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Habitable Worlds Observatory SIG Seminar, 28 Oct 2026

Image: NASA Science

A NASA Habitable Worlds Observatory seminar brings together researchers to review project office milestones, lunar-based astrophysics concepts, and the primary science cases for habitable exoplanets.

Habitable Worlds Observatory Community Gathering

Operating under NASA's Cosmic Origins and Physics of the Cosmos communities, the Habitable Worlds Observatory Science Interest Group (HWO SIG) is hosting a specialized seminar on October 28, 2026. The session opens with announcements and welcoming remarks by Vivian U, followed by status updates from Giada Arney and Aki Roberge representing the HWO Project Office. The meeting serves as an essential forum for aligning the community's scientific objectives with the ongoing systems engineering and mission architecture development for NASA's next-generation flagship observatory.

Astrophysics from the Moon and Mission Highlights

The seminar agenda examines both direct exoplanet observations and complementary observational domains. Marin Anderson presents prospects for astrophysics conducted from the Moon, evaluating how lunar platforms can support cosmic exploration. Furthermore, Rachael Beaton and Sten Hasselquist detail highlights from the HWO Priority Science Initiatives (PSI), focusing on spectroscopic baselines, starlight suppression benchmarks, and the instrument stability necessary to isolate faint planetary photons from blinding stellar glare.

Driving Science Cases and the Hunt for Habitable Worlds

Kevin France outlines the CSIT driving science cases, which define the observatory's core requirements across ultraviolet, optical, and near-infrared wavelengths. By directly imaging temperate terrestrial planets orbiting nearby Sun-like stars, HWO aims to identify key atmospheric constituents, including molecular oxygen, water vapor, and methane. The subsequent open discussion allows astronomers and instrumentation specialists to refine mission criteria, ensuring that HWO will possess the transformative diagnostic power required to detect potential signs of life beyond our solar system.

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