde H2CO masers have also been observed. The monitoring is supplemented by mapping of the astrophysical maser sources with the European large-scale radio interferometry network EVN. Theoretical aspects of ISM and CE are addressed by numerical modelling studies in astrochemistry, studying the accumulation of ices on dust grains in starless and star-forming dense interstellar clouds, often observed in the spiral arms of our Galaxy. Prebiotic organic synthesis occurs in these ices that could be essential for the emergence of life on Earth. Hence, we are also interested in the chemical aspects of the formation of stars, starting in dark cloud cores and up to the appearance of a protoplanetary disk. The above major topics are supported by investigations of radiation transfer in the gas-dust CEs of young protostars and evolved asymptotic giant branch stars.


    Solar system. 

    Systematic radio astronomical observations of solar active regions (sunspots and their groups) are performed with the VSRC radio telescope RT-32 in the microwave domain. Solar radiation maps at different frequencies with different (left and right circles) polarizations have been created with the help of self-built instrumentation. Research in solar physics explores the origin of solar wind originating from solar active regions, as well as magnetohydrodynamic waves and oscillations in the hot solar corona. A separate direction studies small solar-system bodies, focusing on comets that are interesting objects for spacecraft missions and are capable of maser emission. This emission is weak, prompting advances in data processing, and requires technological telescope improvements. An emerging field is investigating processes in the Earth's ionosphere, including single-station observations with LOFAR.

     

    High-energy and extragalactic astronomy. Active galaxies include quasars, radio galaxies, Seyfert galaxies, blazars, Markarian galaxies, and other objects with galactic nuclei hosting accreting supermassive black holes. With the VIRAC radio telescope RT-32, the variability of active galaxies has been studied. The characteristic time of variability cannot be significantly longer than the time (about a day) during which a signal traveling at the speed of light can cross the emitting area. Such observations can help to explain the mechanisms of galactic nuclei variability. Other high-energy astrophysical phenomena studied include fast radio bursts, elementary particle physics, and processes in accretion disks around stellar-mass black holes.


