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HWO Detector System Development Study

HWO Detector System Development Study; Responses Due 7 July 2026

8 June 2026

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.

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 7 July 2026.

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

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

  •  

NASA-DARES Draft Strategy Open for Public Comment

NASA-DARES Draft Strategy Open for Public Comment; Comments Due 2 July 2026

8 June 2026

The NASA Astrobiology Program and DARES Task Force 2 are pleased to announce the opening of the public comment period for the draft Decadal Astrobiology Research and Exploration Strategy (NASA-DARES).Β Β 

The draft report, available in slide form, is available here: NASA-DARES Draft [PDF] . NB: Findings from Focus Area 9: Astrobiology in Society are forthcoming.Β 

An abbreviated summary, presented at AbSciCon, is available for viewing here: NASA-DARES Presentation Video. The NASA-DARES presentation begins at approximately 38:27 in the recording.Β 

Feedback on the draft Strategy should be submitted according to the following guidelines:Β 

  • Email comments to HQ-RFIastrobio@mail.nasa.gov with the subject line β€œNASA-DARES Public Comment”.Β Β 
  • As relevant, please indicate the Focus Area(s) addressed by your comment at the beginning of your response.Β 
  • Comments may be submitted by an individual or on behalf of a community group, organization, or other collective body.Β 
  • Anonymous submissions will not be considered.Β 
  • Comments will only be accepted as attached PDF files or as in-line email text.Β 
  • Comments must be received no later than 11:59p Eastern on 2 July 2026. Comments received after this deadline will not be considered.Β 

As a reminder, NASA-DARES is a non-consensus document. NASA-DARES is not intended to rank priorities, prescribe funding decisions, direct mission selections, establish policy, or replace decadal surveys or other consensus reports. The report is intended to capture a broad range of topics relevant to NASA Astrobiology. Inclusion in NASA-DARES should not be interpreted as an indication of future funding, programmatic priority, mission implementation, or agency commitment.Β 

For inquiries related to this public comment period, please send an email to HQ-RFIastrobio@mail.nasa.gov addressed to Drs. Rachel L. Harris, Hannah Jang-Condell, and Becky McCauley Rench. Kindly use the subject line β€œQuestion RE: NASA-DARES Public Comment Period” when submitting your questions.

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post NASA-DARES Draft Strategy Open for Public Comment appeared first on NASA Science.

  •  

IXPE Cycle 4 Pre-Proposal Workshop Announcement

IXPE Cycle 4 Pre-Proposal Workshop Announcement; Register by 25 June 2026

8 June 2026

We are pleased to send out this first announcement for a pre-proposal workshop in preparation for Cycle 4 of the IXPE General Observer (GO) program.

IXPE (the Imaging X-ray Polarimetry Explorer) provides unique and powerful X-ray polarization capabilities and has been providing crucial insights into our understanding of X-ray production and the geometry of multiple classes of objects such as neutron stars and pulsar wind nebulae, as well as stellar and supermassive black holes, among others. Overall, IXPE provides simultaneous imaging, spectral, timing, and polarization data for 2-8 keV X-rays.

The workshop will be held virtually on Tuesday 30 June 2026, from 12 noon to 3p Eastern (9a to 12 noon Pacific). This session is presented to update the community on opportunities to propose for the upcoming Cycle 4 IXPE GO program, highlighting any changes from previous cycles. A description of the IXPE mission and a summary of its major scientific achievements will be presented. Opportunities for participation through the General Observer Program, which supports a broad range of opportunities, will be described in detail in an interactive forum. Presentations on user support services, data analysis and software tools, catalogs and other online resources will also be included, followed by ample time for general questions and discussion.Β  More information can be found on the GO program website.

Registration is open to everyone. The meeting link will be sent via e-mail a day before the start of the meeting to all registered participants. There is no fee to participate in the workshop. Please register on or before 25 June 2026 to receive the link. To receive the link for the workshop, please register your interest by filling out this Google form.

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post IXPE Cycle 4 Pre-Proposal Workshop Announcement appeared first on NASA Science.

  •  

HELIOTECH and Orbital Flight Symposium

HELIOTECH and Orbital Flight Symposium; Abstracts Due 17 June 2026

8 June 2026

We are thrilled to let you know that both registration and abstract submission are officially open for NASA’s 2026 Joint HELIOTECH and Orbital Flight Symposium! By bringing together NASA’s Heliophysics Technology Symposium and Heliophysics Orbital Flight Missions, this joint meeting aims to spark innovation and foster essential collaboration for advancing technology needed to explore not only the Sun-Earth-Moon system but also Mars and destinations beyond. Our intention is to create an engaging forum where technologists, scientists, and mission Principal Investigators (PIs) can connect, share, and collaborate.

