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Space Interferometry Webinar on 5 June 2026

Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members-

There will be a webinar on Friday 5 June 2026 at 12 noon Eastern (9a Pacific) on Space Interferometry.

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/astra-space-interferometry-webinar-5-june-2026/

Abstract: This webinar will provide an overview of the current landscape of space interferometry, spanning foundational concepts, enabling technologies, mission architectures, and key astrophysical science applications. Experts across the community will explore how interferometric techniques can enable transformative advances in Physics of the Cosmos, Cosmic Origins, and Exoplanets science.

The event is intended both as an introduction for scientists and technologists interested in the field and as a forum for community discussion in support of the ASTRA process. The webinar will conclude with an open discussion aimed at identifying opportunities for collaboration.

A detailed agenda for the webinar, along with connection information, can be found on the event webpage.

Wishing you the best,

Dr Ron Gamble

Cosmic Origins Support Scientist, NASA GSFC

Dr Bernard Kelly

PhysCOS Support Scientist, NASA GSFC

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.