    • Juris Kalvāns

    Dr.phys., Leading researcher, Head of department

    juris.kalvans[at]venta.lv

    Scientific profile


    • Juris Freimanis

    Dr.phys., Leading researcher, assistant professor

    jurisf[at]venta.lv

    Scientific profile


    • Ivars Šmelds

    Dr.phys., leading researcher

    ivarss[at]venta.lv

    Scientific profile


    • Jānis Šteinbergs

    Mg.sc.comp., Research assistant, PhD student

    janis.steinbergs[at]venta.lv

    Scientific profile


    • Gints Jasmonts

    Mg.sc.comp., Research assistant, PhD student

    gints.jasmonts[at]venta.lv

    Scientific profile


    • Karina Šķirmante

    Mg.sc.comp., Researcher, lecturer, PhD candidate

    karina.skirmante[at]venta.lv

    Scientific profile



    • Kristaps Veitners

    Mg.phys., Research assistant

    kristaps.veitners[at]venta.lv

    Scientific profile


    • Jesus Cazares Montes

    PhD, Visiting leading researcher

    jesus.cazares[at]venta.lv

    Scientific profile


    • Aija Kalniņa

    Mg.phys., scientific assistant, PhD student

    aija.kalnina[at]venta.lv

    Scientific profile


    • Boris Ryabov

    Dr.phys., Leading researcher

    borissr[at]venta.lv 

    Scientific profile


    • Dmitrijs Bezrukovs

     Dr.phys., leading researcher

    dmitrijs.bezrukovs[at]venta.lv 

    Scientific profile


    • Vladislavs Bezrukovs

    Mg.sc.ing., Researcher, PhD candidate

    vladislavsb[at]venta.lv

    Scientific profile


    • Artis Aberfelds

     PhD, leading researcher, postdoc

    artis.aberfelds[at]venta.lv

    Scientific profile


    • Anete Egliene

    B.sc.phys.,  Astronomy technician

    anete.egliene[at]venta.lv


    • Valery Nakariakov 

    PhD, Visiting leading researcher

    V.Nakariakov[at]warwick.ac.uk

     Scientific profile


    • Ross Burns

    PhD, Visiting leading researcher

    rossburns88[at]googlemail.com

    Scientific profile


    • Dmitrii Kolotkov

    PhD, Visiting leading researcher

    D.Kolotkov.1[at]warwick.ac.uk

    Scientific profile


    • Artem Sukharev

    PhD, Visiting leading researcher

    magister_phys[at]yahoo.com

     Scientific profile


    • Anatolijs Popovs

     Dr.phys., Visiting leading researcher


    Sihui Zhong

    PhD, Visiting researcher

    S.Zhong3[at]exeter.ac.uk

     Scientific profile


  • Electronics and Satellite Technology Department

    The Electronics and Satellite Technology Department (ESTD) specializes in applied engineering research, with a strong focus on energy systems. Our work encompasses the full development cycle—from conceptual design and mathematical modelling to prototype production and patenting of innovative technologies.

    ESTD researchers actively contribute to scientific literature, including the publication of monographs. Complex engineering challenges, such as behaviour of materials under stress, are tackled using advanced numerical modelling techniques.

    Mathematical modelling and software algorithms are applied for solving real-world problems across diverse fields, including smart engineering systems, intelligent building infrastructure, satellite communications, cybersecurity, economics, and medicine.


    • Matīss Maltisovs

    PhD,  Leading researcher

     matiss.maltisovs[at]venta.lv

    Scientific profile


    • Valērijs Bezrukovs

     Dr.sc.ing., Leading researcher

     valerijs.bezrukovs[at]venta.lv

     Scientific profile


    • Viktors Gopejenko

     Dr.sc.ing., Leading researcher

     viktors.gopejenko[at]venta.lv

     Scientific profile


    • Marina Koņuhova

    Dr.sc.ing., Visiting leading researcher

     marina.konuhova[atventa.lv

     Scientific profile


    • Juris Žagars

    Dr.habil.phys., Visiting leading researcher

     juris.zagars[at]venta.lv 

    Scientific profile


    • Manfreds Leontijs Šneps-Šneppe

    Dr.habil.sc.ing., Visiting leading researcher

     manfreds.sneps[at]venta.lv

     Scientific profile


    • Svetlana Polukoško

     Dr.phys., Visiting leading researcher

     svetlana.polukosko[at]venta.lv

     Scientific profile



  • Engineering and Technical Operations Group

    The main tasks of the Engineering and Technical Operations Group (ETO):

    • Operation control, maintenance, and repair of RT-32 and RT-16 radio telescopes’ kinematic mechanical drive systems. Cleaning, repairing, and painting of the parabolic antenna’s supporting grid element and inspection of their technical condition. Maintenance and repair of RT-32 and RT-16 drive control systems, their operational compliance control, and improvement of functionality.

    • Automation of observations of radio astronomical radiation meeting the requirements of the European VLBI network (EVN). Configuration of field system components; the digitalisation, formatting, storage, and transferring of radio astronomical data. The development of observation procedure scripts and compliance with EVN requirements and provisions. The provision of automated observations of galactic masers and active galactic cores in a single-antenna mode.

    • Operation, control, repair, and reception of RT-32 and RT-16 cryogenic receivers. Maintenance of low-temperature cryostats and liquid He systems. The calibration of radio telescopes’ antenna parameters and receivers. The calibration and development of L-band and S-band receivers.

    • Maintenance of radio telescope complex power supply system. Maintenance, operation control, and technical modernisation of the automated electrical energy storage system established for the continuous operation of RT-32 and RT-16.

    • Maintenance and development of computer hardware and data transmission network. Maintenance, configuration, and repair of radio telescopes’ drive control, receiver control, weather station, and users’ computer systems. The maintenance of data transmission local and global network access devices and data safety systems.

    • Provision of radio telescope operator services. Conducting radio astronomical observations according to the approved observation schedule, signal registration, data compliance control, and data storage. Observations are conducted 24 hours a day, seven days a week.

    • Surveillance of Irbene territory. The continuous physical presence of personnel in the Irbene complex, surveillance of the territory, and control of critical infrastructure facilities.

    • Coordination of tourism and visitors. Creating and replenishing the exhibition with additional features. Coordination of excursions, supervision of guides, and accounting of revenue.

