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Gaseous yellow-orange filaments look like a rose seen from the side and tilted slightly from upper left to lower right, slightly higher than the center of the frame. Extending from the rose to upper left and lower right are gaseous outflows that appear as red lobes that have an overall shape of tall, narrow triangles with rounded tips. Each red triangle is made up of wavy, irregular lines. Dozens of stars are scattered across the field. One particularly bright white star with eight diffraction spikes is located at the top of the yellow rose. Another bright blue star with even more prominent diffraction spikes is to its lower left. The background of space is black.

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Galaxies SIG Seminar 4 February 2026

Monsters in the Dark: Searching Far and Wide for Ultra-Luminous Galaxies at Cosmic Dawn Speaker John Weaver Abstract The first galaxies (z > 10) appear to have formed faster and more efficiently than predicted by standard models, but they are…

Jan 19, 2026
DGCE SIG Seminar, 22 Jan 2026

Mapping Hot Gas Kinematics in Galaxy Clusters with XRISM: What Have We Learned So Far? Speaker Irina Zhuravleva, University of Chicago Abstract The XRISM observatory (JAXA/NASA), launched in September 2023, is now providing the long-awaited high-resolution X-ray spectra of extended…

Jan 16, 2026
AI/ML STIG Lecture Series, 19 Jan 2026

Convolutional Neural Networks (CNNs) Speaker John Wu, STScI Meeting Connection Join the Meeting

Jan 16, 2026
DGCE Seminar, 22 Jan 2026

Mapping Hot Gas Kinematics in Galaxy Clusters with XRISM: What Have We Learned So Far? January 22, 2026 | 4:00pm ET / 1:00pm PT Speaker Irina Zhuravleva | University of Chicago Abstract The XRISM observatory (JAXA/NASA), launched in September 2023, is…

Jan 14, 2026
Science Highlight: NASA’s Webb Delivers

A team led by Dr. Enrique Lopez-Rodriguez from University of South Carolina, a former member of the Cosmic Origins Program Analysis Group (COPAG) Executive Committee, has used NASA’s Webb telescope to apply the Aperture-Mask Interferometry technique to get high contrast,…

Jan 14, 2026
ROSES-25 Amendment 37: New Opportunity: C.12

C.12 Foundational Artificial Intelligence for the Moon and Mars (FAIMM) is intended to enable individual researchers to participate as members of teams who are designing science and exploration applications for large, general artificial intelligence (AI) models known as Foundation Models (FMs)…

Jan 14, 2026
Heising-Simons Foundation Astronova Fellowship Deadline

The Heising-Simons Foundation is excited to announce the launch of a new multi-year fellowship to support postdoctoral scientists who are developing instrumentation to shape the future of astronomy, astrophysics, cosmology, and planetary science. The Astronomical Innovation (Astronova) Fellowship will provide funding for…

Jan 14, 2026
ROSES-25 Amendment 38: D.5 Astrophysics Pioneers Updates

D.5 Astrophysics Pioneers solicits proposals for Astrophysics space and sub-orbital science investigations that are greater in cost, scope, and capability than possible within the Astrophysics Research and Analysis suborbital and CubeSat program but are smaller in cost than what is possible…

Jan 14, 2026
ROSES-25 Amendment 36: New Program Element: F.19

F.19 Collaborative Opportunities for Mentorship, Partnership and Academic Success in Science (COMPASS)funds collaborations between NASA Centers and academic institutions that will advance NASA’s scientific priorities and train the future STEM workforce. COMPASS prioritizes collaborations with academic institutions that have not…

Jan 14, 2026
AI/ML STIG Lecture Series, 12 Jan 2026

Inductive Biases Speaker John Wu, STScI Lecture notes and slides will be up later on the github repo. We’ll be using slido for Q&A: https://app.sli.do/event/9jLSjC8GYLePQD3RPVXNv5 Meeting Connection Join the Meeting

Jan 12, 2026
Next AI/ML STIG Lecture on 12 Jan 2026

The next AI/ML Science and Technology Interest Group (AI/ML STIG) lecture will be on 12 January 2026 at 4 pm ET/1 pm PT. The lecture will be given by Dr. John Wu (STScI) on Inductive Biases in Neural Networks. The…

