[5] Mohini Fluctus, a bright lobate flow feature at least 200 kilometers (120 mi) long, appears to emerge from Doom Mons and extends to the northeast.

[9] Doom Mons is believed to be a twin-peak that rises 1.45 km (0.90 mi) above the relatively flat surrounding plain, and a probable massive cryovolcano.

[10] The permanent hurricane at the southern pole of Titan probably causes an issue of constant erosion on Doom Mons, preventing the mountain from growing taller.

[1] Robert Brown of the University of Arizona, one of the controllers of the Cassini-Huygens probe, gave the following description of Doom Mons at the December 2006 meeting of the American Geophysical Union in San Francisco, California: "This mountain range is tall enough to produce streamers of clouds that extend far around the moon.

Several smaller ranges appear to be nearby, as does a circular feature that might be the crater from an ancient asteroid impact powerful enough to have punched through Titan's outer crust.

The climate of Weinbaum's mountain is described as sub-Arctic, and it is constantly battered by howling ice-needle storms and hurricane-force winds.