    Artūrs Orbidāns

    M.Sc., Acting Head of Department, Electronics Engineer

    arturs.orbidans[at]venta.lv

    Scientific profile


    Dr. Jānis Trokšs

    Dr.phys., Visiting Leading Researcher

    janis.trokss[at]venta.lv

    Scientific profile


    Mārcis Bleiders

    Mg.sc.ing., Electronics Engineer, guest lecturer

    marcis.bleiders[at]venta.lv

    Scientific profile


    Agris Bērziņš

    Mg. oec., Senior Mechanical Engineer

    agris.berzins[at]venta.lv

    Scientific profile


    Tatjana Dāvida

    Technical Specialist

    tatjana.davida[at]venta.lv


    Roksolana Amarova

    Junior Electronics Engineer

    roksolana.amarova[at]venta.lv


    Raitis Raikstiņš

    Senior Specialist

    raitis.raikstins[at]venta.lv


    Arnis Bērziņš

    Technical Specialist

    arnis.berzins[at]venta.lv


    Māra Klausa

    Technical Specialist

    mara.klausa[at]venta.lv


    Roberts Rasmanis

    Astronomy Technician

    roberts.rasmanis[at]venta.lv


    Zigurds Putniņš

    Technical Specialist

    zigurds.putnins[at]venta.lv


    Kristaps Blumbergs

    Junior Electronics Engineer

    kristaps.blumbergs[at]venta.lv


    Rodrigo Laurinovičs

    Junior Electronics Engineer

    rodrigo.laurinovics[at]venta.lv


    Guntis Gailums

    Junior Electronics Engineer

    guntis.gailums[at]venta.lv


    Andrejs Andrievs Dzelme

    Junior Electronics Engineer

    andrejs.dzelme[at]venta.lv


    Lita Bērziņa

    Caretaker

    lita.lapina[at]venta.lv


    Matīss Purviņš

    Developer

    s22purvmati[at]venta.lv


    Ruslans Golubevs

    Developer

    s21golurusl[at]venta.lv


    Kristaps Felzenbergs

    Visiting researcher

    kristaps.felzenbergs[at]venta.lv


    Nansija Jotkus

    Visiting scientific assistant

    nansija.jotkus[at]venta.lv


  • Services

    Observations with VIRAC radio telescopes


    Proposals for the use of the telescopes for scientific and applied (commercial) tasks have to be electronically submitted to VIRAC with the application template.


    Applications for long-term (more than one quarter) work series for the next calendar year have to be submitted by December 1 each year. The decision is announced to the submitters by December 20. Applications for short and medium-term work series have to be submitted quarterly, each year, until December 10, March 15, June 15, and September 15. The decision is announced to the submitters within 10 working days.


    Decisions on awarding or refusing observational time are made by the VIRAC Radio Telescope Time Allocation Commission. The decision of the Commission can be appealed to the VUAS rector within 5 days of the announcement of the decision. Following the “Regulation for employment of VUAS ERI VIRAC radio telescopes”, approved by VUAS Senate on June 21, 2017, a fee is applied for radio telescope employment. The fee may depend on the set of VIRAC services necessary for the proposal. Within the constraints of available budget funds, the cost can be fully or partially waived for the following observation proposals (in priority sequence):

    • observations and other resultative works necessary for the fulfillment of EVN, JIV-ERIC, and other VUAS international commitments;
    • observations and other resultative works in projects funded by the European Union if the outcome is expected to be published in high-impact journals and/or the research is conducted by the scientific personnel of VUAS;
    • observations and other resultative works conducted or led by VUAS ERI VIRAC employees, attracted experts, consultants, if the work is financed by the state budget and/or Ventspils City Council by more than 50 % of the total amount;
    • resultative works for projects and activities that ensure achieving VIRAC strategic aims, contribute new competence, or widen international cooperation;
    • observations and other resultative works for maintaining the VUAS study process;
    • if observations are conducted in the regime of short- or long-base interferometry network, involving telescopes RT-32 and RT-16 simultaneously.

    All data obtained in business-related observations are commercial secrets for at least one year but no longer than five years, and they must not be disclosed to third parties without the customer's consent.



    Computing with a high-performance computing cluster


    Conditions and form of applications for computing tasks with VUAS IE VIRAC High Performance Computing cluster (HPC).

    Applications for HPU use shall be submitted and addressed to the Director of VIRAC and shall be accepted within the following time limits.


