SRON pinpoints large brief methane releases

SRON scientists discover dozens of methane plumes every week using the Dutch space instrument TROPOMI. To locate their sources, they then zoom in with other satellites. However, brief methane releases have typically ended before those satellites arrive at the scene. The team has now developed a new method that is fast enough to catch the largest of such emissions. Publication in Geophysical Research Letters.

Astronomers finally discover double white dwarf set to explode into supernova

A small international team of astronomers including Silvia Toonen (UvA) and Gijs Nelemans (RU, KU Leuven and SRON) has discovered two white dwarf stars orbiting each other that will merge and explode into a type Ia supernova. This missing link in astronomy has long been predicted. The researchers publish their findings today in Nature Astronomy.

Name SRON becomes acronym: Space Research Organisation Netherlands

The Dutch institute for scientific space research SRON has a new logo, a new name, a new corporate identity and a completely revamped website with effect from Wednesday 26 March 2025. From now on, SRON stands for Space Research Organisation Netherlands (SRON).

Earth as seen from space in dark and lighter blue in this picture, is one of the typical new brand style images of SRON
Artist impression van de kern van het Centaurus Cluster

Duo of Satellites Detect Large Methane Emission from Ethiopian Volcano

SRON—als onderdeel van de Europese CAMS service—en GHGSat hebben een grote hoeveelheid methaan gedetecteerd boven Mount Fentale, een actieve vulkaan in Ethiopië. De uitstoot lag op 31 januari rond de 58 ton/uur en is opgespoord door een tip-and-cue-methode, waarbij het TROPOMI Sentinel-5p satellietinstrument van het Europese Copernicus programma en de Canadese satelliet GHGSat samenwerken.

Dutch satellite instrument SPEXone produces aerosol world map

NASA lanceerde op 8 februari 2024 klimaatsatelliet PACE met aan boord het Nederlandse fijnstofinstrument SPEXone. Een jaar lang observeren levert nu een driedelige wereldkaart op van aerosolen. Die toont de verspreiding van fijne en grove aerosolen en van deeltjes die zonlicht reflecteren of juist absorberen. Dat laatste heeft respectievelijk een afkoelend en opwarmend effect op het klimaat. SPEXone is gebouwd door SRON en Airbus Netherlands, met ondersteuning van TNO.

TRAPPIST planet dissected: volcanic rock or atmosphere full of CO2 and haze

Astronomers have used the James Webb Space Telescope to measure the infrared spectrum of a rocky planet in the auspicious planetary system of TRAPPIST-1. It is what you’d expect from a planet covered in volcanic rock. Another scenario includes an atmosphere full of CO2 and smog. The team, including Michiel Min (SRON), publishes the results in Nature Astronomy.

XMM-Newton celebrates 25 years in space

On December 10th, ESA’s X-ray observatory XMM-Newton celebrates 25 years in space. SRON contributed to one of XMM-Newton’s three instruments—the Reflection Grating Spectrometer. From planets to black holes, the space telescope has delivered many ground-breaking observations of a variety of celestial objects. Let’s take a look at four fascinating discoveries from the past five years.

White paper: NL-US collaboration in climate research from space

In oktober 2024 kwamen wetenschappers uit Nederland en de Verenigde Staten bijeen op de Nederlandse ambassade in Washington om hun expertise te delen over broeikasgassen, reactieve gassen, wolken en aerosolen. Deze thema’s zijn belangrijk voor klimaatonderzoek. In een whitepaper formuleren ze acties die  antwoord gaan geven op urgente klimaatvragen.

From atoms to the cosmos: ‘Everything in the universe is connected’

Kunnen we de grootste structuren in het universum onderzoeken door te kijken naar de kleinste deeltjes? Daarover gaat het onderzoek van Lydia Stofanova, promovendus aan de Leidse Sterrewacht en SRON—het Nederlandse instituut voor ruimteonderzoek. Ze bestudeert hoe elementen zoals zuurstof de grootschalige structuur van het universum beïnvloeden. Op 13 november verdedigde ze haar proefschrift.

