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Cosmic Origins Second Early Career Workshop

NASA’s Cosmic Origins Program is excited to invite you to the second Early Career Workshop, designed to support and empower the next generation of astrophysics leaders and PIs. The workshop aims to provide insights to early career scientists about the wide range of work done in the Cosmic Origins Program, to explain and demonstrate the tools and opportunities available to them, and to answer any questions they may have.

Cosmic Origins about Cosmic Origins Second Early Career Workshop

Location

Virtual

Dates

20-22 October 2026
1:00pm - 4:30pm ET

Community

Cosmic Origins

Type

Workshop

Cosmic Origins Community

To Support and Empower the Next Generation of Astrophycists

This workshop will take place virtually on October 20 – 22, 2026, from 1:00pm – 4:30 pm Eastern.

The Pillars of Creation. Wispy silhouettes of three columns against a dark, star-filled background.
A Near-Infrared View of the Pillars of Creation. This NASA Hubble Space Telescope image, taken in near-infrared light, transforms the pillars into eerie, wispy silhouettes, which are seen against a background of myriad stars. The near-infrared light can penetrate much of the gas and dust, revealing stars behind the nebula as well as hidden away inside the pillars. Some of the gas and dust clouds are so dense that even the near-infrared light cannot penetrate them. New stars embedded in the tops of the pillars, however, are apparent as bright sources that are unseen in the visible image. The ghostly bluish haze around the dense edges of the pillars is material getting heated up by the intense ultraviolet radiation from a cluster of young, massive stars and evaporating away into space. The stellar grouping is above the pillars and cannot be seen in the image. At the top edge of the left-hand pillar, a gaseous fragment has been heated up and is flying away from the structure, underscoring the violent nature of star-forming regions. Astronomers used filters that isolate the light from newly formed stars, which are invisible in the visible-light image. At these wavelengths, astronomers are seeing through the pillars and even through the back wall of the nebula cavity and can see the next generations of stars just as they're starting to emerge from their formative nursery.
NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

Workshop Schedule

TBA

Workshop Connection

Join the Workshop

Workshop Science Organizing Committee

Sabrina Stierwalt
Peter Kurczynski
Swara Ravindranath
Ronald Gamble

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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.