MACS0416 Y1

MACS0416 Y1 has several notable properties related to Cosmic dust. The mass of the dust inside the MACS0416 Y1 is estimated to be 4×10⁶ solar masses. The interstellar medium (ISM) of MACS0416 Y1 resembles galaxies at the cosmic noon, located at redshift distances of z = ~2. The gas and dust inside MACS0416 Y1 is also ionized by the active galactic nucleus (AGN) and heated to high temperatures (approximately 95 Kelvin) by the burst of star formation also observed in the galaxy, see below.^[1][2]

The merger of the galaxy has produced three resolved clumps where there is a burst of stellar formation with the central clump being the least massive and possibly formed from a merger of the other two regions.^[1] Around 60 solar masses of stars are formed per year in MACS0416 Y1, and the high star formation rate (SFR) of MACS0416 Y1 heats up the dust inside the rest of the system to high temperatures. These stars have also been polluted by metals from outside their normal formation processes (metallicity).^[3]