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TODAY COR at AAS 248 | Everything but Exoplanets

Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory

Monday, June 15th, 10:00am -11:30am PT

This is your reminder to join the Cosmic Origins community members as they present their science and talk about relevant topics of interest across the astrophysics landscape!

For Cosmic Origins at AAS, please visit the link below. 

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-at-aas-248-june-2026

Special Session: Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory

Highlights from Cosmic Origins Science Interest Groups (SIGs) and Science Analysis Groups (SAGs).

TimeTopicSpeaker
10:20am – 10:30amSpatially Resolved UV Spectroscopy Science Analysis Group in Support of HWOEmily Witt (JHU)
10:30am – 10:40amInvestigating the NIR Discovery Space of the Habitable Worlds Observatory: Updates from the Red Limit Science Analysis GroupKyle Cooke (University of Louisville)
10:40am – 10:50amOpening the OVI Window to Reveal the Diffuse Cosmic Ecosystem with HWOSanchayeeta Borthakur (Arizona State University)
11:00am -11:10amHWO Science Interest Group: Keeping the Community Connected to HWOJessie Christiansen (Caltech/IPAC)

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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.

The post TODAY COR at AAS 248 | Everything but Exoplanets appeared first on NASA Science.

  •  

Join Us at the 248th AAS Meeting, June 2026

Join Us at the 248th AAS Meeting in Pasadena, 14 – 18 June, 2026

Special Session: Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory

Monday, June 15th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT

Highlights from Cosmic Origins Science Interest Groups (SIGs) and Science Analysis Groups (SAGs).

TimeTopicSpeaker
10:20am ‑ 10:30amSpatially Resolved UV Spectroscopy Science Analysis Group in Support of HWOEmily Witt (JHU)
10:30am ‑ 10:40amInvestigating the NIR Discovery Space of the Habitable Worlds Observatory: Updates from the Red Limit Science Analysis GroupKyle Cooke
(University of Louisville)
10:40am ‑ 10:50amOpening the OVI Window to Reveal the Diffuse Cosmic Ecosystem with HWOSanchayeeta Borthakur (Arizona State University)
11:00am ‑ 11:10amHWO Science Interest Group: Keeping the Community Connected to HWOJessie Christiansen (Caltech/IPAC)

Splinter Session: NASA’s Big Science, Small Missions

Tuesday, June 16th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT (Hybrid Session)

For remote participation, please look for the “Join the Session” link above the agenda on the Cosmic Origins at AAS website.

High-impact science.
Smarter, faster, together.

Agenda

Organizers: Swara Ravindranath (NASA/GSFC), Emily Witt (JHU)

TimeTopicSpeaker
10:00am ‑ 10:05amWelcomeSwara Ravindranath (NASA/GSFC)
10:05am ‑ 10:15amFORTIS Sounding RocketEmily Witt (JHU)
10:15am ‑ 10:25amBlackCAT CubeSatAbe Falcone (Pennsylvania State University)
10:25am ‑ 10:35amSunRISE CubeSat ConstellationJoseph Lazio (University of Michigan)
10:35am ‑ 10:45amSPHEREx Medium Explorer MissionRoberta Paladini (IPAC/Caltech)
10:45am ‑ 10:55am Landolt Pioneer MissionPeter Kurczynski (NASA/GSFC)
10:55am ‑ 11:05amNon-Traditional Path to MissionsSanchayeeta Borthakur (Arizona State University)
11:05am ‑ 11:10amBREAK
11:10am ‑ 11:30amPanel DiscussionSwara Ravindranath (NASA/GSFC, moderator)
Panelists: Drew Miles (Caltech), Pablo Saz Parkinson (NASA HQ), Joseph Lazio (University of Michigan), Abe Falcone (Pennsylvania State University), David Ardila (JPL)

Special Session: Planning for the Future of Astrophysics and the ASTRA Initiative

Thursday, June 18th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT

No remote participation is available for this special session.

