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A dazzling Hubble collection of supernova host galaxies


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    • By NASA
      ESA/Hubble & NASA, C. Kilpatrick This NASA/ESA Hubble Space Telescope image treats viewers to a wonderfully detailed snapshot of the spiral galaxy NGC 3430 that lies 100 million light-years from Earth in the constellation Leo Minor. Several other galaxies, located relatively nearby to this one, are just beyond the frame of this image; one is close enough that gravitational interaction is driving some star formation in NGC 3430 — visible as bright-blue patches near to but outside of the galaxy’s main spiral structure. This fine example of a galactic spiral holds a bright core from which a pinwheel array of arms appears to radiate outward. Dark dust lanes and bright star-forming regions help define these spiral arms.
      NGC 3430’s distinct shape may be one reason why astronomer Edwin Hubble used to it to help define his classification of galaxies. Namesake of the Hubble Space Telescope, Edwin Hubble authored a paper in 1926 that outlined the classification of some four hundred galaxies by their appearance — as either spiral, barred spiral, lenticular, elliptical, or irregular. This straightforward typology proved extremely influential, and the detailed schemes astronomers use today are still based on Edwin Hubble’s work. NGC 3430 itself is a spiral lacking a central bar with open, clearly defined arms — classified today as an SAc galaxy.
      Image credit: ESA/Hubble & NASA, C. Kilpatrick
      View the full article
    • By NASA
      2 min read
      Hubble Images a Classic Spiral 
      This NASA/ESA Hubble Space Telescope image features the majestic spiral galaxy NGC 3430. ESA/Hubble & NASA, C. Kilpatrick This NASA/ESA Hubble Space Telescope image treats viewers to a wonderfully detailed snapshot of the spiral galaxy NGC 3430 that lies 100 million light-years from Earth in the constellation Leo Minor. Several other galaxies, located relatively nearby to this one, are just beyond the frame of this image; one is close enough that gravitational interaction is driving some star formation in NGC 3430 — visible as bright-blue patches near to but outside of the galaxy’s main spiral structure. This fine example of a galactic spiral holds a bright core from which a pinwheel array of arms appears to radiate outward. Dark dust lanes and bright star-forming regions help define these spiral arms.
      NGC 3430’s distinct shape may be one reason why astronomer Edwin Hubble used to it to help define his classification of galaxies. Namesake of the Hubble Space Telescope, Edwin Hubble authored a paper in 1926 that outlined the classification of some four hundred galaxies by their appearance — as either spiral, barred spiral, lenticular, elliptical, or irregular. This straightforward typology proved extremely influential, and the detailed schemes astronomers use today are still based on Edwin Hubble’s work. NGC 3430 itself is a spiral lacking a central bar with open, clearly defined arms — classified today as an SAc galaxy.
      Astronomer Edwin Hubble pioneered the study of galaxies based simply on their appearance. This “Field Guide” outlines Hubble’s classification scheme using images from his namesake telescope. Credit: NASA’s Goddard Space Flight Center; Lead Producer: Miranda Chabot; Lead Writer: Andrea Gianopoulos
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      Hubble’s Galaxies


      Astronomer Edwin Hubble

      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
      Claire Andreoli
      NASA’s Goddard Space Flight Center, Greenbelt, MD
      claire.andreoli@nasa.gov
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      Details
      Last Updated Jul 25, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Missions Spiral Galaxies 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.


