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By NASA
This NASA/ESA Hubble Space Telescope reveals clouds of gas and dust near the Tarantula Nebula, located in the Large Magellanic Cloud about 160,000 light-years away.ESA/Hubble & NASA, C. Murray The universe is a dusty place, as this NASA/ESA Hubble Space Telescope image featuring swirling clouds of gas and dust near the Tarantula Nebula reveals. Located in the Large Magellanic Cloud about 160,000 light-years away in the constellations Dorado and Mensa, the Tarantula Nebula is the most productive star-forming region in the nearby universe, home to the most massive stars known.
The nebula’s colorful gas clouds hold wispy tendrils and dark clumps of dust. This dust is different from ordinary household dust, which may include bits of soil, skin cells, hair, and even plastic. Cosmic dust is often comprised of carbon or of molecules called silicates, which contain silicon and oxygen. The data in this image was part of an observing program that aims to characterize the properties of cosmic dust in the Large Magellanic Cloud and other nearby galaxies.
Dust plays several important roles in the universe. Even though individual dust grains are incredibly tiny, far smaller than the width of a single human hair, dust grains in disks around young stars clump together to form larger grains and eventually planets. Dust also helps cool clouds of gas so that they can condense into new stars. Dust even plays a role in making new molecules in interstellar space, providing a venue for individual atoms to find each other and bond together in the vastness of space.
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By NASA
Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read
Hubble Spies a Spiral That May Be Hiding an Imposter
The spiral galaxy UGC 5460 shines in this NASA/ESA Hubble Space Telescope image. UGC 5460 sits about 60 million light-years away in the constellation Ursa Major. ESA/Hubble & NASA, W. Jacobson-Galán, A. Filippenko, J. Mauerhan
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The sparkling spiral galaxy gracing this NASA/ESA Hubble Space Telescope image is UGC 5460, which sits about 60 million light-years away in the constellation Ursa Major. This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms, and bright blue star clusters. Also captured in the upper left-hand corner is a far closer object: a star just 577 light-years away in our own galaxy.
UGC 5460 has hosted two recent supernovae: SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programs that aim to study various kinds of supernovae.
SN 2015as was as a core-collapse supernova: a cataclysmic explosion that happens when the core of a star far more massive than the Sun runs out of fuel and collapses under its own gravity, initiating a rebound of material outside the core. Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a supernova collides with the gas that surrounds the exploded star.
SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae. Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location with the goal of revealing the explosion’s origin.
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The Death Throes of Stars
Homing in on Cosmic Explosions
Media Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
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Last Updated Feb 21, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
Hubble Space Telescope Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Spiral Galaxies Stars Supernovae Keep Exploring Discover More Topics From NASA
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble’s Night Sky Challenge
Hubble’s Galaxies
Reshaping Our Cosmic View: Hubble Science Highlights
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By NASA
NASA’s SPHEREx is situated on a work stand ahead of prelaunch operations at the Astrotech Processing Facility at Vandenberg Space Force Base in California. The SPHEREx space telescope will share its ride to space on a SpaceX Falcon 9 rocket with NASA’s PUNCH mission.
Credit: USSF 30th Space Wing/Christopher
NASA will provide live coverage of prelaunch and launch activities for SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer), the agency’s newest space telescope. This will lift off with another NASA mission, Polarimeter to Unify the Corona and Heliosphere, or PUNCH, which will study the Sun’s solar wind.
The launch window opens at 10:09 p.m. EST (7:09 p.m. PST) Thursday, Feb. 27, for the SpaceX Falcon 9 rocket that will lift off from Space Launch Complex 4 East at Vandenberg Space Force Base in California. Watch coverage on NASA+. Learn how to watch NASA content through a variety of platforms, including social media.
The SPHEREx mission will improve our understanding of how the universe evolved and search for key ingredients for life in our galaxy.
The four small spacecraft that comprise PUNCH will observe the Sun’s corona as it transitions into solar wind.
The deadline for media accreditation for in-person coverage of this launch has passed. NASA’s media credentialing policy is available online. For questions about media accreditation, please email: ksc-media-accreditat@mail.nasa.gov.
NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):
Tuesday, Feb. 25
2 p.m. – SPHEREx and PUNCH Science Overview News Conference
Shawn Domagal-Goldman, acting director, Astrophysics Division, NASA Headquarters Joe Westlake, director, Heliophysics Division, NASA Headquarters Nicholeen Viall, PUNCH Mission Scientist, NASA’s Goddard Space Flight Center Rachel Akeson, SPHEREx science data center lead, Caltech/IPAC Phil Korngut, SPHEREx instrument scientist, Caltech The news conference will stream on NASA+. Media may ask questions in person or via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov.
