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.

Artist impression van de kern van het Centaurus Cluster

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.

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.

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.