WISPIT
Wide Separation Planets in Time
Encouraged by our success with the YSES survey, we expanded our parameter search to include all young stars across the sky visible from the VLT, and ended up with a sample of 180 stars covering ages from 2 Myr up to 20 Myr.
The Wide Separation Planets in Time (WISPIT) survey is being carried out over several periods since 2022, and to date (Jen 2026) has produced two exoplanet systems.
WISPIT 1b and 1c
WISPIT 1 is a stellar binary with a primary star of around one solar mass, with two comoving companions identified as gas giant exoplanets (van Capelleveen et al., 2025).
WISPIT 2
We detected a spectacular circumstellar disk which has several cleared rings within it. The widest ring has a protoplanet of about 5 Jupiter masses (van Capelleveen et al., 2025), and is detected as a point source in the optical Hydrogen alpha line indicating that is is undergoing acitve accretion within this cavity (Close et al., 2025).