Hubble Space Telescope | Tiny Stellar Islands in a Big Old Universe @hubblespacetelescope | Uploaded August 2019 | Updated October 2024, 20 hours ago.
Tiny Stellar Islands in a Big Old Universe
Trisha Ashley of the Space Telescope Science Institute
Galaxies are islands of stars, gas, and dark matter, the smallest of which are called dwarf galaxies. Although dwarf galaxies are the most numerous, astronomers are still trying to understand their structure, composition, and variety. Star formation in dwarf galaxies is especially important. What triggers star formation in dwarf galaxies? Why do some form a lot more stars? Join us to hear how these galaxies compare to our Milky Way galaxy and what makes them special!
Host: Dr. Alex Lockwood of the Space Telescope Science Institute
Recorded live on Tuesday, August 6, 2019, at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A.
More information: www.stsci.edu/public-lectures
Tiny Stellar Islands in a Big Old Universe
Trisha Ashley of the Space Telescope Science Institute
Galaxies are islands of stars, gas, and dark matter, the smallest of which are called dwarf galaxies. Although dwarf galaxies are the most numerous, astronomers are still trying to understand their structure, composition, and variety. Star formation in dwarf galaxies is especially important. What triggers star formation in dwarf galaxies? Why do some form a lot more stars? Join us to hear how these galaxies compare to our Milky Way galaxy and what makes them special!
Host: Dr. Alex Lockwood of the Space Telescope Science Institute
Recorded live on Tuesday, August 6, 2019, at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A.
More information: www.stsci.edu/public-lectures
![The Whirlpool Galaxy: Visible and X-ray Views [UltraHD]](https://i.ytimg.com/vi/u8jGr2WSFD8/hqdefault.jpg "The Whirlpool Galaxy: Visible and X-ray Views [UltraHD]
This sequence uses visible (Hubble) and X-ray (Chandra) imagery to highlight different structures within the Whirlpool galaxy (Messier 51). As seen in visible light, the familiar whirlpool shape is traced out by glowing spiral arms. These arms are composed of billions of stars orbiting about the center of the galaxy over millions of years. The pink color is from hot hydrogen gas that permeates the galaxy and indicates sites of new star formation. Silhouetted in the bright arms are dark lanes of obscuring dust that blocks visible light. The stars farther away from the center orbit more slowly and fall behind, creating the signature spiral winding arm. A massive black hole lies at the galaxy’s center. The black hole can’t be seen directly, but its presence is hinted at by the dense star clusters at the center. A second smaller spiral galaxy can be seen in the upper-right portion of the image. The second image shows the X-ray view, highlighting the very hottest gas at millions of degrees Fahrenheit. The X-rays most closely match the visible pink hot gas in active star-forming regions and are particularly strong near the galactic centers of both galaxies. X-rays are also penetrating obscuring dust.
Video: NASA, ESA, and G. Bacon (STScI)
Image: NASA and The Hubble Heritage Team (STScI)")
