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Cosmic Origins at AAS 248, June 2026 - NASA Science Cosmic Structure SIG Seminar, 30 April 2026 - NASA Science CMB SAG Meeting, 24 April 2026 - NASA Science BBX SAG Meeting, 30 April 2026 - NASA Science Early Career Investigator Program – Earth Science (ROSES A.11) - NASA Science XR SIG Seminar, 1 May 2026 - NASA Science Night and (Earth) Day - NASA SWERV: High-Impact Historical Case Study - NASA Science AAS Meeting 248, June 2026 - NASA Science Earth Day 2026: Posters and Virtual Backgrounds - NASA Science Advancing Earth Observation at NASA since Release of Earthrise Photo - NASA Science X-59 Adds Freedom 250 Logo - NASA Belts of Green in the Washington Suburbs - NASA Science Artemis II Mission Milestones: An Image and Video Recap Curiosity Blog, Sols 4867-4872: Sand Fill In Antofagasta Crater and Finding Our Next Drill Target NASA Invites Media to Jordan Artemis Accords Signing Ceremony New NASA Views of Earth, From (S)PACE - NASA Science Crew Studies Biotech on Tuesday to Advance Health and Space Economy NASA Invests in Small Businesses Innovating for Space and Earth NASA at SXSW: Johnson Director Vanessa Wyche on Why Artemis Changes Everything Researchers: How Would You Extract Meaningful Insights from Just Four Astronauts? BBX SAG Meeting, 23 April 2026 - NASA Science Thailand’s Krabi Coast - NASA Science AI/ML STIG Lecture Series, 20 April 2026 - NASA Science SWERV: Training Overview and Agenda - NASA Science SWERV: REAL-TIME CAPABILITIES AND IONOSPHERIC DISRUPTIONS OF COMMUNICATIONS - NASA Science SWERV: Operationally Significant Phenomena and Impacts for Ground Operations - NASA Science SWERV: Space Weather Impacts on Satellites - NASA Science SWERV: Space Weather Chain of Events - NASA Science CSDA Quality Assessment Report Evaluates Satellogic NewSat Data - NASA Science
Far-IR Space Mission Concepts Workshop, May 2014 - NASA S...
Patricia Tyl · 2026-05-12 · via NASA Science

Cosmic Origins Science

A Community Workshop to Plan the Future of Far Infrared Space Astrophysics

Bringing Fundamental Astrophysical Processes Into Focus

Learn More about A Community Workshop to Plan the Future of Far Infrared Space Astrophysics
A rectangular image of the Serpens Nebula with black vertical rectangles at the bottom left and top right to indicate missing data. A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right at the same angle. At center-left is a larger star that is circled. This star has Webb’s signature diffraction spikes, but along the right also has an arc of white, with the circular edge starting at the center of the star. Mostly blue gas fills the center. There is a particularly bright central star. The gas to the right is a darker orange. Small points of light are sprinkled across the field. The brightest sources have extensive eight-pointed diffraction spikes.

NASA’s James Webb Space Telescope’s 2024 NIRCam image shows protostar EC 53 circled. Researchers using new data from Webb’s MIRI proved that crystalline silicates form in the hottest part of the disk of gas and dust surrounding the star — and may be shot to the system’s edges.

Image: NASA, ESA, CSA, STScI, Klaus Pontoppidan (NASA-JPL), Joel Green (STScI); Image Processing: Alyssa Pagan (STScI)