Agenda

TimeTopicSpeaker
10:00am ‑ 10:10amIntroduction from the NASA Astrophysics Division DirectorShawn Domagal‑Goldman
(NASA HQ)
10:10am ‑ 10:25amThe ASTRA Initiative: Overview& Path ForwardJessica Gaskin (NASA HQ)
10:25am ‑ 10:40amInnovation for Astrophysics Workshop: Initial FindingsKendra Short (JPL)
10:40am ‑ 10:55amAd ASTRA Community Science WorkshopPeter Kurczynski (NASA/GSFC)
10:55am ‑ 11:30amPanel DiscussionFrancesca Civano (NASA/GSFC)

ASTRA Office Hours at Cosmic Origins Exhibit Booth

(June 15 – 17, 2026) at 9am PT

Stop by the AAS / Cosmic Origins Exhibit booth during these times to ask questions about the ASTRA initiative, the September Ad ASTRA workshop, and developing new strategic mission concepts for astrophysics. Monday, Tuesday, Wednesday 9 am PT (Peter Kurczynski)

Best regards,
Swara Ravindranath

American Astronomical Society

The 248th Meeting of the AAS

The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.

Learn More
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American Astronomical Society (AAS)

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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.

The post Join Us at the 248th AAS Meeting, June 2026 appeared first on NASA Science.

  •  

HWO Detector System Development Study Request for Proposals

Habitable Worlds Observatory Detector System Development Study Request for Proposals

12 June 2026

Due by July 7th, 2026

Dear Colleagues,

The Habitable Worlds Observatory Technology Maturation Project Office and Columbus Technologies are excited to invite you to participate in a Detector System Development Study focused on developing critical detector technologies for the Habitable Worlds Observatory. This request for proposals seeks information from qualified organizations capable of supporting detector technology maturation studies to advance candidate technologies toward Technology Readiness Level 5. Specifically, we are seeking responses to address one or more of the following detectors categories: photon-counting detectors for visible and near-infrared coronagraph applications, far-ultraviolet detectors, and large-format detectors for near-ultraviolet and visible applications. Details regarding the call for proposals, eligibility, required deliverables, and study phases are available at the Columbus Technologies website here: https://columbususa.com/opportunities/hwo-detector-rfp/ 

Respondents located at Government agencies including the Jet Propulsion Laboratory or NASA Centers (e.g., Goddard Space Flight Center, Ames Research Center, etc.) should submit their responses directly to Daniel Kelly (daniel.p.kelly@nasa.gov).

Note: Responses are due by July 7, 2026.

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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.

The post HWO Detector System Development Study Request for Proposals appeared first on NASA Science.

  •  

Ad ASTRA Community Science Workshop Updates 

Ad ASTRA Community Science Workshop: Agenda Structure and Abstract Submissions

Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members-

As we prepare for our Ad ASTRA Community Science workshop, we are writing to share important updates regarding the agenda structure and instructions for abstract submissions. 

The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in identifying future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities and Implementation, and Community Discussion—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community interactions and discussion. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio that is consistent with the Astro2020 recommendations and existing and future science gaps.

To best serve the community and facilitate meaningful collaboration, we are splitting the mission concept presentations into two distinct focuses: Science on Day 1, and Capabilities and Implementation on Day 2. We are relying on you—the concept teams and the broader community—to submit abstracts for both days. We are also offering the option to present mission concepts as posters, and will offer the opportunity to present as posters any abstracts for which there is insufficient room in the parallel sessions.

Please review the detailed agenda structure and submission guidelines below:

Day 1: Science Focus

  • Science Questions: Day 1 will focus on open science priorities and questions from strategic documents (Astro 2020 Decadal Survey, Enduring Quests – Daring Visions from 2014) and more recent science questions that the mission concepts submitted to ASTRA will address. 
  • Abstract Submission: Presentations for Day 1 are not restricted to mission concept team members. We strongly encourage other scientists in the community to submit abstracts presenting important science questions and to use this opportunity to connect with concept teams.
  • Breakout Sessions: These sessions will be organized by science themes (Compact Objects and Energetic Phenomena, Cosmology, Galaxies, Exoplanets & Astrobiology, Stars and Stellar Populations). Moderators will present a summary of the panel discussions at the end of Day 1.