Wednesday, Feb. 26
3:30 p.m. – SPHEREx and PUNCH Prelaunch News Conference
Mark Clampin, acting deputy associate administrator, Science Mission Directorate, NASA Headquarters David Cheney, PUNCH program executive, NASA Headquarters James Fanson, SPHEREx project manager, NASA’s Jet Propulsion Laboratory Denton Gibson, launch director, NASA’s Launch Services Program Julianna Scheiman, director, NASA Science Missions, SpaceX U.S. Air Force 1st Lt. Ina Park, 30th Operations Support Squadron launch weather officer Coverage of the prelaunch news conference will stream live on NASA+.
Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov.
Thursday, Feb. 27
12 p.m. – SPHEREx and PUNCH Launch Preview will stream live on NASA+.
9:15 p.m. – Launch coverage begins on NASA+.
10:09 p.m. – Launch window opens.
Audio Only Coverage
Audio only of the launch coverage will be carried on the NASA “V” circuits, which may be accessed by dialing 321-867-1220, or -1240. On launch day, “mission audio,” countdown activities without NASA+ media launch commentary, will be carried on 321-867-7135.
NASA Website Launch Coverage
Launch day coverage of the mission will be available on the agency’s website. Coverage will include links to live streaming and blog updates beginning no earlier than 9:15 p.m., Feb. 27, as the countdown milestones occur. On-demand streaming video and photos of the launch will be available shortly after liftoff.
For questions about countdown coverage, contact the Kennedy newsroom at 321-867-2468. Follow countdown coverage on the SPHEREx blog.
Attend the Launch Virtually
Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch.
Watch, Engage on Social Media
You can also stay connected by following and tagging these accounts:
X: @NASA, @NASAJPL, @NASAUnivese, @NASASun, @NASAKennedy, @NASA_LSP
Facebook: NASA, NASAJPL, NASA Universe, NASASunScience, NASA’s Launch Services Program
Instagram: @NASA, @NASAKennedy, @NASAJPL, @NASAUnivese
For more information about these missions, visit:
https://science.nasa.gov/mission/spherex/
https://science.nasa.gov/mission/punch/
-end-
Alise Fisher – SPHEREx
Headquarters, Washington
202-617-4977
alise.m.fisher@nasa.gov
Sarah Frazier – PUNCH
Goddard Space Flight Center, Greenbelt, Md.
202-853-7191
sarah.frazier@nasa.gov
Laura Aguiar
Kennedy Space Center, Florida
321-593-6245
laura.aquiar@nasa.gov
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Last Updated Feb 18, 2025 LocationNASA Headquarters Related Terms
SPHEREx (Spectro-Photometer for the History of the Universe and Ices Explorer) Missions Polarimeter to Unify the Corona and Heliosphere (PUNCH) Science Mission Directorate View the full article
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By NASA
Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read
Hubble Captures a Cosmic Cloudscape
This NASA/ESA Hubble Space Telescope reveals clouds of gas and dust near the Tarantula Nebula, located in the Large Magellanic Cloud about 160,000 light-years away. ESA/Hubble & NASA, C. Murray
Download this image
The universe is a dusty place, as this NASA/ESA Hubble Space Telescope image featuring swirling clouds of gas and dust near the Tarantula Nebula reveals. Located in the Large Magellanic Cloud about 160,000 light-years away in the constellations Dorado and Mensa, the Tarantula Nebula is the most productive star-forming region in the nearby universe, home to the most massive stars known.
The nebula’s colorful gas clouds hold wispy tendrils and dark clumps of dust. This dust is different from ordinary household dust, which may include of bits of soil, skin cells, hair, and even plastic. Cosmic dust is often comprised of carbon or of molecules called silicates, which contain silicon and oxygen. The data in this image was part of an observing program that aims to characterize the properties of cosmic dust in the Large Magellanic Cloud and other nearby galaxies.
Dust plays several important roles in the universe. Even though individual dust grains are incredibly tiny, far smaller than the width of a single human hair, dust grains in disks around young stars clump together to form larger grains and eventually planets. Dust also helps cool clouds of gas so that they can condense into new stars. Dust even plays a role in making new molecules in interstellar space, providing a venue for individual atoms to find each other and bond together in the vastness of space.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore More
Caldwell 103 / Tarantula Nebula / 30 Doradus
Hubble Studies the Tarantula Nebula’s Outskirts
Hubble’s New View of the Tarantula Nebula
Hubble’s Bubbles in the Tarantula Nebula
Hubble Probes Interior of Tarantula Nebula
Media Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
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Details
Last Updated Feb 13, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
Hubble Space Telescope Absorption or Dark Nebulae Astrophysics Astrophysics Division Emission Nebulae Goddard Space Flight Center Nebulae Star-forming Nebulae The Universe Keep Exploring Discover More Topics From Hubble
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Exploring the Birth of Stars
Hubble’s Night Sky Challenge
Hubble Focus: The Lives of Stars
This e-book highlights the mission’s recent discoveries and observations related to the birth, evolution, and death of stars.