    • Applications for long-term computing tasks shall be submitted by 1 December of each calendar year, and the decision shall be taken by 20 December, respectively. That point also corresponds to VIRAC employees who are required to apply for their planned computing tasks for the calendar year.
    • Applications for computing tasks for the following quarter shall be accepted by the 15th of the month following the previous quarter (15 December, 15 March, 15 June and 15 September).

    The application shall be submitted as an electronic .docx, .doc, .odt, or .pdf file, Times New Roman font, character size not less than 10 points. The applicant shall attach a scanned confirmation (.pdf file) with his or her signature on the authenticity of the application. The application fields marked with an asterisk (*) are mandatory. If the applicant is not an employee of any organisation, it must be indicated in the “Organization name” field.


    Conditions and application form (in Latvian).



  • Contacts

    • Director

    Mārcis Donerblics

    E-mail: marcis.donerblics@venta.lv


    • Chair of VIRAC scientific council:

    Juris Freimanis, jurisf [at] venta.lv


    • Chair of the VIRAC Radio telescope time allocation commission:

    Juris Freimanis, jurisf [at] venta.lv


    • On scientific astronomical matters, including student works, contact the head of VIRAC Astronomy and astrophysics department:

    Juris Kalvāns, juris.kalvans [at] venta.lv



    Excursions

    Questions about excursions, tour prices, excursion offer, tour times:   +37129230818 



    Office

    9:00 - 17:00

    Administration: +37163629656



    E-mail

    General issues,requests, offers. 

    virac@venta.lv



    VIRAC in Ventspils

    Inženieru street 101,Ventspils, LV-3601

    Phone +37163629656

    E-mail virac@venta.lv



    VIRAC in Irbene

    VIRAC, Ventspils district. Ance parish., Irbene, LV-3601

    Security/Guard +37163656081


  • Excursions

    EXCURSION SEASON AT THE IRBENE COMPLEX ISFROM APRIL 1ST TO NOVEMBER 1ST


    As of September 1, 2025, excursions will not be available due to technical reasons.


    Activities included in the excursion:

    • A walk AROUND radio telescope RT-32 in the territory of Irbene
    • RT – 8 tower viewing and expositions about RT – 32 and RT – 16 during the USSR
    • Viewing the “old” RT – 16 antenna next to RT – 8
    • Walk through an underground tunnel

    Book excursion at least 3 days before visiting!


    Tourist service tariff:

    • Excursion for a group of less than 10 people - 100 EUR

    Individual prices (for a group of more than 10 people):

    • Adults – 12 EUR
    • Students, pensioners – 8 EUR
    • For students, children from 6 years of age – 6 EUR

    If you have decided to visit us send an e-mail to virac@venta.lv or call and apply for an excursion by phone +371 29230818


    Rules to follow in the excursion:

    • Excursion time is around 1,5-2 hours.
    • Excursions are possible only with our guide.
    • Excursions happen after a prior set appointment.
    • Visitors have to follow the instructions of the staff.
    • Visitors should switch off their mobile phones and other devices that broadcast in the radio frequency range or turn them on to “flight mode”.

  • Additional information

    VIRAC is responsible for many of VUAS scientific publications and research projects.


    VUAS publications

    VUAS projects

    VIRAC homepage (currently not updated, actual information is available on https://en.venta.lv/about-science-in-vuas )


