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2 min read
Hubble Surveys Cloudy Cluster This new NASA/ESA Hubble Space Telescope image features the nebula LMC N44C. ESA/Hubble & NASA, C. Murray, J. Maíz Apellániz
This new NASA/ESA Hubble Space Telescope image features a cloudy starscape from an impressive star cluster. This scene is in the Large Magellanic Cloud, a dwarf galaxy situated about 160,000 light-years away in the constellations Dorado and Mensa. With a mass equal to 10–20% of the mass of the Milky Way, the Large Magellanic Cloud is the largest of the dozens of small galaxies that orbit our galaxy.
The Large Magellanic Cloud is home to several massive stellar nurseries where gas clouds, like those strewn across this image, coalesce into new stars. Today’s image depicts a portion of the galaxy’s second-largest star-forming region, which is called N11. (The most massive and prolific star-forming region in the Large Magellanic Cloud, the Tarantula Nebula, is a frequent target for Hubble.) We see bright, young stars lighting up the gas clouds and sculpting clumps of dust with powerful ultraviolet radiation.
This image marries observations made roughly 20 years apart, a testament to Hubble’s longevity. The first set of observations, which were carried out in 2002–2003, capitalized on the exquisite sensitivity and resolution of the then-newly-installed Advanced Camera for Surveys. Astronomers turned Hubble toward the N11 star cluster to do something that had never been done before at the time: catalog all the stars in a young cluster with masses between 10% of the Sun’s mass and 100 times the Sun’s mass.
The second set of observations came from Hubble’s newest camera, the Wide Field Camera 3. These images focused on the dusty clouds that permeate the cluster, providing us with a new perspective on cosmic dust.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubbleMedia Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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PAW Participant Discussion
Participants are encouraged to dialogue before, during, and after the workshop. Contact the organizing committee for further questions.
PAW Participant Discussion
Participants are encouraged to dialogue before, during, and after the workshop. Contact the organizing committee for further questions.
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Drag Prediction Workshop Series
The Drag Prediction Workshop series is an extensive international effort to improve transonic aerodynamic predictions. This long-running collaborative effort seeks to mobilize the international aerospace community to improve the computational methods and tools to predict transonic aircraft performance, particularly drag.
More details on the workshop can be found at the workshop website: https://www.aiaa-dpw.org
NASA has a storied history with the workshop series from DPW-I (hosted in 2001) through the upcoming DPW-8, held in concert with Aeroelastic Prediction Workshop 4. In addition to code and methods improvements, the series also resulted in the NASA/Boeing Common Research Model (https://commonresearchmodel.larc.nasa.gov/), an open-access, commercially-relevant aircraft geometry. This geometry has been extensively tested in many facilities throughout the world and been the subject of multiple workshop series.
NASA’s contributions to the upcoming DPW-8 and subsequent work will be highlighted on this page.
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The post This Week's Sky at a Glance, September 12 – 21 appeared first on Sky & Telescope.
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NASA Armstrong to Host Partnership Day Oct. 21-22
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA Graphics
NASA’s Armstrong Flight Research Center in Edwards, California, invites innovative companies, government agencies, and organizations to attend Partnership Days, scheduled for Oct. 21-22, 2025, at the center.
The event offers a unique opportunity to explore collaboration with NASA on cutting-edge research and development in areas such as aerospace, autonomy, sustainability, and more. Attendees will engage with NASA experts and learn how Armstrong’s capabilities can help accelerate innovation and bring transformative technologies to life.
Space is limited, and RSVP is required by Sept. 26.
To register, scan the QR code on the event poster or email AFRC-CAL-330-Partnerships@mail.nasa.gov.
What: NASA Armstrong Partnership Days
When: Oct. 21-22, 2025
Where: NASA’s Armstrong Flight Research Center, Edwards, California
Who: Industry leaders, government agencies, and organizations interested in research and development partnerships with NASA
For information about NASA Armstrong and other agency programs, visit:
https://www.nasa.gov/armstrong
-end-
Dede Dinius
Armstrong Flight Research Center, Edwards, California
661-276-5701
darin.l.dinius@nasa.gov
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Humans in Space
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NASA Armstrong to Host Partnership Day Oct. 21-22
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA GraphicsNASA’s Armstrong Flight Research Center in Edwards, California, invites innovative companies, government agencies, and organizations to attend Partnership Days, scheduled for Oct. 21-22, 2025, at the center.
The event offers a unique opportunity to explore collaboration with NASA on cutting-edge research and development in areas such as aerospace, autonomy, sustainability, and more. Attendees will engage with NASA experts and learn how Armstrong’s capabilities can help accelerate innovation and bring transformative technologies to life.
