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We analyze a rich dataset including Subaru/SuprimeCam, HST/ACS and WFC3,Keck/DEIMOS, Chandra/ACIS-I, and JVLA/C and D array for the merging galaxycluster ZwCl 0008.8+5215. With a joint Subaru/HST weak gravitational lensinganalysis, we identify two dominant subclusters and estimate the masses to beM$_{200}=\text{5.7}^{+\text{2.8}}_{-\text{1.8}}\times\text{10}^{\text{14}}\,\text{M}_{\odot}$and 1.2$^{+\text{1.4}}_{-\text{0.6}}\times10^{14}$ M$_{\odot}$. We estimate theprojected separation between the two subclusters to be924$^{+\text{243}}_{-\text{206}}$ kpc. We perform a clustering analysis onconfirmed cluster member galaxies and estimate the line of sight velocitydifference between the two subclusters to be 92$\pm$164 km s$^{-\text{1}}$. Wefurther motivate, discuss, and analyze the merger scenario through an analysisof the 42 ks of Chandra/ACIS-I and JVLA/C and D polarization data. The X-raysurface brightness profile reveals a remnant core reminiscent of the BulletCluster. The X-ray luminosity in the 0.5-7.0 keV band is1.7$\pm$0.1$\times$10$^{\text{44}}$ erg s$^{-\text{1}}$ and the X-raytemperature is 4.90$\pm$0.13 keV. The radio relics are polarized up to 40$\%$.We implement a Monte Carlo dynamical analysis and estimate the merger velocityat pericenter to be 1800$^{+\text{400}}_{-\text{300}}$ km s$^{-\text{1}}$. ZwCl0008.8+5215 is a low-mass version of the Bullet Cluster and therefore may proveuseful in testing alternative models of dark matter. We do not find significantoffsets between dark matter and galaxies, as the uncertainties are large withthe current lensing data. Furthermore, in the east, the BCG is offset fromother luminous cluster galaxies, which poses a puzzle for defining dark matter-- galaxy offsets.

MC$^2$: Multi-wavelength and dynamical analysis of the merging galaxy cluster ZwCl 0008.8+5215: An older and less massive Bullet Cluster