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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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Cosmic Origins Special Announcement

A very well-deserved Congratulations to our very own Shouleh Nikzad for being elected to the National Academy of Engineering!

Feb 27, 2026
Astrophysics Division Meeting, 10 Mar 2026

Astrophysics Division Update and Astro 2030 Preparations. Speaker: Shawn Domagal-Goldman

Feb 25, 2026
Galaxies SIG Seminar 4 March 2026

Tracing Turbulence in Jellyfish Galaxy Tails Speaker Yuan Li (UMass) Abstract Jellyfish galaxies, found in the outskirts of galaxy clusters, exhibit extended tails of gas stripped away by ram pressure from the intracluster medium (ICM), giving rise to their distinctive…

Feb 25, 2026
IR STIG Seminar, 2 Mar 2026

Near-Infrared Survey Science with the Roman Space Telescope Speaker Maxime Rizzo Abstract The Nancy Grace Roman Space Telescope is set to launch in Fall 2026, ushering in a new era of near-infrared space-based astrophysics. By combining Hubble-like spatial resolution with…

Feb 25, 2026
AI/ML STIG Lecture Series, 2 March 2026

Equivariant Networks – Applications Speaker Anna Scaife, U. of Manchester Meeting Connection Join the Meeting

Feb 24, 2026
DGCE SIG Seminar, 26 Feb 2026

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

Feb 23, 2026
AI/ML STIG Lecture Series, 23 Feb 2026

Build Recurrent Neural Networks from first principles and apply them to real-time classification of astronomical transients. Implement vanilla RNNs, LSTMs, and GRUs in PyTorch and train a classifier on supernova light curves. Topics Covered Meeting Connection Join the Meeting

Feb 23, 2026
New Community Space for Cosmic Pathfinders Program

Follow the link here to join: https://discord.gg/DsDq5UX8TJ Over the past two years the NASA Cosmic Pathfinders Program has been slowly, but surely, developing as a platform for early-career professional growth. A growing number of participants and community members/supporters, both domestic…

Feb 23, 2026
DGCE SIG Seminar, 26 Feb 2026

Illuminating the Galactic Baryon Cycle at Cosmic Noon Speaker Tucker Jones | University of California – Davis Abstract The formation of galaxies is regulated by large-scale inflows and outflows of gas, in a process known as the baryon cycle. This…

Feb 23, 2026
AI/ML STIG Lecture, 23 Feb 2026

The next AI/ML Science and Technology Interest Group (AI/ML STIG) lecture will be on February 23rd, 2026 at 4:00 pm ET/1:00 pm PT. Recurrent Neural Networks (RNNs) Speaker Daniel Muthukrishna | Harvard/MIT Connection information and the link to join the…

Feb 23, 2026
NASA Astrophysics Division Update 10 Mar 2026

The NASA Astrophysics Division Director, Shawn Domagal‑Goldman, will provide an update in a webinar on 10 March 2026, 12p-1p Eastern (9a-10a Pacific).

Feb 19, 2026
Last Call for Summer Internships!

The deadline for NASA internships during summer 2026 is fast approaching and will be here on February 27th! We have compiled an extensive listing of the latest information on astrophysics-related summer internships offered below! All links provided below will take…

Feb 18, 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 12, 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 11, 2026
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
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

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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.