Space is limited, and RSVP is required by Sept. 26.
To register, scan the QR code on the event poster or email AFRC-CAL-330-Partnerships@mail.nasa.gov.
What: NASA Armstrong Partnership Days
When: Oct. 21-22, 2025
Where: NASA’s Armstrong Flight Research Center, Edwards, California
Who: Industry leaders, government agencies, and organizations interested in research and development partnerships with NASA
For information about NASA Armstrong and other agency programs, visit:
https://www.nasa.gov/armstrong
-end-
Dede Dinius
Armstrong Flight Research Center, Edwards, California
661-276-5701
darin.l.dinius@nasa.gov
Missions
Humans in Space
Climate Change
Solar System
NASA Ames Science Directorate: Stars of the Month – September 2025
The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Taejin Park, Lydia Schweitzer, and Rachel Morgan. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond.
Earth Science Star: Taejin Park
Taejin Park is a NASA Earth eXchange (NEX) research scientist within the Biospheric Science Branch, for the Bay Area Environmental Research Institute (BAERI). As the Project Scientist for the Wildfire, Ecosystem Resilience, & Risk Assessment (WERK) project, he has exhibited exemplary leadership and teamwork leading to this multi-year study with the California Natural Resources Agency (CNRA) and California Air Resources Board (CARB) to develop tracking tools of statewide ecological condition, disturbance, and recovery efforts related to wildfires.
Space Science and Astrobiology Star: Lydia Schweitzer
Lydia Schweitzer is a research scientist within the Planetary Systems Branch for the Bay Area Environmental Research Institute (BAERI) as a member of the Neutron Spectrometer System (NSS) team with broad contributions in instrumentation, robotic rovers and lunar exploration. Lydia is recognized for her leadership on a collaborative project to design and build a complex interface unit that is crucial for NSS to communicate with the Japanese Space Agency’s Lunar Polar eXploration rover mission (LUPEX). In addition, she is recognized for her role as an instrument scientist for the Volatiles Investigating Polar Exploration Rover (VIPER) and MoonRanger missions.
Space Science and Astrobiology Star: Rachel Morgan
Rachel Morgan is an optical scientist in the Astrophysics Branch for the SETI Institute. As AstroPIC’s lead experimentalist and the driving force behind the recently commissioned photonic testbed at NASA Ames, this month she achieved a record 92 dB on-chip suppression on a single photonic-integrated chip (PIC) output channel. This advances critical coronagraph technology and is a significant milestone relevant to the Habitable Worlds Observatory.
NASA Ames Science Directorate: Stars of the Month – September 2025
The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Taejin Park, Lydia Schweitzer, and Rachel Morgan. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond.
Earth Science Star: Taejin ParkTaejin Park is a NASA Earth eXchange (NEX) research scientist within the Biospheric Science Branch, for the Bay Area Environmental Research Institute (BAERI). As the Project Scientist for the Wildfire, Ecosystem Resilience, & Risk Assessment (WERK) project, he has exhibited exemplary leadership and teamwork leading to this multi-year study with the California Natural Resources Agency (CNRA) and California Air Resources Board (CARB) to develop tracking tools of statewide ecological condition, disturbance, and recovery efforts related to wildfires.
Space Science and Astrobiology Star: Lydia SchweitzerLydia Schweitzer is a research scientist within the Planetary Systems Branch for the Bay Area Environmental Research Institute (BAERI) as a member of the Neutron Spectrometer System (NSS) team with broad contributions in instrumentation, robotic rovers and lunar exploration. Lydia is recognized for her leadership on a collaborative project to design and build a complex interface unit that is crucial for NSS to communicate with the Japanese Space Agency’s Lunar Polar eXploration rover mission (LUPEX). In addition, she is recognized for her role as an instrument scientist for the Volatiles Investigating Polar Exploration Rover (VIPER) and MoonRanger missions.
Space Science and Astrobiology Star: Rachel MorganRachel Morgan is an optical scientist in the Astrophysics Branch for the SETI Institute. As AstroPIC’s lead experimentalist and the driving force behind the recently commissioned photonic testbed at NASA Ames, this month she achieved a record 92 dB on-chip suppression on a single photonic-integrated chip (PIC) output channel. This advances critical coronagraph technology and is a significant milestone relevant to the Habitable Worlds Observatory.
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Stellar mass black holes have only a few solar masses, and are much different from their gigantic counterparts, supermassive black holes. When these modestly-massive black holes are actively accreting matter, new research shows that the process is anything but orderly. Instead, it's characterized by different velocities, different ionization zones, and other complexities.