PRELIFE consortium receives NWA grant to study origins of life

An interdisciplinary research consortium, including Floris van der Tak (SRON/RUG) and Michiel Min (SRON) has been awarded an NWA grant by the Dutch Research Council (NWO) to investigate the origin of life on Earth and in the universe. The so-called PRELIFE consortium (Pathways, Reactions and Environments) receives €6.7 million to explore this research question.

Gold antenna increases sensitivity detectors for proto-planetary systems

Researchers at SRON and TU Delft have made bolometer detectors thirty percent more sensitive. Bolometers form the heart of terahertz spectrometers that can distinguish colors up to one-millionth of their wavelength. This is needed to observe astrophysical processes such as the birth of stars and planets from gas and dust clouds. The enhancement should cut the time in half that it takes a space telescope to take a spectrum.

Golden antenna improves sensitivity detectors for proto planetary systems

Researchers at SRON and TU Delft have made bolometer detectors thirty percent more sensitive. Bolometers form the heart of terahertz spectrometers that can distinguish colors up to one-millionth of their wavelength. This is needed to observe astrophysical processes such as the birth of stars and planets from gas and dust clouds. The enhancement should cut the time in half that it takes a space telescope to take a spectrum.

Kick-off Astrophysics Centre for Multimessenger studies in Europe

The Astrophysics Centre for Multimessenger studies in Europe (ACME) has kicked off its activities in Paris. This EU-funded project aims to optimize the  European-wide accessibility and cohesion of multiple astroparticle and astronomy research infrastructures, such as VIRGO, KM3NeT, Auger Prime and LOFAR, to realize multi-messenger astrophysics.

PRIMA selected as candidate for NASA’s Probe mission

Out of the eight projects that competed to become NASA’s Probe mission, only two remain. The Probe far-Infrared Mission for Astrophysics (PRIMA) and the Advanced X-ray Imaging Satellite (AXiS) have been selected for the second round. SRON delivers the detectors for PRIMA, developed together with TU Delft.

First XRISM results: ten-billion-degree supernova remnant and dust donut at 0.1 light years from black hole

Following its launch on September 7th, 2023, and the subsequent series of tests, the XRISM X-ray telescope has produced its first two scientific papers. The team marveled at a temperature of ten billion degrees Celsius inside a supernova remnant. And it measured the distance of the dust ring around a supermassive black hole. In the case of NGC 4151, this turns out to be 0.1 light years. SRON has developed the filter wheel and an X-ray source used to calibrate the energy scale of the Resolve instrument.

Astrophysics in the lab: TES detectors measure X-rays from hot plasma

SRON has joined forces with the Max Planck Institute for Nuclear Physics (MPIK) and the Institut de Recherche en Astrophysique et Planetologie (IRAP) to generate reference data for astronomical observations and scrutinize the laws of hot plasma physics. The electron beam ion trap (EBIT) at MPIK in Heidelberg simulates a hot plasma, while superconducting transition-edge sensors (TES) developed by SRON measure the emitted  X-ray spectra with unprecedented energy resolution.

SRON to detect methane plumes for the Copernicus Atmosphere Monitoring Service

SRON has been selected by the European Copernicus Atmosphere Monitoring Service (CAMS) to provide satellite data analysis for its new monitoring service on methane emissions. CAMS provides atmospheric information to policymakers, businesses and citizens. It delivers real-time European air quality analyses and forecasts as well as observation-based emission estimates.

Climate models give different predictions on sulfate aerosol formation

The cooling effect of aerosols adds an uncertainty of almost one degree in climate models. Sulfate aerosols are one of the most impactful types. An analysis of several widely-used models now concludes that their predications on the creation of sulfate aerosols in the atmosphere differ almost as much as a factor of two. The PACE satellite will help to reveal which models are most accurate. Publication in Journal of Geophysical Research