The Community Science (Ad ASTRA) Workshop is organized by Caltech/IPAC, the NASA Astrophysics Division, and the three Astrophysics Program Offices (Physics of the Cosmos, Cosmic Origins, and Exoplanet Exploration), in conjunction with the ASTRA initiative, to engage the community in defining future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities, and Missions—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community input. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio.
I'm going to make a summary of Concepts and Missions, because the scientific community doesn't only look for extraterrestrials, invisible matter, and Moon rocks. I say this only somewhat as a joke...
The documents present an ambitious and multifaceted vision for astrophysics in the coming decades, ranging from the study of the origins of the universe to the search for life beyond our solar system. The missions and concepts can be grouped into several key thematic areas:
1. Cosmology and the Early Universe:
Cosmic Microwave Background (CMB) Missions: A recurring theme is the proposal of a state-of-the-art space observatory. Its main objective would be to measure primordial gravitational waves by searching for the B-mode in order to test cosmic inflation beyond the discussion of how they are measured and what is measured, in addition to providing definitive measurements of the mass of neutrinos—which neutrinos we are looking for and where they originate—and the optical depth to reionization.
Exploration of the Dark Ages: Several concepts, such as radio telescopes on the far side of the Moon, focus on observing the 21 cm signal from neutral hydrogen at high redshifts z > 30. This is the only way to probe the "Dark Ages" of the universe, before the formation of the first stars, and offers a testing ground for physics beyond the standard model—dark matter, inflation, etc.
Spectroscopic Surveys of Galaxies: Missions such as a 2-meter space telescope with multi-object spectroscopy in the near- and mid-infrared. Its goal is to map the large-scale structure of the universe with unprecedented precision, studying dark energy, inflation, and neutrino mass through baryon acoustic oscillations. It is presented as a bridge between current surveys (DESI) and future ones (Euclid, Roman).
2. High-Energy Phenomena and the Extreme Universe:
Next-Generation X-ray Missions: There is a strong commitment to X-ray observatories with enhanced capabilities. These include:
Successors to Chandra: Concepts offering a 10x improvement in sensitivity and 50x in survey speed, with angular resolution of ~1 arcsecond, to study black hole formation, AGN feedback, and the impact on exoplanets.
Broadband Observatories: Missions to cover the 0.1 to 100 keV range, in order to study the spin of supermassive black holes, accretion growth, and resolve the cosmic X-ray background at its energy peak of ~30 keV, where most obscured AGN emit.
X-ray Interferometry: Concepts seeking a quantum leap in angular resolution—microarcseconds—which would allow resolving black hole coronae, studying AGN binaries in their final stages, and observing the impact of stellar flares on exoplanet habitability.
Closing the "MeV Gap": Missions are proposed to explore the MeV energy range, a poorly observed window. Concepts that seek to detect nuclear emission lines from supernovae, study positron physics, and capture counterparts of multi-messenger events.
Cosmology and Particle Physics: Missions for ultra-high-energy cosmic rays and very-high-energy neutrinos, others for MeV gamma rays and the search for dark matter antinuclei, and missions to measure low-energy cosmic antinuclei seek answers to fundamental questions about dark matter, particle acceleration, and nucleosynthetic processes.
3. Planets and the Origin of Life:
Characterization of Exoplanets: Multiple approaches compete to characterize exoplanet atmospheres, especially temperate and rocky ones.
Direct Imaging Missions: A ~40m inflatable telescope and a constellation of 4m telescopes are innovative concepts for obtaining biosignature spectra from planets around M dwarfs. proposes a hybrid between a space-based starshade and extremely large ground-based telescopes to achieve unprecedented contrast and high observation speed.
Transit and Eclipse Missions focus on transit spectroscopy. A dedicated survey to find Earth-sized planets in the habitable zone of M dwarfs.
Non-Transit-Based Technique: Proposes using the "Planetary Infrared Excess" (PIE) technique to characterize the thermal emission of rocky planets that do not transit, which would greatly expand the number of studyable targets.
Infrared and Nulling Interferometry: Concepts such as mid-infrared nulling, based on the European concept, would seek to characterize planets detected by radial velocity.
Magnetospheres and Habitability: The detection of magnetic fields on exoplanets is considered crucial for assessing their habitability. Low-frequency radio missions on the far side of the Moon could detect auroral radio emissions from Earth-like exoplanets and M dwarfs, providing the first direct measurement of their magnetospheres.
4. New Technologies and Architectures:
Enabling Technologies: Advances are highlighted in detectors, X-ray optics (state-of-the-art silicon mirrors), CADR cooling, integrated photonic optics for interferometry, and quantum technologies (atomic clocks, atom interferometers).
Mission Architectures:
Missions on the Moon: The Moon emerges as a strategic destination for astrophysics, offering a radio-quiet, cold, and stable environment for low-frequency radio telescopes, infrared telescopes, and even gravitational wave detectors.
Constellations and Distributed Architectures: Concepts that propose fleets of smaller, coordinated spacecraft instead of a single large observatory. This offers advantages such as redundancy, the ability to conduct multiple simultaneous observations, scalability, and lower cost per mission.
Deep Space Missions: Solar Gravitational Lens Observatory and Interplanetary Laser are concepts for missions in the outer solar system, which would leverage the Sun's gravity or large distances to perform unparalleled fundamental physics and astrophysics measurements.
Fluidic Optics: Which would drastically reduce the mass and cost of future space telescopes.
To wrap things up, I've wanted to participate in an event for a long time to share my ideas and to read what the scientific community is discussing. It was a complete success for the organizers and NASA.
Link:
https://conference.ipac.caltech.edu/community2026
https://science.nasa.gov/astrophysics/programs/physics-of-the-cosmos/community/ad-astra/
![]() |


















