Event Details:

  • Dates: 31 August – 4 September 2026
  • Location: Johns Hopkins Applied Physics Laboratory, Laurel, Maryland
  • Format: Hybridβ€”join us in person or virtually via Zoom

Call for Abstracts: Abstract submission is now open and will close on 17 June 2026. If you’re interested in presenting, please submit your abstract using the link below. Abstracts should be a maximum of 2,000 characters and entered directly into the submission Google form. Be sure to specify your preferred presentation type: oral (in-person preferred or remote) or poster (in-person only).

Registration: Registration for the symposium is now open as well, through the symposium website! We encourage everyone to register early, whether you’re attending on-site or virtually.

For additional information about the agenda, lodging, and ongoing updates, please visit our symposium website. We look forward to your participation and contributions and hope to see everyone for an exciting and impactful event!Β 

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post HELIOTECH and Orbital Flight Symposium appeared first on NASA Science.

  •  

Upcoming SIG and SAG Activities, 15 June – 17 June 2026

Upcoming Science Interest Group & Science Analysis Group Activities

Please note also the following upcoming activities relevant to the Program Analysis Groups:

Monday 15 June at 1p Eastern (10a Pacific)

Wednesday 17 June at 1p Eastern (10a Pacific)

Wednesday 17 June at 2p Eastern (11a Pacific)

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post Upcoming SIG and SAG Activities, 15 June – 17 June 2026 appeared first on NASA Science.

  •  

Cosmic OriginsΒ Seminar, 10 June 2026

Cosmic Origins Seminar

Location

Virtual

Dates

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

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.

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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 OriginsΒ Seminar, 10 June 2026 appeared first on NASA Science.

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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.

  •  

ASTRA Initiative Seminar, June 12, 2026

ASTRA Initiative Seminar

Location

Virtual

Dates

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

Community

Cosmic Origins

TYpe

Seminar

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

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.

  •  

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 ‑ 10:15amFORTISΒ SoundingΒ 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‑TraditionalΒ PathΒ to MissionsSanchayeetaΒ BorthakurΒ (ArizonaΒ StateΒ University)
11:05am ‑ 11:10amBreak
11:10am ‑ 11:30amPanel DiscussionPanelΒ Moderator:Β SwaraΒ RavindranathΒ (NASAΒ 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 InitiativeΒ PasadenaΒ ConventionΒ Center ‑ 
Ballroom G

ASTRA Initiative Special Session

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

Other Cosmic Origins Related Sessions

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

  •  

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.

  •  

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 daysβ€”Science, Capabilities, and Missionsβ€”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:Β 

  • 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
9:00amPlanΒ forΒ theΒ Workshop:Β 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)PresentationsΒ fromΒ 
community/industry members (TBA)
12:30pmLunch
Afternoon
2:00pmAstrophysics Technology: Capabilities Needed

ParallelΒ BreakoutΒ Sessions:Β WhatΒ areΒ 
the capabilities needed (softwareΒ and hardware, platform, location) relevant
to the ASTRA submitted mission concepts?

-Breakout categories TBD
ContributedΒ presentationsΒ fromΒ 
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.

  •  

GW SIG Seminar, 10 June 2026

GW SIG Seminar

Gravitational Wave Science Interest Group

GW SIG about GW SIG Seminar

Location

GSFC B34, W150
& Virtual

Dates

10 June 2026
11:00am – 12:00pm ET

Community

GW SIG

Type

Seminar

Expected Science from deciHz Gravitational Waves

Speaker

Cole Miller, University of Maryland

Abstract

Astrophysical sources have already been detected in gravitational waves, in the tens to hundreds of Hertz range with LIGO, Virgo, and KAGRA, and in the few to tens of nanohertz range with pulsar timing arrays.Β  New sources and physics will also be available with the planned LISA mission, at millihertz frequencies.Β  Here I will talk about the remarkable prospects for physics and astrophysics in the decihertz range, including multimessenger science, essential information about stellar-mass and intermediate-mass black holes, tests of general relativity, and the possibility of a primordial background of gravitational waves. Β 

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

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

  •  

Habitable Worlds Observatory SIG Seminar, 10 June 2026

Habitable Worlds Observatory 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
Session Recording

Downloads

HWO and the ASTRA Initiative

Jun 10, 2026

PDF (1.92 MB)

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post Habitable Worlds Observatory SIG Seminar, 10 June 2026 appeared first on NASA Science.

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GR SIG Seminar, 12 June 2026

GR SIG Seminar

Gamma Ray Science Interest Group

GR SIG about GR SIG Seminar

Location

Virtual

Dates

12 June 2026
1:00pm – 2:00pm ET

Community

GR SIG

Type

Seminar

Agenda

Discussion of the white paper GR SIGΒ plans to submitΒ in response to the ASTRA initiative, as well as the endorsement of and feedback on this white paper by the community.

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

The post GR SIG Seminar, 12 June 2026 appeared first on NASA Science.

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ASTRA Initiative Seminar, 12 June 2026

ASTRA Initiative Seminar

Location

Virtual

Dates

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

Community

Physics of the Cosmos

TYpe

Seminar

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

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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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.

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

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