Suggested Searches

 

Stars

Stars Science Interest Group (Stars SIG) will help NASA understand and implement recommendations from the upcoming decadal survey in the area of stars and stellar populations.

About
News & Events
Leadership
Contact

About Stars SIG

Stars and Stellar Populations

The Cosmic Origins program is forming a science interest group (SIG) that will help NASA understand and implement recommendations from the upcoming decadal survey in the area of stars and stellar populations.

This group will also sponsor discussions, research seminars, and periodic meetings.

Star cluster Westerlund 2 as observed by the Hubble Space Telescope. The overall scene has an L shaped series of bright clouds at the bottom left, and clearer space toward the top right. There is a bright orange-white star cluster to the cloudy region’s immediate right, just above center. The scene is set against the black background of space, which has blue-white, orange-white, and white points of light scattered all across it.
This young cluster of about 3,000 stars in our Milky Way is called Westerlund 2 and contains some of the galaxy's hottest, brightest, and most massive stars. Hubble's infrared vision pierced dust around this stellar nursery to reveal the dense concentration of stars in the...
NASA, ESA, Hubble Heritage Project, Westerlund 2 Science Team, Antonella Nota (ESA, STScI)

News & Events
Stars Science Interest Group (STARS SIG)
1 min read

Leadership Council Name Affiliation and Email Yuan-Sen Ting Australian National UniversityEmail Keith Hawkins University of Texas – AustinEmail Jennifer Johnson…

Topic

Leadership Council

NameAffiliation and Email
Yuan-Sen TingAustralian National University
Email
Keith HawkinsUniversity of Texas - Austin
Email
Jennifer JohnsonOhio State University
Email
Racheal BeatonPrinceton / Carnegie
Email
Ting LiUniversity of Toronto
Email
Kathleen KraemerBoston College
Email
Philip MoczLawrence Livermore National Laboratory
Email
Derek BuzasiFlorida Gulf Coast University
Email
Rosemary WyseJohns Hopkins University
Email

How to Participate

We invite participation from the community, particularly from early-career researchers and those from under represented backgrounds in astronomy. Please contact us for more information about our activities and mission, and how you can get involved.

Contact Us about How to Participate
Webb and Hubble�s Views of Spiral Galaxy NGC 628

News Straight to Your Inbox

Subscribe to your community email news list

We will never share your email address.

Privacy Policy

Sign Up
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.