Events and Highlights

By Rota Rulle November 8, 2025
Electronics engineering students from Ventspils University of Applied Sciences (VUAS) developed a probe that carried a can of “Rudy’s Kombucha” into near space, reaching an impressive altitude of 28,690 meters – nearly 30 kilometers above the Earth’s surface. While trying to locate the probe afterward, the students encountered major GPS signal disturbances across the Kurzeme region, so they called on radio amateurs for assistance. Working together, they successfully located the probe near Dobele. The space mission probe was equipped with a GoPro camera that captured both the launch and the breathtaking flight. After the controlled explosion of the probe’s balloon at nearly 30 kilometers altitude, a parachute opened, ensuring the can’s safe return to Earth. The probe was launched from Ventspils airfield and, after flying approximately 140 kilometers, landed near Dobele. Jānis Šate, Director of the Electronics Engineering study program at Ventspils University of Applied Sciences, explained: “The company knew that our students develop probes, and they had the idea to attach a beverage can and launch it into space. Technically, it’s more accurate to say it was launched into the stratosphere. We discussed it in August, and within a few months, the electronics engineering students built the probe. It’s a group project in the third year of studies, and this collaboration added extra value. The most challenging part of launching the probe is creating the electronic system attached to the parachute and helium balloon. The balloon rises to about 30 kilometers, where air pressure drops, the balloon bursts, and the probe descends to Earth. Launching it is easy – the hard part is tracking and recovering it afterward. A GPS navigation system is required to continuously transmit the probe’s location. The students’ task was to design an electronic system that can operate in the stratosphere, where temperatures drop to –40°C.” “We coordinated the launch with the Civil Aviation Agency since air traffic is affected, and we also arranged it with Ventspils Airport. Eventually, the probe was found near Dobele, though there were unexpected complications – due to the global situation, GPS communications are regularly disrupted from Königsberg (Kaliningrad, Russia). Unfortunately, we launched on one of those days when signal interference over Kurzeme and the Baltic Sea was particularly strong. That meant that when the probe ascended above ten kilometers, our system showed it was no longer over Kuldīga, but over Kaliningrad. From there, spoofed GPS signals were being transmitted to mislead moving objects.
By Rota Rulle November 4, 2025
In October, VUAS COLOURS WP5, headed by Lasma Asme, joined other representatives from COLOURS partner universities gathered at Garage33, Paderborn University, Germany, for a dynamic CoLab dedicated to Mental Health, Body Image, and Equality, Diversity, and Inclusion (EDI). The three-day event, which is part of the COLOURS CoSpace initiative, brought together students, researchers, and staff from across Europe to exchange perspectives and co-create innovative approaches under the smart specialisation area of Health and Well-being. Participants from a very diverse background, under the moderation of Dr Christine Hante-Koch and Dr Alena Diedrich, discussed how issues like body dissatisfaction, eating disorders, anxiety, and depression are closely connected and how promoting a positive body image can make a real difference for people’s health. Using design thinking processes, the group also worked on the importance of creating fair and inclusive support systems that meet the needs of different communities, including women, LGBTQ+ individuals, and people facing disabilities, financial struggles, or migration challenges. The participants were divided into 4 groups and had cases ranging from how to deal with women who survived breast cancer, to isolated international students living in other countries, and how to make gamers more active while utilizing their special skills and enlarging their comfort zone. At the end of the event, each group pitched their ideas, solutions, and next steps. These solutions were evaluated and challenged by a panel of experts from multiple disciplines, with the example of Martin Persson, Professor of Health Sciences at Kristianstad University. The CoLab encouraged teamwork, creativity, and cultural exchange. The ideas developed in Paderborn will help shape future COLOURS activities and strengthen collaboration between partner universities committed to building healthier and more inclusive learning environments and society at large.
By Rota Rulle October 13, 2025
