My dad had this old astronomy encyclopaedia with a photo of the Orion Nebula, and one line about the blister model stuck with me for years before I even knew whose idea it was. Read about Frank Pieter Israel properly for the first time just now. 79.
Their story
Frank Pieter Israel was a Dutch astronomer and professor at Leiden Observatory whose work on star-forming regions and the interstellar medium of nearby galaxies shaped radio and millimetre astronomy for half a century. He died in Leiden on 18 September 2026 at the age of 79. Leiden University and Stichting…
Frank Pieter Israel was a Dutch astronomer and professor at Leiden Observatory whose work on star-forming regions and the interstellar medium of nearby galaxies shaped radio and millimetre astronomy for half a century. He died in Leiden on 18 September 2026 at the age of 79. Leiden University and Stichting Skepsis, the Dutch sceptical organisation he chaired for more than a decade, remembered him as an erudite colleague, sharp debater and gifted storyteller who remained a familiar presence in the Observatory long after formal retirement.
He was born in Delft on 31 December 1946 and attended the Stedelijk Gymnasium in Assen, graduating in 1965. Fascinated by space exploration from an early age, he wrote for amateur astronomy magazines before studying astronomy at Leiden. Under Professor Harm Habing he completed a PhD in 1976 on radio observations of ionised gas with the Westerbork Synthesis Radio Telescope. During that research he developed the blister model of H II regions, in which young massive stars form near the edge of a molecular cloud and drive heated gas outward. Decades later a NASA visualisation of the Orion Nebula closely matched the structure he and colleagues had predicted, bringing renewed attention to an idea first framed in his doctoral years.
From 1977 to 1980 he worked at the Owens Valley Radio Observatory at Caltech in Pasadena. He then joined ESA/ESTEC in Noordwijk for millimetre and submillimetre studies of molecular gas before returning to Leiden Observatory in the mid-1980s. Much of his later research asked how stars form from gas and dust in galaxies beyond the Milky Way. He studied the Magellanic Clouds and the central regions of larger systems, and he showed that using carbon monoxide as a tracer of molecular hydrogen is less straightforward than often assumed when chemistry or radiation fields differ. In 2005 he became full professor and Director of Education in Astronomy, teaching generations of students about nearby galaxies. He became professor emeritus in 2012 but continued to analyse data and publish. Over his career he used successive generations of radio, millimetre and submillimetre facilities, from SEST and JCMT to Herschel, APEX and ALMA. Asteroid 7507 Israel is named after him.
Israel also chaired Stichting Skepsis from 2012 to 2023, arguing for careful, evidence-based scrutiny of extraordinary claims in public life as well as in science. He co-founded Space Expo in Noordwijk, helped preserve Leiden's Old Observatory through the Stichting Behoud Leidse Sterrewacht, and gave many public lectures that made astronomy approachable beyond the university. He is survived by his wife Isa and their children, Marinus and Adriana. Colleagues said they would remember his scientific drive, humour and distinctive short laugh in the corridors of Leiden Observatory.
Biography adapted from Wikipedia (CC BY-SA 4.0), Leiden University in memoriam by Ignas Snellen, Stichting Skepsis, Wikidata. Wikipedia ↗

That NASA visualisation years later matching his prediction still gets me