Day 2: Mission Concepts – Capabilities and Implementation

  • Focus: Day 2 is focused on implementation, capabilities, and technologies (software and hardware) relevant to the ASTRA submitted mission concepts. A summary of the Innovation for Astrophysics Missions Workshop (May 2026) will inform discussions regarding industry and other capabilities and opportunities that may be leveraged. 
  • Breakout Sessions: These sessions will be organized by capability groups, which will be determined once the submitted mission concept documents are reviewed.
  • Format & Goals: Breakout sessions will feature a mix of presentations and flexible discussion. The goal is for teams with concepts at varying maturity levels to collaborate, find commonalities, and strengthen their respective capability groups.
  • Abstract Submission Note: Teams may submit multiple abstracts for these sessions if their concept spans different capabilities (e.g., requiring both UV and X-ray technologies).

Day 3 & Workshop Outcome

A primary goal of this workshop is to refine a draft “science-to-capabilities” matrix, which will be built using inputs from your submitted ASTRA mission concept documents. During the Day 1 and 2 breakout sessions, moderators will capture key discussion points to present during end-of-day summary panels. On Day 3 of the workshop, we will hold a plenary discussion to recap the week and collaboratively revise the “science-to-capabilities” matrix. Together as a community, we will add, refine, and prioritize science questions, mapping them to mission concepts. 

Key Upcoming Dates:

  • 24 June 2026: Abstract submission deadline (link). If you have already submitted an abstract and would like to modify it based on the guidelines above, please delete your previous contribution and send another submission. 
  • 26 June 2026: Mission Concept Document submission deadline (template, submission portal)
  • 10 July 2026: Contributed abstracts selected for talks and posters 

We look forward to your abstract submissions and to a highly collaborative and productive workshop! 

Best regards,

The Ad ASTRA Workshop Organizing Committee

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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.

The post Ad ASTRA Community Science Workshop Updates  appeared first on NASA Science.

  •  

Announcement of Opportunity SMEX 2026

Announcement of Opportunity Astrophysics Explorers Program 2026 Small Explorer (SMEX) Final Text Released

12 June 2026

The National Aeronautics and Space Administration (NASA) Science Mission Directorate (SMD) announces the release of an Announcement of Opportunity (AO) to solicit Principal Investigator (PI)-led space science investigations for the Small Explorer (SMEX) opportunity under the Astrophysics Explorers Program. The SMD strategic goal of expanding human knowledge through new scientific discoveries in astrophysics includes the broad objective: “to understand the Sun, Earth, Solar System, and Universe.” SMD addresses this objective through astrophysics investigations that address one or more of these science goals: 

  • How does the Universe work? Probe the origin and destiny of our universe, including the nature of black holes, dark energy, dark matter and gravity.
  • How did we get here? Explore the origin and evolution of the galaxies, stars, and planets that make up our universe.
  • Are we alone? Discover and study planets around other stars and explore whether they could harbor life. 

The 2026 Astrophysics SMEX (APSMEX26) Schedule:

AO Release Date: June 9, 2026 
Preproposal Conference Date: June 30, 2026
Mandatory Notice of Intent Due Date: July 21, 2026
Proposal Due Date: September 9, 2026

The NASA Solicitation and Proposal Integrated Review and Evaluation System (NSPIRES) is the official source for the full text of the Astrophysics Explorers Program 2026 SMEX AO. To find the full, final text visit https://go.nasa.gov/APSMEX26. Alternatively, visit: http://nspires.nasaprs.com/, select ‘Solicitations’ at the top of the page, and on the next page enter solicitation number NNH26ZDA011O in the search field.

Prospective investigators from any category of organizations or institutions, U.S. or non-U.S. with some restrictions as specified in Section 4.2.1 of the AO, are welcome. Specific categories of organizations and institutions include, but are not limited to, educational, industrial, and not-for-profit organizations, Federally Funded Research and Development Centers (FFRDCs), University Affiliated Research Centers (UARCs), NASA Centers, and other Government agencies. Both U.S. and non-U.S. participation is subject to China restrictions described in Sections 4.2.2 and 5.8.1 of the AO.

All interested parties must read the final APSMEX26 AO carefully for significant changes from the draft AO (NNH25ZDA008J) and prior years’ SMD Explorers Program AOs. Of particular importance is the change in evaluation and selection to a single-step competitive process. NASA intends to select one investigation proposal from the APSMEX26 responses to proceed into a combined Phase A&B. All proposals must comply with the requirements, constraints, and guidelines contained within the AO. 

