This NASA/ESA Hubble Space Telescope features the
nearby galaxy NGC 4449.
ESA/Hubble & NASA, E. Sabbi,
D. Calzetti, A. Aloisi
This portrait from the NASA/ESA Hubble Space Telescope puts the nearby galaxy NGC 4449 in the
spotlight. The galaxy is situated just 12.5 million light-years away in the
constellation Canes Venatici (the Hunting Dogs). It is a member of the M94
galaxy group, which is near the Local Group of galaxies that the Milky Way is
part of.
NGC 4449 is a dwarf galaxy, which
means that it is far smaller and contains fewer stars than the Milky Way. But
don’t let its small size fool you — NGC 4449 packs a punch when it comes to
making stars! This galaxy is currently forming new stars at a much faster rate
than expected for its size, which makes it a starburst galaxy. Most starburst
galaxies churn out stars mainly in their centers, but NGC 4449 is alight with
brilliant young stars throughout. Researchers believe that this global burst of
star formation came about because of NGC 4449’s interactions with its galactic
neighbors. Because NGC 4449 is so close, it provides an excellent opportunity
for Hubble to study how interactions between galaxies can influence the
formation of new stars.
Hubble released an image of NGC 4449 in 2007. This new version incorporates several additional
wavelengths of light that Hubble collected for multiple observing programs.
These programs encompass an incredible range of science, from a deep dive into
NGC 4449’s star-formation history to the mapping of the brightest, hottest, and
most massive stars in more than two dozen nearby galaxies.
The NASA/ESA/CSA James
Webb Space Telescope has also observed NGC 4449, revealing in intricate detail the galaxy’s tendrils of dusty gas, glowing
from the intense starlight radiated by the flourishing young stars.
Text Credit: ESA/Hubble
Source: Hubble Studies Small but Mighty Galaxy - NASA Science
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