A wide US – Europe network of radio telescopes including observing a faraway radio galaxy discovers a small dark object. It is just a pinch in their data but it signifies that low-mass dark matter clumps are widespread, verifying theories of the Universe’s structure and evolution. The telescopes used include those of VUAS institute “Ventspils International Radio Astronomy Centre” (VIRAC). An international team of astronomers has found a low mass dark object in the distant Universe, not by directly observing any emitted light, but by detecting its tiny gravitational distortion of the light from another distant galaxy. This mysterious object has a mass of about one million times that of our Sun, and its discovery seems consistent with the current best theory about how galaxies like our own Milky Way formed. “Since we can’t see dark matter objects directly, we instead use very distant galaxies as a backlight to look for the gravitational imprints of such objects.” “Hunting for dark objects that don't seem to emit any light is clearly challenging,” said Dr. Devon Powell at the Max Planck Institute for Astrophysics (MPA) and lead author of the study published in Nature Astronomy. “Since we can’t see them directly, we instead use very distant galaxies as a backlight to look for their gravitational imprints.” Dark matter is an enigmatic form of matter not expected to emit light, yet it is essential to understanding how the rich tapestry of stars and galaxies we see in the night sky evolved. As a fundamental building block of the universe, a key question for astronomers is whether dark matter is smooth or clumpy, as this could reveal what it is made of. As dark matter cannot be seen, its properties can only be determined by observing the gravitational lensing effect, whereby the light from a more distant object is distorted and deflected by the gravity of the dark object, creating a characteristic arc in the processed image. The team used a network of telescopes from around the world, including the Green Bank Telescope (GBT), the Very Long Baseline Array (VLBA) and the European Very Long Baseline Interferometric Network (EVN). The latter includes the VIRAC radio astronomical observatory in Irbene. The data from this international network were correlated at the Joint Institute for VLBI ERIC (JIVE) in the Netherlands, forming an Earth-sized super-telescope that could capture the subtle signals of gravitational lensing by the dark object. They discovered that the object has a mass a million times greater than that of our Sun and is located in a distant region of space, approximately 10 billion light years from Earth, when the universe was only 6.5 billion years old. “From the first high-resolution image, we immediately saw a pinch in the gravitational arc, which is the tell-tale sign that we were onto something.” This is the lowest mass object to be found using this technique, by a factor of about 100. To achieve this level of sensitivity, the team had to create a high-fidelity image of the sky using radio telescopes located around the world. Professor John McKean from the University of Groningen (RuG), the University of Pretoria (UP) and the South African Radio Astronomy Observatory (SARAO), who led the data collection and is the lead author of a companion paper, said: “ From the first high-resolution image, we immediately saw a pinch in the gravitational arc, which is the tell-tale sign that we were onto something. Only another small clump of mass between us and the distant radio galaxy could cause this.” To analyse the massive dataset, the team had to develop new modelling algorithms that could only be run on supercomputers. “The data are so large and complex that we had to develop new numerical approaches to model them. This was not straightforward as it had never been done before,” said Dr Simona Vegetti at MPA. “We expect every galaxy, including our own Milky Way, to be filled with dark matter clumps, but finding them and convincing the community that they exist requires a great deal of number crunching,” she continued. The team applied a special technique called gravitational imaging, which allowed them to ‘see’ the invisible dark matter clump by mapping its gravitational lensing effect against the radio-luminous arc. “We expect every galaxy, including our own Milky Way, to be filled with dark matter clumps” “Given the sensitivity of our data, we were expecting to find at least one dark object, so our discovery is consistent with the so-called ‘cold dark matter theory’ on which much of our understanding of how galaxies form is based,” said Powell. “Having found one, the question now is whether we can find more and whether the numbers will still agree with the models.” The team are now analysing the data further to better understand what the mysterious dark object could be, but they are also looking into other parts of the sky to see if they can find more examples of such low-mass dark objects using the same technique. If they continue to find such mysterious objects in other parts of the universe, and if they really turn out to be completely devoid of stars, then some theories of dark matter may be ruled out.
By Rota Rulle October 7, 2025
This academic year, the VUAS Lifelong Learning Centre is offering a new lecture cycle, "Science and Culture - for Society", featuring lectures by renowned scientists and distinguished personalities in Latvia, held once a month on Saturdays. On October 11, lectures by Juris Dzelmes, a leading researcher at the Institute of Chemical Physics of the University of Latvia, are scheduled to discuss the challenges of artificial intelligence. In parallel with research in the field of chemical physics, J. Dzelme's interests encompass problems in educational management, philosophy, psychology, and art, and he will discuss the possibilities, development, and threats of artificial intelligence. October 11 at 7 p.m. 11.30–14.30, at Ventspils University of Applied Sciences, J. Dzelme will give an insight into the following topics: Digitalisation, robotisation, artificial intelligence (AI) and superintelligence; Emotions, free will and creativity in artificial and natural neural networks (AI and psyche); AI ethics, value and goal modelling; Supporting communities in an AI-driven world through art and philosophy, through physics and psychology. Application: https://www.venta.lv/muzizglitiba/pieteiksanas Price: 35 EUR More information: mic@venta.lv, tel. 63629650 
