NASA's Hubble Space Telescope has captured an enigmatic galaxy that defies easy categorization: NGC 2775, a celestial body located 67 million light-years away in the constellation Cancer. The galaxy boasts a seemingly elliptical shape with no discernible gas at its center, but is also characterized by a dusty ring and patchy star clusters reminiscent of a spiral galaxy.
The challenge lies in observing NGC 2775 from only one angle, making it difficult to determine whether it should be classified as a spiral or an elliptical galaxy. Some researchers have deemed it a spiral galaxy due to its feathery starry ring, while others label it a lenticular galaxy, a hybrid of both types.
Lenticular galaxies are thought to emerge from the merger of two galaxies or from the depletion of gas that once fueled their spirally-shaped arms. The exact origin of these galaxies remains unclear, but research suggests that NGC 2775 may have merged with other galaxies in the past. A faint tail of hydrogen gas stretching over 100,000 light-years around the galaxy could be the remnant of a collided galaxy.
Astronomers recently released an updated image of NGC 2775 using Hubble's advanced technology, capturing observations at a specific wavelength of red light emitted by clouds of hydrogen gas surrounding massive young stars. This enhanced data allows for better identification of where new stars are forming within the galaxy. Despite this additional detail, the galaxy's peculiar appearance remains puzzling โ does it conform to the characteristics of a spiral galaxy or defy classification as something entirely new?
The challenge lies in observing NGC 2775 from only one angle, making it difficult to determine whether it should be classified as a spiral or an elliptical galaxy. Some researchers have deemed it a spiral galaxy due to its feathery starry ring, while others label it a lenticular galaxy, a hybrid of both types.
Lenticular galaxies are thought to emerge from the merger of two galaxies or from the depletion of gas that once fueled their spirally-shaped arms. The exact origin of these galaxies remains unclear, but research suggests that NGC 2775 may have merged with other galaxies in the past. A faint tail of hydrogen gas stretching over 100,000 light-years around the galaxy could be the remnant of a collided galaxy.
Astronomers recently released an updated image of NGC 2775 using Hubble's advanced technology, capturing observations at a specific wavelength of red light emitted by clouds of hydrogen gas surrounding massive young stars. This enhanced data allows for better identification of where new stars are forming within the galaxy. Despite this additional detail, the galaxy's peculiar appearance remains puzzling โ does it conform to the characteristics of a spiral galaxy or defy classification as something entirely new?