lunes, 19 de marzo de 2018


Messier 82 (The Cigar Galaxy) | NASA

collage of Hubble Messier object images and portrait of Messier

Messier 82 (The Cigar Galaxy)

Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI) and P. Puxley (National Science Foundation)
core of M82
This Hubble image is the most detailed view of M82’s core ever captured. It isolates the light from glowing gas clouds, while blocking out much of the starlight. The image shows the light emitted by sulfur (in red), visible and ultraviolet light from oxygen (in green and blue, respectively), and light from hydrogen (in cyan).
Credits: ESA/Hubble & NASA
M82 or the Cigar galaxy, shines brightly at infrared wavelengths and is remarkable for its star formation activity. The Cigar galaxy experiences gravitational interactions with its galactic neighbor, M81, causing it to have an extraordinarily high rate of star formation — a starburst.
Around the galaxy’s center, young stars are being born 10 times faster than they are inside our entire Milky Way galaxy. Radiation and energetic particles from these newborn stars carve into the surrounding gas, and the resulting galactic wind compresses enough gas to make millions of more stars. The rapid rate of star formation in this galaxy eventually will be self-limiting. When star formation becomes too vigorous, it will consume or destroy the material needed to make more stars. The starburst will then subside, probably in a few tens of millions of years.
M82 was discovered, along with its neighbor M81, by the German astronomer Johann Elert Bode in 1774. Located 12 million light-years from Earth in the constellation Ursa Major, M82 has an apparent magnitude of 8.4 and is best observed in April. Although it is visible as a patch of light with binoculars in the same field of view as M81, larger telescopes are needed in order to resolve the galaxy’s core.
This stunning Hubble image of M82 was assembled using observations at different wavelengths. The red in the image represents hydrogen and infrared light, indicating starburst activity. The blue and greenish-yellow color represent visible wavelengths of light.
For more information about Hubble’s observations of M82, see:
locator star chart for M82
This star chart for M82 represents the view from mid-northern latitudes for the given month and time.
Credits: Image courtesy of Stellarium
Last Updated: Nov. 14, 2017
Editor: Rob Garner

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