The Science Office for Mission Assessments (SOMA) will post the virtual Preproposal Conference agenda, connection information, and related information at: https://explorers.larc.nasa.gov/APSMEX26/SMEX.  SOMA hosts the official “2026 Astrophysics Small Explorer (SMEX)” website that provides further information, including the SMEX Program Library and SMEX Question & Answer (Q&A) page. Anonymity of persons/institutions who submit questions will be preserved. Proposers are encouraged to send comments and questions early so that they may be fully addressed. Questions posed at least one week before the Pre-Proposal Conference may be addressed in the Pre-Proposal Conference presentation or on the SMEXQ&A page. The deadline for other questions is two (2) weeks before the proposal due date.

All questions or comments about the Astrophysics SMEX 2026 AO shall be addressed via email to Daniel Moses, APSMEX26 Lead Program Scientist, dan.moses@nasa.gov; Hannah JangCondell, APSMEX26 Deputy Program Scientist, hannah.jang-condell@nasa.gov; and Omar Torres, Lead Acquisition Manager for the 2026 Astrophysics SMEX AO, SOMA omar.torres@nasa.gov using subject line “APSMEX26” to be properly routed.

Any costs incurred in preparing a submission in response to this notice or the full APSMEX26 AO are solely the responsibility of the submitter. 

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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.

The post Announcement of Opportunity SMEX 2026 appeared first on NASA Science.

  •  

Ad ASTRA Community Science Workshop Announcements

Ad ASTRA Community Science Workshop: Agenda Structure and Abstract Submissions

Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members-

As we prepare for our Ad ASTRA Community Science workshop, we are writing to share important updates regarding the agenda structure and instructions for abstract submissions. 

The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in identifying future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities and Implementation, and Community Discussion—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community interactions and discussion. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio that is consistent with the Astro2020 recommendations and existing and future science gaps.

To best serve the community and facilitate meaningful collaboration, we are splitting the mission concept presentations into two distinct focuses: Science on Day 1, and Capabilities and Implementation on Day 2. We are relying on you—the concept teams and the broader community—to submit abstracts for both days. We are also offering the option to present mission concepts as posters, and will offer the opportunity to present as posters any abstracts for which there is insufficient room in the parallel sessions.

Please review the detailed agenda structure and submission guidelines below:

Day 1: Science Focus

  • Science Questions: Day 1 will focus on open science priorities and questions from strategic documents (Astro 2020 Decadal Survey, Enduring Quests – Daring Visions from 2014) and more recent science questions that the mission concepts submitted to ASTRA will address. 
  • Abstract Submission: Presentations for Day 1 are not restricted to mission concept team members. We strongly encourage other scientists in the community to submit abstracts presenting important science questions and to use this opportunity to connect with concept teams.
  • Breakout Sessions: These sessions will be organized by science themes (Compact Objects and Energetic Phenomena, Cosmology, Galaxies, Exoplanets & Astrobiology, Stars and Stellar Populations). Moderators will present a summary of the panel discussions at the end of Day 1.

Day 2: Mission Concepts – Capabilities and Implementation

  • Focus: Day 2 is focused on implementation, capabilities, and technologies (software and hardware) relevant to the ASTRA submitted mission concepts. A summary of the Innovation for Astrophysics Missions Workshop (May 2026) will inform discussions regarding industry and other capabilities and opportunities that may be leveraged. 
  • Breakout Sessions: These sessions will be organized by capability groups, which will be determined once the submitted mission concept documents are reviewed.
  • Format & Goals: Breakout sessions will feature a mix of presentations and flexible discussion. The goal is for teams with concepts at varying maturity levels to collaborate, find commonalities, and strengthen their respective capability groups.
  • Abstract Submission Note: Teams may submit multiple abstracts for these sessions if their concept spans different capabilities (e.g., requiring both UV and X-ray technologies).

Day 3 & Workshop Outcome

A primary goal of this workshop is to refine a draft “science-to-capabilities” matrix, which will be built using inputs from your submitted ASTRA mission concept documents. During the Day 1 and 2 breakout sessions, moderators will capture key discussion points to present during end-of-day summary panels. On Day 3 of the workshop, we will hold a plenary discussion to recap the week and collaboratively revise the “science-to-capabilities” matrix. Together as a community, we will add, refine, and prioritize science questions, mapping them to mission concepts. 

