A spiral galaxy named NGC 772, captured by the NASA/ESA Hubble Space Telescope. This image was first shared on 11th November 2019. ESA/Hubble & NASA, A. Seth et al.
This elegant image was captured by the Hubble Space Telescope, showing a galaxy called NGC 772 which is located 130 million light-years away in the constellation Aries.
NGC 772 has some distinctive features. One immediately noticeable difference between NGC 772 and our home galaxy is that it does not have a bar, unlike the Milky Way which is a barred galaxy. Bars are bands of bright light caused by structures of dust and gas which run along the center of galaxies. Astronomers believe these bars typically develop later in the lifetime of most galaxies, and between one-third and two-thirds of all galaxies are thought to have bars.
In the Milky Way and other barred galaxies, bars contribute to star formation by funneling the dust and gases which are the building blocks of stars into the galactic core. In a non-barred galaxy like NGC 772, this mechanism is missing, although there is still plenty of dust and gas floating around for the forming of new stars in other regions of the galaxy.
NGC 772 is also an unusual elongated shape, which means it is technically classified as a “peculiar galaxy.” The peculiarity, in this case, is the spiral arm in the upper portion of the image, which has been stretched and extended. The distortion is caused by the movements of a nearby satellite galaxy, which is a term for a smaller galaxy that is gravitationally bound to a larger galaxy and which orbits around it.
One of NGC 772’s satellite galaxies is called NGC 770, which isn’t visible in the image but does have a visible impact. NGC 770 exerts tidal forces on its larger host galaxy, pulling the one spiral arm out deeper into space. That’s why NGC 772 appears asymmetrical.
Our Milky Way also has satellite galaxies including the Large Magellanic Cloud and Small Magellanic Cloud, although data from Hubble suggests that these galaxies may be moving too fast to truly be in orbit around our galaxy. Eventually, however, these smaller galaxies may cause the demise of our galaxy, as researchers believe the Large Magellanic Cloud will eventually collide with the Milky Way and cause the black hole at the heart of our galaxy to explode in size and devour nearby matter.