      Hubble’s Galaxies



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      View the full article
    • By NASA
      3 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      NASA’s pavilion as it will look at EAA AirVenture Oshkosh 2024 is seen in this illustration, Flying into the graphic, clockwise from upper left: the X-66 sustainable flight demonstrator, X-59 quiet supersonic demonstrator, Saab 340B, a small drone, an air taxi concept, and a DeHavillland “Dash 7.” Both the Saaab and Dash 7 are part of the Electrified Powertrain Flight Demonstration project.NASA / Maria Werries Each summer, aviation enthusiasts and experts from around the planet – including NASA’s aeronautical innovators – descend into a regional airport near Oshkosh, Wisconsin, to attend the Experimental Aviation Association’s AirVenture Oshkosh.
      The weeklong airshow and fly-in, where droves of pilots arrive in their own aircraft, draws hundreds of thousands of aviation enthusiasts to enjoy aerial demonstrations, static aircraft displays, aviation-related forums, and hands-on activities for people of all ages and all education levels.
      NASA will appear at Oshkosh with a full slate of interactive exhibits, informative activities, and fascinating people to meet. This year’s event, held July 22-28, is chock-full of things to do and see.
      If you’re attending Oshkosh this year, here’s a brief summary of what you can expect inside the NASA Pavilion and on the forum stages:
      Meet and greet opportunities with NASA’s researchers, leaders, pilots, and maybe even an astronaut Hands-on educational STEM activities and handouts for kids and adults of all ages Talks and panels on NASA activities from our leadership, engineers, pilots, and other subject matter experts Models of NASA aircraft and spacecraft And if you’re looking for certain activities, NASA guides will be available onsite to help you find the ones best suited to you and your group.
      NASA Panel Events
      In addition to the NASA Pavilion and forum talks, there are also several NASA-focused panels that are a can’t miss.
      For example, the “NASA Artemis Campaign: For All Humankind” panel will be held at 7 p.m. CDT on Friday, July 26 at AirVenture’s Theater in the Woods. The event will feature astronaut Randy Bresnik and subject matter experts discussing the upcoming Artemis II mission.
      “Women of NASA,” another great panel, will take place at 8:30 a.m. CDT on Wednesday, July 24, the WomenVenture Center. It will feature several inspiring NASA Women, from senior leaders to project managers and engineers.
      A list of all NASA activities is available on AirVenture’s website, and our aeronautical innovators will be inside the NASA Pavilion to assist you.
      STEM Engagement Activities
      The NASA Pavilion’s STEM Zone will have interactive activities and demonstrations. NASA will also have materials available for educators. The STEM Zone will be open Monday to Sunday, July 22-28, from 9 a.m. to 2:30 p.m. CDT.
      The KidVenture buildings, hosted by the EAA Museum, will include hands-on NASA STEM activities also, and NASA will participate at the AeroEducate Center in Aviation Gateway Park with activities intended for middle- and high-school aged youth – including lectures and a drone flight cage.
      More NASA’s activities are available on the event schedule or on EAA’s app.
      Online Oshkosh Coverage
      Online, NASA will post live updates from Oshkosh with news about NASA’s events and festivities through the week, as well as more information about our flight research goals. The live posts will be a great way to keep up with what’s going on for those who are unable to attend the event in person.
      Additionally, NASA will post on social media using the hashtag #OSH24.
      About the Author
      John Gould
      Aeronautics Research Mission DirectorateJohn Gould is a member of NASA Aeronautics' Strategic Communications team at NASA Headquarters in Washington, DC. He is dedicated to public service and NASA’s leading role in scientific exploration. Prior to working for NASA Aeronautics, he was a spaceflight historian and writer, having a lifelong passion for space and aviation.
      Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More
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      Last Updated Jul 19, 2024 EditorJim BankeContactJim Bankejim.banke@nasa.gov Related Terms
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    • By NASA
      3 min read
      Hubble Studies a Potential Galactic Merger
      This NASA/ESA Hubble Space Telescope image captures the dwarf irregular galaxy NGC 5238. ESA/Hubble & NASA, F. Annibali This NASA/ESA Hubble Space Telescope image features the dwarf irregular galaxy NGC 5238, located 14.5 million light-years from Earth in the constellation Canes Venatici. Its unexciting, blob-like appearance seems to resemble an oversized star cluster more than a classic image of a galaxy. Its lackluster appearance belies its complicated structure, which is the subject of a great deal of research. As the image reveals, Hubble is able to pick out the galaxy’s countless stars, as well as its associated globular clusters — glowing, bright spots both inside and around the galaxy swarmed by even more stars.
      Astronomers theorize that NGC 5238 may have had a close encounter with another galaxy as recently as a billion years ago. NGC 5238’s distorted shape provides evidence for this interaction. As the two galaxies interacted, their gravity caused distortions in the distribution of stars in each galaxy. There’s no nearby galaxy which could have caused this disturbance, so astronomers think NGC 5238 devoured a smaller satellite galaxy. Astronomers look for traces of the consumed galaxy by closely examining the population of stars in NGC 5238, a task made for Hubble’s excellent resolution. One tell-tale sign of the smaller galaxy would be groups of stars with different properties from most of NGC 5238’s other stars, indicating they were originally formed in a separate galaxy. Another sign would be a burst of star formation that occurred abruptly at around the same time the two galaxies merged. The Hubble data used to create this image will help astronomers determine NGC 5238’s history.
      Despite their small size and unremarkable appearance, it’s not unusual for dwarf galaxies like NGC 5238 to drive our understanding of galaxy formation and evolution. One main theory of galaxy evolution is that galaxies formed ‘bottom-up’ in a hierarchical fashion: star clusters and small galaxies were the first to form out of gas and dark matter. Over time, gravity gradually assembled these smaller objects into galaxy clusters and superclusters, which explains the shape of the largest structures we see in the universe today. A dwarf irregular galaxy like NGC 5238 merging with a smaller companion is just the type of event that might have started the process of galaxy assembly in the early universe. Hubble’s observations of tiny NGC 5238 may help test some of our most fundamental ideas of how the universe evolves!

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      Galaxy Details and Mergers


      Tracing the Growth of Galaxies


      Hubble’s Galaxies


      Hubble’s Star Clusters

      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
      Claire Andreoli
      NASA’s Goddard Space Flight Center, Greenbelt, MD
      claire.andreoli@nasa.gov
      Share








      Details
      Last Updated Jul 18, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Irregular Galaxies Missions 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.


      Hubble E-books



      Hubble Science



      Hubble Online Activities


      View the full article
    • By European Space Agency
      A duo of interacting galaxies known as Arp 142 commemorates the second science anniversary of the NASA/ESA/CSA James Webb Space Telescope. Their ongoing interaction was set in motion between 25 and 75 million years ago, when the Penguin (individually catalogued as NGC 2936) and the Egg (NGC 2937) completed their first pass. They will go on to shimmy and sway, completing several additional loops before merging into a single galaxy hundreds of millions of years from now.
      View the full article
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