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A New Census of Dwarf Galaxies Shows More Massive Black Holes than Previously Thought
A new census of more than 8,000 galaxies finds active black holes rising in frequency with galaxy mass, jumping sharply in galaxies similar in mass to the Milky Way.
Hubble Snaps Stellar Baby Pictures
- Hubble Home
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3 min read
Hubble Snaps Stellar Baby Pictures The Cepheus A region is home to a number of infant stars, including a protostar that is responsible for much of the region’s illumination. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) Star-forming region G033.91+0.11 is home to a protostar hidden within a reflection nebula. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) A protostar is swathed in the gas of an emission nebula within star-forming region GAL-305.20+00.21. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) A protostar’s jets of high-speed particles are responsible for the bright region of excited, glowing hydrogen in this Hubble image. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)
Newly developing stars shrouded in thick dust get their first baby pictures in these images from NASA’s Hubble Space Telescope. Hubble took these infant star snapshots in an effort to learn how massive stars form.
Protostars are shrouded in thick dust that blocks light, but Hubble can detect the near-infrared emission that shines through holes formed by the protostar’s jets of gas and dust. The radiating energy can provide information about these “outflow cavities,” like their structure, radiation fields, and dust content. Researchers look for connections between the properties of these young stars – like outflows, environment, mass, brightness – and their evolutionary stage to test massive star formation theories.
These images were taken as part of the SOFIA Massive (SOMA) Star Formation Survey, which investigates how stars form, especially massive stars with more than eight times the mass of our Sun.
The Cepheus A region is home to a number of infant stars, including a protostar that is responsible for much of the region’s illumination. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.7 MB)
The high-mass star-forming region Cepheus A hosts a collection of baby stars, including one large and luminous protostar, which accounts for about half of the region’s brightness. While much of the region is shrouded in opaque dust, light from hidden stars breaks through outflow cavities to illuminate and energize areas of gas and dust, creating pink and white nebulae. The pink area is an HII region, where the intense ultraviolet radiation of the nearby stars has converted the surrounding clouds of gas into glowing, ionized hydrogen.
Cepheus A lies about 2,400 light-years away in the constellation Cepheus.
Download this image (5.8 MB)
Glittering much closer to home, this Hubble image depicts the star-forming region G033.91+0.11 in our Milky Way galaxy. The light patch in the center of the image is a reflection nebula, in which light from a hidden protostar bounces off gas and dust.
A protostar is swathed in the gas of an emission nebula within star-forming region GAL-305.20+00.21. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.8 MB)
This Hubble image showcases the star-forming region GAL-305.20+00.21. The bright spot in the center-right of the image is an emission nebula, glowing gas that is ionized by a protostar buried within the larger complex of gas and dust clouds.
A protostar’s jets of high-speed particles are responsible for the bright region of excited, glowing hydrogen in this Hubble image. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.7 MB)
Shrouded in gas and dust, the massive protostar IRAS 20126+4104 lies within a high-mass star-forming region about 5,300 light-years away in the constellation Cygnus. This actively forming star is a B-type protostar, characterized by its high luminosity, bluish-white color, and very high temperature. The bright region of ionized hydrogen at the center of the image is energized by jets emerging from the poles of the protostar, which ground-based observatories previously observed.
New images added every day between January 12-17, 2026! Follow @NASAHubble on social media for the latest Hubble images and news and see Hubble’s Stellar Construction Zones for more images of young stellar objects.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore MoreExploring the Birth of Stars
Hubble’s Nebulae
Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble’s Stellar Construction Zones
Hubble’s Night Sky Challenge
Hubble’s 35th Anniversary
Hubble Snaps Stellar Baby Pictures
- Hubble Home
- Overview
- Impact & Benefits
- Science
- Observatory
- Team
- Multimedia
- News
- More
3 min read
Hubble Snaps Stellar Baby Pictures The Cepheus A region is home to a number of infant stars, including a protostar that is responsible for much of the region’s illumination. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) Star-forming region G033.91+0.11 is home to a protostar hidden within a reflection nebula. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) A protostar is swathed in the gas of an emission nebula within star-forming region GAL-305.20+00.21. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America) A protostar’s jets of high-speed particles are responsible for the bright region of excited, glowing hydrogen in this Hubble image. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)
Newly developing stars shrouded in thick dust get their first baby pictures in these images from NASA’s Hubble Space Telescope. Hubble took these infant star snapshots in an effort to learn how massive stars form.