By Rota Rulle October 3, 2025
On September 26, the European Researchers’ Night events took place throughout Latvia, where colleges, universities, and scientific institutes opened their doors to visitors, offering a variety of free activities. At the VIZIUM Science Center, activities organized by Ventspils University of Applied Sciences and the Ventspils International Radio Astronomy Center (VIRAC) introduced visitors to the processes of star formation, comets, and other small bodies of the Solar System. Throughout the evening, visitors played language games, observed stars and planets through a telescope, and tried their hand at solving a mathematical puzzle – the Tower of Hanoi. Guests also had the opportunity to test their knowledge in various quizzes related to space and languages, gaining new insights along the way.
By Rota Rulle September 25, 2025
On 24 September 2025, a delegation from the University of Latvia Faculty of Science and Technology (UL FST) visited Ventspils University of Applied Sciences (VUAS). The UL delegation included FST Dean Aigars Ekers, Acting Vice-Dean for Science Sandris Lācis, Vice-Dean for Studies Aiga Švede, Vice-Dean for Development Diāna Šmite, and Head of the Department of Physics Tija Sīle. VUAS and the Ventspils International Radio Astronomy Centre (VIRAC) were represented by Rector Andris Vaivads, Dean of the Faculty of Information Technology Vairis Caune, Head of the Doctoral School Lilita Sproģe, Chairman of the VUAS Senate and, at the same time, Chairman of the VIRAC Scientific Council Juris Freimanis, along with other researchers and teaching staff. The visit began with a trip to the VIRAC radio telescope complex in Irbene, where senior researcher Artis Aberfelds introduced the guests to the telescopes, associated equipment, and laboratories, and their use in astronomical observations. After a joint lunch at VUAS café Panorāma, Jānis Šate showed the guests the university's electronics teaching laboratories and their equipment. The event reached a productive apogee in a joint discussion lasting around two hours in the VUAS Rectorate conference hall. At its opening, Rector Andris Vaivads gave a presentation about VUAS, followed by a presentation by, Juris Kalvāns, Head of the VIRAC Astronomy and Astrophysics Department, about the main research directions in VIRAC astronomy, while researcher Vladislavs Bezrukovs outlined VIRAC's extensive international cooperation, particularly its participation in European Research Infrastructure Consortia (ERIC). “The event reached a productive apogee in a joint discussion lasting around two hours in the VUAS Rectorate conference hall, where Rector Andris Vaivads gave a presentation about VUAS.” The discussion covered a range of topics related to science and studies. Both sides expressed interest in officially involving VUAS in the UL Master’s programme in Physics, alongside Daugavpils University. VIRAC researchers already teach several astronomy courses within this programme. The potential involvement of the VIRAC high-performance computing cluster in a new computing consortium, where UL is expected to take the leading role, was also discussed. Looking further ahead, UL is also interested in gaining access to VIRAC satellite communication abilities. Finally, the UL–VUAS cooperation agreement is to be renewed, including matters of collaboration in doctoral studies and research, as well as Latvia’s participation in the International Astronomical Union. The meeting took place in a frendly atmosphere, giving confidence in the successful continuation of cooperation between UL and VUAS.
By Rota Rulle September 22, 2025
From 8 to 19 September, Ventspils University of Applied Sciences hosted the scientific workshop “VIRAC Summer School on Pulsar Observations at Centimetre and Metre Wavelengths”, organized by the Ventspils International Radio Astronomy Centre (VIRAC). The event brought together researchers and students from Latvia and abroad. The summer school aimed to develop knowledge and practical skills in pulsar observations, radio astronomical data processing, and international scientific collaboration. Over two weeks, participants attended lectures and hands-on sessions on the fundamentals of pulsar astronomy, observation planning, and data analysis, with a special focus on observations with the LOFAR low-frequency antenna array. The summer school was led by VIRAC researchers Jānis Šteinbergs and Vladislavs Bezrukovs. Special guest lecturers Dr. Alisa Shevtsova and Dr. Ihor Kravtsov from the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine shared their expertise on the physical properties of pulsar emission and low-frequency research methods. What are pulsars? - Pulsars are extremely dense, rapidly rotating neutron stars that emit powerful radio pulses at regular intervals. These signals are so precise that they are often compared to cosmic clocks. Observations of pulsars with modern radio telescopes help scientists study extreme physical conditions, the properties of the interstellar