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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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AI/ML STIG Lecture Series, 9 Feb 2026

Build a decoder-only transformer (a small GPT-like language model) from scratch in PyTorch. Train it on the Tiny Shakespeare dataset for character-level language modeling and use it to generate text, understanding every component along the way.

Feb 9, 2026
Next AI/ML STIG Lecture 9 Feb 2026

Build a decoder-only transformer (GPT-style) from scratch in PyTorch. Train it on Tiny Shakespeare for character-level language modeling and generate text.

Feb 9, 2026
HWO SIG Seminar, 11 Feb 2026

This seminar will feature an update from the Habitable Worlds Observatory Community Science & Instrument Team (CSIT), presentations on technical capabilities, and time for groups to advertise their HWO-related work and find collaborators. If you would like an advertisement slot…

Feb 6, 2026
AGN SIG Vision Series Seminar, 17 Feb 2026

We invite everyone to join us for the next AGN SIG Vision Series Talk on Tuesday, February 17, 2026, at 1 pm ET/10 am PT. Our first Vision Series talk for the year will feature Dr. Santiago Garcia-Burillo (Observatorio Astronómico…

Feb 5, 2026
DGCE SIG Seminar, 26 Feb 2026

Illuminating the Galactic Baryon Cycle at Cosmic Noon. Speaker: Tucker Jones

Feb 4, 2026
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…

Feb 4, 2026
Galaxies SIG Seminar, Feb 4, 2026

Monsters in the Dark: Searching Far and Wide for Ultra-Luminous Galaxies at Cosmic Dawn, Speaker | John Weaver

Feb 4, 2026
IR STIG Seminar, 2 Feb 2026

Space Interferometry for Astrophysics in the 2030s? Speaker William C. Danchi, NASA Goddard Space Flight Center Abstract Space interferometry is the next evolutionary step for high angular resolution astronomy, given the maturity and many accomplishments of ground-based interferometry in the…

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

Graph Neural Networks (GNNs) Speaker Tri Nguyen, Northwestern Learn how to build Graph Neural Networks (GNNs) to work with graph-structured data. Explore node classification on citation networks and apply GNNs to model dark matter subhalo interactions with stellar streams using…

Feb 2, 2026
HWO SIG Seminar, 11 Feb 2026

The HWO Science Interest Group invites you to the next seminar: Wednesday, February 11th, at 1:00 pm ET / 10:00 am PT .

Feb 2, 2026
Next AI/ML STIG Lecture, 2 Feb 2026

February 2nd, 2026 at 4:00 pm ET/1:00 pm PT Graph Neural Networks Neural Network Basics: Part 3 | Tri Nguyen, Northwestern University Learn how to build Graph Neural Networks (GNNs) to work with graph-structured data. Explore node classification on citation…

Feb 2, 2026
Fornax Initiative Welcomes Beta Users

NASA’s Fornax Initiative is now accepting beta users on our Science Console, a JupyterLab environment in the cloud for computing next to NASA astrophysics archival data.

Feb 2, 2026
IR STIG Seminar, 2 Feb 2026

Space Interferometry for Astrophysics in the 2030s? Speaker: William C. Danchi, NASA Goddard Space Flight Center

Feb 2, 2026
AGN Spotlight Series Talk, 27 Jan 2026

We invite everyone to join us for the inaugural AGN SIG Spotlight Talk on Tuesday, January 27, 2026, at 1 pm ET/10 am PT.

Jan 27, 2026
AI/ML STIG Lecture Series, 26 Jan 2026

Convolutional Neural Networks (CNNs) Speaker John Wu, STScI Build a convolutional neural network (CNN) to estimate physical properties of galaxies directly from images. Train a model to predict gas-phase metallicity from SDSS galaxy images, replicating the approach from Wu &…

Jan 26, 2026
IR STIG PRIMA Seminar, 26 Jan 2026

Debris Disks in the Far-Infrared with PRIMA Speaker Meredith MacGregor (Johns Hopkins University) Abstract More than 20% of nearby main sequence stars are surrounded by debris disks, where planetesimals, larger bodies similar to asteroids and comets in our own Solar System,…

Jan 26, 2026
ROSES-2026 to be Released July 2026

In 2025, NASA’s Science Mission Directorate (SMD) released the annual Research Opportunities in Space and Earth Sciences (ROSES) solicitation in July rather than February, the traditional target release date. For simplicity, consistency, and to maintain the annual schedule, SMD plans…

Jan 23, 2026
NASA Postdoctoral Program Deadline March 1st, 2026

The NASA Postdoctoral Program (NPP) offers US and international scientists the opportunity to advance their research while contributing to NASA’s scientific goals. The NPP supports fundamental science; explores the undiscovered; promotes intellectual growth; and encourages scientific connections. Selected by a competitive peer-review…

Jan 23, 2026
ROSES-25 Amendment 40: Exoplanets Research Program Step-2

The Exoplanets Research Program (XRP), element F.3 of ROSES-25, solicits basic research proposals to conduct scientific investigations that significantly improve our understanding of exoplanets and exoplanet formation. This program element is cross-divisional and jointly managed by three of the Divisions…

Jan 23, 2026
AGN SIG Inaugural Spotlight Series, 27 Jan 2026

On behalf of the NASA Active Galactic Nuclei Science Interest Group (AGN SIG) Leadership Council, we are excited to announce the launch of the monthly AGN SIG Talk Series beginning in January 2026! This is a new community-focused seminar designed…

Jan 23, 2026
AAS 247 Session Recordings and Talks Uploaded

The 247th Meeting of the American Astronomical Society (joint with the Historical Astronomy Division) was held January 4th-8th 2026 in Phoenix, Arizona and we had A LOT of discussions on everything from next-generation AGN science to early-career leadership to what…

Jan 23, 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 22, 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

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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.