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COPAG Activities at AAS 247

2 January 2026

Cosmic Origins about COPAG Activities at AAS 247

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, AZ. 

The COPAG session will take place on Sunday January 4, 2026, from 9:00am– 2:00 pm local time, at the Phoenix Convention Center (AAS Meeting venue), room 226B . The Joint-PAG will follow in room 301D and will conclude with a Q&A session with the NASA Astrophysics Division Director, Dr. Shawn Domagal-Goldman and the PAG Executive Committee Chairs.

You can see the full agenda on our website: https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-at-aas-247-jan-2026/

We look forward to seeing you in January in Phoenix. 

Best regards,

Peter Kurczyński (COR Chief Scientist)

Swara Ravindranath (COR Deputy Chief Scientist)

Ron Gamble (COR Scientist)

American Astronomical Society

The 247th Meeting of the AAS

The 247th Meeting of the American Astronomical Society (joint with the Historical Astronomy Division) will be held 4-8 January 2026 in Phoenix, Arizona.

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American Astronomical Society

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.