08/21/2025
An Oldie but a Goodie!
The Natural History Museum of Utah’s Wall is an instant classic. Fantastic casts are displayed as a phylogeny, showing the relationships of the taxa within and between the two major groups.
Notice how they cluster into two groups at the base, those directly above me are part of the , those on the right of the photo are .
and are just offscreen, the white diagonal lines just over my right shoulder lead to them.
Centrosaurines are known for large nose horns and crazy-cool spikes on the frills.
Chasmosaurines tend towards huge eye horns and giant frills lacking spikes.
There are other characters, but those two are the quickest to use. Please note, discoveries in the last 20 years mean these shortcuts don’t always work.
As one gets later and later into the they hold up well, but earlier than 75 mya ago, closer to the group’s split, their identification power lessens.
We see this same challenge when trying to figure out what is or isn’t a dinosaur in the . Tis a byproduct of how works. a
When taxa split, being closely related means they share many characters initially. Over time, the groups have change more and more, making it easier to tell them apart.
The Society of Vertebrate Paleontology held its annual meetings in Salt Lake City in 2016, with an event held in this museum. I think every at the meeting engaged in a competitive version of “how many can you name?” My sauropod bias did me no favors…
The ceratopsian specialists shined, though major disagreements could be heard over the validity of some taxa. It was great fun seeing the camaraderie, and competitiveness, of the horned dino crowd.
Note how big Cohuilaceratops is (the Fossil Crates logo), that surprised me!
My love for Styracosaurus is still well-placed after all these years, to me tis the prettiest one on the Wall.
The list: