Two galaxies are entwined in a turbulent gravitational dance in a stunning new view from the Hubble Space Telescope.
The pair includes the large spiral galaxy NGC 3227 and the elliptical galaxy NGC 3226. The galaxies, known collectively as Arp 94, reside relatively close to Earth, 50 to 60 million light-years away near the constellation Leo.
The new Hubble Space Telescope view shows faint tidal streams of gas and dust linking NGC 3227 and NGC 3226 in their gravitational dance. Observations of this duo were captured as part of a program to measure black holes at the center of bright galaxy clusters, according to a NASA statement. (opens in a new tab).
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NGC 3227 is classified as a Seyfert galaxy, a type of galaxy that has an active nucleus and is powered by a supermassive black hole at its core. As the black hole pulls in material from its surroundings, it releases large amounts of radiation, which fuels the active core of the galaxy.
Hubble was used to measure the mass of the galaxy’s black hole by observing the dynamics of incoming gas at its core. The space telescope captured both visible red and near-infrared wavelengths of light, represented by the red areas of the image, according to the NASA statement.
NGC 3227 is captured in the lower left of the Hubble image, while NGC 3226 is in the upper right of its companion. The new photo, released by NASA on May 25, offers a detailed view of NGC 3227’s dark dust lanes and bright star-forming regions, along with the bright streams of material connecting the two galaxies. Previous Hubble observations suggest that these streamers are remnants of a third galaxy that was likely consumed by NGC 3226, which, in turn, would have scattered bits of gas and dust into space, NASA reported in 2014. (opens in a new tab).
Previous observations also suggest that NGC 3226 has a very low rate of star formation, despite large streams of gas and dust (debris from the cannibalized galaxy) flowing into its core.
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