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By NASA
“I’m hopeful anyone, regardless of their scientific background, could read a Hubble post and understand the gist of it and be interested in it,” said Elizabeth Tammi, social media lead for the Hubble Space Telescope. “I also read our stories with the eye of the potential audience member: What are they going to care about? What is going to bring them into this story? What is going to make them want to read more?”Credits: Courtesy of Elizabeth Tammi Name: Elizabeth Tammi
Title: Hubble Space Telescope Social Media Lead
Formal Job Classification: Communications Specialist
Organization: Hubble Space Telescope Operations (Code 441)
What do you do and what is most interesting about your role here at Goddard? How do you help support Goddard’s mission?
I am the social media lead for the Hubble Space Telescope mission at Goddard. In short, Hubble is an orbiting observatory that’s been in low-Earth orbit for more than 30 years. It’s one of NASA’s flagship missions, probably one of its most iconic missions. Hubble has shaped our understanding of how we imagine the universe — visually how we think about it.
I run Hubble’s Twitter, Facebook, Instagram, and Flickr, along with various other multimedia and communications tasks. We’re a very close-knit team, so we collaborate a lot, both within our team, and with other missions across the agency as well.
I’m primarily focused on social media and figuring out how are we going to share our news. On any given day, I might also be working on a script, editing news releases, or working with other accounts on social media campaigns. It’s different every day, which I really like.
What is your educational background?
I went to Mercer University, which is in Macon, Georgia. I graduated in 2020 with a degree in journalism and creative writing. There, they have a great program called the Center for Collaborative Journalism, which allowed us to work in newsrooms for academic credit. That was really useful, especially in this field, getting that hands-on experience and getting published from my freshman year on. I was eventually able to intern at Goddard the summer before my senior year. I really don’t think that would have been possible if I hadn’t had the audio production experience that Mercer allowed me to get, along with just all aspects of journalism, media, and communications.
“Hubble is one of NASA’s flagship missions, probably one of its most iconic missions,” said Elizabeth Tammi, social media lead for the Hubble Space Telescope. “Hubble has shaped our understanding of how we imagine the universe — visually how we think about it.”Credits: Courtesy of Elizabeth Tammi How does your writing experience contribute to your role with Hubble?
I know how to write accessibly and in a straightforward manner. I’m hopeful anyone, regardless of their scientific background, could read a post and understand the gist of it and be interested in it. That’s the goal. I try to come up with interesting turns of phrase when I can. I also read our stories with the eye of the potential audience member: What are they going to care about? What is going to bring them into this story? What is going to make them want to read more?
Outside work, you’ve written and published books. What inspired you to decide to write?
There’s not a day I can remember where I wasn’t absolutely infatuated with books. I think my parents read to me long before I could even understand them. It was just always such a huge part of my life — and I loved, loved, loved reading. When I realized that actual people wrote books, then I knew I wanted to write. To be clear, I didn’t take real steps toward that until I was about 15, 16-ish years old, because I guess in my mind, I still had this idea that authors were more than human.
I’ve since had two novels published. Both are in the fantasy genre and earned complimentary reviews; my second novel even earned a Moonbeam Children’s Book Award.
“I know it can be intimidating, to think about NASA as a place to intern,” said Hubble Space Telescope social media lead Elizabeth Tammi. “If you have any interest in space, I think that’s the most important part: People who are passionate and interested in our space program.”Credits: Courtesy of Elizabeth Tammi What do you most enjoy about sharing the Hubble story?
I think my favorite part is reading the comments that we get from the public, just because everyone has been so supportive of the telescope. Social media can put on display the best and worst aspects of humanity. It’s very nice to see this supportive corner of the Internet.
So far, what I’ve really enjoyed was our “Deep Field Week” social media campaign, which was around the 25th anniversary of the Hubble Deep Field image . To the unaided eye, this was a seemingly empty patch of sky. Hubble revealed it has countless galaxies. It was a really staggering finding and definitely was a huge cultural shift in how we think about our universe.
Previously, you were a NASA intern from the Summer of 2019 to May 2020. How has that experience shaped your current role?
It was absolutely vital. I don’t think I would be here in this position without that internship experience. It was the summer before my senior year of college. I got to go up to Goddard for summer 2019 and I was working primarily as an audio production intern, though the internship afforded me the opportunity to contribute to the newsroom’s work overall.
I worked with Katie Atkinson, who I also went to college with, and we got to work on the 50th anniversary of the Apollo 11 mission. One of my primary tasks that summer was working on an oral history campaign tied to Apollo 11’s 50th anniversary . We encouraged people from all over to send in audio accounts of what they remember experiencing when Apollo 11 landed on the Moon in 1969. Or, if they didn’t remember seeing it as it happened, how did the landing affect them and their view of the world, or their career aspirations, or if they have family stories tied to Apollo.
If I could describe my NASA experience with a book title, it would be the term “Galaxy Brain.” It’s when you have a normal thought but then you think harder, and it gets bigger. From the idea of constantly feeling mind-blown by the work that’s going on around me to being part of it makes me feel, “Oh my gosh!” This “Galaxy Brain” imagery symbolizes the enormous magnitude of everything that is interesting and mysterious. It’s just something that’s constantly engaging.
Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.
By Elissa Fielding
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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