Key Upcoming Dates:

  • 24 June 2026: Abstract submission deadline (link). If you have already submitted an abstract and would like to modify it based on the guidelines above, please delete your previous contribution and send another submission. 
  • 26 June 2026: Mission Concept Document submission deadline (template, submission portal)
  • 10 July 2026: Contributed abstracts selected for talks and posters 

We look forward to your abstract submissions and to a highly collaborative and productive workshop! 

Best regards,

The Ad ASTRA Workshop Organizing Committee

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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.

The post Ad ASTRA Community Science Workshop Announcements appeared first on NASA Science.

  •  

TODAY: Cosmic Origins Community Webinar, 10 June 2026

TODAY: Cosmic Origins Community Webinar, June 10, 2026

10 June 2026

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-seminar-10-june-2026

Dear Cosmic Origins Community,

The ASTRA initiative (linked below) will promote new strategic mission concepts for astrophysics. We would like to encourage you to think about new strategic mission concepts for the coming decades of astrophysics. Please join us for a community webinar next Wednesday, June 10, 12:00 – 1:00 pm ET ( 9:00 – 10:00 am PT) where we will discuss ASTRA.

As part of ASTRA, the Community Science (Ad ASTRA) Workshop will take place 1-3 September 2026 in Pasadena. New concept ideas will be discussed at this event.

To join the ASTRA initiative, mission concept template is now available (linked below). There are also instructions for submission. Submitted concept ideas will be discussed at the September workshop.

Associated links:

We look forward to talking with you next week.

Shouleh Nikzad, Chair
Sabrina Stierwalt, Vice-Chair

COPAG Executive Committee

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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.

The post TODAY: Cosmic Origins Community Webinar, 10 June 2026 appeared first on NASA Science.

  •  

IR STIG Meeting, 12 June 2026

IR STIG Meeting

Infrared Science and Technology Interest Group

IR STIG about IR STIG Meeting

Location

Virtual

Dates

12 June 2026
1:00pm ET / 10:00am PT

Community

IR STIG

Type

Meeting

ASTRA Initiative Community Brainstorming Session

The IRSTIG will host a community brainstorming session from 1-3pm ET / 10am – 12pm PT. We understand this is short notice, however given the rapidly approaching ASTRA workshop abstract deadline (June 24th) and ASTRA mission concept template submission deadline (June 26th), we feel that this coming Friday is our best opportunity to rally the IR community.  As such, we will be holding an open-invite brainstorming session to help energize and organize the community. This will be a rather freeform meeting to allow for flexibility, but a rough schedule is as follows:

  1. We will begin at 1pm ET/ 10am PT with a brief introduction to the ASTRA initiative and our charge in developing concepts from Peter Kurczynski, Chief Scientist of the NASA Cosmic Origins Program Office.
  2. Following this, we will open the floor to any member of the community to present a 3 slide / 2min pitch of a mission pre-concept (i.e. does not have to be a fully formed idea). This could look like one or more interesting science questions that you are looking for collaborators to help build into a well-founded mission concept, to a cutting edge technology that could be infused into or enable a future IR mission and you’d like science investigators to help develop, to a concept that has been already submitted to a competitive mission selection process. The goal here is to bring the community together and encourage a breadth of ideas so that community members may figure out where they can contribute and participate in the ASTRA process.
  3. Following these pitches, we would open the floor for a discussion of the recurrent and over-arching science theme drivers that motivate cosmic origins mission development, distilling the outcome into broad topical/mission bins.
  4. In the last ~hour, we will enable breakout rooms around these topics so that community members can self-organize. The goal here is to form small teams that will eventually complete and submit an ASTRA initiative mission concept template found here.

Meeting connection information will be provided prior to Friday. Please feel free to share amongst your colleagues and students, our community benefits from a diversity of ideas. We hope to see you there!

Meeting Connection

Join the Meeting

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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.

The post IR STIG Meeting, 12 June 2026 appeared first on NASA Science.

  •  

Cosmic Origins Seminar, 10 June 2026

Cosmic Origins Seminar

Location

Virtual

Dates

10 June 2026
12:00pm – 1:00pm ET
9:00am – 10:00am PT 

Community

Cosmic Origins

Type

Seminar

The ASTRA Initiative

Speaker

Jessica Gaskin

The ASTRA initiative will promote new strategic mission concepts for astrophysics, see here. We would like to encourage you to think about new strategic mission concepts for the coming decades of astrophysics.