Jan 12, 2026
Announcing the Opening of the Roman Research Nexus

We are pleased to announce that the Roman Research Nexus is now available for use!  The Nancy Grace Roman Space Telescope will deliver an estimated 20 PB of data in its primary 5-year mission. In just one month, Roman will generate…

Jan 12, 2026
2026 Astrophysics Small Explorer AO Community Announcement

The NASA Science Mission Directorate (SMD) has released a third Community Announcement (CA) via www.SAM.gov that updates the special notice entitled DRAFT Announcement of Opportunity (AO) — 2025 Astrophysics Small Explorer (SMEX) Notice ID NNH25ZDA008J stating NASA’s intention to solicit investigations for the Astrophysics…

Jan 12, 2026
Science Highlight: NASA’s Hubble Examines Cloud-9

A team including Dr. Rachael Beaton from STScI, who is on the leadership council of the Cosmic Origins Stars Science Interest Group (Stars SIG), has used NASA’s Hubble Space Telescope to uncover a new type of astronomical object —

Jan 12, 2026
AI/ML STIG Lecture Series, 9 Feb 2026

Transformers Speaker Helen Qu, Flatiron Meeting Connection Join the Meeting

Jan 12, 2026
AI/ML STIG Lecture Series, 2 Feb 2026

Graph Neural Networks (GNNs) Speaker Tri Nguyen, Northwestern Meeting Connection Join the Meeting

Jan 12, 2026
AI/ML STIG Lecture Series, 26 Jan 2026

Recurrent Neural Networks (RNNs) Speaker Daniel Muthukrishna, Harvard/MIT Meeting Connection Join the Meeting

Jan 12, 2026
Discovery of a Starless Galaxy Reported at AAS

COPAG Executive Committee member Rachael Beaton shared the discovery of a starless galaxy during a press conference at the American Astronomical Society meeting in Phoenix.

Jan 7, 2026
Cosmic Origins at AAS 247, Jan 2026

The 247th AAS meeting (joint with the Historical Astronomy Division) will be held 4-8 January in Phoenix, Arizona at the Phoenix Convention Center. Join us in the exhibit hall at the NASA booth and attend the NASA sessions.

Jan 4, 2026
COPAG Activities at AAS 247, Jan 2026

Dear Cosmic Origins Community, We wish you all a very Happy New Year 2026!! We invite you to join us for the COPAG and Joint-PAG Sessions at the 247th American Astronomical Society Meeting on Sunday, January 4th at the Phoenix Convention Center,…

Jan 2, 2026
AI/ML STIG Lecture Series, 22 Dec 2025

JAX Speaker Philip Cargile (Harvard CfA) Meeting Connection Join the Meeting

Dec 22, 2025
AI/ML STIG Lecture Series, 15 Dec 2025

PyTorch and Autodifferentiation Speaker Philip Cargile (Harvard CfA) Meeting Connection Join the Meeting

Dec 15, 2025
ROSES-25 Amendment 30: Updates to ROSES-25 Summary of Solicitation

ROSES-2025 is an omnibus or umbrella solicitation that contains many program element appendices (listed in Tables 2 and 3) and the ROSES-25 Summary of Solicitation (SoS) lays out the backstop rules that apply by default to those program element appendices. ROSES-2025 Amendment 30 makes a…

Dec 15, 2025
Cosmic Pathfinders Early-Career Lunch with NASA Astrophysics at AAS 247

Express your interest in joining the astrophysics program offices and the Cosmic Pathfinders program for a networking lunch event with NASA Astrophysics leadership during the upcoming 247th American Astronomical Society meeting in January.

Dec 15, 2025

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.

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Labeled "artist’s concept" at bottom right, the graphic shows a closeup of a dwarf galaxy, which appears roughly circular with a light yellow bar in the center. Faint, blue, wispy, cloud-like features surround this yellow bar, and they are sprinkled with tiny white specks. A wide, wispy, purple arc appears to the left of the galaxy. Trailing the galaxy is a large, faint, wide, tail-like  feature.