Protostars are shrouded in thick dust that blocks light, but Hubble can detect the near-infrared emission that shines through holes formed by the protostar’s jets of gas and dust. The radiating energy can provide information about these “outflow cavities,” like their structure, radiation fields, and dust content. Researchers look for connections between the properties of these young stars – like outflows, environment, mass, brightness – and their evolutionary stage to test massive star formation theories.
These images were taken as part of the SOFIA Massive (SOMA) Star Formation Survey, which investigates how stars form, especially massive stars with more than eight times the mass of our Sun.
The Cepheus A region is home to a number of infant stars, including a protostar that is responsible for much of the region’s illumination. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.7 MB)
The high-mass star-forming region Cepheus A hosts a collection of baby stars, including one large and luminous protostar, which accounts for about half of the region’s brightness. While much of the region is shrouded in opaque dust, light from hidden stars breaks through outflow cavities to illuminate and energize areas of gas and dust, creating pink and white nebulae. The pink area is an HII region, where the intense ultraviolet radiation of the nearby stars has converted the surrounding clouds of gas into glowing, ionized hydrogen.
Cepheus A lies about 2,400 light-years away in the constellation Cepheus.
Download this image (5.8 MB)
Glittering much closer to home, this Hubble image depicts the star-forming region G033.91+0.11 in our Milky Way galaxy. The light patch in the center of the image is a reflection nebula, in which light from a hidden protostar bounces off gas and dust.
A protostar is swathed in the gas of an emission nebula within star-forming region GAL-305.20+00.21. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.8 MB)
This Hubble image showcases the star-forming region GAL-305.20+00.21. The bright spot in the center-right of the image is an emission nebula, glowing gas that is ionized by a protostar buried within the larger complex of gas and dust clouds.
A protostar’s jets of high-speed particles are responsible for the bright region of excited, glowing hydrogen in this Hubble image. NASA, ESA, and R. Fedriani (Instituto de Astrofisica de Andalucia); Processing: Gladys Kober (NASA/Catholic University of America)Download this image (5.7 MB)
Shrouded in gas and dust, the massive protostar IRAS 20126+4104 lies within a high-mass star-forming region about 5,300 light-years away in the constellation Cygnus. This actively forming star is a B-type protostar, characterized by its high luminosity, bluish-white color, and very high temperature. The bright region of ionized hydrogen at the center of the image is energized by jets emerging from the poles of the protostar, which ground-based observatories previously observed.
New images added every day between January 12-17, 2026! Follow @NASAHubble on social media for the latest Hubble images and news and see Hubble’s Stellar Construction Zones for more images of young stellar objects.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore MoreExploring the Birth of Stars
Hubble’s Nebulae
Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble’s Stellar Construction Zones
Hubble’s Night Sky Challenge
Hubble’s 35th Anniversary
NASA’s Artemis II mission to the moon is inching toward the launch pad
NASA rolled out the fully stacked Artemis II rocket and Orion capsule on Saturday, embarking on a four-mile journey to the launch pad
This gene may determine if dogs have long, floppy ears or short, study ones
Scientists are just beginning to understand the signals that determine the length of dogs’ ears
World models could unlock the next revolution in artificial intelligence
Why today’s AI systems struggle with consistency, and how emerging world models aim to give machines a steady grasp of space and time
First treaty to protect the high seas comes into force
First treaty to protect the high seas comes into force
Analysis of Chang'e-6 Samples Addresses Mysteries About the Far Side of the Moon.
Our nearest neighbor, the Moon, is still something of a mystery to us. For decades, scientists have wondered why it appears so lopsided, with dark volcanic plains on the near side (the side we see) and rugged, cratered mountains and a thicker crust on the far side. Now we might be closer to knowing why.
NASA’s SpaceX Crew-11 to Discuss Space Station Science Mission
After 167 days in space, the crew members of NASA’s SpaceX Crew-11 mission will hold a news conference at 2:15 p.m. EST, Wednesday, Jan. 21, at the agency’s Johnson Space Center in Houston to discuss their science expedition aboard the International Space Station.
NASA astronauts Zena Cardman and Mike Fincke, JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui, and Roscosmos cosmonaut Oleg Platonov will answer questions about their mission. The crew members returned to Earth on Jan. 15, splashing down off the coast of San Diego, and arrived in Houston on Friday, where they will undergo standard postflight reconditioning and evaluations.
