This NASA/ESA Hubble Space Telescope image features
the asymmetric spiral galaxy Messier 96.
ESA/Hubble & NASA, F. Belfiore, D. Calzetti
This NASA/ESA Hubble Space Telescope image
features a galaxy whose asymmetric appearance may be the result of a galactic
tug of war. Located 35 million light-years away in the constellation Leo, the
spiral galaxy Messier 96 is the brightest of the galaxies in its group. The
gravitational pull of its galactic neighbors may be responsible for Messier
96’s uneven distribution of gas and dust, asymmetric spiral arms, and
off-center galactic core.
This asymmetric appearance is on full
display in the new Hubble image that incorporates data from observations made
in ultraviolet, near infrared, and visible/optical light. Earlier Hubble images
of Messier 96 were released in 2015 and 2018.
Each successive image added new data, building up a beautiful and
scientifically valuable view of the galaxy.
The 2015 image combined two wavelengths
of optical light with one near infrared wavelength. The optical light revealed
the galaxy’s uneven form of dust and gas spread asymmetrically throughout its
weak spiral arms and its off-center core, while the infrared light revealed the
heat of stars forming in clouds shaded pink in the image.
The 2018 image added two more optical
wavelengths of light along with one wavelength of ultraviolet light that
pinpointed areas where high-energy, young stars are forming.
This latest version offers us a new
perspective on Messier 96’s star formation. It includes the addition of light
that reveals regions of ionized hydrogen (H-alpha) and nitrogen (NII). This
data helps astronomers determine the environment within the galaxy and the
conditions in which stars are forming. The ionized hydrogen traces ongoing star
formation, revealing regions where hot, young stars are ionizing the gas. The ionized nitrogen helps astronomers determine the rate
of star formation and the properties of gas between stars, while the
combination of the two ionized gasses helps researchers determine if the galaxy
is a starburst galaxy or one with an active galactic nucleus.
The bubbles of pink gas in this image surround hot, young, massive stars, illuminating a ring of star formation in the galaxy's outskirts. These young stars are still embedded within the clouds of gas from which they were born. Astronomers will use the new data in this image to study how stars are form within giant dusty gas clouds, how dust filters starlight, and how stars affect their environments.
Source: Hubble Homes in on Galaxy’s Star Formation - NASA Science