As part of ASTRA, the Community Science (Ad ASTRA) Workshop will take place 1-3 September 2026 in Pasadena. New concept ideas will be discussed at this event.

To join the ASTRA initiative, mission concept template is now available, see here. There are also instructions for submission. Submitted concept ideas will be discussed at the September workshop.

Seminar Connection

Join the Seminar

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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.

The post Cosmic Origins Seminar, 10 June 2026 appeared first on NASA Science.

  •  

HWO SIG Seminar, 10 June 2026

HWO SIG Seminar

Habitable Worlds Observatory Science Interest Group

HWO SIG about HWO SIG Seminar

Location

Virtual

dates

10 June 2026
10:00am PT / 1:00pm ET

Community

HWO SIG

Type

Seminar

Agenda

HWO SIG Host: Jessie Christiansen

TopicSpeaker
HWO Events at the AASRob Zellem / Raissa Estrella
CSIT UpdateScott Gaudi
Where HWO Fits into ASTRA / the Astro2030 DecadalJessica Gaskin
Pre-Proposal Instrument Study Meeting Report OutAki Roberge

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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.

The post HWO SIG Seminar, 10 June 2026 appeared first on NASA Science.

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ASTRA Initiative Seminar, June 12, 2026

ASTRA Initiative Seminar

Location

Virtual

Dates

12 June 2026
12:00pm-1:00pm ET /
9:00am-10:00am PT 

Community

Cosmic Origins

TYpe

Seminar

Ground- and Space-Based Astronomy in the 2030s/2040s 

Speaker

Rob Petre, NASA / GSFC

Abstract

The three Astrophysics Program Analysis Groups (PAGs) – the Cosmic Origins Program Analysis Group (COPAG), the Exoplanet Exploration Program Analysis Group (ExoPAG), and the Physics of the Cosmos Program Analysis Group (PhysPAG) – have been asked to jointly report up to six community prioritized mission concepts, in addition to the X-ray and Far-IR flagship mission concepts recommended by Astro2020, to the NASA Astrophysics Division Director, for consideration for entrance into the ASTRA Initiative. These concepts should be selected in the context of the current and planned international suite of ground- and space-based observatories. In this talk we present results adapted from one of the Habitable Worlds Observatory (HWO) Community Working Groups, in which we lay out the context of ground- and space-based observatories and missions expected to operate in the 2030s/40s. We summarize outputs from our community-driven mission database, which outlines the science goals and capabilities of observatories and missions expected to operate during that time period. This information enables identification of synergies between these planned facilities and potential new concepts, as well as capability gaps in the planned suite of observatories that could be filled by entrants to the ASTRA Initiative.

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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.

The post ASTRA Initiative Seminar, June 12, 2026 appeared first on NASA Science.

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Cosmic Origins at AAS 248, June 2026

Cosmic Origins at AAS 248

The 248th Meeting of the American Astronomical Society

Cosmic Origins about Cosmic Origins at AAS 248

Location

Pasadena, California

Dates

14-18 June 2026

Community

Cosmic Origins

Type

Meeting

AAS Meeting 248

Joint AAS with HEAD and Laboratory Astrophysics Divisions Meeting

To be held 14-18 June 2026 at the Pasadena Convention Center.

The meeting will be jam-packed with great scientific content and provide ample opportunity for networking with friends and colleagues.

Meeting Overview about Joint AAS with HEAD and Laboratory Astrophysics Divisions Meeting
Pasadena Convention Center

The 248th AAS meeting (joint with HEAD and Laboratory Astrophysics Divisions) will be held 14-18 June in Pasadena, California.

Join us in the exhibit hall at the NASA booth and attend the NASA session

All times Pacific

Tuesday, 16 June 2026

TimeEventLocation
10:00am ‑ 11:30amNASA’s Big Science, Small MissionsPasadena Convention Center – Conference Center, 204

Summary

The opportunity to conduct focused science programs with small missions has increased as access to space becomes easier and more cost effective. This expansion opens the door to greater community participation in space missions, including by early-career scientists and those who may not have prior experience in building and designing such missions. This session seeks to bring together experts from the suborbital and low cost access to space community to hare their mission design process and experience launching missions for dedicated science.