NASA will provide live coverage on the agency’s YouTube channel. Learn how to watch NASA content through a variety of additional online platforms, including social media.
Media are invited to attend in person or virtually. For in-person attendance, contact the NASA Johnson newsroom no later than 5 p.m. CST, Tuesday, Jan. 20, at jsccommu@mail.nasa.gov or 281-483-5111. Media participating by phone must dial into the news conference no later than 10 minutes prior to the start of the event to ask questions. Questions also may be submitted on social media using #AskNASA. A copy of NASA’s media accreditation policy is available on the agency’s website.
The crew spent more than five months in space, including 165 days aboard the orbiting laboratory, traveling nearly 71 million miles, and completing more than 2,670 orbits around Earth. While living and working aboard the station, the crew completed hundreds of science experiments and technology demonstrations.
Get the latest NASA space station news, images, and features on Instagram, Facebook, and X.
NASA’s Commercial Crew Program has delivered on its goal of safe, reliable, and cost-effective transportation to and from the International Space Station from the United States through a partnership with American private industry. This partnership is opening access to low Earth orbit and the space station to more people, more science, and more commercial opportunities. For more than 25 years, people have continuously lived and worked aboard the space station, advancing scientific knowledge and demonstrating new technologies that enable us to prepare for human exploration of the Moon as we prepare for Mars.
Learn more about NASA’s Commercial Crew Program at:
https://www.nasa.gov/commercialcrew
-end-
Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov
Anna Schneider / Shaneequa Vereen
Johnson Space Center, Houston
281-483-5111
anna.c.schneider@nasa.gov / shaneequa.y.vereen@nasa.gov
NASA’s SpaceX Crew-11 to Discuss Space Station Science Mission
After 167 days in space, the crew members of NASA’s SpaceX Crew-11 mission will hold a news conference at 2:15 p.m. EST, Wednesday, Jan. 21, at the agency’s Johnson Space Center in Houston to discuss their science expedition aboard the International Space Station.
NASA astronauts Zena Cardman and Mike Fincke, JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui, and Roscosmos cosmonaut Oleg Platonov will answer questions about their mission. The crew members returned to Earth on Jan. 15, splashing down off the coast of San Diego, and arrived in Houston on Friday, where they will undergo standard postflight reconditioning and evaluations.
NASA will provide live coverage on the agency’s YouTube channel. Learn how to watch NASA content through a variety of additional online platforms, including social media.
Media are invited to attend in person or virtually. For in-person attendance, contact the NASA Johnson newsroom no later than 5 p.m. CST, Tuesday, Jan. 20, at jsccommu@mail.nasa.gov or 281-483-5111. Media participating by phone must dial into the news conference no later than 10 minutes prior to the start of the event to ask questions. Questions also may be submitted on social media using #AskNASA. A copy of NASA’s media accreditation policy is available on the agency’s website.
The crew spent more than five months in space, including 165 days aboard the orbiting laboratory, traveling nearly 71 million miles, and completing more than 2,670 orbits around Earth. While living and working aboard the station, the crew completed hundreds of science experiments and technology demonstrations.
Get the latest NASA space station news, images, and features on Instagram, Facebook, and X.
NASA’s Commercial Crew Program has delivered on its goal of safe, reliable, and cost-effective transportation to and from the International Space Station from the United States through a partnership with American private industry. This partnership is opening access to low Earth orbit and the space station to more people, more science, and more commercial opportunities. For more than 25 years, people have continuously lived and worked aboard the space station, advancing scientific knowledge and demonstrating new technologies that enable us to prepare for human exploration of the Moon as we prepare for Mars.
Learn more about NASA’s Commercial Crew Program at:
https://www.nasa.gov/commercialcrew
-end-
Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov
Anna Schneider / Shaneequa Vereen
Johnson Space Center, Houston
281-483-5111
anna.c.schneider@nasa.gov / shaneequa.y.vereen@nasa.gov
A Simulated Asteroid Impact Reveals the Strength of Iron-Rich Rocks
Physicists at the University of Oxford have contributed to a new study which has found that iron-rich asteroids can tolerate far more energy than previously thought without breaking apart - a breakthrough with direct implications for planetary defence strategies.