medium, and the large-scale structure of the Universe. VIRAC conducts research in radio astronomy, space technologies, and data processing, and operates the Irbene Radio Telescope Complex - one of the most advanced facilities of its kind in Northern Europe. One of the key instruments is LOFAR (Low Frequency Array), a Europe-wide network of low-frequency radio telescopes that connects hundreds of antenna stations across multiple countries, including Latvia. Ventspils University’s participation in the JIV-ERIC and LOFAR-ERIC (European Research Infrastructure Consortium) strengthens Latvia’s integration into the international radio astronomy community. It provides opportunities to conduct observations across the radio spectrum of the Universe. The summer school fostered collaboration between Ventspils University of Applied Sciences, the University of Latvia, and Riga Technical University, while also facilitating the exchange of experience with research institutions from Europe and Ukraine. The event was implemented within the framework of the European Regional Development Fund project No. 1.1.1.5/3/25/I/012 “Ventspils University of Applied Sciences` International Cooperation and Innovation for the Development of Latvia’s Smart Specialisation”
By Rota Rulle September 16, 2025
On Friday, September 12, the Latvian partners of the project “MarTe: Marine technology excellence hub for sustainable blue economy in Baltics” gathered in Ventspils. Representatives from the Ventspils Freeport Authority, the Investment and Development Agency of Latvia (LIAA), the World Wide Fund for Nature (WWF) Latvia, the Kurzeme Planning Region, the Latvian Institute of Aquatic Ecology, the association “Baltic Coasts”, and Ventspils University of Applied Sciences met to learn more about the local business environment and discuss opportunities for cooperation in promoting the blue economy. As part of the visit, the partners toured the Ventspils Freeport Authority to learn about the port’s operational areas and future development directions. They also visited the Freeport’s industrial clients, including SIA “Bio-Venta”, the largest biodiesel production and transshipment complex in the Baltic States, where partners were introduced to the company’s production processes and end products — biodiesel, rapeseed oil, rapeseed meal for animal feed, and glycerine. In addition, the partners visited the manufacturing company SIA “Aspired”, a CNC service provider, and Ventspils University of Applied Sciences to explore production capabilities and potential cooperation in human resource development. The MarTe project is focused on addressing environmental changes and fostering regional economic development. Within the project, a cross-border Centre of Excellence will be established to promote innovation, strengthen the marine value chain, and encourage the adoption of new technologies. The project’s objectives include joint research and development (R&D) activities to support the sustainable use of marine resources, strengthen ecosystems, and drive policy impact. Through quadruple-helix collaboration (linking academia, business, government, and civil society), MarTe aims to advance marine and maritime technologies, enhance stakeholder cooperation, build ecosystem capacity, bridge knowledge gaps, support SMEs and startups, and increase the visibility of blue economy innovation ecosystems in Estonia and Latvia. The project’s strategic framework focuses on coastal energy, smart ports, and marine ecosystem protection, in line with the EU Green Deal and regional Smart Specialisation Strategies. The goal of the project “MarTe: Marine technology excellence hub for sustainable blue economy in Baltics” is to develop practical solutions and policy recommendations to advance the blue economy — the sustainable use of marine and ocean resources — in Estonia and Latvia. A total of 13 organisations are involved in the project, with an emphasis on innovation in marine technologies, particularly in renewable energy, smart port development, and marine environmental protection, thereby strengthening cooperation between science, industry, public administration, and non-governmental organisations. This project has received funding from the European Union’s Horizon Europe programme, under the “Excellence Hubs” subprogramme (HORIZON-WIDERA-2023-ACCESS-07-01). The project’s lead partner is the Estonian Environmental Investment Centre (Sihtasutus Keskkonnainvesteeringute Keskus). The total project budget is €4,999,822.50, of which €367 850,00 is budget of Ventspils University of Applied Sciences. The project will run until 31 December 2028.
By Martina Bertāne September 3, 2025
We are pleased to invite you to participate in the VIRAC Summer School on Pulsar Observations at Centimetre and Metre Wavelengths: Ventspils, Latvia |September 8–19, 2025 This intensive and inspiring summer school is designed for Master’s students, PhD candidates, and early-career researchers in astronomy and astrophysics. The event is hosted by Ventspils University of Applied Sciences. Key Topics: Pulsar observations with the LOFAR telescope Pulsar astronomy fundamentals Observation planning Pulsar data processing and analysis Venue: Engineering Research Institute – Ventspils International Radio Astronomy Centre, Ventspils University of Applied Sciences, Room 407
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