As we approach the Astro2030 decadal survey it is timely to start discussions on innovative ways to perform science observations cheaper and faster by leveraging commercial capabilities for missions of all sizes.

NASA’s Big Science, Small Missions Session Agenda

Join the Session

TimeTopicSpeaker
10:00am ‑ 10:05amWelcomeSwara Ravindranath (NASA GSFC)
10:05am ‑ 10:15amFORTIS Sounding RocketEmily Witt (Johns Hopkins University)
10:15am ‑ 10:25amBlackCAT CubeSatAbe Falcone (Pennsylvania State University)
10:25am ‑ 10:35amSunRISE CubeSat ConstellationJoseph Lazio (University of Michigan)
10:35am ‑ 10:45amSPHEREx Medium Explorer MissionRoberta Paladini (IPAC/Caltech)
10:45am ‑ 10:55amLandolt Pioneer MissionPeter Kurczynski (NASA GSFC)
10:55am ‑ 11:05amNon‑Traditional Path to MissionsSanchayeeta Borthakur (Arizona State University)
11:05am ‑ 11:10amBreak
11:10am ‑ 11:30amPanel DiscussionPanel Moderator: Swara Ravindranath (NASA GSFC)
Drew Miles (Caltech)
Pablo Saz Parkinson (NASA HQ)
Joseph Lazio (University of Michigan)
Abe Falcone (Pennsylvania State University)
David Ardila (JPL)

Thursday, 18 June 2026

TimeSessionLocation
10:00am ‑ 11:30amSpecial Session: Planning for the Future of Astrophysics and the ASTRA Initiative Pasadena Convention Center ‑ 
Ballroom G

ASTRA Initiative Special Session

TimeTopicSpeakerPresentation
10:00am ‑ 10:10amIntroduction from the NASA Astrophysics Division DirectorShawn Domagal‑Goldman
10:10am ‑ 10:25amThe ASTRA Initiative: Overview & Path ForwardJessica Gaskin, NASA HQ
10:25am ‑ 10:40amInnovation for Astrophysics Workshop: Initial FindingsKendra Short, JPL
10:40am ‑ 10:55amAd ASTRA Community Science WorkshopPeter Kurczynski, NASA/GSFC
10:55am ‑ 11:30amPanel DiscussionFrancesca Civano, NASA/GSFC

Other Cosmic Origins Related Sessions

DaySession TitleTimeLocations
Monday, 15 JuneEverything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory10:00am ‑ 11:30amBallroom G
Nancy Grace Roman Space Telescope 12:45pm ‑ 1:45pmBallroom A
(Town Hall)
NASA Update12:45pm ‑ 1:45pmBallroom DE
(Town Hall)
The PRobe Infrared Mission for Astrophysics (PRIMA)2:00pm – 3:30pmBallroom G
Wednesday, 17 JuneThe NASA Astrophysics ROSES Program11:00am ‑ 12:00pmSplinter 204
NASA Infrared Telescope Facility – The Next Decade12:45pm ‑ 1:45pmTown Hall Ballroom F

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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.

The post Cosmic Origins at AAS 248, June 2026 appeared first on NASA Science.

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DGCE SIG Seminar, 25 June 2026

DGCE SIG Seminar

Diffuse Gas in Cosmic Ecosystems Science Interest Group

DGCE SIG about DGCE SIG Seminar

Location

Virtual

Dates

25 June 2026
4:00pm ET / 1:00pm PT

Community

DGCE SIG

Type

Seminar

Cosmic Origins Science in the New Landscape of Space Astrophysics

Speaker

Swara Ravindranath, Deputy Chief Scientist of NASA’s Cosmic Origins Program (NASA GSFC)

Abstract

Cosmic Origins Science covers a broad range of topics that are fundamental to our understanding of the evolution of structure in the Universe and the physical processes that can explain the formation of galaxies, stars, and planets that we observe today. The various space telescopes that operate across the electromagnetic spectrum have been crucial to address some of the most fundamental questions related to our cosmic origins. The landscape of Space Astronomy is evolving fast with innovative technology, industry partnerships, and new commercial launch capabilities. In this talk, I will review the Cosmic Origins Program and discuss the new opportunities that offer strategic pathways for focused-science missions.

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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.

The post DGCE SIG Seminar, 25 June 2026 appeared first on NASA Science.

