Astronomers utilizing the NASA/ESA Hubble House Telescope have captured a spectacular picture of the spiral galaxy NGC 2775.
NGC 2775 is positioned roughly 67 million light-years away within the northern constellation of Most cancers.
The galaxy was found on December 19, 1783 by the German-born British astronomer William Herschel.
It belongs to the Antilia-Hydra Cloud of galaxies and is the primary member of a small group of galaxies referred to as the NGC 2775 group.
Often known as LEDA 25861 or UGC 4820, NGC 2275 has a diameter of 80,000 light-years and is assessed as a flocculent spiral galaxy.
“NGC 2775’s ‘flocculent’ spiral arms point out that the current historical past of star formation of the galaxy has been comparatively quiet,” Hubble astronomers stated.
“There’s just about no star formation within the central a part of the galaxy, which is dominated by an unusually massive and comparatively empty galactic bulge, the place all of the fuel was transformed into stars way back.”
“Tens of millions of shiny, younger, blue stars shine within the advanced, feather-like spiral arms, interlaced with darkish lanes of mud,” they famous.
“Complexes of those sizzling, blue stars are thought to set off star formation in close by fuel clouds.”
“The general feather-like spiral patterns of the arms are then fashioned by shearing of the fuel clouds because the galaxy rotates.”
“The spiral nature of flocculents stands in distinction to the grand design spirals, which have distinguished, effectively defined-spiral arms.”