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Community Science (Ad ASTRA) Workshop, Sept 2026

Community Science (Ad ASTRA) Workshop

The workshop will take place in Baxter Lecture Hall on the Caltech campus in Pasadena, California

ASTRA Initiative about Community Science (Ad ASTRA) Workshop

Location

Pasadena, California
& Virtual

Dates

1-3 September 2026

Community

Cosmic Origins

Type

Workshop

The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in defining future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities, and Missions—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community input. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio.

This workshop is organized by the NASA Astrophysics Program Offices in partnership with the Infrared Processing and Analysis Center (IPAC).

Important Dates: 

  • Registration opens: March 31, 2026
  • Abstract deadline: June 24, 2026
  • Contributed talks/posters selection: July 1, 2026
  • Deadline for in-person registration: August 15, 2026
  • Deadline for virtual registration: August 31, 2026

Session Connection: Join the Session

Day 1 Science

TimeTopicSpeakersPresentations
8:30amIntroduction to ASTRAShawn Domagal-Goldman, APD Director
9:00amPlan for the Workshop: Deliverables and Mandate (Day 1 focus)Jessica Gaskin, APD AD for Concept and Tech Development
9:20amHow did we get here: PhysPAGManel Errando, PhysPAG EC chair
9:40amHow did we get here: COPAGShouleh Nikzad, COPAG EC Chair
10:00amHow did we get here: EXOPAGIan Crossfield, ExoPAG EC Chair
10:20amMorning Break
11:00amPressing Science Questions for Space Missions in the 2030s and Beyond

Parallel Breakout Sessions:
-Compact Objects and Energetic Phenomena
-Cosmology
-Galaxies
-Exoplanets & Astrobiology
-Stars and Stellar Populations
Contributed presentations from community members (TBA after abstract selection)
12:30pmLunch
Afternoon
2:00pmPressing Science Questions for Space Missions in the 2030s and Beyond

Parallel Breakout Sessions:
-Compact Objects and Energetic Phenomena
-Cosmology
-Galaxies
-Exoplanets & Astrobiology
-Stars and Stellar Populations
Contributed presentations from community members (TBA after abstract selection)
3:30pmAfternoon Break
4:00pmSynthesis Panel on Pressing Science Questions for Space Missions in the 2030s and BeyondBreakout Session Moderators
5:00pmEvening Reception
7:00pmEnd of Day 1

Day 2 Capabilities

Session Connection: Join the Session

TimeTopicSpeakersPresentations
9:00amPlan for the Workshop: Deliverables
and Mandate (Day 2 focus)
EC PAG Chairs
9:10amInnovation Workshop SummaryInnovation Workshop SOC speaker
9:50amNASA Strategic Technology GapsChief Technologist from PAGs
10:10amMorning Break
10:40amEmerging Technologies (session)Presentations from 
community/industry members (TBA)
12:30pmLunch
Afternoon
2:00pmAstrophysics Technology: Capabilities Needed

Parallel Breakout Sessions: What are 
the capabilities needed (software and hardware, platform, location) relevant
to the ASTRA submitted mission concepts?

-Breakout categories TBD
Contributed presentations from 
community members (TBA after
abstract selection)
4:00pmAfternoon Break
4:45pmSynthesis panel to summarize the breakout sessions on capabilitiesBreakout Session Moderators
5:45pmEnd of Day 2

Day 3 Wrap UP

Session Connection: Join the Session

TimeTopicSpeakersPresentations
9:00amPlan for the workshop: Deliverables and Mandate (Day 3 focus)EC PAG Chairs
9:10amBeyond the Selection: The Path ForwardJessica Gaskin, APD AD for Concept and Tech Development
9:50amWorkshop synthesis 1: Key Science Questions for the 2030s and Beyond
TBA
10:50amMorning Break
11:20amWorkshop synthesis 2: Key Technology Capabilities for the 2030s and BeyondTBA
12:20pmLunch
Afternoon
2:00pmBuilding the Future: Community consensus on Science, Capabilities, and Missions for the next decadesTBA
3:30pmClosing RemarksTBA
4:00pmEnd of Day 3

Selected Abstracts

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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.

The post Community Science (Ad ASTRA) Workshop, Sept 2026 appeared first on NASA Science.

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